Measurement of elliptic flow of light nuclei at sNN=200 , 62.4, 39, 27, 19.6, 11.5, and 7.7 GeV at the BNL Relativistic Heavy Ion Collider
We present measurements of second-order azimuthal anisotropy (v2) at midrapidity (|y| < 1.0) for light nuclei d,t,3He (for sNN=200, 62.4, 39, 27, 19.6, 11.5, and 7.7 GeV) and antinuclei $ \overline{d}\ $; (sNN=200, 62.4, 39, 27, and 19.6 GeV) and 3H$ \overline{e}\ $(sNN=200 GeV) in the STAR (Sole...
Gespeichert in:
Veröffentlicht in: | Physical review. C 2016-09, Vol.94 (3) |
---|---|
Hauptverfasser: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | |
---|---|
container_issue | 3 |
container_start_page | |
container_title | Physical review. C |
container_volume | 94 |
creator | Agakishiev, G. Aggarwal, M. M. Ahammed, Z. Averichev, G. S. Bhati, A. K. Brandin, A. V. Bunzarov, I. Campbell, J. M. Chattopadhyay, S. Contin, G. Das, S. Derevschikov, A. A. Dunlop, J. C. Engelage, J. Esha, R. Eyser, O. Fedorisin, J. Fisyak, Y. Flores, C. E. Fulek, L. Gupta, S. Hamad, A. I. Harris, J. W. Horvat, S. Huang, B. Humanic, T. J. Jacobs, W. W. Jang, H. Jia, J. Judd, E. G. Kauder, K. Keane, D. Khan, Z. H. Kisiel, A. Kosarzewski, L. K. Lamont, M. A. C. Lednicky, R. Li, W. Lisa, M. A. Ljubicic, T. Llope, W. J. Margetis, S. McDonald, D. Nandi, B. K. Nasim, Md Nayak, T. K. Niida, T. Novak, J. Nurushev, S. B. Okorokov, V. A. Page, B. S. Pile, P. Pluta, J. Poniatowska, K. Posik, M. Poskanzer, A. M. Quintero, A. Raniwala, S. Ray, R. L. Roberts, J. B. Rogachevskiy, O. V. Romero, J. L. Ruan, L. Sahoo, N. R. Sakrejda, I. Sarkar, A. Seger, J. Seyboth, P. Sharma, B. Shou, Q. Y. Smirnov, D. Song, L. Spinka, H. M. Srivastava, B. Strikhanov, M. Sun, X. M. Sun, Y. Tang, Z. Tawfik, A. Thäder, J. Timmins, A. R. Tsai, O. D. Vandenbroucke, M. Vasiliev, A. N. Vertesi, R. Vokal, S. Voloshin, S. A. Wang, Y. Wen, L. Witt, R. Xu, Y. F. Xu, N. Yang, Q. Ye, Z. Yu, N. Zhang, J. Zhang, S. Zhong, C. Zhu, X. Zoulkarneeva, Y. |
description | We present measurements of second-order azimuthal anisotropy (v2) at midrapidity (|y| < 1.0) for light nuclei d,t,3He (for sNN=200, 62.4, 39, 27, 19.6, 11.5, and 7.7 GeV) and antinuclei $ \overline{d}\ $; (sNN=200, 62.4, 39, 27, and 19.6 GeV) and 3H$ \overline{e}\ $(sNN=200 GeV) in the STAR (Solenoidal Tracker at RHIC) experiment. The v2 for these light nuclei produced in heavy-ion collisions is compared with those for p and $ \overline{p}\ $. We observe mass ordering in nuclei v2(pT) at low transverse momenta (pT < 2.0 GeV/c). We also find a centrality dependence of v2 for d and $ \overline{d}\ $. The magnitude of v2 for t and 3He agree within statistical errors. Light-nuclei v2 are compared with predictions from a blast-wave model. Atomic mass number (A) scaling of light-nuclei v2(pT) seems to hold for pT/A < 1.5GeV/c. Results on light-nuclei v2 from a transport-plus-coalescence model are consistent with the experimental measurements. |
doi_str_mv | 10.1103/PhysRevC.94.034908 |
format | Article |
fullrecord | <record><control><sourceid>osti</sourceid><recordid>TN_cdi_osti_scitechconnect_1340398</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1340398</sourcerecordid><originalsourceid>FETCH-LOGICAL-o97t-cbc22cd1ad1b8f22ca7ebb13f1a9968716670120371dd1dde5b6bac747ac06be3</originalsourceid><addsrcrecordid>eNo9jkFLw0AQhRdRsGj_gKfBcxJns-lu9uBBg7aFWqUUr2WzmZjImkh3W-lf8FebogjDzGPgfe8xdsUx4RzFzUtz8CvaF4nOEhSZxvyEjdJM6lhrLU7_dT45Z2Pv3xGRS9SK44h9P5Hxuy19UBegr4Gcaz9Da6F2_dfx4dq3JkC3s45aMAH8cnmbIkIEMk2yCISOIFURcJ3IYfNkEoHpKlCJgim9Hi2hIbhfLmBFzoR23_ojf0Zmf4B530HRD5kVbS_ZWW2cp_HfvWDrx4d1MYsXz9N5cbeIe61CbEubprbipuJlXg_SKCpLLmputJa54lIq5CkKxatqGJqUsjRWZcpYlCWJC3b9i-2HHhtv20C2sX3XkQ0bLjIUOhc_nD1hUA</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Measurement