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SUMMARY:Light Nuclei production in Coalescence Model
DTSTART;VALUE=DATE-TIME:20230531T150500Z
DTEND;VALUE=DATE-TIME:20230531T152500Z
DTSTAMP;VALUE=DATE-TIME:20261010T011113Z
UID:indico-contribution-401@indico.ipb.ac.rs
DESCRIPTION:Speakers: Shanjin Wu (Peking University)\nAs a hadronization m
 odel in relativistic heavy-ion collisions\, coalescence (recombination) mo
 del has achieved great success in the description of the production of had
 ron and light nuclei. This talk focuses on light-nuclei production within 
 the framework of the coalescence model. By employing the characteristic fu
 nction of the phase space density\, we derive the yield of light nuclei in
  terms of various orders of cumulants for the density distribution functio
 n. We found that the leading terms of the phase-space cumulants in the yie
 ld nuclei share a similar form and could be canceled out in light-nuclei r
 atio\, whereas the higher order ones (non-Gaussian shaped density profile)
  remain and play an important role in the interpretation of the behavior o
 f light nuclei yield ratio. In addition\, the critical correlation contrib
 uted to the higher-order phase-space cumulants will also be discussed.\n\n
 https://events.saifa.rs/event/554/contributions/401/
LOCATION:SANU (Serbian Academy of Science and Arts) - Belgrade\, Serbia
URL:https://events.saifa.rs/event/554/contributions/401/
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