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Of Cold Molecules

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Title: Of Cold Molecules


1
Of Cold Molecules
The Molecular Side
Olivier Dulieu Laboratoire Aimé Cotton, CNRS,
Campus dOrsay, Orsay, France olivier.dulieu_at_lac.u
-psud.fr
COMOLHPRN-CT-2002-00290
2
COMOL
3
Molecules are really cool!
  • The subtle flirtation of ultracold atoms
    ,Science, 280, 200 (1998) If high-energy
    accelarators make the rap music of physics-with
    their whirling particles and rapid-free smashups,
    then collisions between ultracold atoms are its
    Wagnerian opera
  • Molecules are cool , J. DoyleB. Friedrich,
    Nature 401, 749 (1999) Under ordinary
    conditions, atoms and molecules of a gas zigzag
    in all directionsand are most likely to move
    at the speed of riffle bullets The emergence of
    methods for slowing and trapping gaseous species
    has lead to a renaissance in atomic physics,
    which is now progressing into molecular/chemical
    physics as well Just as atom cooling is opening
    up new avenues of research, it is likely that the
    same will happen with molecular cooling with
    repercussions for chemistry, and even, perhaps,
    in biology.
  • Hot prospects for ultracold molecules , B.
    Goss Levi, Physics Today, Sept. 2000, p.46
  • Quantum encounters of the cold kind , K.
    Burnett, P.D. Lett, E. Tiesinga, P.Julienne, C.J.
    Williams, Nature 416, 225 (2002) We have
    already seen our dreams of controlling
    interactions on the quantum level come true, and
    the exquisite nature of this control has proved
    remarkable. These achievements have come from
    experimental and theoretical developments that
    have been a joy to be involved in, and their
    impact on new physics, chemistry and quantum
    computation has only just begun.
  • Really cool molecules , P. S. Julienne,
    Nature, 424, 24 (2003)

4
(Envisioned?) Applications of cold molecules
  • Ultra-high resolution spectroscopy ?
  • Test of fundamental theories ?
  • Superchemistry ?
  • Ultracold Photochemistry ?
  • Quantum properties, BCS, superfluidity
  • Ultimate control of reactive collisions
  • Quantum information
  • Biology

5
Which properties do characterize a molecule?
6
Excited state
Chemical bond
Ground state
7
How to get them?
Ask your favorite molecular spectroscopist
because he/she seems to speak like an
experimentalist Or
Ask your favorite theoretician, who may happen to
be a quantum chemist because you have no other
solution!
In both cases, you should be prepared to
understand what he/she is going to talk about
8
  • 1- Introduction, overview
  • 2- Molecular spectroscopy
  • 3- Asymptotic approach for long-range properties
  • 4- Hamiltonian of a diatomic molecule, Molecular
    symmetries Hunds cases Basics of quantum
    chemistry

9
Inversion of spectroscopic data to extract
molecular potential curves
  • Motivations
  • Apetizer some examples
  • Rotating vibrator (or vibrating rotor!) Dunham
    expansion
  • RKR semiclassical approach
  • NDE towards the asymptotic limit
  • IPA perturbative approach
  • DPF brute force approach
  • Applications

10
Motivations
  • Analysis of light/matter interaction
  • Gigantic amount of data synthesis required
  • Yields informations on internal structure
  • Starting point Born-Oppenheimer approximation
  • Other perturbations
  • Cold atoms scattering length determination
  • Combined analysis with (less accurate) quantum
    chemistry calculations
  • Elaborate and efficient tools required
  • High resolution (on energies)

11
Ex 1
  • 3580 transitions resulting in 924 levels

12
Ex 1
  • 3580 transitions resulting in 924 levels

13
Ex 1
  • 3580 transitions resulting in 924 levels

14
Ex 1
  • 3580 transitions resulting in 924 levels

15
Ex 2
16
Dunham expansion for energy levels
  • The energy levels of a rotating vibrator , J.
    L. Dunham, Phys. Rev. 41, 721 (1932)

Anharmonic oscillator
Energy levels term energies
Non-rigid rotator (Herzberg 1950)
Rotational constant
Centrifugal distorsion constant (CDC)
Coupled to each other
17
Dunham expansion (2)
  • Dunham coefficients

