<?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.2015.67095</article-id><article-id pub-id-type="publisher-id">JMP-57372</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>
 
 
  Study of Levy Stability in Relativistic Heavy-Ion Collisions
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>aseem</surname><given-names>Bari</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>Muzamil</surname><given-names>A. Teli</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Shamsul</surname><given-names>H. Thoker</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Qudsia</surname><given-names>Gani</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Department of Physics, University of Kashmir, Srinagar, India</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>baritak@gmail.com(AB)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>11</day><month>06</month><year>2015</year></pub-date><volume>06</volume><issue>07</issue><fpage>912</fpage><lpage>920</lpage><history><date date-type="received"><day>27</day>	<month>April</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>20</month>	<year>June</year>	</date><date date-type="accepted"><day>24</day>	<month>June</month>	<year>2015</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>
 
 
  Multifractal analysis is carried out for the interactions of 4.5 A and 14.5 A GeV/c 28Si beams with emulsion, CNO and AgBr targets using the standard method of Gq moments. The R&#233;nyi dimensions Dq are evaluated and the results on self-similar multifractal spectra are presented. The variation of Dq with q is looked into and the findings reveal that the behaviour is in consistency with the multifractal characteristic of the multiplicity distributions in the various interactions studied. The self-similar multifractal spectra are found to be concave downwards with maximum at αq = 0. Further, L&#233;vy stability analysis is carried out for these interactions. The L&#233;vy stability index μ extracted from multifractal spectrum is found to lie in the range [0, 2] in agreement with the L&#233;vy stability theory.
 
</p></abstract><kwd-group><kwd>Multifractal</kwd><kwd> R&#233;nyi Dimensions</kwd><kwd> L&#233;vy Stability</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Study of high-energy nucleus-nucleus collisions may address several important issues concerning multiparticle production. Besides this, these collisions are envisaged to create conditions necessary for the production of quark-gluon plasma (QGP). Various studies [<xref ref-type="bibr" rid="scirp.57372-ref1">1</xref>] -[<xref ref-type="bibr" rid="scirp.57372-ref4">4</xref>] suggest the possibility of existence of a deconfined phase of matter comprising essentially of quarks and gluons at energy density ~3 GeV/fm<sup>3</sup> with a subsequent phase transition to hadrons. Several important and fascinating signatures [<xref ref-type="bibr" rid="scirp.57372-ref5">5</xref>] for the production of QGP have been proposed. One of the various possible approaches is to investigate the fluctuations in particle densities. Such investigations are carried out with the realization that a phase transition may give rise to fluctuations in individual events which may manifest as clear peaks or spikes in the phase space domains [<xref ref-type="bibr" rid="scirp.57372-ref6">6</xref>] - [<xref ref-type="bibr" rid="scirp.57372-ref8">8</xref>] . In the case of hydrodynamic turbulence, this aspect is studied via scaling properties of the moments of the relevant distributions as functions of the bin sizes of the phase space [<xref ref-type="bibr" rid="scirp.57372-ref9">9</xref>] .</p><p>An attempt to investigate some important characteristics of the mechanism involved in multiparticle production is made by Bialas and Peschanski [<xref ref-type="bibr" rid="scirp.57372-ref10">10</xref>] , who have suggested the power law behaviour for the factorial moments as function of successively decreasing phase space bins which is referred to as intermittency. The search for a link between intermittency and a phase transition leads to a thermodynamic formulation of fractal dimensions of which intermittency is a special case [<xref ref-type="bibr" rid="scirp.57372-ref11">11</xref>] - [<xref ref-type="bibr" rid="scirp.57372-ref14">14</xref>] . A fractal or a self-similar object has the characteristic property of satisfying a power law scaling behaviour which reflects the underlying dynamics [<xref ref-type="bibr" rid="scirp.57372-ref15">15</xref>] . The multifractal nature of the produced particles in heavy-ion collisions is studied in terms of generalized R&#233;nyi dimensions<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x5.png" xlink:type="simple"/></inline-formula>. In the present study, the method of multifractal moments [<xref ref-type="bibr" rid="scirp.57372-ref15">15</xref>] is used to evaluate<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x6.png" xlink:type="simple"/></inline-formula>.