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001 978-3-540-44578-4
003 DE-He213
005 20190213151249.0
007 cr nn 008mamaa
008 121227s2001 gw | s |||| 0|eng d
020 _a9783540445784
_9978-3-540-44578-4
024 7 _a10.1007/3-540-44578-1
_2doi
050 4 _aQB1-991
050 4 _aQB460-466
050 4 _aQB980-991
072 7 _aPGC
_2bicssc
072 7 _aSCI004000
_2bisacsh
072 7 _aPGC
_2thema
082 0 4 _a520
_223
245 1 0 _aPhysics of Neutron Star Interiors
_h[electronic resource] /
_cedited by David Blaschke, Armen Sedrakian, Norman K. Glendenning.
264 1 _aBerlin, Heidelberg :
_bSpringer Berlin Heidelberg,
_c2001.
300 _aXI, 516 p.
_bonline resource.
336 _atext
_btxt
_2rdacontent
337 _acomputer
_bc
_2rdamedia
338 _aonline resource
_bcr
_2rdacarrier
347 _atext file
_bPDF
_2rda
490 1 _aLecture Notes in Physics,
_x0075-8450 ;
_v578
505 0 _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.
520 _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.
650 0 _aAstronomy.
650 1 4 _aAstronomy, Astrophysics and Cosmology.
_0http://scigraph.springernature.com/things/product-market-codes/P22006
650 2 4 _aParticle and Nuclear Physics.
_0http://scigraph.springernature.com/things/product-market-codes/P23002
700 1 _aBlaschke, David.
_eeditor.
_4edt
_4http://id.loc.gov/vocabulary/relators/edt
700 1 _aSedrakian, Armen.
_eeditor.
_4edt
_4http://id.loc.gov/vocabulary/relators/edt
700 1 _aGlendenning, Norman K.
_eeditor.
_4edt
_4http://id.loc.gov/vocabulary/relators/edt
710 2 _aSpringerLink (Online service)
773 0 _tSpringer eBooks
776 0 8 _iPrinted edition:
_z9783642076145
776 0 8 _iPrinted edition:
_z9783540423409
776 0 8 _iPrinted edition:
_z9783662143117
830 0 _aLecture Notes in Physics,
_x0075-8450 ;
_v578
856 4 0 _uhttps://doi.org/10.1007/3-540-44578-1
912 _aZDB-2-PHA
912 _aZDB-2-LNP
912 _aZDB-2-BAE
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