<?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">JMP</journal-id><journal-title-group><journal-title>Journal of Modern Physics</journal-title></journal-title-group><issn pub-type="epub">2153-1196</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jmp.2017.812115</article-id><article-id pub-id-type="publisher-id">JMP-80249</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>
 
 
  The Charge Structure of the Nucleons
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>M.</surname><given-names>Y. Hussein</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>Department of Physics, University of Bahrain, Bahrain</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>myhussein81@gmail.com</email></corresp></author-notes><pub-date pub-type="epub"><day>09</day><month>11</month><year>2017</year></pub-date><volume>08</volume><issue>12</issue><fpage>1933</fpage><lpage>1937</lpage><history><date date-type="received"><day>10,</day>	<month>October</month>	<year>2017</year></date><date date-type="rev-recd"><day>7,</day>	<month>November</month>	<year>2017</year>	</date><date date-type="accepted"><day>10,</day>	<month>November</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>
 
 
  Study of nucleons charge radii and electromagnetic form factors are expected to provide valuable information about the distribution of electric charge within the fundamental particles in nucleon’s inner structure. In the recent years, dramatic progress has been made in the understanding of the nucleon structure and the precision of its partonic content, due to the vast theoretical progress, and the availability of new high precision measurements. Here in this article, we present a simple model for the charge structure of the nucleons and the most available sets of the structure functions to calculate the mean square charge radius &amp;lt;r
  <sub>N</sub>
  <sup>2</sup>&amp;gt; for both protons and neutrons. Our results are consistent with the modern understanding of the nucleons as well as recent experimental data. We discuss the origin of the sign 
  &amp;lt;r
  <sub>N</sub>
  <sup style="margin-left:-6px;">2</sup>
  &amp;gt; for both proton and neutron.
 
</p></abstract><kwd-group><kwd>Nucleon Charge Structure</kwd><kwd> Electromagnetic Form Factors</kwd><kwd> Quark-Parton Model</kwd><kwd> Charge Radius</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Nucleons charge structure has been a subject of extensive investigation for the past years [<xref ref-type="bibr" rid="scirp.80249-ref1">1</xref>] - [<xref ref-type="bibr" rid="scirp.80249-ref7">7</xref>] . The electromagnetic form factors and charge radii of nucleons provide critical information about the distribution of the charge within the nucleons and reveal high valuable information about the dynamic of the strong interaction. The non-uniform charge distribution leads to a finite value for the mean square charge radii of nucleons.</p><p>There have been several attempts to extract more information on inner nucleon structure. Variety of techniques are used in order to calculate nucleons mean square charge radius 〈 r N 2 〉 and the electromagnetic form factors including, the empirical charge distribution, the quark-parton model and composite models of the hadrons have achieved considerable popularity, primarily because the most elementary, non-relativistic quark picture accounts remarkably well for most of the available data on hadronic physics.</p><p>Recently, the question of that the mean square intrinsic charge radius of the nucleons is widely discussed and has been elegantly explained in terms of generalized parton distributions and the charge density related to the electric charge distribution ρ ( r ) inside the nucleon [<xref ref-type="bibr" rid="scirp.80249-ref8">8</xref>] , which has been given by</p><p>〈 r N 2 〉 = ∫ ​     ρ ( r ) r 2 d 3 r (1)</p><p>The non-zero value of the charge radius of the nucleon implies a non-vanishing electric form factors since</p><p>〈 r N 2 〉 = − 6 d G E N ( q 2 ) d q 2 | q 2 = 0 (2)</p><p>where G E N ( q 2 ) is the electromagnetic form factors. The most