Merging stellar-mass binary black holes
نویسندگان
چکیده
The LIGO and Virgo detectors have directly observed gravitational waves from mergers of pairs stellar-mass black holes, along with a smaller number involving neutron stars. These observations raise the hope that compact object could be used as probe stellar binary evolution, perhaps dynamics. This colloquium-style article summarises existing observations, describes theoretical predictions for formation channels merging black-hole binaries their rates observable properties, presents some prospects gravitational-wave astronomy.
منابع مشابه
Mergers of accreting stellar-mass black holes
We present post-Newtonian N -body simulations on mergers of accreting stellarmass black holes (BHs), where such general relativistic effects as the pericentre shift and gravitational wave emission are taken into consideration. To elucidate the key physics that regulates mergers of BHs, the dynamical friction and the mass accretion by ambient gas are incorporated. We consider a system composed o...
متن کاملThe Mass Distribution of Stellar Black Holes
We examine the distribution of masses of black holes in transient low mass X-ray binary systems. A Bayesian analysis suggests that it is probable that six of the seven systems with measured mass functions have black hole masses clustered near seven solar masses. There appears to be a significant gap between the masses of these systems and those of the observed neutron stars. The remaining sourc...
متن کاملMass Measurements of Stellar and Intermediate-Mass Black-Holes
We discuss the method, and potential systematic effects therein, used for measuring the mass of stellar-mass black holes in X-ray binaries. We restrict our discussion to the method that relies on the validity of Kepler’s laws; we refer to this method as the dynamical method. We briefly discuss the implications of the mass distribution of stellar-mass black holes and provide an outlook for futur...
متن کاملSimulating merging binary black holes with nearly extremal spins
Astrophysically realistic black holes may have spins that are nearly extremal (i.e., close to 1 in dimensionless units). Numerical simulations of binary black holes are important tools both for calibrating analytical templates for gravitational-wave detection and for exploring the nonlinear dynamics of curved spacetime. However, all previous simulations of binary-black-hole inspiral, merger, an...
متن کاملAccretion onto the First Stellar Mass Black Holes
The first stars in the universe, forming at redshifts z > 15 in minihalos with masses of order 10M⊙, may leave behind black holes as their remnants. These objects could conceivably serve as "seeds" for much larger black holes observed at redshifts z . 7. We study the growth of the remnant black holes through accretion including for the first time the emitted accretion radiation with adaptive me...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Physics Reports
سال: 2022
ISSN: ['0370-1573', '1873-6270']
DOI: https://doi.org/10.1016/j.physrep.2022.01.003