<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd">
<article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article">
 <front>
  <journal-meta>
   <journal-id journal-id-type="publisher-id">
    jhepgc
   </journal-id>
   <journal-title-group>
    <journal-title>
     Journal of High Energy Physics, Gravitation and Cosmology
    </journal-title>
   </journal-title-group>
   <issn pub-type="epub">
    2380-4327
   </issn>
   <issn publication-format="print">
    2380-4335
   </issn>
   <publisher>
    <publisher-name>
     Scientific Research Publishing
    </publisher-name>
   </publisher>
  </journal-meta>
  <article-meta>
   <article-id pub-id-type="doi">
    10.4236/jhepgc.2025.111002
   </article-id>
   <article-id pub-id-type="publisher-id">
    jhepgc-138766
   </article-id>
   <article-categories>
    <subj-group subj-group-type="heading">
     <subject>
      Articles
     </subject>
    </subj-group>
    <subj-group subj-group-type="Discipline-v2">
     <subject>
      Physics 
     </subject>
     <subject>
       Mathematics
     </subject>
    </subj-group>
   </article-categories>
   <title-group>
    General Maxwell Theory of Fields
   </title-group>
   <contrib-group>
    <contrib contrib-type="author" xlink:type="simple">
     <name name-style="western">
      <surname>
       Yougang
      </surname>
      <given-names>
       Feng
      </given-names>
     </name>
    </contrib>
   </contrib-group> 
   <aff id="affnull">
    <addr-line>
     aCollege of Physics, Guizhou University, Guiyang, China
    </addr-line> 
   </aff> 
   <pub-date pub-type="epub">
    <day>
     02
    </day> 
    <month>
     01
    </month>
    <year>
     2025
    </year>
   </pub-date> 
   <volume>
    11
   </volume> 
   <issue>
    01
   </issue>
   <fpage>
    8
   </fpage>
   <lpage>
    18
   </lpage>
   <history>
    <date date-type="received">
     <day>
      11,
     </day>
     <month>
      November
     </month>
     <year>
      2024
     </year>
    </date>
    <date date-type="published">
     <day>
      5,
     </day>
     <month>
      November
     </month>
     <year>
      2024
     </year> 
    </date> 
    <date date-type="accepted">
     <day>
      5,
     </day>
     <month>
      January
     </month>
     <year>
      2025
     </year> 
    </date>
   </history>
   <permissions>
    <copyright-statement>
     © Copyright 2014 by authors and Scientific Research Publishing Inc. 
    </copyright-statement>
    <copyright-year>
     2014
    </copyright-year>
    <license>
     <license-p>
      This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/
     </license-p>
    </license>
   </permissions>
   <abstract>
    This paper explores Maxwell’s analogy idea between electromagnetic field lines and incompressible fluid, and explains Faraday’s law and Maxwell’s formula for displacement currents by means of fluid dynamics theory: They show the transport properties of electromagnetic field lines as incompressible fluids, not just effects. Combined of the steady electromagnetic fields, Maxwell’s idea of the analogy between the electromagnetic fields and the incompressible fluids has reached a perfect conclusion. Viewing the electromagnetic field as a vacuum state excited by charges, and extending Maxwell analogy, we consider the gravitowagnetic field as a vacuum state excited by mass. This led to the establishment of the generalized Maxwell equations and the application of this new theory to explain various natural phenomena.
   </abstract>
   <kwd-group> 
    <kwd>
     Electromagnetic
    </kwd> 
    <kwd>
      Gravitowagnetic
    </kwd> 
    <kwd>
      Incompressible
    </kwd> 
    <kwd>
      Reynolds
    </kwd>
   </kwd-group>
  </article-meta>
 </front>
 <body>
  <sec id="s1">
   <title>1. Introduction</title>
   <p>In 1857, James Clerk Maxwell published his paper “On Faraday’s Lines of Force”. The analogy he presented for lines of force was the flow of an incompressible fluid. The streamlines of flow represented lines of force either electric or magnetic while the speed and direction of fluid flow at any point represented the density and direction of the lines of force there. It was Maxwell who noticed that lines of force in a field could not cross or coincide, showing their incompressibility. He had given the mathematical interpretation of Faraday’s conceptions regarding the nature of electric and magnetic forces. Maxwell’s imaginary electric or magnetic fluid was weightless, friction-free, and incompressible <xref ref-type="bibr" rid="scirp.138766-1">
     [1]
    </xref>. The author of the reference <xref ref-type="bibr" rid="scirp.138766-1">
     [1]
    </xref> pointed out that the last property (incompressible) was the key to the analogy. Maxwell’s theory of electromagnetic fields encompasses steady and unstable electromagnetic fields. The steady electromagnetic fields include the electrostatic field and steady-state magnetic field, and their properties conform to the laws of fluid mechanics: The electrostatic field conforms to the Gaussian theorem of the fluid, and in turn, the Helmholtz analogy and Maxwell analogy can be used to derive the formula of velocity field by vortex filament (assumed of infinite length) with the help of the Biot-Savart law of the magnetic field <xref ref-type="bibr" rid="scirp.138766-2">
     [2]
    </xref>. There are the following correspondences: 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mrow> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mo>
         / 
       </mo> 
       <mrow> 
        <msub> 
         <mi>
           μ 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mrow> 
      <mo>
        ↔ 
      </mo> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         v 
       </mi> 
      </mstyle> 
     </mrow> 
    </math>, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         I 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        ↔ 
      </mo> 
      <mi>
        Γ 
      </mi> 
     </mrow> 
    </math>, where 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        B 
      </mi> 
     </mstyle> 
    </math> is the magnetic induced intensity, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         μ 
       </mi> 
       <mtext>
         0 
       </mtext> 
      </msub> 
     </mrow> 
    </math> is the space permeability, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        v 
      </mi> 
     </mstyle> 
    </math> is the velocity, 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         I 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> is the electric current, and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       Γ 
     </mi> 
    </math> is the circulation. The velocity field has the same form of formula as the magnetic field</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mtext>
        d 
      </mtext> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         v 
       </mi> 
      </mstyle> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
       </mrow> 
      </mfrac> 
      <mi>
        Γ 
      </mi> 
      <mfrac> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           l 
         </mi> 
        </mstyle> 
        <mo>
          × 
        </mo> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           r 
         </mi> 
        </mstyle> 
       </mrow> 
       <mrow> 
        <msup> 
         <mi>
           r 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math>(1)</p>
   <p>Equation (1) is a mature formula of hydrodynamics and has been around for a long time <xref ref-type="bibr" rid="scirp.138766-2">
     [2]
    </xref>. Obviously, the two parties involved in the analogy can have different dimensions. Unstable electromagnetic fields include Faraday’s law (hereafter referred to as F law) and Maxwell’s formula of displacement current (simply referred to as M law), the two extremely important theories that describe the laws of electromagnetism, without which there would be no electromagnetic wave. Xiao-gang Wen pointed out that the true essence of Maxwell theory is the discovery of a new form of matter: wave-like (or field-like) matter, the electromagnetic wave <xref ref-type="bibr" rid="scirp.138766-3">
     [3]
    </xref>. Unfortunately, these two laws have not yet been explained by fluid dynamics, making Maxwell’s analogy between electromagnetic and fluid fields imperfect. F law of induction states: The induced electromotive force in a closed loop equals the negative of the time rate of change of magnetic flux through the loop. The law reveals that electricity and magnetism can be exchanged with each other. Lenz’s law is a convenient alternative method for determining the direction of an induced current or electromotive force. The law is not an independent principle; it can be derived from F law. It always gives the same results as the sign rules we introduced, in connection with F law, but it is often easier to use. The law states: The direction of any magnetic induction effect is such as to oppose the cause of the effect. The law helps us gain intuitive understanding of various induction effects and of the rule of energy conservation <xref ref-type="bibr" rid="scirp.138766-4">
     [4]
    </xref>. Lenz’s viewpoint is consistent with modern field theory that considers a field as a form of material existence. M law points out that a change of electric field can produce a displacement current in a vacuum or in a perfect insulator, which can produce a magnetic field. We believe that since electromagnetic waves are inseparable from these two laws, if we compare the propagation of electromagnetic waves to the transport of fluids, then these two laws describe the transport characteristics under the condition of conservation of energy: In a local space, two fluid fields (electric field 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        E 
      </mi> 
     </mstyle> 
    </math> and magnetic field 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        B 
      </mi> 
     </mstyle> 
    </math>) must obey the law of change during transport at a certain time interval.</p>
   <p>Further, we consider the electromagnetic field as a vacuum excitation state caused by electric charges, and on this basis, we introduce a new concept: a vacuum excitation state caused by mass. Based on gravitational wave experiments and the Helmholtz theorem, a field excited by moving mass is introduced: the wagnetic field ( 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        W 
      </mi> 
     </mstyle> 
    </math> field), which together with the gravitational field ( 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        G 
