<?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">WJNST</journal-id><journal-title-group><journal-title>World Journal of Nuclear Science and Technology</journal-title></journal-title-group><issn pub-type="epub">2161-6795</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/wjnst.2018.81002</article-id><article-id pub-id-type="publisher-id">WJNST-82029</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Engineering</subject><subject> Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  A Suggestion Complementing the Magic Numbers Interpretation of the Nuclear Fission Phenomena
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Faustino</surname><given-names>Menegus</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>F. Menegus V. Europa, Bussero, Italy</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>menegus.faustino@gmail.com</email></corresp></author-notes><pub-date pub-type="epub"><day>17</day><month>11</month><year>2017</year></pub-date><volume>08</volume><issue>01</issue><fpage>11</fpage><lpage>22</lpage><history><date date-type="received"><day>21,</day>	<month>November</month>	<year>2017</year></date><date date-type="rev-recd"><day>23,</day>	<month>January</month>	<year>2018</year>	</date><date date-type="accepted"><day>26,</day>	<month>January</month>	<year>2018</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>
 
 
  Ideas, solely related on the nuclear shell model, fail to give an interpretation of the experimental central role of 
  <sub>54</sub>Xe in the asymmetric fission of actinides. The same is true for the 
  &amp;beta;-delayed fission of 
  <sup>180</sup>Tl to
  <sup> 80</sup>Kr and 
  <sup>100</sup>Ru. The representation of the natural isotopes, in the Z-Neutron Excess plane, suggests the importance of the of the Neutron Excess evolution mode in the fragments of the asymmetric actinide fission and in the fragments of the 
  &amp;beta;-delayed fission of 
  <sup>180</sup>Tl. The evolution mode of the Neutron Excess, hinged at Kr and Xe, is directed by the 50 and 82 neutron magic numbers. The present isotope representation offers a frame for the interpretation of the post fission evaporation of neutrons, higher for the A
  <sub>L</sub> compared to the AH fragments, a tenet in nuclear fission. Further enlightened is the functional meaning of the 50 proton magic number, marking the start of the yield rise of the A
  <sub>H</sub> fragments in actinide fission.
 
</p></abstract><kwd-group><kwd>Nuclear Structure</kwd><kwd> Neutron Excess</kwd><kwd> Magic Numbers</kwd><kwd> Isotons</kwd><kwd> Binding Energy</kwd><kwd> Kr</kwd><kwd> Xe</kwd><kwd> Actinides</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The strong and short-range nucleon-nucleon attractive forces, granting both the internal nuclear cohesion and the nuclear surface tension, are still at the heart of the interpretation of the atomic nuclear fission, according to the Liquid Drop Model (LDM) [<xref ref-type="bibr" rid="scirp.82029-ref1">1</xref>] . Yet while it is possible to explain the mass and charge symmetrical splitting with the LDM, this is not the case for the asymmetrical nuclear splitting. In this case, exemplified by the nuclear reaction <sup>235</sup>U<sub>(</sub><sub>nt,f</sub><sub>)</sub>, heavy and light fragments of mass close to140 and 80 amu are produced, bearing different charges.</p><p>The nuclear fission, discovered in 1934, was indeed an asymmetric fission. Otto Han [<xref ref-type="bibr" rid="scirp.82029-ref2">2</xref>] was able to reveal the presence of <sub>56</sub>Ba in the nuclear fragments, an element incompatible with the current ideas of that time and incompatible with the LDM soon developed [<xref ref-type="bibr" rid="scirp.82029-ref1">1</xref>] . Nuclear deformation [<xref ref-type="bibr" rid="scirp.82029-ref3">3</xref>] enabled nuclei to progress, under a variety of energy stimuli, towards the separation of the nuclear material into two distinct centres representing the nuclei of the nascent fragments of the nucleus undergoing fission. Sound models, for the interpretation of the asymmetric fission, appeared, after substantial improvements of the LDM [<xref ref-type="bibr" rid="scirp.82029-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.82029-ref5">5</xref>] , only following the ideas of Strutinsky. He suggested to take into consideration the shell effects [<xref ref-type="bibr" rid="scirp.82029-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.82029-ref7">7</xref>] of the proton and neutron magic numbers of the nascent fragments on the Binding Energy (BE) landscape of the nuclei undergoing fission [<xref ref-type="bibr" rid="scirp.82029-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.82029-ref9">9</xref>] .