Physics of Neutron Star Interiors
Neutron stars are the densest observable bodies in our universe. Born during the gravitational collapse of luminous stars - a birth heralded by spectacular supernova explosions - they open a window on a world where the state of the matter and the strengths of the fields are anything but ordinary. Th...
Συγγραφή απο Οργανισμό/Αρχή: | |
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Άλλοι συγγραφείς: | , , |
Μορφή: | Ηλεκτρονική πηγή Ηλ. βιβλίο |
Γλώσσα: | English |
Έκδοση: |
Berlin, Heidelberg :
Springer Berlin Heidelberg : Imprint: Springer,
2001.
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Έκδοση: | 1st ed. 2001. |
Σειρά: | Lecture Notes in Physics,
578 |
Θέματα: | |
Διαθέσιμο Online: | Full Text via HEAL-Link |
Πίνακας περιεχομένων:
- Microscopic Theory of the Nuclear Equation of State and Neutron Star Structure
- Superfluidity in Neutron Star Matter
- Relativistic Superfluid Models for Rotating Neutron Stars
- The Tensor Virial Method and Its Applications to Self-Gravitating Superfluids
- Neutron Star Crusts
- Kaon Condensation in Neutron Stars
- Phases of QCD at High Baryon Density
- Diquarks in Dense Matter
- Color Superconductivity in Compact Stars
- Strange Quark Stars: Structural Properties and Possible Signatures for Their Existence
- Phase Diagram for Spinning and Accreting Neutron Stars
- Signal of Quark Deconfinement in Millisecond Pulsars and Reconfinement in Accreting X-ray Neutron Stars
- Supernova Explosions and Neutron Star Formation
- Evolution of a Neutron Star from Its Birth to Old Age
- Neutron Star Kicks and Asymmetric Supernovae
- Spin and Magnetism in Old Neutron Stars
- Neutrino Cooling of Neutron Stars: Medium Effects.