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)