On September 14, 2015, almost 60 years after Joseph Weber’s first proposal of resonant bar detectors for picking up gravitational waves (Weber 1960), the two American interferometric antennas comprising LIGO (Laser Interferometer Gravitational Observatory) recorded the first detection of a gravitational wave signal. A chirping waveform lasting about two-tenths of a second with a frequency spanning rapidly from 35 Hz to 250 Hz hit the detector in Livingston, Louisiana, and about 7 ms later, the one in Hanford, Washington, 3000 km away
The origins of Virgo and the emergence of the international gravitational wave community / La Rana, Adele. - (2020), pp. 363-406. [10.1007/978-3-030-50754-1_10].
The origins of Virgo and the emergence of the international gravitational wave community
La Rana, Adele
2020
Abstract
On September 14, 2015, almost 60 years after Joseph Weber’s first proposal of resonant bar detectors for picking up gravitational waves (Weber 1960), the two American interferometric antennas comprising LIGO (Laser Interferometer Gravitational Observatory) recorded the first detection of a gravitational wave signal. A chirping waveform lasting about two-tenths of a second with a frequency spanning rapidly from 35 Hz to 250 Hz hit the detector in Livingston, Louisiana, and about 7 ms later, the one in Hanford, Washington, 3000 km away| File | Dimensione | Formato | |
|---|---|---|---|
|
LaRana_The-origins_2020.pdf
solo gestori archivio
Note: Capitolo
Tipologia:
Versione editoriale (versione pubblicata con il layout dell'editore)
Licenza:
Tutti i diritti riservati (All rights reserved)
Dimensione
492.13 kB
Formato
Adobe PDF
|
492.13 kB | Adobe PDF | Contatta l'autore |
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.