      </mi> 
     </mstyle> 
    </math> field) constitutes a vector field related to mass, and called gravitomagnetic field. The reason is that incompressible fluids are composed of matter with mass, which means that moving mass can also generate a force field in the same way that moving electric charges can generate a magnetic field. We introduced the concept of force lines for these two new fields, and drew an analogy with incompressible fluids, thereby deriving several formulas.</p>
   <p>This article adopts a right-handed coordinate system, and for operators and coordinate variables of the left-handed system, a negative sign is added uniformly. The content of this paper is arranged as follows: Section 2 is theory, which compares the F law and M law to the transport process of fluids, and makes an analogy with the Reynolds transport theorem in fluid mechanics, pointing out that F law and M law correspond to two independent transport processes. Subsequently, we derived several important formulas for the gravitowagnetic field. Section 3 is discussion, firstly, from the perspective of macroscopic parity on conservation, explain the rationality of the coexistence of the electromagnetic field and the gravitowagnetic field. Then derive the Lorenz gauge in the gravitowagnetic field under the condition of mass conservation, and pointing out that there exists a force similar to the Lorentz force is caused by the wagnetic field, thereby explaining some natural phenomena including the light bending and photon precession in university, superfluid climbing walls, etc. Section 4 is conclusion.</p>
  </sec><sec id="s2">
   <title>2. Theory</title>
   <sec id="s2_1">
    <title>2.1. The Transport Nature of Electromagnetic Fields</title>
    <p>The dynamics of incompressible fluids are established within the frame work of Newtonian mechanics and must satisfy the conservation laws of Newtonian mechanics: Conservation of mass, conservation of charge, and conservation of energy. These conservation laws can be derived from Reynolds’ transport theorem, which states that the rate of a physical function in the local volume 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        V 
      </mi> 
     </math> of space with time is equal to the rate of change of the physical function in the volume with time plus the flux of the function through the surface 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        S 
      </mi> 
     </math> of the 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        V 
      </mi> 
     </math> at a certain time interval 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         Δ 
       </mi> 
       <mi>
         t 
       </mi> 
      </mrow> 
     </math> <xref ref-type="bibr" rid="scirp.138766-5">
      [5]
     </xref>. The physical function mentioned here can be any physical properties of the system, for the electromagnetic field, a composite system composed of 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         E 
       </mi> 
      </mstyle> 
     </math> and 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         B 
       </mi> 
      </mstyle> 
     </math> fields, the physical functions include electric field strength and magnetic induction intensity. The Reynolds theorem can be formulated as</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mfrac> 
        <mtext>
          d 
        </mtext> 
        <mrow> 
         <mtext>
           d 
         </mtext> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
       <mstyle displaystyle="true"> 
        <mrow> 
         <msub> 
          <mo>
            ∮ 
          </mo> 
          <mi>
            V 
          </mi> 
         </msub> 
         <mrow> 
          <mi>
            f 
          </mi> 
          <mtext>
            d 
          </mtext> 
          <mi>
            v 
          </mi> 
         </mrow> 
        </mrow> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mstyle displaystyle="true"> 
        <mrow> 
         <msub> 
          <mo>
            ∮ 
          </mo> 
          <mi>
            V 
          </mi> 
         </msub> 
         <mrow> 
          <mrow> 
           <mo>
             [ 
           </mo> 
           <mrow> 
            <mfrac> 
             <mrow> 
              <mo>
                ∂ 
              </mo> 
              <mi>
                f 
              </mi> 
             </mrow> 
             <mrow> 
              <mo>
                ∂ 
              </mo> 
              <mi>
                t 
              </mi> 
             </mrow> 
            </mfrac> 
            <mo>
              + 
            </mo> 
            <mo>
              ∇ 
            </mo> 
            <mo>
              ⋅ 
            </mo> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mi>
                f 
              </mi> 
              <mstyle mathvariant="bold" mathsize="normal"> 
               <mi>
                 v 
               </mi> 
              </mstyle> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mo>
             ] 
           </mo> 
          </mrow> 
          <mtext>
            d 
          </mtext> 
          <mi>
            v 
          </mi> 
         </mrow> 
        </mrow> 
       </mstyle> 
      </mrow> 
     </math>(2)</p>
    <p>where 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        f 
      </mi> 
     </math> is the physical function. The theorem implies that only the physical properties corresponding to the two items in the same equation can participate in the transport process at the same time and in the same place, otherwise it is impossible to participate in them.</p>
    <p>Suppose there be only one type of energy transport in a local volume 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        V 
      </mi> 
     </math> of space, 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        ϕ 
      </mi> 
     </math> be the energy density (nothing except it), 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         φ 
       </mi> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          v 
        </mi> 
       </mstyle> 
      </mrow> 
     </math> be the energy flow density, 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         v 
       </mi> 
      </mstyle> 
     </math> be the transporting velocity. The total rate of change of 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        ϕ 
      </mi> 
     </math> in the 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        V 
      </mi> 
     </math> can be expressed by using Equation (2)</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mfrac> 
        <mtext>
          d 
        </mtext> 
        <mrow> 
         <mtext>
           d 
         </mtext> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
       <mstyle displaystyle="true"> 
        <mrow> 
         <msub> 
          <mo>
            ∮ 
          </mo> 
          <mi>
            V 
          </mi> 
         </msub> 
         <mrow> 
          <mi>
            ϕ 
          </mi> 
          <mtext>
            d 
          </mtext> 
          <mi>
            v 
          </mi> 
         </mrow> 
        </mrow> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mstyle displaystyle="true"> 
        <mrow> 
         <msub> 
          <mo>
            ∮ 
          </mo> 
          <mi>
            V 
          </mi> 
         </msub> 
         <mrow> 
          <mrow> 
           <mo>
             [ 
           </mo> 
           <mrow> 
            <mfrac> 
             <mrow> 
              <mo>
                ∂ 
              </mo> 
              <mi>
                ϕ 
              </mi> 
             </mrow> 
             <mrow> 
              <mo>
                ∂ 
              </mo> 
              <mi>
                t 
              </mi> 
             </mrow> 
            </mfrac> 
            <mo>
              + 
            </mo> 
            <mo>
              ∇ 
            </mo> 
            <mo>
              ⋅ 
            </mo> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mi>
                ϕ 
              </mi> 
              <mstyle mathvariant="bold" mathsize="normal"> 
               <mi>
                 v 
               </mi> 
              </mstyle> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mo>
             ] 
           </mo> 
          </mrow> 
          <mtext>
            d 
          </mtext> 
          <mi>
            v 
          </mi> 
         </mrow> 
        </mrow> 
       </mstyle> 
      </mrow> 
     </math>(3)</p>
    <p>If there is no energy loss, the integrand on the right-hand of Equation (3) is equal to zero, and the energy is conserved:</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mfrac> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           ϕ 
         </mi> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         + 
       </mo> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         ⋅ 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mi>
           ϕ 
         </mi> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            v 
          </mi> 
         </mstyle> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>(4)</p>
    <p>This equation is in a fully Eulerian form. The energy of electromagnetic fields is composed of the E-field energy and the B-field energy. There is no electromagnetic wave without F law and M law, and these two laws run through the entire wave propagation process. From this point of view, they describe the energy transport characteristics of electromagnetic fields. The forms of F law and M law are <xref ref-type="bibr" rid="scirp.138766-4">
      [4]
     </xref></p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         × 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mo>
         + 
       </mo> 
       <mfrac> 
        <mtext>
          1 
        </mtext> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            B 
          </mi> 
         </mstyle> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>(5)</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         × 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            E 
          </mi> 
         </mstyle> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>(6)</p>
    <p>Equations (5) and (6) are basic laws for unstable electromagnetic fields, which indicate that 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         E 
       </mi> 
      </mstyle> 
     </math> and 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         B 
       </mi> 
      </mstyle> 
