Constraining the equation of state in neutron-star cores via the long-ringdown signal
Abstract Multimessenger signals from binary neutron star (BNS) mergers are promising tools to infer the properties of nuclear matter at densities inaccessible to laboratory experiments. Gravitational waves (GWs) from BNS merger remnants can constrain the neutron-star equation of state (EOS) compleme...
Saved in:
Main Authors: | Christian Ecker, Tyler Gorda, Aleksi Kurkela, Luciano Rezzolla |
---|---|
Format: | Article |
Language: | English |
Published: |
Nature Portfolio
2025-02-01
|
Series: | Nature Communications |
Online Access: | https://doi.org/10.1038/s41467-025-56500-x |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Physical Environment of Accreting Neutron Stars
by: J. Wang
Published: (2016-01-01) -
Analyzing the speed of sound in neutron star with machine learning
by: Sagnik Chatterjee, et al.
Published: (2024-12-01) -
Influence of Effective Nucleon Mass on Equation of State for Supernova Simulations and Neutron Stars
by: Shuying Li, et al.
Published: (2025-01-01) -
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) -
Tidal Reconstruction of Neutron Star Mergers from Their Late Inspiral
by: Souradeep Pal, et al.
Published: (2025-01-01)