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Matter at High Densities in Astrophysics: Compact Stars and the Equation of State: Springer Tracts in Modern Physics, cartea 133

Autor Harald Riffert, Herbert Müther, Heinz Herold, Hanns Ruder
en Limba Engleză Paperback – 13 noi 2013
This volume is published in honor of Friedrich Hund's 100th birthday. It is a modern review on matter at high densities and pressures in astrophysics from Hund's early contribution to present-day ideas. The relation between the equation of state and the structure of compact cosmic objects is discussed, and two main contributions deal with the equation of state of baryonic matter at nuclear densities and with the numerical solution of the general relativistic field equations for non-rotating and rapidly rotating neutron stars. In a final chapter the present state of asteroseismology is presented as a tool to explore the interior of cosmic objects by analyzing the observed free oscillations of the Earth, the Sun, and white dwarf stars.
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Specificații

ISBN-13: 9783662140901
ISBN-10: 366214090X
Pagini: 292
Ilustrații: XIV, 275 p. 18 illus.
Dimensiuni: 155 x 235 x 15 mm
Greutate: 0.41 kg
Ediția:Softcover reprint of the original 1st ed. 1996
Editura: Springer Berlin, Heidelberg
Colecția Springer
Seria Springer Tracts in Modern Physics

Locul publicării:Berlin, Heidelberg, Germany

Public țintă

Research

Cuprins

The equation of state and the structure of cosmic objects.- Nuclear equations of state.- Neutron stars: Spherically symmetric and rotating models.- Asteroseismology.

Textul de pe ultima copertă

This volume is published in honor of Friedrich Hund's 100th birthday. It is a modern review on matter at high densities and pressures in astrophysics from Hund's early contribution to present-day ideas. The relation between the equation of state and the structure of compact cosmic objects is discussed, and two main contributions deal with the equation of state of baryonic matter at nuclear densities and with the numerical solution of the general relativistic field equations for non-rotating and rapidly rotating neutron stars. In a final chapter the present state of asteroseismology is presented as a tool to explore the interior of cosmic objects by analyzing the observed free oscillations of the Earth, the Sun, and white dwarf stars.