</p><p>It has been proposed [<xref ref-type="bibr" rid="scirp.57372-ref16">16</xref>] [<xref ref-type="bibr" rid="scirp.57372-ref17">17</xref>] that as a self-affine or a self-similar fractal system, the multiparticle final state in high energy collisions can be characterized by an important parameter―the L&#233;vy stability index<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x7.png" xlink:type="simple"/></inline-formula>. This parameter helps in classifying the intermittency regimes due to different kinds of phase transitions during cascading processes [<xref ref-type="bibr" rid="scirp.57372-ref18">18</xref>] . It has been suggested [<xref ref-type="bibr" rid="scirp.57372-ref19">19</xref>] that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x8.png" xlink:type="simple"/></inline-formula> may be an indication of thermal phase transition whereas <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x9.png" xlink:type="simple"/></inline-formula> corresponds to a non-thermal phase transition. According to the L&#233;vy stability theory [<xref ref-type="bibr" rid="scirp.57372-ref20">20</xref>] , the L&#233;vy index <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x10.png" xlink:type="simple"/></inline-formula> is confined to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x11.png" xlink:type="simple"/></inline-formula>. This parameter is also known as the degree of fractality, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x12.png" xlink:type="simple"/></inline-formula>for monofractals, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x13.png" xlink:type="simple"/></inline-formula>corresponds to “calm” singularities, whereas <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x14.png" xlink:type="simple"/></inline-formula> refers to “wild” singularities [<xref ref-type="bibr" rid="scirp.57372-ref20">20</xref>] . In the present work, the L&#233;vy stability index is extracted from the multifractal spectra using the approach formulated by Hu Yuan et al. [<xref ref-type="bibr" rid="scirp.57372-ref17">17</xref>] .</p></sec><sec id="s2"><title>2. Mathematical Formalism</title><p>For studying multifractality, a given pseudorapidity range, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x15.png" xlink:type="simple"/></inline-formula>, is divided into M bins of width<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x16.png" xlink:type="simple"/></inline-formula>. If <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x17.png" xlink:type="simple"/></inline-formula> denotes the particle multiplicity in the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x18.png" xlink:type="simple"/></inline-formula> bin, then the total number of particles in an event is estimated using the relation<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x19.png" xlink:type="simple"/></inline-formula>. The fraction of particles in the j<sup>th</sup> bin is given by:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x20.png" xlink:type="simple"/></inline-formula>. Once this fraction is known, the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x21.png" xlink:type="simple"/></inline-formula> order multifractal moment, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x20.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x22.png" xlink:type="simple"/></inline-formula>, is defined [<xref ref-type="bibr" rid="scirp.57372-ref15">15</xref>] [<xref ref-type="bibr" rid="scirp.57372-ref21">21</xref>] as:</p><disp-formula id="scirp.57372-formula585"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502230x23.png"  xlink:type="simple"/></disp-formula><p>where the summation is carried out over the non-empty bins only which constitute a fractal set.</p><p>On averaging over all the events in a data sample consisting of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x24.png" xlink:type="simple"/></inline-formula> events, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x25.png" xlink:type="simple"/></inline-formula>is expressed as:</p><disp-formula id="scirp.57372-formula586"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502230x26.png"  xlink:type="simple"/></disp-formula><p>For the fractal nature of rapidity distribution, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x27.png" xlink:type="simple"/></inline-formula>should exhibit the power law behaviour [<xref ref-type="bibr" rid="scirp.57372-ref22">22</xref>] over a range of small <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x28.png" xlink:type="simple"/></inline-formula> in the following fashion:</p><disp-formula id="scirp.57372-formula587"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502230x29.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x30.png" xlink:type="simple"/></inline-formula> are the mass exponents and may be determined using:</p><disp-formula id="scirp.57372-formula588"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502230x31.png"  xlink:type="simple"/></disp-formula><p>The spectral function, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x32.png" xlink:type="simple"/></inline-formula>, which can be obtained [<xref ref-type="bibr" rid="scirp.57372-ref15">15</xref>] by Legendre transform by using the standard procedure of multifractals [<xref ref-type="bibr" rid="scirp.57372-ref22">22</xref>] is calculated from</p><disp-formula id="scirp.57372-formula589"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502230x33.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x34.png" xlink:type="simple"/></inline-formula> given by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x34.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x35.png" xlink:type="simple"/></inline-formula> are referred to as the Lipschitz-Holder exponents [<xref ref-type="bibr" rid="scirp.57372-ref23">23</xref>] .