</p><p>As reported in the fine review of G&#246;nnenwein [<xref ref-type="bibr" rid="scirp.82029-ref10">10</xref>] and in several others recent studies [<xref ref-type="bibr" rid="scirp.82029-ref11">11</xref>] [<xref ref-type="bibr" rid="scirp.82029-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.82029-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.82029-ref14">14</xref>] , the asymmetric fission mode is understood to a deep level by the combination of the fundamental ideas of the LDM, the macro part of the models, to which are superimposed the shell effects of the magic numbers, the micro part of the models. An impressive work, relaying mainly on the shell features of the nascent daughter nuclei, allows a detailed description of the fission modes known as St1, St2, Superlong and Superasymmetric fission [<xref ref-type="bibr" rid="scirp.82029-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.82029-ref14">14</xref>] . Very interesting the Superlong mode substantiates the presence of the LDM physics in the asymmetric fission modes in accordance to the separation principle of the macro from the micro effects [<xref ref-type="bibr" rid="scirp.82029-ref13">13</xref>] . Of the asymmetric modes St1 and St2 the first-one is closer to the Superlong mode. The Superasymmetric mode instead stresses the relevance of the proton magic number 28 in the fission phenomena [<xref ref-type="bibr" rid="scirp.82029-ref15">15</xref>] . Unstable nuclei, typically the actinides with Z = 90 to 100, stimulated by thermal neutrons undergo asymmetric fission, possibly the most natural and lowest temperature nuclear fission. Very interesting these reactions where accompanied by the staggering phenomenon: the strong even-odd fluctuations of the fragments charge and mass yields of the Z even nuclei fission [<xref ref-type="bibr" rid="scirp.82029-ref10">10</xref>] . At increasing neutron energy, from 20 up to100 MeV, the asymmetric fission replaces gradually the symmetric-one [<xref ref-type="bibr" rid="scirp.82029-ref10">10</xref>] . The General description of Fission Observables model, exploiting the general lows of mathematics and physics and empirical information, is presently successful in the representation of all the fission phenomena [<xref ref-type="bibr" rid="scirp.82029-ref16">16</xref>] .</p><p>Yet important aspects of the nuclear fission are still obscure not fitting in the magic numbers interpretation of the phenomenon. The β-delayed fission of <sup>180</sup>Tl obeys the reaction, <sup>180</sup>Hg = <sup>80</sup>Kr + <sup>100</sup>Ru, instead of the reaction, <sup>180</sup>Hg = 2<sub>40</sub>Zr<sup>50</sup> [<xref ref-type="bibr" rid="scirp.82029-ref17">17</xref>] . The last reaction is expected because of the neutron magic number 50 and of the half-magic proton number 40 of Zr. Equally the most probable nuclear splitting, with thermal neutrons or by electro-magnetic excitation, of elements from Th to Fm leads to an heavy fragment with an astonishing fixed charge Z = 54. The light fragment instead shows an increasing Z value tailored to complement the charge of the starting nucleus [<xref ref-type="bibr" rid="scirp.82029-ref16">16</xref>] . It is suggested here that the proton numbers 36 and 54 of the elements Kr and Xe, in spite of the corresponding shells absence in the shell model [<xref ref-type="bibr" rid="scirp.82029-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.82029-ref7">7</xref>] , are important in the interpretation of the nuclear fission. The aim of the present paper is to provide support to this statement.</p></sec><sec id="s2"><title>2. Methods</title><p>The isotopes, of any chemical element, can be defined in equivalent ways by couples of two numbers added to the element symbol: z <sup>A</sup>X; <sup>A</sup>X<sup>N</sup>; <sub>Z</sub>X<sub>EN</sub>. Z, A, N, NE, indicate the Proton, the Mass, the Neutron and the Neutron Excess numbers respectively of an isotope, with NE = A-2Z. The third mode allows the isotope representation in the Z-NE plane. The Z, A, N, NE and the isotope BE are derived from G. Audy et al. [<xref ref-type="bibr" rid="scirp.82029-ref18">18</xref>] . Note the mandatory presence, in all the three ways, of the isotope proton number either as the Z number or as the chemical element symbol. All the figures except numbers 6 and 7 have been developed through graphical programs (VB.net), starting from text files containing levels, properties (colors, lines dimension etc.) and all the comments to be visualized.