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Azimuthal anisotropy of K(0)(S) and Lambda+Lambda production at midrapidity from Au+Au collisions at sqrt[s(NN)]=130 GeV
We report STAR results on the azimuthal anisotropy parameter v(2) for strange particles K(0)(S), Lambda, and Lambda at midrapidity in Au+Au collisions at sqrt[s(NN)]=130 GeV at the Relativistic Heavy Ion Collider. The value of v(2) as a function of transverse momentum, p(t), of the produced particle...
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Published in: | Physical review letters 2002-09, Vol.89 (13), p.132301-132301 |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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creator | Adler, C Ahammed, Z Allgower, C Amonett, J Anderson, B D Anderson, M Averichev, G S Balewski, J Barannikova, O Barnby, L S Baudot, J Bekele, S Belaga, V V Bellwied, R Berger, J Bichsel, H Billmeier, A Bland, L C Blyth, C O Bonner, B E Boucham, A Brandin, A Bravar, A Cadman, R V Caines, H Calderón de la Barca Sánchez, M Cardenas, A Carroll, J Castillo, J Castro, M Cebra, D Chaloupka, P Chattopadhyay, S Chen, Y Chernenko, S P Cherney, M Chikanian, A Choi, B Christie, W Coffin, J P Cormier, T M Cramer, J G Crawford, H J Deng, W S Derevschikov, A A Didenko, L Dietel, T Draper, J E Dunin, V B Dunlop, J C Eckardt, V Efimov, L G Emelianov, V Engelage, J Eppley, G Erazmus, B Fachini, P Faine, V Filimonov, K Finch, E Fisyak, Y Flierl, D Foley, K J Fu, J Gagliardi, C A Gagunashvili, N Gans, J Gaudichet, L Germain, M Geurts, F Ghazikhanian, V Grachov, O Grigoriev, V Guedon, M Gushin, E Hallman, T J Hardtke, D Harris, J W Henry, T W Heppelmann, S Herston, T Hippolyte, B Hirsch, A Hjort, E Hoffmann, G W Horsley, M Huang, H Z Humanic, T J Igo, G Ishihara, A Ivanshin, Yu I Jacobs, P Jacobs, W W Janik, M Johnson, I Jones, P G Judd, E G Kaneta, M Kaplan, M Keane, D |
description | We report STAR results on the azimuthal anisotropy parameter v(2) for strange particles K(0)(S), Lambda, and Lambda at midrapidity in Au+Au collisions at sqrt[s(NN)]=130 GeV at the Relativistic Heavy Ion Collider. The value of v(2) as a function of transverse momentum, p(t), of the produced particle and collision centrality is presented for both particles up to p(t) approximately 3.0 GeV/c. A strong p(t) dependence in v(2) is observed up to 2.0 GeV/c. The v(2) measurement is compared with hydrodynamic model calculations. The physics implications of the p(t) integrated v(2) magnitude as a function of particle mass are also discussed. |
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The value of v(2) as a function of transverse momentum, p(t), of the produced particle and collision centrality is presented for both particles up to p(t) approximately 3.0 GeV/c. A strong p(t) dependence in v(2) is observed up to 2.0 GeV/c. The v(2) measurement is compared with hydrodynamic model calculations. The physics implications of the p(t) integrated v(2) magnitude as a function of particle mass are also discussed.</description><identifier>ISSN: 0031-9007</identifier><identifier>PMID: 12225018</identifier><language>eng</language><publisher>United States</publisher><ispartof>Physical review letters, 2002-09, Vol.89 (13), p.132301-132301</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/12225018$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Adler, C</creatorcontrib><creatorcontrib>Ahammed, Z</creatorcontrib><creatorcontrib>Allgower, C</creatorcontrib><creatorcontrib>Amonett, J</creatorcontrib><creatorcontrib>Anderson, B 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O</creatorcontrib><creatorcontrib>Grigoriev, V</creatorcontrib><creatorcontrib>Guedon, M</creatorcontrib><creatorcontrib>Gushin, E</creatorcontrib><creatorcontrib>Hallman, T J</creatorcontrib><creatorcontrib>Hardtke, D</creatorcontrib><creatorcontrib>Harris, J W</creatorcontrib><creatorcontrib>Henry, T