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    Article

    Neutrino radiation in spherically-symmetric gravitational fields II. The structure of the radiation field

    It is shown that the neutrino radiation field emitted by a star may be described by Vaidya's radiating Schwarzschild metric. The gravitational energy shift of the neutrino field is also considered, both in ter.....

    J. B. Griffiths, R. A. Newing in General Relativity and Gravitation (1974)

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    A contribution to the rainich theory of the neutrino field II

    Conditions are given on the metric of a space-time for it to admit a neutrino-gravitational field. The method described involves comparing the spin coefficients of a suitably defined tetrad of null vectors. It...

    J. B. Griffiths in International Journal of Theoretical Physics (1974)

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    Article

    Neutrino radiation in spherically-symmetric gravitational fields I. The energy-momentum tensor for the one-neutrino and many-particle neutrino field

    The physical situation of a star emitting neutrinos is considered. Some difficulties in the classical theory are mentioned, and a more detailed approach to the properties of neutrino radiation in general relat.....

    J. B. Griffiths in General Relativity and Gravitation (1973)

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    Article

    Gravitational radiation and neutrinos

    A class of neutrino-gravitational fields with zero energy-momentum tensor is defined. These space-times may also be interpreted as describing gravitational waves and are of Petrov typeD orN. A wave-like example o...

    J. B. Griffiths in Communications in Mathematical Physics (1972)

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    Article

    A contribution to the Rainich theory of the neutrino field

    The neutrino-gravitational field is divided into fourteen distinct classes. This classification is shown also to determine the class of the space-time. Then for four particular classes of space-time, necessary...

    J. B. Griffiths, R. A. Newing in International Journal of Theoretical Physics (1972)

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    Article

    Some physical properties of neutrino-gravitational fields

    A new solution of the Einstein-neutrino field equations is given. This solution is of Plebanski class [4n]3 and describes a beam of neutrinos propagating along straight geodesies but possessing an inherent angula...

    J. B. Griffiths in International Journal of Theoretical Physics (1972)

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