Azimuthal anisotropy in U+U and Au+Au collisions at RHIC
Collisions between prolate uranium nuclei are used to study how particle production and azimuthal anisotropies depend on initial geometry in heavy-ion collisions. We report the two- and four-particle cumulants, v_2\{2\} and v_2\{4\}, for charged hadrons from U+U collisions at \sqrt{s_{\rm NN}} = 193...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
STAR Collaboration [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2015 |
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| Schlagwörter: |
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| Systematik: |
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| Übergeordnetes Werk: |
Enthalten in: Physical review letters - Ridge, NY : American Physical Society, 1958, (2015) |
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| Übergeordnetes Werk: |
year:2015 |
| Links: |
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| DOI / URN: |
10.1103/PhysRevLett.115.222301 |
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| Katalog-ID: |
OLC1969289252 |
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| 520 | |a Collisions between prolate uranium nuclei are used to study how particle production and azimuthal anisotropies depend on initial geometry in heavy-ion collisions. We report the two- and four-particle cumulants, v_2\{2\} and v_2\{4\}, for charged hadrons from U+U collisions at \sqrt{s_{\rm NN}} = 193 GeV and Au+Au collisions at \sqrt{s_{\rm NN}} = 200 GeV. Nearly fully overlapping collisions are selected based on the amount of energy deposited by spectators in the STAR Zero Degree Calorimeters (ZDCs). Within this sample, the observed dependence of v_2\{2\} on multiplicity demonstrates that ZDC information combined with multiplicity can preferentially select different overlap configurations in U+U collisions. An initial-state model with gluon saturation describes the slope of v_2\{2\} as a function of multiplicity in central collisions better than one based on Glauber with a two-component multiplicity model. | ||
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10.1103/PhysRevLett.115.222301 doi PQ20160211 (DE-627)OLC1969289252 (DE-599)GBVOLC1969289252 (PRQ)a622-afab5778867cb7da8afc709bc9e548cddcddfeaa6f94015286d568d757cdbeb40 (KEY)0009201020150000000000000000azimuthalanisotropyinuuandauaucollisionsatrhic DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk STAR Collaboration verfasserin aut Azimuthal anisotropy in U+U and Au+Au collisions at RHIC 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Collisions between prolate uranium nuclei are used to study how particle production and azimuthal anisotropies depend on initial geometry in heavy-ion collisions. We report the two- and four-particle cumulants, v_2\{2\} and v_2\{4\}, for charged hadrons from U+U collisions at \sqrt{s_{\rm NN}} = 193 GeV and Au+Au collisions at \sqrt{s_{\rm NN}} = 200 GeV. Nearly fully overlapping collisions are selected based on the amount of energy deposited by spectators in the STAR Zero Degree Calorimeters (ZDCs). Within this sample, the observed dependence of v_2\{2\} on multiplicity demonstrates that ZDC information combined with multiplicity can preferentially select different overlap configurations in U+U collisions. An initial-state model with gluon saturation describes the slope of