</p></sec><sec id="s3"><title>3. Results</title><sec id="s3_1"><title>3.1. Isotopes Concerned in the Actinide and in the <sup>180</sup>Tl β-Delayed Fission</title><p><xref ref-type="fig" rid="fig1">Figure 1</xref> represents the natural isotopes of the elements from Fe to Gd that are of interest in the present work. The proton and neutron magic numbers of the shell model [<xref ref-type="bibr" rid="scirp.82029-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.82029-ref7">7</xref>] and the limits of the β-stability valley are highlighted. The salient features of the isotopic representation in the Z-NE plane, with NE = A-2Z, have been reported [<xref ref-type="bibr" rid="scirp.82029-ref19">19</xref>] . Here it is sufficient to recall that the mass number of every isotope is, A = NE + 2Z. To pinpoint any isotope in <xref ref-type="fig" rid="fig1">Figure 1</xref>, its NE number needs to be determined; here it is subscribed behind the element symbol, as in Sn<sub>32</sub>. When appropriate are also employed the usual symbol’s superscripts values of mass and neutron numbers.</p><p>The eight-nucleon isobar tracks (<xref ref-type="fig" rid="fig1">Figure 1</xref>) represent a further help in the determination of the isotopic mass number A [<xref ref-type="bibr" rid="scirp.82029-ref19">19</xref>] . Nuclei with 50 and 82 neutrons will be simply denoted 50 and 82 isotons respectively. The representation of the natural isotopes in the Z-NE plane adds together the features of the Segr&#232; chart of nuclides with those of the Mendeleev’s periodic table of the elements. A bridge between chemistry and physics.</p></sec><sec id="s3_2"><title>3.2. Binding Energy Evolution along the Isotopic Arrays with Constant NE Number</title><p>At the monotonous progress of the Z number any sudden change of the BE of the isotopes lying on the constant NE arrays (<xref ref-type="fig" rid="fig1">Figure 1</xref>), will denote changes in the nuclear structure. As an example <xref ref-type="fig" rid="fig2">Figure 2</xref> shows the BE evolution of the</p><p>isotopes with zero NE, that is the special isotopes with an identical number of protons and neutrons. The double magic numbers 2, 8, 20 and 28, together with the less general half-magic 14 Z number show sudden BE changes.</p><p><xref ref-type="fig" rid="fig3">Figure 3</xref> shows the BE evolution of the isotopes lying on the 8 to 36 NE arrays represented in <xref ref-type="fig" rid="fig1">Figure 1</xref>. The Z and NE numbers, defining every isotope in the Z-NE plane, allow the univocal correspondence of the <xref ref-type="fig" rid="fig3">Figure 3</xref> isotopes with those of <xref ref-type="fig" rid="fig1">Figure 1</xref> and vice versa. Stressed is the known relevance of the proton magic number 50. Interestingly its influence extends well beyond the limits of the β-stability valley up to Sn<sub>36</sub>. It is maximal at the double magic <sup>132</sup>Sn<sub>32</sub>. Also clear is the importance of the proton magic number 28. Its influence on the BE is marked at the upper border of the β-stability valley, shows a decrease with the NE increase and practically fades at the double magic <sup>78</sup>Ni<sub>22</sub>.</p><p>Of particular interest are the effects of the Z progress on the 82 and 50 isotons: the green parabolas (<xref ref-type="fig" rid="fig3">Figure 3</xref>). In the first case the BE maximum is set at Z = 54, the nuclear charge of the most probable fission mode of an extended chain of actinide nuclei [<xref ref-type="bibr" rid="scirp.82029-ref16">16</xref>] . In the second case the BE maximum is set at Z = 38, not a casual value, see discussion. The sudden BE changes along the NE arrays correspond to the Z even charge of the elements displaying the top abundance in the</p><p>charge-mass staggering typical of actinide fission (<xref ref-type="fig" rid="fig4">Figure 4</xref>) [<xref ref-type="bibr" rid="scirp.82029-ref11">11</xref>] . For the isotopes lying on the 9 to 35 NE arrays the BE maxima of the 82 and 50 isotons shift to Z = 55 and Z = 39 respectively: the broken-line parabolas (<xref ref-type="fig" rid="fig3">Figure 3</xref>). In <xref ref-type="fig" rid="fig3">Figure 3</xref>, the concurrent increase of both Z and NE numbers causes a fast increase of the isotopic mass numbers and the consequent fast drop in the related BE. This is why same curves are truncated and curves tend to crowd at the right lower corner.