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: Blaschke, David
Další autoři: Glendenning, Norman K. (Šéfredaktor, odpovědný redaktor), Sedrakian, A., 1965- (Šéfredaktor, odpovědný redaktor)
Médium: Livre numérique
Jazyk:Anglais
Vydáno: Berlin [etc.] : Springer [20..].
Cham : Springer Nature
Edice:Lecture notes in physics 578
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Poznámka: Archives Springer e-books (Licence nationale)
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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.