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SUMMARY:Strange Quark Matter with $\\beta$-equilibrium condition
DTSTART;VALUE=DATE-TIME:20201006T084500Z
DTEND;VALUE=DATE-TIME:20201006T090000Z
DTSTAMP;VALUE=DATE-TIME:20261015T233606Z
UID:indico-contribution-2159@cern.ch
DESCRIPTION:Speakers: MANISHA KUMARI (Dr. B. R. Ambedkar National Institut
 e of Technology\, Jalandhar)\nThe present study explores the properties of
  strange quark matter (SQM) or strange quark star (SQS) within the Polyako
 v extended chiral $\\text{SU(3)}$ quark mean field (PCQMF) model. Using $\
 \beta$- equilibrium condition in the PCQMF model\, the analysis of effecti
 ve quark masses\, effective quark chemical potential\, and equation of sta
 te for strange quark matter at different values of vector coupling constan
 t is carried out. Three different conditions of Proto-Quark Star (PQS) alo
 ng the star evolution ($S/n_B=1\, Y_l=0.4\;~S/n_B=2\, Y_{\\nu_l}=0\;~S/n_B
 =0\, Y_{\\nu_l}=0$) are considered to performed the theoretical simulation
 . Providing a significant vector coupling constant\, the change in effecti
 ve quark masses with baryon density is found to be less as compared to zer
 o vector interaction. Further\, pressure density shows monotonically and s
 moothly increasing with the increase in energy density. The study thus car
 ried out\, anticipated to give a better insight into the role that the sup
 erdense matter created in heavy-ion collision experiments plays an importa
 nt role in understanding the properties of matter inside the core of super
 massive stars in the universe.\n\nhttps://indico.particle.mephi.ru/event/3
 5/contributions/2159/
LOCATION:Zoom HEP Theory
URL:https://indico.particle.mephi.ru/event/35/contributions/2159/
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