<?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><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jhepgc.2017.33034</article-id><article-id pub-id-type="publisher-id">JHEPGC-78065</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Limit Treatment of Space-Time Foam Calculations If Non Pathological Big Bang Singularity Is Accessible to Modified Einstein Equations
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Andrew</surname><given-names>Beckwith</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Physics Department, College of Physics, Chongqing University, Chongqing, China</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>rwill9955b@gmail.com</email></corresp></author-notes><pub-date pub-type="epub"><day>09</day><month>06</month><year>2017</year></pub-date><volume>03</volume><issue>03</issue><fpage>438</fpage><lpage>453</lpage><history><date date-type="received"><day>March</day>	<month>2,</month>	<year>2017</year></date><date date-type="rev-recd"><day>Accepted:</day>	<month>July</month>	<year>26,</year>	</date><date date-type="accepted"><day>July</day>	<month>29,</month>	<year>2017</year></date></history><permissions><copyright-statement>&#169; 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><p><html>
 <head></head>
 
  When initial radius 
  <img src="Edit_78cd4431-55b4-48e6-a155-9757d41ada82.bmp" alt="" /> if Stoica actually derived Einstein equations in a formalism which removes the big bang singularity pathology, then the reason for Planck length no longer holds. We follow what Ng derived as limit calculations as to a space time length factor 
  <img src="Edit_8eca03c2-3702-4439-8325-ab03dd38f630.bmp" alt="" /> Without 
  <img src="Edit_1bf667c4-4f13-4784-ab35-11793927b8f9.bmp" alt="" /> the drop off of the vacuum energy as given by 
  <img src="Edit_0ce6a505-4cb9-4df6-981a-8ddbdc1f21b5.bmp" alt="" /> is at least 
  <img src="Edit_f581912f-138d-458d-b04b-955c4dbf7915.bmp" alt="" /> the value of 
  <img src="Edit_1510c91e-b910-460d-99e7-89d41246e5b1.bmp" alt="" /> . We review the work by Ng as to quantum foam as to how that affects a general expression as to energy 
  <img src="Edit_3c64286e-4d0f-41b1-81bf-126ee719fb8f.bmp" alt="" /> when 
  <img src="Edit_c64c2975-9121-4b65-9ec0-756da9ded749.bmp" alt="" /> , with 
  <img src="Edit_a0a83fb5-31a3-4fcd-b03e-b56ff8dbd459.bmp" alt="" />determined at least approximately by arguments he presented in 2008 in the Dark side of the universe conference. Well before 
  <img src="Edit_6502b868-e8e7-4b34-b3f6-8d97f6e03695.bmp" alt="" /> certain effects make themselves apparent, in ways which are illustrated in the manuscript. Having 
  <img src="Edit_a84c6dfe-85af-4983-8511-6192ebc1c856.bmp" alt="" /> at a point singularity would remove expansion by the scale factor, 
  <img src="Edit_bbbe2196-7878-4a4d-af30-9ee234d80d82.bmp" alt="" /> so that the extreme version of Stoica’s treatment in an isolated 4-dimensional universe would be no expansion at all.
 
</html></p></abstract><kwd-group><kwd>Fjortoft Theorem</kwd><kwd> Thermodynamic Potential</kwd><kwd> Matter Creation</kwd><kwd> Vacuum Energy Mach’s Theorem</kwd><kwd> Non-Pathological Singularity Affecting Einstein Equations</kwd><kwd> Planck Length. Brane Worlds</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>This article is to investigate what happens physically if there is a non pathological singularity.</p><p>At the start of space-time, i.e. no reason to have a minimum nonzero length, the reasons for such a proposal come from [<xref ref-type="bibr" rid="scirp.78065-ref1">1</xref>] by Stoica who may have removed the reason for the development of Planck’s length as a minimum safety net to remove what appears to be unavoidable pathologies at the start of applying the Einstein equations at a space-time singularity. What shows is unavoidable collapse of the usual assumptions of the inter relationships of the number of operations in space-time, of the number of bits, and also of the average energy per bit</p><p>of space time. We will work on the assumption of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x14.png" xlink:type="simple"/></inline-formula> and</p><p>only invoke the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x15.png" xlink:type="simple"/></inline-formula> value to make an extreme point as to back up assertions made earlier, without calculations in a prior paper. Certain physics effects</p><p>make themselves apparent well before <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x16.png" xlink:type="simple"/></inline-formula> limit, and are commented upon</p><p>in this article. <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x17.png" xlink:type="simple"/></inline-formula>in particular is remarked upon. This is a counterpart to Fjortoft theorem in Appendix I.</p></sec><sec id="s2"><title>2. Mach’s Principle as Initially Stated, in EW to Present Day Era. Preserving Planck’s Constant</title><p>We first of all review an earlier proposed Mach’s principle for the Gravitinos in the electro weak era, and then the 2<sup>nd</sup> modern day Mach’s principle, as organized by the author are as seen in [<xref ref-type="bibr" rid="scirp.78065-ref2">2</xref>] . This construction was used in an earlier article to argue in favor of a constant value of h bar, i.e. Planck’s constant. For the sake of review, we will state that the values in</p><disp-formula id="scirp.78065-formula173"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x18.png"  xlink:type="simple"/></disp-formula><p>are really a statement of information conservation. i.e. the amount of information stored in the left hand side of (1) is the same as information as in the right hand side of (1) above. Here, M as in the electro weak era refers to M = N times m, where M is the total “mass” of the gravitinos, N the number of Gravitinos, and R for the electro weak as an infinitely small spatial radius. Whereas the Right hand side is for M for gravitons (not super partner objects) = N as the (number of gravitons) and m (the ultra-low mass of the graviton) in the right hand side of (1). This formula (1) should be compared with a change in entropy formula given by Lee [<xref ref-type="bibr" rid="scirp.78065-ref3">3</xref>] about the inter relationship between energy, entropy and temperature as given by</p><disp-formula id="scirp.78065-formula174"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x19.png"  xlink:type="simple"/></disp-formula><p>Lee’s formula is crucial for what we will bring up in the latter part of this document. Namely that changes in initial energy could effectively vanish if [<xref ref-type="bibr" rid="scirp.78065-ref1">1</xref>] is right, i.e. Stoica removing the non-pathological nature of a big bang singularity.