Azimuthal anisotropy at the relativistic heavy ion collider: the first and fourth harmonics
We report the first observations of the first harmonic (directed flow, v(1)) and the fourth harmonic (v(4)), in the azimuthal distribution of particles with respect to the reaction plane in Au+Au collisions at the BNL Relativistic Heavy Ion Collider (RHIC). Both measurements were done taking advanta...
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creator | Adams, J Adler, C Aggarwal, M M Ahammed, Z Amonett, J Anderson, B D Anderson, M Arkhipkin, D Averichev, G S Badyal, S K Balewski, J Barannikova, O Barnby, L S Baudot, J Bekele, S Belaga, V V Bellwied, R Berger, J Bezverkhny, B I Bhardwaj, S Bhaskar, P Bhati, A K Bichsel, H Billmeier, A Bland, L C Blyth, C O Bonner, B E Botje, M Boucham, A Brandin, A Bravar, A Cadman, R V Cai, X Z Caines, H Calderón de la Barca Sánchez, M Carroll, J Castillo, J Castro, M Cebra, D Chaloupka, P Chattopadhyay, S Chen, H F 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 Das, D Das, S Derevschikov, A A Didenko, L Dietel, T Dong, W J Dong, X Draper, J E Du, F Dubey, A K Dunin, V B Dunlop, J C Dutta Majumdar, M R Eckardt, V Efimov, L G Emelianov, V Engelage, J Eppley, G Erazmus, B Estienne, M Fachini, P Faine, V Faivre, J Fatemi, R Filimonov, K Filip, P Finch, E Fisyak, Y Flierl, D Foley, K J Fu, J Gagliardi, C A Gagunashvili, N Gans, J Ganti, M S Gaudichet, L Germain, M Geurts, F Ghazikhanian, V Ghosh, P Gonzalez, J E Grachov, O Grigoriev, V Gronstal, S Grosnick, D Guedon, M Guertin, S M Gupta, A |
description | We report the first observations of the first harmonic (directed flow, v(1)) and the fourth harmonic (v(4)), in the azimuthal distribution of particles with respect to the reaction plane in Au+Au collisions at the BNL Relativistic Heavy Ion Collider (RHIC). Both measurements were done taking advantage of the large elliptic flow (v(2)) generated at RHIC. From the correlation of v(2) with v(1) it is determined that v(2) is positive, or in-plane. The integrated v(4) is about a factor of 10 smaller than v(2). For the sixth (v(6)) and eighth (v(8)) harmonics upper limits on the magnitudes are reported. |
doi_str_mv | 10.1103/physrevlett.92.062301 |
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Both measurements were done taking advantage of the large elliptic flow (v(2)) generated at RHIC. From the correlation of v(2) with v(1) it is determined that v(2) is positive, or in-plane. The integrated v(4) is about a factor of 10 smaller than v(2). For the sixth (v(6)) and eighth (v(8)) harmonics upper limits on the magnitudes are reported.</description><identifier>ISSN: 0031-9007</identifier><identifier>EISSN: 1079-7114</identifier><identifier>DOI: 10.1103/physrevlett.92.062301</identifier><identifier>PMID: 14995231</identifier><language>eng</language><publisher>United States: American Physical Society</publisher><subject>High Energy Physics - Phenomenology ; Physics</subject><ispartof>Physical review letters, 2004-02, Vol.92 (6), p.062301-062301, Article 062301</ispartof><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c454t-f25cc0af9ced4d34bac52ed3dc04a576425578efc31cf398ab024dc0557b2ae3</citedby><cites>FETCH-LOGICAL-c454t-f25cc0af9ced4d34bac52ed3dc04a576425578efc31cf398ab024dc0557b2ae3</cites><orcidid>0000-0001-7382-1609 ; 0000-0001-8890-1273 ; 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Collaboration</creatorcontrib><title>Azimuthal anisotropy at the relativistic heavy ion collider: the first and fourth harmonics</title><title>Physical review letters</title><addtitle>Phys Rev Lett</addtitle><description>We report the first observations of the first harmonic (directed flow, v(1)) and the fourth harmonic (v(4)), in the azimuthal distribution of particles with respect to the reaction plane in Au+Au collisions at the BNL Relativistic Heavy Ion Collider (RHIC). Both measurements were done taking advantage of the large elliptic flow (v(2)) generated at RHIC. From the correlation of v(2) with v(1) it is determined that v(2) is positive, or in-plane. The integrated v(4) is about a factor of 10 smaller than v(2). For the sixth (v(6)) and eighth (v(8)) harmonics upper limits on the magnitudes are reported.</description><subject>High Energy Physics - Phenomenology</subject><subject>Physics</subject><issn>0031-9007</issn><issn>1079-7114</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2004</creationdate><recordtype>article</recordtype><recordid>eNpFkVtLxDAQhYMoul5-gpInX6Tr5NJ249si3mBBEd98CNk0pZG2qUlaWH-90V30aWDmOzOcOQidE5gTAux6aDbBm6k1Mc4FnUNBGZA9NCNQiqwkhO-jGQAjmQAoj9BxCB8AQGixOERHhAuRU0Zm6H35ZbsxNqrFqrfBRe-GDVYRx8Zgb1oV7WRDtBo3Rk0bbF2PtWtbWxl_8wvV1oeYxBWu3ehjgxvlO9dbHU7RQa3aYM529QS93d-93T5mq-eHp9vlKtM85zGraa41qFpoU_GK8bXSOTUVqzRwlZcFp3leLkytGdE1Ewu1BsrTMHXXVBl2gq62a5MJOXjbKb-RTln5uFxJ29OByeSckgJgIom-3NKDd5-jCVF2NmjTtqo3bgyyJIWgQiwSmG9B7V1Ir67_dhOQPxHIlxTBq5lWKQIpqNxGkHQXuwPjujPVv2r3c_YNiHKG0Q</recordid><startdate>20040213</startdate><enddate>20040213</enddate><creator>Adams, J</creator><creator>Adler, C</creator><creator>Aggarwal, M M</creator><creator>Ahammed, Z</creator><creator>Amonett, J</creator><creator>Anderson, B D</creator><creator>Anderson, M</creator><creator>Arkhipkin, D</creator><creator>Averichev, G S</creator><creator>Badyal, S K</creator><creator>Balewski, J</creator><creator>Barannikova, O</creator><creator>Barnby, L S</creator><creator>Baudot, J</creator><creator>Bekele, S</creator><creator>Belaga, V V</creator><creator>Bellwied, R</creator><creator>Berger, J</creator><creator>Bezverkhny, B I</creator><creator>Bhardwaj, S</creator><creator>Bhaskar, P</creator><creator>Bhati, A K</creator><creator>Bichsel, H</creator><creator>Billmeier, A</creator><creator>Bland, L C</creator><creator>Blyth, C O</creator><creator>Bonner, B E</creator><creator>Botje, M</creator><creator>Boucham, A</creator><creator>Brandin, A</creator><creator>Bravar, A</creator><creator>Cadman, R V</creator><creator>Cai, X Z</creator><creator>Caines, H</creator><creator>Calderón de la Barca Sánchez, M</creator><creator>Carroll, J</creator><creator>Castillo, 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Society</general><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7X8</scope><scope>1XC</scope><orcidid>https://orcid.org/0000-0001-7382-1609</orcidid><orcidid>https://orcid.org/0000-0001-8890-1273</orcidid><orcidid>https://orcid.org/0000-0001-5920-6271</orcidid><orcidid>https://orcid.org/0000-0003-0687-5580</orcidid><orcidid>https://orcid.org/0000-0002-9781-2632</orcidid></search><sort><creationdate>20040213</creationdate><title>Azimuthal