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  2. Weber bar - Wikipedia

    en.wikipedia.org/wiki/Weber_bar

    A Weber bar is a device designed to detect gravitational waves, first devised and constructed by physicist Joseph Weber at the University of Maryland. The device consisted of aluminium cylinders, 2 meters in length and 1 meter in diameter , antennae for detecting gravitational waves .

  3. Gravitational-wave observatory - Wikipedia

    en.wikipedia.org/wiki/Gravitational-wave_observatory

    The earliest type was the room-temperature bar-shaped antenna called a Weber bar; these were dominant in 1960s and 1970s and many were built around the world. It was claimed by Weber and some others in the late 1960s and early 1970s that these devices detected gravitational waves; however, other experimenters failed to detect gravitational ...

  4. Allegro gravitational-wave detector - Wikipedia

    en.wikipedia.org/wiki/Allegro_gravitational-wave...

    Allegro was a ground-based, cryogenic resonant Weber bar, gravitational-wave detector [1] run by Warren Johnson, et al. at Louisiana State University in Baton Rouge, Louisiana. The detector was commissioned in the early 1990s, and was decommissioned in 2008.

  5. LIGO - Wikipedia

    en.wikipedia.org/wiki/LIGO

    Joseph Weber pioneered the effort to detect gravitational waves in the 1960s through his work on resonant mass bar detectors. Bar detectors continue to be used at six sites worldwide. By the 1970s, scientists including Rainer Weiss realized the applicability of laser interferometry to gravitational wave measurements. Robert Forward operated an ...

  6. Download or update your web browser - AOL Help

    help.aol.com/articles/download-or-upgrade-your...

    Download or update your web browser Newer browsers provide added benefits, such as increased web surfing security, private browsing, and faster web page uploads. To get the best experience with AOL websites and applications, it's important to use the latest version of a supported browser.

  7. Virgo interferometer - Wikipedia

    en.wikipedia.org/wiki/Virgo_interferometer

    Virgo is a wide-band detector whose sensitivity ranges from a few Hz to 10 kHz; a 2011 Virgo sensitivity curve is plotted with a log-log scale. [94] The most common measure of gravitational-wave-detector sensitivity is the horizon distance, defined as the distance at which a reference target produces a signal-to-noise ratio of 8

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