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Energy Dependence of Moments of Net-proton Multiplicity Distributions at RHIC
We report the beam energy (\sqrt s_{NN} = 7.7 - 200 GeV) and collision centrality dependence of the mean (M), standard deviation (\sigma), skewness (S), and kurtosis (\kappa) of the net-proton multiplicity distributions in Au+Au collisions. The measurements are carried out by the STAR experiment at...
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creator | Adamczyk, L Adkins, J K Arkhipkin, D Aschenauer, E C Banerjee, A Bellwied, R Bielcikova, J Bland, L C Brandin, A V Brovko, S G Bunzarov, I Caines, H Cendejas, R Chang, Z Chwastowski, J Cramer, J G Crawford, H J Debbe, R R Ding, F Dong, X Du, C M Dunlop, J C Engle, K S Fatemi, R Filip, P Finch, E Gagliardi, C A Guryn, W Hajkova, O L-X Han Hirsch, A Horvat, S Humanic, T J Kauder, K Ke, H W Keane, D Kechechyan, A Kikola, D P Koetke, D D Kravtsov, P Landgraf, J M Lauret, J Leight, W X Li Lima, L M Ljubicic, T Ma, G L Ma, Y G Majka, R Margetis, S McDonald, D Mustafa, M K Nurushev, S B K Oh Ohlson, A Okorokov, V Pal, S K Pawlik, B Perkins, C Planinic, M Porter, J Przybycien, M Qiu, H Raniwala, S Ray, R L Ruan, L Sakrejda, I Sangaline, E Schambach, J Schmah, A M Schmidke, W B Singaraju, R N Skoby, M J Sorensen, P Sun, Y Sun, Z Szanto de Toledo, A Takahashi, J Tang, Z Tokarev, M Trentalange, S Tribble, R E Trzeciak, B A Tsai, O D Turnau, J Jr Varma, R Videbæk, F Vossen, A Walker, M Wang, H Webb, J C Witt, R Yang, Y Yepes, P L Yi Zhang, S Zhao, F Zhao, J Zhu, X |
description | We report the beam energy (\sqrt s_{NN} = 7.7 - 200 GeV) and collision centrality dependence of the mean (M), standard deviation (\sigma), skewness (S), and kurtosis (\kappa) of the net-proton multiplicity distributions in Au+Au collisions. The measurements are carried out by the STAR experiment at midrapidity (|y| < 0.5) and within the transverse momentum range 0.4 < pT < 0.8 GeV/c in the first phase of the Beam Energy Scan program at the Relativistic Heavy Ion Collider. These measurements are important for understanding the Quantum Chromodynamic (QCD) phase diagram. The products of the moments, S\sigma and \kappa\sigma^{2}, are sensitive to the correlation length of the hot and dense medium created in the collisions and are related to the ratios of baryon number susceptibilities of corresponding orders. The products of moments are found to have values significantly below the Skellam expectation and close to expectations based on independent proton and anti-proton production. The measurements are compared to a transport model calculation to understand the effect of acceptance and baryon number conservation, and also to a hadron resonance gas model. |
doi_str_mv | 10.48550/arxiv.1309.5681 |
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The measurements are carried out by the STAR experiment at midrapidity (|y| < 0.5) and within the transverse momentum range 0.4 < pT < 0.8 GeV/c in the first phase of the Beam Energy Scan program at the Relativistic Heavy Ion Collider. These measurements are important for understanding the Quantum Chromodynamic (QCD) phase diagram. The products of the moments, S\sigma and \kappa\sigma^{2}, are sensitive to the correlation length of the hot and dense medium created in the collisions and are related to the ratios of baryon number susceptibilities of corresponding orders. The products of moments are found to have values significantly below the Skellam expectation and close to expectations based on independent proton and anti-proton production. The measurements are compared to a transport model calculation to understand the effect of acceptance and baryon number conservation, and also to a hadron resonance gas model.