G-Pisa gyrolaser (Contributo in atti di convegno)

Type
Label
  • G-Pisa gyrolaser (Contributo in atti di convegno) (literal)
Anno
  • 2009-01-01T00:00:00+01:00 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi
  • 10.1109/FREQ.2009.5168282 (literal)
Alternative label
  • J Belfi, N Beverini, F Bosi, G Carelli, A Di Virgilio, R Graham, E Maccioni, M Pizzocaro, A Porzio, U Schreiber, S Solimeno, F Sorrentino, A Velikoseltsev (2009)
    G-Pisa gyrolaser
    in Frequency Control Symposium, 2009 Joint with the 22nd European Frequency and Time forum, Besancon, France, 20-24 April 2009
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • J Belfi, N Beverini, F Bosi, G Carelli, A Di Virgilio, R Graham, E Maccioni, M Pizzocaro, A Porzio, U Schreiber, S Solimeno, F Sorrentino, A Velikoseltsev (literal)
Pagina inizio
  • 738 (literal)
Pagina fine
  • 741 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#titoloVolume
  • 2009 JOINT MEETING OF THE EUROPEAN FREQUENCY AND TIME FORUM AND THE IEEE INTERNATIONAL FREQUENCY CONTROL SYMPOSIUM, VOLS 1 AND 2 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#pagineTotali
  • 4 (literal)
Note
  • ISI Web of Science (WOS) (literal)
  • Scopus (literal)
  • Google Scholar (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
  • a Dipartimento di Fisica, Universitá di Pisa, Pisa, 56127, Italy b INFN, Sezione di Pisa, Italy c CNISM, Unitá di Pisa, Italy d Dipartimento di Fisica Universitá Federico II, and CNISM, Unitá di Napoli, Napoli, Italy e Forschungseinrichtung Satellitengeodaesie der Technischen, Universität München Fundamentalstation, Wettzell, Germany f Dipartimento di Fisica, Universitá di Firenze, Sesto Fiorentino, Italy (literal)
Titolo
  • G-Pisa gyrolaser (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#isbn
  • 978-1-4244-3511-1 (literal)
Abstract
  • G-Pisa is an experiment which is investigating the possibility to operate a laser-gyro with area less than 1 m(2) and high sensitivity in order to improve the performances of the mirrors suspension of the gravitational wave antenna Virgo. The experimental set-up consists of a 4 mirrors square cavity, the mechanical drawing allows us to scale the area from 2 down to 0.81 m(2). G-Pisa is working since July 2008, in the following the results so far obtained are reported. At low frequency, below 1 Hz, the sensitivity is typically in the range of 10(-8) rad/s/root Hz, it has been checked that G-Pisa is working properly in single mode and multimode good stable operation has been observed up to 4 mode (literal)
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