recent determination of the thermal neutron-electron interaction predicts a value of [<xref ref-type="bibr" rid="scirp.80249-ref9">9</xref>]</p><p>d G E N ( q 2 ) d q 2 | q 2 = 0 = 0.02 &#177; 0.0014   f m 2 (3)</p><p>where G E N ( q 2 ) is the electromagnetic form factors. Earlier electron-deuteron and electron-proton scattering data has been analyzed very precisely in q 2 . The low q 2 part of the data has been used to extract the slope of G E n , the value obtained was</p><p>d G E n ( q 2 ) d q 2 | q 2 = 0.02 &#177; 0.0014   f m 2 (4)</p><p>where G E N ( q 2 ) is the electromagnetic form factors. Equation (3) and Equation (4) show essential agreement between both low q<sup>2</sup> scattering electron proton and electron Deuteron with data from thermal neutron-electron experiment. The neutron charge radius is far from small on the scale of proton. The available data [<xref ref-type="bibr" rid="scirp.80249-ref9">9</xref>] imply that</p><p>〈 r n 2 〉 〈 r p 2 〉 ≅ − 0.155 (5)</p><p>where 〈 r p 2 〉 and 〈 r n 2 〉 is the corresponding proton and neutron mean square charge radius.</p></sec><sec id="s2"><title>2. Nucleon Charge Structure</title><p>In the context of the proton model, a connection has been established by Sehgal [<xref ref-type="bibr" rid="scirp.80249-ref10">10</xref>] between the sign of the neutron charge radius and the distribution of proton transverse momenta. Moreover, a contradiction between the observed negative sign and the trend of deep inelastic data was noted in ref. [<xref ref-type="bibr" rid="scirp.80249-ref11">11</xref>] . Calculation in ref. [<xref ref-type="bibr" rid="scirp.80249-ref11">11</xref>] [<xref ref-type="bibr" rid="scirp.80249-ref12">12</xref>] related the negativeness of 〈 r n 2 〉 to the nucleons possible quark-diquark structure. The effect of nucleons quark-diquark structure is added to the usual constituent quark model to calculate nucleons charge square radius. All results of 〈 r p 2 〉 and 〈 r n 2 〉 are fitted to the experimental value extremely well.</p><p>In this work we try to relate the negative value of 〈 r n 2 〉 to the distribution of parton transverse momentum with the general prescriptions of quark-parton model. Our consideration is that the nucleon can be described in the parton model by a set of functions regarded as an integral over a transverse and longitudinal momentum distribution as:</p><p>f i ( x ) = ∫ h i ( x , b ) d b (6)</p><p>With, h i ( x , b ) = [ π A ( x ) ] f i ( x ) exp [ − b 2 / A ( x ) ] , f i ( y ) = ∫ 0 z o g i ( y , z ) d z and</p><p>g i ( y , z ) = [ z o ( 1 − z o 2 3 B ( y ) ) ] − 1 f i ( y ) ( 1 − z 2 B ( y ) ) ,</p><p>where z o is an appropriate cutoff related to the thickness of the nucleon. Our considerations are based on the hypothesis that the nucleon has a disc-like look instead of a spherical object on account of the relativistic contraction as suggested in ref. [<xref ref-type="bibr" rid="scirp.80249-ref12">12</xref>] , which characterized by Equation (6). In this simple model of the nucleon, the complete quark-parton distribution function can be written in a separable form as</p><p>ρ i ( x , b ; y , z ) = h i ( x , b ) g i ( y , z ) (7)</p><p>Expression [<xref ref-type="bibr" rid="scirp.80249-ref1">1</xref>] for the mean square charge radius can be rewritten in the form</p><p>〈 r 2 〉 = ∬ d x d y     δ ( x 2 + y 2 − 1 ) ∑ e i ∫ d 3 r     r 2 ρ ( r ) (8)</p><p>With x 2 + y 2 = 1 ,   d 3 r = d 2 b d z ,   r 2 = b 2 + z 2 .</p><p>Integrating Equation (8) over r and y, the resulting expression explicitly gives</p><p>〈 r 2 〉 = ∫ 0 1 d x [ A ( x ) + η ( y ) ] L ( x ) 2 y (9)</p><p>Having A ( x ) = exp ( − β x ) , η ( y ) = z 0 2 5 ( 5 A ( y ) − 3 z 0 2 3 A ( y ) − z 0 2 ) .