of elliptic flow of light nuclei at sNN=200 , 62.4, 39, 27, 19.6, 11.5, and 7.7 GeV at the BNL Relativistic Heavy Ion Collider</title><source>American Physical Society Journals</source><creator>Agakishiev, G. ; Aggarwal, M. M. ; Ahammed, Z. ; Averichev, G. S. ; Bhati, A. K. ; Brandin, A. V. ; Bunzarov, I. ; Campbell, J. M. ; Chattopadhyay, S. ; Contin, G. ; Das, S. ; Derevschikov, A. A. ; Dunlop, J. C. ; Engelage, J. ; Esha, R. ; Eyser, O. ; Fedorisin, J. ; Fisyak, Y. ; Flores, C. E. ; Fulek, L. ; Gupta, S. ; Hamad, A. I. ; Harris, J. W. ; Horvat, S. ; Huang, B. ; Humanic, T. J. ; Jacobs, W. W. ; Jang, H. ; Jia, J. ; Judd, E. G. ; Kauder, K. ; Keane, D. ; Khan, Z. H. ; Kisiel, A. ; Kosarzewski, L. K. ; Lamont, M. A. C. ; Lednicky, R. ; Li, W. ; Lisa, M. A. ; Ljubicic, T. ; Llope, W. J. ; Margetis, S. ; McDonald, D. ; Nandi, B. K. ; Nasim, Md ; Nayak, T. K. ; Niida, T. ; Novak, J. ; Nurushev, S. B. ; Okorokov, V. A. ; Page, B. S. ; Pile, P. ; Pluta, J. ; Poniatowska, K. ; Posik, M. ; Poskanzer, A. M. ; Quintero, A. ; Raniwala, S. ; Ray, R. L. ; Roberts, J. B. ; Rogachevskiy, O. V. ; Romero, J. L. ; Ruan, L. ; Sahoo, N. R. ; Sakrejda, I. ; Sarkar, A. ; Seger, J. ; Seyboth, P. ; Sharma, B. ; Shou, Q. Y. ; Smirnov, D. ; Song, L. ; Spinka, H. M. ; Srivastava, B. ; Strikhanov, M. ; Sun, X. M. ; Sun, Y. ; Tang, Z. ; Tawfik, A. ; Thäder, J. ; Timmins, A. R. ; Tsai, O. D. ; Vandenbroucke, M. ; Vasiliev, A. N. ; Vertesi, R. ; Vokal, S. ; Voloshin, S. A. ; Wang, Y. ; Wen, L. ; Witt, R. ; Xu, Y. F. ; Xu, N. ; Yang, Q. ; Ye, Z. ; Yu, N. ; Zhang, J. ; Zhang, S. ; Zhong, C. ; Zhu, X. ; Zoulkarneeva, Y.</creator><creatorcontrib>Agakishiev, G. ; Aggarwal, M. M. ; Ahammed, Z. ; Averichev, G. S. ; Bhati, A. K. ; Brandin, A. V. ; Bunzarov, I. ; Campbell, J. M. ; Chattopadhyay, S. ; Contin, G. ; Das, S. ; Derevschikov, A. A. ; Dunlop, J. C. ; Engelage, J. ; Esha, R. ; Eyser, O. ; Fedorisin, J. ; Fisyak, Y. ; Flores, C. E. ; Fulek, L. ; Gupta, S. ; Hamad, A. I. ; Harris, J. W. ; Horvat, S. ; Huang, B. ; Humanic, T. J. ; Jacobs, W. W. ; Jang, H. ; Jia, J. ; Judd, E. G. ; Kauder, K. ; Keane, D. ; Khan, Z. H. ; Kisiel, A. ; Kosarzewski, L. K. ; Lamont, M. A. C. ; Lednicky, R. ; Li, W. ; Lisa, M. A. ; Ljubicic, T. ; Llope, W. J. ; Margetis, S. ; McDonald, D. ; Nandi, B. K. ; Nasim, Md ; Nayak, T. K. ; Niida, T. ; Novak, J. ; Nurushev, S. B. ; Okorokov, V. A. ; Page, B. S. ; Pile, P. ; Pluta, J. ; Poniatowska, K. ; Posik, M. ; Poskanzer, A. M. ; Quintero, A. ; Raniwala, S. ; Ray, R. L. ; Roberts, J. B. ; Rogachevskiy, O. V. ; Romero, J. L. ; Ruan, L. ; Sahoo, N. R. ; Sakrejda, I. ; Sarkar, A. ; Seger, J. ; Seyboth, P. ; Sharma, B. ; Shou, Q. Y. ; Smirnov, D. ; Song, L. ; Spinka, H. M. ; Srivastava, B. ; Strikhanov, M. ; Sun, X. M. ; Sun, Y. ; Tang, Z. ; Tawfik, A. ; Thäder, J. ; Timmins, A. R. ; Tsai, O. D. ; Vandenbroucke, M. ; Vasiliev, A. N. ; Vertesi, R. ; Vokal, S. ; Voloshin, S. A. ; Wang, Y. ; Wen, L. ; Witt, R. ; Xu, Y. F. ; Xu, N. ; Yang, Q. ; Ye, Z. ; Yu, N. ; Zhang, J. ; Zhang, S. ; Zhong, C. ; Zhu, X. ; Zoulkarneeva, Y. ; Brookhaven National Lab. (BNL), Upton, NY (United States) ; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)</creatorcontrib><description>We present measurements of second-order azimuthal anisotropy (v2) at midrapidity (|y| < 1.0) for light nuclei d,t,3He (for sNN=200, 62.4, 39, 27, 19.6, 11.5, and 7.7 GeV) and antinuclei $ \overline{d}\ $; (sNN=200, 62.4, 39, 27, and 19.6 GeV) and 3H$ \overline{e}\ $(sNN=200 GeV) in the STAR (Solenoidal Tracker at RHIC) experiment. The v2 for these light nuclei produced in heavy-ion collisions is compared with those for p and $ \overline{p}\ $. We observe mass ordering in nuclei v2(pT) at low transverse momenta (pT < 2.0 GeV/c). We also find a centrality dependence of v2 for d and $ \overline{d}\ $. The magnitude of v2 for t and 3He agree within statistical errors. Light-nuclei v2 are compared with predictions from a blast-wave model. Atomic mass number (A) scaling of light-nuclei v2(pT) seems to hold for pT/A < 1.5GeV/c. Results on light-nuclei v2 from a transport-plus-coalescence model are consistent with the experimental measurements.</description><identifier>ISSN: 2469-9985</identifier><identifier>EISSN: 2469-9993</identifier><identifier>DOI: 10.1103/PhysRevC.94.034908</identifier><language>eng</language><publisher>United States: American Physical Society (APS)</publisher><subject>NUCLEAR PHYSICS AND RADIATION PHYSICS</subject><ispartof>Physical review. C, 2016-09, Vol.94 (3)</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,776,780,881,27901,27902</link.rule.ids><backlink>$$Uhttps://www.osti.gov/servlets/purl/1340398$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Agakishiev, G.</creatorcontrib><creatorcontrib>Aggarwal, M. M.</creatorcontrib><creatorcontrib>Ahammed, Z.</creatorcontrib><creatorcontrib>Averichev, G. S.</creatorcontrib><creatorcontrib>Bhati, A. K.</creatorcontrib><creatorcontrib>Brandin, A. V.</creatorcontrib><creatorcontrib>Bunzarov, I.</creatorcontrib><creatorcontrib>Campbell, J. M.</creatorcontrib><creatorcontrib>Chattopadhyay, S.</creatorcontrib><creatorcontrib>Contin, G.</creatorcontrib><creatorcontrib>Das, S.</creatorcontrib><creatorcontrib>Derevschikov, A. A.</creatorcontrib><creatorcontrib>Dunlop, J. C.</creatorcontrib><creatorcontrib>Engelage, J.</creatorcontrib><creatorcontrib>Esha, R.</creatorcontrib><creatorcontrib>Eyser, O.</creatorcontrib><creatorcontrib>Fedorisin, J.</creatorcontrib><creatorcontrib>Fisyak, Y.</creatorcontrib><creatorcontrib>Flores, C. E.</creatorcontrib><creatorcontrib>Fulek, L.</creatorcontrib><creatorcontrib>Gupta, S.</creatorcontrib><creatorcontrib>Hamad, A. I.</creatorcontrib><creatorcontrib>Harris, J. W.</creatorcontrib><creatorcontrib>Horvat, S.</creatorcontrib><creatorcontrib>Huang, B.</creatorcontrib><creatorcontrib>Humanic, T. J.</creatorcontrib><creatorcontrib>Jacobs, W. W.</creatorcontrib><creatorcontrib>Jang, H.</creatorcontrib><creatorcontrib>Jia, J.</creatorcontrib><creatorcontrib>Judd, E. G.</creatorcontrib><creatorcontrib>Kauder, K.</creatorcontrib><creatorcontrib>Keane, D.</creatorcontrib><creatorcontrib>Khan, Z. H.</creatorcontrib><creatorcontrib>Kisiel, A.</creatorcontrib><creatorcontrib>Kosarzewski, L. K.</creatorcontrib><creatorcontrib>Lamont, M. A. C.</creatorcontrib><creatorcontrib>Lednicky, R.</creatorcontrib><creatorcontrib>Li, W.</creatorcontrib><creatorcontrib>Lisa, M. A.</creatorcontrib><creatorcontrib>Ljubicic, T.</creatorcontrib><creatorcontrib>Llope, W. J.</creatorcontrib><creatorcontrib>Margetis, S.</creatorcontrib><creatorcontrib>McDonald, D.</creatorcontrib><creatorcontrib>Nandi, B. K.</creatorcontrib><creatorcontrib>Nasim, Md</creatorcontrib><creatorcontrib>Nayak, T. K.</creatorcontrib><creatorcontrib>Niida, T.</creatorcontrib><creatorcontrib>Novak, J.</creatorcontrib><creatorcontrib>Nurushev, S. B.</creatorcontrib><creatorcontrib>Okorokov, V. A.</creatorcontrib><creatorcontrib>Page, B. S.</creatorcontrib><creatorcontrib>Pile, P.</creatorcontrib><creatorcontrib>Pluta, J.</creatorcontrib><creatorcontrib>Poniatowska, K.</creatorcontrib><creatorcontrib>Posik, M.</creatorcontrib><creatorcontrib>Poskanzer, A. M.</creatorcontrib><creatorcontrib>Quintero, A.