Published April 1994 | Version v1
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Influence of supersymmetric particle pair emission by electron on evolution of neutron star

Creators

  • 1. Moscow State Univ., Moscow (Russian Federation). Dept. of Theoretical Physics

Description

The processes of emission of a pair of supersymmetric particles (wino and sneutrino or selection and photino) by electron in strong magnetic field of neutron star are discussed. The contributions to the energy losses of the neutron star due to these processes are calculated. The comparison of these new proposed mechanisms of energy losses with the standard neutrino mechanism is presented. (author). 25 refs

Availability note (English)

MF available from INIS under the Report Number.

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Additional details

Publishing Information

Imprint Pagination
12 p.
Report number
IC--94/60

INIS

Country of Publication
International Atomic Energy Agency (IAEA)
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
26045789
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Descriptors DEI
COSMIC ELECTRONS; ENERGY LOSSES; LUMINOSITY; MAGNETIC FIELDS; NEUTRINOS; NEUTRON STARS; PAIR PRODUCTION; SPARTICLES; SUPERSYMMETRY; TEMPERATURE DEPENDENCE
Descriptors DEC
COSMIC RADIATION; ELECTRONS; ELEMENTARY PARTICLES; FERMIONS; IONIZING RADIATIONS; LEPTONS; MASSLESS PARTICLES; OPTICAL PROPERTIES; PARTICLE PRODUCTION; PHYSICAL PROPERTIES; POSTULATED PARTICLES; RADIATIONS; SECONDARY COSMIC RADIATION; STARS; SYMMETRY