<?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.2016.712137</article-id><article-id pub-id-type="publisher-id">JMP-70090</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>
 
 
  Complete Destruction of Ag Br Emulsion Nuclei BY&lt;sup&gt;28&lt;/sup&gt;Si Ions with 4.5 GeV/Nucleon Energy
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>A.</surname><given-names>Abd EL-Daiem</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Physics Department, Faculty of Science, Sohag University, Sohag, Egypt</addr-line></aff><author-notes><corresp id="cor1">* E-mail:</corresp></author-notes><pub-date pub-type="epub"><day>02</day><month>08</month><year>2016</year></pub-date><volume>07</volume><issue>12</issue><fpage>1506</fpage><lpage>1511</lpage><history><date date-type="received"><day>4</day>	<month>July</month>	<year>2016</year></date><date date-type="rev-recd"><day>accepted</day>	<month>22</month>	<year>August</year>	</date><date date-type="accepted"><day>25</day>	<month>August</month>	<year>2016</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>
 
 
  The main experimental characteristics (multiplicity characteristics) of secondary particles have been investigated in interactions of 
  <sup>28</sup>Si with emulsion at 4.5 GeV/c per nucleon at rest of emulsion, nuclei. The complete destruction of the heavy target nuclei (Ag, Br) has been studied. The average of shower particles &lt; n
  <sub>s</sub> &gt; is weakly dependent on the target mass whereas the average multiplicity of grey particles &lt; n
  <sub>g</sub> &gt; is strongly dependent on it. The correlations between the multiplicities of the charged secondaries at different mass number of the projectile and center-of-mass-available energy are investigated.
 
</p></abstract><kwd-group><kwd>Multiplicity Characteristics</kwd><kwd> Probability and Energy Available</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The study of the phenomena of complete destruction of heavy target nuclei is very interesting. This interest stems from the fact that most of these interactions are due to central collisions. The central collisions provide a unique opportunity to investigate the consequences of nuclear compression, such as hydrodynamic effects [<xref ref-type="bibr" rid="scirp.70090-ref1">1</xref>] - [<xref ref-type="bibr" rid="scirp.70090-ref4">4</xref>] . In addition, there is a good possibility to obtain valuable information on the excitation and consequent decay of residual target nucleus. A detailed and systematic study of this phenomenon was carried out in [<xref ref-type="bibr" rid="scirp.70090-ref5">5</xref>] . In this work the criterion n<sub>h</sub> ≥ 28, since [n<sub>h</sub> = (n<sub>g</sub> + n<sub>b</sub>) gray particles and black particles] was used to select events of complete destruction of (Ag, Br) nuclei. Nowadays, there are huge amounts of data concerning the study of this phenomenon. Different beam nuclei at various energies have been used in the experiments. There are two main directions for the interpretation of the experimental results of complete destructions. The first direction considers such events as a tail in the multiplicity distribution which can be accounted for by the cascade evaporation process inside the target nucleus. The second one implies a one-step like process which occurs due to the collectivity of the target nucleons together. In the present work, we study complete destruction n<sub>h</sub> ≥ 28 of (Ag, Br) emulsion nuclei induced by 4.5 A GeV/c <sup>28</sup>Si nuclei. The average multiplicities of the different emitted charged particles have been compared with the corresponding experimental values obtained from the interactions of different types of nuclei with emulsion at the same incident momentum per nucleon. The energy available in the centre of mass system for the complete destruction of the target nucleus has been studied for different projectiles. The multiplicity correlations between the charged secondaries produced in these interactions and both the mass number of the projectile and the available energy have also been analyzed. The previous detailed analysis [<xref ref-type="bibr" rid="scirp.70090-ref6">6</xref>] has shown that the selection criterion n<sub>h</sub> ≥ 28 corresponds to the complete destruction of the target nucleus, nearly, into individual nucleons and light fragments leaving no measurable residual nucleus.