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Pregled bibliografske jedinice broj: 1184046

Kinematic dependence of azimuthal anisotropies in p+Au, d+Au, and He3+Au at sqrt(s)_NN=200GeV


(PHENIX Collaboration) Acharya U.A.; ...; Dumančić, Mirta; ...; Makek, Mihael; ...; Vukman, Nikola; ...; Zou, L.
Kinematic dependence of azimuthal anisotropies in p+Au, d+Au, and He3+Au at sqrt(s)_NN=200GeV // Physical review. C, 105 (2022), 2; 024901, 13 doi:10.1103/physrevc.105.024901 (međunarodna recenzija, članak, znanstveni)


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Naslov
Kinematic dependence of azimuthal anisotropies in p+Au, d+Au, and He3+Au at sqrt(s)_NN=200GeV

Autori
Acharya U.A. ; ... ; Dumančić, Mirta ; ... ; Makek, Mihael ; ... ; Vukman, Nikola ; ... ; Zou, L.

Kolaboracija
PHENIX Collaboration

Izvornik
Physical review. C (2469-9985) 105 (2022), 2; 024901, 13

Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni

Ključne riječi
Anisotropy ; p+Au ; d+Au ; He3+Au ; 200 GeV ; PHENIX ; RHIC

Sažetak
There is strong evidence for the formation of small droplets of quark-gluon plasma in p/d/He3+Au collisions at the Relativistic Heavy Ion Collider (RHIC) and in p+p/Pb collisions at the Large Hadron Collider. In particular, the analysis of data at RHIC for different geometries obtained by varying the projectile size and shape has proved insightful. In the present analysis, we find excellent agreement with the previously published PHENIX at RHIC results on elliptical and triangular flow with an independent analysis via the two-particle correlation method, which has quite different systematic uncertainties and an independent code base. In addition, the results are extended to other detector combinations with different kinematic (pseudorapidity) coverage. These results provide additional constraints on contributions from nonflow and longitudinal decorrelations.

Izvorni jezik
Engleski

Znanstvena područja
Fizika



POVEZANOST RADA


Ustanove:
Prirodoslovno-matematički fakultet, Zagreb

Profili:

Avatar Url Nikola Vukman (autor)

Avatar Url Mihael Makek (autor)

Poveznice na cjeloviti tekst rada:

doi arxiv.org journals.aps.org

Citiraj ovu publikaciju:

(PHENIX Collaboration) Acharya U.A.; ...; Dumančić, Mirta; ...; Makek, Mihael; ...; Vukman, Nikola; ...; Zou, L.
Kinematic dependence of azimuthal anisotropies in p+Au, d+Au, and He3+Au at sqrt(s)_NN=200GeV // Physical review. C, 105 (2022), 2; 024901, 13 doi:10.1103/physrevc.105.024901 (međunarodna recenzija, članak, znanstveni)
(PHENIX Collaboration) (PHENIX Collaboration) Acharya U.A., ..., Dumančić, M., ..., Makek, M., ..., Vukman, N., ... & Zou, L. (2022) Kinematic dependence of azimuthal anisotropies in p+Au, d+Au, and He3+Au at sqrt(s)_NN=200GeV. Physical review. C, 105 (2), 024901, 13 doi:10.1103/physrevc.105.024901.
@article{article, author = {Duman\v{c}i\'{c}, Mirta and Makek, Mihael and Vukman, Nikola and Zou, L.}, year = {2022}, pages = {13}, DOI = {10.1103/physrevc.105.024901}, chapter = {024901}, keywords = {Anisotropy, p+Au, d+Au, He3+Au, 200 GeV, PHENIX, RHIC}, journal = {Physical review. C}, doi = {10.1103/physrevc.105.024901}, volume = {105}, number = {2}, issn = {2469-9985}, title = {Kinematic dependence of azimuthal anisotropies in p+Au, d+Au, and He3+Au at sqrt(s)\_NN=200GeV}, keyword = {Anisotropy, p+Au, d+Au, He3+Au, 200 GeV, PHENIX, RHIC}, chapternumber = {024901} }
@article{article, author = {Duman\v{c}i\'{c}, Mirta and Makek, Mihael and Vukman, Nikola and Zou, L.}, year = {2022}, pages = {13}, DOI = {10.1103/physrevc.105.024901}, chapter = {024901}, keywords = {Anisotropy, p+Au, d+Au, He3+Au, 200 GeV, PHENIX, RHIC}, journal = {Physical review. C}, doi = {10.1103/physrevc.105.024901}, volume = {105}, number = {2}, issn = {2469-9985}, title = {Kinematic dependence of azimuthal anisotropies in p+Au, d+Au, and He3+Au at sqrt(s)\_NN=200GeV}, keyword = {Anisotropy, p+Au, d+Au, He3+Au, 200 GeV, PHENIX, RHIC}, chapternumber = {024901} }

Časopis indeksira:


  • Current Contents Connect (CCC)
  • Web of Science Core Collection (WoSCC)
    • Science Citation Index Expanded (SCI-EXP)
    • SCI-EXP, SSCI i/ili A&HCI
  • Scopus


Citati:





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