Accurate%20energy%20functionals%20for%20evaluating%20electron%20correlation%20energies PowerPoint PPT Presentation

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Title: Accurate%20energy%20functionals%20for%20evaluating%20electron%20correlation%20energies


1
Accurate energy functionals for evaluating
electron correlation energies
  • ???
  • ?????????????,
  • ???

2
Outline (??)
  • History and context.
  • Theory.
  • Example 1. Homogeneous Electron Gas.
  • Example 2. Metal slabs.
  • Conclusions and perspectives.


3
Earlier achievements
4
Discovery of the electron
  • 1897
  • Could anything at first sight seem more
    impractical than a body which is so small that
    its mass is an insignificant fraction of the mass
    of an atom of hydrogen?

J.J. Thompson (1856-1940) discovers the
electron. (Cambridge, UK)
Nobel Prize in Physics, 1906
5
Advent of new physics
  • 1900

Quantization of energy Nobel Prize in Physics,
1918
  • 1905

Photoelectric effect Nobel Prize in Physics, 1921
M. Planck (1858-1947)
6
  • 1909

Measurement of electron charge and photoelectric
effect. Nobel Prize in Physics, 1923
Robert Millikan (1868-1953)
  • 1911

Disintegration of radiactive elements Nobel Prize
in Chemistry, 1908
7
Development of quantum mechanics
  • 1913

Quantum theory of the atom. Nobel Prize in
Physics, 1922
Niels Bohr (1885-1962)
8
Development of quantum mechanics
  • 1921
  • 1925

1929
Statistical mechanics of electrons
W. Pauli (1900-1958) 1945
E. Fermi (1901-1954) 1938
Louis De Broglie (1892-1987)
9
Development of quantum mechanics
  • 1926

1933
1932
Erwin Schrodinger (1887-1961)
W. Heisenberg (1901-1976)
10
Applications in solids
  • 1928

1952
Forbidden region
Felix Bloch 1905-1983
11
First attempts in electronic structre calculation
  • 1928 - 1932
  • Egil Hylleraas. Configuration interaction,
    correlated basis functions.
  • Douglas Hartree and Vladimir Fock. Mean field
    calculations.
  • Wigner and Seitz. Cellular method.

12
More milestones
(According to D. Pines)
  • Bohr Mottelson. Collective model of nucleus.
    (1953)
  • Bohm Pines. Random Phase Approximation. (1953)
  • Gell-Mann Brueckner. Many body perturbation
    theory. (1957)

13
More milestones
(According to P. Coleman)
  • BCS theory of superconductivity.
  • Renormalization group.
  • Quantum hall effect, integer and fractionary.
  • Heavy fermions.
  • High temperature superconductivity.

14
More is different
  • At each level of complexity, entirely new
    properties appear, and the understanding of these
    behaviors requires research which I think is as
    fundamental in its nature as any other
  • P. W. Anderson. Science, 177393, 1972.

15
Theory
  • First principles electronics structure calculation

16
Quotation from H. Lipkin
  • We can begin by looking at the
    fundamental paradox of the many-body problem
    namely that people who do not know how to solve
    the three-body problem are trying to solve the
    N-body problem.
  • Our choice of wave functions is very
    limited we only know how to use independent
    particle wave functions. The degree to which this
    limitation has invaded our thinking is marked by
    our constant use of concepts which have meaning
    only in terms of independent particle wave
    functions shell structure, the occupation
    number, the Fermi sea and the Fermi surface, the
    representation of perturbation theory by Feynman
    diagrams.
  • All of these concepts are based upon the
    assumption that it is reasonable to talk about a
    particular state being occupied or unoccupied by
    a particle independently of what the other
    particles are doing. This assumption is generally
    not valid, because there are correlations between
    particles. However, independent particle wave
    functions are the only wave functions that we
    know how to use. We must therefore find some
    method to treat correlations using these very bad
    independent particle wave functions.

Annals of Physics 8, 272 (1960)
17
Currently available methods
  • Configuration Interaction. Quantum Monte Carlo.
    (Wave function)
  • Many-body perturbation theory.
  • (Greens function)
  • Kohn-Sham Density Functional Theory (Density).

18
Configuration Interaction(Wave function method)

19
Currently available methods
  • Configuration Interaction. Quantum Monte Carlo.
    (Wave function)
  • Many-body perturbation theory.
  • (Greens function)
  • Kohn-Sham Density Functional Theory (Density).

20
Many-body theory
  • Electronic and optical experiments often measure
    some aspect of the one-particle Greens function
  • The spectral function, Im G, tells you about the
    single-particle-like approximate eigenstates of
    the system the quasiparticles
  • Can formulate an iterative expansion of the
    self-energy S in powers of W, the screened
    Coulomb interaction, the leading term of which is
    the GW approximation
  • Can now perform such calculations computationally
    for real materials, without adjustable parameters.


21
Currently available methods
  • Configuration Interaction. Quantum Monte Carlo.
    (Wave function)
  • Many-body perturbation theory.
  • (Greens function)
  • Kohn-Sham Density Functional Theory (Density).

22
KS-DFT formalism
  • It provides an independent particle scheme that
    describes the exact ground state density and
    energy.

23
KS-DFT formalism
  • Given the KS orbitals of the system we have.

24
KS-DFT formalism
  • The effective potential associated to the
    fictitious system is

25
KS-DFT formalism
  • The effective potential associated to the
    fictitious system is

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29
Example 1
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Homogeneous Electron Gas
Independent electron approximation
31
Exchange energy
32
Correlation energy
  • RPA. Bohm and Pines. (1953)
  • Gell-Mann and Brueckner. ( 1957)
  • Sawada. (1957)
  • Hubbard. (1957)
  • Nozieres and Pines. (1958)
  • Quinn and Ferrel. (1958)
  • Ceperley and Alder. (1980)

?????
33
Ground-state energy of HEG
Phys. Rev. Lett. 45, 566 (1980)
34
Exchange-Correlation energy
35
Structure factor
36
Density-density response function. (or
Polarization)
37
Density-density response function. (or
Polarization)
RPA response function
38
Density-density response function. (or
Polarization)
Exact response function
39
Density-density response function. (or
Polarization)
Hubbard response function
Hubbard local field factor
40
Hubbard vertex correction
Considers the Coulomb repulsion between electrons
with antiparallel spins.
41
Many-body effects
  • Local field factor TDDFT fxc kernel
  • Lets remember that

42
Approximations for fxc
  • The simplest form is ALDA
  • But it gives too poor energy when used with the
    ACFD formula.

Reminder
43
HEG Correlation energies
  • Phys. Rev. B 61, 13431, (2000)

44
Energy optimized kernels
  • Dobson and Wang.
  • Optimized Hubbard.

where
45
Performance of kernels
Phys. Rev. B 70, 205107 (2004)
46
Example 2
47
Jellium metal slabs
48
One Jellium Slab
Thickness L 6.4rs
49
Two slabs
  • Binding energies. (mHa/elec)
  • Surface energies. (erg/cm2)

50
Interaction energies
  • Thickness L 3rs and rs 1.25

51
Cancellation of errors
52
Conclusion and perspectives
53
Conclusions
54
Perspectives
  • TDDFT for excited states
  • Development of fxc kernels
  • Transport and spectroscopic properties
  • cond-mat/0604317
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