</p></sec><sec id="s2"><title>2. Experimental Techniques</title><p>Nuclear emulsions of the type BR-2 were exposed to 4.5 A GeV/c <sup>28</sup>Si beams at the Dubnasynchrophasotron. The pellicles of emulsion have the dimensions of 20 cm &#215; 10 cm &#215; 600 &#181;m (undeveloped emulsion). The intensity of the beam was ~10<sup>4</sup> particles/cm<sup>2</sup> and the beam diameter was approximately 1 cm. Along the track, a double scanning has been carried out fast in the forward direction and slow in the backward one. In the measured interactions, all the charged secondary particles have been classified according to the range L in the emulsion and the relative ionization g<sup>*</sup> = g/g<sub>0</sub>, where g is the particle track ionization and g<sub>0 </sub>is the ionization of a relativistic shower track in the narrow forward cone of an polar angle θ ≤ 3˚, (the polar angle θ of each track, i.e. the space angle between the direction of the beam and that of the given tracks) into the following groups:</p><p>1) Shower tracks of produced particles, “s-particles”; have a relative ionization g<sup>*</sup> ≤ 1.4; these tracks have an emission angle θ ≤ 3˚; they have been further subjected to multiple scattering measurements for momentum determination in order to separate the produced pions from the single charged projectile fragments. 2) Grey tracks of produced particles, “g-particles”, having a relative ionization (1.4 ≤ g<sup>*</sup> &lt; 10) and L &gt; 3 mm. 3) Black tracks of produced particles, “b-particles”, having L ≤ 3 mm. 4) The b and g tracks, taking together, are both called heavily ionizing particles, “h-particles”.</p></sec><sec id="s3"><title>3. The Multiplicity Characteristics</title><p>To investigate the dependence of the average multiplicity s&gt; and g&gt; on the mass number of the beam nucleus A <sub>p</sub>, we consider the reactions listed in <xref ref-type="table" rid="table1">Table 1</xref>. <sub> <sub></sub></sub></p><p>In these reactions, the momentum per incident nucleon is constant and it equals 4.5 GeV/c. The experiments were carried out under the same conditions. <xref ref-type="fig" rid="fig1">Figure 1</xref>(a) and <xref ref-type="fig" rid="fig1">Figure 1</xref>(b) show the dependence of the average multiplicities s&gt; and g&gt; on the mass number of the beam nucleus A <sub>p</sub>. The points are the experimental data while the continuous lines are the result of fitting by the relation <sub> <sub></sub></sub></p><disp-formula id="scirp.70090-formula293"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-7502565x6.png"  xlink:type="simple"/></disp-formula><p>where i = s or g. The values of the coefficients a<sub>i</sub> are 0.39 &#177; 0.05 and 0.18 &#177; 0.01 and a<sub>i</sub> are 2.21 &#177; 0.66 and</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> The average multiplicities s&gt; and g&gt; of shower and grey tracks produced in the reactions of different projectiles with emulsion at 4.5 A GeV/c. <sub> <sub></sub></sub></title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Projectile</th><th align="center" valign="middle" >s&gt;</th><th align="center" valign="middle" >g&gt;</th><th align="center" valign="middle" >Ref</th></tr></thead><tr><td align="center" valign="middle" ><sup>1</sup>H</td><td align="center" valign="middle" >1.6 &#177; 0.1</td><td align="center" valign="middle" >2.8 &#177; 0.1</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.70090-ref7">7</xref>]</td></tr><tr><td align="center" valign="middle" ><sup>2</sup>H</td><td align="center" valign="middle" >2.5 &#177; 0.1</td><td align="center" valign="middle" >3.9 &#177; 0.1</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.70090-ref8">8</xref>]</td></tr><tr><td align="center" valign="middle" ><sup>3</sup>H</td><td align="center" valign="middle" >3.6 &#177; 0.1</td><td align="center" valign="middle" >3.1 &#177; 0.1</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.70090-ref9">9</xref>]</td></tr><tr><td align="center" valign="middle" ><sup>4</sup>He</td><td align="center" valign="middle" >3.8 &#177; 0.1</td><td align="center" valign="middle" >4.4 &#177; 0.1</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.70090-ref7">7</xref>]</td></tr><tr><td align="center" valign="middle" ><sup>12</sup>C</td><td align="center" valign="middle" >7.6 &#177; 0.2</td><td align="center" valign="middle" >5.9 &#177; 0.3</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.70090-ref7">7</xref>]</td></tr><tr><td align="center" valign="middle" ><sup>16</sup>O</td><td align="center" valign="middle" >10.5 &#177; 0.6</td><td align="center" valign="middle" >7.6 &#177; 0.6</td><td align="center" valign="middle" >[<xref ref-type="bibr" rid="scirp.70090-ref10">10</xref>]</td></tr><tr><td align="center" valign="middle" ><sup>28</sup>Si</td><td align="center" valign="middle" >11.9 &#177; 0.5</td><td align="center" valign="middle" >7.3 &#177; 0.3</td><td align="center" valign="middle" >Present work</td></tr></tbody></table></table-wrap><fig-group id="fig1"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Projectile mass number for different elements at 4.5 GeV/c per Nucleon: (a) versus s&gt; and (b) versus g&gt; plots. <sub> <sub></sub></sub></title></caption><fig id ="fig1_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/12-7502565x7.png"/></fig><fig id ="fig1_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/12-7502565x8.png"/></fig></fig-group><p>3.11 &#177; 0.06 for shower and grey particles respectively. This result agrees with the fact that the interaction cross section is proportional to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-7502565x9.png" xlink:type="simple"/></inline-formula> and