W</creatorcontrib><creatorcontrib>Heppelmann, S</creatorcontrib><creatorcontrib>Herston, T</creatorcontrib><creatorcontrib>Hippolyte, B</creatorcontrib><creatorcontrib>Hirsch, A</creatorcontrib><creatorcontrib>Hjort, E</creatorcontrib><creatorcontrib>Hoffmann, G W</creatorcontrib><creatorcontrib>Horsley, M</creatorcontrib><creatorcontrib>Huang, H Z</creatorcontrib><creatorcontrib>Humanic, T J</creatorcontrib><creatorcontrib>Igo, G</creatorcontrib><creatorcontrib>Ishihara, A</creatorcontrib><creatorcontrib>Ivanshin, Yu I</creatorcontrib><creatorcontrib>Jacobs, P</creatorcontrib><creatorcontrib>Jacobs, W W</creatorcontrib><creatorcontrib>Janik, M</creatorcontrib><creatorcontrib>Johnson, 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The value of v(2) as a function of transverse momentum, p(t), of the produced particle and collision centrality is presented for both particles up to p(t) approximately 3.0 GeV/c. A strong p(t) dependence in v(2) is observed up to 2.0 GeV/c. The v(2) measurement is compared with hydrodynamic model calculations. The physics implications of the p(t) integrated v(2) magnitude as a function of particle mass are also discussed.</description><issn>0031-9007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2002</creationdate><recordtype>article</recordtype><recordid>eNo10E9LwzAYBvAeFDenX0Fyko1ReJO2aXPwUIZOccyDw4tISZsEI-3S5Q9YP72VzdMDDz9eXp6zaAqQ4JgB5JPo0rkvAMCEFhfRBBNCMsDFNPouf3QX_CdvEd9rZ7w1_YCMQs9zWMxfF2Mr0IZ3teDLY6DeGhEar80ecY86LSzvtdB-QMqaDpVhWQbUmLbVbjTuD7mD9e9uvt0uPu5wAmgt366ic8VbJ69POYt2D_e71WO8eVk_rcpN3GdpEaeYNxnFgGvMC8pSmTcFBZWngtWJqhmnTCmRUUIaSFkuSC2JoGrkVApMsmQW3R7Pjl8fgnS-6rRrZNvyvTTBVTmBggBmI7w5wVB3UlS91R23Q_U_VfIL8gNi1Q</recordid><startdate>20020923</startdate><enddate>20020923</enddate><creator>Adler, C</creator><creator>Ahammed, Z</creator><creator>Allgower, C</creator><creator>Amonett, J</creator><creator>Anderson, B D</creator><creator>Anderson, M</creator><creator>Averichev, G S</creator><creator>Balewski, J</creator><creator>Barannikova, 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V</creatorcontrib><creatorcontrib>Efimov, L G</creatorcontrib><creatorcontrib>Emelianov, V</creatorcontrib><creatorcontrib>Engelage, J</creatorcontrib><creatorcontrib>Eppley, G</creatorcontrib><creatorcontrib>Erazmus, B</creatorcontrib><creatorcontrib>Fachini, P</creatorcontrib><creatorcontrib>Faine, V</creatorcontrib><creatorcontrib>Filimonov, K</creatorcontrib><creatorcontrib>Finch, E</creatorcontrib><creatorcontrib>Fisyak, Y</creatorcontrib><creatorcontrib>Flierl, D</creatorcontrib><creatorcontrib>Foley, K J</creatorcontrib><creatorcontrib>Fu, J</creatorcontrib><creatorcontrib>Gagliardi, C A</creatorcontrib><creatorcontrib>Gagunashvili, N</creatorcontrib><creatorcontrib>Gans, J</creatorcontrib><creatorcontrib>Gaudichet, L</creatorcontrib><creatorcontrib>Germain, M</creatorcontrib><creatorcontrib>Geurts, F</creatorcontrib><creatorcontrib>Ghazikhanian, V</creatorcontrib><creatorcontrib>Grachov, O</creatorcontrib><creatorcontrib>Grigoriev, V</creatorcontrib><creatorcontrib>Guedon, M</creatorcontrib><creatorcontrib>Gushin, E</creatorcontrib><creatorcontrib>Hallman, T J</creatorcontrib><creatorcontrib>Hardtke, D</creatorcontrib><creatorcontrib>Harris, J W</creatorcontrib><creatorcontrib>Henry, T W</creatorcontrib><creatorcontrib>Heppelmann, S</creatorcontrib><creatorcontrib>Herston, T</creatorcontrib><creatorcontrib>Hippolyte, B</creatorcontrib><creatorcontrib>Hirsch, A</creatorcontrib><creatorcontrib>Hjort, E</creatorcontrib><creatorcontrib>Hoffmann, G W</creatorcontrib><creatorcontrib>Horsley, M</creatorcontrib><creatorcontrib>Huang, H Z</creatorcontrib><creatorcontrib>Humanic, T J</creatorcontrib><creatorcontrib>Igo, G</creatorcontrib><creatorcontrib>Ishihara, A</creatorcontrib><creatorcontrib>Ivanshin, Yu I</creatorcontrib><creatorcontrib>Jacobs, P</creatorcontrib><creatorcontrib>Jacobs, W W</creatorcontrib><creatorcontrib>Janik, M</creatorcontrib><creatorcontrib>Johnson, I</creatorcontrib><creatorcontrib>Jones, P G</creatorcontrib><creatorcontrib>Judd, E