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Global polarization of Λ and Λ¯ hyperons in Au+Au collisions at √sNN = 19.6 and 27 GeV

Abdulhamid, M. I. ; Galatyuk, Tetyana ; Harabasz, Szymon ; Seck, Florian
Hrsg.: STAR Collaboration (2023)
Global polarization of Λ and Λ¯ hyperons in Au+Au collisions at √sNN = 19.6 and 27 GeV.
In: Physical Review C, 108 (1)
doi: 10.1103/PhysRevC.108.014910
Artikel, Bibliographie

Kurzbeschreibung (Abstract)

In relativistic heavy-ion collisions, a global spin polarization, PH, of Λ and ¯Λ hyperons along the direction of the system angular momentum was discovered and measured across a broad range of collision energies and demonstrated a trend of increasing PH with decreasing √sNN. A splitting between Λ and ¯Λ polarization may be possible due to their different magnetic moments in a late-stage magnetic field sustained by the quark-gluon plasma which is formed in the collision. The results presented in this study find no significant splitting at the collision energies of √sNN=19.6 and 27 GeV in the BNL Relativistic Heavy Ion Collisions Beam Energy Scan Phase II using the STAR detector, with an upper limit of P¯Λ−PΛ<0.24% and P¯Λ−PΛ<0.35%, respectively, at a 95% confidence level. We derive an upper limit on the naive extraction of the late-stage magnetic field of B<9.4×1012 T and B<1.4×1013 T at √sNN=19.6 and 27 GeV, respectively, although more thorough derivations are needed. Differential measurements of PH were performed with respect to collision centrality, transverse momentum, and rapidity. With our current acceptance of |y|<1 and uncertainties, we observe no dependence on transverse momentum and rapidity in this analysis. These results challenge multiple existing model calculations following a variety of different assumptions which have each predicted a strong dependence on rapidity in this collision-energy range.

Typ des Eintrags: Artikel
Erschienen: 2023
Autor(en): Abdulhamid, M. I. ; Galatyuk, Tetyana ; Harabasz, Szymon ; Seck, Florian
Art des Eintrags: Bibliographie
Titel: Global polarization of Λ and Λ¯ hyperons in Au+Au collisions at √sNN = 19.6 and 27 GeV
Sprache: Deutsch
Publikationsjahr: 27 Juli 2023
Verlag: APS
Titel der Zeitschrift, Zeitung oder Schriftenreihe: Physical Review C
Jahrgang/Volume einer Zeitschrift: 108
(Heft-)Nummer: 1
DOI: 10.1103/PhysRevC.108.014910
Kurzbeschreibung (Abstract):

In relativistic heavy-ion collisions, a global spin polarization, PH, of Λ and ¯Λ hyperons along the direction of the system angular momentum was discovered and measured across a broad range of collision energies and demonstrated a trend of increasing PH with decreasing √sNN. A splitting between Λ and ¯Λ polarization may be possible due to their different magnetic moments in a late-stage magnetic field sustained by the quark-gluon plasma which is formed in the collision. The results presented in this study find no significant splitting at the collision energies of √sNN=19.6 and 27 GeV in the BNL Relativistic Heavy Ion Collisions Beam Energy Scan Phase II using the STAR detector, with an upper limit of P¯Λ−PΛ<0.24% and P¯Λ−PΛ<0.35%, respectively, at a 95% confidence level. We derive an upper limit on the naive extraction of the late-stage magnetic field of B<9.4×1012 T and B<1.4×1013 T at √sNN=19.6 and 27 GeV, respectively, although more thorough derivations are needed. Differential measurements of PH were performed with respect to collision centrality, transverse momentum, and rapidity. With our current acceptance of |y|<1 and uncertainties, we observe no dependence on transverse momentum and rapidity in this analysis. These results challenge multiple existing model calculations following a variety of different assumptions which have each predicted a strong dependence on rapidity in this collision-energy range.

Zusätzliche Informationen:

Art.No.: 014910

Fachbereich(e)/-gebiet(e): 05 Fachbereich Physik
05 Fachbereich Physik > Institut für Kernphysik
05 Fachbereich Physik > Institut für Kernphysik > Experimentelle Kernphysik
05 Fachbereich Physik > Institut für Kernphysik > Experimentelle Kernphysik > Untersuchung von Quark-Materie mit virtuellen Photonen
Hinterlegungsdatum: 09 Nov 2023 12:04
Letzte Änderung: 15 Dez 2023 10:03
PPN: 514117362
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