     </math> are not independent, they are influence and restrict each other. Consider the electric field and magnetic field as fluid fields by Maxwell’s analogy, and notice that the materiality of the field indicates that the two formulas are certainly energy transport equations.</p>
    <p>By definition, the direction of the curl field 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         × 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
      </mrow> 
     </math> is the direction in which the circulation density is maximized, which can ensure the conservation of energy in the energy transition process <xref ref-type="bibr" rid="scirp.138766-6">
      [6]
     </xref>:</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         × 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <munder> 
        <mrow> 
         <mi>
           lim 
         </mi> 
        </mrow> 
        <mrow> 
         <mi>
           Δ 
         </mi> 
         <mi>
           S 
         </mi> 
         <mo>
           → 
         </mo> 
         <mn>
           0 
         </mn> 
        </mrow> 
       </munder> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <mi>
           Δ 
         </mi> 
         <mi>
           S 
         </mi> 
        </mrow> 
       </mfrac> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          n 
        </mi> 
       </mstyle> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mrow> 
         <mrow> 
          <mo>
            { 
          </mo> 
          <mrow> 
           <mstyle displaystyle="true"> 
            <mrow> 
             <msub> 
              <mo>
                ∮ 
              </mo> 
              <mi>
                L 
              </mi> 
             </msub> 
             <mstyle mathvariant="bold" mathsize="normal"> 
              <mi>
                E 
              </mi> 
             </mstyle> 
            </mrow> 
           </mstyle> 
           <mo>
             ⋅ 
           </mo> 
           <mtext>
             d 
           </mtext> 
           <mstyle mathvariant="bold" mathsize="normal"> 
            <mi>
              l 
            </mi> 
           </mstyle> 
          </mrow> 
          <mo>
            } 
          </mo> 
         </mrow> 
        </mrow> 
        <mrow> 
         <mi>
           max 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math>(7)</p>
    <p>where 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        L 
      </mi> 
     </math> is the closed path surrounding 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        S 
      </mi> 
     </math>, the 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        S 
      </mi> 
     </math> is the surface of the volume 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        V 
      </mi> 
     </math>, 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         n 
       </mi> 
      </mstyle> 
     </math> is the unit normal vector of the 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         Δ 
       </mi> 
       <mi>
         S 
       </mi> 
      </mrow> 
     </math>. The choice of 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         n 
       </mi> 
      </mstyle> 
     </math> ensures that the circulating current has a maximum value. Because of the conservation of electromagnetic energy, the change of energy in the volume 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        V 
      </mi> 
     </math> should equal to the change of energy passing through the surface S of the 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        V 
      </mi> 
     </math>, namely that</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mstyle displaystyle="true"> 
        <mrow> 
         <msub> 
          <mo>
            ∫ 
          </mo> 
          <mi>
            S 
          </mi> 
         </msub> 
         <mrow> 
          <mrow> 
           <mo>
             [ 
           </mo> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mo>
                ∇ 
              </mo> 
              <mo>
                × 
              </mo> 
              <mstyle mathvariant="bold" mathsize="normal"> 
               <mi>
                 E 
               </mi> 
              </mstyle> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
            <mo>
              + 
            </mo> 
            <mfrac> 
             <mn>
               1 
             </mn> 
             <mi>
               c 
             </mi> 
            </mfrac> 
            <mfrac> 
             <mrow> 
              <mo>
                ∂ 
              </mo> 
              <mstyle mathvariant="bold" mathsize="normal"> 
               <mi>
                 B 
               </mi> 
              </mstyle> 
             </mrow> 
             <mrow> 
              <mo>
                ∂ 
              </mo> 
              <mi>
                t 
              </mi> 
             </mrow> 
            </mfrac> 
           </mrow> 
           <mo>
             ] 
           </mo> 
          </mrow> 
          <mo>
            ⋅ 
          </mo> 
          <mstyle mathvariant="bold" mathsize="normal"> 
           <mi>
             n 
           </mi> 
          </mstyle> 
          <mo>
            ⋅ 
          </mo> 
          <mtext>
            d 
          </mtext> 
          <mi>
            s 
          </mi> 
          <mo>
            = 
          </mo> 
          <mn>
            0 
          </mn> 
         </mrow> 
        </mrow> 
       </mstyle> 
      </mrow> 
     </math>(8)</p>
    <p>There is an analogy between equations (8) and (3), the correspondences are</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mfrac> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           ϕ 
         </mi> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         ↔ 
       </mo> 
       <mfrac> 
        <mtext>
          1 
        </mtext> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            B 
          </mi> 
         </mstyle> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         ⋅ 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          n 
        </mi> 
       </mstyle> 
      </mrow> 
     </math>, 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         ⋅ 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mi>
           ϕ 
         </mi> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            v 
          </mi> 
         </mstyle> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         ↔ 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           ∇ 
         </mo> 
         <mo>
           × 
         </mo> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            E 
          </mi> 
         </mstyle> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         ⋅ 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          n 
        </mi> 
       </mstyle> 
      </mrow> 
     </math>(9)</p>
    <p>Similarly, another correspondences are</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mfrac> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           ϕ 
         </mi> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         ↔ 
       </mo> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mtext>
          1 
        </mtext> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            E 
          </mi> 
         </mstyle> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         ⋅ 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          n 
        </mi> 
       </mstyle> 
      </mrow> 
     </math>, 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         ⋅ 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mi>
           ϕ 
         </mi> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            v 
          </mi> 
         </mstyle> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         ↔ 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           ∇ 
         </mo> 
         <mo>
           × 
         </mo> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            B 
          </mi> 
         </mstyle> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         ⋅ 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          n 
        </mi> 
       </mstyle> 
      </mrow> 
     </math>(10)</p>
    <p>These show that F law and M law are respectively the representations of Reynolds’ theorem for free electromagnetic fields under the condition of energy conservation.</p>
   </sec>
   <sec id="s2_2">
    <title>2.2. Generalization of Maxwell’s Analogy Idea</title>
    <p>Biot-Savart law is an experimental law, the current intensity 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          I 
        </mi> 
        <mn>
          0 
        </mn> 
       </msub> 
      </mrow> 
     </math> is actually contributed by the negative charge of electrons, which current intensity is 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          I 
        </mi> 
        <mi>
          e 
        </mi> 
       </msub> 
      </mrow> 
     </math>, and 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         − 
       </mo> 
       <msub> 
        <mi>
          I 
        </mi> 
        <mn>
          0 
        </mn> 
       </msub> 
       <mo>
         = 
       </mo> 
       <msub> 
        <mi>
          I 
        </mi> 
        <mi>
          e 
        </mi> 
       </msub> 
      </mrow> 
     </math>, the formula is rewritten as</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mtext>
         d 
       </mtext> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mrow> 
         <msub> 
          <mi>
            μ 
          </mi> 
          <mn>
            0 
          </mn> 
         </msub> 
        </mrow> 
        <mrow> 
         <mn>
           4 
         </mn> 
         <mi>
           π 
         </mi> 
        </mrow> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <msub> 
          <mi>
            I 
          </mi> 
          <mi>
            e 
          </mi> 
         </msub> 
         <mtext>
           d 
         </mtext> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            l 
          </mi> 
         </mstyle> 
         <mo>
           × 
         </mo> 
         <msub> 
          <mstyle mathvariant="bold" mathsize="normal"> 
           <mi>
             r 
           </mi> 
          </mstyle> 
          <mn>
            0 
          </mn> 
         </msub> 
        </mrow> 
        <mrow> 
         <msup> 
          <mi>
            r 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math>(11)</p>
    <p>where 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           r 
         </mi> 