</p><p>For a multifractal structure, the spectral function is a smooth function, concave downwards with its maximum at<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x36.png" xlink:type="simple"/></inline-formula>. The left <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x37.png" xlink:type="simple"/></inline-formula> and right <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x38.png" xlink:type="simple"/></inline-formula> wings of the plots of the function give a quantitative description of the fluctuation density in the dense and sparse regions of a single particle pseudorapidity distribution [<xref ref-type="bibr" rid="scirp.57372-ref21">21</xref>] - [<xref ref-type="bibr" rid="scirp.57372-ref23">23</xref>] . Inhomogeneity of the pseudorapidity distribution is determined by the width of the distribution. The non-exis- tence of a sharp peak in <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x39.png" xlink:type="simple"/></inline-formula> versus <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x40.png" xlink:type="simple"/></inline-formula> plot at <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x41.png" xlink:type="simple"/></inline-formula> corresponding to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x42.png" xlink:type="simple"/></inline-formula> reveals non-smooth nature of the pseudorapidity distribution in the phase space [<xref ref-type="bibr" rid="scirp.57372-ref24">24</xref>] .</p><p>One of the most basic properties of the fractals which describe the scaling behaviour are the multifractal R&#233;nyi dimensions, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x43.png" xlink:type="simple"/></inline-formula>, defined [<xref ref-type="bibr" rid="scirp.57372-ref25">25</xref>] as:</p><disp-formula id="scirp.57372-formula590"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502230x44.png"  xlink:type="simple"/></disp-formula><p>It may be of interest to note that if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x45.png" xlink:type="simple"/></inline-formula> decreases with increasing q, the pattern is known as multifractal and on the other hand, if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x46.png" xlink:type="simple"/></inline-formula> is constant, the pattern is referred to as monofractal [<xref ref-type="bibr" rid="scirp.57372-ref25">25</xref>] [<xref ref-type="bibr" rid="scirp.57372-ref26">26</xref>] .</p><p>The <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x47.png" xlink:type="simple"/></inline-formula> order multifractal R&#233;nyi dimensions <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x48.png" xlink:type="simple"/></inline-formula> can also be obtained from the multifractal spectrum <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x49.png" xlink:type="simple"/></inline-formula> through [<xref ref-type="bibr" rid="scirp.57372-ref9">9</xref>]</p><disp-formula id="scirp.57372-formula591"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502230x50.png"  xlink:type="simple"/></disp-formula><p>The L&#233;vy stability index <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x51.png" xlink:type="simple"/></inline-formula> is obtained by fitting the ratio <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x52.png" xlink:type="simple"/></inline-formula> to the formula [<xref ref-type="bibr" rid="scirp.57372-ref27">27</xref>]</p><disp-formula id="scirp.57372-formula592"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502230x53.png"  xlink:type="simple"/></disp-formula><p>which can be simplified to the form</p><disp-formula id="scirp.57372-formula593"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502230x54.png"  xlink:type="simple"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x55.png" xlink:type="simple"/></inline-formula>. Using the above equations, one gets</p><disp-formula id="scirp.57372-formula594"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502230x56.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.57372-formula595"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502230x57.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.57372-formula596"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502230x58.png"  xlink:type="simple"/></disp-formula><p>Therefore, if one defines</p><disp-formula id="scirp.57372-formula597"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502230x59.png"  xlink:type="simple"/></disp-formula><p>we get</p><disp-formula id="scirp.57372-formula598"><label>(14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502230x60.png"  xlink:type="simple"/></disp-formula><p>when<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x61.png" xlink:type="simple"/></inline-formula>.</p><p>On the basis of the above formalism, it has been proposed [<xref ref-type="bibr" rid="scirp.57372-ref17">17</xref>] that the L&#233;vy stability index <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x62.png" xlink:type="simple"/></inline-formula> can be obtained using the following procedure:</p><p> Find out the value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x63.png" xlink:type="simple"/></inline-formula> where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x64.png" xlink:type="simple"/></inline-formula>. call it B.</p><p> Fit the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x65.png" xlink:type="simple"/></inline-formula> part of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x66.png" xlink:type="simple"/></inline-formula> versus <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x66.