Structure and cooling of compact stars |
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Authors: | H Grigorian |
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Institution: | (1) Laboratory for Information Technologies at JINR, 141980 Dubna, Russia;(2) Department of Physics, Yerevan State University, 375025 Yerevan, Armenia |
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Abstract: | We study the structure and evolution of neutron stars (NSs), the interiors of which are modeled using microscopic approaches
and constrained by the condition that the equation of state (EoS) of matter extrapolated to high densities should not contradict
known observational data from compact stars and experimental data from heavy-ion collisions (HIC). We use modern cooling simulations
to extract distributions of NS masses required to reproduce those of the yet sparse data in the Temperature-Age (TA) plane.
By comparing the results with the mass distribution for young, nearby NSs used in population synthesis, we can sharpen the
NS cooling constraints.
The text was submitted by the author in English. |
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