NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Photoneutrino energy losses in strong magnetic fields.Previously computed rates of energy losses (Petrosian et al., 1967) ignored the presence of strong magnetic fields, hence the change brought in when such a field (about 10 to the 12th to 10 to the 13th power G) is included is studied. The results indicate that for T about 10 to the 8th power K and densities rho of about 10,000 g/cu cm, the presence of a strong H field decreases the energy losses by at the most a factor between 10 and 100 in the region up to rho = 1,000,000 g/cu cm. At higher densities the neutrino emissivities are almost identical.
Document ID
19730041613
Document Type
Reprint (Version printed in journal)
Authors
Canuto, V. (NASA Goddard Institute for Space Studies; City College New York, N.Y., United States)
Fassio-Canuto, L. (New York Institute of Technology New York, N.Y., United States)
Date Acquired
August 7, 2013
Publication Date
March 15, 1973
Publication Information
Publication: Physical Review D - Particles and Fields
Subject Category
PHYSICS, ATOMIC, MOLECULAR, AND NUCLEAR
Distribution Limits
Public
Copyright
Other