is proportional to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-7502565x10.png" xlink:type="simple"/></inline-formula> from s&gt; and g&gt;. <sub> <sub></sub></sub></p></sec><sec id="s4"><title>4. Probability of Complete Destruction of Target Nuclei</title><p>In the present work, the probability of complete destruction of (Ag, Br) emulsion nuclei p is defined as the ratio between the number of events of n<sub>h</sub> &#179; 28 to the total number of inelastic interactions of the incident particle with (Ag, Br) nuclei. <xref ref-type="fig" rid="fig2">Figure 2</xref> illustrates the dependence of the probability p on A<sub>p</sub> for various projectile nuclei, all at 4.5 A GeV/c. It is seen that the probability p increases linearly with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-7502565x11.png" xlink:type="simple"/></inline-formula> up to the carbon nucleus<sup>.</sup> The values of the probability p, predicted by the cascade evaporation model [<xref ref-type="bibr" rid="scirp.70090-ref8">8</xref>] , are larger than the corresponding experimental values. Moreover, the behavior of probability p versus A<sub>p</sub> in the present experiment does not agree with the calculations of the cascade evaporation model.</p></sec><sec id="s5"><title>5. Energy Available</title><p>For the events having n<sub>h</sub> ≥ 28, and implying the complete destruction of the target nuclei, the relation between s&gt; and the energy available E <sub>av</sub> in the centre of mass system is shown in <xref ref-type="fig" rid="fig3">Figure 3</xref>. The value of E <sub>av</sub> is given by: <sub></sub></p><disp-formula id="scirp.70090-formula294"><label>, (2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-7502565x12.png"  xlink:type="simple"/></disp-formula><p>where M<sub>p</sub>, is the projectile rest mass in GeV and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-7502565x13.png" xlink:type="simple"/></inline-formula> where p<sub>0</sub> is the projectile momentum in</p><p>GeV/c. The effective target mass M<sub>t</sub> is equal to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-7502565x14.png" xlink:type="simple"/></inline-formula>, where m = 0.931 GeV. The relation between s&gt; <sub></sub></p><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> The probability, p, of complete destruction of (Ag, Br) nuclei due to the interactions of different projectile at 4.5 GeV/c per nucleon</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/12-7502565x15.png"/></fig><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> The average multiplicity of shower particles s&gt; versus the energy in available c.m.s. for different projectile mass numbers having momentum 4.5 GeV/c per nucleon . for the collisions characterized by n <sub>h</sub> ≥ 28. <sub></sub></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/12-7502565x16.png"/></fig><p>and the energy available in the centre of mass system, E<sub>av</sub>, for different projectiles at the same incident momentum, which shows that as the projectile mass number increases, E<sub>av</sub> increases and consequently s&gt; increases. The dependence of s&gt; on E <sub>av</sub>, shown in <xref ref-type="fig" rid="fig3">Figure 3</xref>, can be fitted by the universal relation: <sub> <sub></sub></sub></p><disp-formula id="scirp.70090-formula295"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/12-7502565x17.png"  xlink:type="simple"/></disp-formula><p>with A = −13.09 and B = 11.46.</p></sec><sec id="s6"><title>6. Multiplicity Correlation in Complete Destruction of <sup>28</sup>Si Ions</title><p>In the present work, we studied the correlation of complete destruction (n<sub>h</sub> ≥ 28) of (Ag, Br) emulsion nuclei in&#173;duced by 4.5 A GeV/c <sup>28</sup>Si nuclei. The probability of complete destruction of AgBr nuclei different projectile at various energies is shown in [<xref ref-type="bibr" rid="scirp.70090-ref11">11</xref>] . The correlation in complete destruction dependencies between the charge particle multiplicities allows us to discuss the mechanism of nucleus-nucleus interactions. The dependencies = f (n <sub>s</sub>) and s&gt; = f (n <sub>g</sub>) for the event with n <sub>h</sub> ≥ 28 accompanied by total target disintegration are presented in <xref ref-type="fig" rid="fig4">Figure 4</xref> and <xref ref-type="table" rid="table2">Table 2</xref>. In this case there is no strong dependence of g&gt; on the value of ns or of s&gt; on the value of n <sub>g</sub>. This can be seen from the value of χ <sup>2</sup> for each type of particle. This means that the degree of <sub> <sub> <sub> </sub></sub></sub></p><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> The correlations between the secondary particles multiplicities for complete destructions (events with n<sub>h</sub> &gt; 28) in Si<sup>28</sup> interactions with emulsions</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/12-7502565x18.png"/></fig><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> Results of approximate fit of the experimental data for the multiplicity correlation from complete destruction in <sup>28</sup>Si ions interactions with emulsion using the dependence i&gt; = a + kn <sub>j</sub>. <sub></sub></title></caption><table><tbody><thead><tr><th align="center" valign="middle" ></th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-7502565x19.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-7502565x20.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-7502565x21.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-7502565x22.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-7502565x23.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-7502565x24.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-7502565x25.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-7502565x26.png" xlink:type="simple"/></inline-formula></th></tr></thead><tr><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-7502565x27.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" >…</td><td align="center" valign="middle" >…</td><td align="center" valign="middle" >14.02 &#177; 0.23 <sup> </sup></td><td align="center" valign="middle" >0.87</td><td align="center" valign="middle" >−15.60 &#177; 0.07</td><td align="center" valign="middle" >0.56</td><td align="center" valign="middle" >29.65 &#177; 0.16</td><td align="center" valign="middle" >0.95</td></tr><tr><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-7502565x31.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" >10.42 &#177; 0.76</td><td align="center" valign="middle" >0.96</td><td align="center" valign="middle" >…</td><td align="center" valign="middle" >…</td><td align="center" valign="middle" >19.60 &#177; 0.25</td><td align="center" valign="middle" >0.65</td><td align="center" valign="middle" >20.30 &#177; 0.69</td><td align="center" valign="middle" >0.95</td></tr><tr><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-7502565x35.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" >−33.10 &#177; 0.54</td><td align="center" valign="middle" >0.94</td><td align="center" valign="middle" >14.02 &#177; 0.23</td><td align="center" valign="middle" >0.84</td><td align="center" valign="middle" >…</td><td align="center" valign="middle" >…</td><td align="center" valign="middle" >27.09 &#177; 0.58</td><td align="center" valign="middle" >0.87</td></tr></tbody></table></table-wrap><p>disintegration of the target does not depend strongly on the number of shower particles. One can observe the correlation between the fast and the slow stages of the inelastic interactions of tow nuclei by studying the dependencies b&gt; = f (n <sub>s</sub>), b&gt; = f (n <sub>g</sub>) and (n <sub>s</sub>), (n <sub>g</sub>) on the (n <sub>b</sub>). From <xref ref-type="fig" rid="fig4">Figure 4</xref>, one can see that the correlations have a different character. This can be seen from the fast that the b&gt; dependencies on n <sub>s</sub> and n <sub>g</sub> have negative slopes. Also, from the correlation dependencies of s&gt;, g&gt; and h&gt; on n <sub>b</sub>, one can see that the slope of h&gt; is positive while the slopes of others are negative. From the above results, one can see that b&gt; has a negative cor&#173;relation with n <sub>s</sub> and n <sub>g</sub> and the correlation of s&gt; and g&gt; with the n <sub>b</sub> is negative. This may be due to increase the number of interacting projectile nucleons as the impact parameter decreases. <sub> <sub> <sub> <sub> <sub> <sub> <sub> <sub> <sub> <sub></sub></sub></sub></sub></sub></sub></sub></sub></sub></sub></p></sec><sec id="s7"><title>7. Conclusion</title><p>From the present study, one may concluded that the average number of the shower particles is proportional to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-7502565x39.png" xlink:type="simple"/></inline-formula> and the average number of grey particles is proportional to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-7502565x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/12-7502565x40.png" xlink:type="simple"/></inline-formula>. While that the probability of the complete destruction increases with increasing projectile mass number A<sub>p</sub>, and the average multiplicity of the emitted shower particles depends strongly on the projectile mass number, while does not for the grey and black can be particles. A good correlation between the energy available at the center of mass system, E<sub>av</sub>, and the average multiplicity of the shower particles emitted in the complete destruction is found.</p></sec><sec id="s8"><title>Cite this paper</title><p>A. Abd EL-Daiem, (2016) Complete Destruction of Ag Br Emulsion Nuclei BY<sup>28</sup>Si Ions with 4.5 GeV/Nucleon Energy. Journal of Modern Physics,07,1506-1511. doi: 10.4236/jmp.2016.712137</p></sec></body><back><ref-list><title>References</title><ref id="scirp.70090-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Beavis, D., et al. 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