{"title":"Event-by-Event Particle Ratio Fluctuations at LHC Energies","authors":"Shaista Khan, B. Ali, A. Chandra, S. Ahmad","doi":"10.1155/2021/6663846","DOIUrl":null,"url":null,"abstract":"<jats:p>A Monte Carlo study of identified particle ratio fluctuations at LHC energies is carried out in the framework of HIJING model using the fluctuation variable <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M1\">\n <msub>\n <mrow>\n <mi>ν</mi>\n </mrow>\n <mrow>\n <mtext>dyn</mtext>\n </mrow>\n </msub>\n </math>\n </jats:inline-formula>. The simulated events for Pb-Pb collisions at <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M2\">\n <msub>\n <mrow>\n <msqrt>\n <mrow>\n <mi>s</mi>\n </mrow>\n </msqrt>\n </mrow>\n <mrow>\n <mi>N</mi>\n <mi>N</mi>\n </mrow>\n </msub>\n <mo>=</mo>\n <mn>2.76</mn>\n </math>\n </jats:inline-formula> and 5.02 TeV and Xe-Xe collisions at <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M3\">\n <msub>\n <mrow>\n <msqrt>\n <mrow>\n <mi>s</mi>\n </mrow>\n </msqrt>\n </mrow>\n <mrow>\n <mi>N</mi>\n <mi>N</mi>\n </mrow>\n </msub>\n <mo>=</mo>\n <mn>5.44</mn>\n <mtext> </mtext>\n <mtext>TeV</mtext>\n </math>\n </jats:inline-formula> are analyzed. From this study, it is observed that the values of <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M4\">\n <mfenced open=\"[\" close=\"]\">\n <mrow>\n <mi>π</mi>\n <mo>,</mo>\n <mi>K</mi>\n </mrow>\n </mfenced>\n </math>\n </jats:inline-formula>, <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M5\">\n <mfenced open=\"[\" close=\"]\">\n <mrow>\n <mi>p</mi>\n <mo>,</mo>\n <mi>K</mi>\n </mrow>\n </mfenced>\n </math>\n </jats:inline-formula>, and <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M6\">\n <mfenced open=\"[\" close=\"]\">\n <mrow>\n <mi>π</mi>\n <mo>,</mo>\n <mi>p</mi>\n </mrow>\n </mfenced>\n </math>\n </jats:inline-formula> follow the similar trends of energy dependence as observed in the most central collision data by NA49, STAR, and ALICE experiments. It is also observed that <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M7\">\n <msub>\n <mrow>\n <mi>ν</mi>\n </mrow>\n <mrow>\n <mtext>dyn</mtext>\n </mrow>\n </msub>\n </math>\n </jats:inline-formula> for all the three combinations of particles for semicentral and central collisions, the model predicted values of <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M8\">\n <msub>\n <mrow>\n <mi>ν</mi>\n </mrow>\n <mrow>\n <mtext>dyn</mtext>\n </mrow>\n </msub>\n <mfenced open=\"[\" close=\"]\">\n <mrow>\n <mi>A</mi>\n <mo>,</mo>\n <mi>B</mi>\n </mrow>\n </mfenced>\n </math>\n </jats:inline-formula> for Pb-Pb collisions at <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M9\">\n <msub>\n <mrow>\n <msqrt>\n <mrow>\n <mi>s</mi>\n </mrow>\n </msqrt>\n </mrow>\n <mrow>\n <mi>N</mi>\n <mi>N</mi>\n </mrow>\n </msub>\n <mo>=</mo>\n <mn>2.76</mn>\n <mtext> </mtext>\n <mtext>TeV</mtext>\n </math>\n </jats:inline-formula> agree fairly well with those observed in the ALICE experiment. For peripheral collisions, however, the model predicted values of <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M10\">\n <msub>\n <mrow>\n <mi>ν</mi>\n </mrow>\n <mrow>\n <mtext>dyn</mtext>\n </mrow>\n </msub>\n <mfenced open=\"[\" close=\"]\">\n <mrow>\n <mi>π</mi>\n <mo>,</mo>\n <mi>K</mi>\n </mrow>\n </mfenced>\n </math>\n </jats:inline-formula> are somewhat smaller, whereas for <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M11\">\n <mfenced open=\"[\" close=\"]\">\n <mrow>\n <mi>p</mi>\n <mo>,</mo>\n <mi>K</mi>\n </mrow>\n </mfenced>\n </math>\n </jats:inline-formula> and <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M12\">\n <mfenced open=\"[\" close=\"]\">\n <mrow>\n <mi>π</mi>\n <mo>,</mo>\n <mi>p</mi>\n </mrow>\n </mfenced>\n </math>\n </jats:inline-formula> it predicts larger values as compared to the corresponding experimental values. The possible reasons for the observed differences are discussed. The <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M13\">\n <msub>\n <mrow>\n <mi>ν</mi>\n </mrow>\n <mrow>\n <mtext>dyn</mtext>\n </mrow>\n </msub>\n </math>\n </jats:inline-formula> values scaled with charged particle density when plotted against <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M14\">\n <mfenced open=\"〈\" close=\"〉\">\n <mrow>\n <msub>\n <mrow>\n <mi>N</mi>\n </mrow>\n <mrow>\n <mtext>part</mtext>\n </mrow>\n </msub>\n </mrow>\n </mfenced>\n </math>\n </jats:inline-formula> exhibit a flat behaviour, as expected from the independent particle emission sources. For <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M15\">\n <mfenced open=\"[\" close=\"]\">\n <mrow>\n <mi>p</mi>\n <mo>,</mo>\n <mi>K</mi>\n </mrow>\n </mfenced>\n </math>\n </jats:inline-formula> and <jats:inline-formula>\n <math xmlns=\"http://www.w3.org/1998/Math/MathML\" id=\"M16\">\n <mfenced open=\"[\" close=\"]\">\n <mrow>\n <mi>π</mi>\n <mo>,</mo>\n ","PeriodicalId":7498,"journal":{"name":"Advances in High Energy Physics","volume":" ","pages":""},"PeriodicalIF":1.5000,"publicationDate":"2021-08-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Advances in High Energy Physics","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1155/2021/6663846","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"PHYSICS, PARTICLES & FIELDS","Score":null,"Total":0}
引用次数: 1
Abstract
A Monte Carlo study of identified particle ratio fluctuations at LHC energies is carried out in the framework of HIJING model using the fluctuation variable . The simulated events for Pb-Pb collisions at and 5.02 TeV and Xe-Xe collisions at are analyzed. From this study, it is observed that the values of , , and follow the similar trends of energy dependence as observed in the most central collision data by NA49, STAR, and ALICE experiments. It is also observed that for all the three combinations of particles for semicentral and central collisions, the model predicted values of for Pb-Pb collisions at agree fairly well with those observed in the ALICE experiment. For peripheral collisions, however, the model predicted values of are somewhat smaller, whereas for and it predicts larger values as compared to the corresponding experimental values. The possible reasons for the observed differences are discussed. The values scaled with charged particle density when plotted against exhibit a flat behaviour, as expected from the independent particle emission sources. For and
期刊介绍:
Advances in High Energy Physics publishes the results of theoretical and experimental research on the nature of, and interaction between, energy and matter. Considering both original research and focussed review articles, the journal welcomes submissions from small research groups and large consortia alike.