contributions to the theory of atoms and molecules in strong...
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Contributions to the Theory ofAtoms and Molecules in Strong
Electromagnetic Fields
Defence of Dissertation for the Degree of PhD.
Sølve Selstø
Department of Physics and TechnologyUniversity of Bergen
The atom
Light
The interaction between atoms and light
Hydrogen atoms in strong, short laser pulses
The hydrogen molecular ion in laser pulses
The Landau-Zener model and single electron transport in adouble quantum dot
Summary
Atoms
http://www.physics.queensu.ca/˜nanophys/stm.html
9 nm × 6.3 nm
Some ”highlights” in the evolution of quantum mechanics
Planck and Einstein, early 1900-s: Lightsometime behaves as particles, not just waves
Bohr-model, 1913
DeBroglie, 1923: Matter sometimes behave aswaves, not just particles
Schrodinger, 1932: Wave description of matter
Some ”highlights” in the evolution of quantum mechanics
Planck and Einstein, early 1900-s: Lightsometime behaves as particles, not just waves
Bohr-model, 1913
DeBroglie, 1923: Matter sometimes behave aswaves, not just particles
Schrodinger, 1932: Wave description of matter
Some ”highlights” in the evolution of quantum mechanics
Planck and Einstein, early 1900-s: Lightsometime behaves as particles, not just waves
Bohr-model, 1913
DeBroglie, 1923: Matter sometimes behave aswaves, not just particles
Schrodinger, 1932: Wave description of matter
Some ”highlights” in the evolution of quantum mechanics
Planck and Einstein, early 1900-s: Lightsometime behaves as particles, not just waves
Bohr-model, 1913
DeBroglie, 1923: Matter sometimes behave aswaves, not just particles
Schrodinger, 1932: Wave description of matter
The time independent Schrodinger Equation:
HΨ(r) = E Ψ(r)
H = − ~2
2m∇2 + V (r)
|Ψ(r)|2 gives the probability of finding the particle near position rHydrogen:Quantum numbers n, l and m, energy En = −B0
n2
n, l ,m =1, 0, 0 2, 1, 0 2, 1, 1 3, 2, 1 4, 3, 0 7, 3, 1
Light
-Consists of variouscolours/ wavelengths
Traveling electromagnetic wave
Specter
LASER
Produced through stimulatedemission
One single colour
Very intense, coherent light
• Treat the field classically
• The Dipole Approximation
E(r, t) → E(t)
The interaction between matter and light
The time dependent Schrodinger equation:
HΨ = i~∂
∂tΨ
Hamiltonian: H = Hatom + Hint
Different descriptions of the interaction:
Length gauge Velocity gauge KH frameHint = −qr · E(t) Hint = − q
mp · A(t) r → r −α(t)• Classical trajectory of a free particle in the electric field E(t):
α(t) = − q
m
∫ t
t0
∫ t′
t0
E(t ′′) dt ′′ dt ′
The Kramers Henneberger frame
HKH = − ~2
2m∇2 + V (r −α(t)) +
(q2
2mA(t)
)The particle ”sees” a moving potentialThe transition from velocity gauge to KH frame can be donewithout the dipole approximation;
HNDKH → − ~2
2m∇2 + V (r −α(r, t)) +
q2
2m(A(r, t))2
corresponding to a non-homogeneous field E(r, t)
Hyrogen atom exposed to short,intense laser pulse
E0 r
+
−
λ
Atomic Stabilisation
0 5 10 15 20 250
0.1
0.2
0.3
0.4
0.5
0.6
0.7
Electric Field Strength (a.u.)
Ioni
zatio
n P
roba
bilit
y
High frequency
Probability of ionisation decreases with increasing intensity/frequency
Claim: Artifact of the dipole approximation
Found that the phenomena sustains inclusion of the spatialdependence of the field
The stabilistaion mechanism understood at a consequence ofthe multi-photon channel ”closing down”
Dynamics described by the time averaged KH potential:VKH(r, t) ∼ − 1
|r−α(t)| → V 0KH(r) = − 1
T
∫T
1|r−α(t)| dt
VKH(r, t) V 0KH(r)
For strong fields of high frequency, the dipole approximationbreaks downAngular distribution of the photo electron after ionization ofatomic hydrogen:
Dipole Non dipole
The interplay between the Coulomb, electric and magnetic fieldleads to the appearance of a third lobe in the angular distribution
Photo-ionisation of H+2
E
+
+R
−r
Fixed nuclei approximation
PI (R,E0) for θ = 0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
1 2 3 4 5
2
4
6
8
10
R (a.u.)
