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The Evolution of Supernova Remnants as Radio Sources

Symposium - International Astronomical Union Cambridge University Press (CUP) 101 (1983) 187-192

Authors:

R Cowsik, S Sarkar

Abstract:

The acceleration of relativistic electrons by hydromagnetic turbulence in shell-type supernova remnants (SNRs) is examined within the framework of previous studies of their structural evolution through interaction with the interstellar medium. The predicted evolution of the synchrotron radio emission by the electrons is in agreement with a wide variety of observations.
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Does the galactic synchrotron radio background originate in old supernova remnants?

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 199:1 (1982) 97-108
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A NEW PROPOSAL FOR MONTE-CARLO SIMULATION OF FERMIONS ON A LATTICE

PHYSICS LETTERS B 116:4 (1982) 287-290

Authors:

SJ ANTHONY, CHL SMITH, JF WHEATER
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ELECTROWEAK RADIATIVE-CORRECTIONS TO NEUTRINO AND ELECTRON-SCATTERING AND THE VALUE OF SIN2-THETA-W

NUCLEAR PHYSICS B 208:1 (1982) 27-76

Authors:

JF WHEATER, CHL SMITH
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ELECTROWEAK RADIATIVE-CORRECTIONS

JOURNAL DE PHYSIQUE 43:NC3 (1982) 305-309
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