Neutron stars are the densest objects known in our universe that have not collapsed in on themselves to form a singularity (a black hole). Like black holes they are formed when stars run out of nuclear fuel and radiation pressure can no longer withstand the pull of gravitational forces.This book gives you an in-depth look at how the Direct Urca process is a central element in the cooling of neutron stars after their forming, however it also provides brief introductions to neutron star physics in general, the history of neutron star physics, and pulsars - the pulsating stars that form the observational basis for neutron stars.The book also introduces the different relevant models for an equations of state for neutron stars and a chapter on hyperon matter, before it finally goes on to describe the cooling processes of neutron stars, all with the necessary mathemathical framework for an in-depth analysis.
Neutron stars are the densest objects known in our universe that have not collapsed in on themselves to form a singularity (a black hole). Like black holes they are formed when stars run out of nuclear fuel and radiation pressure can no longer withstand the pull of gravitational forces.This book gives you an in-depth look at how the Direct Urca process is a central element in the cooling of neutron stars after their forming, however it also provides brief introductions to neutron star physics in general, the history of neutron star physics, and pulsars - the pulsating stars that form the observational basis for neutron stars.The book also introduces the different relevant models for an equations of state for neutron stars and a chapter on hyperon matter, before it finally goes on to describe the cooling processes of neutron stars, all with the necessary mathemathical framework for an in-depth analysis.
The idea for organizing an Advanced Study Institute devoted largely to neutron star timing arose independently in three places, at Istanbul, Garching and Amster dam; when we became aware of each...
Thermonuclear burning in the matter accumulated on the surface of an accreting neutron star is unstable under certain conditions, which leads to powerful explosions also called Type I X-ray bursts...
The book gives an extended review of theoretical and observational aspects of neutron star physics. With masses comparable to that of the Sun and radii of about ten kilometres, neutron stars are the...
This NATO AS! was the third in the series of Advanced Study Institutes on neutron stars, which started with 'Timing Neutron Stars', held in Qe§me near izmir, Turkey (April 1988), followed by 'Neutron...
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