        </mstyle> 
        <mn>
          0 
        </mn> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           r 
         </mi> 
        </mstyle> 
        <mo>
          / 
        </mo> 
        <mi>
          r 
        </mi> 
       </mrow> 
      </mrow> 
     </math>, 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         r 
       </mi> 
      </mstyle> 
     </math> is radius vector, 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          μ 
        </mi> 
        <mn>
          0 
        </mn> 
       </msub> 
      </mrow> 
     </math> is the permeability of vacuum, 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          I 
        </mi> 
        <mi>
          e 
        </mi> 
       </msub> 
       <mtext>
         d 
       </mtext> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          l 
        </mi> 
       </mstyle> 
      </mrow> 
     </math> is the current-carrying element for the electrons. The mass flow intensity of electrons formed by the masses of electrons are 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          I 
        </mi> 
        <mi>
          m 
        </mi> 
       </msub> 
      </mrow> 
     </math>, which is in the same direction as 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          I 
        </mi> 
        <mi>
          e 
        </mi> 
       </msub> 
      </mrow> 
     </math>, and the resulting 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         W 
       </mi> 
      </mstyle> 
     </math> can be expressed as</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mtext>
         d 
       </mtext> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          W 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mrow> 
         <msub> 
          <mi>
            ξ 
          </mi> 
          <mn>
            0 
          </mn> 
         </msub> 
        </mrow> 
        <mrow> 
         <mn>
           4 
         </mn> 
         <mi>
           π 
         </mi> 
        </mrow> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <msub> 
          <mi>
            I 
          </mi> 
          <mi>
            m 
          </mi> 
         </msub> 
         <mtext>
           d 
         </mtext> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            l 
          </mi> 
         </mstyle> 
         <mo>
           × 
         </mo> 
         <msub> 
          <mstyle mathvariant="bold" mathsize="normal"> 
           <mi>
             r 
           </mi> 
          </mstyle> 
          <mn>
            0 
          </mn> 
         </msub> 
        </mrow> 
        <mrow> 
         <msup> 
          <mi>
            r 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math>(12)</p>
    <p>where 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mrow> 
        <mrow> 
         <msub> 
          <mi>
            ξ 
          </mi> 
          <mn>
            0 
          </mn> 
         </msub> 
        </mrow> 
        <mo>
          / 
        </mo> 
        <mrow> 
         <mn>
           4 
         </mn> 
         <mi>
           π 
         </mi> 
        </mrow> 
       </mrow> 
      </mrow> 
     </math> is proportional constant. The negative sign in the right side of this formula indicates that the wagnetic field obeys the left-handed rule. On one hand, Newton’s equation of gravitational field and Coulomb’s equation of electrostatic field have similar algebraic forms (parity); on the other hand, 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mtext>
         d 
       </mtext> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          W 
        </mi> 
       </mstyle> 
      </mrow> 
     </math> and 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mtext>
         d 
       </mtext> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
      </mrow> 
     </math> share a similar algebraic form (parity). This suggests that we can describe the properties of the gravitowagnetic field using force lines, which can be likened to an incompressible fluid. Helmholtz theorem provides a theoretical reason for the existence of wagnetic field. By vector properties, the gravitational field is a longitudinal field like electrostatic field, and wagnetic field is a transverse field like magnetic field.</p>
    <p>Helmholtz’s theorem is only applicable vector fields in an infinite space <xref ref-type="bibr" rid="scirp.138766-4">
      [4]
     </xref>. It also indicates that: 1) a vector field in an infinite space is uniquely determined by its divergence and rotation. If both the divergence and rotation of a vector are zero, the vector field also vanish; 2) any vector field can be expressed by the sum of an irrotational field and a non-divergence field. The existence of electromagnetic waves indicates that the electromagnetic field conforms to this theorem. In recent years, gravitational waves have been detected, reminding us that the vector field excited by mass may also conform to this theorem. Introduce the scalar potential and vector potential, and represent the field excited by mas as</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          G 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mo>
         ∇ 
       </mo> 
       <msub> 
        <mi>
          φ 
        </mi> 
        <mi>
          m 
        </mi> 
       </msub> 
      </mrow> 
     </math>, 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          W 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         × 
       </mo> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           A 
         </mi> 
        </mstyle> 
        <mi>
          m 
        </mi> 
       </msub> 
      </mrow> 
     </math>(13)</p>
    <p>where 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         G 
       </mi> 
      </mstyle> 
     </math> is static gravitational field, 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         W 
       </mi> 
      </mstyle> 
     </math> is steady-state wagnetic field, 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          φ 
        </mi> 
        <mi>
          m 
        </mi> 
       </msub> 
      </mrow> 
     </math> is scalar potential, and 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           A 
         </mi> 
        </mstyle> 
        <mi>
          m 
        </mi> 
       </msub> 
      </mrow> 
     </math> is vector potential. For fields excited by electric charge, there are interactions between charges of the same sign as well between charges of opposite signs. For fields excited by mass, there is no interaction between negative mass and mass; there is only interaction between the masses of two objects. Therefore, the interaction between the masses of two objects is similar to the interaction two electric charges of the same sign. The difference lies in the fact that the force related to mass is gravitational, while the force related to electric charge is repulse. This means that the gravitowagnetic field follows left-handed rules.</p>
    <p>The experimental law of magnetic induction intensity states</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         × 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <mn>
           4 
         </mn> 
         <mi>
           π 
         </mi> 
        </mrow> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           j 
         </mi> 
        </mstyle> 
        <mn>
          0 
        </mn> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mrow> 
         <mn>
           4 
         </mn> 
         <mi>
           π 
         </mi> 
        </mrow> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           j 
         </mi> 
        </mstyle> 
        <mi>
          e 
        </mi> 
       </msub> 
      </mrow> 
     </math>(14)</p>
    <p>where 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           j 
         </mi> 
        </mstyle> 
        <mi>
          e 
        </mi> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           j 
         </mi> 
        </mstyle> 
        <mn>
          0 
        </mn> 
       </msub> 
      </mrow> 
     </math>, 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           j 
         </mi> 
        </mstyle> 
        <mn>
          0 
        </mn> 
       </msub> 
      </mrow> 
     </math> is current density, 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           j 
         </mi> 
        </mstyle> 
        <mi>
          e 
        </mi> 
       </msub> 
      </mrow> 
     </math> is current density contributed by electronic charges, the corresponding electronic mass flux density is 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           j 
         </mi> 
        </mstyle> 
        <mi>
          m 
        </mi> 
       </msub> 
      </mrow> 
     </math>, which has the same direction as 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           j 
         </mi> 
        </mstyle> 
        <mi>
          e 
        </mi> 
       </msub> 
      </mrow> 
     </math>, So</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         × 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          W 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mrow> 
         <mn>
           4 
         </mn> 
         <mi>
           π 
         </mi> 
        </mrow> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           j 
         </mi> 
        </mstyle> 
        <mi>
          m 
        </mi> 
       </msub> 
      </mrow> 
     </math>(15)</p>
   </sec>
   <sec id="s2_3">
    <title>2.3. The F Law and M Law in Gravitowagnetic Field</title>
    <p>During the transition from a high energy orbit to a low energy orbit, an electron emits electromagnetic wave. Since the speed of the wave is limited, the electromagnetic wave continues to propagate after the transition is complete, and the received radiation wave can be considered as a source-free wave. After the process of gravitowagnetic waves generated in the distant depths of the universe has ended, the Earth receives this radiation waves, and therefore it is also considered a source-free waves. Since the properties of 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         G 
       </mi> 
      </mstyle> 
     </math> and 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         W 
       </mi> 
      </mstyle> 
     </math> are similar to those of 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         E 
       </mi> 
      </mstyle> 
     </math> and 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         B 
       </mi> 
      </mstyle> 
     </math>, we can write similar wave equations,</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msup> 