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x67.png" xlink:type="simple"/></inline-formula> to a straight line and get the slope C.</p><p> Get the L&#233;vy stability index as</p><disp-formula id="scirp.57372-formula599"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502230x68.png"  xlink:type="simple"/></disp-formula></sec><sec id="s3"><title>3. Experimental Details</title><p>In the present study, a stack of ILFORD G5 emulsion, exposed to 14.5 A GeV/c <sup>28</sup>Si nuclei from the AGS (BNL) has been used. A random sample comprising of 283 interactions with<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x69.png" xlink:type="simple"/></inline-formula>, where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x70.png" xlink:type="simple"/></inline-formula> represents the number of charged particles produced in an interaction with relative velocity<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x71.png" xlink:type="simple"/></inline-formula>, is analyzed. In order to examine the dependence of various parameters of multiparticle production on beam energy, the data involving 530 interactions, with the same description, produced by 4.5 A GeV/c <sup>28</sup>Si nuclei from Synchrophasotron (Dubna), available in our laboratory are also analyzed. Various details, such as scanning procedure, criteria for selecting events and the method of measurements, etc may be found elsewhere [<xref ref-type="bibr" rid="scirp.57372-ref28">28</xref>] [<xref ref-type="bibr" rid="scirp.57372-ref29">29</xref>] . For the classification of the various particles emitted in the various interactions considered for the present study, the usual emulsion terminology [<xref ref-type="bibr" rid="scirp.57372-ref30">30</xref>] has been used. The emitted particles are classified in three categories, black, grey and shower particles, depending upon their limit of ionization and the relative velocity. Black particles <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x72.png" xlink:type="simple"/></inline-formula> refer to the particles with relative velocity<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x73.png" xlink:type="simple"/></inline-formula>. These are mainly target fragments with ionization<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x74.png" xlink:type="simple"/></inline-formula>, where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x75.png" xlink:type="simple"/></inline-formula> represents the the minimum ionization of a single charged particle. Grey particles <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x75.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x76.png" xlink:type="simple"/></inline-formula> exhibit ionization range <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x75.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x77.png" xlink:type="simple"/></inline-formula> and their relative velocity is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x75.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x77.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x78.png" xlink:type="simple"/></inline-formula>. And the shower particles <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x75.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x77.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x79.png" xlink:type="simple"/></inline-formula> which consist mainly of relativistic charged particles have the velocity <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x75.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x77.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x79.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x80.png" xlink:type="simple"/></inline-formula> and these are heavily ionizing in nature.</p><p>In the present study, we have classified the interactions due to different targets on the basis of the number of heavily ionizing particles <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x81.png" xlink:type="simple"/></inline-formula> produced in an interaction. Heavy particles are defined as the sum of black and grey tracks produced in an interaction i.e.,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x82.png" xlink:type="simple"/></inline-formula>. The interaction events for which <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x82.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x83.png" xlink:type="simple"/></inline-formula> are considered to be the interactions resulting from the CNO target of emulsion whereas, all the interaction events for which <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x82.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x83.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x84.png" xlink:type="simple"/></inline-formula> are attributed to the interactions due to AgBr target. The phase space variable which has been utilized to characterize the relativistic charged particles in the various interactions is the pseudorapidity variable</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x85.png" xlink:type="simple"/></inline-formula>with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x85.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x86.png" xlink:type="simple"/></inline-formula> representing the emission angle of the particle with respect to the direction of the pro-</p><p>jectile beam.