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Dynamical Casimir emission Dynamical Casimir emission and back-action effects and back-action effects
in optically modulated microcavitiesin optically modulated microcavities
Iacopo CarusottoINO-CNR BEC Center and Università di Trento, Italy
In collaboration with:● Cristiano Ciuti and Simone De Liberato (MPQ, Université Paris-Diderot)● Dario Gerace ( Università di Pavia )
International Workshop on Dynamical Casimir Effect, Padova, June 6-8, 2011
The dynamical Casimir effect
Mechanically shake it very fast
Take an optical cavityin the e.m. vacuum state
Beware when you open it again: (a few) photons may burn you !!
Mechanism of photon generation:● theoretically well understood● first experimental evidences now available
Open questions:● back-action of DCE emission onto mirrors● how does one feel the DCE photons while mechanically shaking the cavity?
How strong is the back-action effect?
Half-space slab of refractive index n and mass M Mechanically oscillating at frequency Ω Prediction for the dissipated energy within 1D scalar model:
(from Barton and Eberlein, Ann. Phys. 227, 222 (1993))
➔ value is ridiculously small➔ very little hope of experimental observation
Q−1=
2Eosc
dEdiss
dt=1
6 n−1n
2 ℏMc2
n
Ω
What matters is optical length of cavity Lopt
= n L
Mechanical oscillation of mirrors ↔ Modulation of refractive index
Emission strongest on resonance with cavity modes: Ω = ωi + ω
j
All-optical Dynamical Casimir effect
Ω Ω
n(t)=n0+ dn cos(Ωt)
V. V. Dodonov et al., PRA 47, 4422 (1993); Yablonovitch, PRL. 62, 1742 (1989); Law, PRA 49, 433 (1994).
Photo-excitation of carriers in mirrorBraggio et al., EPL 70 754 (2005)
χ(3) nonlinear medium pumped by ultrashort pulsed laser
IC and D. Faccio, in preparation
DCE vs. optical parametric oscillatorDezael and Lambrecht, EPL 89 14001 (2010)
Time-dependent EIT in atomic Mott insulatorIC et al., PRA77, 063621 2008
Circuit QED: effective cavity length modulated via external B on SQUID
Wilson et al.,, PRL 105, 233907 (2010); arXiv:1105.4714
Physical implementations
θ } Doped QWs
Conduction band
1
2
Energy
mirror
mirror
cavity modetuned in the
far-IR,resonant withintersubbandtransition indoped QW doping provides electrons
in lowest subband ofconduction band
Intersubband transition in doped quantum wellsembedded in a semiconductor microcavity
D. Dini et al., PRL 90, 116401 (2003)
L. Sapienza et al., PRL 100, 136806 (2008)
Upper Polariton
Ultra-strong coupling regime
For each value of in-plane wavevector k:● one cavity-photon state coupled to
one matter excitation● bosonic mixed polaritonic excitations
(a kind of dressed photons)● strong-coupling Ω
R > Γ
● ultra-strong coupling ΩR~ ω
0
Theory: C. Ciuti, G. Bastard, IC, PRB 72, 115303 (2005)
(Bosonized) system Hamiltonian
System Hamiltonian quadratic in bosonic field operators:● a
q → cavity photon; b
q → intersubband collective excitation
● Rabi frequency ΩR couples cavity photon ↔ intersubband excitation
● if ΩR comparable to
ω
cav, ω
12 → anti-RWA terms relevant,
create/destroy pairs of excitations● ground state contains finite number of excitations
C. Ciuti, G. Bastard, IC, PRB 72, 115303 (2005)
Ground state of system: polaritonic vacuum
contains (virtual) photons and intersubband excitations
The non-trivial vacuum state
Hamiltonian diagonalized via Bogoliubov transformation
New bosonic operators:
C. Ciuti, G. Bastard, IC, PRB 72, 115303 (2005); C. Ciuti, IC, PRA 74, 033811 (2006)
Extra photons are released as radiation at the bare cavity frequency
Non-adiabatic jump of ΩR
Polaritonic vacuum
C. Ciuti, G. Bastard, IC, PRB 72, 115303 (2005)
Periodic modulation of ΩR at frequency ω
mod
● Steady-state emission of photons
● Intensity maximum on resonance with polariton frequencies
● As a function ωmod
three peaks A,B,C : 2xLP, UP+LP, 2xUP
● Emission spectrum peaked at polaritons
● Resonant-cavity-enhanced parametric luminescence
● Significant emission intensity
S. De Liberato, C. Ciuti, IC, PRL 98, 103602 �(2007)
Semiconductor devices in the ultra-strong coupling regime
G. Guenter, et al., Nature 458, 178 (2009)
How to modulate ΩR ?
● Electrons excited from valence to conduction band via interband transition in the visible range
● Coherent control of interband transition(Rabi oscillations, π-pulses...)
● Modulate effective electron density active in intersubband transition
● Switch-on and off of ultra-strong-couplingon short time scale as comparedto far-IR oscillation period
Quantum model
Isolated system Hamiltonian:
Master equation to include losses
Dissipation super-operator (weak loss approx):
Jump operators:
Dissipation baths not white(otherwise unphysical predictions)
Density of final states vj(ω), effective decay rate in → fin:
IC, S. De Liberato, D. Gerace, C. Ciuti, Back-action effects in an all-optical model of dynamical Casimir emission, in preparation
Dynamical Casimir Emission
Steady state under resonant laser g → e with Rabi frequency Ωeg
f ↔ e transition strongly coupled to cavity
Observe:● spontaneous emission on f ↔ e ● cavity emission (DCE)
For increasing Ωeg
/ωcav
:
● First threshold at Ωeg
/ωcav
= 0.5
● Stronger threshold at Ωeg
/ωcav
= 1
● Narrow and weak peak around Ωeg
/ωcav
= 1
● Strong peak around Ωeg
/ωcav
= 2
Physical origin of thresholds
Dressed state picture: g,e mixed and split by 2Ωeg
At Ωeg
/ωcav
= 0.5 :
● |g0>-|e0> exceeds in energy |g1>+|e1>● transition weakly allowed e→ f by cavity mixing
At Ωeg
/ωcav
= 1 :
● |g0>-|e0> exceeds in energy |f0>● transition fully allowed e→ f
Physical origin of peaks
Strong peak at Ωeg
/ωcav
= 1 :
● Rabi oscillations g ↔e at 2Ωeg
● periodic switch-on/off of emitter-cavity coupling● like periodic shaking of cavity mirrors: resonant DCE● resonant non-RWA coupling |g0>-|e0> ↔ |f1>
Weak peak at Ωeg
/ωcav
= 0.5 : analogous coupling via cavity
Backaction effect
Drive laser on g ↔ e transition experiences absorption by emitter
● Absorbed energy:
● Peaks in DCE give dip in absorption
● Stronger “friction” reduces absorption rate
● Easily observed with optical techniques
Conclusions
All-optical techniques to study Dynamical Casimir effect most promising:● experimental observation in circuit QED system● read-out of back-action effect on optical quantities,
much more sensitive than mechanical ones
Ultra-strong coupling systems:● vacuum state is non-trivial squeezed state with virtual photons● non-adiabatic modulation required to release them as observable radiation● possibility of sub-cycle control of intersubband far-IR transition
via interband transition driven with visible light● complete solution of simple three-level model with realistic dissipation● interesting model also from the Quantum Optics point of view
IC, S. De Liberato, D. Gerace, C. Ciuti, Back-action effects in an all-optical model of dynamical Casimir emission, in preparation