</creatorcontrib><creatorcontrib>Raniwala, S.</creatorcontrib><creatorcontrib>Ray, R. L.</creatorcontrib><creatorcontrib>Roberts, J. B.</creatorcontrib><creatorcontrib>Rogachevskiy, O. V.</creatorcontrib><creatorcontrib>Romero, J. L.</creatorcontrib><creatorcontrib>Ruan, L.</creatorcontrib><creatorcontrib>Sahoo, N. R.</creatorcontrib><creatorcontrib>Sakrejda, I.</creatorcontrib><creatorcontrib>Sarkar, A.</creatorcontrib><creatorcontrib>Seger, J.</creatorcontrib><creatorcontrib>Seyboth, P.</creatorcontrib><creatorcontrib>Sharma, B.</creatorcontrib><creatorcontrib>Shou, Q. Y.</creatorcontrib><creatorcontrib>Smirnov, D.</creatorcontrib><creatorcontrib>Song, L.</creatorcontrib><creatorcontrib>Spinka, H. M.</creatorcontrib><creatorcontrib>Srivastava, B.</creatorcontrib><creatorcontrib>Strikhanov, M.</creatorcontrib><creatorcontrib>Sun, X. M.</creatorcontrib><creatorcontrib>Sun, Y.</creatorcontrib><creatorcontrib>Tang, Z.</creatorcontrib><creatorcontrib>Tawfik, A.</creatorcontrib><creatorcontrib>Thäder, J.</creatorcontrib><creatorcontrib>Timmins, A. R.</creatorcontrib><creatorcontrib>Tsai, O. D.</creatorcontrib><creatorcontrib>Vandenbroucke, M.</creatorcontrib><creatorcontrib>Vasiliev, A. N.</creatorcontrib><creatorcontrib>Vertesi, R.</creatorcontrib><creatorcontrib>Vokal, S.</creatorcontrib><creatorcontrib>Voloshin, S. A.</creatorcontrib><creatorcontrib>Wang, Y.</creatorcontrib><creatorcontrib>Wen, L.</creatorcontrib><creatorcontrib>Witt, R.</creatorcontrib><creatorcontrib>Xu, Y. F.</creatorcontrib><creatorcontrib>Xu, N.</creatorcontrib><creatorcontrib>Yang, Q.</creatorcontrib><creatorcontrib>Ye, Z.</creatorcontrib><creatorcontrib>Yu, N.</creatorcontrib><creatorcontrib>Zhang, J.</creatorcontrib><creatorcontrib>Zhang, S.</creatorcontrib><creatorcontrib>Zhong, C.</creatorcontrib><creatorcontrib>Zhu, X.</creatorcontrib><creatorcontrib>Zoulkarneeva, Y.</creatorcontrib><creatorcontrib>Brookhaven National Lab. (BNL), Upton, NY (United States)</creatorcontrib><creatorcontrib>Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)</creatorcontrib><title>Measurement of elliptic flow of light nuclei at sNN=200 , 62.4, 39, 27, 19.6, 11.5, and 7.7 GeV at the BNL Relativistic Heavy Ion Collider</title><title>Physical review. C</title><description>We present measurements of second-order azimuthal anisotropy (v2) at midrapidity (|y| < 1.0) for light nuclei d,t,3He (for sNN=200, 62.4, 39, 27, 19.6, 11.5, and 7.7 GeV) and antinuclei $ \overline{d}\ $; (sNN=200, 62.4, 39, 27, and 19.6 GeV) and 3H$ \overline{e}\ $(sNN=200 GeV) in the STAR (Solenoidal Tracker at RHIC) experiment. The v2 for these light nuclei produced in heavy-ion collisions is compared with those for p and $ \overline{p}\ $. We observe mass ordering in nuclei v2(pT) at low transverse momenta (pT < 2.0 GeV/c). We also find a centrality dependence of v2 for d and $ \overline{d}\ $. The magnitude of v2 for t and 3He agree within statistical errors. Light-nuclei v2 are compared with predictions from a blast-wave model. Atomic mass number (A) scaling of light-nuclei v2(pT) seems to hold for pT/A < 1.5GeV/c. Results on light-nuclei v2 from a transport-plus-coalescence model are consistent with the experimental measurements.</description><subject>NUCLEAR PHYSICS AND RADIATION PHYSICS</subject><issn>2469-9985</issn><issn>2469-9993</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><recordid>eNo9jkFLw0AQhRdRsGj_gKfBcxJns-lu9uBBg7aFWqUUr2WzmZjImkh3W-lf8FebogjDzGPgfe8xdsUx4RzFzUtz8CvaF4nOEhSZxvyEjdJM6lhrLU7_dT45Z2Pv3xGRS9SK44h9P5Hxuy19UBegr4Gcaz9Da6F2_dfx4dq3JkC3s45aMAH8cnmbIkIEMk2yCISOIFURcJ3IYfNkEoHpKlCJgim9Hi2hIbhfLmBFzoR23_ojf0Zmf4B530HRD5kVbS_ZWW2cp_HfvWDrx4d1MYsXz9N5cbeIe61CbEubprbipuJlXg_SKCpLLmputJa54lIq5CkKxatqGJqUsjRWZcpYlCWJC3b9i-2HHhtv20C2sX3XkQ0bLjIUOhc_nD1hUA</recordid><startdate>20160923</startdate><enddate>20160923</enddate><creator>Agakishiev, G.