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Gravitational Wave Detection by Using Mossbauer Effect

IP.com Disclosure Number: IPCOM000065556D
Original Publication Date: 1985-Dec-01
Included in the Prior Art Database: 2005-Feb-19

Publishing Venue

IBM

Related People

Authors:
Erbil, A [+details]

Abstract

Gravitational wave detection has been a very active field after the pioneering work of Weber [l]. A gravitational wave produces tiny relative displacements between various parts of a detector. Currently, gravitational wave detection efforts involve three distinct types of detectors: Doppler tracking of spacecraft, laser interferometers, and Weber-type resonant bars [2]. These detectors have achieved a burst sensitivity capable of detecting gravitational waves with an amplitude of h = 3 x 10-16 at frequencies N 30 to 104 Hz. A detector for gravitational waves is proposed using the Mossbauer effect [3] in long lifetime nuclear isomers. This new type of detector can achieve a sensitivity of h = 10-16 or better depending on the nuclear isomer used. A nuclear isomer is an excited state of nuclei with a very long lifetime.