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  • 1
    Electronic Resource
    Electronic Resource
    Gravitational Radiation (1989)
    Oxford, UK : Blackwell Publishing Ltd
    Annals of the New York Academy of Sciences 571 (1989), S. 0 
    Details
    ISSN: 1749-6632
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Natural Sciences in General
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1111/j.1749-6632.1989.tb50494.x
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  • 2
    Electronic Resource
    Electronic Resource
    Special relativity (1979)
    [s.l.] : Nature Publishing Group
    Nature 278 (1979), S. 824-824 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Special Relativity: The Foundation of Macroscopic Physics. By W. G. Dixon. Pp. 261. (Cambridge University Press: Cambridge and London, 1978.) £14.50. DON'T let the title deceive you: this is not another introduction to special relativity. This is a book for those of us, working physicists or ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/278824a0
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  • 3
    Electronic Resource
    Electronic Resource
    Determining the Hubble constant from gravitational wave observations (1986)
    [s.l.] : Nature Publishing Group
    Nature 323 (1986), S. 310-311 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] The signal from a system of two IM stars (where M is the mass of the Sun) will sweep from 100 Hz to 1 kHz in ~3 s. There might be three events'per year out to 100 Mpc, and if the detectors achieve their current design sensitivity, such events will be detectable with a signal-to-noise ratio of 30. ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/323310a0
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  • 4
    Electronic Resource
    Electronic Resource
    Coalescing binaries—Probe of the universe (1987)
    Springer
    General relativity and gravitation 19 (1987), S. 1163-1171 
    Details
    ISSN: 1572-9532
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract At present, coalescing binary systems containing neutron stars or black holes are thought to be the most likely sources of gravitational waves to be detected by long baseline interferometers being currently designed. In this essay we calculate the characteristics of the signal from a coalescing binary to the first post-Newtonian order. We show that at coalescence the eccentricity of the orbit, tidal effects, and magnetic interactions can be neglected. We also consider the effects of the expansion of the universe on the signal. We show that observations of gravitational waves from coalescing binaries by a network of detectors will provide a wealth of astrophysical information, e.g., determination of the Hubble constant, new rungs on the cosmic distance ladder, estimates of the masses of components of the binary systems, information about the mass distribution in the universe, highly accurate tests of general relativity, and constraints on neutron-star equations of state. Further development of laser interferometers may enable determination of the deceleration parameter, provide new information about evolution of the universe, and even enable observation of such effects as gravitational lensing.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00759095
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  • 5
    Electronic Resource
    Electronic Resource
    Motion of primordial black holes in the early universe and their likely distribution today (1980)
    Springer
    General relativity and gravitation 12 (1980), S. 881-893 
    Details
    ISSN: 1572-9532
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract We look in detail at those effects which slow down black holes of mass ∼1015 g and affect their spatial distribution today. In particular we treat effects caused by the charge fluctuations of the hole which result from quantum-mechanical processes. The dominant energyloss mechanism for the holes is the expansion of the universe, which leaves them virtually at rest at the time of galaxy formation. The resultant violent relaxation should concentrate roughly half of them in present-day galaxies and their halos.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00757357
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  • 6
    Electronic Resource
    Electronic Resource
    Normal modes of a model radiating system (1986)
    Springer
    General relativity and gravitation 18 (1986), S. 913-921 
    Details
    ISSN: 1572-9532
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract In order to gain insight into normal modes of realistic radiating systems, we study the simple model problem of a finite string and a semi-infinite string coupled by a spring. As expected there is a family of modes which are basically the modes of the finite string slowly damped by the “radiation” of energy to infinity on the semi-infinite string. But we also study another family of modes, found by Dyson in a different model problem, which are strongly damped modes of the semi-infinite string itself. These may be analogous to the modes of black holes, and they are likely to be present in relativistic stars as well. The question of whether the instability in these modes which Dyson found is present in realistic stars remains open.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00773556
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  • 7
    Electronic Resource
    Electronic Resource
    Robinson-Trautman equations and Chandrasekhar's special perturbation of the Schwarzschild metric (1993)
    Springer
    General relativity and gravitation 25 (1993), S. 1185-1188 
    Details
    ISSN: 1572-9532
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract A perturbation wave solution of the Robinson-Trautman equations is proved to be a perturbation of the Schwarzschild black hole which describes an outgoing axial gravitational wave and corresponds to a special case of Chandrasekhar's algebraically special perturbation of the Schwarzschild metric.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00763761
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