v_2\{2\} as a function of multiplicity in central collisions better than one based on Glauber with a two-component multiplicity model. Nuclear Experiment Nuclear Theory Adamczyk, L oth Adkins, J. K oth Agakishiev, G oth Aggarwal, M. M oth Ahammed, Z oth Alekseev, I oth Alford, J oth Aparin, A oth Arkhipkin, D oth Aschenauer, E. C oth Averichev, G. S oth Bairathi, V oth Banerjee, A oth Bellwied, R oth Bhasin, A oth Bhati, A. K oth Bhattarai, P oth Bielcik, J oth Bielcikova, J oth Bland, L. C oth Bordyuzhin, I. G oth Bouchet, J oth Brandin, A. V oth Bunzarov, I oth Butterworth, J oth Caines, H oth Sánchez, M. Calderón de la Barca oth Campbell, J. M oth Cebra, D oth Cervantes, M. C oth Chakaberia, I oth Chaloupka, P oth Chang, Z oth Chattopadhyay, S oth Chen, J. H oth Chen, X oth Cheng, J oth Cherney, M oth Christie, W oth Contin, G oth Crawford, H. J oth Das, S oth De Silva, L. C oth Debbe, R. R oth Dedovich, T. G oth Deng, J oth Derevschikov, A. A oth di Ruzza, B oth Didenko, L oth Dilks, C oth Dong, X oth Drachenberg, J. L oth Draper, J. E oth Du, C. M oth Dunkelberger, L. E oth Dunlop, J. C oth Efimov, L. G oth Engelage, J oth Eppley, G oth Esha, R oth Evdokimov, O oth Eyser, O oth Fatemi, R oth Fazio, S oth Federic, P oth Fedorisin, J oth Feng, Z oth Filip, P oth Fisyak, Y oth Flores, C. E oth Fulek, L oth Gagliardi, C. A oth Garand, D oth Geurts, F oth Gibson, A oth Girard, M oth Greiner, L oth Grosnick, D oth Gunarathne, D. S oth Guo, Y oth Gupta, A oth Gupta, S oth Guryn, W oth Hamad, A oth Hamed, A oth Haque, R oth Harris, J. W oth He, L oth Heppelmann, S oth Hirsch, A oth Hoffmann, G. W oth Hofman, D. J oth Horvat, S oth Huang, B oth Huang, H. Z oth Huang, X oth Huck, P oth Humanic, T. J oth Igo, G oth ... oth Enthalten in Physical review letters Ridge, NY : American Physical Society, 1958 (2015) (DE-627)129503959 (DE-600)208853-8 (DE-576)014907267 0031-9007 nnns year:2015 http://dx.doi.org/10.1103/PhysRevLett.115.222301 Volltext http://arxiv.org/abs/1505.07812 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2004 GBV_ILN_2016 GBV_ILN_2095 GBV_ILN_2192 GBV_ILN_2279 GBV_ILN_2286 UA 1000 AR 2015 |
| spelling |
10.1103/PhysRevLett.115.222301 doi PQ20160211 (DE-627)OLC1969289252 (DE-599)GBVOLC1969289252 (PRQ)a622-afab5778867cb7da8afc709bc9e548cddcddfeaa6f94015286d568d757cdbeb40 (KEY)0009201020150000000000000000azimuthalanisotropyinuuandauaucollisionsatrhic DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk STAR Collaboration verfasserin aut Azimuthal anisotropy in U+U and Au+Au collisions at RHIC 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Collisions between prolate uranium nuclei are used to study how particle production and azimuthal anisotropies depend on initial geometry in heavy-ion collisions. We report the two- and four-particle cumulants, v_2\{2\} and v_2\{4\}, for charged hadrons from U+U collisions at \sqrt{s_{\rm NN}} = 193 GeV and Au+Au collisions at \sqrt{s_{\rm NN}} = 200 GeV. Nearly fully overlapping collisions are selected based on the amount of energy deposited by spectators in the STAR Zero Degree Calorimeters (ZDCs). Within this sample, the observed dependence of v_2\{2\} on multiplicity demonstrates that ZDC information combined with multiplicity can preferentially select different overlap configurations in U+U collisions. An initial-state model with gluon saturation describes