000 | 03598nam a22005295i 4500 | ||
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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 |
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024 | 7 |
_a10.1007/3-540-44578-1 _2doi |
|
050 | 4 | _aQB1-991 | |
050 | 4 | _aQB460-466 | |
050 | 4 | _aQB980-991 | |
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_aPGC _2bicssc |
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_aSCI004000 _2bisacsh |
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_aPGC _2thema |
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_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. |
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336 |
_atext _btxt _2rdacontent |
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337 |
_acomputer _bc _2rdamedia |
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338 |
_aonline resource _bcr _2rdacarrier |
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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 |
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_iPrinted edition: _z9783540423409 |
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_iPrinted edition: _z9783662143117 |
830 | 0 |
_aLecture Notes in Physics, _x0075-8450 ; _v578 |
|
856 | 4 | 0 | _uhttps://doi.org/10.1007/3-540-44578-1 |
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