Possible origin of RHIC Rout/Rsid HBT results

Padula, Sandra S.

Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/67230

Title:

Possible origin of RHIC Rout/Rsid HBT results

Author(s):

Padula, Sandra S.

Institution:

Universidade Estadual Paulista (UNESP)
MS106
Brookhaven National Laboratory

ISSN:

0375-9474

Abstract:

The effects of opacity of the nuclei together with a blackbody type of emission along the system history are considered as a means to explain the ratio Rout/Rsid observed by STAR and PHENIX collaborations at RHIC. Within our model, no flow is required to explain the data trend of this ratio for large surface emissivities. © 2003 Elsevier Science B.V. All rights reserved.

Issue Date:

10-Mar-2003

Citation:

Nuclear Physics A, v. 715, p. 637C-640C, 2003.

Source:

http://dx.doi.org/10.1016/S0375-9474(02)01550-6

URI:

Access Rights:

Acesso restrito

Type:

outro

Source:

http://repositorio.unesp.br/handle/11449/67230

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