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Hadron star modelsThe 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 about 25%. During hadron star formation, much of this energy will be released. The consequences, resulting from the release of this energy, are examined.
Document ID
19740049645
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Cohen, J. M. (NASA Goddard Space Flight Center High Energy Astrophysics Laboratory, Greenbelt, Md.; Pennsylvania, University, Philadelphia, Pa., United States)
Boerner, G. (NASA Goddard Space Flight Center High Energy Astrophysics Laboratory, Greenbelt, Md.; Max-Planck-Institut fuer Physik und Astrophysik, Germany)
Date Acquired
August 7, 2013
Publication Date
January 1, 1974
Subject Category
Space Sciences
Meeting Information
Meeting: Symposium on Physics of dense matter
Location: Boulder, CO
Start Date: August 21, 1972
End Date: August 25, 1972
Accession Number
74A32395
Distribution Limits
Public
Copyright
Other

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