Note zero-point energy correction
18
Determination of the Dunham coefficients
N measured term energies M Dunham coefficients to
fit
C. Amiot and O. Dulieu, 2002, J. Chem. Phys. 117,
5155
  • Minimization of the reduced standard error
    (dimensionless) by adjustment on measured term
    energies

19
  • 47 Dunham coefficients
  • to represent
  • 16900 transitions, obtained by analysis of 348
    fluorescence series excited with
  • 21 wave lengths
  • r.m.s 0.0011cm-1

20
Dunham expansion summary
  • Compact, accurate, empirical representation of a
    large number of energies
  • Not suitable for extrapolation at large distances
  • Not suitable for extrapolation at high J, for
    heavy molecules
  • High-order coefficients highly correlated, and
    not physically meaningful
  • No information on the molecular structure

21
Centrifugal distorsion constants
22
RKR Rydberg-Klein-Rees analysis (1)
  • R. Rydberg, Z. Phys. 73, 376 (1931) Z. Phys. 80,
    514O (1933)
  • Klein, Z. Phys. 76, 226 (1932) A. L. G. Rees,
    Proc. Phys. Soc. London 59, 998 (1947)

Bohr-Sommerfeld quantification for a particle
with mass m in a potential V
Classical inner and outer turning points
RKR-1
inversion
23
RKR approach (2)
inversion
RKR-2
24
RKR potential curve
RKR-2
RKR-1
  • Use Gv and Bv from experiment, Dunham expansion
  • Extract a set of turning point for all energies
  • Specific codes (Le Roys group, U. Waterloo,
    Canada)
  • Limitations smooth functions of v, poor
    extrapolation high v, or large distances

Note extension with 3rd order quantification
(C. Schwartz and R. J. Le Roy 1984 J. Chem. Phys.
81, 3996 )
25
Near-dissociation expansion (NDE)
C. L. Beckel, R. B. Kwong, A. R. Hashemi-Attar,
and R. J. Le Roy 1984 J. Chem. Phys. 81, 66
  • Fit (a subset of) Gv and Bv with an expansion
    incorporating the long-range behavior of the
    potential (Cn/Rn)

R.J. Le Roy, R.B. Bernstein, J. Chem. Phys. 52,
3869 (1970) W.C. Stwalley, Chem. Phys. Lett. 6,
241 (1970) J. Chem. Phys. 58, 3867 (1973).
More elaborate form, for more flexibility
outer Padé expression
New input for RKR analysis
26
Ex
27
IPA Inverted perturbation approach (1)
  • R. J. Le Roy and J. van Kranendonk 1974 J. Chem.
    Phys. 61, 4750
  • W. M. Kosman and J. Hinze 1975 J. Mol. Spectrosc.
    56, 93
  • C. R. Vidal and H. Scheingraber 1977 J. Mol.
    Spectrosc. 65, 46.

Adjust an effective potential on experimental
energies, no Dunham expansion
Good initial approximation RKR potential V(0)(R).
Treat DV(R)V(R)-V(0)(R) as a perturbation
HH(0)DV(R).
Expansion
Modified energies
Zero-order eigenfunctions
Generally over-determined Least-square fit
28
IPA (2)
Cut-off function
Legendre polynomials
  • Choice of basis functions

Functional relation, useful for strongly
anharmonic potentials
Inner turning point
Outer turning point
Equlibrium distance
Standard error on ci, through the covariance
matrix
New determination of Gv, Bv No unique solution
29
IPA example
  • C.R. Vidal, Comments At. Mol. Phys. 17, 173 (1986)

Energy differences
RKR
IPA
30
DPF Direct potential fit (1)
  • Generalization of IPA approach
  • Choose an analytical function to be fitted on
    experimental energies
  • Need a good initial potential
  • Package available DSPotFit, from Le Roys group

Y. Huang 2000, Chemical Physics Research Report
649, University of Waterloo.
simple
Morse family
generalized
extended
modified
Modified Lennard-Jones Better asymptotic behavior
General power expansion
31
DPF (2)
  • Pure long-range states in alkali dimers (e.g.
    double-well state in Cs2)

