Effects of the microphysical equation of state in the mergers of magnetized neutron stars with neutrino cooling
نویسندگان
چکیده
Carlos Palenzuela, Steven L. Liebling, David Neilsen, Luis Lehner, O. L. Caballero, Evan O’Connor, and Matthew Anderson Departament de Física, Universitat de les Illes Balears and Institut d’Estudis Espacials de Catalunya, Palma de Mallorca, Baleares E-07122, Spain Department of Physics, Long Island University, Brookville, New York 11548, USA Department of Physics and Astronomy, Brigham Young University, Provo, Utah 84602, USA Perimeter Institute for Theoretical Physics, Waterloo, Ontario N2L 2Y5, Canada Department of Physics, University of Guelph, Guelph, Ontario N1G 2W1, Canada Department of Physics, North Carolina State University, Raleigh, North Carolina 27695, USA Pervasive Technology Institute, Indiana University, Bloomington, Indiana 47405, USA (Received 8 May 2015; published 25 August 2015)
منابع مشابه
2D Cooling of Magnetized Neutron Stars
Context. Many thermally emitting, isolated neutron stars have magnetic fields that are larger than 1013 G. A realistic cooling model that includes the presence of high magnetic fields should be reconsidered. Aims. We investigate the effects of an anisotropic temperature distribution and Joule heating on the cooling of magnetized neutron stars. Methods. The 2D heat transfer equation with anisotr...
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