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

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References 241[39] Liddle A R 2000 An introduction to cosmological inflation: high energy physics andcosmology Proc. ICTP Summer School ed A Masiero and A Smirnov (Singapore:World Scientific) astro-ph/9901124[40] Turner M S 1997 Ten things everyone should know about inflation Generation ofCosmological Large Scale Structure ed P Galeotti and D Schramm (Dordrecht:Kluwer) pp 153–92 (astro-ph/9704062)[41] Guth A H 1981 Phys. Rev. D 23 347[42] Linde A 1982 Phys. Lett. B 108 389[43] Albrecht A and Steinhardt P 1982 Phys. Rev. Lett. 48 1220[44] Linde A 1983 Phys. Lett. B 129 177[45] Birrel N D and Davies P C W 1982 Quantum Field Theory in Curved Space(Cambridge: Cambridge University Press)[46] Allen B 1988 Phys. Rev. D 37 2078[47] Allen B 1996 Proc. Les Houches School on Astrophysical Sources of GravitationalWaves ed J Marck and J Lasota (Cambridge: Cambridge University Press)Allen B 1996 Preprint gr-qc/9604033[48] Veneziano G 1991 Phys. Lett. B 265 287Gasperini M and Veneziano G 1993 Astropart. Phys. 1 317Gasperini M and Veneziano G 1993 Mod. Phys. Lett. A 8 3701 (an upto-datecollection of references on string cosmology can be found athttp://www.to.infn.it/∼gasperin/[49] Antoniadis I, Arkani-Hamed N, Dimopoulos S and Dvali G 1998 Phys. Lett. B 429263[50] Gasperini M, Maggiore M and Veneziano G 1997 Nucl. Phys. B 494 315[51] Maggiore M 1998 Nucl. Phys. B 525 413[52] Brustein R and Madden R 1997 Phys. Lett. B 410 110Brustein R and Madden R 1998 Phys. Rev. D 57 712[53] Foffa S, Maggiore M and Sturani R 1999 Phys. Rev. D 59 043507[54] Foffa S, Maggiore M and Sturani R 1999 Nucl. Phys. B 552 395[55] Maggiore M and Riotto A 1999 Nucl. Phys. B 548 427[56] Brustein R, Gasperini M, Giovannini M and Veneziano G 1995 Phys. Lett. B 361 45[57] Buonanno A, Maggiore M and Ungarelli C 1997 Phys. Rev. D 55 3330[58] Maggiore M and Sturani R 1997 Phys. Lett. B 415 335[59] Coleman S 1977 Phys. Rev. D 15 2929Callan C G and Coleman S 1977 Phys. Rev. D 16 1762[60] Turner M S et al 1992 Phys. Rev. D 46 2384See also Hogan C J 1983 Phys. Lett. B 133 172[61] Kamionkowsky M et al 1994 Phys. Rev. D 49 2837[62] Kosowsky A et al 1992 Phys. Rev. Lett. 69 2026[63] Thorne K S 1995 Proc. Snowmass 1994 Summer Study on Particle and NuclearAstrophysics and Cosmology ed E Kolb and R Peccei (Singapore: WorldScientific) p 398[64] Ferrari V and Palomba C 1998 Is the gravitational collapse to black holesand interesting source for VIRGO? VIRGO Note VIR-NOT-ROM-1390-109,unpublished[65] Schutz B F 1997 Low-frequency sources of gravitational waves: a tutorial Proc. 1997Alpbach Summer School on Fundamental Physics in Space ed A Wilson (ESA)[66] Giazotto A, Bonazzola S and Gourgoulhon E 1997 Phys. Rev. D 55 2014
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GRAVITATIONAL WAVES
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c IOP Publishing Ltd 2001All righ
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viContents4 Astrophysics of gravita
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viiiContents11.3 Gravitational wave
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xContents16.5 Cosmological perturba
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PrefaceGravitational waves today re
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2 Gravitational waves, theory and e
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10 Gravitational waves, theory and
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SynopsisGravitational waves and the
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Chapter 2Elements of gravitational
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Using the TT gauge to understand gr
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Interaction of gravitational waves
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Analysis of beam detectors 21This d
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Exercises for chapter 2 232. Show t
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Gravitational-wave detectors 25indi
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Gravitational-wave observables 27th
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The physics of interferometers 29
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The physics of interferometers 31Dr
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The physics of interferometers 33Fi
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The physics of resonant mass detect
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The physics of resonant mass detect
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A detector in space 39LISA has been
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Gravitational and electromagnetic w
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Chapter 4Astrophysics of gravitatio
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Sources detectable from ground and
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Variational principles and the ener
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Variational principles and the ener
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Practical applications of the Isaac
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Exercises for chapter 5 57(f)This s
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Expansion for the far field of a sl
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Application of the TT gauge to the
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6.4.1 Mass-quadrupole radiationEner
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Chapter 7Source calculationsNow tha
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The r-modes 73As we mentioned in ch
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The r-modes 75instability. In an id
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The r-modes 77Table 7.1. Gravitatio
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The r-modes 79evolution turns out t
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ReferencesWe have divided the refer
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References 83[19] van der Klis M 19
