Gebunden. Etat : New. An extended review of theoretical and observational aspects of neutron star physicsDescribes all layers of neutron stars, from the surface to the core, with the emphasis on their structure and equation of stateTheories of dens. N� de r�f. du vendeur 458429249

Contacter le vendeur

Acheter neuf

EUR 178,14

Autre devise

Frais de port : EUR 48,99

De Allemagne vers Etats-Unis

Destinations, frais et d�lais

Quantit� disponible : Plus de 20 disponibles

Ajouter au panier

Image d'archives

Neutron Stars 1: Equation of State and Structure

P. Haensel

Edit� par Springer-Verlag New York Inc., 2006

ISBN 10 : 0387335439 ISBN 13 : 9780387335438

Neuf Couverture rigide

impression � la demande

Vendeur : THE SAINT BOOKSTORE, Southport, Royaume-Uni

�valuation du vendeur 5 sur 5 �toiles

Hardback. Etat : New. This item is printed on demand. New copy - Usually dispatched within 5-9 working days 1029. N� de r�f. du vendeur C9780387335438

Contacter le vendeur

Acheter neuf

EUR 215,05

Autre devise

Frais de port : EUR 20,06

De Royaume-Uni vers Etats-Unis

Destinations, frais et d�lais

Quantit� disponible : Plus de 20 disponibles

Ajouter au panier

Image fournie par le vendeur

Neutron Stars 1 : Equation of State and Structure

P. Haensel

Edit� par Springer New York Nov 2006, 2006

ISBN 10 : 0387335439 ISBN 13 : 9780387335438

Neuf Couverture rigide

Vendeur : AHA-BUCH GmbH, Einbeck, Allemagne

�valuation du vendeur 5 sur 5 �toiles

Buch. Etat : Neu. Neuware - Neutron stars play a unique role in physics and astrophysics. On the one hand, they contain matter under extreme physical conditions, and their theories are based on risky and far extrapolations of what we consider reliable physical theories of the structure of matter tested in laboratory. On the other hand, their observationsoffertheuniqueopportunitytotestthesetheories. Moreover, n- tronstarsareimportantdramaticpersonaeonthestageofmodernastrophysics; they participate in many astronomical phenomena. 3 Neutronstarscontainthematterofdensityrangingfromafew g cm attheir 15 3 surface, where the pressure is small, to more than 10 gcm at the center, 36 2 wherethepressureexceeds10 dyncm . Tocalculateneutronstarstructure, one needs the dependence of the pressure on density, the so called equation of state (EOS), in this huge density range, taking due account of temperature, 9 more than10 K in young neutron stars, and magnetic elds, sometimes above 15 10 G. The present book is mainly devoted to the theory of the EOS of neutron star matter and its consequences for neutron star structure. As one moves from the neutron star surface to the center, the methods to calculate the EOS change. Atomic structure and plasma theories are used for the surface stellar layers. Deeper layers of the neutron star crust require nuclear theory combined with plasma physics, both in very exotic density-temperature regimes. Finally, the neutron star core necessitates many-body theory of dense strongly interacting systems,togetherwiththephysicsofstronginteractionsofelementaryparticles. N� de r�f. du vendeur 9780387335438

Contacter le vendeur

Acheter neuf

EUR 247,94

Autre devise

Frais de port : EUR 33,13

De Allemagne vers Etats-Unis

Destinations, frais et d�lais

Quantit� disponible : 2 disponible(s)

Ajouter au panier

Articles li�s � Neutron Stars 1: Equation of State And Structure

Neutron Stars 1: Equation of State And Structure - Couverture rigide

Haensel, P.; Potekhin, A.Y.; Yakovlev, D.G.

Synopsis

Acheter neuf

R�sultats de recherche pour Neutron Stars 1: Equation of State And Structure

Neutron Stars 1: Equation of State and Structure (Astrophysics and Space Science Library, 326)

Acheter neuf

Neutron Stars 1: Equation of State and Structure (Astrophysics and Space Science Library, 326)

Acheter neuf

Neutron Stars 1: Equation of State and Structure

Acheter neuf

Neutron Stars 1: Equation of State and Structure

Acheter neuf

Neutron Stars 1 : Equation of State and Structure

Acheter neuf