Titlebook: Handbook of Gravitational Wave Astronomy; Cosimo Bambi,Stavros Katsanevas,Konstantinos D. Ko Living reference work 20200th edition Gravit

BUST

Formation Channels of Single and Binary Stellar-Mass Black Holes, and merger rates. In this review, we discuss the main formation channels of BBHs from stellar evolution and dynamics. Uncertainties on massive star evolution (e.g., stellar winds, rotation, overshooting, and nuclear reaction rates), core-collapse supernovae, and pair instability still hamper our co

tattle

disparage

Inferring the Properties of a Population of Compact Binaries in Presence of Selection Effects,: do all sources come from the same underlying population, or several populations are required? What are the properties of these populations? As the detection of gravitational waves is becoming routine and the size of the event catalog increases, finer and finer details of the astrophysical distribu

向下

蜿蜒而流

Isolated Neutron Stars,observations is, however, a challenging endeavor, as the radiation is only emitted by the outermost layers and is scattered by the interstellar medium. Gravitational waves, on the other hand, while challenging to detect, interact weakly with matter and are likely to carry a clean imprint of the high

Galactogogue

DRILL

LISA and the Galactic Population of Compact Binaries,ible to the space-based gravitational wave detector LISA. A few tens of thousands of these systems will be individually resolvable in frequency space, while the remainder will contribute to a confusion-limited foreground at frequencies below about 1 mHz. In addition to the close white dwarf binaries

爆炸

Living reference work 20200th editionnts, from ground and space based laser interferometers to pulsar timing arrays and indirect detection from the cosmic microwave background. In the second part, it discusses a number of astrophysical and cosmological gravitational wave sources, including black holes, neutron stars, possible more exot

慌張

Indecisive