</p></sec><sec id="s3_3"><title>3.3. Relevant Results of P.M&#246;ller</title><p>To put the results of the <xref ref-type="fig" rid="fig3">Figure 3</xref> in the perspective of what learned about the nuclear fission, it is useful to reproduce (with permission) the results of the electro- magnetic induced fission of <sup>234</sup>U from the <xref ref-type="fig" rid="fig2">Figure 2</xref> of P. M&#246;ller [<xref ref-type="bibr" rid="scirp.82029-ref11">11</xref>] . It is important to keep in mind that the experimental data where converted to the mass- yield distribution before neutron evaporation by assuming that the proton/neutron ratio Z/N is the same in each of the two fission fragments as in the original nucleus.</p><p>The M&#246;ller figure, placed upon the natural isotopes representation in the Z-NE plane of <xref ref-type="fig" rid="fig1">Figure 1</xref>, produce <xref ref-type="fig" rid="fig4">Figure 4</xref>.. Notably the most probable light and heavy fragments of <sup>234</sup>U, Sr<sub>12</sub> and Xe<sub>28</sub> respectively, are in agreement with the maximum BE of these isotopes in <xref ref-type="fig" rid="fig3">Figure 3</xref>. The heavy fragment is an isotope of <sub>54</sub>Xe, the Xe<sup>82</sup> isoton, the chemical element that shows the best performance in the accommodation of the EN, compared with the flanking elements (<xref ref-type="fig" rid="fig1">Figure 1</xref>). This is not the case for the light fragment where the choice is the <sub>38</sub>Sr<sup>50</sup> isoton, in spite of the fact that the flanking element <sub>36</sub>Kr has a highest ability in the accommodation of the NE. Very important <xref ref-type="fig" rid="fig4">Figure 4</xref> shows that, albeit at a low probability, the symmetric splitting is always present in the asymmetric fission mode. The magic proton number 50 marks the beginning of the mass increase for the heavy fragment (<xref ref-type="fig" rid="fig6">Figure 6</xref>).</p></sec><sec id="s3_4"><title>3.4. A Different View of the <xref ref-type="fig" rid="fig3">Figure 3</xref> Results</title><p>The BE of the 50 and 82 isotons (<xref ref-type="fig" rid="fig3">Figure 3</xref>) are compared in <xref ref-type="fig" rid="fig5">Figure 5</xref>, to the BE of the most stable natural isotope of the elements from Fe to Gd, allowing some interesting considerations. First of all the known decrease of the isotopic BE beyond Fe is clear. It is accompanied by a marked shoulder, with the levelling-off of the BE, between Ge and Y. A result not discussed here.</p><p>The green numbers denote the NE of the 50 and 82 isotons. The black numbers represent the NE of the most stable isotope of the elements considered. The red numbers refer to the important isotopes highlighted in <xref ref-type="fig" rid="fig1">Figure 1</xref>. These numbers allow an easy spotting of the corresponding isotopes both in <xref ref-type="fig" rid="fig3">Figure 3</xref> and in <xref ref-type="fig" rid="fig1">Figure 1</xref>. It is important here to stress the different effects of the 50 and 82 neutron magic numbers on Sr, Kr and Xe isotopes respectively. With Sr it is the neutron magic number 50 that rises the BE of the Sr<sub>12</sub> isotope at the maximum causing the pick on the shoulder mentioned above. The Kr<sub>12</sub> isotope instead is more stable than the Kr<sub>14</sub> isotope in spite of the 50 neutrons contained in the latter isotope. Turning to the Xe isotopes, the magic neutron number 82 denotes again the maximum BE of the isoton 82 family set at the Xe<sub>28</sub> isotope. Instead the maximum BE of the Xe isotopes coincides with Xe<sub>18</sub>, clearly out of reach of the 82 neutron effects (<xref ref-type="fig" rid="fig3">Figure 3</xref>). Notably the 82 isoton Xe<sub>28</sub> is the less stable of all the natural isotopes of Xe. To summarize both Kr and Xe isotopes may reach maximum stability without the aid of the 50 and 82 neutron magic numbers. <xref ref-type="fig" rid="fig5">Figure 5</xref> complements <xref ref-type="fig" rid="fig3">Figure 3</xref>. The important isotopes, red labelled in <xref ref-type="fig" rid="fig3">Figure 3</xref>, are shown in the Z-BE plane in <xref ref-type="fig" rid="fig5">Figure 5</xref> together with a more extended list of the 50 and 82 isotons.