Stellar interferometry for gravitational waves

被引：13

作者：

Park, I. H. ^{[1
]}

Choi, K-Y ^{[1
]}

Hwang, J. ^{[1
]}

Jung, S. ^{[2
]}

Kim, D. H. ^{[3
]}

Kim, M. H. ^{[1
]}

Lee, C-H ^{[4
]}

Lee, K. H. ^{[1
]}

Oh, S. H. ^{[5
]}

Park, M-G ^{[6
]}

Park, S. C. ^{[7
,8
]}

Pozanenko, A. ^{[9
,10
,11
]}

Rho, C. D. ^{[12
]}

Vedenkin, N. ^{[1
]}

Won, E. ^{[13
]}

机构：

[1] Sungkyunkwan Univ SKKU, Dept Phys, 2066 Seobu Ro, Suwon 16419, South Korea

[2] Seoul Natl Univ, Ctr Theoret Phys, Dept Phys & Astron, 1 Gwanak Ro, Seoul 08826, South Korea

[3] Seoul Natl Univ, Dept Phys & Astron, Astron Program, 1 Gwanak Ro, Seoul 08826, South Korea

[4] Pusan Natl Univ, Dept Phys, 2 Busandaehak Ro 63Beon Gil, Busan 46241, South Korea

[5] Natl Inst Math Sci, Div Fundamental Res Publ Agenda, 70 Yuseong Daero 1689 Beon Gil, Daejeon 34047, South Korea

[6] Kyungpook Natl Univ, Dept Astron & Atmospher Sci, 80 Daehak Ro, Daegu 41566, South Korea

[7] Yonsei Univ, Dept Phys, 50 Yonsei Ro, Seoul 03722, South Korea

[8] Yonsei Univ, IPAP, 50 Yonsei Ro, Seoul 03722, South Korea

[9] Russian Acad Sci IKI, Space Res Inst, 84-32 Profsoyuznaya Str, Moscow 117997, Russia

[10] Natl Res Univ, Higher Sch Econ, Myasnitskaya 20, Moscow 101000, Russia

[11] Moscow Inst Phys & Technol MIPT, 9 Inst Skiy,Pereulok St, Dolgoprudnyi 141701, Russia

[12] Univ Seoul, Nat Sci Res Inst, 163 Seoulsiripdaero, Seoul 02504, South Korea

[13] Korea Univ, Dept Phys, 145 Anam Ro, Seoul 02841, South Korea

来源：

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2021年 / 11期

基金：

新加坡国家研究基金会;

关键词：

gravitational wave detectors; gravitational waves / experiments; BLACK-HOLE;

D O I：

10.1088/1475-7516/2021/11/008

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We propose a new method to detect gravitational waves, based on spatial coherence interferometry with stellar light, as opposed to the conventional temporal coherence interferometry with laser sources. The proposed method detects gravitational waves by using two coherent beams of light from a single distant star measured at separate space-based detectors with a long baseline. This method can be applied to either the amplitude or intensity interferometry. This experiment allows for the search of gravitational waves in the lower frequency range of 10(-6) to 10(-4) Hz. In this work, we present the detection sensitivity of the proposed stellar interferometer by taking the detector response and shot and acceleration noises into account. Furthermore, the proposed experimental setup is capable of searching for primordial black holes and studying the size of the target neutron star, which are also discussed in the paper.

引用

页数：20

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