the slope of v_2\{2\} as a function of multiplicity in central collisions better than one based on Glauber with a two-component multiplicity model. Nuclear Experiment Nuclear Theory Adamczyk, L oth Adkins, J. K oth Agakishiev, G oth Aggarwal, M. M oth Ahammed, Z oth Alekseev, I oth Alford, J oth Aparin, A oth Arkhipkin, D oth Aschenauer, E. C oth Averichev, G. S oth Bairathi, V oth Banerjee, A oth Bellwied, R oth Bhasin, A oth Bhati, A. K oth Bhattarai, P oth Bielcik, J oth Bielcikova, J oth Bland, L. C oth Bordyuzhin, I. G oth Bouchet, J oth Brandin, A. V oth Bunzarov, I oth Butterworth, J oth Caines, H oth Sánchez, M. Calderón de la Barca oth Campbell, J. M oth Cebra, D oth Cervantes, M. C oth Chakaberia, I oth Chaloupka, P oth Chang, Z oth Chattopadhyay, S oth Chen, J. H oth Chen, X oth Cheng, J oth Cherney, M oth Christie, W oth Contin, G oth Crawford, H. J oth Das, S oth De Silva, L. C oth Debbe, R. R oth Dedovich, T. G oth Deng, J oth Derevschikov, A. A oth di Ruzza, B oth Didenko, L oth Dilks, C oth Dong, X oth Drachenberg, J. L oth Draper, J. E oth Du, C. M oth Dunkelberger, L. E oth Dunlop, J. C oth Efimov, L. G oth Engelage, J oth Eppley, G oth Esha, R oth Evdokimov, O oth Eyser, O oth Fatemi, R oth Fazio, S oth Federic, P oth Fedorisin, J oth Feng, Z oth Filip, P oth Fisyak, Y oth Flores, C. E oth Fulek, L oth Gagliardi, C. A oth Garand, D oth Geurts, F oth Gibson, A oth Girard, M oth Greiner, L oth Grosnick, D oth Gunarathne, D. S oth Guo, Y oth Gupta, A oth Gupta, S oth Guryn, W oth Hamad, A oth Hamed, A oth Haque, R oth Harris, J. W oth He, L oth Heppelmann, S oth Hirsch, A oth Hoffmann, G. W oth Hofman, D. J oth Horvat, S oth Huang, B oth Huang, H. Z oth Huang, X oth Huck, P oth Humanic, T. J oth Igo, G oth ... oth Enthalten in Physical review letters Ridge, NY : American Physical Society, 1958 (2015) (DE-627)129503959 (DE-600)208853-8 (DE-576)014907267 0031-9007 nnns year:2015 http://dx.doi.org/10.1103/PhysRevLett.115.222301 Volltext http://arxiv.org/abs/1505.07812 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2004 GBV_ILN_2016 GBV_ILN_2095 GBV_ILN_2192 GBV_ILN_2279 GBV_ILN_2286 UA 1000 AR 2015 |
| allfields_unstemmed |
10.1103/PhysRevLett.115.222301 doi PQ20160211 (DE-627)OLC1969289252 (DE-599)GBVOLC1969289252 (PRQ)a622-afab5778867cb7da8afc709bc9e548cddcddfeaa6f94015286d568d757cdbeb40 (KEY)0009201020150000000000000000azimuthalanisotropyinuuandauaucollisionsatrhic DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk STAR Collaboration verfasserin aut Azimuthal anisotropy in U+U and Au+Au collisions at RHIC 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Collisions between prolate uranium nuclei are used to study how particle production and azimuthal anisotropies depend on initial geometry in heavy-ion collisions. We report the two- and four-particle cumulants, v_2\{2\} and v_2\{4\}, for charged hadrons from U+U collisions at \sqrt{s_{\rm NN}} = 193 GeV and Au+Au collisions at \sqrt{s_{\rm NN}} = 200 GeV. Nearly fully overlapping collisions are selected based on the amount of energy deposited by spectators in the STAR Zero Degree Calorimeters (ZDCs). Within this sample, the observed dependence of v_2\{2\} on multiplicity demonstrates that ZDC information combined with multiplicity can preferentially select different overlap configurations in U+U collisions. An initial-state model