LEADER 03873nam 22006495 450 001 996466795503316 005 20200703043026.0 010 $a3-540-44578-1 024 7 $a10.1007/3-540-44578-1 035 $a(CKB)1000000000778211 035 $a(SSID)ssj0000325677 035 $a(PQKBManifestationID)11285601 035 $a(PQKBTitleCode)TC0000325677 035 $a(PQKBWorkID)10253158 035 $a(PQKB)10801585 035 $a(DE-He213)978-3-540-44578-4 035 $a(MiAaPQ)EBC3072079 035 $a(PPN)155223518 035 $a(EXLCZ)991000000000778211 100 $a20121227d2001 u| 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt 182 $cc 183 $acr 200 10$aPhysics of Neutron Star Interiors$b[electronic resource] /$fedited by D. Blaschke, N.K. Glendenning, A. Sedrakian 205 $a1st ed. 2001. 210 1$aBerlin, Heidelberg :$cSpringer Berlin Heidelberg :$cImprint: Springer,$d2001. 215 $a1 online resource (XI, 516 p.) 225 1 $aLecture Notes in Physics,$x0075-8450 ;$v578 300 $aBibliographic Level Mode of Issuance: Monograph 311 $a3-540-42340-0 320 $aIncludes bibliographical references and index. 327 $aMicroscopic 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. 330 $aNeutron stars are the densest observable bodies in our universe. Born during the gravitational collapse of luminous stars - a birth heralded by spectacular supernova explosions - they open a window on a world where the state of the matter and the strengths of the fields are anything but ordinary. This book is a collection of pedagogical lectures on the theory of neutron stars, and especially their interiors, at the forefront of current research. It addresses graduate students and researchers alike, and should be particularly suitable as a text bridging the gap between standard textbook material and the research literature. 410 0$aLecture Notes in Physics,$x0075-8450 ;$v578 606 $aAstronomy 606 $aAstrophysics 606 $aNuclear physics 606 $aAstronomy, Astrophysics and Cosmology$3https://scigraph.springernature.com/ontologies/product-market-codes/P22006 606 $aParticle and Nuclear Physics$3https://scigraph.springernature.com/ontologies/product-market-codes/P23002 615 0$aAstronomy. 615 0$aAstrophysics. 615 0$aNuclear physics. 615 14$aAstronomy, Astrophysics and Cosmology. 615 24$aParticle and Nuclear Physics. 676 $a523.8/874 702 $aBlaschke$b D$4edt$4http://id.loc.gov/vocabulary/relators/edt 702 $aGlendenning$b N.K$4edt$4http://id.loc.gov/vocabulary/relators/edt 702 $aSedrakian$b A$4edt$4http://id.loc.gov/vocabulary/relators/edt 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a996466795503316 996 $aPhysics of Neutron Star Interiors$9377936 997 $aUNISA