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010   $a1-280-38210-4
010   $a9786613560018
010   $a3-642-12866-1
024 7 $a10.1007/978-3-642-12866-0
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035   $a(SSID)ssj0000449296
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035   $a(PQKBTitleCode)TC0000449296
035   $a(PQKBWorkID)10427811
035   $a(PQKB)11504853
035   $a(DE-He213)978-3-642-12866-0
035   $a(MiAaPQ)EBC3065689
035   $z(PPN)25884602X
035   $a(PPN)14902049X
035   $a(EXLCZ)992670000000036615
100   $a20100825d2010      u|             0
101 0 $aeng
135   $aurnn|008mamaa
181   $ctxt
182   $cc
183   $acr
200 10$aDense Matter in Compact Stars$b[electronic resource] $eA Pedagogical Introduction /$fby Andreas Schmitt
205   $a1st ed. 2010.
210  1$aBerlin, Heidelberg :$cSpringer Berlin Heidelberg :$cImprint: Springer,$d2010.
215   $a1 online resource (X, 147 p. 23 illus.) 
225 1 $aLecture Notes in Physics,$x0075-8450 ;$v811
300   $aBibliographic Level Mode of Issuance: Monograph
311   $a3-642-12865-3 
320   $aIncludes bibliographical references and index.
327   $aMass and Radius of the Star -- Basic Models and Properties of Dense Nuclear Matter -- Superconductivity and Superfluidity in a Compact Star -- Neutrino Emissivity and Cooling of the Star -- Discussion.
330   $aThe purpose of these lectures is to address the following two strongly coupled issues: ? What is the ground state (and its properties) of dense (quark) matter? ? What is the matter composition of a compact star? In order to fulfill their primary goal - to remain both concise and accessible to the beginning graduate student or other newcomers to the field - the only prerequisites are a working knowledge of statistical mechanics and thermodynamics as well as a first course in quantum field theory. More advanced material will be introduced as the text progresses and an appendix covers basic elements of thermal quantum field theory at finite chemical potential. Instead of developing all relevant formal tools (which is not even fully possible in the regime of QCD considered here), calculations are physically motivated, making the reader familiar with the theories and technicalities by ?learning by doing?. In this way these lectures will guide and prepare the reader towards further investigations and own theoretical research in this exciting field at the interface of nuclear, particle and astrophysics.
410  0$aLecture Notes in Physics,$x0075-8450 ;$v811
606   $aAstrophysics
606   $aSpace sciences
606   $aNuclear physics
606   $aHeavy ions
606   $aElementary particles (Physics)
606   $aQuantum field theory
606   $aAstrophysics and Astroparticles$3https://scigraph.springernature.com/ontologies/product-market-codes/P22022
606   $aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics)$3https://scigraph.springernature.com/ontologies/product-market-codes/P22030
606   $aNuclear Physics, Heavy Ions, Hadrons$3https://scigraph.springernature.com/ontologies/product-market-codes/P23010
606   $aElementary Particles, Quantum Field Theory$3https://scigraph.springernature.com/ontologies/product-market-codes/P23029
615  0$aAstrophysics.
615  0$aSpace sciences.
615  0$aNuclear physics.
615  0$aHeavy ions.
615  0$aElementary particles (Physics).
615  0$aQuantum field theory.
615 14$aAstrophysics and Astroparticles.
615 24$aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics).
615 24$aNuclear Physics, Heavy Ions, Hadrons.
615 24$aElementary Particles, Quantum Field Theory.
676   $a523.8
700   $aSchmitt$b Andreas$4aut$4http://id.loc.gov/vocabulary/relators/aut$0515327
906   $aBOOK
912   $a996466708503316
996   $aDense Matter in Compact Stars$9855611
997   $aUNISA