        <mo>
          ∇ 
        </mo> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          G 
        </mi> 
       </mstyle> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msup> 
          <mi>
            c 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            2 
          </mn> 
         </msup> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            G 
          </mi> 
         </mstyle> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <msup> 
          <mi>
            t 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>(16)</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msup> 
        <mo>
          ∇ 
        </mo> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          W 
        </mi> 
       </mstyle> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msup> 
          <mi>
            c 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            2 
          </mn> 
         </msup> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            W 
          </mi> 
         </mstyle> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <msup> 
          <mi>
            t 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>(17)</p>
    <p>The corresponding Poynting vector (obeys the left-handed rule) is</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           S 
         </mi> 
        </mstyle> 
        <mi>
          m 
        </mi> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mi>
          c 
        </mi> 
        <mrow> 
         <mn>
           4 
         </mn> 
         <mi>
           π 
         </mi> 
        </mrow> 
       </mfrac> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          G 
        </mi> 
       </mstyle> 
       <mo>
         × 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          W 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mi>
          c 
        </mi> 
        <mrow> 
         <mn>
           4 
         </mn> 
         <mi>
           π 
         </mi> 
        </mrow> 
       </mfrac> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          W 
        </mi> 
       </mstyle> 
       <mo>
         × 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          G 
        </mi> 
       </mstyle> 
      </mrow> 
     </math>(18)</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           S 
         </mi> 
        </mstyle> 
        <mi>
          m 
        </mi> 
       </msub> 
      </mrow> 
     </math> is parallel to z-axis. The plane wave solutions fro equations (16) and (17) are</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          G 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mi>
            G 
          </mi> 
          <mrow> 
           <mi>
             max 
           </mi> 
          </mrow> 
         </msub> 
         <mo>
           ⋅ 
         </mo> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            j 
          </mi> 
         </mstyle> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mi>
         sin 
       </mi> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mi>
            k 
          </mi> 
          <mi>
            z 
          </mi> 
         </msub> 
         <mo>
           ⋅ 
         </mo> 
         <mi>
           z 
         </mi> 
         <mo>
           − 
         </mo> 
         <mi>
           ω 
         </mi> 
         <mi>
           t 
         </mi> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <msub> 
        <mi>
          G 
        </mi> 
        <mi>
          y 
        </mi> 
       </msub> 
       <mo>
         ⋅ 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          j 
        </mi> 
       </mstyle> 
      </mrow> 
     </math>(19)</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          W 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mi>
            W 
          </mi> 
          <mrow> 
           <mi>
             max 
           </mi> 
          </mrow> 
         </msub> 
         <mo>
           ⋅ 
         </mo> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            i 
          </mi> 
         </mstyle> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mi>
         sin 
       </mi> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mi>
            k 
          </mi> 
          <mi>
            z 
          </mi> 
         </msub> 
         <mo>
           ⋅ 
         </mo> 
         <mi>
           z 
         </mi> 
         <mo>
           − 
         </mo> 
         <mi>
           ω 
         </mi> 
         <mi>
           t 
         </mi> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <msub> 
        <mi>
          W 
        </mi> 
        <mi>
          x 
        </mi> 
       </msub> 
       <mo>
         ⋅ 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          i 
        </mi> 
       </mstyle> 
      </mrow> 
     </math>(20)</p>
    <p>where 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          G 
        </mi> 
        <mrow> 
         <mi>
           max 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <msub> 
        <mi>
          W 
        </mi> 
        <mrow> 
         <mi>
           max 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math>, 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         i 
       </mi> 
      </mstyle> 
     </math> and 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         j 
       </mi> 
      </mstyle> 
     </math> are basis vectors of the x-axis and y-axis, 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          k 
        </mi> 
        <mi>
          z 
        </mi> 
       </msub> 
      </mrow> 
     </math> is wave vector in the z-axis, 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        ω 
      </mi> 
     </math> is frequency, 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          k 
        </mi> 
        <mi>
          z 
        </mi> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mi>
         ω 
       </mi> 
       <mi>
         c 
       </mi> 
      </mrow> 
     </math>,</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         × 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          G 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           − 
         </mo> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            i 
          </mi> 
         </mstyle> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <msub> 
        <mi>
          G 
        </mi> 
        <mrow> 
         <mi>
           max 
         </mi> 
        </mrow> 
       </msub> 
       <mi>
         cos 
       </mi> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mi>
            k 
          </mi> 
          <mi>
            z 
          </mi> 
         </msub> 
         <mo>
           ⋅ 
         </mo> 
         <mi>
           z 
         </mi> 
         <mo>
           − 
         </mo> 
         <mi>
           ω 
         </mi> 
         <mi>
           t 
         </mi> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          k 
        </mi> 
        <mi>
          z 
        </mi> 
       </msub> 
      </mrow> 
     </math>(21)</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mfrac> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            W 
          </mi> 
         </mstyle> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mi>
            W 
          </mi> 
          <mrow> 
           <mi>
             max 
           </mi> 
          </mrow> 
         </msub> 
         <mo>
           ⋅ 
         </mo> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            i 
          </mi> 
         </mstyle> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mi>
         cos 
       </mi> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mi>
            k 
          </mi> 
          <mi>
            z 
          </mi> 
         </msub> 
         <mo>
           ⋅ 
         </mo> 
         <mi>
           z 
         </mi> 
         <mo>
           − 
         </mo> 
         <mi>
           ω 
         </mi> 
         <mi>
           t 
         </mi> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         ⋅ 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           − 
         </mo> 
         <mi>
           ω 
         </mi> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
      </mrow> 
     </math>(22)</p>
    <p>From Equations (21) and (22), we get the F law for the gravitowagnetic field</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         × 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          G 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            W 
          </mi> 
         </mstyle> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math>(23)</p>
    <p>With the same reason, the relevant M law is</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         × 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          W 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            G 
          </mi> 
         </mstyle> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math>(24)</p>
    <p>In contrast to the F law and M law of electromagnetic field, the F law and M law embody compliance and resistance, respectively.</p>
   </sec>
  </sec><sec id="s3">
   <title>3. Discussion</title>
   <sec id="s3_1">
    <title>3.1. General Maxwell’s Equations</title>
    <p>General Maxwell’s equations include electromagnetic field equations and gravitowagnetic field equations,</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         ⋅ 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mn>
         4 
       </mn> 
       <mi>
         π 
       </mi> 
       <msub> 
        <mi>
          ρ 
        </mi> 
        <mtext>
          0 
        </mtext> 
       </msub> 
      </mrow> 
     </math>, 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         − 
       </mo> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         ⋅ 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          G 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mn>
         4 
       </mn> 
       <mi>
         π 
       </mi> 
       <msub> 
        <mi>
          ρ 
        </mi> 
        <mi>
          m 
        </mi> 
       </msub> 
      </mrow> 
     </math>(25)</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         × 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            B 
          </mi> 
         </mstyle> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math>, 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         − 
