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Relativistic Mean Field Models of Neutron Stars (2007)
EN PB USISBN: 9788322617069 bzw. 8322617062, in Englisch, 196 Seiten, Silesia University Press, Taschenbuch, gebraucht.
Lieferung aus: Vereinigtes Königreich Großbritannien und Nordirland, Usually dispatched within 1-2 business days, plus shipping (if shipped).
Von Händler/Antiquariat, killarneybookseu.
1 Introduction 2 Stellar structure equations 3 Thermodynamic properties of stellar matter 3.1 Photon gas 3.2 Fermion gas 3.2.1 Completely degenerate fermion gas 3.2.2 Partially degenerate fermion gas 3.2.3 Neutrino gas 4 Equation of state of stellar matter 4.1 The ideal classical gas 4.2 The degenerate gas 4.2.1 White dwarfs 4.2.2 Proto-neutron stars 4.2.3 Neutron stars 5 The nuclear equation of state 5.1 Compressibility of nuclear matter 5.2 Nuclear symmetry energy 6 Relativistic mean field model 6.1 Walecka model and its extensions 6.2 Model with nonlinear isoscalar-isovector interaction terms 6.3 Model with δ meson 6.4 Model with nonzero temperature 6.5 Leptons 7 Strange nuclear matter 7.1 The effective field theoretical model 8 Properties of nuclear matter 8.1 Infinite symmetric nuclear matter 8.2 Infinite symmetric strange hadronic matter 8.3 Asymmetric nuclear matter 8.4 Asymmetric strangeness-rich matter 9 Neutron star matter 9.1 The equilibrium conditions and composition of stellar matter 9.2 Neutron star matter with zero strangeness 10 Strange neutron star matter 11 Astrophysical constraints on the equation of state 12 Proto-neutron star model 12.1 Neutrino opacities 12.2 The influence of neutrino trapping on proto-neutron star properties and evolution 13 Conclusions / Bibliography, Paperback, Label: Silesia University Press, Silesia University Press, Product group: Book, Published: 2007-01-01, Studio: Silesia University Press.
Von Händler/Antiquariat, killarneybookseu.
1 Introduction 2 Stellar structure equations 3 Thermodynamic properties of stellar matter 3.1 Photon gas 3.2 Fermion gas 3.2.1 Completely degenerate fermion gas 3.2.2 Partially degenerate fermion gas 3.2.3 Neutrino gas 4 Equation of state of stellar matter 4.1 The ideal classical gas 4.2 The degenerate gas 4.2.1 White dwarfs 4.2.2 Proto-neutron stars 4.2.3 Neutron stars 5 The nuclear equation of state 5.1 Compressibility of nuclear matter 5.2 Nuclear symmetry energy 6 Relativistic mean field model 6.1 Walecka model and its extensions 6.2 Model with nonlinear isoscalar-isovector interaction terms 6.3 Model with δ meson 6.4 Model with nonzero temperature 6.5 Leptons 7 Strange nuclear matter 7.1 The effective field theoretical model 8 Properties of nuclear matter 8.1 Infinite symmetric nuclear matter 8.2 Infinite symmetric strange hadronic matter 8.3 Asymmetric nuclear matter 8.4 Asymmetric strangeness-rich matter 9 Neutron star matter 9.1 The equilibrium conditions and composition of stellar matter 9.2 Neutron star matter with zero strangeness 10 Strange neutron star matter 11 Astrophysical constraints on the equation of state 12 Proto-neutron star model 12.1 Neutrino opacities 12.2 The influence of neutrino trapping on proto-neutron star properties and evolution 13 Conclusions / Bibliography, Paperback, Label: Silesia University Press, Silesia University Press, Product group: Book, Published: 2007-01-01, Studio: Silesia University Press.
2
Relativistic Mean Field Models of Neutron Stars (2007)
EN PB USISBN: 9788322617069 bzw. 8322617062, in Englisch, 196 Seiten, Silesia University Press, Taschenbuch, gebraucht.
