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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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4 Gravitational waves, theory and e
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6 Gravitational waves, theory and e
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8 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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Sources detectable from ground and
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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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Application of the TT gauge to the
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Application of the TT gauge to the
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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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- Page 165 and 166: Introduction 153detect GWs with a s
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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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The overlap reduction function 191O
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The overlap reduction function 193T
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The overlap reduction function 195F
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Achievable sensitivities to the SGW
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Achievable sensitivities to the SGW
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Achievable sensitivities to the SGW
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Achievable sensitivities to the SGW
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Achievable sensitivities to the SGW
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Observational bounds 207Table 12.10
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equation gives immediately(ρgwρ
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Chapter 13Sources of SGWBHere we re
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Topological defects 213This correla
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Topological defects 215It can be sh
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Topological defects 217(i)A loop ra
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Topological defects 219• A peak n
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Topological defects 22113.1.2 Hybri
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Inflation 223Hubble radius and when
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Inflation 225as a first approximati
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Inflation 227the lower bound to the
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String cosmology 22913.3 String cos
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String cosmology 231HPre-big bangPo
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String cosmology 233Figure 13.6. h
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First-order phase transitions 23580
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Astrophysical sources 237which is t
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References 239of [71]). However, fo
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References 241[39] Liddle A R 2000
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PART 4THEORETICAL DEVELOPMENTSHerma
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246 Infinite-dimensional symmetries
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248 Infinite-dimensional symmetries
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250 Infinite-dimensional symmetries
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252 Infinite-dimensional symmetries
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254 Infinite-dimensional symmetries
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256 Infinite-dimensional symmetries
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258 Infinite-dimensional symmetries
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260 Infinite-dimensional symmetries
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262 Infinite-dimensional symmetries
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264 Infinite-dimensional symmetries
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266 Infinite-dimensional symmetries
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Chapter 15Gyroscopes and gravitatio
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270 Gyroscopes and gravitational wa
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272 Gyroscopes and gravitational wa
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274 Gyroscopes and gravitational wa
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276 Gyroscopes and gravitational wa
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278 Gyroscopes and gravitational wa
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Chapter 16Elementary introduction t
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282 Elementary introduction to pre-
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284 Elementary introduction to pre-
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286 Elementary introduction to pre-
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288 Elementary introduction to pre-
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290 Elementary introduction to pre-
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292 Elementary introduction to pre-
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294 Elementary introduction to pre-
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296 Elementary introduction to pre-
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298 Elementary introduction to pre-
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300 Elementary introduction to pre-
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302 Elementary introduction to pre-
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304 Elementary introduction to pre-
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306 Elementary introduction to pre-
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308 Elementary introduction to pre-
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310 Elementary introduction to pre-
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312 Elementary introduction to pre-
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314 Elementary introduction to pre-
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316 Elementary introduction to pre-
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318 Elementary introduction to pre-
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320 Elementary introduction to pre-
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322 Elementary introduction to pre-
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324 Elementary introduction to pre-
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326 Elementary introduction to pre-
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328 Elementary introduction to pre-
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330 Elementary introduction to pre-
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332 Elementary introduction to pre-
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334 Elementary introduction to pre-
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336 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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342 Post-Newtonian computation of b
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344 Post-Newtonian computation of b
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346 Post-Newtonian computation of b
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348 Post-Newtonian computation of b
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350 Post-Newtonian computation of b
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352 Post-Newtonian computation of b
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354 Post-Newtonian computation of b
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356 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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394 Numerical relativityFigure 18.2
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396 Numerical relativityof these re
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398 Numerical relativityFigure 18.4
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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,