       </mo> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         × 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          G 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            W 
          </mi> 
         </mstyle> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math>(26)</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         ⋅ 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>, 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         ⋅ 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          W 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>(27)</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         × 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            E 
          </mi> 
         </mstyle> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         + 
       </mo> 
       <mfrac> 
        <mrow> 
         <mn>
           4 
         </mn> 
         <mi>
           π 
         </mi> 
        </mrow> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           j 
         </mi> 
        </mstyle> 
        <mtext>
          0 
        </mtext> 
       </msub> 
      </mrow> 
     </math>, 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         − 
       </mo> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         × 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          W 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            G 
          </mi> 
         </mstyle> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         + 
       </mo> 
       <mfrac> 
        <mrow> 
         <mn>
           4 
         </mn> 
         <mi>
           π 
         </mi> 
        </mrow> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           j 
         </mi> 
        </mstyle> 
        <mi>
          m 
        </mi> 
       </msub> 
      </mrow> 
     </math>(28)</p>
    <p>The equations indicate that electromagnetic field and gravitowagnetic field maintain the parity of the excited vacuum, with no overall time reversal, meaning time maintains a forward direction. Locally, there is time reversal and parity violation, where a weak force field exists. Such states exist only momentarily and do not interfere with the overall parity and unidirectionality of time. As T. D. Lee pointed out: symmetry breaking is observable and there should exist field and force that disrupt symmetry <xref ref-type="bibr" rid="scirp.138766-7">
      [7]
     </xref>. To date, no force or field has been observed that violates the vacuum excitation-state’s parity on a large scale. Here it needs to be emphasized that parity is a property of topological space, and it’s not related to numerical value because measure is not a topological quantity, a topological space can exist without a metric.</p>
   </sec>
   <sec id="s3_2">
    <title>3.2. Lorenz Gauge in Gravitowagnetic Field</title>
    <p>The F law and M law should exhibit transport characteristics, from which the wave equations can be derived.</p>
    <p>Take the time derivative of the second equation in (28), then substitute the second equation of (26) into the differential expression to eliminate 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         W 
       </mi> 
      </mstyle> 
     </math>,</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msup> 
          <mi>
            c 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            2 
          </mn> 
         </msup> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            G 
          </mi> 
         </mstyle> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <msup> 
          <mi>
            t 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         × 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           ∇ 
         </mo> 
         <mo>
           × 
         </mo> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            G 
          </mi> 
         </mstyle> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mrow> 
         <mn>
           4 
         </mn> 
         <mi>
           π 
         </mi> 
        </mrow> 
        <mrow> 
         <msup> 
          <mi>
            c 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <msub> 
          <mstyle mathvariant="bold" mathsize="normal"> 
           <mi>
             j 
           </mi> 
          </mstyle> 
          <mi>
            m 
          </mi> 
         </msub> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math>(29)</p>
    <p>Using the formula of vectors 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         × 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           ∇ 
         </mo> 
         <mo>
           × 
         </mo> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            G 
          </mi> 
         </mstyle> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mo>
         ∇ 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           ∇ 
         </mo> 
         <mo>
           ⋅ 
         </mo> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            G 
          </mi> 
         </mstyle> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         − 
       </mo> 
       <msup> 
        <mo>
          ∇ 
        </mo> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          G 
        </mi> 
       </mstyle> 
      </mrow> 
     </math>, get active wave equation,</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msup> 
        <mo>
          ∇ 
        </mo> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          G 
        </mi> 
       </mstyle> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msup> 
          <mi>
            c 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            2 
          </mn> 
         </msup> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            G 
          </mi> 
         </mstyle> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <msup> 
          <mi>
            t 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mn>
         4 
       </mn> 
       <mi>
         π 
       </mi> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           − 
         </mo> 
         <mo>
           ∇ 
         </mo> 
         <msub> 
          <mi>
            ρ 
          </mi> 
          <mi>
            m 
          </mi> 
         </msub> 
         <mo>
           + 
         </mo> 
         <mfrac> 
          <mn>
            1 
          </mn> 
          <mrow> 
           <msup> 
            <mi>
              c 
            </mi> 
            <mn>
              2 
            </mn> 
           </msup> 
          </mrow> 
         </mfrac> 
         <mfrac> 
          <mrow> 
           <mo>
             ∂ 
           </mo> 
           <msub> 
            <mstyle mathvariant="bold" mathsize="normal"> 
             <mi>
               j 
             </mi> 
            </mstyle> 
            <mi>
              m 
            </mi> 
           </msub> 
          </mrow> 
          <mrow> 
           <mo>
             ∂ 
           </mo> 
           <mi>
             t 
           </mi> 
          </mrow> 
         </mfrac> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
      </mrow> 
     </math>(30)</p>
    <p>The radiation wave equation is</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msup> 
        <mo>
          ∇ 
        </mo> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          G 
        </mi> 
       </mstyle> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msup> 
          <mi>
            c 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            2 
          </mn> 
         </msup> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            G 
          </mi> 
         </mstyle> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <msup> 
          <mi>
            t 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>(31)</p>
    <p>Similarly, for the 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         W 
       </mi> 
      </mstyle> 
     </math></p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msup> 
        <mo>
          ∇ 
        </mo> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          W 
        </mi> 
       </mstyle> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msup> 
          <mi>
            c 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            2 
          </mn> 
         </msup> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            W 
          </mi> 
         </mstyle> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <msup> 
          <mi>
            t 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <mn>
           4 
         </mn> 
         <mi>
           π 
         </mi> 
        </mrow> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           j 
         </mi> 
        </mstyle> 
        <mi>
          m 
        </mi> 
       </msub> 
      </mrow> 
     </math>(32)</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msup> 
        <mo>
          ∇ 
        </mo> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          W 
        </mi> 
       </mstyle> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msup> 
          <mi>
            c 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            2 
          </mn> 
         </msup> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            W 
          </mi> 
         </mstyle> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <msup> 
          <mi>
            t 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>(33)</p>
    <p>Apart from the plane wave solutions, Equations (31) and (33) also have other forms of solutions. This indicates that the F law and M law are universally applicable, even though they were derived from the solutions for plane waves. Using the second formula of (13) and Equation (23), we get 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         × 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            G 
          </mi> 
         </mstyle> 
         <mo>
           + 
         </mo> 
         <mfrac> 
          <mn>
            1 
          </mn> 
          <mi>
            c 
          </mi> 
         </mfrac> 
         <mfrac> 
          <mrow> 
           <mo>
             ∂ 
           </mo> 
           <msub> 
            <mstyle mathvariant="bold" mathsize="normal"> 
             <mi>
               A 
             </mi> 
            </mstyle> 
            <mi>
              m 
            </mi> 
           </msub> 
          </mrow> 
          <mrow> 
           <mo>
             ∂ 
           </mo> 
           <mi>
             t 
