Evolution of LMXBs under Different Magnetic Braking Prescriptions
arXiv:2101.12427 · doi:10.3847/1538-4357/abe0b2
Abstract
Magnetic braking (MB) likely plays a vital role in the evolution of low-mass X-ray binaries (LMXBs). However, it is still uncertain about the physics of MB, and there are various proposed scenarios for MB in the literature. To examine and discriminate the efficiency of MB, we investigate the LMXB evolution with five proposed MB laws. Combining detailed binary evolution calculation with binary population synthesis, we obtain the expected properties of LMXBs and their descendants binary millisecond pulsars. We then discuss the strength and weakness of each MB law by comparing the calculated results with observations. We conclude that the -boosted MB law seems to best match the observational characteristics.
30 pages, 9 figures, 3 tables, accepted for publication in ApJ
References in corpus (15)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Modules for Experiments in Stellar Astrophysics (MESA)
- Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation
- The ATNF Pulsar Catalogue
- A catalogue of low-mass X-ray binaries in the Galaxy, LMC, and SMC (Fourth edition)
- The effect of magnetic topology on thermally-driven winds: towards a general formulation of the braking law
- Formation of millisecond pulsars with CO white dwarf companions - II. Accretion, spin-up, true ages and comparison to MSPs with He white dwarf companions
- Accretion-Powered Stellar Winds II: Numerical Solutions for Stellar Wind Torques
- The formation of low-mass helium white dwarfs orbiting pulsars: Evolution of low-mass X-ray binaries below the bifurcation period
- The timescale of low-mass proto-helium white dwarf evolution
- Low Mass X-ray Binaries: The Effects of the Magnetic Braking Prescription
- A semi-empirical model for magnetic braking of solar-type stars
- Low mass X-ray binaries with pre-main sequence companions
- Formation of Millisecond Pulsars with Low-Mass Helium White Dwarf Companions in Very Compact Binaries
- Formation of Black Hole Low-Mass X-ray Binaries