Forms of the Symmetry Energy Relevant to Neutron Stars
The symmetry energy is an invaluable tool for studying dense nuclear matter. Unfortunately, its definition is somewhat implicit, and therefore, phenomenological methods are necessary to describe experimental facts. This paper discusses the differences arising from the use of Taylor series expansion...
Main Authors: | Ilona Bednarek, Jan Sładkowski, Jacek Syska |
---|---|
Format: | Article |
Language: | English |
Published: |
MDPI AG
2020-06-01
|
Series: | Symmetry |
Subjects: | |
Online Access: | https://www.mdpi.com/2073-8994/12/6/898 |
Similar Items
-
A Statistical Approach to Neutron Stars’ Crust–Core Transition Density and Pressure
by: Ilona Bednarek, et al.
Published: (2023-12-01) -
Translating Neutron Star Observations to Nuclear Symmetry Energy via Deep Neural Networks
by: Plamen G. Krastev
Published: (2022-01-01) -
Temperature Effects on Core g-Modes of Neutron Stars
by: Nicholas Lozano, et al.
Published: (2022-06-01) -
Nuclear Pasta in Cold Non-Accreting Neutron Stars: Symmetry Energy Effects
by: Nikolai N. Shchechilin, et al.
Published: (2023-02-01) -
Symmetry energy of super-dense neutron-rich matter from integrating barotropic pressures in neutron stars and heavy-ion reactions
by: Bao-An Li, et al.
Published: (2020-07-01)