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Tests of General Relativity with GWTC-3
/ LIGO Scientific Collaboration
The ever-increasing number of detections of gravitational waves (GWs) from compact binaries by the Advanced LIGO and Advanced Virgo detectors allows us to perform ever-more sensitive tests of general relativity (GR) in the dynamical and strong-field regime of gravity. [...]
arXiv:2112.06861 ; LIGO-P2100275.
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41 p.
Fulltext
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The Gravitational Wave Antennas Explorer And Nautilus: A Progress Report
/ Bassan, Massimo (Rome U., Tor Vergata ; INFN, Rome2) ; Astone, P (Rome U. ; INFN, Rome) ; Cosmelli,C (Rome U. ; INFN, Rome) ; Frasca, S (Rome U. ; INFN, Rome) ; Pallottino, G V (Rome U. ; INFN, Rome) ; Coccia, E (Rome U., Tor Vergata ; INFN, Rome2) ; Minenkov, Y (Rome U., Tor Vergata ; INFN, Rome2) ; Modena, I (Rome U., Tor Vergata ; INFN, Rome2) ; Moleti, A (Rome U., Tor Vergata ; INFN, Rome2) ; Pizzella, G (Rome U., Tor Vergata ; INFN, Rome2) et al.
/ROG
We report the most recent results obtained with the two cryogenic gravitational wave (g.w.) detectors of the Rome group. A new cross correlation measurement of stochastic background is described, as well as a test of Newton inverse square law at laboratory distances [...]
2000 - 5 p.
- Published in : , pp. 39-44
Fulltext: PDF;
In : 34th Rencontres de Moriond, Les Arcs, France, 23 - 30 Jan 1999, pp.39-44
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EXPLORER and NAUTILUS: Present status
/ Astone, P (Rome U. ; INFN, Rome) ; Cosmelli, C (Rome U. ; INFN, Rome) ; Pallottino, G V (Rome U. ; INFN, Rome) ; Bassan, M (Rome U., Tor Vergata ; INFN, Rome2) ; Carelli, P (Rome U., Tor Vergata ; INFN, Rome2) ; Coccia, E (Rome U., Tor Vergata ; INFN, Rome2) ; Modena, I (Rome U., Tor Vergata ; INFN, Rome2) ; Minenkov, Y (Rome U., Tor Vergata ; INFN, Rome2) ; Moleti, A (Rome U., Tor Vergata ; INFN, Rome2) ; Pizzella, G (Rome U., Tor Vergata ; INFN, Rome2) et al.
2003 - 10 p.
- Published in : 10.1142/9789812704030_0249
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IGEC2: A 17-month search for gravitational wave bursts in 2005-2007
/ Astone, P. (INFN, Rome) ; Baggio, L. (LATMOS, Guyancourt) ; Bassan, M. (Rome U. ; INFN, Rome) ; Bignotto, M. (Padua U. ; INFN, Padua) ; Bonaldi, M. (IFN, Rome ; INFN, Padua) ; Bonifazi, P. (INFN, Rome ; INAF, Rome) ; Cavallari, G. (CERN) ; Cerdonio, M. (Padua U. ; INFN, Padua) ; Coccia, E. (Rome U. ; INFN, Rome) ; Conti, L. (INFN, Padua) et al.
We present here the results of a 515 days long run of the IGEC2 observatory, consisting of the four resonant mass detectors ALLEGRO, AURIGA, EXPLORER and NAUTILUS. The reported results are related to the fourfold observation time from Nov. [...]
arXiv:1002.3515.-
2010 - 10 p.
- Published in : Phys. Rev. D 82 (2010) 022003
APS Published version, local copy: PDF; Fulltext: PDF; External link: Preprint
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EXPLORER and NAUTILUS gravitational wave detectors : a status report
/ Astone, P (INFN, Rome) ; Ballantini, R (INFN, Genova) ; Babusci, D (INFN, Frascati ; Frascati) ; Bassan, M (Rome U., Tor Vergata ; INFN, Rome) ; Bonifazi, P (INFN, Rome ; INAF, Rome) ; Cavallari, G (CERN) ; Chincarini, A (INFN, Genova) ; Coccia, E (Rome U., Tor Vergata ; Gran Sasso) ; D'Antonio, S (INFN, Rome) ; Di Paolo Emilio, M (Gran Sasso ; Aquila U.) et al.
The two cryogenic resonant bar detectors of the ROG Collaboration, EXPLORER and NAUTILUS, have been taking data continuously with a high duty cycle for several years. We report here on the status of recent analysis of the data and in particular on the results of the burst searches in the year 2004..
2008
- Published in : Class. Quantum Gravity 25 (2008) 114048
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Detection of high energy cosmic rays with the resonant gravitational wave detector NAUTILUS and EXPLORER
/ Astone, P. (INFN, Rome) ; Babusci, D. (Frascati) ; Bassan, M. (INFN, Rome2 ; Rome U., Tor Vergata) ; Bonifazi, P. (INFN, Rome ; IFSI, Rome) ; Cavallari, G. (CERN) ; Coccia, E. (INFN, Rome2 ; Rome U., Tor Vergata) ; D'Antonio, S. (INFN, Rome2) ; Fafone, V. (INFN, Rome2 ; Rome U., Tor Vergata) ; Giordano, G. (Frascati) ; Ligi, C. (Frascati) et al.
The cryogenic resonant gravitational wave detectors NAUTILUS and EXPLORER, made of an aluminum alloy bar, can detect cosmic ray showers. At temperatures above 1 K, when the material is in the normal conducting state, the measured signals are in good agreement with the values expected based on the cosmic rays data and on the thermo-acoustic model. [...]
arXiv:0806.1335.-
2008 - 21 p.
- Published in : Astropart. Phys. 30 (2008) 200-208
Fulltext: PDF; External link: Preprint
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