with gluon saturation describes the slope of v_2\{2\} as a function of multiplicity in central collisions better than one based on Glauber with a two-component multiplicity model. Nuclear Experiment Nuclear Theory Adamczyk, L oth Adkins, J. K oth Agakishiev, G oth Aggarwal, M. M oth Ahammed, Z oth Alekseev, I oth Alford, J oth Aparin, A oth Arkhipkin, D oth Aschenauer, E. C oth Averichev, G. S oth Bairathi, V oth Banerjee, A oth Bellwied, R oth Bhasin, A oth Bhati, A. K oth Bhattarai, P oth Bielcik, J oth Bielcikova, J oth Bland, L. C oth Bordyuzhin, I. G oth Bouchet, J oth Brandin, A. V oth Bunzarov, I oth Butterworth, J oth Caines, H oth Sánchez, M. Calderón de la Barca oth Campbell, J. M oth Cebra, D oth Cervantes, M. C oth Chakaberia, I oth Chaloupka, P oth Chang, Z oth Chattopadhyay, S oth Chen, J. H oth Chen, X oth Cheng, J oth Cherney, M oth Christie, W oth Contin, G oth Crawford, H. J oth Das, S oth De Silva, L. C oth Debbe, R. R oth Dedovich, T. G oth Deng, J oth Derevschikov, A. A oth di Ruzza, B oth Didenko, L oth Dilks, C oth Dong, X oth Drachenberg, J. L oth Draper, J. E oth Du, C. M oth Dunkelberger, L. E oth Dunlop, J. C oth Efimov, L. G oth Engelage, J oth Eppley, G oth Esha, R oth Evdokimov, O oth Eyser, O oth Fatemi, R oth Fazio, S oth Federic, P oth Fedorisin, J oth Feng, Z oth Filip, P oth Fisyak, Y oth Flores, C. E oth Fulek, L oth Gagliardi, C. A oth Garand, D oth Geurts, F oth Gibson, A oth Girard, M oth Greiner, L oth Grosnick, D oth Gunarathne, D. S oth Guo, Y oth Gupta, A oth Gupta, S oth Guryn, W oth Hamad, A oth Hamed, A oth Haque, R oth Harris, J. W oth He, L oth Heppelmann, S oth Hirsch, A oth Hoffmann, G. W oth Hofman, D. J oth Horvat, S oth Huang, B oth Huang, H. Z oth Huang, X oth Huck, P oth Humanic, T. J oth Igo, G oth ... oth Enthalten in Physical review letters Ridge, NY : American Physical Society, 1958 (2015) (DE-627)129503959 (DE-600)208853-8 (DE-576)014907267 0031-9007 nnns year:2015 http://dx.doi.org/10.1103/PhysRevLett.115.222301 Volltext http://arxiv.org/abs/1505.07812 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2004 GBV_ILN_2016 GBV_ILN_2095 GBV_ILN_2192 GBV_ILN_2279 GBV_ILN_2286 UA 1000 AR 2015 |
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10.1103/PhysRevLett.115.222301 doi PQ20160211 (DE-627)OLC1969289252 (DE-599)GBVOLC1969289252 (PRQ)a622-afab5778867cb7da8afc709bc9e548cddcddfeaa6f94015286d568d757cdbeb40 (KEY)0009201020150000000000000000azimuthalanisotropyinuuandauaucollisionsatrhic DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk STAR Collaboration verfasserin aut Azimuthal anisotropy in U+U and Au+Au collisions at RHIC 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Collisions between prolate uranium nuclei are used to study how particle production and azimuthal anisotropies depend on initial geometry in heavy-ion collisions. We report the two- and four-particle cumulants, v_2\{2\} and v_2\{4\}, for charged hadrons from U+U collisions at \sqrt{s_{\rm NN}} = 193 GeV and Au+Au collisions at \sqrt{s_{\rm NN}} = 200 GeV. Nearly fully overlapping collisions are selected based on the amount of energy deposited by spectators in the STAR Zero Degree Calorimeters (ZDCs). Within this sample, the observed dependence of v_2\{2\} on multiplicity demonstrates that ZDC information combined with multiplicity can preferentially select different