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Hadron Star Models

Published online by Cambridge University Press:  14 August 2015

Jeffrey M. Cohen  and
Gerhard Börner
Jeffrey M. Cohen*
Affiliation:
High Energy Astrophysics Laboratory, Goddard Space Flight Center, Greenbelt, Md., U.S.A.
Gerhard Börner*
Affiliation:
High Energy Astrophysics Laboratory, Goddard Space Flight Center, Greenbelt, Md., U.S.A.
*
∗Permanent address: Physics Department, University of Pennsylvania, Philadelphia, Pa. 19104. National Academy of Science – NRC Senior Research Associate.
∗∗Permanent address: Max-Planck Institut für Physik and Astrophysik, München, Germany. National Academy of Science – NRC Research Associate.

Abstract

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The properties of fully relativistic rotating hadron star models are discussed using models based on recently developed equations of state. All of these stable neutron star models are bound with binding energies as high as ∼ 25%. During hadron star formation, much of this energy will be released. The consequences, resulting from the release of this energy, are examined.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 53: Physics of Dense Matter , 1974 , pp. 237 - 250
Copyright
Copyright © Reidel 1974 

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