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Curvature radiation radio maser in a pulsar magnetosphere

Journal Article · · Astrophysics (Engl. Transl.); (United States)
DOI:https://doi.org/10.1007/BF01014857· OSTI ID:6069502
;
The mechanism of generation of radio emission of pulsars due to the motion of charged relativistic particles along curved magnetic field lines is considered. The reabsorption of electromagnetic waves by a stream of charged relativistic particles moving along a curved trajectory is calculated and investigated in the kinetic approximation. The conditions under which maser amplification of waves in neutron star magnetospheres is possible are found.
Research Organization:
Institute of Applied Physics, Gor'kii (USSR)
OSTI ID:
6069502
Journal Information:
Astrophysics (Engl. Transl.); (United States), Journal Name: Astrophysics (Engl. Transl.); (United States) Vol. 28:1; ISSN ATPYA
Country of Publication:
United States
Language:
English

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Related Subjects

640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ABSORPTION
AMPLIFICATION
AMPLIFIERS
ATMOSPHERES
CHARGED PARTICLES
CHARGED-PARTICLE TRANSPORT THEORY
COSMIC RADIO SOURCES
ELECTROMAGNETIC RADIATION
ELECTRON DRIFT
ELECTRONIC EQUIPMENT
ELECTRONS
ELEMENTARY PARTICLES
EMISSION
ENERGY ABSORPTION
ENERGY RANGE
ENERGY-LEVEL TRANSITIONS
EQUIPMENT
FERMIONS
INHOMOGENEOUS FIELDS
LEPTONS
MAGNETIC FIELDS
MASERS
MICROWAVE AMPLIFIERS
MICROWAVE EQUIPMENT
MICROWAVE RADIATION
NEUTRON STARS
POPULATION INVERSION
PULSARS
RADIATIONS
RADIOWAVE RADIATION
RELATIVISTIC RANGE
STARS
STELLAR ATMOSPHERES
STELLAR MAGNETOSPHERES
STIMULATED EMISSION
TRAJECTORIES
TRANSPORT THEORY
WAVE PROPAGATION