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Neutron Stars
Haensel, P. (Copernicus Astronomical Center); Potekhin, A. Y. (Ioffe Physical Technical Institute); Yakovlev, D. G.
€ 205.20
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Description for Neutron Stars
Hardback. The book gives an extended review of theoretical and observational aspects of neutron star physics. It describes all layers of neutron stars, from the surface to the core, with the emphasis on their structure and equation of state. Series: Astrophysics and Space Science Library. Num Pages: 644 pages, biography. BIC Classification: PGM. Category: (P) Professional & Vocational. Dimension: 234 x 156 x 34. Weight in Grams: 2370.
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 ... Read more
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 ... Read more
Product Details
Format
Hardback
Publication date
2006
Publisher
Springer-Verlag New York Inc. United States
Number of pages
644
Condition
New
Series
Astrophysics and Space Science Library
Number of Pages
620
Place of Publication
New York, NY, United States
ISBN
9780387335438
SKU
V9780387335438
Shipping Time
Usually ships in 15 to 20 working days
Ref
99-15
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