</p></sec><sec id="s4"><title>4. Results and Discussion</title><sec id="s4_1"><title>4.1. R&#233;nyi Dimensions</title><p>Variations of the generalized R&#233;nyi dimensions, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x87.png" xlink:type="simple"/></inline-formula>, with the order of the moment, q, for <sup>28</sup>Si-Em interactions at the two incident energies are exhibited in <xref ref-type="fig" rid="fig1">Figure 1</xref>. For both the energies, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x87.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x88.png" xlink:type="simple"/></inline-formula>satisfies the multifractality condition, namely, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x87.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x88.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x89.png" xlink:type="simple"/></inline-formula>for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x87.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x88.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x90.png" xlink:type="simple"/></inline-formula>. The generalized R&#233;nyi dimensions are found to be positive for all orders of the moment q and demonstrate a decreasing trend with increasing q. The behaviour is in excellent agreement with the predictions of multifractal cascade model [<xref ref-type="bibr" rid="scirp.57372-ref31">31</xref>] . It may be noted that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x87.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x88.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x90.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x91.png" xlink:type="simple"/></inline-formula> turns out to be</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Variation of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x93.png" xlink:type="simple"/></inline-formula> with q for <sup>28</sup>Si-Em interactions at 4.5 A GeV/c and 14.5 A GeV/c</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-7502230x92.png"/></fig><p>more than unity for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x94.png" xlink:type="simple"/></inline-formula>, a result in agreement with those reported [<xref ref-type="bibr" rid="scirp.57372-ref32">32</xref>] earlier for different projectiles over a wide range of beam energies. It is also noticed in <xref ref-type="fig" rid="fig1">Figure 1</xref> that the generalized dimensions tend to attain higher values for higher projectile energy in the region characterized by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x94.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x95.png" xlink:type="simple"/></inline-formula>, i.e., for negative order moments. However, in the region having<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x94.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x95.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x96.png" xlink:type="simple"/></inline-formula>, this trend seems to change, but not very significantly. In order to examine whether there exists any dependence of the R&#233;nyi dimensions corresponding to a certain order of moment on the target size, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x94.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x95.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x96.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x97.png" xlink:type="simple"/></inline-formula>vs q plots for the interactions of <sup>28</sup>Si nuclei with CNO and AgBr targets are plotted in <xref ref-type="fig" rid="fig2">Figure 2</xref>. The R&#233;nyi dimensions have higher values for the interactions due to heavier targets for each order of the moment although the effect appears to be rather more pronounced for the situation corresponding to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x94.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x95.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x96.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x97.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x98.png" xlink:type="simple"/></inline-formula>. One of the reasons for the higher values of the R&#233;nyi dimensions for the interactions due to heavier targets may be attributed to increase in the average multiplicity with increasing target mass [<xref ref-type="bibr" rid="scirp.57372-ref33">33</xref>] .</p></sec><sec id="s4_2"><title>4.2. Multifractal Spectra</title><p><xref ref-type="fig" rid="fig3">Figure 3</xref> shows the variation of the spectral function, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x99.png" xlink:type="simple"/></inline-formula>, with the Lipschitz-Holder exponents, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x100.png" xlink:type="simple"/></inline-formula>, for 4.5 A and 14.5 A GeV/c <sup>28</sup>Si-Em interactions. The spectra are concave downwards centered around <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x101.png" xlink:type="simple"/></inline-formula> corresponding to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x102.png" xlink:type="simple"/></inline-formula> and a common tangent at an angle of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x103.png" xlink:type="simple"/></inline-formula>. This observation agrees fairly well with the predictions of gluon model [<xref ref-type="bibr" rid="scirp.57372-ref15">15</xref>] . However, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x103.