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(ed.). Gravitational waves (IOP, 2001)(422s).

(ed.). Gravitational waves (IOP, 2001)(422s).

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82 ReferencesSources of gravitational <strong>waves</strong>Again, there have been a number of conference publications on this subject. Thethird and fourth references are recent reviews of sources. The first two survey theproblem of data analysis.Schutz B F (<strong>ed</strong>) 1989 <strong>Gravitational</strong> Wave Data Analysis (Dordrecht: Kluwer)——1997 The detection of gravitational <strong>waves</strong> Relativistic Gravitation and <strong>Gravitational</strong>Radiation <strong>ed</strong> J A Marck and J P Lasota (Cambridge: Cambridge University Press)pp 447–75Thorne K S 1987 <strong>Gravitational</strong> radiation 300 Years of Gravitation <strong>ed</strong> S W Hawking andW Israel (Cambridge: Cambridge University Press) pp 330–458——1995 Proc. 1994 Summer Study on Particle and Nuclear Astrophysics and Cosmology<strong>ed</strong> E W Kolb and R Peccei (Singapore: World Scientific)Text references[1] Schutz B F 1984 <strong>Gravitational</strong> <strong>waves</strong> on the back of an envelope Am. J. Phys. 52412–19[2] Nicholson D et al 1996 Results of the first coincident observations by 2 laserinterferometricgravitational-wave detectors Phys. Lett. A 218 175–80[3] Meers B J 1988 Recycling in laser-interferometric gravitational wave detectors Phys.Rev. D 38 2317–26[4] TAMA300 project website, http://tamago.mtk.nao.ac.jp/[5] GEO600 project website, http://www.geo600.uni-hannover.de/[6] LIGO project website, http://ligo.caltech.<strong>ed</strong>u/[7] VIRGO project website, http://virgo4p.pg.infn.it/virgo/[8] Caves C M et al 1980 Rev. Mod. Phys. 52 341–92[9] Astone P, Lobo J A and Schutz B F 1994 Coincidence experiments betweeninterferometric and resonant bar detectors of gravitational <strong>waves</strong> Class. QuantumGrav. 11 2093–112[10] Rome gravitational wave group website, http://www.roma1.infn.it/rog/rogmain.html[11] Auriga detector website, http://axln01.lnl.infn.it/[12] LISA project websites, http://www.lisa.uni-hannover.de/ and http://lisa.jpl.nasa.gov/[13] Bender P et al LISA: Pre-Phase A Report MPQ 208 (Max-Planck-Institut fürQuantenoptik, Garching, Germany) (also see the 2nd <strong>ed</strong>n, July 1998)[14] Lipunov V M, Postnov K A and Prokhorov M E 1997 Formation and coalescence ofrelativistic binary stars: the effect of kick velocity Mon. Not. R. Astron. Soc. 288245–59[15] Yungelson L R and Swart S F P 1998 Formation and evolution of binary neutron starsAstron. Astrophys. 332 173–88[16] ZwartSFPandMcMillain S L W 2000 Black hole mergers in the universe Astrophys.J. 528 L17–20 (gr-qc/9910061)[17] Andersson N 1998 A new class of unstable modes of rotating relativistic starsAstrophys. J. 502 708–13 (gr-qc/9706075)[18] Lindblom L, Owen B J and Morsink S M 1998 <strong>Gravitational</strong> radiation instability inhot young neutron stars Phys. Rev. Lett. 80 4843–6 (gr-qc 9803053)

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