           </mi> 
          </mrow> 
         </mfrac> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>, the brackets enclose a longitudinal field, referring to the first formula of Equation (13) and noticing the parity of 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         G 
       </mi> 
      </mstyle> 
     </math> and 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         E 
       </mi> 
      </mstyle> 
     </math>:</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <mo>
         ∇ 
       </mo> 
       <msub> 
        <mi>
          φ 
        </mi> 
        <mi>
          e 
        </mi> 
       </msub> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <msub> 
          <mstyle mathvariant="bold" mathsize="normal"> 
           <mi>
             A 
           </mi> 
          </mstyle> 
          <mi>
            e 
          </mi> 
         </msub> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math>, it can be represented as 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         ∇ 
       </mo> 
       <msub> 
        <mi>
          φ 
        </mi> 
        <mi>
          m 
        </mi> 
       </msub> 
      </mrow> 
     </math>, and</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          G 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mo>
         ∇ 
       </mo> 
       <msub> 
        <mi>
          φ 
        </mi> 
        <mi>
          m 
        </mi> 
       </msub> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <msub> 
          <mstyle mathvariant="bold" mathsize="normal"> 
           <mi>
             A 
           </mi> 
          </mstyle> 
          <mi>
            m 
          </mi> 
         </msub> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math>(34)</p>
    <p>Substituting Equation (34) into the second formula of Equation (25), we obtain the wave equation of the scalar vector,</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msup> 
        <mo>
          ∇ 
        </mo> 
        <mn>
          2 
        </mn> 
       </msup> 
       <msub> 
        <mi>
          φ 
        </mi> 
        <mi>
          m 
        </mi> 
       </msub> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msup> 
          <mi>
            c 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            2 
          </mn> 
         </msup> 
         <msub> 
          <mi>
            φ 
          </mi> 
          <mi>
            m 
          </mi> 
         </msub> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <msup> 
          <mi>
            t 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <mn>
         4 
       </mn> 
       <mi>
         π 
       </mi> 
       <msub> 
        <mi>
          ρ 
        </mi> 
        <mi>
          m 
        </mi> 
       </msub> 
      </mrow> 
     </math>(35)</p>
    <p>The radiation wave equation is</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msup> 
        <mo>
          ∇ 
        </mo> 
        <mn>
          2 
        </mn> 
       </msup> 
       <msub> 
        <mi>
          φ 
        </mi> 
        <mi>
          m 
        </mi> 
       </msub> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msup> 
          <mi>
            c 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            2 
          </mn> 
         </msup> 
         <msub> 
          <mi>
            φ 
          </mi> 
          <mi>
            m 
          </mi> 
         </msub> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <msup> 
          <mi>
            t 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>(36)</p>
    <p>On the other hand, Equation (35) can be rewritten as</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <mfrac> 
        <mo>
          ∂ 
        </mo> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
       <mrow> 
        <mo>
          [ 
        </mo> 
        <mrow> 
         <mo>
           − 
         </mo> 
         <mo>
           ∇ 
         </mo> 
         <mo>
           ⋅ 
         </mo> 
         <msub> 
          <mstyle mathvariant="bold" mathsize="normal"> 
           <mi>
             A 
           </mi> 
          </mstyle> 
          <mi>
            m 
          </mi> 
         </msub> 
         <mo>
           + 
         </mo> 
         <mfrac> 
          <mn>
            1 
          </mn> 
          <mi>
            c 
          </mi> 
         </mfrac> 
         <mfrac> 
          <mrow> 
           <mo>
             ∂ 
           </mo> 
           <msub> 
            <mi>
              φ 
            </mi> 
            <mi>
              m 
            </mi> 
           </msub> 
          </mrow> 
          <mrow> 
           <mo>
             ∂ 
           </mo> 
           <mi>
             t 
           </mi> 
          </mrow> 
         </mfrac> 
        </mrow> 
        <mo>
          ] 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>(37)</p>
    <p>The sum of the two terms in brackets of the formula is constant, let it be zero,</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         − 
       </mo> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           A 
         </mi> 
        </mstyle> 
        <mi>
          m 
        </mi> 
       </msub> 
       <mo>
         + 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <msub> 
          <mi>
            A 
          </mi> 
          <mi>
            m 
          </mi> 
         </msub> 
         <msub> 
          <mrow></mrow> 
          <mi>
            m 
          </mi> 
         </msub> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>(38)</p>
    <p>This is the Lorenz gauge for the gravitowagnetic field. Below, we prove the rationality of the Lorenz gauge. Let the left side of Equation (38) be</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mrow> 
         <mrow> 
          <mi>
            H 
          </mi> 
          <mo>
            | 
          </mo> 
         </mrow> 
        </mrow> 
        <mrow> 
         <mi>
           t 
         </mi> 
         <mo>
           = 
         </mo> 
         <mn>
           0 
         </mn> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <msub> 
        <mrow> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mo>
             − 
           </mo> 
           <mo>
             ∇ 
           </mo> 
           <mo>
             ⋅ 
           </mo> 
           <msub> 
            <mstyle mathvariant="bold" mathsize="normal"> 
             <mi>
               A 
             </mi> 
            </mstyle> 
            <mi>
              m 
            </mi> 
           </msub> 
           <mo>
             + 
           </mo> 
           <mfrac> 
            <mn>
              1 
            </mn> 
            <mi>
              c 
            </mi> 
           </mfrac> 
           <mfrac> 
            <mrow> 
             <mo>
               ∂ 
             </mo> 
             <msub> 
              <mi>
                A 
              </mi> 
              <mi>
                m 
              </mi> 
             </msub> 
             <msub> 
              <mrow></mrow> 
              <mi>
                m 
              </mi> 
             </msub> 
            </mrow> 
            <mrow> 
             <mo>
               ∂ 
             </mo> 
             <mi>
               t 
             </mi> 
            </mrow> 
           </mfrac> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
        </mrow> 
        <mrow> 
         <mi>
           t 
         </mi> 
         <mo>
           = 
         </mo> 
         <mn>
           0 
         </mn> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>(39)</p>
    <p>If 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        H 
      </mi> 
     </math> meets this initial condition, then at any given moment 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         H 
       </mi> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>. From the derivation of the Lorenz gauge, it is known that the initial values must satisfy the following equation</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mrow> 
         <mrow> 
          <mo>
            [ 
          </mo> 
          <mrow> 
           <mo>
             − 
           </mo> 
           <mfrac> 
            <mn>
              1 
            </mn> 
            <mi>
              c 
            </mi> 
           </mfrac> 
           <mfrac> 
            <mo>
              ∂ 
            </mo> 
            <mrow> 
             <mo>
               ∂ 
             </mo> 
             <mi>
               t 
             </mi> 
            </mrow> 
           </mfrac> 
           <mrow> 
            <mo>
              ( 
            </mo> 
            <mrow> 
             <mo>
               ∇ 
             </mo> 
             <mo>
               ⋅ 
             </mo> 
             <msub> 
              <mstyle mathvariant="bold" mathsize="normal"> 
               <mi>
                 A 
               </mi> 
              </mstyle> 
              <mi>
                m 
              </mi> 
             </msub> 
            </mrow> 
            <mo>
              ) 
            </mo> 
           </mrow> 
           <mo>
             + 
           </mo> 
           <msup> 
            <mo>
              ∇ 
            </mo> 
            <mn>
              2 
            </mn> 
           </msup> 
           <msub> 
            <mi>
              φ 
            </mi> 
            <mi>
              m 
            </mi> 
           </msub> 
           <mo>
             + 
           </mo> 
           <mn>
             4 
           </mn> 
           <mi>
             π 
           </mi> 
           <msub> 
            <mi>
              ρ 
            </mi> 
            <mi>
              m 
            </mi> 
           </msub> 
          </mrow> 
          <mo>
            ] 
          </mo> 
         </mrow> 
        </mrow> 
        <mrow> 
         <mi>
           t 
         </mi> 
         <mo>
           = 
         </mo> 
         <mn>
           0 
         </mn> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>(40)</p>
    <p>Combine (39), get</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mrow> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mo>
             ∇ 
           </mo> 
           <mo>
             ⋅ 
           </mo> 
           <mstyle mathvariant="bold" mathsize="normal"> 
            <mi>
              G 
            </mi> 
           </mstyle> 
           <mo>
             + 
           </mo> 
           <mn>
             4 
           </mn> 
           <mi>
             π 
           </mi> 
           <msub> 