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Solutions to exercises 85For this p
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Solutions to exercises 87The gauge
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Chapter 8Resonant detectors for gra
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Sensitivity and bandwidth of resona
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8.2 Sensitivity for various GW sign
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Sensitivity for various GW signals
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Recent results obtained with the re
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Discussion and conclusions 101Figur
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Chapter 9The Earth-based large inte
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Introduction 105Figure 9.1. The sim
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h(sqrt(1/Hz))10 −610 −810 −10
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18.5 cmThe SA suspension and requir
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A few words about the Low Frequency
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Conclusion 113Figure 9.7. The R and
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Chapter 10LISA: A proposed joint ES
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Description of the LISA mission 117
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Expected gravitational-wave results
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References 149[8] Folkner W M 1998
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References 151[68] Miralda-Escuda J
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Introduction 153detect GWs with a s
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Testing theories of gravity 155•
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0Testing theories of gravity 157the
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Taking the scalar product we findGr
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Gravitational wave radiation in the
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The hollow sphere 169and introduced
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Scalar-tensor cross sections 171mon
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Scalar-tensor cross sections 173Tab
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Scalar-tensor cross sections 175Tab
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References 177Frossati G and Coccia
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Chapter 12Generalities on the stoch
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Introduction 183contribution to the
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Definitions 185The value of H 0 is
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Definitions 18712.2.2 The character
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Definitions 189or, dividing by the
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Page 222 and 223: Chapter 13Sources of SGWBHere we re
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Page 232 and 233: Topological defects 22113.1.2 Hybri
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Page 236 and 237: Inflation 225as a first approximati
Page 238 and 239: Inflation 227the lower bound to the
Page 240 and 241: String cosmology 22913.3 String cos
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Page 244 and 245: String cosmology 233Figure 13.6. h
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Page 248 and 249: Astrophysical sources 237which is t
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Page 254: PART 4THEORETICAL DEVELOPMENTSHerma
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292 Elementary introduction to pre-
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Chapter 17Post-Newtonian computatio
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340 Post-Newtonian computation of b
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PART 5NUMERICAL RELATIVITYEdward Se
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362 Numerical relativityspite of mo
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364 Numerical relativityterms, of m
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366 Numerical relativityHere we hav
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368 Numerical relativityinformation
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370 Numerical relativityThe Palma,
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372 Numerical relativityHyperbolic
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374 Numerical relativityEinstein di
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376 Numerical relativityare the abi
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378 Numerical relativityeach cell i
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380 Numerical relativityFigure 18.1
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382 Numerical relativity1D code [45
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384 Numerical relativityfunctions,
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386 Numerical relativityto a very a
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388 Numerical relativity18.5 Comput
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390 Numerical relativitynumerics an
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392 Numerical relativityinitial dis
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396 Numerical relativityof these re
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400 Numerical relativityof Einstein
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402 Numerical relativity18.9.5.2 Co
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404 Numerical relativity[23] Ashby
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406 Numerical relativity[101] Shapi
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408 Numerical relativity(Singapore:
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410 IndexEhlers Lagrangian, 254Eins
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412 Indexscalarspherical harmonics,
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