A Abramovici

A Araya

A Brillet

A Gillespie

A Rüdiger

AD Farinas

AM Campbell

AS Nowick

B Willke

BC Barish

BF Schutz

BJ Meers

BS Lunin

C M Will

CC Harb

CD Nabors

CM Caves

D Golla

D Robertson

D Shoemaker

DH Douglass

E Amaldi

E Gustafson

E Mizuno

F Bondu

G Giampieri

G Heinzel

G Losurdo

GA Kerr

GA Prodi

GE Moss

GV Pallottino

H Billing

H Kogelnik

Institute of Physics Publishing

IS Heng

J f t L S T Hough

J Faller

J Hough

J Weber

J Winterflood

JA Tyson

JE Faller

JH Taylor

K Danzmann

K Tsubono

KA Strain

KD Skeldon

KS Thorne

L Ju

M Beccaria

M Harris

M Plissi

NA Robertson

O Cregut

P Fritschel

PR Saulson

PW McNamara

R J Decher

R Loudon

R Weiss

RA Hulse

RE Spero

RJ Shine Jr.

RL Forward

RWP Drever

S Braccini

S Hughes

S Rowan

TJ Kane

VB Braginsky

W Weichmann

WA Edelstein

WJ Startin

WM Tulloch

YU Levin

AbstractSignificant progress has been made in recent years on the development of gravitational wave detectors. Sources such as coalescing compact binary systems, low-mass X-ray binaries, stellar collapses and pulsars are all possible candidates for detection. The most promising design of gravitational wave detector uses test masses a long distance apart and freely suspended as pendulums on Earth or in drag-free craft in space. The main theme of this review is a discussion of the mechanical and optical principles used in the various long baseline systems being built around the world — LIGO (USA), VIRGO (Italy/France), TAMA 300 (Japan) and GEO 600 (Germany/UK) — and in LISA, a proposed space-borne interferometer.</jats:p

Gravitational Wave Detection by Interferometry (Ground and Space)

Abstract

Similar works

Full text

Available Versions

Crossref