</p></sec></sec><sec id="s4"><title>4. Discussion</title><p>Two principal considerations underlie the idea of the present work. The first- one concerns the display of the natural isotopes of the elements from Fe to Gd in the Z-NE plane (<xref ref-type="fig" rid="fig1">Figure 1</xref>). At the monotonous progress of Z, coming near to Kr and Xe, there is an increasing trend of the elements ability to harbour the NE. There is a net reduction of that ability beyond Kr and Xe, and a resumption afterwards. The result are two picks in the NE accommodation ability at Kr and Xe characterized, in addition, by the neutron magic numbers 50 and 82 respectively. The total number of the natural isotopes per element equally shows an increase</p><p>and decrease hinged at Kr and Xe; Xe has only one isotope less than those of Sn. To summarize the evolution of the ability to harbour neutrons, at the progress of Z, reaches maxima at Kr and Xe and appear influenced by the magic neutron numbers 50 and 82. For the sake of the ideas suggested here it is clear that the above-mentioned ability must extend above the β-stability valley into the region of the primary neutron-rich fragments of the nuclear fissions (<xref ref-type="fig" rid="fig1">Figure 1</xref>, <xref ref-type="fig" rid="fig5">Figure 5</xref>). The second consideration concerns the accurate experimental demonstration that, in the asymmetric fission of a long actinide chain from Th to Fm, the most probable charge of the heavy fragment is fixed at Z = 54, the Xe charge [<xref ref-type="bibr" rid="scirp.82029-ref16">16</xref>] . Moreover in the β-delayed fission of the neutron poor <sup>180</sup>Tl nucleus the light fragment charge is Z = 36, the Kr charge, ruling out any possible dominance of the Xe charge of the heavy fragment. The proton numbers 36 and 54 appear hence somehow “magic” in spite of related shells absence in the shell model. In the long chain of actinide fission the Z = 54 charge of the heavy fragment automatically fixes the charge of the light fragment [<xref ref-type="bibr" rid="scirp.82029-ref16">16</xref>] , because of the proton number conservation in nuclear fission. Then <sub>38</sub>Sr appears less magic than <sub>54</sub>Xe since its top stability (<xref ref-type="fig" rid="fig3">Figure 3</xref> and <xref ref-type="fig" rid="fig5">Figure 5</xref>) is entirely due to the neutron magic number 50. The choice of Sr, to complement the most probable Sr-Xe couple of <xref ref-type="fig" rid="fig4">Figure 4</xref>, dictated by the Xe charge, appears in addition backed up by the top BE of the Sr isotope (<xref ref-type="fig" rid="fig3">Figure 3</xref>, <xref ref-type="fig" rid="fig5">Figure 5</xref>). An unknown physical situation helps the choice of the Z<sub>L</sub> fragment, of the Z<sub>L</sub>-Z<sub>H</sub> couples, in all of the low energy fissions of the actinides (<xref ref-type="fig" rid="fig3">Figure 3</xref>, <xref ref-type="fig" rid="fig6">Figure 6</xref>). Reasoning on the manifestation of fragment shells in nuclei undergoing fission the existence of a “shell” at Z = 54 was suggested, [<xref ref-type="bibr" rid="scirp.82029-ref14">14</xref>] <xref ref-type="fig" rid="fig7">Figure 7</xref>. The same figure, elaborated from a study of nuclear fission</p><p>down to <sub>83</sub>Tl, Itkis et al. [<xref ref-type="bibr" rid="scirp.82029-ref21">21</xref>] , may well justify a “shell” at Z = 36. The importance attributed here to the proton numbers 36 and 54 stems from the Kr and Xe features stressed above coupled with the experimental data. The physics behind the present idea awaits investigation. It appears hidden in the nature of the Z number.</p><p>The apparent slay down of the block of isotopes, encompassed between the 50N and the 82N arrays (<xref ref-type="fig" rid="fig1">Figure 1</xref>), caused by the NE lowering of the 50N isoton array, if correct [<xref ref-type="bibr" rid="scirp.82029-ref19">19</xref>] , has an interesting outcome. It offers a frame for the interpretation of the post fission evaporation of neutrons, higher for the Z<sub>L</sub> compared to the Z<sub>H</sub> fragments; a tenet in actinide fission. This is because the 50N array interacts more extensively with the Z<sub>L</sub> fragments than the 82N array can do with the Z<sub>H</sub> fragments (<xref ref-type="fig" rid="fig4">Figure 4</xref>, <xref ref-type="fig" rid="fig6">Figure 6</xref>).