G</creatorcontrib><creatorcontrib>Kaneta, M</creatorcontrib><creatorcontrib>Kaplan, M</creatorcontrib><creatorcontrib>Keane, D</creatorcontrib><creatorcontrib>STAR Collaboration</creatorcontrib><collection>PubMed</collection><collection>MEDLINE - Academic</collection><jtitle>Physical review letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Adler, C</au><au>Ahammed, Z</au><au>Allgower, C</au><au>Amonett, J</au><au>Anderson, B D</au><au>Anderson, M</au><au>Averichev, G S</au><au>Balewski, J</au><au>Barannikova, O</au><au>Barnby, L S</au><au>Baudot, J</au><au>Bekele, S</au><au>Belaga, V V</au><au>Bellwied, R</au><au>Berger, J</au><au>Bichsel, H</au><au>Billmeier, A</au><au>Bland, L C</au><au>Blyth, C O</au><au>Bonner, B E</au><au>Boucham, A</au><au>Brandin, A</au><au>Bravar, A</au><au>Cadman, R V</au><au>Caines, H</au><au>Calderón de la Barca Sánchez, M</au><au>Cardenas, A</au><au>Carroll, J</au><au>Castillo, J</au><au>Castro, M</au><au>Cebra, D</au><au>Chaloupka, P</au><au>Chattopadhyay, S</au><au>Chen, Y</au><au>Chernenko, S P</au><au>Cherney, M</au><au>Chikanian, A</au><au>Choi, B</au><au>Christie, W</au><au>Coffin, J P</au><au>Cormier, T M</au><au>Cramer, J G</au><au>Crawford, H J</au><au>Deng, W S</au><au>Derevschikov, A A</au><au>Didenko, L</au><au>Dietel, T</au><au>Draper, J E</au><au>Dunin, V B</au><au>Dunlop, J C</au><au>Eckardt, V</au><au>Efimov, L G</au><au>Emelianov, V</au><au>Engelage, J</au><au>Eppley, G</au><au>Erazmus, B</au><au>Fachini, P</au><au>Faine, V</au><au>Filimonov, K</au><au>Finch, E</au><au>Fisyak, Y</au><au>Flierl, D</au><au>Foley, K J</au><au>Fu, J</au><au>Gagliardi, C A</au><au>Gagunashvili, N</au><au>Gans, J</au><au>Gaudichet, L</au><au>Germain, M</au><au>Geurts, F</au><au>Ghazikhanian, V</au><au>Grachov, O</au><au>Grigoriev, V</au><au>Guedon, M</au><au>Gushin, E</au><au>Hallman, T J</au><au>Hardtke, D</au><au>Harris, J W</au><au>Henry, T W</au><au>Heppelmann, S</au><au>Herston, T</au><au>Hippolyte, B</au><au>Hirsch, A</au><au>Hjort, E</au><au>Hoffmann, G W</au><au>Horsley, M</au><au>Huang, H Z</au><au>Humanic, T J</au><au>Igo, G</au><au>Ishihara, A</au><au>Ivanshin, Yu I</au><au>Jacobs, P</au><au>Jacobs, W W</au><au>Janik, M</au><au>Johnson, I</au><au>Jones, P G</au><au>Judd, E G</au><au>Kaneta, M</au><au>Kaplan, M</au><au>Keane, D</au><aucorp>STAR Collaboration</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Azimuthal anisotropy of K(0)(S) and Lambda+Lambda production at midrapidity from Au+Au collisions at sqrt[s(NN)]=130 GeV</atitle><jtitle>Physical review letters</jtitle><addtitle>Phys Rev Lett</addtitle><date>2002-09-23</date><risdate>2002</risdate><volume>89</volume><issue>13</issue><spage>132301</spage><epage>132301</epage><pages>132301-132301</pages><issn>0031-9007</issn><abstract>We report STAR results on the azimuthal anisotropy parameter v(2) for strange particles K(0)(S), Lambda, and Lambda at midrapidity in Au+Au collisions at sqrt[s(NN)]=130 GeV at the Relativistic Heavy Ion Collider. The value of v(2) as a function of transverse momentum, p(t), of the produced particle and collision centrality is presented for both particles up to p(t) approximately 3.0 GeV/c. A strong p(t) dependence in v(2) is observed up to 2.0 GeV/c. The v(2) measurement is compared with hydrodynamic model calculations. The physics implications of the p(t) integrated v(2) magnitude as a function of particle mass are also discussed.</abstract><cop>United States</cop><pmid>12225018</pmid><tpages>1</tpages></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0031-9007 |
ispartof | Physical review letters, 2002-09, Vol.89 (13), p.132301-132301 |
issn | 0031-9007 |
language | eng |
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source | American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list) |
title | Azimuthal anisotropy of K(0)(S) and Lambda+Lambda production at midrapidity from Au+Au collisions at sqrt[s(NN)]=130 GeV |
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