anisotropy at the relativistic heavy ion collider: the first and fourth harmonics</title><author>Adams, J ; Adler, C ; Aggarwal, M M ; Ahammed, Z ; Amonett, J ; Anderson, B D ; Anderson, M ; Arkhipkin, D ; Averichev, G S ; Badyal, S K ; Balewski, J ; Barannikova, O ; Barnby, L S ; Baudot, J ; Bekele, S ; Belaga, V V ; Bellwied, R ; Berger, J ; Bezverkhny, B I ; Bhardwaj, S ; Bhaskar, P ; Bhati, A K ; Bichsel, H ; Billmeier, A ; Bland, L C ; Blyth, C O ; Bonner, B E ; Botje, M ; Boucham, A ; Brandin, A ; Bravar, A ; Cadman, R V ; Cai, X Z ; Caines, H ; Calderón de la Barca Sánchez, M ; Carroll, J ; Castillo, J ; Castro, M ; Cebra, D ; Chaloupka, P ; Chattopadhyay, S ; Chen, H F ; 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 ; Das, D ; Das, S ; Derevschikov, A A ; Didenko, L ; Dietel, T ; Dong, W J ; Dong, X ; Draper, J E ; Du, F ; Dubey, A K ; Dunin, V B ; Dunlop, J C ; Dutta Majumdar, M R ; Eckardt, V ; Efimov, L G ; Emelianov, V ; Engelage, J ; Eppley, G ; Erazmus, B ; Estienne, M ; Fachini, P ; Faine, V ; Faivre, J ; Fatemi, R ; Filimonov, K ; Filip, P ; Finch, E ; Fisyak, Y ; Flierl, D ; Foley, K J ; Fu, J ; Gagliardi, C A ; Gagunashvili, N ; Gans, J ; Ganti, M S ; Gaudichet, L ; Germain, M ; Geurts, F ; Ghazikhanian, V ; Ghosh, P ; Gonzalez, J E ; Grachov, O ; Grigoriev, V ; Gronstal, S ; Grosnick, D ; Guedon, M ; Guertin, S M ; Gupta, A</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c454t-f25cc0af9ced4d34bac52ed3dc04a576425578efc31cf398ab024dc0557b2ae3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2004</creationdate><topic>High Energy Physics - Phenomenology</topic><topic>Physics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Adams, J</creatorcontrib><creatorcontrib>Adler, C</creatorcontrib><creatorcontrib>Aggarwal, M M</creatorcontrib><creatorcontrib>Ahammed, Z</creatorcontrib><creatorcontrib>Amonett, J</creatorcontrib><creatorcontrib>Anderson, B D</creatorcontrib><creatorcontrib>Anderson, M</creatorcontrib><creatorcontrib>Arkhipkin, D</creatorcontrib><creatorcontrib>Averichev, G S</creatorcontrib><creatorcontrib>Badyal, S K</creatorcontrib><creatorcontrib>Balewski, J</creatorcontrib><creatorcontrib>Barannikova, O</creatorcontrib><creatorcontrib>Barnby, L S</creatorcontrib><creatorcontrib>Baudot, J</creatorcontrib><creatorcontrib>Bekele, S</creatorcontrib><creatorcontrib>Belaga, V V</creatorcontrib><creatorcontrib>Bellwied, R</creatorcontrib><creatorcontrib>Berger, J</creatorcontrib><creatorcontrib>Bezverkhny, B I</creatorcontrib><creatorcontrib>Bhardwaj, S</creatorcontrib><creatorcontrib>Bhaskar, P</creatorcontrib><creatorcontrib>Bhati, A K</creatorcontrib><creatorcontrib>Bichsel, H</creatorcontrib><creatorcontrib>Billmeier, A</creatorcontrib><creatorcontrib>Bland, L C</creatorcontrib><creatorcontrib>Blyth, C O</creatorcontrib><creatorcontrib>Bonner, B E</creatorcontrib><creatorcontrib>Botje, M</creatorcontrib><creatorcontrib>Boucham, A</creatorcontrib><creatorcontrib>Brandin, A</creatorcontrib><creatorcontrib>Bravar, A</creatorcontrib><creatorcontrib>Cadman, R