lecture - Ettore Majorana - Infn

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AURIGA - LNLNAUTILUS - LNFData AUNA Taking We are here´06 ´07 ´08 ´09 ´10 ´11 ´12 ´13 ´14 ´15 ´16 ´17 ´18 ´19 ´20 ´21 ´22VirgoGEOLIGOLISAHanfordLivingstonVirgo+LIGO+Advanced VirgoGEO HFAdvanced LIGOLaunch Transfer dataE.T.DS PCP Construction CommissioningdataWindow of opportunityfor AURIGA and NAUTILUS62
exercise in recovering injected gw signals of 8•10 -5 M solar total energywith coherent wavebursts analysis (G.Vedovato for AUNA)Sn explosions according to the acoustic model s25.0; chirps ofrandom polarization randomly injected in the Galaxy accordingly tothe star density; injections over 1day of AUNA datadetection efficiency vsdistanceDistribution in the Galactic planeof the injections (colour) and ofthe recovered signals (black)
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“Ettore Majorana” Foundation an
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PSR1913+16: GWs do exist • Pulsar
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Gravitational radiation is a tool f
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• GWs are detectable in principle
Page 12 and 13: Coupling constants strong e.m. weak
Page 14 and 15: GW OBJECTIVESFIRST DETECTIONtest Ei
Page 16 and 17: The search for gravitational waves
Page 18 and 19: THE INTERFEROMETER NETWORK LIGO -
Page 20 and 21: Some perspective: 40 years of attem
Page 22 and 23: MAIN FEATURESThermal noiseS F = MkT
Page 24 and 25: 12 hours of typical data
Page 26 and 27: 09 10Results published on CQG or PR
Page 28 and 29: Cosmic rayinteraction in the barThe
Page 31 and 32: Nautilus as acoustic particle detec
Page 33 and 34: Exploiting the resonant-mass detect
Page 36 and 37: LAPP - AnnecyINFN - Firenze/UrbinoI
Page 38 and 39: Vacuum: 10 -9 mbarA real detector s
Page 44: Virgo "• Virgo"- European collabo
Page 47 and 48: Seismic noisereduction:Superattenua
Page 49 and 50: LSC and Virgo recent papersDirectio
Page 51: 1st GENERATIONDETECTORS 1 ST GENER
Page 54 and 55: A Global Array of GWDetectors"LIGOG
Page 56 and 57: • Project approved July 2010"Larg
Page 58 and 59: Localization capability:LIGO-Virgo
Page 60 and 61: LIGO-India Concept"• A direct par
Page 64: Newtonian Gravitational NoiseBARS!!
Page 71 and 72: TestMassesTelescopesSpacecrafts5 10
Page 73: More about GW and HEP
Page 77 and 78: Another potential candidate for the
Page 81 and 82: GRAVITATIONAL WAVES MEET NEUTRINOS:
Page 83: Moreover, we can use gravitational
Page 86 and 87: Conclusion
Page 88 and 89: • We are on the threshold of a ne
Page 91 and 92: VisibleInfraredCOBEγ-rayThere are
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lecture - Ettore Majorana - Infn

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