Black Holes LIGO/Virgo Domination and Single-lined Binaries with a Black Hole Candidate Component
arXiv:2101.08979 · doi:10.1093/mnras/stab051
Abstract
In this letter, we note that the observed in the LIGO / Virgo experiment ratio of the detection rate of black holes to the rate of detection of binary neutron stars requires the assumption of a "conservative" collapse of massive stars into a black hole: almost all the mass of the collapsing star goes under the horizon. This is consistent with the large masses of black holes detected by LIGO/Virgo. On the other hand, the assumption of a small loss of matter during the collapse into a black hole is in good agreement with the small eccentricity of Single-lined Binaries. At the same time, the absence of X-rays from most black holes in binary systems with blue stars is explained. We argue that three sets of LIGO / Virgo observations and data on the Single-lined Binary with a Candidate Black Hole Component confirm the scenario of the evolution of massive field binaries.
arXiv comment15 pages, 3 figures. MNRAS accepted
References in corpus (38)
- Cosmic Star Formation History
- Multi-messenger Observations of a Binary Neutron Star Merger
- GW190521: A Binary Black Hole Merger with a Total Mass of
- The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars
- Astrophysical Implications of the Binary Black-Hole Merger GW150914
- Advection-Dominated Accretion: Self-Similarity and Bipolar Outflows
- Pulsational Pair-Instability Supernovae
- Pulsational pair instability as an explanation for the most luminous supernovae
- On The Maximum Mass of Stellar Black Holes
- Compact Binary Merger Rates: Comparison with LIGO/Virgo Upper Limits
- A wide star-black-hole binary system from radial-velocity measurements
- Low metallicity natal environments and black hole masses in Ultraluminous X-ray Sources
- Formation and coalescence of relativistic binary stars: effect of kick velocity
- Black hole mergers from quadruples
- Binary black holes in the pair-instability mass gap
- Low metallicity and ultra-luminous X-ray sources in the Cartwheel galaxy
- Population synthesis of black hole binary mergers from star clusters
- Black hole-neutron star mergers from triples
- Beyond the Standard Model Explanations of GW190521
- Not so fast: LB-1 is unlikely to contain a 70 black hole
- APOGEE Kinematics I: Overview of the Kinematics of the Galactic Bulge as Mapped by APOGEE
- First LIGO events: binary black holes mergings
- Evolution of the double neutron star merging rate and the cosmological origin of gamma-ray burst sources
- The Formation of a 70 Msun Black Hole at High Metallicity
- Modelling Double Neutron Stars: Radio and Gravitational Waves
- Weighing in on black hole binaries with BPASS: LB-1 does not contain a 70M black hole
- Toward Understanding the B[e] Phenomenon. VII. AS 386, a single-lined binary with a candidate black hole component
- Early-type Eclipsing Binaries with Intermediate Orbital Periods
- The first gravitational-wave burst GW150914, as predicted by the scenario machine
- The mechanism of Supernova Ia explosion in elliptical galaxies
- A detailed non-LTE analysis of LB-1: Revised parameters and surface abundances
- Scenario Machine: fast radio bursts, short gamma-ray burst, dark energy and Laser Interferometer Gravitational-wave Observatory silence
- Astrophysical sense of the gravitational waves discovery
- Electromagnetic Radiation Accompanying Gravitational Waves from Black Hole Binaries
- Discovery of the neutron stars merger GW170817/GRB170817A and Binary Stellar Evolution
- Why Do We See So Few Black Holes in Massive Binaries?
- Binary Evolution in World Wide Web
- Luminosity function of binary X-ray sources calculated using the Scenario Machine