</creator><creator>Aggarwal, M. M.</creator><creator>Ahammed, Z.</creator><creator>Averichev, G. S.</creator><creator>Bhati, A. K.</creator><creator>Brandin, A. V.</creator><creator>Bunzarov, I.</creator><creator>Campbell, J. M.</creator><creator>Chattopadhyay, S.</creator><creator>Contin, G.</creator><creator>Das, S.</creator><creator>Derevschikov, A. A.</creator><creator>Dunlop, J. C.</creator><creator>Engelage, J.</creator><creator>Esha, R.</creator><creator>Eyser, O.</creator><creator>Fedorisin, J.</creator><creator>Fisyak, Y.</creator><creator>Flores, C. E.</creator><creator>Fulek, L.</creator><creator>Gupta, S.</creator><creator>Hamad, A. I.</creator><creator>Harris, J. W.</creator><creator>Horvat, S.</creator><creator>Huang, B.</creator><creator>Humanic, T. J.</creator><creator>Jacobs, W. W.</creator><creator>Jang, H.</creator><creator>Jia, J.</creator><creator>Judd, E. G.</creator><creator>Kauder, K.</creator><creator>Keane, D.</creator><creator>Khan, Z. H.</creator><creator>Kisiel, A.</creator><creator>Kosarzewski, L. K.</creator><creator>Lamont, M. A. C.</creator><creator>Lednicky, R.</creator><creator>Li, W.</creator><creator>Lisa, M. A.</creator><creator>Ljubicic, T.</creator><creator>Llope, W. J.</creator><creator>Margetis, S.</creator><creator>McDonald, D.</creator><creator>Nandi, B. K.</creator><creator>Nasim, Md</creator><creator>Nayak, T. K.</creator><creator>Niida, T.</creator><creator>Novak, J.</creator><creator>Nurushev, S. B.</creator><creator>Okorokov, V. A.</creator><creator>Page, B. S.</creator><creator>Pile, P.</creator><creator>Pluta, J.</creator><creator>Poniatowska, K.</creator><creator>Posik, M.</creator><creator>Poskanzer, A. M.</creator><creator>Quintero, A.</creator><creator>Raniwala, S.</creator><creator>Ray, R. L.</creator><creator>Roberts, J. B.</creator><creator>Rogachevskiy, O. V.</creator><creator>Romero, J. L.</creator><creator>Ruan, L.</creator><creator>Sahoo, N. R.</creator><creator>Sakrejda, I.</creator><creator>Sarkar, A.</creator><creator>Seger, J.</creator><creator>Seyboth, P.</creator><creator>Sharma, B.</creator><creator>Shou, Q. Y.</creator><creator>Smirnov, D.</creator><creator>Song, L.</creator><creator>Spinka, H. M.</creator><creator>Srivastava, B.</creator><creator>Strikhanov, M.</creator><creator>Sun, X. M.</creator><creator>Sun, Y.</creator><creator>Tang, Z.</creator><creator>Tawfik, A.</creator><creator>Thäder, J.</creator><creator>Timmins, A. R.</creator><creator>Tsai, O. D.</creator><creator>Vandenbroucke, M.</creator><creator>Vasiliev, A. N.</creator><creator>Vertesi, R.</creator><creator>Vokal, S.</creator><creator>Voloshin, S. A.</creator><creator>Wang, Y.</creator><creator>Wen, L.</creator><creator>Witt, R.</creator><creator>Xu, Y. F.</creator><creator>Xu, N.</creator><creator>Yang, Q.</creator><creator>Ye, Z.</creator><creator>Yu, N.</creator><creator>Zhang, J.</creator><creator>Zhang, S.</creator><creator>Zhong, C.</creator><creator>Zhu, X.</creator><creator>Zoulkarneeva, Y.</creator><general>American Physical Society (APS)</general><scope>OIOZB</scope><scope>OTOTI</scope></search><sort><creationdate>20160923</creationdate><title>Measurement of elliptic flow of light nuclei at sNN=200 , 62.4, 39, 27, 19.6, 11.5, and 7.7 GeV at the BNL Relativistic Heavy Ion Collider</title><author>Agakishiev, G. ; Aggarwal, M. M. ; Ahammed, Z. ; Averichev, G. S. ; Bhati, A. K. ; Brandin, A. V. ; Bunzarov, I. ; Campbell, J. M. ; Chattopadhyay, S. ; Contin, G. ; Das, S. ; Derevschikov, A. A. ; Dunlop, J. C. ; Engelage, J. ; Esha, R. ; Eyser, O. ; Fedorisin, J. ; Fisyak, Y. ; Flores, C. E. ; Fulek, L. ; Gupta, S. ; Hamad, A. I. ; Harris, J. W. ; Horvat, S. ; Huang, B. ; Humanic, T. J. ; Jacobs, W. W. ; Jang, H. ; Jia, J. ; Judd, E. G. ; Kauder, K. ; Keane, D. ; Khan, Z. H. ; Kisiel, A. ; Kosarzewski, L. K. ; Lamont, M. A. C. ; Lednicky, R. ; Li, W. ; Lisa, M. A. ; Ljubicic, T. ; Llope, W. J. ; Margetis, S. ; McDonald, D. ; Nandi, B. K. ; Nasim, Md ; Nayak, T. K. ; Niida, T. ; Novak, J. ; Nurushev, S. B. ; Okorokov, V. A. ; Page, B. S. ; Pile, P. ; Pluta, J. ; Poniatowska, K. ; Posik, M. ; Poskanzer, A. M. ; Quintero, A. ; Raniwala, S. ; Ray, R. L. ; Roberts, J. B. ; Rogachevskiy, O. V. ; Romero, J. L. ; Ruan, L. ; Sahoo, N. R. ; Sakrejda, I. ; Sarkar, A. ; Seger, J. ; Seyboth, P. ; Sharma, B. ; Shou, Q. Y. ; Smirnov, D. ; Song, L. ; Spinka, H. M. ; Srivastava, B. ; Strikhanov, M. ; Sun, X. M. ; Sun, Y. ; Tang, Z. ; Tawfik, A. ; Thäder, J. ; Timmins, A. R. ; Tsai, O. D. ; Vandenbroucke, M. ; Vasiliev, A. N. ; Vertesi, R. ; Vokal, S. ; Voloshin, S. A. ; Wang, Y. ; Wen, L. ; Witt, R. ; Xu, Y. F. ; Xu, N. ; Yang, Q. ; Ye, Z. ; Yu, N. ; Zhang, J. ; Zhang, S. ; Zhong, C. ; Zhu, X. ; Zoulkarneeva, Y.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-o97t-cbc22cd1ad1b8f22ca7ebb13f1a9968716670120371dd1dde5b6bac747ac06be3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>NUCLEAR PHYSICS AND RADIATION PHYSICS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Agakishiev, G.</creatorcontrib><creatorcontrib>Aggarwal, M. M.</creatorcontrib><creatorcontrib>Ahammed, Z.</creatorcontrib><creatorcontrib>Averichev, G. S.</creatorcontrib><creatorcontrib>Bhati, A. K.</creatorcontrib><creatorcontrib>Brandin, A. V.</creatorcontrib><creatorcontrib>Bunzarov, I.</creatorcontrib><creatorcontrib>Campbell, J. M.</creatorcontrib><creatorcontrib>Chattopadhyay, S.</creatorcontrib><creatorcontrib>Contin, G.</creatorcontrib><creatorcontrib>Das, S.</creatorcontrib><creatorcontrib>Derevschikov, A. A.</creatorcontrib><creatorcontrib>Dunlop, J. C.</creatorcontrib><creatorcontrib>Engelage, J.</creatorcontrib><creatorcontrib>Esha, R.</creatorcontrib><creatorcontrib>Eyser, O.</creatorcontrib><creatorcontrib>Fedorisin, J.</creatorcontrib><creatorcontrib>Fisyak, Y.</creatorcontrib><creatorcontrib>Flores, C. E.</creatorcontrib><creatorcontrib>Fulek, L.</creatorcontrib><creatorcontrib>Gupta, S.</creatorcontrib><creatorcontrib>Hamad, A. I.</creatorcontrib><creatorcontrib>Harris, J. W.</creatorcontrib><creatorcontrib>Horvat, S.</creatorcontrib><creatorcontrib>Huang, B.</creatorcontrib><creatorcontrib>Humanic, T. J.</creatorcontrib><creatorcontrib>Jacobs, W. W.</creatorcontrib><creatorcontrib>Jang, H.</creatorcontrib><creatorcontrib>Jia, J.</creatorcontrib><creatorcontrib>Judd, E. G.</creatorcontrib><creatorcontrib>Kauder, K.</creatorcontrib><creatorcontrib>Keane, D.</creatorcontrib><creatorcontrib>Khan, Z. H.</creatorcontrib><creatorcontrib>Kisiel, A.</creatorcontrib><creatorcontrib>Kosarzewski, L. K.</creatorcontrib><creatorcontrib>Lamont, M. A. C.</creatorcontrib><creatorcontrib>Lednicky, R.</creatorcontrib><creatorcontrib>Li, W.</creatorcontrib><creatorcontrib>Lisa, M. A.</creatorcontrib><creatorcontrib>Ljubicic, T.</creatorcontrib><creatorcontrib>Llope, W. J.</creatorcontrib><creatorcontrib>Margetis, S.</creatorcontrib><creatorcontrib>McDonald, D.</creatorcontrib><creatorcontrib>Nandi, B. K.</creatorcontrib><creatorcontrib>Nasim, Md</creatorcontrib><creatorcontrib>Nayak, T. K.</creatorcontrib><creatorcontrib>Niida, T.</creatorcontrib><creatorcontrib>Novak, J.</creatorcontrib><creatorcontrib>Nurushev, S. B.