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x104.png" xlink:type="simple"/></inline-formula>is not peaked in any of the cases studied which is an indication of non-smooth nature of the multiplicity distribution of the particles produced in the interactions considered in the present study. The left wings <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x103.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x104.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x105.png" xlink:type="simple"/></inline-formula> of the spectra are sensitive to the peaks whilst the right wings <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x103.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x104.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x105.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x106.png" xlink:type="simple"/></inline-formula> belong to the valleys in their respective pseudorapidity distributions. The spectra at the two energies are nearly similar in the left wings. However, in the right wing corresponding to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x103.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x104.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x105.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x106.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x107.png" xlink:type="simple"/></inline-formula>, the spectrum for the higher energy tends to broaden.</p><fig-group id="fig2"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Variation of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x110.png" xlink:type="simple"/></inline-formula> with q for the interactions of <sup>28</sup>Si nuclei with CNO and AgBr targets at: (a) 4.5 A GeV/c and (b) 14.5 A GeV/c.</title></caption><fig id ="fig2_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-7502230x108.png"/></fig><fig id ="fig2_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-7502230x109.png"/></fig></fig-group><fig-group id="fig3"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Variation of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x113.png" xlink:type="simple"/></inline-formula> with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x113.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x114.png" xlink:type="simple"/></inline-formula> for <sup>28</sup>Si-Em interactions at: (a) 4.5 A GeV/c and (b) 14.5 A GeV/c.</title></caption><fig id ="fig3_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-7502230x111.png"/></fig><fig id ="fig3_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-7502230x112.png"/></fig></fig-group><p>For investigating whether <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x115.png" xlink:type="simple"/></inline-formula> spectra depend on target mass, the spectra for the interactions of <sup>28</sup>Si nuclei with CNO and AgBr targets are plotted in <xref ref-type="fig" rid="fig4">Figure 4</xref> for both the energies. It is observed that for the interactions due to AgBr targets the spectra have larger widths in comparison to the spectra for the interactions due to lighter (CNO) targets. It may further be noted that the contribution to the broadening of the width of the spectra with increasing target mass comes mainly from the regions corresponding to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x115.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x116.png" xlink:type="simple"/></inline-formula>. However, all the spectra are wide enough to indicate the occurrence of multifractality for the interactions considered.</p></sec><sec id="s4_3"><title>4.3. L&#233;vy Stability Index</title><p>The variation of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x117.png" xlink:type="simple"/></inline-formula> with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x117.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x118.png" xlink:type="simple"/></inline-formula> for the interaction of <sup>28</sup>Si nuclei with emulsion at 4.5 A and 14.5 A GeV/c are presented in <xref ref-type="fig" rid="fig5">Figure 5</xref>. The solid lines in the figures represent linear fittings to the data. Si- milar plots for interactions with CNO and AgBr targets are represented in <xref ref-type="fig" rid="fig6">Figure 6</xref> and <xref ref-type="fig" rid="fig7">Figure 7</xref>. The L&#233;vy sta- bility indicies for the various types of interactions evaluated by linear fittings to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x117.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x118.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x119.png" xlink:type="simple"/></inline-formula> with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x117.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x118.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x119.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x120.png" xlink:type="simple"/></inline-formula> plots are given in <xref ref-type="table" rid="table1"><xref ref-type="table" rid="table">Table </xref>1</xref>. It is clearly evident from the <xref ref-type="table" rid="table">Table </xref>that the L&#233;vy stable index for all the interactions studied in the present work lies in the range [0, 2] in consistency with the L&#233;vy stability theory.