Abstract
We estimate that the moment of inertia of star A in the recently discovered double pulsar system PSR J0737-3039 may be determined after a few years of observation to ∼ 10% accuracy. This would enable accurate estimates of the radius of the star and the pressure of matter in the vicinity of 1-2 times the nuclear saturation density, which would in turn provide strong constraints on the equation of state of neutron stars and the physics of their interiors.
| Original language | English |
|---|---|
| Pages (from-to) | 979-984 |
| Number of pages | 6 |
| Journal | Astrophysical Journal |
| Volume | 629 |
| Issue number | 2 I |
| DOIs | |
| State | Published - Aug 20 2005 |
Keywords
- Binaries: close
- Equation of state
- Pulsars: general
Fingerprint
Dive into the research topics of 'Constraining the equation of state with moment of inertia measurements'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver