Produto disponível no mesmo dia no aplicativo Kobo, após a confirmação  do pagamento!
Você pode ler este livro digital em vários dispositivos:
IOs - Clique para baixar o app gratuitoAndroid - Clique para baixar o app gratuitoPC - Clique para baixar o app gratuitoBlackBerry - Clique para baixar o app gratuitoWindows Phone - Clique para baixar o app gratuitoKobo - Conheça nossa linha de leitores digitais
The monograph presents a comparative analysis of different thermodynamic models of the equations of state. The basic ideological premises of the theoretical methods and the experiment are considered. The principal attention is on the description of states that are of greatest interest for the physics of high energy concentrations which are either already attained or can be reached in the near future in controlled terrestrial conditions, or are realized in astrophysical objects at different stages of their evolution. Ultra-extreme astrophysical and nuclear-physical applications are also analyzed where the thermodynamics of matter is affected substantially by relativism, high-power gravitational and magnetic fields, thermal radiation, transformation of nuclear particles, nucleon neutronization, and quark deconfinement.
The book is intended for a wide range of specialists engaged in the study of the equations of state of matter and high energy density physics, as well as for senior students and postgraduates.
Phase States of Matter, Their Classification
Equations of State of Gases and Liquids
Quantum-Mechanical Models of a Solid
Monte Carlo and Molecular Dynamics Methods
Statistical Substance Model
Density Functional Method
Semi-Empirical Equations of State
Relativistic Plasma. Wide–Range Description
Nuclear Transformations Under Strong Compression
Quark–Gluon Plasma and Strange Matter
Semi-Empiric Nuclear Models
Readership: The book is intended for a wide range of specialists engaged in the study of the equations of state of matter and high energy density physics, as well as for senior students and postgraduates.