Properties of Neutron Stars Related to Gravitational Waves
ABSTRACT Neutron stars are natural laboratories of cold, dense strong interacting matter. In this article, we briefly review the gravitational waves related to neutron stars. Tidal deformability is a significant value that relates the observation of gravitational waves to the equation of state of cold, dense matter. The implicants of GW170817 and GW190814 are discussed. We also give an outlook for future work.
Authors
- Zhi‐Fu Gao (ORCID: https://orcid.org/0000-0002-0138-3360)
- Weifeng Zhang (ORCID: https://orcid.org/0000-0003-1336-771X)
- Hui Wang (ORCID: https://orcid.org/0009-0005-2954-6298)
- Yan Yan (ORCID: https://orcid.org/0000-0001-5298-9816)
Institutions
- Yuncheng University (CN)
- Xinjiang Astronomical Observatory (CN)
- Changzhou University (CN)
Publication Details
- Journal
- Astronomische Nachrichten
- Published
- 2025-06-29
- DOI
- https://doi.org/10.1002/asna.70028
- Primary Topic
- Pulsars and Gravitational Waves Research
- Type
- article
- Field-Weighted Citation Impact
- 0.00
Funders
- National Natural Science Foundation of China