Astroparticle Physics [lg article] by G. Giacomelli

By G. Giacomelli

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The Supernova 1987A in the large Magellanic Cloud could probably have produced a distortion 10 times smaller. A collapse in the Virgo cluster (at ∼ 17 MPc), should yield relative variations of 10−21 . Two astronomers, R. Hulse and J. Taylor, studied the neutron star binary system PSR 1913+16. 4 solar masses; they are at a distance of about 2 million km and the revolution time is 8 hours. 3. The layout of the LIGO Michelson interferometer with Fabry–Perot cavities. 4. Sensitivities of gravitational wave detectors: cryogenic detectors (AURIGA and NAUTILUS) and appended interferometers (LIGO and VIRGO).

Phys. Rev. Lett. B406 (1997) 249; hep-ex/0009002. G. Giacomelli and L. Patrizii, hep-ex/0002032 (2000); hep-ex/0112009 (2001). 7] P. B. Price, Phys. Rev. D38 (1988) 3813; D. , Europhys. Lett. 12 (1990) 25. 8] S. Nakamura et al. , Lett. B263 (1991) 529. 9] G. Domogatsky, (The Baikal Neutrino Project Status Report) XIX Int. Conf. on Neutrino Physics and Astrophysics, Sudbury, Canada (2000); P. , AMANDA Coll, Proceedings of the ICRC 2001, Hamburg 2001. 10] D. , hep-ex/0003028 (2000); S. , Nuovo Cimento 24 C (2001) 639; J.

A GW is a transverse wave which travels at the speed of light. 2. The binary system PSR1916+13, containing two neutron stars, exhibits a speedup of the orbital period. Over 25 years the total shift recorded is about 25 s. The black points are the data; the solid line is the prediction (not a fit to the data) from the parameters of the system. The agreement is impressive and this experiment provides strong evidence for the existence of gravitational waves. itational wave should modify the distances between objects in the plane perpendicular to the direction of propagation of the wave, Fig.

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