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SUMMARY:Correlations of Neutron Star Observables with Properties of Nucleo
 nic and Hyperonic Interactions
DTSTART;VALUE=DATE-TIME:20241023T141200Z
DTEND;VALUE=DATE-TIME:20241023T142400Z
DTSTAMP;VALUE=DATE-TIME:20260719T192824Z
UID:indico-contribution-4093@cern.ch
DESCRIPTION:Speakers: Artur Nasakin (Faculty of Physics\, Lomonosov Moscow
  State University)\nA wide range of extreme states of the nuclear matter t
 hat cannot be studied in terrestrial conditions is realized in neutron sta
 rs\, making them a source of information on the properties of baryonic int
 eractions and nuclear matter under conditions different from those in the 
 most stable nuclei. Under such conditions\, additional sensitivity to cert
 ain properties of baryonic interactions may arise. At densities several ti
 mes higher than the normal nuclear density\, hyperons may appear in the ne
 utron star matter.\n\nIn this paper\, we study the dependence of the obser
 vables of neutron stars\, such as the maximum mass\, the corresponding min
 imum radius\, the tidal deformability coefficient for stars with a mass of
  1.4M$\\odot$ and their radius on the properties of hyperon-nucleon and nu
 cleon-nucleon interactions.\n\nIn particular\, a strong interplay was esta
 blished between the parameters of neutron stars and the density at which h
 yperons appear\, as well as the contracting power of YN interactions.\n\nT
 his work was supported by the Russian Science Foundation under Grant No 24
 -22-00077\n\nhttps://indico.particle.mephi.ru/event/436/contributions/4093
 /
LOCATION: Moskvorechye 2
URL:https://indico.particle.mephi.ru/event/436/contributions/4093/
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