CaltechAUTHORS
  A Caltech Library Service

Correlation analysis of stochastic gravitational wave background around 0.1–1 Hz

Seto, Naoki (2006) Correlation analysis of stochastic gravitational wave background around 0.1–1 Hz. Physical Review D, 73 (6). Art. No. 063001. ISSN 2470-0010. http://resolver.caltech.edu/CaltechAUTHORS:SETprd06b

[img]
Preview
PDF - Published Version
See Usage Policy.

480Kb

Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:SETprd06b

Abstract

We discuss prospects for direct measurement of stochastic gravitational wave background around 0.1–1 Hz with future space missions. It is assumed to use correlation analysis technique with the optimal time-delay-interferometry (TDI) variables for two sets of LISA-type interferometers. The signal to noise for detection of the background and the estimation errors for its basic parameters (amplitude, spectral index) are evaluated for proposed missions.


Item Type:Article
Additional Information:© 2006 The American Physical Society. (Received 17 January 2006; published 1 March 2006) The author thanks S. Kawamura and S. Phinney for valuable discussions. He also thanks N. Cornish for discussions on astrophysical foreground, C. Cutler for helpful conversations on the noise curves of BBO, and J. Yokoyama for directing his interest to this research through a collaboration.
Group:LIGO
Subject Keywords:gravitational wave detectors; gravitational waves; cosmology; light interferometers
Issue or Number:6
Record Number:CaltechAUTHORS:SETprd06b
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:SETprd06b
Alternative URL:http://dx.doi.org/10.1103/PhysRevD.73.063001
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:6319
Collection:CaltechAUTHORS
Deposited By: Archive Administrator
Deposited On:01 Dec 2006
Last Modified:06 Sep 2019 22:12

Repository Staff Only: item control page