Gravitational Waves: a new window to observe the Universe

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Elements of a Resonant Bar Modern Weber Bars • cryogenically cooled • with superconducting quantum interference devices to detect the motion Aluminium cylinder Resonant frequency 1660 Hz
with bars… 1x10 -19 supernova in the Galaxy 1x10 -20 S hh 0.5 [Hz -1/2 ] 1x10 -21 1x10 -22 800 850 900 950 1000 Frequency [Hz]
Page 1 and 2: Gravitational Waves: a new window t
Page 3 and 4: The gravitational waves are describ
Page 5 and 6: The gravitational waves are describ
Page 7 and 8: Weisberg & Taylor, 2004 The first i
Page 9 and 10: The Classical Detection Method: Web
Page 11: Elements of a Resonant Bar Aluminiu
Page 15 and 16: GRAVITATIONAL ASTRONOMY OBSERVATORI
Page 17 and 18: The laser interferometer detectors
Page 19 and 20: The Interferometer Network LIGO GEO
Page 22 and 23: LIGO Livingston Observatory
Page 24 and 25: About VIRGO.. • French-Italian in
Page 26 and 27: About VIRGO • construction comple
Page 28 and 29: Orbit
Page 30 and 31: Instruments on board Each of the sp
Page 32 and 33: Instruments on board The cubes are
Page 34 and 35: • Current bar detectors will see

Gravitational Waves: a new window to observe the Universe

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