PIRSA:11060031 Conference Particle Physics

DOI10.48660/11060031

Conference/School: Microphysics in computational relativistic astrophysics - 2011

Duez, M. (2011). Unsolved Problems in Modelin Neutron Star-Neutron Star and Black Hole Neutron Star Binary Mergers. Perimeter Institute. https://pirsa.org/11060031

Duez, Matthew. Unsolved Problems in Modelin Neutron Star-Neutron Star and Black Hole Neutron Star Binary Mergers. Perimeter Institute, Jun. 23, 2011, https://pirsa.org/11060031 

@misc{ pirsa_PIRSA:11060031,
  doi = {10.48660/11060031},
  url = {https://pirsa.org/11060031},
  author = {Duez, Matthew},
  keywords = {Particle Physics},
  language = {en},
  title = {Unsolved Problems in Modelin Neutron Star-Neutron Star and Black Hole Neutron Star Binary Mergers},
  publisher = {Perimeter Institute},
  year = {2011},
  month = {jun},
  note = {PIRSA:11060031 see, \url{https://pirsa.org}}
}

Abstract

Black hole-neutron star (BHNS) binary mergers areimportant gravitational wave sources and (possibly) gamma ray burst progenitors. Fully relativisticsimulations have only recently begun to try to capture neutron star physics beyond the polytrope approximation. In this talk we discuss the numerical challenges of replacing polytropes with realistic neutron stars--particularly those relating to sharper neutron star surface features and to the effects of neutrino radiation--and we present the current status of simulations by the (Caltech-Cornell-CITA-WSU) SXS collaboration and how they are dealing with these issues.

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