V</creatorcontrib><creatorcontrib>Cai, X Z</creatorcontrib><creatorcontrib>Caines, H</creatorcontrib><creatorcontrib>Calderón de la Barca Sánchez, M</creatorcontrib><creatorcontrib>Carroll, J</creatorcontrib><creatorcontrib>Castillo, J</creatorcontrib><creatorcontrib>Castro, M</creatorcontrib><creatorcontrib>Cebra, D</creatorcontrib><creatorcontrib>Chaloupka, P</creatorcontrib><creatorcontrib>Chattopadhyay, S</creatorcontrib><creatorcontrib>Chen, H F</creatorcontrib><creatorcontrib>Chen, Y</creatorcontrib><creatorcontrib>Chernenko, S P</creatorcontrib><creatorcontrib>Cherney, M</creatorcontrib><creatorcontrib>Chikanian, A</creatorcontrib><creatorcontrib>Choi, B</creatorcontrib><creatorcontrib>Christie, W</creatorcontrib><creatorcontrib>Coffin, J P</creatorcontrib><creatorcontrib>Cormier, T M</creatorcontrib><creatorcontrib>Cramer, J G</creatorcontrib><creatorcontrib>Crawford, H J</creatorcontrib><creatorcontrib>Das, D</creatorcontrib><creatorcontrib>Das, S</creatorcontrib><creatorcontrib>Derevschikov, A A</creatorcontrib><creatorcontrib>Didenko, L</creatorcontrib><creatorcontrib>Dietel, T</creatorcontrib><creatorcontrib>Dong, W J</creatorcontrib><creatorcontrib>Dong, X</creatorcontrib><creatorcontrib>Draper, J E</creatorcontrib><creatorcontrib>Du, F</creatorcontrib><creatorcontrib>Dubey, A K</creatorcontrib><creatorcontrib>Dunin, V B</creatorcontrib><creatorcontrib>Dunlop, J C</creatorcontrib><creatorcontrib>Dutta Majumdar, M R</creatorcontrib><creatorcontrib>Eckardt, V</creatorcontrib><creatorcontrib>Efimov, L G</creatorcontrib><creatorcontrib>Emelianov, V</creatorcontrib><creatorcontrib>Engelage, J</creatorcontrib><creatorcontrib>Eppley, G</creatorcontrib><creatorcontrib>Erazmus, B</creatorcontrib><creatorcontrib>Estienne, M</creatorcontrib><creatorcontrib>Fachini, P</creatorcontrib><creatorcontrib>Faine, V</creatorcontrib><creatorcontrib>Faivre, J</creatorcontrib><creatorcontrib>Fatemi, R</creatorcontrib><creatorcontrib>Filimonov, K</creatorcontrib><creatorcontrib>Filip, P</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>Ganti, M S</creatorcontrib><creatorcontrib>Gaudichet, L</creatorcontrib><creatorcontrib>Germain, M</creatorcontrib><creatorcontrib>Geurts, F</creatorcontrib><creatorcontrib>Ghazikhanian, V</creatorcontrib><creatorcontrib>Ghosh, P</creatorcontrib><creatorcontrib>Gonzalez, J E</creatorcontrib><creatorcontrib>Grachov, O</creatorcontrib><creatorcontrib>Grigoriev, V</creatorcontrib><creatorcontrib>Gronstal, S</creatorcontrib><creatorcontrib>Grosnick, D</creatorcontrib><creatorcontrib>Guedon, M</creatorcontrib><creatorcontrib>Guertin, S M</creatorcontrib><creatorcontrib>Gupta, A</creatorcontrib><creatorcontrib>STAR Collaboration</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><collection>Hyper Article en Ligne (HAL)</collection><jtitle>Physical review letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Adams, J</au><au>Adler, C</au><au>Aggarwal, M M</au><au>Ahammed, Z</au><au>Amonett, J</au><au>Anderson, B D</au><au>Anderson, M</au><au>Arkhipkin, D</au><au>Averichev, G S</au><au>Badyal, S K</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>Bezverkhny, B