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SUMMARY:Using a variational method to study nuclear matter\, hyper nuclear
  matter and neutron stars
DTSTART;VALUE=DATE-TIME:20190222T093000Z
DTEND;VALUE=DATE-TIME:20190222T110000Z
DTSTAMP;VALUE=DATE-TIME:20261013T133458Z
UID:indico-event-60@events.ift.uni.wroc.pl
DESCRIPTION:We investigate the equation of state of nuclear matter\, hyper
  nuclear matter and compact stars within our variational method. Chemical 
 potentials of nucleons in asymmetric nuclear matter are calculated in a co
 mpletely self-consistent manner\, using the lowest order constrained varia
 tional (LOCV) method. Employing different nucleon–nucleon potentials\, t
 hreshold density of free hyperons formation and the maximum mass of hypern
 uclear star are determined. Furthermore\, the particles fraction in beta s
 table and charge neutral matter is calculated as well. The effects of thre
 e-body force (TBF) on the onset of hyperons\, particle composition and max
 imum mass of the star are discussed.\nOn the basis of this method which is
  reformulated by using two-body central potentials for Λ-N and Λ-Λ inte
 raction that were determined so as to reproduce the experimental data on s
 ingle- and double-Λ hypernuclei\, the equation of state of hyper nuclear 
 matter is found for the first time in this method. Calculation of correla
 tion functions for N-Y and Y-Y interaction  for each JLSTMT-channel is do
 ne for the first time as well.\n\nhttps://events.ift.uni.wroc.pl/event/60/
LOCATION:IFT 422
URL:https://events.ift.uni.wroc.pl/event/60/
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