</creatorcontrib><creatorcontrib>Okorokov, V. A.</creatorcontrib><creatorcontrib>Page, B. S.</creatorcontrib><creatorcontrib>Pile, P.</creatorcontrib><creatorcontrib>Pluta, J.</creatorcontrib><creatorcontrib>Poniatowska, K.</creatorcontrib><creatorcontrib>Posik, M.</creatorcontrib><creatorcontrib>Poskanzer, A. M.</creatorcontrib><creatorcontrib>Quintero, A.</creatorcontrib><creatorcontrib>Raniwala, S.</creatorcontrib><creatorcontrib>Ray, R. L.</creatorcontrib><creatorcontrib>Roberts, J. B.</creatorcontrib><creatorcontrib>Rogachevskiy, O. V.</creatorcontrib><creatorcontrib>Romero, J. L.</creatorcontrib><creatorcontrib>Ruan, L.</creatorcontrib><creatorcontrib>Sahoo, N. R.</creatorcontrib><creatorcontrib>Sakrejda, I.</creatorcontrib><creatorcontrib>Sarkar, A.</creatorcontrib><creatorcontrib>Seger, J.</creatorcontrib><creatorcontrib>Seyboth, P.</creatorcontrib><creatorcontrib>Sharma, B.</creatorcontrib><creatorcontrib>Shou, Q. Y.</creatorcontrib><creatorcontrib>Smirnov, D.</creatorcontrib><creatorcontrib>Song, L.</creatorcontrib><creatorcontrib>Spinka, H. M.</creatorcontrib><creatorcontrib>Srivastava, B.</creatorcontrib><creatorcontrib>Strikhanov, M.</creatorcontrib><creatorcontrib>Sun, X. M.</creatorcontrib><creatorcontrib>Sun, Y.</creatorcontrib><creatorcontrib>Tang, Z.</creatorcontrib><creatorcontrib>Tawfik, A.</creatorcontrib><creatorcontrib>Thäder, J.</creatorcontrib><creatorcontrib>Timmins, A. R.</creatorcontrib><creatorcontrib>Tsai, O. D.</creatorcontrib><creatorcontrib>Vandenbroucke, M.</creatorcontrib><creatorcontrib>Vasiliev, A. N.</creatorcontrib><creatorcontrib>Vertesi, R.</creatorcontrib><creatorcontrib>Vokal, S.</creatorcontrib><creatorcontrib>Voloshin, S. A.</creatorcontrib><creatorcontrib>Wang, Y.</creatorcontrib><creatorcontrib>Wen, L.</creatorcontrib><creatorcontrib>Witt, R.</creatorcontrib><creatorcontrib>Xu, Y. F.</creatorcontrib><creatorcontrib>Xu, N.</creatorcontrib><creatorcontrib>Yang, Q.</creatorcontrib><creatorcontrib>Ye, Z.</creatorcontrib><creatorcontrib>Yu, N.</creatorcontrib><creatorcontrib>Zhang, J.</creatorcontrib><creatorcontrib>Zhang, S.</creatorcontrib><creatorcontrib>Zhong, C.</creatorcontrib><creatorcontrib>Zhu, X.</creatorcontrib><creatorcontrib>Zoulkarneeva, Y.</creatorcontrib><creatorcontrib>Brookhaven National Lab. (BNL), Upton, NY (United States)</creatorcontrib><creatorcontrib>Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)</creatorcontrib><collection>OSTI.GOV - Hybrid</collection><collection>OSTI.GOV</collection><jtitle>Physical review. C</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Agakishiev, G.</au><au>Aggarwal, M. M.</au><au>Ahammed, Z.</au><au>Averichev, G. S.</au><au>Bhati, A. K.</au><au>Brandin, A. V.</au><au>Bunzarov, I.</au><au>Campbell, J. M.</au><au>Chattopadhyay, S.</au><au>Contin, G.</au><au>Das, S.</au><au>Derevschikov, A. A.</au><au>Dunlop, J. C.</au><au>Engelage, J.</au><au>Esha, R.</au><au>Eyser, O.</au><au>Fedorisin, J.</au><au>Fisyak, Y.</au><au>Flores, C. E.</au><au>Fulek, L.</au><au>Gupta, S.</au><au>Hamad, A. I.</au><au>Harris, J. W.</au><au>Horvat, S.</au><au>Huang, B.</au><au>Humanic, T. J.</au><au>Jacobs, W. W.</au><au>Jang, H.</au><au>Jia, J.</au><au>Judd, E. G.</au><au>Kauder, K.</au><au>Keane, D.</au><au>Khan, Z. H.</au><au>Kisiel, A.</au><au>Kosarzewski, L. K.</au><au>Lamont, M. A. C.</au><au>Lednicky, R.</au><au>Li, W.</au><au>Lisa, M. A.</au><au>Ljubicic, T.</au><au>Llope, W. J.</au><au>Margetis, S.</au><au>McDonald, D.</au><au>Nandi, B. K.</au><au>Nasim, Md</au><au>Nayak, T. K.</au><au>Niida, T.</au><au>Novak, J.</au><au>Nurushev, S. B.</au><au>Okorokov, V. A.</au><au>Page, B. S.