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SUMMARY:Hyperons in hot neutron stars
DTSTART;VALUE=DATE-TIME:20241119T170800Z
DTEND;VALUE=DATE-TIME:20241119T171500Z
DTSTAMP;VALUE=DATE-TIME:20260424T154123Z
UID:indico-contribution-25465@indico.ific.uv.es
DESCRIPTION:Speakers: Hristijan Kochankovski (Universitat de Barcelona)\nI
 n this work\, a temperature-dependent equation of state of nuclear\nand hy
 peronic matter suitable for use in relativistic simulations of neutron\nst
 ar mergers and supernovae is presented. We investigate the impact of\nthe 
 uncertainty in the hyperonic sector on the astrophysical observables.\nWe 
 show that these uncertainties have a significant effect on the global\npro
 perties of the stars\, such as mass\, radius\, tidal deformability\, and m
 oment of inertia. The effects are mostly visible for the most massive star
 s\nand at higher temperature\, where the hyperon abundance is significant.
 \nThe findings directly impact the results of relativistic simulations inv
 olving\nneutron star mergers and supernovae\, as they underscore the impor
 tance\nof incorporating hyperonic uncertainties to guarantee the precision
  and\ndependability of these simulations in astrophysical scenarios.\n\nht
 tps://indico.ific.uv.es/event/7664/contributions/25465/
LOCATION:
URL:https://indico.ific.uv.es/event/7664/contributions/25465/
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