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Phys Rev Lett ; 86(18): 3950-4, 2001 Apr 30.
Artigo em Inglês | MEDLINE | ID: mdl-11328068

RESUMO

TAMA300, an interferometric gravitational-wave detector with 300-m baseline length, has been developed and operated with sufficient sensitivity to detect gravitational-wave events within our galaxy and sufficient stability for observations; the interferometer was operated for over 10 hours stably and continuously. With a strain-equivalent noise level of h approximately 5x10(-21)/sqrt[Hz], a signal-to-noise ratio of 30 is expected for gravitational waves generated by a coalescence of 1.4M-1.4M binary neutron stars at 10 kpc distance. We evaluated the stability of the detector sensitivity with a 2-week data-taking run, collecting 160 hours of data to be analyzed in the search for gravitational waves.


Assuntos
Astronomia/métodos , Gravitação , Astronomia/instrumentação , Lasers , Sensibilidade e Especificidade
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