</p><p>L ( x ) represents the compound quark density function for the nucleon</p><p>L p ( x ) = 2 3 u v ( x ) u v ( y ) − 1 3 d v ( x ) d v ( y ) (10a)</p><p>L n ( x ) = 2 3 d v ( x ) d v ( y ) − 1 3 u v ( x ) u v ( y ) (10b)</p><p>where u v ( x ) and d v ( x ) are the parton distribution function as extracted from global fits to a wide range of deep-inelastic and other related data [<xref ref-type="bibr" rid="scirp.80249-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.80249-ref14">14</xref>] . The v subscript refers to the valance constituency only. The form of A(x) in Equation (9) is not unique and parameterized with β which is itself a function of the scale Q in GeV. The form of A(x) does not have to be the same for all nucleons. For u v and d v we make use of the structure distribution function from MSTW [<xref ref-type="bibr" rid="scirp.80249-ref13">13</xref>] and CTEQ [<xref ref-type="bibr" rid="scirp.80249-ref14">14</xref>] .</p></sec><sec id="s3"><title>3. Results</title><p>Equation (9) depends on the disc model itself and hence the simplicity of this treatment allows us to point out the following:</p><p>1) By choosing an appropriate value for β we can reproduce the current signs and values for both 〈 r n 2 〉 and 〈 r p 2 〉 as shown in <xref ref-type="table" rid="table1">Table 1</xref>.</p><p>2) Because u v is significantly larger than d v in x-space, and considering Equation (10), the calculation of 〈 r 2 〉 is dominated by u v such that Equation (10) can be well approximated by</p><p>L p ( x ) ≅ 2 3 u v ( x ) u v ( y ) (11a)</p><p>L n ( x ) ≅ − 1 3 u v ( x ) u v ( y ) (11b)</p><p>This clearly shows that 〈 r p 2 〉 &gt; 0 , while 〈 r n 2 〉 &lt; 0 .</p><p>In fact, for the same β one obtains a factor of −0.15 for the ratio in Equation (5). Thus even with the arbitrariness of choosing β the signs of 〈 r 2 〉 are well understood in this treatment which suggest that the u-quark is the dominating factor in the nucleon charge distribution.</p><p>3) The uncertainty associated with the choice of parton distribution function do not affect our conclusions as we have used different sets and obtained similar results. In fact usually a limited shift in β is all it took to reproduce the same results with a different set of parton distribution functions.</p></sec><sec id="s4"><title>4. Conclusion</title><p>We have used a simple model of the nucleon in connection with the quark-parton model and the current information on parton distributions to re-establish both the value and the sign of the nucleon charge radii. It seems that the up quark is dominating the calculations of the root mean square charge radii. Equations (11a) and (11b) shows clearly why positive sign appear in mean square charge radius for the proton and why negative sign appear for the neutron. The major uncertainty in this work is the fact that the parton distributions</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Results reproduce the current signs and values for both 〈 r n 2 〉 and 〈 r p 2 〉 </title></caption><table><tbody><thead><tr><th align="center" valign="middle" >A) With 〈 r p 2 〉 fixed at 0.707 fm<sup>2</sup></th><th align="center" valign="middle" ></th><th align="center" valign="middle" ></th></tr></thead><tr><td align="center" valign="middle" >Parton distribution</td><td align="center" valign="middle" >β</td><td align="center" valign="middle" >〈 r n 2 〉 in fm<sup>2</sup></td></tr><tr><td align="center" valign="middle" >MRS T</td><td align="center" valign="middle" >14.15</td><td align="center" valign="middle" >−0.378</td></tr><tr><td align="center" valign="middle" >CTEQ</td><td align="center" valign="middle" >9.13</td><td align="center" valign="middle" >−0.376</td></tr><tr><td align="center" valign="middle" >B) Independent 〈 r p 2 〉</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Parton distribution</td><td align="center" valign="middle" >β</td><td align="center" valign="middle" >〈 r n 2 〉 in fm<sup>2</sup></td></tr><tr><td align="center" valign="middle" >MRS T</td><td align="center" valign="middle" >12.72</td><td align="center" valign="middle" >−0.120</td></tr><tr><td align="center" valign="middle" >CTEQ</td><td align="center" valign="middle" >7.70</td><td align="center" valign="middle" >−0.120</td></tr></tbody></table></table-wrap><p>used for both the neutron and the proton are those extracted from proton data only.</p></sec><sec id="s5"><title>Cite this paper</title><p>Hussein, M.Y. 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