Circular polarization of electromagnetic radiation during stellar collapse

Details Circular polarization of electromagnetic radiation during stellar collapse Circular polarization of electromagnetic radiation during stellar collapse

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981pazh....7..623r&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 7, Oct. 1981, p. 623-626.) Soviet Astronomy Letters, vol. 7, Sept.-Oct. 1981, p. 345-34

Astronomy and Astrophysics

Astronomy

Circular Polarization, Electromagnetic Radiation, Gravitational Collapse, Neutrinos, Particle Interactions, Stellar Evolution, Bremsstrahlung, Flux (Rate), Stellar Envelopes, Supernovae

Scientific paper

The interaction of neutrino radiation with the material in the outer layers of a collapsing star will generate hard radiation: X-rays and gamma-rays. Because of parity nonconservation in the neutrino interactions, this electromagnetic radiation will be circularly polarized. The polarization should be highly sensitive to the presence of hydrogen in the outer layers and to the intensity ratio of the electron neutrino, electron antineutrino radiation. The intensity and time parameters of the electromagnetic pulse and those of the neutrino radiation will be strongly correlated.

Affiliated with

Also associated with

No associations

Rating

Circular polarization of electromagnetic radiation during stellar collapse does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Circular polarization of electromagnetic radiation during stellar collapse, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Circular polarization of electromagnetic radiation during stellar collapse will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1470710