000 | 03439nam a22005055i 4500 | ||
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001 | 978-3-642-12866-0 | ||
003 | DE-He213 | ||
005 | 20190213151710.0 | ||
007 | cr nn 008mamaa | ||
008 | 100825s2010 gw | s |||| 0|eng d | ||
020 |
_a9783642128660 _9978-3-642-12866-0 |
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024 | 7 |
_a10.1007/978-3-642-12866-0 _2doi |
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050 | 4 | _aQB460-466 | |
072 | 7 |
_aPHVB _2bicssc |
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_aSCI005000 _2bisacsh |
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_aPHVB _2thema |
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082 | 0 | 4 |
_a523.01 _223 |
100 | 1 |
_aSchmitt, Andreas. _eauthor. _4aut _4http://id.loc.gov/vocabulary/relators/aut |
|
245 | 1 | 0 |
_aDense Matter in Compact Stars _h[electronic resource] : _bA Pedagogical Introduction / _cby Andreas Schmitt. |
264 | 1 |
_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg : _bImprint: Springer, _c2010. |
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300 |
_aX, 147 p. 23 illus. _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 |
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490 | 1 |
_aLecture Notes in Physics, _x0075-8450 ; _v811 |
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505 | 0 | _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. | |
520 | _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. | ||
650 | 0 | _aAstrophysics. | |
650 | 0 | _aNuclear physics. | |
650 | 0 | _aQuantum theory. | |
650 | 1 | 4 |
_aAstrophysics and Astroparticles. _0http://scigraph.springernature.com/things/product-market-codes/P22022 |
650 | 2 | 4 |
_aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). _0http://scigraph.springernature.com/things/product-market-codes/P22030 |
650 | 2 | 4 |
_aNuclear Physics, Heavy Ions, Hadrons. _0http://scigraph.springernature.com/things/product-market-codes/P23010 |
650 | 2 | 4 |
_aElementary Particles, Quantum Field Theory. _0http://scigraph.springernature.com/things/product-market-codes/P23029 |
710 | 2 | _aSpringerLink (Online service) | |
773 | 0 | _tSpringer eBooks | |
776 | 0 | 8 |
_iPrinted edition: _z9783642128653 |
776 | 0 | 8 |
_iPrinted edition: _z9783642128677 |
830 | 0 |
_aLecture Notes in Physics, _x0075-8450 ; _v811 |
|
856 | 4 | 0 | _uhttps://doi.org/10.1007/978-3-642-12866-0 |
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912 | _aZDB-2-LNP | ||
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