References SMO P. M. Morse 1929 Phys. Rev. 54,
57 GMO J. A. Coxon and P. J. Hajigeorgiou 1991
J. Mol. Spectrosc. 150, 1 MMO H. G. Hedderich,
M. Dulick, and P. F. Bernath 1993, J. Chem. Phys.
99, 8363 EMO E. G. Lee, J. Y. Seto, T. Hirao,
P. F. Bernath, and R. J. Le Roy 1999 J. Mol.
Spectrosc. 194, 197 MLJ P. G. Hajigeorgiou and
R. J. Le Roy 2000, J. Chem. Phys. 112, 3949 G
C. Samuelis, E. Tiesinga, T. Laue, M. Elbs, H.
Knöckel, and E. Tiemann 2000, Phys. Rev. A, 63,
012710
32
Dunham/RKRNDE/IPA example
33
DPF example
34
DPFExample
  • 3580 transitions resulting in 924 levels

Short distances
Large distances
Note 1st estimate for the Ca scattering length
35
  • 1- Introduction, overview
  • 2- Molecular spectroscopy
  • 3- Asymptotic approach for long-range properties
  • 4- Hamiltonian of a diatomic molecule, Molecular
    symmetries Hunds cases Basics of quantum
    chemistry

36
Very elaborated calculations
  • Bussery, Aubert-Frécon, JCP 82, 3224 (1985)
  • Marinescu, Sadeghpour, Dalgarno, PRA 49, 982
    (1994)
  • Patil, Tang, JCP 106, 2298 (1997)
  • Derevianko, Johnson, Safronova, Babb, PRL 82,
    3589 (1999)
  • Derevianko, Babb, Dalgarno, PRA 63, 052704 (2001)
  • Derevianko, Porsev, PRA 65, 053403 (2002)

37
General formalism
Asymptotic expansion of the electrostatic
interaction between two ground state atoms
2l-pole dynamic polarizability w0 static pol.
Electric multipole operators
Sum over a complete set of atomic states
(N electrons)
Accurate determination of atomic wave functions
and energies needed
Spherical harmonics
38
Most advanced and accurate developments by
Derevianko and coll
  • Separation of atomic states in summations

Excitation of valence electrons
of core electrons
of core electrons tooccupied valence states
  • Relativistic many-body perturbation theory

Relativistic frozen core Hamiltonian
Corrections due to core excitations core
polarization term
39
Typical results
  • Contribution of core polarization term to
    4 (Li), 38 (Cs)
  • Contribution of to the total 0.01
    (Li), 0.8 (Cs)
  • Estimated precision on 0.3 (Li), 3.7
    (Cs)
  • C8 0.5 (Li), 4 (Cs)
  • C10 10
  • Contribution of to C8 0.2 (Li), 10 (Cs)

40
  • 1- Introduction, overview
  • 2- Molecular spectroscopy
  • 3- Asymptotic approach for long-range properties
  • 4- Hamiltonian of a diatomic molecule, Molecular
    symmetries Hunds cases Basics of quantum
    chemistry

41
Main steps
  • Definition of the exact Hamiltonian
  • Definition of a complete set of basis functions
  • Matrix representation of finite
    dimensionperturbations
  • Comparison to observations to determine molecular
    parameters

42
Non-relativistic Hamiltonian for 2 nuclei and n
electrons in the lab-fixed frame
  • General problem
  • Leaads to a non separable equation due to
    interactions
  • Born-Oppenheimer approximation nuclei/electrons
  • Configuration Interaction electronic correlation

electrons
nuclei
with
n-n
e-e
e-n
and
Relative distances
43
Separation of center-of-mass motion
  • Originmidpoint of the axis ?center of mass
  • Change of variables

Total mass
Reduced mass
for homonuclear molecules
44
Hamiltonian in new coordinates
Radial relative motion
Hvib HrotHCoriolis
Electronic Hamiltonian
He
  • Kinetic couplings ? m/m
  • Isotopic effect
  • Origin?center of mass

He
Study of the internal Hamiltonian
Center-of-mass motion
45
Born-Oppenheimer approximation
  • HHeHeHvibHrotHCoriolis.

