An inversion-asymmetric source function for HBT analysis in relativistic heavy ion collisions

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dc.creatorLianshou, Liu
dc.creatorShusu, Shi
dc.creatorJiaxin, Du
dc.date2006-08-26
dc.date2006-08-31
dc.date.accessioned2026-07-07T07:25:38Z
dc.date.available2026-07-07T07:25:38Z
dc.descriptionThe inversion-asymmetry of the emission source in relativistic heavy ion collision under the Bertsch-Pratt convention is discussed and explicitly exhibited by a Monte Carlo model. The Gaussian source function popularly used in the HBT analysis of relativistic heavy ion collisions is invalid in this case. An inversion-asymmetric source function is suggested. A method for extracting the inversion-asymmetry degree of the source together with the source size from experimental data is proposed.
dc.description4 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/nucl-th/0608060
dc.identifierhttp://arxiv.org/abs/nucl-th/0608060
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/116785
dc.subjectNuclear Theory
dc.titleAn inversion-asymmetric source function for HBT analysis in relativistic heavy ion collisions
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