Possible Origin of RHIC R_{out}/R_{sid} HBT Results
| dc.creator | Padula, Sandra S. | |
| dc.date | 2002-09-19 | |
| dc.date.accessioned | 2026-07-07T11:32:39Z | |
| dc.date.available | 2026-07-07T11:32:39Z | |
| dc.description | 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 $R_{out}/R_{sid}$ 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. | |
| dc.description | 4 pages, 2 Postscript figures, uses espcrc1.sty. Talk presented at Quark Matter 2002, Nantes, France, July 18-24, 2002; to appear in the proceedings (Nucl. Phys. A) | |
| dc.identifier | https://arxiv.org/abs/nucl-th/0209059 | |
| dc.identifier | http://arxiv.org/abs/nucl-th/0209059 | |
| dc.identifier | Nucl.Phys.A715:637-640,2003 | |
| dc.identifier | doi:10.1016/S0375-9474(02)01550-6 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/197671 | |
| dc.subject | Nuclear Theory | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | Nuclear Experiment | |
| dc.title | Possible Origin of RHIC R_{out}/R_{sid} HBT Results | |
| dc.type | text |