2005Unpublished venueRequires access

Virgo: a wide band gravitational wave detector

R. Flaminio

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Abstract

Virgo is a gravitational wave antenna aiming at the detection of gravitational waves emitted by astrophysical sources in a frequency range comprised between 10 Hz and a few kHz. The detector design and its present status are presented.

About this research paper

What this paper is about

Virgo is a gravitational wave antenna aiming at the detection of gravitational waves emitted by astrophysical sources in a frequency range comprised between 10 Hz and a few kHz. The detector design and its present status are presented.

Why it matters

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Key contribution

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Method / approach

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Main findings

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Available abstract

Virgo is a gravitational wave antenna aiming at the detection of gravitational waves emitted by astrophysical sources in a frequency range comprised between 10 Hz and a few kHz. The detector design and its present status are presented.

Key concepts: Gravitational wave, Physics, Detector, Gravitational-wave observatory, Antenna (radio), Range (aeronautics), Frequency band, Acoustics

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