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Zustand: acceptable. Ausreichend/Acceptable: Exemplar mit vollständigem Text und sämtlichen Abbildungen oder Karten. Schmutztitel oder Vorsatz können fehlen. Einband bzw. Schutzumschlag weisen unter Umständen starke Gebrauchsspuren auf. / Describes a book or dust jacket that has the complete text pages (including those with maps or plates) but may lack endpapers, half-title, etc. (which must be noted). Binding, dust jacket (if any), etc may also be worn.

Zustand: very good. Gut/Very good: Buch bzw. Schutzumschlag mit wenigen Gebrauchsspuren an Einband, Schutzumschlag oder Seiten. / Describes a book or dust jacket that does show some signs of wear on either the binding, dust jacket or pages.

Zustand: New. In.

Zustand: New. In.

Taschenbuch. Zustand: Sehr gut. Gebraucht - Sehr gut SG - leichte Beschädigungen oder Verschmutzungen, ungelesenes Mängelexemplar, gestempelt - The book gives an extended review of theoretical and observational aspects of neutron star physics. With masses comparable to that of the Sun and radii of about ten kilometres, neutron stars are the densest stars in the Universe. This book describes all layers of neutron stars, from the surface to the core, with the emphasis on their structure and equation of state. Theories of dense matter are reviewed, and used to construct neutron star models. Hypothetical strange quark stars and possible exotic phases in neutron star cores are also discussed. Also covered are the effects of strong magnetic fields in neutron star envelopes.

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - 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,togetherwiththephysicsofstronginteractionsofelementaryp articles.

Paperback. Zustand: Brand New. 640 pages. 9.21x5.98x1.42 inches. In Stock.

XVIII, 285, 40 S. Hlwd. m. Rsign. St. verso Tit. (Finanzwirtschaftliche u. volkswirtschaftliche Studien 10) Sprache: Deutsch.

VI, 204 S. OLwd. M. Rsign. St. verso Tit. Sprache: Deutsch 0 gr.

Hardcover. Zustand: sehr gut. Originalhefte. 8°. je ca. 61 Seiten. teils kleine Knicke. in deutscher Sprache.

Broschur. Zustand: gut. Vol. 1: XIV, 275 S.; vol. 2: XIV, 348 S.; vol. 3: XII, 250 S., 24 cm, Aufkleber, Bibliotheksexemplare, leicht gebräunt. Sprache: deu.

Broschur. Zustand: Gut. 204 Separatdruck separate printing offprint Archäologie Jugoslawien Botanik Zoologie guter Zustand Mit zahlr. Abb. Einband mit kleinem Riss, leichte Knickspur. ha1058394 Sprache: Deutsch Gewicht in Gramm: 650.

Hardcover. Zustand: Brand New. reprint edition. 276 pages. German language. 6.69x0.69x9.61 inches. In Stock.