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|2 bisacsh
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|a HCDD
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| 100 |
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|a Maggiore, Michele,
|e author.
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|a Gravitational waves :
|n Volume 1,
|p Theory and experiments /
|c Michele Maggiore.
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| 260 |
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|a Oxford :
|b Oxford University Press,
|c 2007.
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| 300 |
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|a 1 online resource (572 pages)
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| 336 |
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|a text
|b txt
|2 rdacontent
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|a computer
|b c
|2 rdamedia
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|a online resource
|b cr
|2 rdacarrier
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|a data file
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|a The aim of this book is to become a major reference text for gravitational-wave physics, covering in detail both the experimental and the theoretical aspects. The book brings the reader to the forefront of present-day research, and assumes no previous knowledge of gravitational-wave physics.
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|a Print version record.
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|a Includes bibliographical references and index.
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|6 880-01
|a Cover ; Title page; Copyright page; Contents; Preface; Notation; Part I Gravitational-wave theory; 1 The geometric approach to GWs; 1.1 Expansion around at space; 1.2 The transverse-traceless gauge; 1.3 Interaction of GWs with test masses; 1.3.1 Geodesic equation and geodesic deviation; 1.3.2 Local inertial frames and freely falling frames; 1.3.3 TT frame and proper detector frame; 1.4 The energy of GWs; 1.4.1 Separation of GWs from the background; 1.4.2 How GWs curve the background; 1.4.3 The energy-momentum tensor of GWs; 1.5 Propagation in curved space-time.
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|a 2.3.1 Phenomenological bounds2.3.2 Field theory of massive gravitons; 2.4 Solved problems; 2.1. The helicity of gravitons; 2.2. Angular momentum and parity of graviton states; Further reading; 3 Generation of GWs in linearized theory; 3.1 Weakeld sources with arbitrary velocity; 3.2 Low-velocity expansion; 3.3 Mass quadrupole radiation; 3.3.1 Amplitude and angular distribution; 3.3.2 Radiated energy; 3.3.3 Radiated angular momentum; 3.3.4 Radiation reaction on non-relativistic sources; 3.3.5 Radiation from a closed system of point masses; 3.4 Mass octupole and current quadrupole.
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|a 4.1.2 Elliptic orbits. (I) Total power and frequency spectrum of the radiation emitted4.1.3 Elliptic orbits. (II) Evolution of the orbit under back-reaction; 4.1.4 Binaries at cosmological distances; 4.2 Radiation from rotating rigid bodies; 4.2.1 GWs from rotation around a principal axis; 4.2.2 GWs from freely precessing rigid bodies; 4.3 Radial infall into a black hole; 4.3.1 Radiation from an infalling point-like mass; 4.3.2 Tidal disruption of a real star falling into a black hole. Coherent and incoherent radiation; 4.4 Radiation from accelerated masses.
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| 546 |
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|a English.
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| 650 |
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|a Gravitational waves.
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| 650 |
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|a SCIENCE
|x Astronomy.
|2 bisacsh
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| 650 |
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|a Gravitational waves
|2 fast
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| 710 |
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|a Oxford University Press.
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| 758 |
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|i has work:
|a Gravitational waves Volume 1 Theory and experiments (Text)
|1 https://id.oclc.org/worldcat/entity/E39PCFJWdbjGgpkwXHRVVtyYpq
|4 https://id.oclc.org/worldcat/ontology/hasWork
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| 776 |
0 |
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|i Print version:
|t Gravitational waves. Volume 1, Theory and experiments [Texte imprimé] / Michele Maggiore ...
|d Oxford : Oxford University Press, cop. 2008
|h 1 vol. (XVII-554 p.)
|o 978-0-19-857074-5
|w (ABES)119544768
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| 856 |
4 |
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|u https://holycross.idm.oclc.org/login?auth=cas&url=https://academic.oup.com/book/41655
|y Click for online access
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| 880 |
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|6 505-00/(S
|a 1.5.1 Geometric optics in curved space1.5.2 Absorption and scattering of GWs; 1.6 Solved problems; 1.1. Linearization of the Riemann tensor in curved space; 1.2. Gauge transformation of hμν and R(1) μνρσ; Further reading; 2 The field-theoretical approach to GWs; 2.1 Linearized gravity as a classical eld theory; 2.1.1 Noether's theorem; 2.1.2 The energ-momentum tensor of GWs; 2.1.3 The angular momentum of GWs; 2.2 Gravitons; 2.2.1 Why a spin-2 field; 2.2.2 The Pauli-Fierz action; 2.2.3 From gravitons to gravity; 2.2.4 E ective field theories and the Planck scale; 2.3 Massive gravitons.
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|6 505-01/(S
|a 3.5 Systematic multipole expansion3.5.1 Symmetric-trace-free (STF) form; 3.5.2 Spherical tensor form; 3.6 Solved problems; 3.1. Quadrupole radiation from an oscillating mass; 3.2. Quadrupole radiation from a mass in circular orbit; 3.3. Mass octupole and current quadrupole radiation from a mass in circular orbit; 3.4. Decomposition of Skl, m into irreducible epresenta-tions of SO(3); 3.5. Computation of ∫ dΩ (TE2,B2 lm) *ijnij ... niα; Further reading; 4 Applications; 4.1 Inspiral of compact binaries; 4.1.1 Circular orbits. The chirp amplitude.
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