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Phys. Rev. Lett. 87, 221103 (2001) [4 pages]

Possibility of Direct Measurement of the Acceleration of the Universe Using 0.1 Hz Band Laser Interferometer Gravitational Wave Antenna in Space

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Naoki Seto1, Seiji Kawamura2, and Takashi Nakamura3
1Department of Earth and Space Science, Osaka University, Toyonaka 560-0043, Japan
2National Astronomical Observatory, Mitaka 181-8588, Japan
3Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502, Japan

Received 4 June 2001; published 9 November 2001

It may be possible to construct a laser interferometer gravitational wave antenna in space with hrms10-27 at f0.1Hz in this century. Using this antenna, (1) typically 105 chirp signals of coalescing binary neutron stars per year may be detected with S/N104; (2) we can directly measure the acceleration of the universe by a 10 yr observation of binary neutron stars; and (3) the stochastic gravitational waves of ΩGW10-20 predicted by the inflation may be detected by correlation analysis. Our formula for phase shift due to accelerating motion might be applied for binary sources of LISA.

© 2001 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.87.221103
DOI:
10.1103/PhysRevLett.87.221103
PACS:
95.55.Ym, 04.80.Nn, 98.80.Es