</p><p>If the mass m, i.e. for gravitons is set by acceleration (of the net universe) and a change in entropy <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x20.png" xlink:type="simple"/></inline-formula> between the electroweak regime and the final</p><p>entropy value of, if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x21.png" xlink:type="simple"/></inline-formula> for acceleration is used, so then we obtain</p><disp-formula id="scirp.78065-formula175"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x22.png"  xlink:type="simple"/></disp-formula><p>Then we are really forced to look at (1) as a paring between gravitons (today) and gravitons (electro weak) in the sense of preservation of information.</p><p>Having said this, we state that (3) above is based upon certain assumptions usually congruent with the quantum foam model [<xref ref-type="bibr" rid="scirp.78065-ref4">4</xref>] , and that what happens, especially to (3) is profoundly affected as we enter a regime for which</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x23.png" xlink:type="simple"/></inline-formula>. We follow Ng’s derivation [<xref ref-type="bibr" rid="scirp.78065-ref4">4</xref>] to make a cautionary point,</p><p>while removing his worry about black holes, to state something about not only energy E, but also <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x24.png" xlink:type="simple"/></inline-formula> and by extension<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x25.png" xlink:type="simple"/></inline-formula>. As ρ changes</p><p>due to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x26.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x27.png" xlink:type="simple"/></inline-formula>, then<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x28.png" xlink:type="simple"/></inline-formula> is also altered.</p><p>The point we make, is to go to the case of having <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x29.png" xlink:type="simple"/></inline-formula>means there would be no net expansion at all. If the universe were 4 dimensional and closed. We do not take the case of having no initial energy at the beginning of a closed universe as feasible or even realistic to refer to. The information theory implications though of what Stoica implies [<xref ref-type="bibr" rid="scirp.78065-ref1">1</xref>] as to bits and also holography need to be studied.</p><p>What will determine the answer to this question is if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x30.png" xlink:type="simple"/></inline-formula> goes to zero if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x31.png" xlink:type="simple"/></inline-formula> which happens if there is no minimum distance mandated to avoid the pathology of singularity behavior at the heart of the Einstein equations. In doing this, we avoid using the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x32.png" xlink:type="simple"/></inline-formula> situation, and instead refer to a nonzero energy, with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x32.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x33.png" xlink:type="simple"/></inline-formula> instead vanishing.</p></sec><sec id="s3"><title>3. Review of Ng, [<xref ref-type="bibr" rid="scirp.78065-ref4">4</xref>] with Comments</title><p>First of all, Ng refers to the Margolus-Levitin theorem with the rate of operations</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x35.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x35.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x34.png" xlink:type="simple"/></inline-formula>. Ng wishes to avoid black-hole for- mation<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x35.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x34.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x36.png" xlink:type="simple"/></inline-formula>. This last step is not important to our view point, but we</p><p>refer to it to keep fidelity to what Ng brought up in his presentation. Later on, Ng refers to the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x37.png" xlink:type="simple"/></inline-formula> with R<sub>H</sub> the Hubble radius. Next Ng refers to the<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x38.png" xlink:type="simple"/></inline-formula>. Each bit energy is <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x39.png" xlink:type="simple"/></inline-formula> with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x40.png" xlink:type="simple"/></inline-formula></p><p>The key point as seen by Ng [<xref ref-type="bibr" rid="scirp.78065-ref4">4</xref>] and the author is in</p><disp-formula id="scirp.78065-formula176"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x41.png"  xlink:type="simple"/></disp-formula><p>Assuming that E of the universe is not set equal to zero, which the author views as impossible, the above equation says that the number of available bits</p><p>goes down dramatically if one sets <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x42.png" xlink:type="simple"/></inline-formula> Also Ng writesentropy</p><p>S as proportional to a particle count via N.</p><disp-formula id="scirp.78065-formula177"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x43.png"  xlink:type="simple"/></disp-formula><p>We rescale <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x44.png" xlink:type="simple"/></inline-formula> to be</p><disp-formula id="scirp.78065-formula178"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x45.png"  xlink:type="simple"/></disp-formula><p>The upshot is that the entropy, in terms of the number of available particles drops dramatically if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x46.png" xlink:type="simple"/></inline-formula> becomes larger.</p><p>So, as <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x47.png" xlink:type="simple"/></inline-formula> grows smaller, as <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x48.png" xlink:type="simple"/></inline-formula> becomes larger</p><p>1) The initial entropy drops;</p><p>2) The number of bits initially available also drops.</p><p>The limiting case of (4) and (5) in a closed universe, with no higher dimensional embedding is that both would vanish, i.e. appear to go to zero if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x49.png" xlink:type="simple"/></inline-formula> becomes very much larger.</p></sec><sec id="s4"><title>4. Examination of Mitra’s [<xref ref-type="bibr" rid="scirp.78065-ref5">5</xref>] Formation of Mass, Energy and Its Possible Effects on the Cosmological “Constant” Vacuum Energy</title><p>The prior result was to state that Avession’s [<xref ref-type="bibr" rid="scirp.78065-ref6">6</xref>] time varying <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x50.png" xlink:type="simple"/></inline-formula> in fact is a constant value, with no variation as due to alleged behavior represented by Mach’s principle as represented by (1) above. What will be done next will be to look at the role of energy of the universe, and what it says about quintessence. The construction comes from Mitra [<xref ref-type="bibr" rid="scirp.78065-ref5">5</xref>] and is adapted to what Beckwith did with the Machian universe relations [<xref ref-type="bibr" rid="scirp.78065-ref1">1</xref>] as given in (1) to (3) above. Mitra [<xref ref-type="bibr" rid="scirp.78065-ref5">5</xref>] in lieu of working with a FRLW universe, wrote</p><disp-formula id="scirp.78065-formula179"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x51.png"  xlink:type="simple"/></disp-formula><p>The density factor so parlayed in this treatment in the 1<sup>st</sup> equation in (7) was cited to have the relationship [<xref ref-type="bibr" rid="scirp.78065-ref5">5</xref>] by Mitra</p><disp-formula id="scirp.78065-formula180"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x52.png"  xlink:type="simple"/></disp-formula><p>And the author put in, subsequently the following scaling factors</p><disp-formula id="scirp.78065-formula181"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x53.png"  xlink:type="simple"/></disp-formula><p>In addition is the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x54.png" xlink:type="simple"/></inline-formula> associated with the Hubble parameter and all that.</p><p>This leads to the energy value of the last equation of (7) to be written as</p><disp-formula id="scirp.78065-formula182"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x55.png"  xlink:type="simple"/></disp-formula><p>Using a typical cubic solution for real valued roots, this comes out to be:</p><p>If we say that E = M, in the sense of the speed of light being set = 1, then</p><disp-formula id="scirp.78065-formula183"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x56.png"  xlink:type="simple"/></disp-formula><p>This M though is for the total mass of the universe. But still we have</p><disp-formula id="scirp.78065-formula184"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x57.png"  xlink:type="simple"/></disp-formula><p>In so many words, the parameter for quintessence goes to almost zero today, i.e.</p><disp-formula id="scirp.78065-formula185"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x58.png"  xlink:type="simple"/></disp-formula><p>Question to ask is as follows. i.e. look at what the author derived</p><disp-formula id="scirp.78065-formula186"><label>(14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x59.png"  xlink:type="simple"/></disp-formula><p>This equation breaks down if<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x60.png" xlink:type="simple"/></inline-formula>. What would replace it?</p></sec><sec id="s5"><title>5. Does It Make Sense to Talk of Vacuum Energy If <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x61.png" xlink:type="simple"/></inline-formula> Is Changed to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x62.png" xlink:type="simple"/></inline-formula>? Only Answerable Straightforwardly If an Embedding Superstructure Is Assigned. Otherwise Difficult</title><p>The adaptation of the Mitra [<xref ref-type="bibr" rid="scirp.78065-ref5">5</xref>] relation for mass as given by (7) presupposes that there is a well-defined nonzero initial radius for cosmological evolution. We summarize what may be the high lights of this inquiry leading to the present paper as follows.</p><p>1) One could have the situation if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x63.png" xlink:type="simple"/></inline-formula> of an infinite point mass, if there is an initial nonzero energy in the case of just four dimensions and no higher dimensional embedding even if [<xref ref-type="bibr" rid="scirp.78065-ref1">1</xref>] goes through verbatim. The author sees this as unlikely, but is prepared to be wrong. The infinite point mass construction is verbatim if one assumes a closed universe, with no embedding superstructure. Note this appears to nullify the parallel brane world construction author, in lieu of the manuscript sees no reason as to what would perturb this infinite point structure, so as to be able to enter in a big bang era. In such a situation, one would not have vacuum energy.</p><p>2) The most problematic scenario. <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x64.png" xlink:type="simple"/></inline-formula>And no initial cosmological energy, i.e. this in a 4 dimensional closed universe. Then there would be no vacuum energy at all. Initially, a literal completely empties initial state, which is not held to be viable by Volovik [<xref ref-type="bibr" rid="scirp.78065-ref6">6</xref>] .</p><p>3) Finding that additional dimensions are involved, than just 4 dimensions may give credence to the authors speculation as to initial degrees of freedom reaching up to 1000, and the nature of a phase transition from essentially very low degrees of freedom, to over 1000 maybe in fact a chaotic mapping as speculated by the author in 2010 [<xref ref-type="bibr" rid="scirp.78065-ref7">7</xref>] .</p><p>4) What the author would be particularly interested in knowing would be if actual semi classical reasoning could be used to get to an initial prequantum cosmological state. This would be akin to using [<xref ref-type="bibr" rid="scirp.78065-ref8">8</xref>] , but even more to the point, using [<xref ref-type="bibr" rid="scirp.78065-ref9">9</xref>] and [<xref ref-type="bibr" rid="scirp.78065-ref10">10</xref>] , with both these last references relevant to forming Planck’s constant from electromagnetic wave equations. The author points to the enor- mous Electromagnetic fields in the electroweak era as perhaps being part of the background necessary for such a semi classical derivation, plus a possible Octonionic space-time regime, as before inflation flattens space-time, as forming a boundary condition for such constructions to occur [<xref ref-type="bibr" rid="scirp.78065-ref11">11</xref>] .</p><p>The relevant template for examining such questions is given in <xref ref-type="table" rid="table1">Table 1</xref> as printed below.</p><p>5) The meaning of Octonionic geometry prior to the introduction of quantum physics presupposes a form of embedding geometry and in many ways is similar to Penrose’s cyclic conformal cosmology speculation Note the following argument, as:</p><p>6) We are stuck with how a semi classical argument can be used to construct <xref ref-type="table" rid="table1">Table 1</xref> below. In particular, we look at how Planck’s constant is derived, as in the electroweak regime of space-time, for a total derivative [<xref ref-type="bibr" rid="scirp.78065-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.78065-ref10">10</xref>]</p><disp-formula id="scirp.78065-formula187"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x65.png"  xlink:type="simple"/></disp-formula><p>Similarly [<xref ref-type="bibr" rid="scirp.78065-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.78065-ref10">10</xref>]</p><disp-formula id="scirp.78065-formula188"><label>(16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x66.png"  xlink:type="simple"/></disp-formula><p>The A field so given would be part of the Maxwell’s equations given by [<xref ref-type="bibr" rid="scirp.78065-ref9">9</xref>] as, when <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x67.png" xlink:type="simple"/></inline-formula> represents a D’Albertain operator, that in a vacuum, one would have for an A field [<xref ref-type="bibr" rid="scirp.78065-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.78065-ref10">10</xref>]</p><disp-formula id="scirp.78065-formula189"><label>(17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x68.png"  xlink:type="simple"/></disp-formula><p>And for a scalar field <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x69.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.78065-formula190"><label>(18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x70.png"  xlink:type="simple"/></disp-formula><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Time interval dynamical consequences do QM/WdW apply</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Just before Electroweak era</th><th align="center" valign="middle" >Form <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x71.png" xlink:type="simple"/></inline-formula> from early E &amp; M fields, and use Maxwell’s Equations with necessary to implement boundary conditions created from change from Octonionic geometry to flat space</th><th align="center" valign="middle" >NO</th></tr></thead><tr><td align="center" valign="middle" >Electro-Weak Era</td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x72.png" xlink:type="simple"/></inline-formula>kept constant due to Machian relations</td><td align="center" valign="middle" >YES Use (1) as linkage</td></tr><tr><td align="center" valign="middle" >Post Electro-Weak Era to today</td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x73.png" xlink:type="simple"/></inline-formula>kept constant due to Machian relations</td><td align="center" valign="middle" >YES Wave function of Universe</td></tr></tbody></table></table-wrap><p>Following this line of thought we then would have an energy density given by, if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x74.png" xlink:type="simple"/></inline-formula> is the early universe permeability [<xref ref-type="bibr" rid="scirp.78065-ref9">9</xref>]</p><disp-formula id="scirp.78065-formula191"><label>(19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x75.png"  xlink:type="simple"/></disp-formula><p>We integrate (19) over a specified E and M boundary, so that, then we can write the following condition namely [<xref ref-type="bibr" rid="scirp.78065-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.78065-ref10">10</xref>] .</p><disp-formula id="scirp.78065-formula192"><label>(20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x76.png"  xlink:type="simple"/></disp-formula><p>(20) would be integrated over the boundary regime from the transition from the Octonionic regime of space time, to the non Octonionic regime, assuming an abrupt transition occurs, and we can write, the volume integral as representing [<xref ref-type="bibr" rid="scirp.78065-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.78065-ref10">10</xref>]</p><disp-formula id="scirp.78065-formula193"><label>(21)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x77.png"  xlink:type="simple"/></disp-formula><p>Our contention for the rest of this paper, is that Mach’s principle will be necessary as an information storage container so as to keep the following, i.e. having no variation in the Planck’s parameter after its formation from electrodynamics considerations as in (20) and (21). Then by applying [<xref ref-type="bibr" rid="scirp.78065-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.78065-ref10">10</xref>] we get <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x78.png" xlink:type="simple"/></inline-formula>formed by semi classical reasons and need to have Machs principle (1) to have the same value up to the present era.</p><disp-formula id="scirp.78065-formula194"><label>(Constant value) (22)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x79.png"  xlink:type="simple"/></disp-formula><p>The question we can ask, is that can we have a prequantum regime com-</p><p>mencing for (20) and (21) for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x80.png" xlink:type="simple"/></inline-formula> if<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x81.png" xlink:type="simple"/></inline-formula>? And a closed 4 di-</p><p>mensional universe? If so, then what is the necessary geometrical regime of space-time so that the integration performed in (20) can commence properly? Also, what can we say about the formation of (21) above, as a number, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x82.png" xlink:type="simple"/></inline-formula>gets</p><p>larger and larger, effectively leading to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x83.png" xlink:type="simple"/></inline-formula>? We need to know seriously</p><p>how much space-time is needed to form (21) above? Do infinitesimal amounts of space-time suffice in order to fill in the following table as given below? If the</p><p>answer is no, then when <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x84.png" xlink:type="simple"/></inline-formula> leading to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x84.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x85.png" xlink:type="simple"/></inline-formula>,</p><p>the semi classical derivation of (20) leading to (21) may not work. This is the ta-</p><p>ble to consider if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x86.png" xlink:type="simple"/></inline-formula> and not zero. Also,</p><p>with an Octonionic geometry regime which is a pre quantum state [<xref ref-type="bibr" rid="scirp.78065-ref11">11</xref>] .</p><p>In so many words, the formation period for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x87.png" xlink:type="simple"/></inline-formula> is our pre-quantum regime. <xref ref-type="table" rid="table1">Table 1</xref> could even hold if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x87.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x88.png" xlink:type="simple"/></inline-formula> but that the 4 dimensional space-time exhibiting such behavior is embedded in a higher dimensional template.</p></sec><sec id="s6"><title>6. Having Not<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x89.png" xlink:type="simple"/></inline-formula>, But <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x90.png" xlink:type="simple"/></inline-formula> Growing Smaller, as <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x90.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x91.png" xlink:type="simple"/></inline-formula> Becomes Larger</title><p>If there is only an isolated 4 dimensional universe a situation for which:</p><p>1) The initial entropy drops;</p><p>2) The number of bits initially available also drops.</p><p>Then, we argue that dramatically cutting the initial entropy and also the bits would lead to real trouble as far as preserving the formation of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x92.png" xlink:type="simple"/></inline-formula> as given in [<xref ref-type="bibr" rid="scirp.78065-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.78065-ref10">10</xref>] and may lead to difficulties in application of (1) especially if bits for a computation for expansion cannot be formed in a general way at the start of inflation. This uses the ideas in [<xref ref-type="bibr" rid="scirp.78065-ref11">11</xref>] and [<xref ref-type="bibr" rid="scirp.78065-ref12">12</xref>] precisely.</p></sec><sec id="s7"><title>7. If <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x93.png" xlink:type="simple"/></inline-formula> then If There Is an Isolated, Closed Universe, There Is a Messy Situation</title><p>One does not have initial entropy, and the number of bits initially disappears.</p><p>Abandoning the idea of a completely empty universe, this unperturbed point of matter-energy appears to be a recipe for a static point with no perturbation, as may be the end result of applying Fjortoft theorem [<xref ref-type="bibr" rid="scirp.78065-ref13">13</xref>] to the thermodynamic potential as given in [<xref ref-type="bibr" rid="scirp.78065-ref13">13</xref>] , i.e. the non-definitive answer for fulfillment of criteria of instability by applying Fjortoft’s theorem [<xref ref-type="bibr" rid="scirp.78065-ref13">13</xref>] to the potential [<xref ref-type="bibr" rid="scirp.78065-ref11">11</xref>] leading to no instability as given by the potential given in [<xref ref-type="bibr" rid="scirp.78065-ref11">11</xref>] may lead to a point of space-time with no change, i.e. a singular point with “infinite” mass which does not change at all.</p></sec><sec id="s8"><title>8. Can an Alternative to a Minimum Length Be Put in? Consider the Example of Planck Time as the Minimal Component, Not PLANCK Length</title><p>From J. Dickau, the following was given to the author, as a counter part as to how to view thresholds as to how a Mandelbrot set may pre select for critical behavior different from what is being pre supposed in this manuscript [<xref ref-type="bibr" rid="scirp.78065-ref14">14</xref>] .</p><p>Dickau writes:</p><p>“If we examine the Mandelbrot Set along the Real axis, it informs us about behaviors that also pertain in the Quaternion and Octonic case-because the real axis is invariant over the number types. If numbers larger than 0.25 are squared and summed recursively (i.e. ?z = z<sup>2</sup> + c) the result will blow up, but numbers below this threshold never get to infinity, no matter how many times they are iterated. But once space-like dimensions are added i.e. an imaginary component- the equation blows up exponentially, faster than when iterated”.</p><p>Dickau concludes:</p><p>“Anyhow there may be a minimum (space-time length) involved but it is probably in the time direction”.</p><p>This is a counter pose to the idea of minimum length, i.e. the idea being a replacement for what the author put in here: looking at a beginning situation with a crucial parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x94.png" xlink:type="simple"/></inline-formula> even if the initial time step is “put in by hand”. First of all, look at [<xref ref-type="bibr" rid="scirp.78065-ref4">4</xref>] , if E is M, due to setting c = 1, then</p><disp-formula id="scirp.78065-formula195"><label>(23)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x95.png"  xlink:type="simple"/></disp-formula><p>Everything depends upon the parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x96.png" xlink:type="simple"/></inline-formula> which can go to zero. The choice as to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x96.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x97.png" xlink:type="simple"/></inline-formula> going to zero, or not going to zero will be conclusion of our article.</p><p>We have to look at what (23) tells us, even if we have an initial time step for which time is initially indeterminate, as given by a redoing of Mitra’s g<sub>00</sub> formula [<xref ref-type="bibr" rid="scirp.78065-ref4">4</xref>] which we put in to establish the indeterminacy of the initial time step if quantum processes hold.</p><disp-formula id="scirp.78065-formula196"><label>(24)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x98.png"  xlink:type="simple"/></disp-formula><p>What Dickau is promoting is, that the Mandelbrot set, if applicable to early universe geometry, that what the author wrote, with</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x99.png" xlink:type="simple"/></inline-formula>potentially going to zero, is less im-</p><p>portant than a minimum time length. To which the author states, if Dickau is correct as to applicability of the Mandelbrot set, that he, the author is happily corrected, but he also thinks that the Mandelbrot set is a beautiful example of the fungability of space-time metrics used. i.e. how one sets the initial space-time potential is to determine the correctness of the Mandelbrot set. i.e. the [<xref ref-type="bibr" rid="scirp.78065-ref13">13</xref>] reference, as given, by Padmanabhan appears not to have a Mandelbrot set, in its thermodynamic potential. The instability issue is reviewed in Appendix II. For those who are interested in the author’s views as to lack proof of instability. It uses [<xref ref-type="bibr" rid="scirp.78065-ref13">13</xref>] which the author views as THE reference as far as thermodynamic potentials and the early universe.</p></sec><sec id="s9"><title>9. We Need to Reconsider the Role of Quantum Gravity Models at the Onset of Inflation</title><p>We are stuck in all Quantum gravity models as of putting in an initial time step “by hand” so to speak which raises fundamental issues of what would form an initial time step in Quantum gravity. How the transition from the left to the right hand side of (22) occurs is crucial and it comes about because of a transition from Octonionic geometry to quantum accessible and analyzable flat space geometry.</p><p>1) Having not<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x100.png" xlink:type="simple"/></inline-formula>, but <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x101.png" xlink:type="simple"/></inline-formula> grows smaller, as <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x102.png" xlink:type="simple"/></inline-formula></p><p>becomes larger leads to, if there is only an isolated 4 dimensional universe a situation for which:</p><p>The initial entropy drops;</p><p>And the number of bits initially available also drops.</p><p>We argue that dramatically cutting the initial entropy and also the bits would lead to real trouble as far as preserving the invariance of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x103.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.78065-ref15">15</xref>] .</p><p>2) If <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x104.png" xlink:type="simple"/></inline-formula> then if there is an isolated, closed universe, one does not have initialentropy, and the number of bits initially disappears. i.e. in lieu of [<xref ref-type="bibr" rid="scirp.78065-ref11">11</xref>] and [<xref ref-type="bibr" rid="scirp.78065-ref13">13</xref>] there may be no perturbation from an infinite point of space-time which remains invariant.</p></sec><sec id="s10"><title>10. Conclusions</title><p>1) The universe if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x105.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.78065-ref1">1</xref>] and if it is an isolated system, i.e. not as embedded in higher dimensions as referred to in [<xref ref-type="bibr" rid="scirp.78065-ref16">16</xref>] may have no bits, or computations as thought of by Ng [<xref ref-type="bibr" rid="scirp.78065-ref4">4</xref>] . This would be in tandem with the author’s conclusion that one would have an initial infinite point mass and no evolution, and no generation of entropy.</p><p>2) If <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x106.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.78065-ref1">1</xref>] but the universe is embedded in a higher dimensional system, as given by [<xref ref-type="bibr" rid="scirp.78065-ref16">16</xref>] , then there is no reason to say there are no bits, or computations, and the universe will continue to evolve with entropy as a byproduct of that evolution.</p><p>3) The universe if one does not have<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x107.png" xlink:type="simple"/></inline-formula>, i.e. if [<xref ref-type="bibr" rid="scirp.78065-ref1">1</xref>] does not hold, then there will be bits, entropy being generated, and also loop quantum gravity and quantum measures [<xref ref-type="bibr" rid="scirp.78065-ref17">17</xref>] so long as the minimum <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x107.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x108.png" xlink:type="simple"/></inline-formula> Planck length grid exists. The reacceleration of the universe commences as given in [<xref ref-type="bibr" rid="scirp.78065-ref18">18</xref>] due to DE being the same as vacuum energy. The author in Appendix III gives a derivation as to how the DE will be put in, via branes, which holds for both 8b and 8c , as a to be proven sideline.</p><p>4) Appendix IV lists the references that are pertinent to the study of non-linear electrodynamics, which is useful for nonsingular starts to the beginning of the universe, and which is a mainstay of application the Author uses in other parallel publications. The reader is urged to review this partial list which is an important addendum in its own right.</p></sec><sec id="s11"><title>Acknowledgements</title><p>This work is supported in part by National Nature Science Foundation of China Grant No. 11375279.</p></sec><sec id="s12"><title>Cite this paper</title><p>Beckwith, A. (2017) Limit Treatment of Space-Time Foam Calculations If Non Pathological Big Bang Singularity Is Accessible to Modified Einstein Equations. Journal of High Energy Physics, Gravitation and Cosmology, 3, 438- 453. https://doi.org/10.4236/jhepgc.2017.33034</p></sec><sec id="s13"><title>Appendix I. Fjortoft Theorem</title><p>A necessary condition for instability is that if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x109.png" xlink:type="simple"/></inline-formula> is a point in space-time for</p><p>which <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x110.png" xlink:type="simple"/></inline-formula> for any given potential<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x110.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x111.png" xlink:type="simple"/></inline-formula>, then there must be some value <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x110.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x111.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x112.png" xlink:type="simple"/></inline-formula></p><p>in the range <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x113.png" xlink:type="simple"/></inline-formula> such that</p><disp-formula id="scirp.78065-formula197"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x114.png"  xlink:type="simple"/></disp-formula><p>For the proof, see [<xref ref-type="bibr" rid="scirp.78065-ref12">12</xref>] and also consider that the main discussion is to find instability in a physical system which will be described by a given potential<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x115.png" xlink:type="simple"/></inline-formula>. Next, we will construct in the boundary of the EW era, a way to come up with an optimal description for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x115.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x116.png" xlink:type="simple"/></inline-formula></p></sec><sec id="s14"><title>Appendix II. Constructing an Appropriate Potential for Using Fjortoft Theorem in Cosmology for the Early Universe Cannot Be Done. We Show Why</title><p>To do this, we will look at Padamanabhan [<xref ref-type="bibr" rid="scirp.78065-ref12">12</xref>] and his construction of (in Dice 2010) of thermodynamic potentials he used to have another construction of the Einstein GR equations. To start, Padamanabhan [<xref ref-type="bibr" rid="scirp.78065-ref5">5</xref>] wrote</p><p>If <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x117.png" xlink:type="simple"/></inline-formula> is a so called Lovelock entropy tensor, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x117.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x118.png" xlink:type="simple"/></inline-formula> a stress energy tensor</p><disp-formula id="scirp.78065-formula198"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x119.png"  xlink:type="simple"/></disp-formula><p>We now will look at</p><disp-formula id="scirp.78065-formula199"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x120.png"  xlink:type="simple"/></disp-formula><p>So happens that in terms of looking at the partial derivative of the top (1) equation, we are looking at</p><disp-formula id="scirp.78065-formula200"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x121.png"  xlink:type="simple"/></disp-formula><p>Thus, we then will be looking at if there is a specified <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x122.png" xlink:type="simple"/></inline-formula> for which the following holds.</p><disp-formula id="scirp.78065-formula201"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x123.png"  xlink:type="simple"/></disp-formula><p>What this is saying is that there is no unique point, using this <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x124.png" xlink:type="simple"/></inline-formula> for which (4) holds. Therefore, we say there is no official point of instability of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x124.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x125.png" xlink:type="simple"/></inline-formula> due to (3). The Lagrangian structure of what can be built up by the potentials given in (3) with respect to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x124.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x125.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x126.png" xlink:type="simple"/></inline-formula> mean that we cannot expect an inflection point with respect to a 2<sup>nd</sup> derivative of a potential system. Such an inflection point designating a speed up of acceleration due to DE exists a billion years ago [<xref ref-type="bibr" rid="scirp.78065-ref19">19</xref>] . Also note that the reason for the failure for (4) to be congruent to Fjoroft’s theorem is due to</p><disp-formula id="scirp.78065-formula202"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x127.png"  xlink:type="simple"/></disp-formula></sec><sec id="s15"><title>Appendix III. Modifying a Parallel Brane-Anti Brane Argument to Obtain Massive Gravitons</title><p>Part I, of Appendix III. We come into this situation if, as in applying Fjorofts theorem, that we find Appendix II, Equation (5), holds, and then if so, we have to find another way to induce vacuum energy.</p><p>What (5), appendix II tells us is that there is an embedding structure for early universe geometry, some of which may take the form of the following diagram.</p><p>Part II of Appendix III. Working with a way to achieve energy injection into the universe, without appealing to Fjortoft theorem for alleged instabilities starting from Padmanabhan thermodynamic potential terms</p><p>Padmanabhan [<xref ref-type="bibr" rid="scirp.78065-ref13">13</xref>] introduced the following discussion as to entropy, namely starting with energy, we have</p><disp-formula id="scirp.78065-formula203"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x128.png"  xlink:type="simple"/></disp-formula><p>And the n value as in (7) is given by</p><disp-formula id="scirp.78065-formula204"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x129.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x130.png" xlink:type="simple"/></inline-formula> is a so called Lovelock entropy tensor, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x130.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x131.png" xlink:type="simple"/></inline-formula> a bi normal on the codimension −2 cross section, and then entropy is stated to be</p><disp-formula id="scirp.78065-formula205"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x132.png"  xlink:type="simple"/></disp-formula><p>The end result, is that energy is induced via the temperature<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x133.png" xlink:type="simple"/></inline-formula>, while [<xref ref-type="bibr" rid="scirp.78065-ref13">13</xref>]</p><disp-formula id="scirp.78065-formula206"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x134.png"  xlink:type="simple"/></disp-formula><p>Also, the change in n can be given by, if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x135.png" xlink:type="simple"/></inline-formula> is the Planck’s length value [<xref ref-type="bibr" rid="scirp.78065-ref5">5</xref>]</p><disp-formula id="scirp.78065-formula207"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x136.png"  xlink:type="simple"/></disp-formula><p>Looking at (9) and (11) we state that the change in number count given in (4) is really a holographic surface phenomena, with N defined [<xref ref-type="bibr" rid="scirp.78065-ref13">13</xref>]</p><disp-formula id="scirp.78065-formula208"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x137.png"  xlink:type="simple"/></disp-formula><p>The upshot is that we can, as implied by Ng [<xref ref-type="bibr" rid="scirp.78065-ref4">4</xref>] easily reference a change in entropy via [<xref ref-type="bibr" rid="scirp.78065-ref4">4</xref>]</p><disp-formula id="scirp.78065-formula209"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x138.png"  xlink:type="simple"/></disp-formula><p>While having a change in n as due to a change in the spatial surface of space-time as given in (6), we have to realistically infer that the local acceleration temperature (4) is from another pre universe construction and that local instability is ruled out by Appendix II, Equation (5). This leads us to ask as to what would be an acceptable way to form the formation of mass, i.e. say the mass of a graviton, via external factors introduced into our universe prior to the electroweak era, in cosmology. To do that, look at if there are two branes on the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x139.png" xlink:type="simple"/></inline-formula> space-time so that with one moving and one stationary, we can look at <xref ref-type="fig" rid="fig1">Figure 1</xref> as background as to introduce such external factors in our present space-time universe during its initial expansion phase</p><p>Part III, of Appendix III: Fall out from adopting <xref ref-type="fig" rid="fig1">Figure 1</xref> and that due to no instability in the Padamanabhan supplied potentials. i.e. a way to obtain graviton mass via a root finding method.</p><p>Using [<xref ref-type="bibr" rid="scirp.78065-ref16">16</xref>] what we find is that there are two branes on the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x140.png" xlink:type="simple"/></inline-formula> space-time so that with one moving and one stationary, we can look at <xref ref-type="fig" rid="fig1">Figure 1</xref> which is part of the geometry used in the spatial decomposition of the differential operator acting upon the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x140.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x141.png" xlink:type="simple"/></inline-formula> Fourier modes of the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x140.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x141.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x142.png" xlink:type="simple"/></inline-formula> operator [<xref ref-type="bibr" rid="scirp.78065-ref16">16</xref>] . As given by [<xref ref-type="bibr" rid="scirp.78065-ref16">16</xref>] , we have that</p><disp-formula id="scirp.78065-formula210"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x143.png"  xlink:type="simple"/></disp-formula><p>Using [<xref ref-type="bibr" rid="scirp.78065-ref16">16</xref>] the solution to (14) above takes the form of having</p><disp-formula id="scirp.78065-formula211"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x144.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x145.png" xlink:type="simple"/></inline-formula>is a polarization tensor, and the function <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x145.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x146.png" xlink:type="simple"/></inline-formula> is a 2<sup>nd</sup> order Bessel function [<xref ref-type="bibr" rid="scirp.78065-ref20">20</xref>] . A generalization offered by Durrer et al. [<xref ref-type="bibr" rid="scirp.78065-ref16">16</xref>] leads to</p><disp-formula id="scirp.78065-formula212"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x147.png"  xlink:type="simple"/></disp-formula><p>With the factor of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-2180106x148.png" xlink:type="simple"/></inline-formula> coming in due to a boundary condition</p><p>upon the wall of a brane put in, i.e. looking at [<xref ref-type="bibr" rid="scirp.78065-ref16">16</xref>] . With the right hand side of (10) due to a domain wall tension of a brane.</p><disp-formula id="scirp.78065-formula213"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x149.png"  xlink:type="simple"/></disp-formula><p>This will be in our example set as not equal to zero, in the right hand side, but equal to an extremely small parameter, namely</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> From [<xref ref-type="bibr" rid="scirp.78065-ref16">16</xref>] </title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-2180106x150.png"/></fig><disp-formula id="scirp.78065-formula214"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x151.png"  xlink:type="simple"/></disp-formula><p>With this turned into</p><disp-formula id="scirp.78065-formula215"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x152.png"  xlink:type="simple"/></disp-formula><p>The right hand side of (13) represents very small brane tension, which is understandable. Then using [<xref ref-type="bibr" rid="scirp.78065-ref16">16</xref>] [<xref ref-type="bibr" rid="scirp.78065-ref20">20</xref>] , i.e.</p><disp-formula id="scirp.78065-formula216"><label>(14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x153.png"  xlink:type="simple"/></disp-formula><p>And</p><disp-formula id="scirp.78065-formula217"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x154.png"  xlink:type="simple"/></disp-formula><p>The upshot is, that afterwards,</p><disp-formula id="scirp.78065-formula218"><label>(16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x155.png"  xlink:type="simple"/></disp-formula><p>Should the term</p><disp-formula id="scirp.78065-formula219"><label>(17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x156.png"  xlink:type="simple"/></disp-formula><p>Then, (17) is acting much as in [<xref ref-type="bibr" rid="scirp.78065-ref16">16</xref>] , whereas, one is recovering a simple numerical exercise as to obtain a suitable solution as given by (18), and (19) due to [<xref ref-type="bibr" rid="scirp.78065-ref3">3</xref>] where the domain tension of the brane vanishes. The novelty as to this approach given in (17) is to obtain a time dependent behavior of the mass of the graviton,</p><disp-formula id="scirp.78065-formula220"><label>(18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-2180106x157.png"  xlink:type="simple"/></disp-formula><p>Needless to say, (16) can only be solved for, numerically, i.e. fourth order polynomial solutions for quartic equations still give over simplified dynamics, especially if (18) holds, and makes things more complicated. This is all being done to keep fidelity with respect to [<xref ref-type="bibr" rid="scirp.78065-ref16">16</xref>] , as a possible feature of brane world dynamics as reflected in [<xref ref-type="bibr" rid="scirp.78065-ref16">16</xref>] , as well as certain issues brought up in [<xref ref-type="bibr" rid="scirp.78065-ref8">8</xref>] as to what is a semi classical argument can obtain a usually quantum result. If this semi classical result is true, it has profound implications for [<xref ref-type="bibr" rid="scirp.78065-ref21">21</xref>] , and [<xref ref-type="bibr" rid="scirp.78065-ref22">22</xref>] which are held to be M theory results with no classical analogues.</p></sec><sec id="s16"><title>Appendix IV. Brief Listing of Non Linear Electrodynamics References for Non Singular Start to the Universe</title><p>We will list a number of essential references in Non linear electrodynamics which complement the work done in this document</p><p>First of which is [<xref ref-type="bibr" rid="scirp.78065-ref19">19</xref>] . In it, important to the idea of R squared gravity having the consequence of a removal of early space-time singularities. The main result is in the quote that</p><p>“A non-singular early cosmology is proposed, where, adding a nonlinear electrodynamics Lagrangian to the high-order action, a bouncing is present and a power-law inflation is obtained. In the model the Ricci scalar R works like an inflaton field.”</p><p>We will search for a similar identification in our future followups as to the importants of the Ricci scalar.</p><p>Secondly is [<xref ref-type="bibr" rid="scirp.78065-ref23">23</xref>] and [<xref ref-type="bibr" rid="scirp.78065-ref24">24</xref>] . [<xref ref-type="bibr" rid="scirp.78065-ref23">23</xref>] outlines the program of identifying electromagnetic contributions to a non singular dense state of initial space-time matter-energy, and [<xref ref-type="bibr" rid="scirp.78065-ref24">24</xref>] by Corda et al. specifically uses in its quote that:</p><p>“Such analysis will be improved by applying the Oppenheimer-Volkoff equation to the black hole case. At the end, fixed the radius of the star, the final density depends only on the introduced quintessential density term ργ and on the mass.”</p><p>NLED identifies inputs for aquintessential density term ργ and we will be examining if our agument given in the text has any commonality with the Oppenheimer-Volkoff equation in a future update to our research endeavor.</p><disp-formula id="scirp.78065-formula221"><graphic  xlink:href="http://html.scirp.org/file/2-2180106x158.png"  xlink:type="simple"/></disp-formula><p>Submit or recommend next manuscript to SCIRP and we will provide best service for you:</p><p>Accepting pre-submission inquiries through Email, Facebook, LinkedIn, Twitter, etc.</p><p>A wide selection of journals (inclusive of 9 subjects, more than 200 journals)</p><p>Providing 24-hour high-quality service</p><p>User-friendly online submission system</p><p>Fair and swift peer-review system</p><p>Efficient typesetting and proofreading procedure</p><p>Display of the result of downloads and visits, as well as the number of cited articles</p><p>Maximum dissemination of your research work</p><p>Submit your manuscript at: http://papersubmission.scirp.org/</p><p>Or contact jhepgc@scirp.org</p></sec></body><back><ref-list><title>References</title><ref id="scirp.78065-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Stoica, C. 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