Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group

Gaussian-optical approach to stable periodic orbit resonances of partially chaotic dielectric micro-cavities

Open Access Open Access

Abstract

The quasi-bound modes localized on stable periodic ray orbits of dielectric micro-cavities are constructed in the short-wavelength limit using the parabolic equation method. These modes are shown to coexist with irregularly spaced “chaotic” modes for the generic case. The wavevector quantization rule for the quasi-bound modes is derived and given a simple physical interpretation in terms of Fresnel reflection; quasi-bound modes are explictly constructed and compared to numerical results. The effect of discrete symmetries of the resonator is analyzed and shown to give rise to quasi-degenerate multiplets; the average splitting of these multiplets is calculated by methods from quantum chaos theory.

©2002 Optical Society of America

Full Article  |  PDF Article
More Like This
Separatrix modes in weakly deformed microdisk cavities

Chang-Hwan Yi, Julius Kullig, Ji-Won Lee, Ji-Hwan Kim, Hyeon-Hye Yu, Jan Wiersig, and Chil-Min Kim
Opt. Express 25(7) 8048-8062 (2017)

Kolmogorov–Arnold–Moser transition and laser action on scar modes in semiconductor diode lasers with deformed resonators

Claire Gmachl, Evgueni E. Narimanov, Federico Capasso, James N. Baillargeon, and Alfred Y. Cho
Opt. Lett. 27(10) 824-826 (2002)

Dramatic shape sensitivity of directional emission patterns from similarly deformed cylindrical polymer lasers

Harald G. L. Schwefel, Nathan B. Rex, Hakan E. Tureci, Richard K. Chang, A. Douglas Stone, Tahar Ben-Messaoud, and Joseph Zyss
J. Opt. Soc. Am. B 21(5) 923-934 (2004)

Cited By

Optica participates in Crossref's Cited-By Linking service. Citing articles from Optica Publishing Group journals and other participating publishers are listed here.

Alert me when this article is cited.


Figures (8)

Fig. 1.
Fig. 1. Surface of section illustrating the different regions of phase space for a closed quadrupole billiard with boundary given by r(ϕ) = R(1 + cos 2ϕ) for = 0.072. Real-space ray trajectories corresponding to each region are indicated at right: a) A quasi-periodic, marginally stable orbit. b) A stable four-bounce “diamond” periodic orbit (surrounded by stability “islands” in the SOS) c) A chaotic ray trajectory. Orbits of type (b) have associated with them regular gaussian solutions as we will show below.
Fig. 2.
Fig. 2. Black background gives the surface of section for the quadrupole at = 0.17 for which the four small islands correspond to a stable bow-tie shaped orbit (inset). A numerical solution of the Helmholtz equation for this resonator can be projected onto this surface of section via the Husimi transform[28] and is found to have high intensity (in false color scale) precisely on these islands, indicating that this is a mode associated with the bow-tie orbit.
Fig. 3.
Fig. 3. (a) Vertical lines indicate wavevectors of bound states of the closed quadrupole resonator for = 0.17; no regular spacings are visible. (b) Spectrum weighted by overlap of the Husimi function of the solution with the bow-tie island as in Fig. 2. Note the emergence of regularly spaced levels with two main spacings Δklong and Δktrans . These spacings, indicated by the arrows, are calculated from the length of the bow-tie orbit and the associated Floquet phase (see Section 2.4 below). The color coding corresponds to the four possible symmetry types of the solutions (see Section 4 below). In the inset is a magnified view showing the splitting of quasi-degenerate doublets as discussed in Section 4.3. Note the pairing of the (+, +) and (+, -) symmetry types as predicted in section 4.2. The different symmetry pairs alternate every free spectral range (Δklong ).
Fig. 4.
Fig. 4. Illustration of the reduction of the Maxwell equation for an infinite dielectric cylinder to the 2D Helmholtz equation for the TM case (E field parallel to axis) and k = 0.
Fig. 5.
Fig. 5. Coordinate system and variables used in the text displayed for the case of a quadrupolar boundary ∂D and the diamond four-bounce PO. A fixed coordinate system (X, Z) is attached to the origin. The “mobile” coordinate systems (xm ,zm ) are fixed on segments of the periodic orbit so that their respective z-axes are parallel to the segment, while their origins are set back a distance Lm (or nLm for transmitted beam axes), so as to account for zeroth order phase accumulation between successive bounce-points. ξ 1, ξ 2 are the common local coordinates at each bounce (index m suppressed). Scaled coordinates are denoted by tildes, e.g. m = √kxm . The coordinate transformations at each bounce m are given by zi = Lm + ξ 1 sin χi + ξ 2 cos χi , zr = Lm + ξ 1 sin χi - ξ 2 cos χi , zt = nLm + ξ 1 sin χt + ξ 2 cos χt and xi = ξ 1 cos χi - ξ 2 sin χi , xr = ξ 1 cos χi + ξ 2 sin χi , xt = ξ 1 cos χt - ξ 2 sin χt , where i, r, t refer to the incident, transmitted and reflected solutions.
Fig. 6.
Fig. 6. Intensity of the TM solution for a bow-tie mode plotted in a false color scale, (a) calculated numerically and (b) from the gaussian optical theory with parameters m = 100, φ = 2.11391, Nμ = 1 and N = 4. Note the excellent agreement of the quantized values for kR (R is the average radius of the quadrupole).
Fig. 7.
Fig. 7. Schematic indicating a direct tunneling process (black arrow) and a chaos-assisted tunneling process (yellow arrow) which would contribute to splitting of bow-tie doublets.
Fig. 8.
Fig. 8. The numerically determined splittings of bow-tie doublets for a closed quadrupole resonator with ε = 0.14 (black dots) vs kR; the red line denotes the prediction of Eq. (60) for the average splitting, the blue line an estimate of the splitting based on the “direct” coupling. Note the large enhancement due to chaos-assisted tunneling and the large fluctuations around the mean splitting.

