Abstract
Recently, observational searches for gravitational wave background (GWB) have been developed and given constraints on the energy density of GWB in a broad range of frequencies. However, at 100 MHz, there is no strict upper limit from direct observation. In this article, we will propose a direct observation with interferometers. We investigated the detector designs, which can effectively respond to GW at high frequencies, and an optimal location of two detectors for correlation analysis of GWB.
Original language | English |
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Pages | 212-215 |
Number of pages | 4 |
State | Published - 2007 |
Event | 17th Workshop on General Relativity and Gravitation in Japan, JGRG 2007 - Nagoya, Japan Duration: 2007/12/03 → 2007/12/07 |
Conference
Conference | 17th Workshop on General Relativity and Gravitation in Japan, JGRG 2007 |
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Country/Territory | Japan |
City | Nagoya |
Period | 2007/12/03 → 2007/12/07 |
ASJC Scopus subject areas
- Atomic and Molecular Physics, and Optics