Black Hole Science With the Laser Interferometer Space Antenna

被引：15

作者：

Sesana, Alberto ^{[1
]}

机构：

[1] Univ Milano Bicocca, Dept Phys G Occhialini, Piazza Sci 3, Milan, Italy

来源：

FRONTIERS IN ASTRONOMY AND SPACE SCIENCES | 2021年 / 8卷

基金：

欧洲研究理事会;

关键词：

gravitational waves; black hole physics; binary systems; cosmology; tests of gravity; GRAVITATIONAL-WAVE ASTRONOMY; BINARY-SYSTEMS; LOW-FREQUENCY; MASS; ACCRETION; STARS; POPULATION; EVOLUTION; DYNAMICS; HISTORY;

D O I：

10.3389/fspas.2021.601646

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The author reviews the scientific potential of the Laser Interferometer Space Antenna (LISA), a space-borne gravitational wave (GW) observatory to be launched in the early 30s. Thanks to its sensitivity in the milli-Hz frequency range, LISA will reveal a variety of GW sources across the Universe, from our Solar neighborhood potentially all the way back to the Big Bang, promising to be a game changer in our understanding of astrophysics, cosmology, and fundamental physics. This review dives in the LISA Universe, with a specific focus on black hole science, including the formation and evolution of massive black holes in galaxy centers, the dynamics of dense nuclei and formation of extreme mass ratio inspirals, and the astrophysics of stellar-origin black hole binaries.

引用

页数：8

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