m/mgt1800 approximate separation of
electron/nuclei motion
Potential curves
BO or adiabatic approximation factorization of
the total wave function
Mean potential
All act on the electronic wave function
46
General form of the electronic solution
Slater determinant eigenfunction of He,
neglecting e-e interaction
  • Interaction of configurations built on Slater
    determinants for the electronic correlation
  • Two options ab initio or semi-empirical
    approaches
  • Here treatment of small systems, ie small number
    of electrons
  • Semi-empirical approach polarizable ionic core
    valence electrons
  • Atomic calculation definition of the core
    potential, atomic orbital basis
  • Molecular Hartree-Fock calculation, molecular
    orbitals
  • Configuration Interaction
  • CIPSI package from the quantum chemistry group in
    Toulouse (coll. P. Millié, F. Spiegelmann)

47
Atomic calculation effective potential for the
core representation
  • Empirical Model Potential (Klapisch 1969), with
    parameters fitted on the atomic experimental
    spectrum
  • Ab-initio pseudo-potential (Barthelat, Durand
    1975), with parameters fitted on the
    full-electron Hartree-Fock wave functions outside
    the core

48
Core polarization representation
  • BottcherDalgarno (1966), Foucrault, Millié,
    Daudey (1992)
  • Electric field seen by a core embedded in a
    molecular system,due to valence electrons and
    other cores
  • Induced dipole moment on the core l
  • Core Polarization Potential
  • cut-off functions, with l-dependent cut-off
    radii fitted on the atomic spectrum

49
Self-consistent field approximation Molecular
Hartree-Fock calculation
  • Partly includes e-e correlation as a mean field
    contribution, maintaining then an orbital product
    description of the wavefunction.
  • Fock operatoreffective one-electron hamiltonian
  • Starting from a large set of trial orbitals
    (built from gaussian atomic orbital centered at
    each core), iterative resolution of the
    Hartree-Fock equation for each electron (ie
    spectrum of the Fock operator), to get the HF
    potential, until convergence self-consistent
    field .
  • Hartree-Fock ground state F0gt Slater
    determinant built from the Nv orbitals with
    lowest energies (occupied orbitals)

50
Configuration interaction
  • Determination of the correlation energy
  • Diagonalization of He in a space of
    configurations obtained from F0gt by promoting an
    electron in an unoccupied orbital.
  • Full CI configurations for N electrons,
    from K molecular orbitals complete active space
    (CAS)
  • Tractable only for 2-3 electrons.
  • Potential energy curves

From Vcpp
Empirical terms Pavolini et al, JPB 22, 1721
(1989)
51
(No Transcript)
52
Example GTOs for alkali atoms
  • Updated static polarizabilities
  • Careful adjustments of cut-off radii
  • Systematic calculations upon request for all
    alkali pairs, through an automated procedure

53
Generalities on molecular symmetries
  • Determine the spectroscopy of the molecule
  • Guide the elaboration of dynamical models
  • Allow a complete classification of molecular
    states by
  • Solving the Schrödinger equation
  • Looking at the separated atom limit (R??)
  • Looking at the united atom limit (R?0)
  • Adding electron one by one to build electronic
    configurations

54
Symmetry properties of electronic functions (1)
spin
Planar symmetry
  • Axial symmetry 2p rotation

Central symmetry
gerade
ungerade
55
Symmetry properties of electronic functions (2)
  • is not a good quantum number (precession around
    the axis)
  • is a good quantum number if electrostatic
    interaction is dominant

Ex
2S1 multiplicity
S states spin fixed in space, 2S1 degenerate
components L states precession around the axis,
multiplet structure, almost equidistant in energy
56
Symmetry properties of electronic functions (3)
Otherwise
57
References
  • H. Lefebvre-BrionR.W. Field, The Spectra and
    Dynamics of Diatomic Molecules , Elsevier
    Academic Press, 2004
  • G. Herzberg, The Spectra od Diatomic Molecules
    , Van Nostrand-Reinhold, Princeton, 1950,
    reprinted in 1989 by Krieger, Malabar.
  • P.R. BunkerP. Jensen, Fundamentals of
    molecular symmetry , IOP series in Chemical
    Physics, 2005.
  • Tutorials from G. Amat (Paris), A. Beswick
    (Orsay), C. Jungen (Orsay)
  • Bibliographic Databases
  • DiRef a bibliographic database for diatomic
    molecules, J. Mol. Spectrosc. 207, 287 (2001)
    http//diref.uwaterloo.ca
  • Cold Molecules http//www.lac.u-psud.fr/coldmolec
    ules, in progress
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