Three Hundred Years of Gravitation by Stephen Hawking

Three Hundred Years of Gravitation by Stephen Hawking

Author:Stephen Hawking [Hawking, Stephen]
Language: eng
Format: epub
ISBN: 9780521379762
Barnesnoble:
Published: 2022-07-04T19:14:27+00:00


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K. S. Thorne

elementary of all ways to compute wave generation, the ‘quadrupole formalism’, and its relationship to radiation reaction in the emitting system (Section 9.3.2). Unfortunately, the most strongly emitting systems should violate the mathematical approximations that underlie the quadrupole formalism and thus can be analyzed only in rough order of magnitude using it; for more accurate analyses one must use a more sophisticated wavegeneration formalism. A catalog of more sophisticated formalisms is given in Section 9.3.3 - which is an updated version of a review I wrote ten years ago (Thome, 1977). The theory of the propagation of the waves from source to earth is sketched in Section 9.3.4, and various wave-propagation effects (absorption, scattering, dispersion, tails, gravitational focusing, diffraction, parametric amplification by background curvature, non-linear coupling of waves to themselves, and generation of background curvature by the waves’

energy and momentum) are described in Section 9.3.5 -which with 9.3.4 is a shortened version of my recent (Thome, 1983), long review of wave propagation. Section 9.3 concludes with very brief descriptions of elegant mathematical work on idealized wave-propagation situations : the asymptotic structure of waves propagating toward ‘future null infinity’ in an asymptotically flat spacetime (Section 9.3.6), and exact, analytic solutions to the Einstein equations for wave generation and propagation (Section 9.3.7).

It is nearly a decade since a detailed and thorough review has been written of astrophysical sources and detectors for gravitational waves (Smarr, ed., 1979; Douglass and Braginsky, 1979); and in the intervening time these topics have changed enormously. (For recent reviews of a number of subtopics see the chapters in Deruelle and Piran, 1983.) Sections 9.4 and 9.5

attempt a comprehensive review in a manner that closely ties the sources to the detection efforts. In these sections the sources and the detection strategies are split up into three categories : those for gravitational-wave

‘bursts’ (Section 9.4. 1 and Fig. 9.4); those for periodic gravitational waves (Section 9.4.2 and Fig. 9.6); and those for a stochastic gravitational-wave background (Section 9.4.3 and Fig. 9.7). All previous reviews have been cavalier about factors of 2 in the definitions of wave strengths and detector sensitivities. This review tries to standardize the definitions, including factors of 2. The standardization is based on signal-to-noise-ratio analyses that are given at the beginnings of Sections 9.4. 1 , 9.4.2, and 9.4.3. For each source that looks favorable for wave detection, Section 9.4 gives a description of our current state of knowledge of the source and gives current estimates of the wave strengths and other wave characteristics.

The burst sources treated in Section 9.4. 1 include supernovae (collapse of

Gravitational radiation

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a normal stellar core to form a neutron star, subsection c), the collapse of a star or star cluster to form a black hole (subsection d), the inspiral and coalescence of compact binaries (neutron stars and black holes, subsection e), and the fall of stars and small holes into supermassive holes (subsection f).

Because our knowledge of sources is so poor, it is useful to estimate how strong the strongest wave bursts



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