E0 (a
.u.)
PI (R, θ) for E0 = 3.0 a.u.
0 1 2 3 4 5 030
60900
0.2
0.4
0.6
0.8
1
θ (degrees)Internuclear distance (a.u.)
Ioni
satio
n pr
obab
ility E
+
+R
−r
Model:
Interfering waves traveling from each of the protons:
ψout = f (Ω1)exp(ikr1)
r1+ f (Ω2)
exp(ikr2)
r2
Angular Distributions
Model: ψout → f (Ω) cos(1/2 k r · R)e ikr/r⇒ dP
dΩk∝ |f (Ω)|2 cos(1/2 k · R)
Does not give very good agreement for parallel polarisationReason: Coulomb scattering
Accounted for by the eikonal (WKB) approximation
θ = 0 θ = 45 θ = 90
k
E
R = 2a.u.
−90 −60 −30 0 30 60 900
0.01
0.02
0.03
0.04
0.05
0.06
−90 −60 −30 0 30 60 900
0.02
0.04
0.06
0.08
0.1
0.12
0.14
−90 −60 −30 0 30 60 900
0.05
0.1
0.15
0.2
R = 3a.u.
−90 −60 −30 0 30 60 900
0.05
0.1
0.15
0.2
0.25
0.3
−90 −60 −30 0 30 60 900
0.02
0.04
0.06
0.08
0.1
0.12
0.14
0.16
−90 −60 −30 0 30 60 900
0.05
0.1
0.15
0.2
Two photon ionisation with moving nuceli
Born-Oppenheimer approximationCorrect asymptotic behaviour in the final electronic states
Ψ(R, r, t) =∑n
∫∑νn
cn,νn(t)χνn(R)ψeln (R; r) +
∑l
∫dε
∫∑νε
c lε,νε
(t)χνε(R)ψell ,ε(R; r)
The Landau-Zener modelEnergies (adiabatic) Populations
−30 −20 −10 0 10 20 30−40
−30
−20
−10
0
10
20
30
40
Time
Ene
rgy
−30 −20 −10 0 10 20 300
0.2
0.4
0.6
0.8
1
Time (a.u.)
Pop
ulat
ion
The transition probabilities at each avoided crossing may befound analytically
The dynamcs are given by trivial phase evolution betweenavioded crossings
These ideas have been used to describe electron transport in acoupled quantum dot
Gorman et al. Phys. Rev. Lett. 95, 090502 (2005)
-Artificial molecule
4-state model:
g1 g2
e1 e2
ε
Ve
Vg
D
21
−4 −2 0 2 4
−10
−5
0
5
10
TimeE
nerg
y
E (t) = E0 sin(ωt)
In summaryStudied ionization dynamics of hydrogen• Shown that atomic stabilsation is not an artifact of thedipole approximation• Describe the phenomena accounting for dynamicstabilisation• Found signature of non-dipole interaction inphoto-ionisation in the strong field regime
Investigated the importance of geometrical factors inphoto-ionisation of H+
2 and explain its origin in terms ofinterference and refraction.• Describe angular distribution of the photoelctron includinginternuclear vibration.
Application of analytical models to describe few-level systems• Feasible method of coherent single electron transportbetween couple quantum dots
In alphabetical order
A. Palacios F. Martın I. Sundvor J. P. Hansen
J. Fernandez J. McCann L. Kocbach L. B. Madsen
M. Volkov M. Førre T. Birkeland V. Ostrovsky
The Keldysh parameter
γ =ω√
2mIp
|q|E0
0 5 10 150
0.5
1
1.5
2
2.5
3
3.5
Field strength (a.u.)
Kel
dysh
Par
amet
er
0 5 10 15 20 250
1
2
3
4
5
6
7
8
Field strength (a.u.)
Kel
dysh
Par
amet
er