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The Physics of Supernovae and Their Mathematical Models

The Physics of Supernovae and Their Mathematical Models

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"The Physics of Supernovae and Their Mathematical Models" by Alexey G Aksenov, Valery Mihailovich Chechetkin is a mathematics book and learning resource focused on Deep Sky & Solar System. Best for teachers, students, and readers looking for stronger mathematical understanding.

"This book is dedicated to the theory of supernovae, focussing on new computational methods and simulations. It contains three parts: basic principles, numerical methods, and applications. The first part contains the non-formal introduction into the topics 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 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 collects not only generally accepted simulations methods, it also includes original approaches of the authors from two Russian groups in Supernovae, from the Keldysh Institute of Applied Mathematics and Institute for Theoretical and Experimental Physics. The book closes with a presentation of original works about the regime of burning in degenerate carbon-oxygen cores, a neutrino transport in supernovae type II, simulation of GR coalescence of neutron stars, aspherical nucleosynthesis in a core-collapse supernova, and thermalization in pair of plasma wind from a compact strange star. It contains the necessary information for a person to start independent research in this fast-developing field. It is therefore an important read for new researchers in this subject"--

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Best For: Researchers and graduate students in astrophysics focusing on supernovae.
Focus: Theoretical and computational aspects of supernovae, including kinetic equations and hydrodynamic modeling.
Covers: Basic principles of supernovae, numerical methods for simulations, and practical applications of these models.
Why It Matters: Provides detailed mathematical and computational frameworks essential for understanding and simulating supernova phenomena accurately.

"The Physics of Supernovae and Their Mathematical Models" by Alexey G Aksenov, Valery Mihailovich Chechetkin is a mathematics book and learning resource focused on Deep Sky & Solar System. Best for teachers, students, and readers looking for stronger mathematical understanding.

Topic: Deep Sky & Solar System

Author: Alexey G Aksenov, Valery Mihailovich Chechetkin

Who this is for:

  • Teachers and classroom instructors
  • Students building subject mastery
  • Readers looking for practical learning support

Why this book matters: It stands out as a practical math resource that helps explain concepts, strengthen problem-solving, and support classroom or independent learning.

"This book is dedicated to the theory of supernovae, focussing on new computational methods and simulations. It contains three parts: basic principles, numerical methods, and applications. The first part contains the non-formal introduction into the topics 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 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 collects not only generally accepted simulations methods, it also includes original approaches of the authors from two Russian groups in Supernovae, from the Keldysh Institute of Applied Mathematics and Institute for Theoretical and Experimental Physics. The book closes with a presentation of original works about the regime of burning in degenerate carbon-oxygen cores, a neutrino transport in supernovae type II, simulation of GR coalescence of neutron stars, aspherical nucleosynthesis in a core-collapse supernova, and thermalization in pair of plasma wind from a compact strange star. It contains the necessary information for a person to start independent research in this fast-developing field. It is therefore an important read for new researchers in this subject"--

AuthorAlexey G Aksenov, Valery Mihailovich Chechetkin
PublisherWorld Scientific Publishing Company
Published2024
ISBN-139789811285097
BindingHardcover
LanguageEnglish
SubjectsScience
TopicDeep Sky & Solar System

Format: Hardcover

Language: English

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