overlap configurations in U+U collisions. An initial-state model with gluon saturation describes the slope of v_2\{2\} as a function of multiplicity in central collisions better than one based on Glauber with a two-component multiplicity model. Nuclear Experiment Nuclear Theory Adamczyk, L oth Adkins, J. K oth Agakishiev, G oth Aggarwal, M. M oth Ahammed, Z oth Alekseev, I oth Alford, J oth Aparin, A oth Arkhipkin, D oth Aschenauer, E. C oth Averichev, G. S oth Bairathi, V oth Banerjee, A oth Bellwied, R oth Bhasin, A oth Bhati, A. K oth Bhattarai, P oth Bielcik, J oth Bielcikova, J oth Bland, L. C oth Bordyuzhin, I. G oth Bouchet, J oth Brandin, A. V oth Bunzarov, I oth Butterworth, J oth Caines, H oth Sánchez, M. Calderón de la Barca oth Campbell, J. M oth Cebra, D oth Cervantes, M. C oth Chakaberia, I oth Chaloupka, P oth Chang, Z oth Chattopadhyay, S oth Chen, J. H oth Chen, X oth Cheng, J oth Cherney, M oth Christie, W oth Contin, G oth Crawford, H. J oth Das, S oth De Silva, L. C oth Debbe, R. R oth Dedovich, T. G oth Deng, J oth Derevschikov, A. A oth di Ruzza, B oth Didenko, L oth Dilks, C oth Dong, X oth Drachenberg, J. L oth Draper, J. E oth Du, C. M oth Dunkelberger, L. E oth Dunlop, J. C oth Efimov, L. G oth Engelage, J oth Eppley, G oth Esha, R oth Evdokimov, O oth Eyser, O oth Fatemi, R oth Fazio, S oth Federic, P oth Fedorisin, J oth Feng, Z oth Filip, P oth Fisyak, Y oth Flores, C. E oth Fulek, L oth Gagliardi, C. A oth Garand, D oth Geurts, F oth Gibson, A oth Girard, M oth Greiner, L oth Grosnick, D oth Gunarathne, D. S oth Guo, Y oth Gupta, A oth Gupta, S oth Guryn, W oth Hamad, A oth Hamed, A oth Haque, R oth Harris, J. W oth He, L oth Heppelmann, S oth Hirsch, A oth Hoffmann, G. W oth Hofman, D. J oth Horvat, S oth Huang, B oth Huang, H. Z oth Huang, X oth Huck, P oth Humanic, T. J oth Igo, G oth ... oth Enthalten in Physical review letters Ridge, NY : American Physical Society, 1958 (2015) (DE-627)129503959 (DE-600)208853-8 (DE-576)014907267 0031-9007 nnns year:2015 http://dx.doi.org/10.1103/PhysRevLett.115.222301 Volltext http://arxiv.org/abs/1505.07812 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2004 GBV_ILN_2016 GBV_ILN_2095 GBV_ILN_2192 GBV_ILN_2279 GBV_ILN_2286 UA 1000 AR 2015 |
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10.1103/PhysRevLett.115.222301 doi PQ20160211 (DE-627)OLC1969289252 (DE-599)GBVOLC1969289252 (PRQ)a622-afab5778867cb7da8afc709bc9e548cddcddfeaa6f94015286d568d757cdbeb40 (KEY)0009201020150000000000000000azimuthalanisotropyinuuandauaucollisionsatrhic DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk STAR Collaboration verfasserin aut Azimuthal anisotropy in U+U and Au+Au collisions at RHIC 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Collisions between prolate uranium nuclei are used to study how particle production and azimuthal anisotropies depend on initial geometry in heavy-ion collisions. We report the two- and four-particle cumulants, v_2\{2\} and v_2\{4\}, for charged hadrons from U+U collisions at \sqrt{s_{\rm NN}} = 193 GeV and Au+Au collisions at \sqrt{s_{\rm NN}} = 200 GeV. Nearly fully overlapping collisions are selected based on the amount of energy deposited by spectators in the STAR Zero Degree Calorimeters (ZDCs). Within this sample, the observed dependence of v_2\{2\} on multiplicity demonstrates that ZDC information combined