Quantum-Statistical Models of Hot Dense Matter: Methods for Computation Opacity and Equation of State
In the processes studied in contemporary physics one encounters the most diverse conditions: temperatures ranging from absolute zero to those found in the cores of stars, and densities ranging from those of gases to densities tens of times larger than those of a solid body. Accordingly, the solution of many problems of modern physics requires an increasingly large volume of information about the propertiesofmatterundervariousconditions,includingextremeones. Atthesame time, there is a demand for an increasing accuracy of these data, due to the fact thatthereliabilityandcomputationalsubstantiationofmanyuniquetechnological devices and physical installations depends on them. The relatively simple models ordinarily described in courses on theoretical physics are not applicable when we wish to describe the properties of matter in a sufficiently wide range of temperatures and densities. On the other hand, expe- ments aimed at generating data on properties of matter under extreme conditions usually face considerably technical difficulties and in a number of instances are exceedingly expensive. It is precisely for these reasons that it is important to - velop and refine in a systematic manner quantum-statistical models and methods for calculating properties of matter, and to compare computational results with data acquired through observations and experiments. At this time, the literature addressing these issues appears to be insufficient. If one is concerned with opacity, which determines the radiative heat conductivity of matter at high temperatures, then one can mention, for example, the books of D. A. Frank-Kamenetskii [67], R. D. Cowan [49], and also the relatively recently published book by D.
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Quantum-Statistical Models of Hot Dense Matter: Methods for Computation Opacity and Equation of State
In the processes studied in contemporary physics one encounters the most diverse conditions: temperatures ranging from absolute zero to those found in the cores of stars, and densities ranging from those of gases to densities tens of times larger than those of a solid body. Accordingly, the solution of many problems of modern physics requires an increasingly large volume of information about the propertiesofmatterundervariousconditions,includingextremeones. Atthesame time, there is a demand for an increasing accuracy of these data, due to the fact thatthereliabilityandcomputationalsubstantiationofmanyuniquetechnological devices and physical installations depends on them. The relatively simple models ordinarily described in courses on theoretical physics are not applicable when we wish to describe the properties of matter in a sufficiently wide range of temperatures and densities. On the other hand, expe- ments aimed at generating data on properties of matter under extreme conditions usually face considerably technical difficulties and in a number of instances are exceedingly expensive. It is precisely for these reasons that it is important to - velop and refine in a systematic manner quantum-statistical models and methods for calculating properties of matter, and to compare computational results with data acquired through observations and experiments. At this time, the literature addressing these issues appears to be insufficient. If one is concerned with opacity, which determines the radiative heat conductivity of matter at high temperatures, then one can mention, for example, the books of D. A. Frank-Kamenetskii [67], R. D. Cowan [49], and also the relatively recently published book by D.
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Quantum-Statistical Models of Hot Dense Matter: Methods for Computation Opacity and Equation of State

Quantum-Statistical Models of Hot Dense Matter: Methods for Computation Opacity and Equation of State

Quantum-Statistical Models of Hot Dense Matter: Methods for Computation Opacity and Equation of State

Quantum-Statistical Models of Hot Dense Matter: Methods for Computation Opacity and Equation of State

Hardcover(2005)

$109.99 
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Overview

In the processes studied in contemporary physics one encounters the most diverse conditions: temperatures ranging from absolute zero to those found in the cores of stars, and densities ranging from those of gases to densities tens of times larger than those of a solid body. Accordingly, the solution of many problems of modern physics requires an increasingly large volume of information about the propertiesofmatterundervariousconditions,includingextremeones. Atthesame time, there is a demand for an increasing accuracy of these data, due to the fact thatthereliabilityandcomputationalsubstantiationofmanyuniquetechnological devices and physical installations depends on them. The relatively simple models ordinarily described in courses on theoretical physics are not applicable when we wish to describe the properties of matter in a sufficiently wide range of temperatures and densities. On the other hand, expe- ments aimed at generating data on properties of matter under extreme conditions usually face considerably technical difficulties and in a number of instances are exceedingly expensive. It is precisely for these reasons that it is important to - velop and refine in a systematic manner quantum-statistical models and methods for calculating properties of matter, and to compare computational results with data acquired through observations and experiments. At this time, the literature addressing these issues appears to be insufficient. If one is concerned with opacity, which determines the radiative heat conductivity of matter at high temperatures, then one can mention, for example, the books of D. A. Frank-Kamenetskii [67], R. D. Cowan [49], and also the relatively recently published book by D.

Product Details

ISBN-13: 9783764321833
Publisher: Birkhäuser Basel
Publication date: 04/06/2005
Series: Progress in Mathematical Physics , #37
Edition description: 2005
Pages: 430
Product dimensions: 6.10(w) x 9.25(h) x 0.04(d)

Table of Contents

Preface.- I. Quantum-statistical self-consistent field models - 1. The generalized Thomas-Fermi model - 2. Electron wave functions in a given potential - 3. Quantum-statistical self-consistent field models - 4. The Hartree-Fock-Slater model for the average atom.- II. Radiative and thermodynamical properties of high-temperature dense plasma - 5. Interaction of radiation with matter - 6. The equation of state.- III. Appendix. Methods for solving the Schrödinger and Dirac equations.- Bibliography.- Index
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