</p><p><xref ref-type="fig" rid="fig6">Figure 6</xref> stresses that, for all thermal neutron actinide fissions, the yields of the heavy mass fragment groups start rising at A<sub>H</sub> = 130 amu, corresponding to the magic proton charge Z = 50. At <sup>100</sup>Sn<sup>50</sup> the suggested reduction of the element’s ability to harbour the EN vanishes, because the EN zeroes, and the element Sn rises its ability to harbour the NE. See the sharp rise, from Cd to Sn, of the NE accommodation ability (<xref ref-type="fig" rid="fig1">Figure 1</xref>). This observation from one side gives further credit to the element’s isotopes layout interpretation [<xref ref-type="bibr" rid="scirp.82029-ref19">19</xref>] and for the other side offers a hint for the interpretation of the 50 proton Z charge function in the <xref ref-type="fig" rid="fig6">Figure 6</xref>.</p><p>The importance of the 28 magic proton number in nuclear fission (<xref ref-type="fig" rid="fig3">Figure 3</xref>) is evident by the yield shoulder marked by <sup>70</sup>Ni isotope (<xref ref-type="fig" rid="fig7">Figure 7</xref>). At variance with <xref ref-type="fig" rid="fig4">Figure 4</xref>, the fission fragments yield is extended dawn to 10<sup>−</sup><sup>6</sup> %.</p><p>Few additional comments. <xref ref-type="fig" rid="fig1">Figure 1</xref> highlights, besides the double magic <sup>78</sup>Ni<sup>28</sup> (Ni<sub>22</sub>) and <sup>132</sup>Sn<sup>82</sup> (Sn<sub>32</sub>) other interesting isotopes (<xref ref-type="fig" rid="fig1">Figure 1</xref> legend). With the help of the NE numbers, it is easy to spot these isotopes in <xref ref-type="fig" rid="fig3">Figure 3</xref> and in <xref ref-type="fig" rid="fig5">Figure 5</xref>. The <sup>70</sup>Ni isotope is important because it marks the yield shoulder in the super asymmetric fission of <sup>245</sup>Cm<sub>(</sub><sub>n,f</sub><sub>)</sub> and of others actinides, <xref ref-type="fig" rid="fig7">Figure 7</xref> reproduced with permission [<xref ref-type="bibr" rid="scirp.82029-ref10">10</xref>] . The post neutron evaporation fragments and their β-decay to stable isotopes are an example of the <sup>235</sup>U<sub>(</sub><sub>n,f</sub><sub>)</sub> asymmetric fission [<xref ref-type="bibr" rid="scirp.82029-ref20">20</xref>] . The isotopic couples Xe-Sr, Te-Zr and Ba-Kr represent the pre neutron evaporation fragments of the three most probable charge yield in the electromagnetic induced fission of <sup>234</sup>U shown in <xref ref-type="fig" rid="fig4">Figure 4</xref> [<xref ref-type="bibr" rid="scirp.82029-ref11">11</xref>] . With the exception of the BE of Ni<sub>22</sub>, lying at the border of the neutron drip line, all other neutron rich isotopes appear removed from that line (<xref ref-type="fig" rid="fig3">Figure 3</xref>) [<xref ref-type="bibr" rid="scirp.82029-ref19">19</xref>] .</p></sec><sec id="s5"><title>5. Concluding Remarks</title><p>The element’s ability to harbour the NE (<xref ref-type="fig" rid="fig1">Figure 1</xref>) is central in nuclear fission. Xe and Kr proton charges rule the actinide and the <sup>180</sup>Tl β-delayed fission respectively, however all element’s proton numbers are important. In actinide fission the choice of Sr, in the most probable Sr-Xe caple, is not casual (<xref ref-type="fig" rid="fig3">Figure 3</xref>). An unknown physical determinant complement the fragment’s charges setting by the Xe charge. The phenomenon is general assisting all the fragmentations in actinide fission and the charge-mass staggering effect.</p></sec><sec id="s6"><title>Acknowledgements</title><p>The author thanks Maurizio Zanardini for the graphical work.</p></sec><sec id="s7"><title>Cite this paper</title><p>Menegus, F. (2018) A Suggestion Complementing the Magic Numbers Interpretation of the Nuclear Fission Phenomena. World Journal of Nuclear Science and Technology, 8, 11-22. https://doi.org/10.4236/wjnst.2018.81002</p></sec></body><back><ref-list><title>References</title><ref id="scirp.82029-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Bohr, N. and Wheeler, J.A. (1939) The Mechanism of the Nuclear Fission. 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