Gravitational radiation from supernova neutrino bursts

Details Gravitational radiation from supernova neutrino bursts Gravitational radiation from supernova neutrino bursts

Aug 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978natur.274..565t&link_type=abstract

Nature, vol. 274, Aug. 10, 1978, p. 565, 566.

Astronomy and Astrophysics

Astronomy

16

Astronomical Models, Gravitational Waves, Neutrinos, Supernovae, Angular Distribution, Feynman Diagrams, Fourier Transformation, Minkowski Space, Particle Interactions, Riemann Manifold

Scientific paper

Attention is given to the electromagnetic analog of the gravitational effects of neutrinos from supernova bursts. Neutrino emission is thus considered in light of quantum dynamics. The zero frequency limit (ZFL) technique of Weinberg is employed to obtain a classical source. Three problems in the analysis are outlined: (1) the source is relativistic (v = c),(2) the source is unbounded (because it moves with the radiation), and (3) an expression must be formulated to represent the stress-energy tensor involved in the creation of a neutrino. Photon radiation from beta-decay is considered as a specific example in the electromagnetic analogy.

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