A Statistical Approach to Neutron Stars’ Crust–Core Transition Density and Pressure
In this paper, a regression model between neutron star crust–core pressure and the symmetry energy characteristics was estimated using the Akaike information criterion and the adjusted coefficient of determination <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" di...
Main Authors: | Ilona Bednarek, Wiesław Olchawa, Jan Sładkowski, Jacek Syska |
---|---|
Format: | Article |
Language: | English |
Published: |
MDPI AG
2023-12-01
|
Series: | Entropy |
Subjects: | |
Online Access: | https://www.mdpi.com/1099-4300/25/12/1652 |
Similar Items
-
Forms of the Symmetry Energy Relevant to Neutron Stars
by: Ilona Bednarek, et al.
Published: (2020-06-01) -
From neutron skins and neutron matter to the neutron star crust
by: William G. Newton, et al.
Published: (2022-11-01) -
Neutron Star Properties: Quantifying the Effect of the Crust–Core Matching Procedure
by: Márcio Ferreira, et al.
Published: (2020-11-01) -
Temperature Effects on Core g-Modes of Neutron Stars
by: Nicholas Lozano, et al.
Published: (2022-06-01) -
Neutron Star Constraints on Neutron Dark Decays
by: Dake Zhou
Published: (2023-11-01)