Superdense QCD Matter and Compact Stars
2 Homogeneous superconducting state 210 3 Superconducting phases with broken space symmetries 213 4 Flavor asymmetric quark condensates 219 5 Concluding remarks 221 Acknowledgments 222 References 223 Neutral Dense Quark Matter 225 Mei Huang and Igor Shovkovy 1 Introduction 225 2 Local charge neutral...
Συγγραφή απο Οργανισμό/Αρχή: | |
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Άλλοι συγγραφείς: | , |
Μορφή: | Ηλεκτρονική πηγή Ηλ. βιβλίο |
Γλώσσα: | English |
Έκδοση: |
Dordrecht :
Springer Netherlands,
2006.
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Σειρά: | NATO Science Series II: Mathematics, Physics and Chemistry,
197 |
Θέματα: | |
Διαθέσιμο Online: | Full Text via HEAL-Link |
Πίνακας περιεχομένων:
- Compact Stars
- DYNAMIC STABILITY OF COMPACT STARS
- CONSTRAINTS ON SUPERDENSEMATTER FROM X-RAY BINARIES
- POSTGLITCH RELAXATIONS OF ANGULAR VELOCITY OF PULSARS
- ISOLATED NEUTRON STARS: AN ASTROPHYSICAL PERSPECTIVE
- Superdense QCD Matter
- CLUSTERS AND CONDENSATES IN THE NUCLEARMATTER EQUATIONOF STATE
- NUCLEAR EQUATION OF STATE AND THESTRUCTURE OF NEUTRON STARS
- NEUTRON STAR STRUCTURE WITH HYPERONS AND QUARKS
- THE QCD EQUATION OF STATE AND QUARK STAR PROPERTIES
- EFFECTIVE LAGRANGIANS FOR QCD: DUALITY AND EXACT RESULTS
- COLOR SUPERCONDUCTIVITY AND HIGH DENSITY EFFECTIVE THEORY
- COLOR SUPERCONDUCTING QUARK MATTERAND THE INTERIOR OF NEUTRON STARS
- SUPERCONDUCTIVITY WITH DEFORMED FERMI SURFACES AND COMPACT STARS
- NEUTRAL DENSE QUARK MATTER
- POSSIBILITY OF COLOR MAGNETIC SUPERCONDUCTIVITY
- MAGNETIC FIELDS OF COMPACT STARS WITH SUPERCONDUCTING QUARK CORES
- THERMAL COLOR-SUPERCONDUCTING FLUCTUATIONS IN DENSE QUARK MATTER
- THE INNER STRUCTURE OF HYBRID STARS
- Signals for Superdense QCD Matter in Compact Stars
- GAMMA-RAY BURSTS AND THEIR CENTRAL ENGINES
- SUPERDENSE STARSWITH A QUARK CORE
- DIQUARKCONDENSATION EFFECTSON HOT QUARK STAR CONFIGURATIONS
- GAMMA RAY BURSTS AND DELAYED QUARK-DECONFINEMENT
- COLOR SUPERCONDUCTING QUARK MATTER AND COMPACT STAR OBSERVABLES
- LOOKING INSIDE THE EARTHWITH SOLARAND SUPERNOVA NEUTRINOS: AN ANALYTIC APPROACH
- DECONFINEMENT PHASE TRANSITION IN RELATIVISTIC NEUTRON STAR MERGERS.