Low-frequency terrestrial gravitational-wave detectors

被引：72

作者：

Harms, Jan ^{[1
]}

Slagmolen, Bram J. J. ^{[2
]}

Adhikari, Rana X. ^{[3
]}

Miller, M. Coleman ^{[4
,5
,6
]}

Evans, Matthew ^{[7
]}

Chen, Yanbei ^{[8
]}

Mueller, Holger ^{[9
]}

Ando, Masaki ^{[10
,11
]}

机构：

[1] Ist Nazl Fis Nucl, Sez Firenze, I-50019 Sesto Fiorentino, Italy

[2] Australian Natl Univ, Ctr Gravitat Phys, Canberra, ACT 0200, Australia

[3] CALTECH, LIGO Lab, Div Phys Math & Astron, Pasadena, CA 91125 USA

[4] Univ Maryland, Dept Astron, College Pk, MD 20742 USA

[5] Univ Maryland, Joint Space Sci Inst, College Pk, MD 20742 USA

[6] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA

[7] MIT, Kavli Inst Astrophys, Cambridge, MA 02139 USA

[8] CALTECH, Div Phys Math & Astron, Pasadena, CA 91125 USA

[9] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[10] Univ Tokyo, Dept Phys, Tokyo 1130033, Japan

[11] Natl Astron Observ Japan, Tokyo 1818588, Japan

来源：

PHYSICAL REVIEW D | 2013年 / 88卷 / 12期

基金：

美国国家科学基金会; 澳大利亚研究理事会;

关键词：

REMNANT TREE SWAY; BLACK-HOLE BINARIES; SUPERCONDUCTING GRAVIMETERS; FOREST CUTBLOCKS; NOISE; INTERMEDIATE; SUSPENSION; LASER; WIND; INTERFEROMETRY;

D O I：

10.1103/PhysRevD.88.122003

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Direct detection of gravitational radiation in the audio band is being pursued with a network of kilometer-scale interferometers (LIGO, Virgo, KAGRA). Several space missions (LISA, DECIGO, BBO) have been proposed to search for sub-hertz radiation from massive astrophysical sources. Here we examine the potential sensitivity of three ground-based detector concepts aimed at radiation in the 0.1-10 Hz band. We describe the plethora of potential astrophysical sources in this band and make estimates for their event rates and thereby, the sensitivity requirements for these detectors. The scientific payoff from measuring astrophysical gravitational waves in this frequency band is great. Although we find no fundamental limits to the detector sensitivity in this band, the remaining technical limits will be extremely challenging to overcome.

引用

页数：19

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