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The Stability of Matter: From Atoms to Stars

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Table of Contents

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    Book Overview
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    Chapter 1 Introduction
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    Chapter 2 The Stability of Matter: From Atoms to Stars
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    Chapter 3 Lower bound to the energy of complex atoms
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    Chapter 4 Improved Lower Bound on the Indirect Coulomb Energy
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    Chapter 5 Monotonicity of the molecular electronic energy in the nuclear coordinates
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    Chapter 6 Proof of the Stability of Highly Negative Ions in the Absence of the Pauli Principle
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    Chapter 7 Atomic and Molecular Negative Ions
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    Chapter 8 Bound on the maximum negative ionization of atoms and molecules
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    Chapter 9 Asymptotic Neutrality of Large- Z Ions
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    Chapter 10 Approximate Neutrality of Large- Z Ions
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    Chapter 11 Universal nature of van der Waals forces for Coulomb systems
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    Chapter 12 Electron density near the nucleus of a large atom
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    Chapter 13 Proof of a conjecture about atomic and molecular cores related to Scott’s correction
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    Chapter 14 Asymptotics of Natural and Artificial Atoms in Strong Magnetic Fields
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    Chapter 15 Ground states of large quantum dots in magnetic fields
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    Chapter 16 Kinetic Energy Bounds and Their Application to the Stability of Matter
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    Chapter 17 Inequalities for the Moments of the Eigenvalues of the Schrödinger Hamiltonian and Their Relation to Sobolev Inequalities
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    Chapter 18 On Semi-Classical Bounds for Eigenvalues of Schrödinger Operators
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    Chapter 19 The Number of Bound States of One-Body Schroedinger Operators and the Weyl Problem
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    Chapter 20 Variational Principle for Many-Fermion Systems
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    Chapter 21 Erratum to: Variational Principle for Many-Fermion Systems
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    Chapter 22 Thomas-fermi and related theories of atoms and molecules
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    Chapter 23 Erratum to: Thomas-fermi and related theories of atoms and molecules
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    Chapter 24 Erratum to: Thomas-fermi and related theories of atoms and molecules
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    Chapter 25 The Hartree-Fock Theory for Coulomb Systems
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    Chapter 26 There Are No Unfilled Shells in Unrestricted Hartree-Fock Theory
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    Chapter 27 Many-Body Atomic Potentials in Thomas-Fermi Theory
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    Chapter 28 The Positivity of the Pressure in Thomas Fermi Theory
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    Chapter 29 Erratum to: The Positivity of the Pressure in Thomas Fermi Theory
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    Chapter 30 The Thomas—Fermi—von Weizsäcker Theory of Atoms and Molecules
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    Chapter 31 Analysis of the Thomas-Fermi-von Weizsäcker Equation for an Infinite Atom Without Electron Repulsion
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    Chapter 32 The most negative ion in the Thomas—Fermi—von Weizsäcker theory of atoms and molecules
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    Chapter 33 Bound for the Kinetic Energy of Fermions Which Proves the Stability of Matter
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    Chapter 34 Erratum to: Bound for the Kinetic Energy of Fermions Which Proves the Stability of Matter
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    Chapter 35 The N 5/3 Law for Bosons
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    Chapter 36 Stability of Coulomb Systems with Magnetic Fields
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    Chapter 37 Stability of Coulomb Systems with Magnetic Fields
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    Chapter 38 Stability of Matter in Magnetic Fields
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    Chapter 39 A Rigorous Examination of the Chandrasekhar Theory of Stellar Collapse
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    Chapter 40 The Chandrasekhar Theory of Stellar Collapse as the Limit of Quantum Mechanics
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    Chapter 41 One-Electron Relativistic Molecules with Coulomb Interaction
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    Chapter 42 Many-Body Stability Implies a Bound on the Fine-Structure Constant
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    Chapter 43 The Stability and Instability of Relativistic Matter
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    Chapter 44 Stability of Relativistic Matter via Thomas-Fermi Theory
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    Chapter 45 Stability and Instability of Relativistic Electrons in Classical Electromagnetic Fields
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    Chapter 46 The N 7/5 Law for Charged Bosons
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    Chapter 47 The stability of matter
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    Chapter 48 Existence of Thermodynamics for Real Matter with Coulomb Forces
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    Chapter 49 Lectures on the Thermodynamic Limit for Coulomb Systems
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    Chapter 50 The Thermodynamic Limit for Jellium
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    Chapter 51 Erratum to: The Thermodynamic Limit for Jellium
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Title
The Stability of Matter: From Atoms to Stars
Published by
Springer Berlin Heidelberg, June 2013
DOI 10.1007/978-3-662-03436-1
ISBNs
978-3-66-203438-5, 978-3-66-203436-1
Editors

Thirring, Walter

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Geographical breakdown

Country Count As %
Unknown 1 100%

Demographic breakdown

Readers by professional status Count As %
Student > Postgraduate 1 100%
Readers by discipline Count As %
Chemistry 1 100%