Tables (2)

Tables Icon

Table 1. Comparison of the gaussian optical predictions

Tables Icon

Table 2. Illustration of the symmetry rules for the quadrupole

Equations (72)

Equations on this page are rendered with MathJax. Learn more.

( 2 + k 2 ) E = 0
E ( X , Z ) = m = 1 N E m ( x m ( X , Z ) , z m ( X , Z ) )
E m ( x m , z m ) = u m ( x m , z m ) e ik z m
( m 2 + k 2 ) E m = 0
E m + E m + 1 | D = 0
u xx + u zz + 2 ik u z = 0
u x ˜ x ˜ + 1 k u zz + 2 i u z = 0 .
u ( x ˜ , z ) = 0
u ( x , z ) = c A ( z ) exp [ i 2 Ω ( z ) x ˜ 2 ]
Ω 2 + Ω = 0
A Ω + 2 A = 0
Ω = Q ( z ) Q ( z )
Q = 0
Q Q + 2 A A = 0
c m Q m ( z m ) exp ( ik z m + i 2 Ω ( z m ) x ˜ m 2 )
+ c m + 1 Q m + 1 ( z m + 1 ) exp ( ik z m + 1 + i 2 Ω ( z m + 1 ) x ˜ m + 1 2 ) | D = 0
k ( l m + 1 k ξ ˜ 1 sin χ m 1 k ξ ˜ 1 2 2 ρ m cos χ m ) + 1 2 Q m Q m ( ξ ˜ 1 cos χ m + 1 k ξ ˜ 1 2 2 ρ m sin χ m ) 2 =
k ( l m + 1 k ξ ˜ 1 sin χ m + 1 k ξ ˜ 1 2 2 ρ m cos χ m ) + 1 2 Q m + 1 Q m + 1 ( ξ ˜ 1 cos χ m + 1 k ξ ˜ 1 2 2 ρ m sin χ m ) 2
c m Q m ( L m ) + c m + 1 Q m + 1 ( L m ) = 0
( Q m + 1 Q m + 1 ) = ( 1 0 2 ρ m cos χ m 1 ) ( Q m Q m ) m ( Q m Q m )
C m + 1 = e i π C m
= ( Q 1 Q 2 P 1 P 2 )
d dz = H
( Q ( z ) P ( z ) ) = ( z ) h m
( Q m ( z + l ) P m ( z + l ) ) = ( l ) ( Q m ( z ) P m ( z ) ) .
( Q m + 1 ( z ) P m + 1 ( z ) ) = ( z L m ) m ( L m z ) ( Q m ( z ) P m ( z ) )
𝚳 ( z ) = ( z L m 1 ) m 1 ( l m 1 ) ( l m + 1 ) m ( L m z )
E ( x , z + L ) = E ( x , z ) .
u ( x , z + L ) e ikL = u ( x , z ) .
p q * q p * = i .
u ( x ˜ , z + L ) = e i φ 2 ( N μ + N ) u ( x ˜ , z )
kL = 1 2 φ + 2 π m + mod 2 π [ ( N + N μ ) π ]
N μ = [ 1 2 π i 0 L d ( ln q ( z ) ) ]
Λ ( z ) = iq ( z ) x ˜ + p ( z ) x ˜
Λ ( z ) = i q * ( z ) x ˜ + p * ( z ) x ˜ .
u ( l ) ( x ˜ , z ) = ( Λ ) l u ( 0 )
kL = ( l + 1 2 ) φ + 2 π m + mod 2 π [ ( N + N μ ) π ]
u ( l ) ( x ˜ , z ) = ( i q * ( z ) 2 q ( z ) ) l H l ( I m [ p ( z ) q ( z ) ] x ˜ ) u ( 0 ) ( x ˜ , z )
( 2 + n ( r ) 2 k 2 ) Ψ = 0
