Actions for Quark core stars, quark stars and strange stars [electronic resource].
Quark core stars, quark stars and strange stars [electronic resource].
- Published
- Batavia, Ill. : Fermi National Accelerator Laboratory, 1988.
Oak Ridge, Tenn. : Distributed by the Office of Scientific and Technical Information, U.S. Dept. of Energy. - Physical Description
- Pages: 38 : digital, PDF file
- Additional Creators
- Fermi National Accelerator Laboratory and United States. Department of Energy. Office of Scientific and Technical Information
Access Online
- Restrictions on Access
- Free-to-read Unrestricted online access
- Summary
- A recent one flavor quark matter equation of state is generalized to several flavors. It is shown that quarks undergo a first order phase transition. In addition, this equation of state depends on just one parameter in the two flavor case, two parameters in the three flavor case, and these parameters are constrained by phenomenology. This equation of state is then applied to the hadron-quark transition in neutron stars and the determination of quark star stability, the investigation of strange matter stability and possible strange star existence. 43 refs., 6 figs.
- Report Numbers
- E 1.99:fnal/pub-88/19-a
fnal/pub-88/19-a - Subject(s)
- Other Subject(s)
- Quark Matter
- Equations Of State
- Flavor Model
- Stars
- Boundary Conditions
- Differential Equations
- Equilibrium
- Free Energy
- General Relativity Theory
- Neutron Stars
- Phase Transformations
- Quark-Hadron Interactions
- Stability
- Composite Models
- Energy
- Equations
- Field Theories
- Interactions
- Mathematical Models
- Matter
- Particle Interactions
- Particle Models
- Physical Properties
- Quark Model
- Thermodynamic Properties
- Note
- Published through SciTech Connect.
01/01/1988.
"fnal/pub-88/19-a"
"DE88006991"
Grassi, F. - Funding Information
- AC02-76CH03000
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