Muutke küpsiste eelistusi

E-raamat: Nuclear Matter Theory [Taylor & Francis e-raamat]

(Istituto Nazionale di Fisica Nucleare, Roma, Italy),
  • Formaat: 158 pages, 2 Tables, black and white; 50 Illustrations, black and white
  • Ilmumisaeg: 05-May-2020
  • Kirjastus: CRC Press Inc
  • ISBN-13: 9781351175340
Teised raamatud teemal:
  • Taylor & Francis e-raamat
  • Hind: 253,89 €*
  • * hind, mis tagab piiramatu üheaegsete kasutajate arvuga ligipääsu piiramatuks ajaks
  • Tavahind: 362,70 €
  • Säästad 30%
Nuclear Matter TheorySuurem pilt
  • Formaat: 158 pages, 2 Tables, black and white; 50 Illustrations, black and white
  • Ilmumisaeg: 05-May-2020
  • Kirjastus: CRC Press Inc
  • ISBN-13: 9781351175340
Teised raamatud teemal:
Taylor & Francis e-raamatudRohkem infot Taylor & Francis e-raamatute kohta
Raamatu kodulehekülg: https://www.taylorfrancis.com/books/9781351175340

Authored by two of the most respected experts in the field of nuclear matter, this book provides an up-to-date account of developments in nuclear matter theory and a critical comparison of the existing theoretical approaches in the field.

It provides information needed for researchers working with applications in a variety of research fields, ranging from nuclear physics to astrophysics and gravitational physics, and the computational techniques discussed in the book are relevant for the broader condensed matter and quantum fluids community.

  • The first book to provide an up-to-date and comprehensive overview of nuclear matter theory
  • Authored by two world-leading academics in this field
  • Includes a description of the most advanced computational techniques and a discussion of state-of-the art applications, such as the study of gravitational-wave emission from neutron stars
Preface ix
Chapter 1 Introduction
1(6)
1.1 Nuclear Matter In Atomic Nuclei
1(4)
1.2 Nuclear Matter In Neutron Stars
5(2)
Chapter 2 Nuclear Dynamics
7(14)
2.1 The Paradigm Of Many-Body Theory
7(1)
2.2 Empirical Facts On Nuclear Forces
8(2)
2.3 Phenomenological Potentials
10(7)
2.3.1 The nucleon-nucleon potential
10(4)
2.3.2 Three-nucleon forces
14(3)
2.4 Boson-Exchange Potentials
17(1)
2.5 Potentials Based On Chiral Lagrangians
17(4)
Chapter 3 Nuclear Matter Properties
21(12)
3.1 The Fermi Gas Model
21(4)
3.1.1 Energy-density and pressure of the degenerate Fermi gas
23(1)
3.1.2 Transition to the relativistic regime
23(1)
3.1.3 Extension to non-zero temperature
24(1)
3.2 The Equation Of State
25(4)
3.2.1 Equation of state of cold nuclear matter
26(1)
3.2.2 Symmetry energy
27(1)
3.2.3 Pressure
28(1)
3.3 Single-Nucleon Properties
29(4)
3.3.1 Green's function and spectral function
30(3)
Chapter 4 Nuclear Matter Theory
33(48)
4.1 The Mean-Field Approximation
33(3)
4.1.1 Limits of the mean-field approximation
35(1)
4.2 Renormalisation Of The Nn Interaction
36(1)
4.3 G-Matrix Perturbation Theory
37(6)
4.4 The Jastrow Variational Approach
43(17)
4.4.1 Cluster expansion
46(9)
4.4.2 Kinetic energy
55(2)
4.4.3 Low-order variational calculation of nuclear matter energy
57(3)
4.5 Advanced Perturbative Methods
60(5)
4.5.1 Coupled cluster method
60(2)
4.5.2 Self-consistent Green's function method
62(3)
4.6 Monte Carlo Methods
65(6)
4.6.1 Variational Monte Carlo
66(1)
4.6.2 Auxiliary field diffusion Monte Carlo
67(4)
4.7 Relativity
71(10)
4.7.1 Boost corrections to the nucleon-nucleon potential
71(2)
4.7.2 Dirac-Brueckner formalism
73(1)
4.7.3 Relativistic mean-field approximation
74(7)
Chapter 5 Advanced Variational Methods
81(28)
5.1 Correlated Basis Functions Theory
81(2)
5.2 Hyper-Netted-Chain Summation Scheme
83(8)
5.2.1 Fermi Hyper-Netted Chain
83(3)
5.2.2 RFHNC equations
86(5)
5.3 Extension To Spin-Isospin Dependent Correlations
91(11)
5.3.1 Diagrammatic rules
93(3)
5.3.2 RFHNC/SOC approximation
96(2)
5.3.3 Determination of the correlation functions
98(1)
5.3.4 Applications to the study of nuclear matter properties
99(3)
5.4 Cbf Effective Interaction
102(7)
Chapter 6 Neutron Stars
109(12)
6.1 Neutron Star Formation
109(2)
6.2 Neutron Star Structure
111(3)
6.2.1 Crust region
111(2)
6.2.2 Core region
113(1)
6.3 Equation Of State Of Neutron Star Matter
114(2)
6.4 Hydrostatic Equilibrium
116(5)
6.4.1 The equations of Tolman, Oppenheimer and Volkoff
117(4)
Chapter 7 Constraints From Astrophysical Data
121(14)
7.1 Measurements Of Mass And Radius
121(3)
7.2 Neutrino Emission And Cooling
124(2)
7.3 Gravitational-Wave Observations
126(9)
7.3.1 Neutron star merger
127(2)
7.3.2 Quasi-normal Modes
129(6)
Outlook 135(2)
Appendix A Two- and Three-Body Cluster Contributions 137(5)
Bibliography 142(13)
Index 155
Omar Benhar is an INFN research director and teaches Relativistic Quantum Mechanics and Quantum Electrodynamics at the University of Rome, "La Sapienza". He has worked extensively in the United States, and since 2013 has served as an adjunct professor at the Center for Neutrino Physics of Virginia Polytechnic Institute and State University. Prof. Benhar has co-authored two textbooks on Relativistic Quantum Mechanics and Gauge Theories, and published more than one hundred scientific papers on the theory of many-particle systems, the structure of compact stars and electroweak interactions of nuclei.



Stefano Fantoni has been Professor of Theory of Nuclear Interactions at the International School for Advanced Studies (SISSA), in Trieste, since 1992, and served as Director of the School between 2004 and 2010. He has authored and co-authored over two hundred papers published in international journals. In 2007, Prof. Fantoni has been the recipient of the Eugene Feenberg Memorial Medal for Many-Body Physics. In recognition of his role to improve communication between the scientific community and the general public, in 2009 he has been awarded the UNESCO Kalinga Prize for the popularization of Science.
Püsilink: https://www.kriso.ee/db/9781351175340_pe.html
Märksõnad: