<?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.2023.94078</article-id><article-id pub-id-type="publisher-id">JHEPGC-128240</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>
 
 
  Gravitational Term in Semi Empirical Mass Formula
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Mohamed</surname><given-names>E. Kelabi</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Ahmed</surname><given-names>E. Elhmassi</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Department of Physics, Faculty of Science, University of Tripoli, Tripoli, Libya</addr-line></aff><pub-date pub-type="epub"><day>18</day><month>08</month><year>2023</year></pub-date><volume>09</volume><issue>04</issue><fpage>1067</fpage><lpage>1072</lpage><history><date date-type="received"><day>16,</day>	<month>June</month>	<year>2023</year></date><date date-type="rev-recd"><day>8,</day>	<month>October</month>	<year>2023</year>	</date><date date-type="accepted"><day>11,</day>	<month>October</month>	<year>2023</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>
 
 
  A new term was added to the well-known semi-empirical mass formula to account for the changes due to gravitational attraction between nucleons in the liquid drop, as well as, accommodates for the necessary corrections in the binding energy of a nucleus. The results of our calculations show a straight forward evidence that the gravitational attraction bears a reasonable contribution to the binding energy. On the other hand, employing the gravitational term in the semi empirical mass formula was led to the calculation of gravitational constant at subnuclear level.
 
</p></abstract><kwd-group><kwd>Liquid Drop</kwd><kwd> Binding Energy</kwd><kwd> &lt;i&gt;Odd-A&lt;/i&gt; Nuclei</kwd><kwd> Gravitation</kwd><kwd> Weak Interaction</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>In the resulting liquid-drop model [<xref ref-type="bibr" rid="scirp.128240-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.128240-ref2">2</xref>] , the nucleus has an energy which arises partly from some aspects e.g., surface tension, electrical repulsion, etc. The liquid-drop model is able to reproduce many features of nuclei, including the general trend of binding energy, as well as the nuclear fission. A basic property of a nucleus is the mass defect [<xref ref-type="bibr" rid="scirp.128240-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.128240-ref3">3</xref>] which implies that the mass of the nucleus is less than the sum of the masses of its constituent nucleons:</p><p>Δ M ( A , Z ) = ( Z m p + N m n ) − M ( A , Z )</p><p>where m p and m n are the masses of proton and neutron, respectively and Δ M c 2 is now termed the binding energy (BE) of the nucleus [<xref ref-type="bibr" rid="scirp.128240-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.128240-ref5">5</xref>] . The formula accounts for the binding energy of the nucleus was developed by Weizsacker [<xref ref-type="bibr" rid="scirp.128240-ref2">2</xref>] under assumption that the nucleus is considered as a droplet of incompressible matter which is maintained by the strong nuclear interaction that exists between nucleons. The binding energy is expressed by a relation containing few terms, e.g., five terms formula [<xref ref-type="bibr" rid="scirp.128240-ref6">6</xref>] is:</p><p>B E = E v − E s − E c − E a &#177; E p</p><p>namely, volume energy, surface energy, Coulomb energy, asymmetry energy, and pairing energy, respectively [<xref ref-type="bibr" rid="scirp.128240-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.128240-ref8">8</xref>] . Although the formula contains a number of constants that have to be extracted by fitting with data. The theoretical part arises from two major properties common to all nuclei: The interior mass densities are approximately equal, and that the total binding energies are approximately proportional to the masses. The common expression for the binding energy can have the following form [<xref ref-type="bibr" rid="scirp.128240-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.128240-ref10">10</xref>] [<xref ref-type="bibr" rid="scirp.128240-ref11">11</xref>] [<xref ref-type="bibr" rid="scirp.128240-ref12">12</xref>]</p><p>B E ( A , Z ) = a v A − a s A 2 / 3 − a c Z ( Z − 1 ) A 1 / 3 − a a ( A − 2 Z ) 2 A &#177; a p A λ (1)</p><p>where a p with the polarity either positive for e-e nuclei, negative for o-o nuclei, or zero for odd-A nuclei, with the value λ was assumed to be −3/4, but recent evaluations indicate a value of −1/2 for convenience [<xref ref-type="bibr" rid="scirp.128240-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.128240-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.128240-ref15">15</xref>] [<xref ref-type="bibr" rid="scirp.128240-ref16">16</xref>] .</p><p>In this work, we wish to propose a new term through the semi-empirical mass formula accounts for the gravitational attraction between nucleons.</p></sec><sec id="s2"><title>2. Theory and Approach</title><p>Gravity is the most significant interaction between objects at the macroscopic scale, its influence also exists at subnuclear level [<xref ref-type="bibr" rid="scirp.128240-ref17">17</xref>] . The gravitational force has an infinite range, although its effects become weaker as objects get farther away. In a liquid drop, the effect of gravity between particles cannot be simply ignored. For a spherical body of uniform density, the gravitational binding energy E g is given by classical expression [<xref ref-type="bibr" rid="scirp.128240-ref18">18</xref>] [<xref ref-type="bibr" rid="scirp.128240-ref19">19</xref>] of the form</p><p>E g ∝ − G M 2 R (2)</p><p>where G is the universal gravitational constant, M is the mass of the sphere, and R its radius. However, expression (2) is not guaranteed to be valid for subnuclear particles, where the gravitational effects is still incomplete [<xref ref-type="bibr" rid="scirp.128240-ref20">20</xref>] , therefore we generally consider the gravitational attraction between subnuclear particle of the proportional form</p><p>E g = − a g A ( A − 1 ) A 1 / 3 (3)</p><p>where we have used the empirical radius R = r 0 A 1 / 3 and the mass of the form M 2 = A ( A − 1 ) , this reflects the fact that gravitational attraction will appear only if there are more than single particle, and the proportionality constant a g needs to be determined from fitting the data. For convenience, we use Equation (1) to calculate the binding energy of odd-A nuclei, with vanishing asymmetry term a p = 0 . In this context, the semi-empirical mass formula given by Equation (1) may take the following form:</p><p>B E ( A , Z ) = a v A − a s A 2 / 3 − a c Z ( Z − 1 ) A 1 / 3 − a a ( A − 2 Z ) 2 A − a g A ( A − 1 ) A 1 / 3 (4)</p><p>Equation (4) is our fundamental expression and will be used throughout our calculations.</p></sec><sec id="s3"><title>3. Results and Comparisons</title><p>We tabulate hereunder the results of different approaches for the purpose of comparisons (<xref ref-type="table" rid="table1">Table 1</xref>; <xref ref-type="table" rid="table2">Table 2</xref>).</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> A list of the results in chronological order of various sets of calculated coefficient as cited in ref. [<xref ref-type="bibr" rid="scirp.128240-ref21">21</xref>] [<xref ref-type="bibr" rid="scirp.128240-ref22">22</xref>] </title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Coefficients [MeV]</th><th align="center" valign="middle" >Years</th><th align="center" valign="middle" >a v</th><th align="center" valign="middle" >a s</th><th align="center" valign="middle" >a c</th><th align="center" valign="middle" >a a</th><th align="center" valign="middle" >a p</th></tr></thead><tr><td align="center" valign="middle" >Benzaid et al. [<xref ref-type="bibr" rid="scirp.128240-ref22">22</xref>]</td><td align="center" valign="middle" >2019</td><td align="center" valign="middle" >14.64</td><td align="center" valign="middle" >14.08</td><td align="center" valign="middle" >0.64</td><td align="center" valign="middle" >21.07</td><td align="center" valign="middle" >11.54</td></tr><tr><td align="center" valign="middle" >Mavrodiev et al. [<xref ref-type="bibr" rid="scirp.128240-ref22">22</xref>]</td><td align="center" valign="middle" >2018</td><td align="center" valign="middle" >19.12</td><td align="center" valign="middle" >18.19</td><td align="center" valign="middle" >0.52</td><td align="center" valign="middle" >12.54</td><td align="center" valign="middle" >28.99</td></tr><tr><td align="center" valign="middle" >Kirson [<xref ref-type="bibr" rid="scirp.128240-ref22">22</xref>]</td><td align="center" valign="middle" >2007</td><td align="center" valign="middle" >15.36</td><td align="center" valign="middle" >16.43</td><td align="center" valign="middle" >0.69</td><td align="center" valign="middle" >22.54</td><td align="center" valign="middle" >–</td></tr><tr><td align="center" valign="middle" >Chowdhury et al. [<xref ref-type="bibr" rid="scirp.128240-ref22">22</xref>]</td><td align="center" valign="middle" >2005</td><td align="center" valign="middle" >15.78</td><td align="center" valign="middle" >18.34</td><td align="center" valign="middle" >0.71</td><td align="center" valign="middle" >23.21</td><td align="center" valign="middle" >12</td></tr><tr><td align="center" valign="middle" >Samanta &amp; Adhikuri [<xref ref-type="bibr" rid="scirp.128240-ref22">22</xref>]</td><td align="center" valign="middle" >2004</td><td align="center" valign="middle" >15.77</td><td align="center" valign="middle" >18.34</td><td align="center" valign="middle" >0.71</td><td align="center" valign="middle" >23.21</td><td align="center" valign="middle" >12</td></tr><tr><td align="center" valign="middle" >Myers &amp; Myers [<xref ref-type="bibr" rid="scirp.128240-ref22">22</xref>]</td><td align="center" valign="middle" >1996</td><td align="center" valign="middle" >16.24</td><td align="center" valign="middle" >18.63</td><td align="center" valign="middle" >–</td><td align="center" valign="middle" >–</td><td align="center" valign="middle" >–</td></tr><tr><td align="center" valign="middle" >Wapstra [<xref ref-type="bibr" rid="scirp.128240-ref22">22</xref>]</td><td align="center" valign="middle" >1958</td><td align="center" valign="middle" >15.84</td><td align="center" valign="middle" >18.33</td><td align="center" valign="middle" >0.18</td><td align="center" valign="middle" >23.2</td><td align="center" valign="middle" >11.2</td></tr><tr><td align="center" valign="middle" >Evans [<xref ref-type="bibr" rid="scirp.128240-ref21">21</xref>]</td><td align="center" valign="middle" >1955</td><td align="center" valign="middle" >14.1 &#177; 0.2</td><td align="center" valign="middle" >13 &#177; 0.1</td><td align="center" valign="middle" >0.595 &#177; 0.02</td><td align="center" valign="middle" >19.0 &#177; 0.9</td><td align="center" valign="middle" >–</td></tr><tr><td align="center" valign="middle" >Green [<xref ref-type="bibr" rid="scirp.128240-ref21">21</xref>]</td><td align="center" valign="middle" >1954</td><td align="center" valign="middle" >15.75</td><td align="center" valign="middle" >17.8</td><td align="center" valign="middle" >0.71</td><td align="center" valign="middle" >23.7</td><td align="center" valign="middle" >–</td></tr><tr><td align="center" valign="middle" >Metropolis &amp; Reitweisner [<xref ref-type="bibr" rid="scirp.128240-ref21">21</xref>]</td><td align="center" valign="middle" >1950</td><td align="center" valign="middle" >14.0</td><td align="center" valign="middle" >13.0</td><td align="center" valign="middle" >0.583</td><td align="center" valign="middle" >19.3</td><td align="center" valign="middle" >33.5A<sup>−3/4</sup></td></tr><tr><td align="center" valign="middle" >Friedlander &amp; Kennedy [<xref ref-type="bibr" rid="scirp.128240-ref21">21</xref>]</td><td align="center" valign="middle" >1949</td><td align="center" valign="middle" >14.1</td><td align="center" valign="middle" >13.1</td><td align="center" valign="middle" >0.585</td><td align="center" valign="middle" >18.1</td><td align="center" valign="middle" >132A<sup>−1</sup></td></tr><tr><td align="center" valign="middle" >Rosenfeld [<xref ref-type="bibr" rid="scirp.128240-ref21">21</xref>]</td><td align="center" valign="middle" >1949</td><td align="center" valign="middle" >14.66</td><td align="center" valign="middle" >15.4</td><td align="center" valign="middle" >0.602</td><td align="center" valign="middle" >20.54</td><td align="center" valign="middle" >–</td></tr><tr><td align="center" valign="middle" >Feenberg [<xref ref-type="bibr" rid="scirp.128240-ref21">21</xref>]</td><td align="center" valign="middle" >1947</td><td align="center" valign="middle" >14.1</td><td align="center" valign="middle" >13.1</td><td align="center" valign="middle" >0.585</td><td align="center" valign="middle" >18.1</td><td align="center" valign="middle" >33.5A<sup>−3/4</sup></td></tr><tr><td align="center" valign="middle" >Fowler [<xref ref-type="bibr" rid="scirp.128240-ref21">21</xref>]</td><td align="center" valign="middle" >1947</td><td align="center" valign="middle" >15.3</td><td align="center" valign="middle" >16.7</td><td align="center" valign="middle" >0.69</td><td align="center" valign="middle" >22.6</td><td align="center" valign="middle" >–</td></tr><tr><td align="center" valign="middle" >Fermi [<xref ref-type="bibr" rid="scirp.128240-ref21">21</xref>]</td><td align="center" valign="middle" >1945</td><td align="center" valign="middle" >14.0</td><td align="center" valign="middle" >13.0</td><td align="center" valign="middle" >0.583</td><td align="center" valign="middle" >19.3</td><td align="center" valign="middle" >33.5A<sup>−3/4</sup></td></tr><tr><td align="center" valign="middle" >Can. Nat. Res. Council [<xref ref-type="bibr" rid="scirp.128240-ref21">21</xref>]</td><td align="center" valign="middle" >1945</td><td align="center" valign="middle" >14.05</td><td align="center" valign="middle" >14.0</td><td align="center" valign="middle" >0.61</td><td align="center" valign="middle" >19.6</td><td align="center" valign="middle" >–</td></tr><tr><td align="center" valign="middle" >Mattauch &amp; Flugge [<xref ref-type="bibr" rid="scirp.128240-ref21">21</xref>]</td><td align="center" valign="middle" >1942</td><td align="center" valign="middle" >14.66</td><td align="center" valign="middle" >15.4</td><td align="center" valign="middle" >0.602</td><td align="center" valign="middle" >20.5</td><td align="center" valign="middle" >–</td></tr><tr><td align="center" valign="middle" >Feenberg [<xref ref-type="bibr" rid="scirp.128240-ref21">21</xref>]</td><td align="center" valign="middle" >1939</td><td align="center" valign="middle" >–</td><td align="center" valign="middle" >13.3</td><td align="center" valign="middle" >0.62</td><td align="center" valign="middle" >–</td><td align="center" valign="middle" >–</td></tr><tr><td align="center" valign="middle" >Bethe &amp; Bacher [<xref ref-type="bibr" rid="scirp.128240-ref21">21</xref>]</td><td align="center" valign="middle" >1936</td><td align="center" valign="middle" >13.86</td><td align="center" valign="middle" >13.2</td><td align="center" valign="middle" >0.58</td><td align="center" valign="middle" >19.5</td><td align="center" valign="middle" >–</td></tr></tbody></table></table-wrap><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> Showing the effect of adding a new thermal term a T to the semi-empirical mass formula, by Khadri and others, as it discussed in ref. [<xref ref-type="bibr" rid="scirp.128240-ref23">23</xref>] </title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Coefficients [MeV]</th><th align="center" valign="middle" >Year</th><th align="center" valign="middle" >a v</th><th align="center" valign="middle" >a s</th><th align="center" valign="middle" >a c</th><th align="center" valign="middle" >a a</th><th align="center" valign="middle" >a p</th><th align="center" valign="middle" >a T</th></tr></thead><tr><td align="center" valign="middle" >Khdari et al.</td><td align="center" valign="middle" >2020</td><td align="center" valign="middle" >15.829</td><td align="center" valign="middle" >17.992</td><td align="center" valign="middle" >0.739</td><td align="center" valign="middle" >20.89</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.631</td></tr><tr><td align="center" valign="middle" >Khdari et al.</td><td align="center" valign="middle" >2020</td><td align="center" valign="middle" >15.832</td><td align="center" valign="middle" >18.399</td><td align="center" valign="middle" >0.705</td><td align="center" valign="middle" >24.172</td><td align="center" valign="middle" >23.489</td><td align="center" valign="middle" >0.440</td></tr></tbody></table></table-wrap><table-wrap id="table3" ><label><xref ref-type="table" rid="table3">Table 3</xref></label><caption><title> A sample of our results of odd-A nuclei compared with nuclei suggested in ref. [<xref ref-type="bibr" rid="scirp.128240-ref21">21</xref>] </title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Coefficients [MeV]</th><th align="center" valign="middle" >Year</th><th align="center" valign="middle" >a v</th><th align="center" valign="middle" >a s</th><th align="center" valign="middle" >a c</th><th align="center" valign="middle" >a a</th><th align="center" valign="middle" >a g</th></tr></thead><tr><td align="center" valign="middle" >Present Work</td><td align="center" valign="middle" >2022</td><td align="center" valign="middle" >15.587</td><td align="center" valign="middle" >17.649</td><td align="center" valign="middle" >0.699</td><td align="center" valign="middle" >23.458</td><td align="center" valign="middle" >1.192 &#215; 10<sup>−</sup><sup>3</sup></td></tr><tr><td align="center" valign="middle" >Jos&#233; et al.</td><td align="center" valign="middle" >2016</td><td align="center" valign="middle" >15.593</td><td align="center" valign="middle" >17.345</td><td align="center" valign="middle" >0.694</td><td align="center" valign="middle" >23.601</td><td align="center" valign="middle" >–</td></tr></tbody></table></table-wrap><table-wrap id="table4" ><label><xref ref-type="table" rid="table4">Table 4</xref></label><caption><title> A sample of our results of odd-A nuclei compared with ref. [<xref ref-type="bibr" rid="scirp.128240-ref24">24</xref>] </title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Coefficients [MeV]</th><th align="center" valign="middle" >Year</th><th align="center" valign="middle" >a v</th><th align="center" valign="middle" >a s</th><th align="center" valign="middle" >a c</th><th align="center" valign="middle" >a a</th><th align="center" valign="middle" >a g</th></tr></thead><tr><td align="center" valign="middle" >Present Work</td><td align="center" valign="middle" >2022</td><td align="center" valign="middle" >15.531</td><td align="center" valign="middle" >17.503</td><td align="center" valign="middle" >0.681</td><td align="center" valign="middle" >24.899</td><td align="center" valign="middle" >1.192 &#215; 10<sup>−</sup><sup>3</sup></td></tr><tr><td align="center" valign="middle" >Mirzaei et al.</td><td align="center" valign="middle" >2017</td><td align="center" valign="middle" >15.519</td><td align="center" valign="middle" >17.746</td><td align="center" valign="middle" >0.674</td><td align="center" valign="middle" >24.576</td><td align="center" valign="middle" >–</td></tr></tbody></table></table-wrap><p>In <xref ref-type="table" rid="table3">Table 3</xref> and <xref ref-type="table" rid="table4">Table 4</xref>, we compare the results of our calculations with samples of selected approaches focused on odd-A nuclei.</p><p>On the other hand, the obtained value of gravitational constant a g is further employed to determine the renormalized gravitation constant [<xref ref-type="bibr" rid="scirp.128240-ref25">25</xref>] , associated with interactions at subnuclear scale. From Equations (2) and (3), we write</p><p>a g = Γ m N 2 r 0 (5)</p><p>where m N is the mass of a nucleon and Γ is the subnuclear gravitational constant, which absorbing Newton gravitational constant G, giving</p><p>Γ = 1.23 &#215; 10 33 G = 8.02 &#215; 10 28   m 3 ⋅ kg − 1 ⋅ s − 2 (6)</p><p>This value agrees with the one suggested by Onofrio [<xref ref-type="bibr" rid="scirp.128240-ref26">26</xref>] [<xref ref-type="bibr" rid="scirp.128240-ref27">27</xref>] , and also falls within the range of weak interactions as also suggested in ref. [<xref ref-type="bibr" rid="scirp.128240-ref28">28</xref>] .</p></sec><sec id="s4"><title>4. Conclusion</title><p>It is known that the gravitational effect at subnuclear scale is still under considerations, we thus encouraged to add a new term to the semi-empirical mass formula to account for any deviation in binding energy due to gravitational effects between subnuclear particles. The added gravitational term is consistent, hence the semi-empirical mass formula shows agreement compared with earlier studies. On the other hand, we could extract a new constant representing the gravitational constant at subnuclear scale, which bears an excellent agreement compared with available studies concerning gravitational interaction at subnuclear scale.</p></sec><sec id="s5"><title>Conflicts of Interest</title><p>The authors declare no conflicts of interest regarding the publication of this paper.</p></sec><sec id="s6"><title>Cite this paper</title><p>Kelabi, M.E. and Elhmassi, A.E. (2023) Gravitational Term in Semi Empirical Mass Formula. Journal of High Energy Physics, Gravitation and Cosmology, 9, 1067-1072. https://doi.org/10.4236/jhepgc.2023.94078</p></sec></body><back><ref-list><title>References</title><ref id="scirp.128240-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Gamow, G. (1930) Mass Defect Curve and Nuclear Constitution. 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