Name: The Physics of Supernovae and Their Mathematical Models (en Inglés)
Price: 487.63 PEN
Availability: InStock
Author: Aksenov, Alexey G. ; Chechetkin, Valery Mihailovich
ISBN: 9789811285097

portada The Physics of Supernovae and Their Mathematical Models (en Inglés)

Formato

Libro Físico

Autor

Alexey G. Aksenov

Valery Mihailovich Chechetkin

Editorial

World Scientific Publishing Company

Idioma

Inglés

N° páginas

296

Encuadernación

Tapa Dura

Dimensiones

22.9 x 15.2 x 1.8 cm

Peso

0.56 kg.

ISBN13

9789811285097

Categorías

Cosmología y el universo
Astrofísica

The Physics of Supernovae and Their Mathematical Models (en Inglés)

Alexey G. Aksenov (Autor) · Valery Mihailovich Chechetkin (Autor) · World Scientific Publishing Company · Tapa Dura

Libro Físico

S/ 487,63

S/ 975,26

Ahorras: S/ 487,63

50% descuento

Envío normal

Origen: Estados Unidos (Costos de importación incluídos en el precio)

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Reseña del libro "The Physics of Supernovae and Their Mathematical Models (en Inglés)"

This book is dedicated to the theory of supernovae, focusing on new computational methods and simulations. It contains three parts: basic principles, numerical methods, and applications. The first part contains a non-formal introduction into the basics of supernovae, Boltzmann kinetic equations -- with details of two particles reaction rate calculations -- and the transformation of Boltzmann kinetic equations into hydrodynamic elements of statistical physics. It also contains the equation of state for matter of high energy density, with details of calculations for thermodynamic parameters, weak interactions, reaction rate details, and thermonuclear burning. The second part introduces elements of computational physics.The book closes with a presentation of original thought regarding the regime of burning in degenerate carbon-oxygen cores, a neutrino transport in Type II supernovae, a simulation of general relativity (GR) coalescence of neutron stars, aspherical nucleosynthesis in a core-collapse supernova, and thermalization in a pair of plasma winds from a compact strange star.This book brings together generally accepted simulations methods as well as original material written by two respected members of Russian research groups: the Keldysh Institute of Applied Mathematics and Institute of Theoretical and Experimental Physics. It contains the necessary information for a person to start independent research in this fast-developing field, and is therefore an important read for new researchers in this subject.