Dense Matter in Compact Stars [recurso electrónico] : A Pedagogical Introduction / by Andreas Schmitt.

Por: Schmitt, Andreas [author.]Colaborador(es): SpringerLink (Online service)Tipo de material: TextoTextoSeries Lecture Notes in Physics ; 811Editor: Berlin, Heidelberg : Springer Berlin Heidelberg : Imprint: Springer, 2010Descripción: X, 147p. online resourceTipo de contenido: text Tipo de medio: computer Tipo de portador: online resourceISBN: 9783642128660Tema(s): Physics | Nuclear physics | Quantum theory | Physics | Astrophysics and Astroparticles | Nuclear Physics, Heavy Ions, Hadrons | Elementary Particles, Quantum Field TheoryFormatos físicos adicionales: Printed edition:: Sin títuloClasificación CDD: 523.01 Clasificación LoC:QB460-466Recursos en línea: Libro electrónicoTexto
Contenidos:
Mass 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.
En: Springer eBooksResumen: The 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.
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Tipo de ítem Biblioteca actual Colección Signatura Copia número Estado Fecha de vencimiento Código de barras
Libro Electrónico Biblioteca Electrónica
Colección de Libros Electrónicos QB460 -466 (Browse shelf(Abre debajo)) 1 No para préstamo 374365-2001

Mass 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.

The 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.

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