Possibility of direct measurement of the acceleration of the universe using 0.1 Hz band laser interferometer gravitational wave antenna in space

被引：776

作者：

Seto, N ^{[1
]}

Kawamura, S

Nakamura, T

机构：

[1] Osaka Univ, Dept Earth & Space Sci, Toyonaka, Osaka 5600043, Japan

[2] Natl Astron Observ, Mitaka, Tokyo 1818588, Japan

[3] Kyoto Univ, Yukawa Inst Theoret Phys, Kyoto 6068502, Japan

来源：

PHYSICAL REVIEW LETTERS | 2001年 / 87卷 / 22期

关键词：

D O I：

10.1103/PhysRevLett.87.221103

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

It may be possible to construct a laser interferometer gravitational wave antenna in space with h(rms) similar to 10(-27) at f similar to 0.1 Hz in this century. Using this antenna, (1) typically 10(5) chirp signals of coalescing binary neutron stars per year may be detected with S/N similar to 10(4); (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 Omega (GW) greater than or similar to 10(-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.

引用

页码：221103 / 221103

页数：4

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