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...
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| Hlavní autor: | |
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| Další autoři: | , |
| Médium: | Livre numérique |
| Jazyk: | Anglais |
| Vydáno: |
Berlin [etc.] :
Springer
[20..].
Cham : Springer Nature |
| Edice: | Lecture notes in physics
578 |
| Témata: | |
| On-line přístup: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
| Poznámka: |
Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| Autres localisations: | Voir dans le Sudoc |
| Edition sous un autre format: | • Physics of neutron star interiors, D. Blaschke, N.K. Glendenning, A. Sedrakian, eds., New York, Springer, 2001, 1 volume (XI - 509 p.), Lecture notes in physics, 3-540-42340-0 • Physics of Neutron Star Interiors, Texte imprimé, 9783642076145 • Physics of Neutron Star Interiors, Texte imprimé, 9783662143117 |
Obsah:
- 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.