E i + E r | D = E t | D +
n E i + n E r | D = n E t | D +
Φ i = nk ( L m + 1 nk ξ ˜ 1 sin χ 1 nk ξ ˜ 1 2 2 ρ cos χ ) + 1 2 Q i Q i ( ξ ˜ 1 cos χ + 1 nk ξ ˜ 1 2 2 ρ sin χ ) 2
Φ t = k ( n L m + 1 nk ξ ˜ 1 sin χ t 1 nk ξ ˜ 1 2 2 ρ cos χ t ) + 1 2 Q t Q t ( ξ ˜ 1 cos χ t + 1 nk ξ ˜ 1 2 2 ρ sin χ t ) 2
( Q t Q t ) = ( 1 μ 0 2 ( 1 μ ) ρ cos χ n μ ) ( Q i Q i )
c i Q i + c r Q r = c t Q t
c i + c r = μ c t
c i n Φ i + c r n Φ r = μ c t n Φ t .
n μ ( c i c r ) = c t
c r = 1 + 1 c i .
c r 2 = n cos χ i cos χ t 2 n cos χ i + cos χ t 2 c i 2
E ( x , z + L ) = E ( x , z )
u ( x , z + L ) e inkL = u ( x , z )
nkL = 1 2 φ + 2 πm + mod 2 π [ ( N + N μ ) π ] i b = 1 N log [ n μ b 1 n μ n + 1 ] .
Re [ nkL ] = 2 πm + mod 2 π [ ( N + N μ ) π ] + φ 2 + φ f
Im [ nkL ] = γ f .
P m E ( x ) = d m G g G χ m ( g ) E ( g x )
E ( + + ) = 1 4 ( e 1 + e 2 + e 3 + e 4 ) , E ( + ) = 1 4 ( e 1 + e 2 e 3 e 4 )
E ( + ) = 1 4 ( e 1 e 2 + e 3 e 4 ) , E ( ) = 1 4 ( e 1 e 2 e 3 + e 4 )
e 1 = E ( X , Z ) , e 2 = E ( X , Z ) , e 3 = E ( X , Z ) , e 4 = E ( X , Z ) .
e 1 = E ( g x ) = 1 q ( z ) exp [ ikz + i 2 Ω ( z ) x 2 ]
e 2 = E ( g x ) = e 1 2 i π 1 e i φ 2 q ( z ) exp [ ik ( z + L 2 + i 2 Ω ( z ) x 2 ) ] e i ζ e 1
e 3 = E ( g x ) = 1 q ( 1 z ) exp [ ik ( 1 z ) + i 2 Ω ( 1 z ) x 2 ]
e 4 = E ( g x ) = e 1 2 i π 1 e i φ 2 q ( 1 z ) exp [ ik ( L 2 + 1 z ) + i 2 Ω ( 1 z ) x 2 ] e i ζ e 3
E ( + + ) = 1 2 ( e 1 + e 3 ) e i ζ 2 cos ζ 2
E ( + ) = 1 2 ( e 1 e 3 ) e i ζ 2 cos ζ 2
E ( + ) = 1 2 i ( e 1 + e 3 ) e i ζ 2 sin ζ 2
E ( ) = 1 2 i ( e 1 + e 3 ) e i ζ 2 sin ζ 2
E ( + + ) , E ( + ) cos ζ 2 = 0 m = 1,3,5 , . . .
E ( + ) , E ( ) sin ζ 2 = 0 m = 0,2,4 , . . .
Δ E CAT V RC 2 E R E C
V RC 2 d ϕ d sin χ W C ( ϕ , sin χ ) W R ( ϕ , sin χ )
Δ E CAT exp ( Ak R 0 )
Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All rights reserved, including rights for text and data mining and training of artificial technologies or similar technologies.