</au><au>Pile, P.</au><au>Pluta, J.</au><au>Poniatowska, K.</au><au>Posik, M.</au><au>Poskanzer, A. M.</au><au>Quintero, A.</au><au>Raniwala, S.</au><au>Ray, R. L.</au><au>Roberts, J. B.</au><au>Rogachevskiy, O. V.</au><au>Romero, J. L.</au><au>Ruan, L.</au><au>Sahoo, N. R.</au><au>Sakrejda, I.</au><au>Sarkar, A.</au><au>Seger, J.</au><au>Seyboth, P.</au><au>Sharma, B.</au><au>Shou, Q. Y.</au><au>Smirnov, D.</au><au>Song, L.</au><au>Spinka, H. M.</au><au>Srivastava, B.</au><au>Strikhanov, M.</au><au>Sun, X. M.</au><au>Sun, Y.</au><au>Tang, Z.</au><au>Tawfik, A.</au><au>Thäder, J.</au><au>Timmins, A. R.</au><au>Tsai, O. D.</au><au>Vandenbroucke, M.</au><au>Vasiliev, A. N.</au><au>Vertesi, R.</au><au>Vokal, S.</au><au>Voloshin, S. A.</au><au>Wang, Y.</au><au>Wen, L.</au><au>Witt, R.</au><au>Xu, Y. F.</au><au>Xu, N.</au><au>Yang, Q.</au><au>Ye, Z.</au><au>Yu, N.</au><au>Zhang, J.</au><au>Zhang, S.</au><au>Zhong, C.</au><au>Zhu, X.</au><au>Zoulkarneeva, Y.</au><aucorp>Brookhaven National Lab. (BNL), Upton, NY (United States)</aucorp><aucorp>Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Measurement of elliptic flow of light nuclei at sNN=200 , 62.4, 39, 27, 19.6, 11.5, and 7.7 GeV at the BNL Relativistic Heavy Ion Collider</atitle><jtitle>Physical review. C</jtitle><date>2016-09-23</date><risdate>2016</risdate><volume>94</volume><issue>3</issue><issn>2469-9985</issn><eissn>2469-9993</eissn><abstract>We present measurements of second-order azimuthal anisotropy (v2) at midrapidity (|y| < 1.0) for light nuclei d,t,3He (for sNN=200, 62.4, 39, 27, 19.6, 11.5, and 7.7 GeV) and antinuclei $ \overline{d}\ $; (sNN=200, 62.4, 39, 27, and 19.6 GeV) and 3H$ \overline{e}\ $(sNN=200 GeV) in the STAR (Solenoidal Tracker at RHIC) experiment. The v2 for these light nuclei produced in heavy-ion collisions is compared with those for p and $ \overline{p}\ $. We observe mass ordering in nuclei v2(pT) at low transverse momenta (pT < 2.0 GeV/c). We also find a centrality dependence of v2 for d and $ \overline{d}\ $. The magnitude of v2 for t and 3He agree within statistical errors. Light-nuclei v2 are compared with predictions from a blast-wave model. Atomic mass number (A) scaling of light-nuclei v2(pT) seems to hold for pT/A < 1.5GeV/c. Results on light-nuclei v2 from a transport-plus-coalescence model are consistent with the experimental measurements.</abstract><cop>United States</cop><pub>American Physical Society (APS)</pub><doi>10.1103/PhysRevC.94.034908</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 2469-9985 |
ispartof | Physical review. C, 2016-09, Vol.94 (3) |
issn | 2469-9985 2469-9993 |
language | eng |
recordid | cdi_osti_scitechconnect_1340398 |
source | American Physical Society Journals |
subjects | NUCLEAR PHYSICS AND RADIATION PHYSICS |
title | Measurement of elliptic flow of light nuclei at sNN=200 , 62.4, 39, 27, 19.6, 11.5, and 7.7 GeV at the BNL Relativistic Heavy Ion Collider |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-18T23%3A06%3A15IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-osti&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Measurement%20of%20elliptic%20flow%20of%20light%20nuclei%20at%20sNN=200%20,%2062.4,%2039,%2027,%2019.6,%2011.5,%20and%207.7%20GeV%20at%20the%20BNL%20Relativistic%20Heavy%20Ion%20Collider&rft.jtitle=Physical%20review.%20C&rft.au=Agakishiev,%20G.&rft.aucorp=Brookhaven%20National%20Lab.%20(BNL),%20Upton,%20NY%20(United%20States)&rft.date=2016-09-23&rft.volume=94&rft.issue=3&rft.issn=2469-9985&rft.eissn=2469-9993&rft_id=info:doi/10.1103/PhysRevC.94.034908&rft_dat=%3Costi%3E1340398%3C/osti%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |