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

ISBN 10: 383832546X / ISBN 13: 9783838325460

Published by LAP LAMBERT Academic Publishing, 2010

About this Item

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.

Seller Inventory # 101429781

Bibliographic Details

• Title: 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
• Publisher: LAP LAMBERT Academic Publishing
• Publication Date: 2010
• Language: English
• ISBN 10: 383832546X
• ISBN 13: 9783838325460
• Binding: Taschenbuch
• Condition: Neu
• Dimensions: 220W x 150H x 10D millimeters 220 millimeters width by 150 millimeters height by 10 millimeters depth
• Weight: 244 grams
• Seller catalogs:
  • Bücher

About this title

Synopsis

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.