Physics Of Supernovae And Their Mathematical Models, The
Regular price
€112.99
Regular price
€113.99
Sale
Sale price
€112.99
14 days return policy
Shipping & Delivery
A01=Alexey G Aksenov
A01=Valery Mihailovich Chechetkin
Age Group_Uncategorized
Age Group_Uncategorized
Author_Alexey G Aksenov
Author_Valery Mihailovich Chechetkin
automatic-update
Binary System
Category1=Non-Fiction
Category=PHN
Category=PHVB
Collision Integral
COP=Singapore
Core Collapse
Degenerate Relativistic Electrons
Delivery_Delivery within 10-20 working days
eq_bestseller
eq_isMigrated=0
eq_isMigrated=2
eq_nobargain
eq_non-fiction
eq_science
Equation of State
Finite Difference Scheme
Gamma-Ray Burst
Godunov Type Methods
Hydrodynamics
Hyperbolic Equation
Kinetic Boltzmann Equation
Language_English
Large-Scale Convection
Neutrino
Neutron Star
Nucleosynthesis
PA=Available
Partial Differential Equations
Price_€100 and above
PS=Active
Rotating Star
softlaunch
Stiff Ordinary Differential Equations System
Supernova
Thermalization in Plasma
Thermonuclear Burning
Product details
- ISBN 9789811285097
- Publication Date: 26 Mar 2024
- Publisher: World Scientific Publishing Co Pte Ltd
- Publication City/Country: SG
- Product Form: Hardback
- Language: English
Secure
checkout
Fast Shipping
Easy returns
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.
