9783838325460 - Properties of nuclear matter and implication for astrophysical systems: Study the dense nuclear matter properties using field theoretical chiral sigm ... astrophysi... (9 resultados)

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Taschenbuch. Condición: Neu. Properties of nuclear matter and implication for astrophysical systems | Study the dense nuclear matter properties using field theoretical chiral sigm model and application to some astrophysical systems such as neutro stars | Pradip Kumar Sahu | Taschenbuch | 152 S. | Englisch | 2010 | LAP LAMBERT Academic Publishing | EAN 9783838325460 | Verantwortliche Person für die EU: BoD - Books on Demand, In de Tarpen 42, 22848 Norderstedt, info[at]bod[dot]de | Anbieter: preigu.

Paperback. Condición: Brand New. 152 pages. 8.66x5.91x0.35 inches. In Stock.

Taschenbuch. Condición: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -This book is very useful for undergraduate scholars, because it gives a good, detailed overview of early works on equation of states at high density nuclear matter. Then this book deals the properties of dense nuclear matter using relativistic field theoretical approach. A detailed study of the chiral sigma model based on mean field theory is done and it is used to derive an equation of state of asymmetric nuclear matter, because, the chiral symmetry seems to possess such a desirable property at high densities. The calculation of this model is extended to finite temperature and is examined it in the context of the question of a possible phase transition from hadronic matter to quark matter at high densities. Then certain astrophysical applications of this model are considered. These are the modeling of stable neutron star structure, radial oscillations of quark stars and cooling rates of neutron stars, if these objects possess (u, d, s) quark matter in their cores. The structure of neutron stars, quark stars and quark star oscillations are discussed. The limitation of previously suggested neutrino emissivity formula for the quark matter in the neutron stars is also discussed. 152 pp. Englisch.

Condición: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Autor/Autorin: SAHU PRADIP KUMARBorn on 16-05-1966 in Orissa, India. At present serving as professor at Institute of Physics, Bhubaneswar, India. Published more than 50 papers in scientific International Journals. Received Ph.D.(Physics) in 1995 an.

Condición: New. Print on Demand.

Condición: New. PRINT ON DEMAND.

Taschenbuch. Condición: Neu. This item is printed on demand - Print on Demand Titel. Neuware -This book is very useful for undergraduate scholars, because it gives a good, detailed overview of early works on equation of states at high density nuclear matter. Then this book deals the properties of dense nuclear matter using relativistic field theoretical approach. A detailed study of the chiral sigma model based on mean field theory is done and it is used to derive an equation of state of asymmetric nuclear matter, because, the chiral symmetry seems to possess such a desirable property at high densities. The calculation of this model is extended to finite temperature and is examined it in the context of the question of a possible phase transition from hadronic matter to quark matter at high densities. Then certain astrophysical applications of this model are considered. These are the modeling of stable neutron star structure, radial oscillations of quark stars and cooling rates of neutron stars, if these objects possess (u, d, s) quark matter in their cores. The structure of neutron stars, quark stars and quark star oscillations are discussed. The limitation of previously suggested neutrino emissivity formula for the quark matter in the neutron stars is also discussed.VDM Verlag, Dudweiler Landstraße 99, 66123 Saarbrücken 152 pp. Englisch.

Taschenbuch. Condición: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - This book is very useful for undergraduate scholars, because it gives a good, detailed overview of early works on equation of states at high density nuclear matter. Then this book deals the properties of dense nuclear matter using relativistic field theoretical approach. A detailed study of the chiral sigma model based on mean field theory is done and it is used to derive an equation of state of asymmetric nuclear matter, because, the chiral symmetry seems to possess such a desirable property at high densities. The calculation of this model is extended to finite temperature and is examined it in the context of the question of a possible phase transition from hadronic matter to quark matter at high densities. Then certain astrophysical applications of this model are considered. These are the modeling of stable neutron star structure, radial oscillations of quark stars and cooling rates of neutron stars, if these objects possess (u, d, s) quark matter in their cores. The structure of neutron stars, quark stars and quark star oscillations are discussed. The limitation of previously suggested neutrino emissivity formula for the quark matter in the neutron stars is also discussed.