with multiplicity can preferentially select different overlap configurations in U+U collisions. An initial-state model with gluon saturation describes the slope of v_2\{2\} as a function of multiplicity in central collisions better than one based on Glauber with a two-component multiplicity model. Nuclear Experiment Nuclear Theory Adamczyk, L oth Adkins, J. K oth Agakishiev, G oth Aggarwal, M. M oth Ahammed, Z oth Alekseev, I oth Alford, J oth Aparin, A oth Arkhipkin, D oth Aschenauer, E. C oth Averichev, G. S oth Bairathi, V oth Banerjee, A oth Bellwied, R oth Bhasin, A oth Bhati, A. K oth Bhattarai, P oth Bielcik, J oth Bielcikova, J oth Bland, L. C oth Bordyuzhin, I. G oth Bouchet, J oth Brandin, A. V oth Bunzarov, I oth Butterworth, J oth Caines, H oth Sánchez, M. Calderón de la Barca oth Campbell, J. M oth Cebra, D oth Cervantes, M. C oth Chakaberia, I oth Chaloupka, P oth Chang, Z oth Chattopadhyay, S oth Chen, J. H oth Chen, X oth Cheng, J oth Cherney, M oth Christie, W oth Contin, G oth Crawford, H. J oth Das, S oth De Silva, L. C oth Debbe, R. R oth Dedovich, T. G oth Deng, J oth Derevschikov, A. A oth di Ruzza, B oth Didenko, L oth Dilks, C oth Dong, X oth Drachenberg, J. L oth Draper, J. E oth Du, C. M oth Dunkelberger, L. E oth Dunlop, J. C oth Efimov, L. G oth Engelage, J oth Eppley, G oth Esha, R oth Evdokimov, O oth Eyser, O oth Fatemi, R oth Fazio, S oth Federic, P oth Fedorisin, J oth Feng, Z oth Filip, P oth Fisyak, Y oth Flores, C. E oth Fulek, L oth Gagliardi, C. A oth Garand, D oth Geurts, F oth Gibson, A oth Girard, M oth Greiner, L oth Grosnick, D oth Gunarathne, D. S oth Guo, Y oth Gupta, A oth Gupta, S oth Guryn, W oth Hamad, A oth Hamed, A oth Haque, R oth Harris, J. W oth He, L oth Heppelmann, S oth Hirsch, A oth Hoffmann, G. W oth Hofman, D. J oth Horvat, S oth Huang, B oth Huang, H. Z oth Huang, X oth Huck, P oth Humanic, T. J oth Igo, G oth ... oth Enthalten in Physical review letters Ridge, NY : American Physical Society, 1958 (2015) (DE-627)129503959 (DE-600)208853-8 (DE-576)014907267 0031-9007 nnns year:2015 http://dx.doi.org/10.1103/PhysRevLett.115.222301 Volltext http://arxiv.org/abs/1505.07812 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2004 GBV_ILN_2016 GBV_ILN_2095 GBV_ILN_2192 GBV_ILN_2279 GBV_ILN_2286 UA 1000 AR 2015 |
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STAR Collaboration @@aut@@ Adamczyk, L @@oth@@ Adkins, J. K @@oth@@ Agakishiev, G @@oth@@ Aggarwal, M. M @@oth@@ Ahammed, Z @@oth@@ Alekseev, I @@oth@@ Alford, J @@oth@@ Aparin, A @@oth@@ Arkhipkin, D @@oth@@ Aschenauer, E. C @@oth@@ Averichev, G. S @@oth@@ Bairathi, V @@oth@@ Banerjee, A @@oth@@ Bellwied, R @@oth@@ Bhasin, A @@oth@@ Bhati, A. K @@oth@@ Bhattarai, P @@oth@@ Bielcik, J @@oth@@ Bielcikova, J @@oth@@ Bland, L. C @@oth@@ Bordyuzhin, I. G @@oth@@ Bouchet, J @@oth@@ Brandin, A. V @@oth@@ Bunzarov, I @@oth@@ Butterworth, J @@oth@@ Caines, H @@oth@@ Sánchez, M. Calderón de la Barca @@oth@@ Campbell, J. M @@oth@@ Cebra, D @@oth@@ Cervantes, M. C @@oth@@ Chakaberia, I @@oth@@ Chaloupka, P @@oth@@ Chang, Z @@oth@@ Chattopadhyay, S @@oth@@ Chen, J. H @@oth@@ Chen, X @@oth@@ Cheng, J @@oth@@ Cherney, M @@oth@@ Christie, W @@oth@@ Contin, G @@oth@@ Crawford, H. J @@oth@@ Das, S @@oth@@ De Silva, L. C @@oth@@ Debbe, R. R @@oth@@ Dedovich, T. G @@oth@@ Deng, J @@oth@@ Derevschikov, A. A @@oth@@ di Ruzza, B @@oth@@ Didenko, L @@oth@@ Dilks, C @@oth@@ Dong, X @@oth@@ Drachenberg, J. L @@oth@@ Draper, J. E @@oth@@ Du, C. M @@oth@@ Dunkelberger, L. E @@oth@@ Dunlop, J. C @@oth@@ Efimov, L. G @@oth@@ Engelage, J @@oth@@ Eppley, G @@oth@@ Esha, R @@oth@@ Evdokimov, O @@oth@@ Eyser, O @@oth@@ Fatemi, R @@oth@@ Fazio, S @@oth@@ Federic, P @@oth@@ Fedorisin, J @@oth@@ Feng, Z @@oth@@ Filip, P @@oth@@ Fisyak, Y @@oth@@ Flores, C. E @@oth@@ Fulek, L @@oth@@ Gagliardi, C. A @@oth@@ Garand, D @@oth@@ Geurts, F @@oth@@ Gibson, A @@oth@@ Girard, M @@oth@@ Greiner, L @@oth@@ Grosnick, D @@oth@@ Gunarathne, D. S @@oth@@ Guo, Y @@oth@@ Gupta, A @@oth@@ Gupta, S @@oth@@ Guryn, W @@oth@@ Hamad, A @@oth@@ Hamed, A @@oth@@ Haque, R @@oth@@ Harris, J. W @@oth@@ He, L @@oth@@ Heppelmann, S @@oth@@ Hirsch, A @@oth@@ Hoffmann, G. W @@oth@@ Hofman, D. J @@oth@@ Horvat, S @@oth@@ Huang, B @@oth@@ Huang, H. Z @@oth@@ Huang, X @@oth@@ Huck, P @@oth@@ Humanic, T. J @@oth@@ Igo, G @@oth@@ ... @@oth@@ |
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Azimuthal anisotropy in U+U and Au+Au collisions at RHIC |
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Azimuthal anisotropy in U+U and Au+Au collisions at RHIC |
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Collisions between prolate uranium nuclei are used to study how particle production and azimuthal anisotropies depend on initial geometry in heavy-ion collisions. We report the two- and four-particle cumulants, v_2\{2\} and v_2\{4\}, for charged hadrons from U+U collisions at \sqrt{s_{\rm NN}} = 193 GeV and Au+Au collisions at \sqrt{s_{\rm NN}} = 200 GeV. Nearly fully overlapping collisions are selected based on the amount of energy deposited by spectators in the STAR Zero Degree Calorimeters (ZDCs). Within this sample, the observed dependence of v_2\{2\} on multiplicity demonstrates that ZDC information combined with multiplicity can preferentially select different overlap configurations in U+U collisions. An initial-state model with gluon saturation describes the slope of v_2\{2\} as a function of multiplicity in central collisions better than one based on Glauber with a two-component multiplicity model. |
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Collisions between prolate uranium nuclei are used to study how particle production and azimuthal anisotropies depend on initial geometry in heavy-ion collisions. We report the two- and four-particle cumulants, v_2\{2\} and v_2\{4\}, for charged hadrons from U+U collisions at \sqrt{s_{\rm NN}} = 193 GeV and Au+Au collisions at \sqrt{s_{\rm NN}} = 200 GeV. Nearly fully overlapping collisions are selected based on the amount of energy deposited by spectators in the STAR Zero Degree Calorimeters (ZDCs). Within this sample, the observed dependence of v_2\{2\} on multiplicity demonstrates that ZDC information combined with multiplicity can preferentially select different overlap configurations in U+U collisions. An initial-state model with gluon saturation describes the slope of v_2\{2\} as a function of multiplicity in central collisions better than one based on Glauber with a two-component multiplicity model. |
| abstract_unstemmed |
Collisions between prolate uranium nuclei are used to study how particle production and azimuthal anisotropies depend on initial geometry in heavy-ion collisions. We report the two- and four-particle cumulants, v_2\{2\} and v_2\{4\}, for charged hadrons from U+U collisions at \sqrt{s_{\rm NN}} = 193 GeV and Au+Au collisions at \sqrt{s_{\rm NN}} = 200 GeV. Nearly fully overlapping collisions are selected based on the amount of energy deposited by spectators in the STAR Zero Degree Calorimeters (ZDCs). Within this sample, the observed dependence of v_2\{2\} on multiplicity demonstrates that ZDC information combined with multiplicity can preferentially select different overlap configurations in U+U collisions. An initial-state model with gluon saturation describes the slope of v_2\{2\} as a function of multiplicity in central collisions better than one based on Glauber with a two-component multiplicity model. |
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Azimuthal anisotropy in U+U and Au+Au collisions at RHIC |
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Adamczyk, L Adkins, J. K Agakishiev, G Aggarwal, M. M Ahammed, Z Alekseev, I Alford, J Aparin, A Arkhipkin, D Aschenauer, E. C Averichev, G. S Bairathi, V Banerjee, A Bellwied, R Bhasin, A Bhati, A. K Bhattarai, P Bielcik, J Bielcikova, J Bland, L. C Bordyuzhin, I. G Bouchet, J Brandin, A. V Bunzarov, I Butterworth, J Caines, H Sánchez, M. Calderón de la Barca Campbell, J. M Cebra, D Cervantes, M. C Chakaberia, I Chaloupka, P Chang, Z Chattopadhyay, S Chen, J. H Chen, X Cheng, J Cherney, M Christie, W Contin, G Crawford, H. J Das, S De Silva, L. C Debbe, R. R Dedovich, T. G Deng, J Derevschikov, A. A di Ruzza, B Didenko, L Dilks, C Dong, X Drachenberg, J. L Draper, J. E Du, C. M Dunkelberger, L. E Dunlop, J. C Efimov, L. G Engelage, J Eppley, G Esha, R Evdokimov, O Eyser, O Fatemi, R Fazio, S Federic, P Fedorisin, J Feng, Z Filip, P Fisyak, Y Flores, C. E Fulek, L Gagliardi, C. A Garand, D Geurts, F Gibson, A Girard, M Greiner, L Grosnick, D Gunarathne, D. S Guo, Y Gupta, A Gupta, S Guryn, W Hamad, A Hamed, A Haque, R Harris, J. W He, L Heppelmann, S Hirsch, A Hoffmann, G. W Hofman, D. J Horvat, S Huang, B Huang, H. Z Huang, X Huck, P Humanic, T. J Igo, G . |
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Adamczyk, L Adkins, J. K Agakishiev, G Aggarwal, M. M Ahammed, Z Alekseev, I Alford, J Aparin, A Arkhipkin, D Aschenauer, E. C Averichev, G. S Bairathi, V Banerjee, A Bellwied, R Bhasin, A Bhati, A. K Bhattarai, P Bielcik, J Bielcikova, J Bland, L. C Bordyuzhin, I. G Bouchet, J Brandin, A. V Bunzarov, I Butterworth, J Caines, H Sánchez, M. Calderón de la Barca Campbell, J. M Cebra, D Cervantes, M. C Chakaberia, I Chaloupka, P Chang, Z Chattopadhyay, S Chen, J. H Chen, X Cheng, J Cherney, M Christie, W Contin, G Crawford, H. J Das, S De Silva, L. C Debbe, R. R Dedovich, T. G Deng, J Derevschikov, A. A di Ruzza, B Didenko, L Dilks, C Dong, X Drachenberg, J. L Draper, J. E Du, C. M Dunkelberger, L. E Dunlop, J. C Efimov, L. G Engelage, J Eppley, G Esha, R Evdokimov, O Eyser, O Fatemi, R Fazio, S Federic, P Fedorisin, J Feng, Z Filip, P Fisyak, Y Flores, C. E Fulek, L Gagliardi, C. A Garand, D Geurts, F Gibson, A Girard, M Greiner, L Grosnick, D Gunarathne, D. S Guo, Y Gupta, A Gupta, S Guryn, W Hamad, A Hamed, A Haque, R Harris, J. W He, L Heppelmann, S Hirsch, A Hoffmann, G. W Hofman, D. J Horvat, S Huang, B Huang, H. Z Huang, X Huck, P Humanic, T. J Igo, G . |
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