Lieferung aus: Deutschland, Versandfertig in 1 - 2 Werktagen, plus shipping (if shipped).
Von Händler/Antiquariat, killarneybookseu.
1 Introduction 2 Stellar structure equations 3 Thermodynamic properties of stellar matter 3.1 Photon gas 3.2 Fermion gas 3.2.1 Completely degenerate fermion gas 3.2.2 Partially degenerate fermion gas 3.2.3 Neutrino gas 4 Equation of state of stellar matter 4.1 The ideal classical gas 4.2 The degenerate gas 4.2.1 White dwarfs 4.2.2 Proto-neutron stars 4.2.3 Neutron stars 5 The nuclear equation of state 5.1 Compressibility of nuclear matter 5.2 Nuclear symmetry energy 6 Relativistic mean field model 6.1 Walecka model and its extensions 6.2 Model with nonlinear isoscalar-isovector interaction terms 6.3 Model with δ meson 6.4 Model with nonzero temperature 6.5 Leptons 7 Strange nuclear matter 7.1 The effective field theoretical model 8 Properties of nuclear matter 8.1 Infinite symmetric nuclear matter 8.2 Infinite symmetric strange hadronic matter 8.3 Asymmetric nuclear matter 8.4 Asymmetric strangeness-rich matter 9 Neutron star matter 9.1 The equilibrium conditions and composition of stellar matter 9.2 Neutron star matter with zero strangeness 10 Strange neutron star matter 11 Astrophysical constraints on the equation of state 12 Proto-neutron star model 12.1 Neutrino opacities 12.2 The influence of neutrino trapping on proto-neutron star properties and evolution 13 Conclusions / Bibliography, Taschenbuch, Label: Silesia University Press, Silesia University Press, Product group: Book, Published: 2007-01-01, Studio: Silesia University Press.
Von Händler/Antiquariat, killarneybookseu.
1 Introduction 2 Stellar structure equations 3 Thermodynamic properties of stellar matter 3.1 Photon gas 3.2 Fermion gas 3.2.1 Completely degenerate fermion gas 3.2.2 Partially degenerate fermion gas 3.2.3 Neutrino gas 4 Equation of state of stellar matter 4.1 The ideal classical gas 4.2 The degenerate gas 4.2.1 White dwarfs 4.2.2 Proto-neutron stars 4.2.3 Neutron stars 5 The nuclear equation of state 5.1 Compressibility of nuclear matter 5.2 Nuclear symmetry energy 6 Relativistic mean field model 6.1 Walecka model and its extensions 6.2 Model with nonlinear isoscalar-isovector interaction terms 6.3 Model with δ meson 6.4 Model with nonzero temperature 6.5 Leptons 7 Strange nuclear matter 7.1 The effective field theoretical model 8 Properties of nuclear matter 8.1 Infinite symmetric nuclear matter 8.2 Infinite symmetric strange hadronic matter 8.3 Asymmetric nuclear matter 8.4 Asymmetric strangeness-rich matter 9 Neutron star matter 9.1 The equilibrium conditions and composition of stellar matter 9.2 Neutron star matter with zero strangeness 10 Strange neutron star matter 11 Astrophysical constraints on the equation of state 12 Proto-neutron star model 12.1 Neutrino opacities 12.2 The influence of neutrino trapping on proto-neutron star properties and evolution 13 Conclusions / Bibliography, Taschenbuch, Label: Silesia University Press, Silesia University Press, Product group: Book, Published: 2007-01-01, Studio: Silesia University Press.
3
Relativistic Mean Field Models of Neutron Stars (2007)
EN USISBN: 9788322617069 bzw. 8322617062, in Englisch, 196 Seiten, Silesia University Press, gebraucht.
Lieferung aus: Frankreich, Expédition sous 1 à 2 jours ouvrés.
Von Händler/Antiquariat, killarneybookseu.
1 Introduction 2 Stellar structure equations 3 Thermodynamic properties of stellar matter 3.1 Photon gas 3.2 Fermion gas 3.2.1 Completely degenerate fermion gas 3.2.2 Partially degenerate fermion gas 3.2.3 Neutrino gas 4 Equation of state of stellar matter 4.1 The ideal classical gas 4.2 The degenerate gas 4.2.1 White dwarfs 4.2.2 Proto-neutron stars 4.2.3 Neutron stars 5 The nuclear equation of state 5.1 Compressibility of nuclear matter 5.2 Nuclear symmetry energy 6 Relativistic mean field model 6.1 Walecka model and its extensions 6.2 Model with nonlinear isoscalar-isovector interaction terms 6.3 Model with δ meson 6.4 Model with nonzero temperature 6.5 Leptons 7 Strange nuclear matter 7.1 The effective field theoretical model 8 Properties of nuclear matter 8.1 Infinite symmetric nuclear matter 8.2 Infinite symmetric strange hadronic matter 8.3 Asymmetric nuclear matter 8.4 Asymmetric strangeness-rich matter 9 Neutron star matter 9.1 The equilibrium conditions and composition of stellar matter 9.2 Neutron star matter with zero strangeness 10 Strange neutron star matter 11 Astrophysical constraints on the equation of state 12 Proto-neutron star model 12.1 Neutrino opacities 12.2 The influence of neutrino trapping on proto-neutron star properties and evolution 13 Conclusions / Bibliography, Broché, Label: Silesia University Press, Silesia University Press, Product group: Book, Published: 2007-01-01, Studio: Silesia University Press.
Von Händler/Antiquariat, killarneybookseu.
1 Introduction 2 Stellar structure equations 3 Thermodynamic properties of stellar matter 3.1 Photon gas 3.2 Fermion gas 3.2.1 Completely degenerate fermion gas 3.2.2 Partially degenerate fermion gas 3.2.3 Neutrino gas 4 Equation of state of stellar matter 4.1 The ideal classical gas 4.2 The degenerate gas 4.2.1 White dwarfs 4.2.2 Proto-neutron stars 4.2.3 Neutron stars 5 The nuclear equation of state 5.1 Compressibility of nuclear matter 5.2 Nuclear symmetry energy 6 Relativistic mean field model 6.1 Walecka model and its extensions 6.2 Model with nonlinear isoscalar-isovector interaction terms 6.3 Model with δ meson 6.4 Model with nonzero temperature 6.5 Leptons 7 Strange nuclear matter 7.1 The effective field theoretical model 8 Properties of nuclear matter 8.1 Infinite symmetric nuclear matter 8.2 Infinite symmetric strange hadronic matter 8.3 Asymmetric nuclear matter 8.4 Asymmetric strangeness-rich matter 9 Neutron star matter 9.1 The equilibrium conditions and composition of stellar matter 9.2 Neutron star matter with zero strangeness 10 Strange neutron star matter 11 Astrophysical constraints on the equation of state 12 Proto-neutron star model 12.1 Neutrino opacities 12.2 The influence of neutrino trapping on proto-neutron star properties and evolution 13 Conclusions / Bibliography, Broché, Label: Silesia University Press, Silesia University Press, Product group: Book, Published: 2007-01-01, Studio: Silesia University Press.
4
Relativistic Mean Field Models of Neutron Stars (2007)
EN PB USISBN: 9788322617069 bzw. 8322617062, in Englisch, 196 Seiten, Silesia University Press, Taschenbuch, gebraucht.
Lieferung aus: Deutschland, Versandfertig in 1 - 2 Werktagen, plus koszty przesyłki (Jeśli wysłane).
Von Händler/Antiquariat, killarneybookseu.
1 Introduction 2 Stellar structure equations 3 Thermodynamic properties of stellar matter 3.1 Photon gas 3.2 Fermion gas 3.2.1 Completely degenerate fermion gas 3.2.2 Partially degenerate fermion gas 3.2.3 Neutrino gas 4 Equation of state of stellar matter 4.1 The ideal classical gas 4.2 The degenerate gas 4.2.1 White dwarfs 4.2.2 Proto-neutron stars 4.2.3 Neutron stars 5 The nuclear equation of state 5.1 Compressibility of nuclear matter 5.2 Nuclear symmetry energy 6 Relativistic mean field model 6.1 Walecka model and its extensions 6.2 Model with nonlinear isoscalar-isovector interaction terms 6.3 Model with δ meson 6.4 Model with nonzero temperature 6.5 Leptons 7 Strange nuclear matter 7.1 The effective field theoretical model 8 Properties of nuclear matter 8.1 Infinite symmetric nuclear matter 8.2 Infinite symmetric strange hadronic matter 8.3 Asymmetric nuclear matter 8.4 Asymmetric strangeness-rich matter 9 Neutron star matter 9.1 The equilibrium conditions and composition of stellar matter 9.2 Neutron star matter with zero strangeness 10 Strange neutron star matter 11 Astrophysical constraints on the equation of state 12 Proto-neutron star model 12.1 Neutrino opacities 12.2 The influence of neutrino trapping on proto-neutron star properties and evolution 13 Conclusions / Bibliography, Taschenbuch, Etykieta: Silesia University Press, Silesia University Press, Grupy produktów: Book, Opublikowany: 2007-01-01, Studio: Silesia University Press.
Von Händler/Antiquariat, killarneybookseu.
1 Introduction 2 Stellar structure equations 3 Thermodynamic properties of stellar matter 3.1 Photon gas 3.2 Fermion gas 3.2.1 Completely degenerate fermion gas 3.2.2 Partially degenerate fermion gas 3.2.3 Neutrino gas 4 Equation of state of stellar matter 4.1 The ideal classical gas 4.2 The degenerate gas 4.2.1 White dwarfs 4.2.2 Proto-neutron stars 4.2.3 Neutron stars 5 The nuclear equation of state 5.1 Compressibility of nuclear matter 5.2 Nuclear symmetry energy 6 Relativistic mean field model 6.1 Walecka model and its extensions 6.2 Model with nonlinear isoscalar-isovector interaction terms 6.3 Model with δ meson 6.4 Model with nonzero temperature 6.5 Leptons 7 Strange nuclear matter 7.1 The effective field theoretical model 8 Properties of nuclear matter 8.1 Infinite symmetric nuclear matter 8.2 Infinite symmetric strange hadronic matter 8.3 Asymmetric nuclear matter 8.4 Asymmetric strangeness-rich matter 9 Neutron star matter 9.1 The equilibrium conditions and composition of stellar matter 9.2 Neutron star matter with zero strangeness 10 Strange neutron star matter 11 Astrophysical constraints on the equation of state 12 Proto-neutron star model 12.1 Neutrino opacities 12.2 The influence of neutrino trapping on proto-neutron star properties and evolution 13 Conclusions / Bibliography, Taschenbuch, Etykieta: Silesia University Press, Silesia University Press, Grupy produktów: Book, Opublikowany: 2007-01-01, Studio: Silesia University Press.
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Relativistic Mean Field Models of Neutron Stars (2007)
EN PB USISBN: 9788322617069 bzw. 8322617062, in Englisch, Silesia University Press, Katowice, Taschenbuch, gebraucht.
Lieferung aus: Vereinigtes Königreich Großbritannien und Nordirland, plus shipping, Shipping area: EUR.
Von Händler/Antiquariat, Any Amount of Books, . London, [RE:4].
8vo. pp 196. Large format paperback. ISBN: 8322617062. First Paperback Edition.
Von Händler/Antiquariat, Any Amount of Books, . London, [RE:4].
8vo. pp 196. Large format paperback. ISBN: 8322617062. First Paperback Edition.
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