Long-term operation of the Rome "Explorer" cryogenic gravitational wave detector

Astone, P.; Bassan, M.; Bonifazi, P.; Carelli, P.; Castellano, M. G.; Cavallari, G.; Coccia, E.; Cosmelli, C.; Fafone, V.; Frasca, S.; Majorana, E.; Modena, I.; Pallottino, G. V.; Pizzella, G.; Rapagnani, P.; Ricci, F.; Visco, M.

doi:10.1103/physrevd.47.362

Cited by 149 publications

(127 citation statements)

References 22 publications

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“…Astone et al [67,68] report on a search for a statistical association between GRBs and gravitational waves using data from the resonant mass detectors EXPLORER [69] and NAUTILUS [70]. They report a Bayesian upper limit on gravitational-wave signal amplitudes of 1:2 10 ÿ18 , at 95% probability, when the maximum delay between the GRB and gravitational wave is kept at 400 sec.…”

Section: A Comparison With Previous Searches For Gravitational Wavesmentioning

confidence: 99%

Search for gravitational waves associated with the gamma ray burst GRB030329 using the LIGO detectors

Abbott¹,

Abbott²,

Adhikari³

et al. 2005

Phys. Rev. D

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Section: A Comparison With Previous Searches For Gravitational Wavesmentioning

confidence: 99%

Search for gravitational waves associated with the gamma ray burst GRB030329 using the LIGO detectors

Abbott¹,

Abbott²,

Adhikari³

et al. 2005

Phys. Rev. D

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“…Various resonant mass detectors are now operating [21][22][23][24][25]. In [38], the first experiment of cross-correlation…”

Section: A Gw Detectors and Bbn Boundmentioning

confidence: 99%

Big bang nucleosynthesis, matter-antimatter regions, extra relativistic species, and relic gravitational waves

2002

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Provided that matter-antimatter domains are present at the onset of big bang nucleosynthesis (BBN), the number of allowed additional relativistic species increases, compared to the standard scenario when matter-antimatter domains are absent. The extra relativistic species may take the form of massless fermions or even massless bosons, like relic gravitons. The number of additional degrees of freedom compatible with BBN depends, in this framework, upon the typical scale of the domains and the antimatter fraction. Since the presence of matter-antimatter domains allows a reduction of the neutron to proton ratio prior to the formation of 4 He, large amounts of radiation-like energy density are allowed. Our results are compared with other constraints on the number of supplementary relativistic degrees of freedom and with different nonstandard BBN scenarios where the reduction of the neutron to proton ratio occurs via a different physical mechanism. The implications of our considerations for the upper limits on stochastic gravitational waves backgrounds of cosmological origin are outlined.

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“…In the case of a cylinder this is a formidable task; although its formal solution is known [27,28], cylindrical antennas happen in practice tobe narrow and long [29,30], and so approximate solutions can be used instead which are much simpler to handle, and sufficiently good -see also [15].…”

Section: Cylindersmentioning

confidence: 99%

The detection of gravitational waves

Barish¹

1992

Choice Reviews Online

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Abstract. This chapter is concerned with the question: how do gravitational waves (GWs) interact with their detectors? It is intended to be a theoretical review of the fundamental concepts involved in interferometric and acoustic (Weber bar) GW antennas. In particular, the type of signal the GW deposits in the detector in each case will be assessed, as well as its intensity and deconvolution. Brief reference will also be made to detector sensitivity characterisation, including very summary data on current state of the art GW detectors.

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Long-term operation of the Rome "Explorer" cryogenic gravitational wave detector

Cited by 149 publications

References 22 publications

Search for gravitational waves associated with the gamma ray burst GRB030329 using the LIGO detectors

Search for gravitational waves associated with the gamma ray burst GRB030329 using the LIGO detectors

Big bang nucleosynthesis, matter-antimatter regions, extra relativistic species, and relic gravitational waves

The detection of gravitational waves

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