Institut Laue Langevin Grenoble, France.
Noise of quantum chaotic systems in the classical limit Robert S Whitney
R.W. Phys. Rev. B 75
235404 (2007)
R.W. and Ph. Jacquod, Phys. Rev. Lett. 96 206804 (2006) Ph. Jacquod and R.W. Phys. Rev. B 73 195115 (2006) R.W. and Ph. Jacquod, Phys. Rev. Lett. 94 116801 (2005)
OUTLINE
Quantum particles: Noise in current
y0
!
Classical particles: No noise in current y
...and classical limit of quantum? Random matrix theory (RMT)
⇒ “noise in classical limit” NEW REGIME in classical limit — Not RMT Should revisit old questions for new regime:
Tunnel-barriers on leads
NOISE DUE TO TUNNEL-BARRIER Multi-mode quantum wire:
Independent processes ⇒ central limit theorum Fano factor, F = (1− transmission prob.)
"δI 2 # = F × e × I
Classical limit: wavelength λF & other scales barriers ⇒ impenetrable/transparent ⇒ noiseless
CLASSICAL DETERMINISM
NOISE DUE TO CHAOTIC SYSTEM
λF & W & L
Chaotic system: L "F W
Bohigas-Giannoni-Schmit (1984): obeys random matrix theory??
"δI 2 # = F × e × I
Fano factor, F = 1/4
Classical limit (λF & W, L) : noise in I remains
NO CLASSICAL DETERMINISM ...similar for integrable system (i.e. rectangle): not RMT, but expect noise
EXPERIMENT SAYS “NOT RMT”
"δI 2 # =
Oberholtzer et al, Nature (2002)
F × eI
...fits theory for smooth disorder
F
Aleiner-Larkin (1996,1997) Agam-Aleiner-Larkin (2000)
W/λF
R
λF & R
...introduced Ehrenfest time
RAY-OPTICS for the 21st century Landauer-B¨ uttiker:
scattering matrix
⇒ Fano-factor
S=
!
r t t! r!
semiclassics (vanVleck/Gutzwiller):
tnm =
y0
!
y
&
%
"
F =
# $ Bnm × Aγ exp iSγ /¯ h
γ classical action/stability
⇒ Sγ , Aγ
join lead-modes
y0
y
!2 y0 y’0
y y’
!4 !2 !3
⇒ Bnm
!2 =!1 average
y0
average
y0 y’0
!1
tr[t† tt† t] =
$
over classical paths from mode m to n
!1
tr[t† t] =
#
tr t† t−t† tt† t tr[t† t]
y
!1 !4 !2 !3 encounter
y y’
DYNAMICS OF CLASSICAL PATHS Relative dynamics of paths y0
hyperbolic chaos: Lyapunov exponent =
(r,p)
hyperbolic dynamics uncorr. correlated escape escape
(r,p)
rmin
W
y0
λ
random dynamics ~L
W
T (rmin ) Log. timescale: T (rmin ) = 2λ−1 ln[W/rmin ] Semiclassics: Integrate over exp[iδS(rmin )/¯ h]
⇒ Encounter size ∼
√
λF
⇒ T (rmin ) ∼ Ehrenfest time =λ−1 ln[L/λF ]
CALCULATING THE NOISE Closed system: RMT level-statistics Sieber(2001)
⇒ non-perturb.
Haake group (2006)
L
L
encounter
encounter L
W
Open system: RMT weak-localization Richter-Sieber(2001)
~ #E
#E W
W
encounter
~#E W
W
encounter
encounter
< #E
⇒ RMT result classical limit
encounter Braun-Heusler-M¨ uller-Haake (2006), Whitney-Jacquod (2006)
Hand-waving argument for noise
1/2
"F
W wavepacket escapes in pieces
⇒ RMT NOISE
1/2
"F
W
wavepacket escape as whole
⇒ NO NOISE
Suppression in classical limit W
W
W
encounter
encounter
< #E
W
encounter
Classical limit: escapes without diverging to ) W
encounter
# $ F ∝ tr t† t − t† tt† t → zero
Recover CLASSICAL DETERMINISM Classical limit noiseless ⇒ not random matrix theory (RMT)
proposed in Beenakker, van Houten (1991)
NEW CLASSICAL REGIME Closed system level−statistics, etc
1 Open system Noise, cond. fluct., etc
RMT regime
system specific 10 system specific
system size/wavelength RMT regime
classical regime
# E #D
Dwell time, τD , is time to escape system
Weight of non-classical contributions = probability to escape before Ehrenfest time, τE = exp[−τE //τD ]
⇒ RMT-to-CLASSICAL cross-over powerlaw in L/λF , exponent= (λτD )−1 & 1
PHASE-SPACE (PS) BASIS
• complete & orthonormal basis:
states localized in r and p
p/p F
States on large bands (area > ¯ h) ~WR /L exp[−"t 1 ]
1-to-1: ingoing ↔ outgoing
~WR /L exp[−" t2 ]
WL /L
phase−space
phase−space
L lead
R lead
q/L
Classical limit: DIAGONALIZE scattering matrix ALL eigenvalues = 0,1 ALL cummulants of noise = 0
TUNNEL-BARRIERS ON LEADS Whitney (2007)
system ⇒ classical limit barriers ⇒ quantum tunnel probability
= ρj
V 1
for lead j
2
⇒ usual semiclassics
PS-basis not useful
I
3
[A] a quantum contribution
⇒ Random matrix result chaotic system
[B] a classical contribution
path 1
Lead m0
Lead m
path 3
chaotic system
??
Lead m0
??
path 1
Lead m
path 3
Exhausive list of contributions m
(b)
m0 path 1
path 1 path 3
path 3
m
path 1
0
m0
(e) m 0
path 3
m
(f) m 0
path 1
path 3 path 3 CLASSICAL limit
m0 (g) m 0 path (a) 1 path 3
path 1 $ path 3
m
(d) m 0 path 1
m
path 1
m
path 3
(b) m 0
m
path 1
m
(e) m 0 path 1
m
path 3
(h) m 0
m
path 3
(f) m 0 path 1
m
path 3
m
path 1
m
path 3
path 3
path 1
(c) m 0 path 1
path 3
path 3
(g) m 0
m path 1
er
(d) m
(c)
m
ov s−
m0
os
(a)
cr
RMT limit
(i) m 0
m path 1 path 3
EXAMPLE: Tunnel-barrier on third lead
F
V 1 2 3
1/2 I
4/9
RMT 1/4
classical 0 0
61/2 5−12 = 0.088 61/2 6−12
(61/2−2) =0.42
1
%
CONCLUSIONS Noiseless transport in classical limit • “wavepacket” escapes as a whole before spreading to lead width Closed system
RMT regime
system specific
level−statistics, etc
1 Open system Noise, cond. fluct., etc
10 system specific
system size/wavelength RMT regime
classical regime
# E #D
F 1/2 4/9
RMT 1/4
classical 0 0
1/2
(6 −2) =0.42
61/2 5−12 = 0.088 61/2 6−12
1
%