</p><fig-group id="fig4"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Variation of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x123.png" xlink:type="simple"/></inline-formula> with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x123.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x124.png" xlink:type="simple"/></inline-formula> for the interactions of <sup>28</sup>Si nuclei with CNO and AgBr targets at: (a) 4.5 A GeV/c and (b) 14.5 A GeV/c.</title></caption><fig id ="fig4_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-7502230x121.png"/></fig><fig id ="fig4_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-7502230x122.png"/></fig></fig-group><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> Variation of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x126.png" xlink:type="simple"/></inline-formula> with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x126.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x127.png" xlink:type="simple"/></inline-formula> for <sup>28</sup>Si-Em interactions at 4.5 A GeV/c and 14.5 A GeV/c</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-7502230x125.png"/></fig><fig id="fig6"  position="float"><label><xref ref-type="fig" rid="fig6">Figure 6</xref></label><caption><title> Variation of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x129.png" xlink:type="simple"/></inline-formula> with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x129.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x130.png" xlink:type="simple"/></inline-formula> for the interactions of <sup>28</sup>Si nuclei with CNO and AgBr targets at 4.5 A GeV/c</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-7502230x128.png"/></fig><fig id="fig7"  position="float"><label><xref ref-type="fig" rid="fig7">Figure 7</xref></label><caption><title> Variation of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x132.png" xlink:type="simple"/></inline-formula> with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x132.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x133.png" xlink:type="simple"/></inline-formula> for the interactions of <sup>28</sup>Si nuclei with CNO and AgBr targets at 14.5 A GeV/c</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-7502230x131.png"/></fig></sec></sec><sec id="s5"><title>5. Conclusion</title><p>The multifractal R&#233;nyi dimensions for the interactions of 4.5 A and 14.5 A GeV/c <sup>28</sup>Si nuclei with CNO and AgBr targets exhibit a behaviour which manifests the multifractal nature of the multiparticle final state in these interactions. The R&#233;nyi dimensions are found to obey the basic law of multifractality. Further, the R&#233;nyi dimensions exhibit a dependence on the target mass; the values of R&#233;nyi dimensions are higher for heavier target mass. The multifractal spectrum is observed to be concave downwards with maximum corresponding to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x134.png" xlink:type="simple"/></inline-formula> which supports the multifractality in the multiparticle production in the various interactions studied in the present work.</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1"><xref ref-type="table" rid="table">Table </xref>1</xref></label><caption><title> Values of the L&#233;vy stability index <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x135.png" xlink:type="simple"/></inline-formula> for the collisions of 4.5 A GeV/c <sup>28</sup>Si nuclei with emulsion, CNO and AgBr obtained from the fitting a straight line to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x135.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x136.png" xlink:type="simple"/></inline-formula> versus <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x135.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x136.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502230x137.png" xlink:type="simple"/></inline-formula> plots</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Type of interaction</th><th align="center" valign="middle" >Energy (GeV)</th><th align="center" valign="middle" >L&#233;vy index (m)</th></tr></thead><tr><td align="center" valign="middle" >Si-Em</td><td align="center" valign="middle" >4.5 A</td><td align="center" valign="middle" >1.8036 &#177; 0.1144</td></tr><tr><td align="center" valign="middle" >Si-Em</td><td align="center" valign="middle" >14.5 A</td><td align="center" valign="middle" >1.8001 &#177; 0.1137</td></tr><tr><td align="center" valign="middle" >Si-CNO</td><td align="center" valign="middle" >4.5 A</td><td align="center" valign="middle" >1.8715 &#177; 0.0120</td></tr><tr><td align="center" valign="middle" >Si-CNO</td><td align="center" valign="middle" >14.5 A</td><td align="center" valign="middle" >1.7791 &#177; 0.1097</td></tr><tr><td align="center" valign="middle" >Si-AgBr</td><td align="center" valign="middle" >4.5 A</td><td align="center" valign="middle" >1.8239 &#177; 0.0608</td></tr><tr><td align="center" valign="middle" >Si-AgBr</td><td align="center" valign="middle" >14.5 A</td><td align="center" valign="middle" >1.7828 &#177; 0.0896</td></tr></tbody></table></table-wrap><p>The L&#233;vy stability indicies evaluated from the multifractal spectra for these interactions lie in the range [0, 2] which is in consistency with the L&#233;vy stability theory.</p></sec><sec id="s6"><title>Acknowledgements</title><p>The authors are thankful to Professor Nisar A. 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