6533b860fe1ef96bd12c3bc4

RESEARCH PRODUCT

Dispersion of pressure at the inner edge of the neutron star crust

Jacek SyskaJan SładkowskiW. OlchawaIlona Bednarek

subject

Physicstransition densityMass distributionEquation of state (cosmology)Astrophysics::High Energy Astrophysical Phenomenadense nuclear matterCrustFunction (mathematics)Edge (geometry)Computational physicsNeutron starQuality (physics)Dispersion (optics)Astrophysics::Earth and Planetary Astrophysicsneutron star

description

This paper presents a method for estimating the pressure variance at the inner edge of a neutron star crust. The obtained results quantify uncertainty in the estimation of pressure at the core-crust interface, implying that they depend on the selected equation of state and the neutron star’s mass distribution function. The quality of the transition pressure determination depends on the neutron star’s mass, with a significant decrease in accuracy for configurations with masses close to 2M . The method used makes it possible to control the theoretical part of the core-crust pressure dispersion in determining the observational quantities.

10.1103/physrevc.104.035802http://hdl.handle.net/20.500.12128/21401