Low-Mass Neutron Stars with Rotation
arXiv:2005.04428 · doi:10.1134/S1063773719120077
Abstract
The properties of low-mass neutron stars with rigid rotation are considered. The possible evolution paths of such stars in a close binary system with mass transfer are calculated. The properties of the gamma-ray burst GRB 170817A interpreted in terms of the stripping model, a natural ingredient of which is the explosion of a low-mass neutron star - a binary component, are briefly discussed.
arXiv comment16 pages, 3 figs, 1 table
References in corpus (10)
- Shapiro delay measurement of a two solar mass neutron star
- Multi-messenger Observations of a Binary Neutron Star Merger
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- Neutron Star Structure and the Equation of State
- The Combined Ultraviolet, Optical, and Near-Infrared Light Curves of the Kilonova Associated with the Binary Neutron Star Merger GW170817: Unified Data Set, Analytic Models, and Physical Implications
- Analytical representations of unified equations of state of neutron-star matter
- A turnover in the radio light curve of GW170817
- GW170817the first observed neutron star merger and its kilonova: implications for the astrophysical site of the r-process
- Equation of state of dense matter and the minimum mass of cold neutron stars
- Mass and radius formulas for low-mass neutron stars
Cited by in corpus (8)
- Neutron Star Mergers and Gamma-Ray Bursts: Stripping Model
- Production of Heavy Elements During the Explosion of a Low-Mass Neutron Star in a Close Binary
- The fate of twin stars on the unstable branch: implications for the formation of twin stars
- Dynamics of direct impact accretion in degenerate binary systems
- Accretion spin-up of the massive component in the neutron star stripping model for short gamma-ray bursts
- True Unicorns and False Positives: Simulated Probabilities of Dark Massive Companions to Bright Stars
- Short gamma-ray bursts and the decompression of neutron star matter in tidal streams
- Numerical Study of Polytropes with n=1 and Differential Rotation