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1309.5681</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Antiparticles ; Antiprotons ; Baryons ; Collisions ; Dependence ; Heavy ions ; Kurtosis ; Phase diagrams ; Protons ; Quantum chromodynamics ; Quarks ; Relativistic Heavy Ion Collider ; Transverse momentum</subject><ispartof>arXiv.org, 2013-09</ispartof><rights>2013. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). 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A</creatorcontrib><creatorcontrib>Okorokov, V</creatorcontrib><creatorcontrib>Pal, S K</creatorcontrib><creatorcontrib>Pawlik, B</creatorcontrib><creatorcontrib>Perkins, C</creatorcontrib><creatorcontrib>Planinic, M</creatorcontrib><creatorcontrib>Porter, J</creatorcontrib><creatorcontrib>Przybycien, M</creatorcontrib><creatorcontrib>Qiu, H</creatorcontrib><creatorcontrib>Raniwala, S</creatorcontrib><creatorcontrib>Ray, R L</creatorcontrib><creatorcontrib>Ruan, L</creatorcontrib><creatorcontrib>Sakrejda, I</creatorcontrib><creatorcontrib>Sangaline, E</creatorcontrib><creatorcontrib>Schambach, J</creatorcontrib><creatorcontrib>Schmah, A M</creatorcontrib><creatorcontrib>Schmidke, W B</creatorcontrib><creatorcontrib>Singaraju, R N</creatorcontrib><creatorcontrib>Skoby, M J</creatorcontrib><creatorcontrib>Sorensen, P</creatorcontrib><creatorcontrib>Sun, Y</creatorcontrib><creatorcontrib>Sun, Z</creatorcontrib><creatorcontrib>Szanto de Toledo, A</creatorcontrib><creatorcontrib>Takahashi, J</creatorcontrib><creatorcontrib>Tang, Z</creatorcontrib><creatorcontrib>Tokarev, M</creatorcontrib><creatorcontrib>Trentalange, S</creatorcontrib><creatorcontrib>Tribble, R E</creatorcontrib><creatorcontrib>Trzeciak, B A</creatorcontrib><creatorcontrib>Tsai, O D</creatorcontrib><creatorcontrib>Turnau, J</creatorcontrib><creatorcontrib>Jr</creatorcontrib><creatorcontrib>Varma, R</creatorcontrib><creatorcontrib>Videbæk, F</creatorcontrib><creatorcontrib>Vossen, A</creatorcontrib><creatorcontrib>Walker, M</creatorcontrib><creatorcontrib>Wang, H</creatorcontrib><creatorcontrib>Webb, J C</creatorcontrib><creatorcontrib>Witt, R</creatorcontrib><creatorcontrib>Yang, Y</creatorcontrib><creatorcontrib>Yepes, P</creatorcontrib><creatorcontrib>L Yi</creatorcontrib><creatorcontrib>Zhang, S</creatorcontrib><creatorcontrib>Zhao, F</creatorcontrib><creatorcontrib>Zhao, J</creatorcontrib><creatorcontrib>Zhu, X</creatorcontrib><title>Energy Dependence of Moments of Net-proton Multiplicity Distributions at RHIC</title><title>arXiv.org</title><description>We report the beam energy (\sqrt s_{NN} = 7.7 - 200 GeV) and collision centrality dependence of the mean (M), standard deviation (\sigma), skewness (S), and kurtosis (\kappa) of the net-proton multiplicity distributions in Au+Au collisions. The measurements are carried out by the STAR experiment at midrapidity (|y| < 0.5) and within the transverse momentum range 0.4 < pT < 0.8 GeV/c in the first phase of the Beam Energy Scan program at the Relativistic Heavy Ion Collider. These measurements are important for understanding the Quantum Chromodynamic (QCD) phase diagram. The products of the moments, S\sigma and \kappa\sigma^{2}, are sensitive to the correlation length of the hot and dense medium created in the collisions and are related to the ratios of baryon number susceptibilities of corresponding orders. The products of moments are found to have values significantly below the Skellam expectation and close to expectations based on independent proton and anti-proton production. The measurements are compared to a transport model calculation to understand the effect of acceptance and baryon number conservation, and also to a hadron resonance gas model.</description><subject>Antiparticles</subject><subject>Antiprotons</subject><subject>Baryons</subject><subject>Collisions</subject><subject>Dependence</subject><subject>Heavy ions</subject><subject>Kurtosis</subject><subject>Phase diagrams</subject><subject>Protons</subject><subject>Quantum chromodynamics</subject><subject>Quarks</subject><subject>Relativistic Heavy Ion Collider</subject><subject>Transverse momentum</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNotjsFLwzAYxYMgOObuHgOeW5PvS9r0KHW6waogu48kzSSjJrNJRf97K3p6Dx6_9x4hN5yVQknJ7vT45T9LjqwpZaX4BVkAIi-UALgiq5ROjDGoapASF6RbBze-fdMHd3ahd8E6Go-0i-8u5PRrn10uzmPMMdBuGrI_D976PAM-5dGbKfsYEtWZvm627TW5POohudW_Lsn-cb1vN8Xu5Wnb3u8KLTkW2DQ9gjJWCIVVXWtuhEFojAPWKDmnYKUwztZMWS6VxMohB2X7HjQ0HJfk9q92PvYxuZQPpziNYV48AFOCi0pIxB9I6k38</recordid><startdate>20130923</startdate><enddate>20130923</enddate><creator>Adamczyk, L</creator><creator>Adkins, J K</creator><creator>Arkhipkin, D</creator><creator>Aschenauer, E C</creator><creator>Banerjee, A</creator><creator>Bellwied, R</creator><creator>Bielcikova, J</creator><creator>Bland, L C</creator><creator>Brandin, A V</creator><creator>Brovko, S G</creator><creator>Bunzarov, I</creator><creator>Caines, H</creator><creator>Cendejas, R</creator><creator>Chang, 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Multiplicity Distributions at RHIC</title><author>Adamczyk, L ; Adkins, J K ; Arkhipkin, D ; Aschenauer, E C ; Banerjee, A ; Bellwied, R ; Bielcikova, J ; Bland, L C ; Brandin, A V ; Brovko, S G ; Bunzarov, I ; Caines, H ; Cendejas, R ; Chang, Z ; Chwastowski, J ; Cramer, J G ; Crawford, H J ; Debbe, R R ; Ding, F ; Dong, X ; Du, C M ; Dunlop, J C ; Engle, K S ; Fatemi, R ; Filip, P ; Finch, E ; Gagliardi, C A ; Guryn, W ; Hajkova, O ; L-X Han ; Hirsch, A ; Horvat, S ; Humanic, T J ; Kauder, K ; Ke, H W ; Keane, D ; Kechechyan, A ; Kikola, D P ; Koetke, D D ; Kravtsov, P ; Landgraf, J M ; Lauret, J ; Leight, W ; X Li ; Lima, L M ; Ljubicic, T ; Ma, G L ; Ma, Y G ; Majka, R ; Margetis, S ; McDonald, D ; Mustafa, M K ; Nurushev, S B ; K Oh ; Ohlson, A ; Okorokov, V ; Pal, S K ; Pawlik, B ; Perkins, C ; Planinic, M ; Porter, J ; Przybycien, M ; Qiu, H ; Raniwala, S ; Ray, R L ; Ruan, L ; Sakrejda, I ; Sangaline, E ; Schambach, J ; Schmah, A M ; Schmidke, W B ; Singaraju, R N ; Skoby, M J ; Sorensen, P ; Sun, Y ; Sun, Z ; Szanto de Toledo, A ; Takahashi, J ; Tang, Z ; Tokarev, M ; Trentalange, S ; Tribble, R E ; Trzeciak, B A ; Tsai, O D ; Turnau, J ; Jr ; Varma, R ; Videbæk, F ; Vossen, A ; Walker, M ; Wang, H ; Webb, J C ; Witt, R ; Yang, Y ; Yepes, P ; L Yi ; Zhang, S ; Zhao, F ; Zhao, J ; Zhu, X</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a513-399d328bc4483677a1b4b329be2098599d2c54bec708c158536e3128cdd2a2913</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Antiparticles</topic><topic>Antiprotons</topic><topic>Baryons</topic><topic>Collisions</topic><topic>Dependence</topic><topic>Heavy ions</topic><topic>Kurtosis</topic><topic>Phase diagrams</topic><topic>Protons</topic><topic>Quantum chromodynamics</topic><topic>Quarks</topic><topic>Relativistic Heavy Ion Collider</topic><topic>Transverse 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C</creatorcontrib><creatorcontrib>Engle, K