PoS - Proceedings of Science
Volume 262 - The Modern Physics of Compact Stars 2015 (MPCS2015) - Session iii neutron star dynamics
Numerical models of isolated rotating compact stars
J. Novak*, M. Oertel, D. Chatterjee and A. Sourie
Full text: pdf
Published on: December 30, 2016
Abstract
Realistic global neutron star models require numerical approach. Here, we briefly motivate and
recall the general-relativistic framework for the description of rotating compact stars and show
how global observable quantities can be computed unambiguously. Then, we present some recent
results on the building of more detailed physical models, including realistic microphysics, fol-
lowing two directions. First, we describe the inclusion of magnetic field and its effects on both,
global equilibrium and equation of state, and finally we discuss superfluid (two-fluid) models in
an attempt to model glitch phenomena.
DOI: https://doi.org/10.22323/1.262.0012
How to cite

Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in "proceeding" format which is more detailed and complete.

Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.