Continuous Gravitational Waves from Thermal Mountains on Accreting Neutron Stars: Effect of the Nuclear Pasta Phase
As density increases, the shape of nuclei transitions to nonspherical “nuclear pasta” structures. The physical properties of the nuclear pasta, such as thermal conductivity and elasticity, have implications for detecting continuous gravitational waves from a rapidly rotating neutron star. In this wo...
Saved in:
Main Authors: | Hong-Bo Li, Lijing Shao, Cheng-Jun Xia, Ren-Xin Xu |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2025-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/adadf2 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Long-term Evolution of Sco X-1: Implications for the Current Spin Frequency and Ellipticity of the Neutron Star
by: Abhijnan Kar, et al.
Published: (2025-01-01) -
Quadrupole Moment of a Magnetically Confined Mountain on an Accreting Neutron Star in General Relativity
by: Pedro H. B. Rossetto, et al.
Published: (2025-01-01) -
On the Use of Galaxy Catalogs in Gravitational-wave Parameter Estimation
by: Geoffrey Mo, et al.
Published: (2025-01-01) -
GR-Athena++: General-relativistic Magnetohydrodynamics Simulations of Neutron Star Spacetimes
by: William Cook, et al.
Published: (2025-01-01) -
Nucleon-nucleon short-range correlations: A hidden driver in binary neutron star inspiral gravitational waves
by: Bin Hong, et al.
Published: (2025-01-01)