S</creatorcontrib><creatorcontrib>Fatemi, R</creatorcontrib><creatorcontrib>Filip, P</creatorcontrib><creatorcontrib>Finch, E</creatorcontrib><creatorcontrib>Gagliardi, C A</creatorcontrib><creatorcontrib>Guryn, W</creatorcontrib><creatorcontrib>Hajkova, O</creatorcontrib><creatorcontrib>L-X Han</creatorcontrib><creatorcontrib>Hirsch, A</creatorcontrib><creatorcontrib>Horvat, S</creatorcontrib><creatorcontrib>Humanic, T J</creatorcontrib><creatorcontrib>Kauder, K</creatorcontrib><creatorcontrib>Ke, H W</creatorcontrib><creatorcontrib>Keane, D</creatorcontrib><creatorcontrib>Kechechyan, A</creatorcontrib><creatorcontrib>Kikola, D P</creatorcontrib><creatorcontrib>Koetke, D D</creatorcontrib><creatorcontrib>Kravtsov, P</creatorcontrib><creatorcontrib>Landgraf, J M</creatorcontrib><creatorcontrib>Lauret, J</creatorcontrib><creatorcontrib>Leight, W</creatorcontrib><creatorcontrib>X Li</creatorcontrib><creatorcontrib>Lima, L M</creatorcontrib><creatorcontrib>Ljubicic, T</creatorcontrib><creatorcontrib>Ma, G L</creatorcontrib><creatorcontrib>Ma, Y G</creatorcontrib><creatorcontrib>Majka, R</creatorcontrib><creatorcontrib>Margetis, S</creatorcontrib><creatorcontrib>McDonald, D</creatorcontrib><creatorcontrib>Mustafa, M K</creatorcontrib><creatorcontrib>Nurushev, S B</creatorcontrib><creatorcontrib>K Oh</creatorcontrib><creatorcontrib>Ohlson, A</creatorcontrib><creatorcontrib>Okorokov, V</creatorcontrib><creatorcontrib>Pal, S K</creatorcontrib><creatorcontrib>Pawlik, B</creatorcontrib><creatorcontrib>Perkins, C</creatorcontrib><creatorcontrib>Planinic, M</creatorcontrib><creatorcontrib>Porter, J</creatorcontrib><creatorcontrib>Przybycien, M</creatorcontrib><creatorcontrib>Qiu, H</creatorcontrib><creatorcontrib>Raniwala, S</creatorcontrib><creatorcontrib>Ray, R L</creatorcontrib><creatorcontrib>Ruan, L</creatorcontrib><creatorcontrib>Sakrejda, I</creatorcontrib><creatorcontrib>Sangaline, E</creatorcontrib><creatorcontrib>Schambach, J</creatorcontrib><creatorcontrib>Schmah, A M</creatorcontrib><creatorcontrib>Schmidke, W B</creatorcontrib><creatorcontrib>Singaraju, R N</creatorcontrib><creatorcontrib>Skoby, M J</creatorcontrib><creatorcontrib>Sorensen, P</creatorcontrib><creatorcontrib>Sun, Y</creatorcontrib><creatorcontrib>Sun, Z</creatorcontrib><creatorcontrib>Szanto de Toledo, A</creatorcontrib><creatorcontrib>Takahashi, J</creatorcontrib><creatorcontrib>Tang, Z</creatorcontrib><creatorcontrib>Tokarev, M</creatorcontrib><creatorcontrib>Trentalange, S</creatorcontrib><creatorcontrib>Tribble, R E</creatorcontrib><creatorcontrib>Trzeciak, B A</creatorcontrib><creatorcontrib>Tsai, O D</creatorcontrib><creatorcontrib>Turnau, J</creatorcontrib><creatorcontrib>Jr</creatorcontrib><creatorcontrib>Varma, R</creatorcontrib><creatorcontrib>Videbæk, F</creatorcontrib><creatorcontrib>Vossen, A</creatorcontrib><creatorcontrib>Walker, M</creatorcontrib><creatorcontrib>Wang, H</creatorcontrib><creatorcontrib>Webb, J C</creatorcontrib><creatorcontrib>Witt, R</creatorcontrib><creatorcontrib>Yang, Y</creatorcontrib><creatorcontrib>Yepes, P</creatorcontrib><creatorcontrib>L Yi</creatorcontrib><creatorcontrib>Zhang, S</creatorcontrib><creatorcontrib>Zhao, F</creatorcontrib><creatorcontrib>Zhao, J</creatorcontrib><creatorcontrib>Zhu, X</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Adamczyk, L</au><au>Adkins, J K</au><au>Arkhipkin, D</au><au>Aschenauer, E C</au><au>Banerjee, A</au><au>Bellwied, R</au><au>Bielcikova, J</au><au>Bland, L C</au><au>Brandin, A V</au><au>Brovko, S G</au><au>Bunzarov, I</au><au>Caines, H</au><au>Cendejas, R</au><au>Chang, Z</au><au>Chwastowski, J</au><au>Cramer, J G</au><au>Crawford, H J</au><au>Debbe, R R</au><au>Ding, F</au><au>Dong, X</au><au>Du, C M</au><au>Dunlop, J C</au><au>Engle, K S</au><au>Fatemi, R</au><au>Filip, P</au><au>Finch, E</au><au>Gagliardi, C A</au><au>Guryn, W</au><au>Hajkova, O</au><au>L-X Han</au><au>Hirsch, A</au><au>Horvat, S</au><au>Humanic, T J</au><au>Kauder, K</au><au>Ke, H W</au><au>Keane, D</au><au>Kechechyan, A</au><au>Kikola, D P</au><au>Koetke, D D</au><au>Kravtsov, P</au><au>Landgraf, J M</au><au>Lauret, J</au><au>Leight, W</au><au>X Li</au><au>Lima, L M</au><au>Ljubicic, T</au><au>Ma, G L</au><au>Ma, Y G</au><au>Majka, R</au><au>Margetis, S</au><au>McDonald, D</au><au>Mustafa, M K</au><au>Nurushev, S B</au><au>K Oh</au><au>Ohlson, A</au><au>Okorokov, V</au><au>Pal, S K</au><au>Pawlik, B</au><au>Perkins, C</au><au>Planinic, M</au><au>Porter, J</au><au>Przybycien, M</au><au>Qiu, H</au><au>Raniwala, S</au><au>Ray, R L</au><au>Ruan, L</au><au>Sakrejda, I</au><au>Sangaline, E</au><au>Schambach, J</au><au>Schmah, A M</au><au>Schmidke, W B</au><au>Singaraju, R N</au><au>Skoby, M J</au><au>Sorensen, P</au><au>Sun, Y</au><au>Sun, Z</au><au>Szanto de Toledo, A</au><au>Takahashi, J</au><au>Tang, Z</au><au>Tokarev, M</au><au>Trentalange, S</au><au>Tribble, R E</au><au>Trzeciak, B A</au><au>Tsai, O D</au><au>Turnau, J</au><au>Jr</au><au>Varma, R</au><au>Videbæk, F</au><au>Vossen, A</au><au>Walker, M</au><au>Wang, H</au><au>Webb, J C</au><au>Witt, R</au><au>Yang, Y</au><au>Yepes, P</au><au>L Yi</au><au>Zhang, S</au><au>Zhao, F</au><au>Zhao, J</au><au>Zhu, X</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Energy Dependence of Moments of Net-proton Multiplicity Distributions at RHIC</atitle><jtitle>arXiv.org</jtitle><date>2013-09-23</date><risdate>2013</risdate><eissn>2331-8422</eissn><abstract>We report the beam energy (\sqrt s_{NN} = 7.7 - 200 GeV) and collision centrality dependence of the mean (M), standard deviation (\sigma), skewness (S), and kurtosis (\kappa) of the net-proton multiplicity distributions in Au+Au collisions. The measurements are carried out by the STAR experiment at midrapidity (|y| < 0.5) and within the transverse momentum range 0.4 < pT < 0.8 GeV/c in the first phase of the Beam Energy Scan program at the Relativistic Heavy Ion Collider. These measurements are important for understanding the Quantum Chromodynamic (QCD) phase diagram. The products of the moments, S\sigma and \kappa\sigma^{2}, are sensitive to the correlation length of the hot and dense medium created in the collisions and are related to the ratios of baryon number susceptibilities of corresponding orders. The products of moments are found to have values significantly below the Skellam expectation and close to expectations based on independent proton and anti-proton production. The measurements are compared to a transport model calculation to understand the effect of acceptance and baryon number conservation, and also to a hadron resonance gas model.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1309.5681</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2013-09 |
issn | 2331-8422 |
language | eng |
recordid | cdi_proquest_journals_2084146453 |
source | Publicly Available Content Database |
subjects | Antiparticles Antiprotons Baryons Collisions Dependence Heavy ions Kurtosis Phase diagrams Protons Quantum chromodynamics Quarks Relativistic Heavy Ion Collider Transverse momentum |
title | Energy Dependence of Moments of Net-proton Multiplicity Distributions at RHIC |
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