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SUMMARY:Macroscopic rotational constraints on the neutron-star radius
DTSTART;VALUE=DATE-TIME:20260923T081000Z
DTEND;VALUE=DATE-TIME:20260923T083000Z
DTSTAMP;VALUE=DATE-TIME:20260914T063924Z
UID:indico-contribution-560@indico.bitp.kiev.ua
DESCRIPTION:Speakers: Alexander Magner (IInstitute for Nuclear Research of
  the National Academy of Sciences)\nThe macroscopic model for neutron star
 s (NSs) as a cold perfect fluid in equilibrium within the Tolman-Oppenhiem
 er-Volkoff (TOV) theory is extended to a small rotational angular momentum
  I around the symmetry axis. The deformed NS surface was taken into accoun
 t in the leptodermic approximation $a/R R$) and Hogan inner ($r \n\nhttps:
 //indico.bitp.kiev.ua/event/18/contributions/560/
LOCATION:Bogolyubov Institute for Theoretical Physics Conference Hall
URL:https://indico.bitp.kiev.ua/event/18/contributions/560/
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