            <mi>
              ρ 
            </mi> 
            <mi>
              m 
            </mi> 
           </msub> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
        </mrow> 
        <mrow> 
         <mi>
           t 
         </mi> 
         <mo>
           = 
         </mo> 
         <mn>
           0 
         </mn> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>(41)</p>
    <p>Substitute Equation (35) into (40), get</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mrow> 
         <mrow> 
          <mrow> 
           <mfrac> 
            <mrow> 
             <mo>
               ∂ 
             </mo> 
             <mi>
               H 
             </mi> 
            </mrow> 
            <mrow> 
             <mo>
               ∂ 
             </mo> 
             <mi>
               t 
             </mi> 
            </mrow> 
           </mfrac> 
          </mrow> 
          <mo>
            | 
          </mo> 
         </mrow> 
        </mrow> 
        <mrow> 
         <mi>
           t 
         </mi> 
         <mo>
           = 
         </mo> 
         <mn>
           0 
         </mn> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>(42)</p>
    <p>Take the derivation of the wave equation of 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          φ 
        </mi> 
        <mi>
          m 
        </mi> 
       </msub> 
      </mrow> 
     </math> with respect to 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        t 
      </mi> 
     </math>, and then take the divergence of the wave equation of 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           A 
         </mi> 
        </mstyle> 
        <mi>
          m 
        </mi> 
       </msub> 
      </mrow> 
     </math>, get</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msup> 
        <mo>
          ∇ 
        </mo> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mi>
         H 
       </mi> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msup> 
          <mi>
            c 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            2 
          </mn> 
         </msup> 
         <mi>
           H 
         </mi> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <msup> 
          <mi>
            t 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <mn>
           4 
         </mn> 
         <mi>
           π 
         </mi> 
        </mrow> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           ∇ 
         </mo> 
         <mo>
           ⋅ 
         </mo> 
         <msub> 
          <mstyle mathvariant="bold" mathsize="normal"> 
           <mi>
             j 
           </mi> 
          </mstyle> 
          <mi>
            m 
          </mi> 
         </msub> 
         <mo>
           + 
         </mo> 
         <mfrac> 
          <mrow> 
           <mo>
             ∂ 
           </mo> 
           <msub> 
            <mi>
              ρ 
            </mi> 
            <mi>
              m 
            </mi> 
           </msub> 
          </mrow> 
          <mrow> 
           <mo>
             ∂ 
           </mo> 
           <mi>
             t 
           </mi> 
          </mrow> 
         </mfrac> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
      </mrow> 
     </math>(43)</p>
    <p>The two terms within the parentheses on the right side of Equation (43) precisely form the mass continuity equation, which equals zero when mass is conservation. 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        H 
      </mi> 
     </math> satisfies the homogeneous wave equation</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msup> 
        <mo>
          ∇ 
        </mo> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mi>
         H 
       </mi> 
       <mo>
         − 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msup> 
          <mi>
            c 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            2 
          </mn> 
         </msup> 
         <mi>
           H 
         </mi> 
        </mrow> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <msup> 
          <mi>
            t 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>(44)</p>
    <p>Combining Equations (38) and (39), it can be derived that 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         H 
       </mi> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math> at any time. Therefore, under the condition of mass conservation, the Lorenz gauge holds true.</p>
   </sec>
   <sec id="s3_3">
    <title>3.3. Lorentz Force in the Wagnetic Field</title>
    <p>The generalized Maxwell’s equations indicate that the wagnetic field and the magnetic field have similar properties. Therefore, we believe that there is an action of the wagnetic field on moving mass, analogous to the action of the magnetic field on moving charges. We collectively refer to this force as the Lorentz force 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           f 
         </mi> 
        </mstyle> 
        <mi>
          g 
        </mi> 
       </msub> 
      </mrow> 
     </math>,</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           f 
         </mi> 
        </mstyle> 
        <mi>
          g 
        </mi> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <mi>
         m 
       </mi> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          v 
        </mi> 
       </mstyle> 
       <mo>
         × 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          W 
        </mi> 
       </mstyle> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          p 
        </mi> 
       </mstyle> 
       <mo>
         × 
       </mo> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          W 
        </mi> 
       </mstyle> 
      </mrow> 
     </math>(45)</p>
    <p>where 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         v 
       </mi> 
      </mstyle> 
     </math> is velocity, 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         p 
       </mi> 
      </mstyle> 
     </math> is momentum, and the negative sign indicates that the force conforms the let-handed rule.</p>
    <p>The diameter of the Sun is about 1.39 million kilometers, which is 109 times that of the Earth’s diameter. The volume of the Sun is 1.3 million times that of the Earth, and its mass is 330,000 times that of the Earth. The Sun is a star located at the center of the solar system and is almost an ideal sphere. Due to the presence of flowing hot plasma, the wagnetic field generated by its rotation fluctuates unpredictably in space, resembling an alternating field. The photons emitted from the Sun may exhibit a precession similar to that electrons in an alternating magnetic field, under the action of the Lorentz force of the alternating wagnetic field. In addition, the influence of the Sun’s wagnetic field on Mercury’s motion cannot be ignored when calculating the position of Mercury’s perihelion.</p>
    <p>When photons approach a massive star in the universe, they are subjected to the Lorentz force of the wagnetic field of the rotating star, causing the path of light to bend. The more higher the frequency, the more the momentum, and the more curved the path.</p>
    <fig id="fig1" position="float">
     <label>Figure 1</label>
     <caption>
      <title>Figure 1. The Lorentz force experienced by the molecules in the upper layer of the superfluid.</title>
     </caption>
     <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/2181224-rId296.jpeg?20250108085339" />
    </fig>
    <p>Consider the phenomena observed in superfluid experiments. From equation (23), F law, it is known that the wagnetic field induced by the superfluid is aligned with the Earth’s wagnetic field, and the Lorentz force 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           f 
         </mi> 
        </mstyle> 
        <mi>
          g 
        </mi> 
       </msub> 
      </mrow> 
     </math> acting on the upper layer of the superfluid molecules is as illustrated in <xref ref-type="fig" rid="fig1">
      Figure 1
     </xref>, where 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           W 
         </mi> 
        </mstyle> 
        <mi>
          a 
        </mi> 
       </msub> 
      </mrow> 
     </math> is the wagnetic field of the Earth, 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         v 
       </mi> 
      </mstyle> 
     </math> is the velocity of the molecules in the upper fluid layer. In the experiment, on the cross-section perpendicular to 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           W 
         </mi> 
        </mstyle> 
        <mi>
          a 
        </mi> 
       </msub> 
      </mrow> 
     </math>, the liquid circulate in a counterclockwise direction: It is this force that drives the superfluid molecules in the upper layer to climb up the walls of the container. As shown in <xref ref-type="fig" rid="fig1">
      Figure 1
     </xref>, the climbing phenomenon exhibits a distinct directional nature, with no such effect observed on the opposite side of the container. If the force were due to molecular interactions with the container material, the wall climbing phenomenon would be no directionality. Similarly, at the bottom of the container, the superfluid molecules experience a downward Lorentz force from the Earth’s wagnetic field because their velocity direction is opposite to that of the upper layer molecules, causing them to penetrate through the bottom and exit the container. The osmosis also occurs at the side walls parallel to 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           W 
         </mi> 
        </mstyle> 
        <mi>
          a 
        </mi> 
       </msub> 
      </mrow> 
     </math>, with no osmosis at the side walls perpendicular to 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           W 
         </mi> 
        </mstyle> 
        <mi>
          a 
        </mi> 
       </msub> 
      </mrow> 
     </math>. In summary, the phenomena of wall climbing and penetration demonstrate directionality <xref ref-type="bibr" rid="scirp.138766-8">
      [8]
     </xref>.</p>
   </sec>
  </sec><sec id="s4">
   <title>4. Conclusion</title>
   <p>All objects are in motion; what we perceive as stillness is merely relative. Therefore, the fact that moving charges and masses can excite fields is absolute. General Maxwell theory of fields reveals that the vacuum in an excited state maintains global parity. The properties of the gravitowagnetic field will help us gain a profound understanding of the essence of natural phenomena.</p>
  </sec>
 </body><back>
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