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Neutron Stars: Theory and Observation (Paperback, Softcover reprint of the original 1st ed. 1991)
Loot Price: R8,665
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Neutron Stars: Theory and Observation (Paperback, Softcover reprint of the original 1st ed. 1991)
Series: NATO Science Series C, 344
Expected to ship within 10 - 15 working days
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Some twenty-three years after the discovery of pulsars and their
identification as rotating neutron stars, neutron star physics may
be regarded as comingofage. Pul sars and accreting neutron stars
have now been studied at every wavelength, from the initial radio
observations, through optical, X-, and "{-ray, up to the very
recent observations in the TeV region, while theorists have studied
in some detail relevant physical processes both outside and inside
neutron stars. As a result, comparisonof theory with observation
provides a test ofour theoretical ideas in fields as diverse as
neutron and nuclear matter, superfluidity and superconductivity,
the acceleration of high energy particles, and the generation and
maintenance of intense magnetic fields. For example, through
observations of glitches and post glitch behavior of pulsars, it
has become possible to establish the presence ofsuperfluid neutron
mat ter in the inner crust of neutron stars, and to determine some
of its properties, while neutron stars in compact binary systems
offer one ofthe most efficient energy generation mechanisms known.
It is in fact the interactive interpretation of these ,diverse
pieces of information that can lead to major advances in our
understanding of the physics of these exotic objects, and justifies
the characterization of neutron stars as hadron physics
laboratories.
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