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Title: POSSIBLE ORIGIN OF RHIC R OUT/R SID HBT RESULTS.

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 R{sub out}/R{sub sid} 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.

Authors:
Publication Date:
Research Org.:
Brookhaven National Lab., Upton, NY (US)
Sponsoring Org.:
USDOE Office of Energy Research (ER) (US)
OSTI Identifier:
804086
Report Number(s):
BNL-69354-02/10-REV.
R&D Project: PO006; KB03; TRN: US0300600
DOE Contract Number:  
AC02-98CH10886
Resource Type:
Conference
Resource Relation:
Conference: QUARK MATTER 2002, NANTES (FR), 07/18/2002--07/24/2002; Other Information: PBD: 18 Jul 2002
Country of Publication:
United States
Language:
English
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; NUCLEI; OPACITY; ORIGIN; QUARK MATTER; STARS

Citation Formats

PADULA, S S. POSSIBLE ORIGIN OF RHIC R OUT/R SID HBT RESULTS.. United States: N. p., 2002. Web.
PADULA, S S. POSSIBLE ORIGIN OF RHIC R OUT/R SID HBT RESULTS.. United States.
PADULA, S S. Thu . "POSSIBLE ORIGIN OF RHIC R OUT/R SID HBT RESULTS.". United States. https://www.osti.gov/servlets/purl/804086.
@article{osti_804086,
title = {POSSIBLE ORIGIN OF RHIC R OUT/R SID HBT RESULTS.},
author = {PADULA, S S},
abstractNote = {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 R{sub out}/R{sub sid} 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.},
doi = {},
journal = {},
number = ,
volume = ,
place = {United States},
year = {2002},
month = {7}
}

Conference:
Other availability
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