Indirect Observation of an In-Medium η Mass Reduction in sNN=200GeV Au+Au Collisions

T. Csörgő, R. Vértesi, and J. Sziklai
Phys. Rev. Lett. 105, 182301 – Published 25 October 2010

Abstract

PHENIX Collaboration and STAR Collaboration data on the intercept parameter of the two-pion Bose-Einstein correlation functions in sNN=200GeV Au+Au collisions are analyzed in terms of different models of hadronic multiplicities. To describe this combined PHENIX and STAR data set, an in-medium η mass reduction of at least 200 MeV is needed, at the 99.9% confidence level in the considered model class. Such a significant η mass modification may indicate the restoration of the UA(1) symmetry in a hot and dense hadronic matter and the return of the 9th “prodigal” Goldstone boson.

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  • Received 31 December 2009

DOI:https://doi.org/10.1103/PhysRevLett.105.182301

© 2010 The American Physical Society

Authors & Affiliations

T. Csörgő

  • Department of Physics, Harvard University, 17 Oxford Street, Cambridge, Massachusetts 02138, USA and MTA KFKI RMKI, H–1525 Budapest 114, P.O. Box 49, Hungary

R. Vértesi and J. Sziklai

  • MTA KFKI RMKI, H–1525 Budapest 114, P.O. Box 49, Hungary

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Vol. 105, Iss. 18 — 29 October 2010

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