I</au><au>Bhardwaj, S</au><au>Bhaskar, P</au><au>Bhati, A K</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>Botje, M</au><au>Boucham, A</au><au>Brandin, A</au><au>Bravar, A</au><au>Cadman, R V</au><au>Cai, X Z</au><au>Caines, H</au><au>Calderón de la Barca Sánchez, M</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, H F</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>Das, D</au><au>Das, S</au><au>Derevschikov, A A</au><au>Didenko, L</au><au>Dietel, T</au><au>Dong, W J</au><au>Dong, X</au><au>Draper, J E</au><au>Du, F</au><au>Dubey, A K</au><au>Dunin, V B</au><au>Dunlop, J C</au><au>Dutta Majumdar, M R</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>Estienne, M</au><au>Fachini, P</au><au>Faine, V</au><au>Faivre, J</au><au>Fatemi, R</au><au>Filimonov, K</au><au>Filip, P</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>Ganti, M S</au><au>Gaudichet, L</au><au>Germain, M</au><au>Geurts, F</au><au>Ghazikhanian, V</au><au>Ghosh, P</au><au>Gonzalez, J E</au><au>Grachov, O</au><au>Grigoriev, V</au><au>Gronstal, S</au><au>Grosnick, D</au><au>Guedon, M</au><au>Guertin, S M</au><au>Gupta, A</au><aucorp>STAR Collaboration</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Azimuthal anisotropy at the relativistic heavy ion collider: the first and fourth harmonics</atitle><jtitle>Physical review letters</jtitle><addtitle>Phys Rev Lett</addtitle><date>2004-02-13</date><risdate>2004</risdate><volume>92</volume><issue>6</issue><spage>062301</spage><epage>062301</epage><pages>062301-062301</pages><artnum>062301</artnum><issn>0031-9007</issn><eissn>1079-7114</eissn><abstract>We report the first observations of the first harmonic (directed flow, v(1)) and the fourth harmonic (v(4)), in the azimuthal distribution of particles with respect to the reaction plane in Au+Au collisions at the BNL Relativistic Heavy Ion Collider (RHIC). Both measurements were done taking advantage of the large elliptic flow (v(2)) generated at RHIC. From the correlation of v(2) with v(1) it is determined that v(2) is positive, or in-plane. The integrated v(4) is about a factor of 10 smaller than v(2). For the sixth (v(6)) and eighth (v(8)) harmonics upper limits on the magnitudes are reported.</abstract><cop>United States</cop><pub>American Physical Society</pub><pmid>14995231</pmid><doi>10.1103/physrevlett.92.062301</doi><tpages>1</tpages><orcidid>https://orcid.org/0000-0001-7382-1609</orcidid><orcidid>https://orcid.org/0000-0001-8890-1273</orcidid><orcidid>https://orcid.org/0000-0001-5920-6271</orcidid><orcidid>https://orcid.org/0000-0003-0687-5580</orcidid><orcidid>https://orcid.org/0000-0002-9781-2632</orcidid><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0031-9007 |
ispartof | Physical review letters, 2004-02, Vol.92 (6), p.062301-062301, Article 062301 |
issn | 0031-9007 1079-7114 |
language | eng |
recordid | cdi_hal_primary_oai_HAL_in2p3_00021600v1 |
source | American Physical Society Journals |
subjects | High Energy Physics - Phenomenology Physics |
title | Azimuthal anisotropy at the relativistic heavy ion collider: the first and fourth harmonics |
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