Massive Black Hole Science with eLISA

被引：26

作者：

Barausse, Enrico ^{[1
,2
]}

Bellovary, Jillian ^{[3
,4
]}

Berti, Emanuele ^{[5
]}

Holley-Bockelmann, Kelly ^{[3
,4
]}

Farris, Brian ^{[6
,7
]}

Sathyaprakash, Bangalore ^{[8
]}

Sesana, Alberto ^{[9
]}

机构：

[1] CNRS, UMR 7095, Inst Astrophys Paris, F-75014 Paris, France

[2] Univ Paris 06, Sorbonne Univ, UMR 7095, F-75014 Paris, France

[3] Vanderbilt Univ, Dept Phys & Astron, Nashville, TN 37235 USA

[4] Fisk Univ, Dept Phys, Nashville, TN 37208 USA

[5] Univ Mississippi, Dept Phys & Astron, University, MS 38677 USA

[6] NYU, Dept Phys, Ctr Cosmol & Particle Phys, New York, NY 10003 USA

[7] Columbia Univ, Dept Astron, New York, NY 10027 USA

[8] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales

[9] Albert Einstein Inst, Max Planck Inst Gravitat Phys, D-14476 Golm, Germany

来源：

10TH INTERNATIONAL LISA SYMPOSIUM | 2015年 / 610卷

基金：

美国国家科学基金会;

关键词：

WAVE STANDARD SIRENS; VIRIAL TEMPERATURES; GENERAL-RELATIVITY; ACCRETION DISKS; GALACTIC NUCLEI; DIRECT COLLAPSE; BINARY-SYSTEMS; BULGE MASS; COLD FLOWS; 1ST STARS;

D O I：

10.1088/1742-6596/610/1/012001

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The evolving Laser Interferometer Space Antenna (eLISA) will revolutionize our understanding of the formation and evolution of massive black holes (MBHs) along cosmic history, by probing massive black hole binaries (MBHBs) in the 10(3) - 10(7) M-circle dot range out to redshift z greater than or similar to 10. High signal-to-noise ratio detections of similar to 10 - 100 MBHB coalescences per year will allow accurate measurements of the parameters of individual MBHBs (such as their masses, spins and luminosity distance), and a deep understanding of the underlying cosmic MBH parent population. This wealth of unprecedented information can lead to breakthroughs in many areas of physics, including astrophysics, cosmology and fundamental physics. We review the current status of the field, recent progress and future challenges.

引用

页数：22

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