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HAL Id: jpa-00210190

https://hal.archives-ouvertes.fr/jpa-00210190

Submitted on 1 Jan 1986

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Vectorial bistability in a quasi-isotropic laser

D. Hugon, G. Stéphan

To cite this version:

D. Hugon, G. Stéphan. Vectorial bistability in a quasi-isotropic laser. Journal de Physique, 1986, 47

(2), pp.153-156. �10.1051/jphys:01986004702015300�. �jpa-00210190�

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153

Vectorial bistability in a quasi-isotropic laser.

D. Hugon* and G. Stéphan**

Université de Rennes, Laboratoire de Spectroscopie+, Avenue du Général

Leclerc, 35042 Rennes Cedex, France

(Reçu Ze 29 août 1985, aaaepté Ze 25 novembre 1985)

Résumé.2014 Nous montrons théoriquement et ex- périmentalement que le domaine de bistabi- lité vectorielle observable lors du bascu- lement de polarisation dans un laser quasi- isotrope diminue quand l’intensité de la lumière augmente.

Abstract.2014 The domain of vectorial bistabi- lity observable in the polarization flip of

a quasi-isotropic laser is theoretically

and experimentally shown to decrease when

light intensity increases.

LE JOURNAL DE PHYSIQUE

J. Physique 47 (1986) 153-156 FÉVRIER 1986, PA

Classification Physics Abstracts

42.55 B - 42.60 H

The polarization of light in a la-

ser can generally be defined by two eigen-

vectors. Quite often these vectors do not

depend on the laser frequency and their ei- genvalues are so different from each other that the light polarization remains always the same. This is the case of lasers con-

taining Brewster windows. But in the case of a quasi-isotropic laser the eigenvectors

may be frequency-dependent and vary within the emission line. And even if they didn’t their associated eigenvalues might show a

variation introducing a polarization flip.

We have recently produced [1] such an ef- fect using a 3.39 um single mode He-Ne la-

ser. In this experiment the amplifying tube

was closed with quasi-perpendicular windows

at 86° to the laser propagation axis z (Fig. 1). Therefore there was a slight pha-

se and loss anisotropy and the preferred polarization of the tube was in the windows incidence plane yz. However this anisotropy

could be neglected when compared to that induced by the optical feedback of the de- tector system. The polarizer had its axis aligned with the cavity y axis. Therefore the eigenvectors of the system were unchan- ged when optical feedback was taken into

account. This effect can be accounted for

Fig. 1.- Experimental arrangement. 1 : mir-

ror Ra (plane mirror) ; 2 : mirror Rb (con-

cave mirror) ; 3 : polarizer ; 4 : detector (InAs) ; 5 : LiF lens ; 6 : tube window ; 7 : piezo-electric ceramic ; 8 : magnetic shielding ; 9 : diaphragm. d is the geome- trical length of the laser and L is the op- tical distance between the output mirror Rb

and the detector. In this experiment the optical feedback is provided by the light diffused by the detector. Numerical data

are the same as in ref. 1.

theoretically by an anisotropic reflectivi- ty of the exit mirror Rb : Rx = Rb on the x

axis and Ry = Rb+ E exp (iO) on the y axis.

Rb is the isotropic reflectivity coeffi- cient of the mirror and E and (b represent the feedback amplitude and phase. Because

E « Rb one writes IR, I = Rb + E cos 4). Let n, be the angular frequency of the laser when oscillating on the y axis, L the opti- cal distance separating the exit mirror Rb

from the detector and d the cavity length.

As (0=211yL/c, one obtains M = 2TEL/d within

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01986004702015300

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154

Fig. 2.- Light intensity of the single mode

laser vs. frequency detected through the polarizer. Because L = d, cos ~ varies

slowly and the region AB of bistability of polarization in clearly seen. In (a) the

discharge current is i c = 5 mA, in (b) ic =

7 mA in (c) ic = 9 mA. The plane mirror

vibrates at 50 Hz and the exposure time was

0.5 s i.e. each picture contains a superposition of 25 forward and backward

curves. It is clearly seen that the domain

AB decreases as light intensity increases

in ,this case. Other experiments with L > d reveal the same result, but less clearly.

the spectral range aw

=

itc/d. This means that 0 will go through L/d cycles within this range. jR j will then be alternatively larger and smaller than Rx and the emission

line, when observed through the polarizer,

will be sliced up with dark crenels.

This letter is meant to study the hysteresis phenomenon of a polarization flip : the flip does not occur at the same frequency for increasing or decreasing fre- quencies [2]. This is shown in figure 2 in

a case where L=d and where the origin our 40 is adjusted so that cos 0

=

0 is within the line. This can be done by either rotating the polarizer around its y axis or slightly tilting the fixed mirror (here the output mirror Rb). One can then observe that the

hysteresis or polarization bistability ran-

ge decreases with an increase of the laser

intensity.

In order to describe this effect,

we use Lamb’s homogeneous theory ; this is justified as, in this experiment, we are studying the laser polarization and fre-

quency which are independent of the loca- tion within the sytem. The amplifying me- dium is represented by a saturated tensor

a .

.

Its components may be written as fol- lows when the field is oscillating on the x

axis [3]:

In these equations S, Sp and Sz are sums

containing squares of electric dipole ma-

trix elements. No is the positive popula- tion difference between the two transition states. E2 is the intensity of the satura-

ting field. The line shape is described by the plasma dispersion function Z(C) (posi-

tive imaginary part) and by the two func- tions II and I_I (negative real parts).

Further details may be found in reference [3]. The losses are spread over the pheno- menological Lamb’s medium and are represen- ted by the following tensor [4]:

p (components q>.and PY 1 is the phase angle and Q (components Qx and Q y) the quality

factor associated with each axis at the

corresponding resonance frequency for the empty cavity. By deriving Lamb’s evolution equations [5] we get :

II is the laser resonance frequency and w

.

the actual field frequency. 0 and E repre-

sent the field phase and amplitude varia-

tions. These equations are valid as long as

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~

the medium polarization P is constant over

the time interval considered. A flip time is of the order of the field variation time in the cavity, i.e. 10-8 s for our experi-

~

mental setting. P varies with the atomic quantities of the sytems. Its characteris- tic time is about 10-’ s. Here we only con- sider the very beginning of the flip and

not the way with which it develops. Within this approximation we assume that the field oscillates on the x axis (E ) and we are

x

looking for a condition at which the initi- ally inexistent Ey mode (on the y axis) be-

gins to grow. Equation (3b) will give the difference in the speed of variation of two

probes : one launched along the y axis (the rising Ey mode) and the other one superim-

posed on the Ex lasing field. However befo-

re making the calculation we have to look at the actual Q factor seen by Ex. For this

purpose let us first examine the definition of the quality factor in the case of a pas- sive cavity with mirrors characterized by reflectances R. and Rb . In this cavity af-

ter a round trip the field becomes :

with 6t = 2d/c and 9 the usual phase P = - 2wd/c . Therefore E = E0 e-yt with

T 2- 2d (1- Ra Rb e1.). The intensity varies

with the real part of T : I = I o e-Zyrt and

yr - _c (1-R Rb cos q>). Q which is by defi- 2d ’ °

nition Q = wI/(-dI/dt) can then be written

as follows : Q = wd/(l- RaRb c cos(P). By ana-

logy and following Lamb’s method [6], we attribute Qx y (n,) to the rising Ey mode such

as : Q. (11 = 2fl (04/ C (1- R a IR v [ cos 9 xv ) with

d

[7] Oxy loy + y (1 + 0153r ’ 12£ 0 ). Even when

4P. = T. (isotropic cavity) one can see that

Q is out of resonance as e pe y ar . x Now by

writting equation (3b) separately for each

Ex and Ey f ield with y y

= (X x,y Ex y

and by subtracting their speed of variation :

When dV becomes positive, Ey grows faster than Ex which means that the polarization

will switch to the y axis. This equation

contains several different terms each of them representing a physical mechanism.

When a term is positive it tends to incre-

ase OV and to accelerate the apparition of

the flip. While if it is negative it pre- vents the laser from switching to the Ey

mode. In order to separate the different terms, we first ignore the saturation ef- fects :

a) Let us consider an empty cavity without

any phase anisotropy.

At the frequency 91v for which R - Rx beco-

mes positive an Ex ----> Ey f lip will be ob-

served. This is illustrated schematically in figure 3 where the curve a shows an in-

Fig. 3.- Scheme showing the four different mechanisms contributing to AV. Curves a,b, c,d, and a’, b’, c’, d’ are related respec-

tively to the E -->

E and E --+ E flips.

(a) (and (a)) describe the variation with the laser length of the difference R - R

(and Rx - Ry ) in the region of changing

sign. In the preceding experiment R - R =

t cos

(2fl L/c) and the sign variation was

primarily responsible for the polarization flip. (b) (and (b’)) are obtained when

and 1- 0153 1 (n ) I - !- 0153 1 (n ) I > 0.

These curves escribe

Ry y Rx 12 ) x + 1° or.

I (ay h I (x I en" ) I / &

.

and show the

role of the inear gain originating from

the frequency difference between the two ween the two fields E and E for a same

x y

length d in a laser having a linear phase anisotropy. (c) (and (c’)) show the influ-

ence of the saturation on

Q.v (and Qy x ) :

curves (b) and (b’) are lowered together.

(d) (and(d’)) show the influence of the sa-

turation dichroism on Qt.1 - Qt.1 which rise

y x

curves (c) and (c’).

A and B are the points where polarization flips occur. It is seen that the domain of

bistability AB depends strongly on the pha-

se anisotropy and that it decreases when

the light intensity increases : in this ca-

se the (d) and (d’) curves rise together

and the points A and B draw nearer.

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156

crease in Ry- Rx with an increasing fre-

quency. In the same way and E -+ E flip will occur while decreasing the frequency

when Rx- Ry becomes positive. Obviously

the two flips occur at the same frequency.

b) If we consider now a cavity with a phase anisotropy, the resonance frequencies 12 y

and 11 y for the two modes Ex and Ey are

different although the geometrical length of the laser is the same. One has :

°03B1 is the linear part of a. Here it is the total quantity (gain-losses) which must be compared for each pair of frequencies. We

have chosen the case

|°03B11i(fl y I > 0a1 (a ) x I

to draw the curve b in figure : X

to draw the curve b in figure : being positive, the term O(xl (fly Iocr.) (ill[ ) ac-

celerates the appearance o the phenomenon

which occurs now at a lower frequency. In the same manner curve b’ is obtained from

curve a’ by adding the term

Here we assume that n n x y so that no

mode hopping can appear.

c) The saturation phenomenon first affect the quality factor ax,. Because 8 is not

in general a multiple of 2n it decreases

Qxy on the y axis :

Qx y Qy (we have Q. = ’*d/ (1 - Ra c IR I) at

resonance). Therefore it slows down the de- velopment of a By mode : on figure 3 this

effect corresponds to an additional negati-

ve term to the curve b. This results in

curve c. In the same way it also lowers the b’ curve giving curve c’.

d) Then the saturation phenomenon induces

an anisotropy of the gain. When Ll. = 12 y one

may write :

This is a positive term as the gain is lar-

ger on the y axis due to Zeeman coherences of the atomic sublevels. This last effect therefore accelerates the development of a

E mode. It then rises curve c on figure 3

and results in curve d which crosses the w

axis at point B where the flip occurs. The

same effect applied to the situation where

the Ey mode oscillates and frequency decre-

ases lead to an increased gain on the x axis which accelerates also the advent of the flip (point A on Fig. 3).

It appears that the saturation induced ani- sotropy of the gas is responsible for the polarization bistability domain in our ex-

periment : its real part (induced birefrin- gence) tends to increase the stability of a mode by decreasing the Q factor of the other while its imaginary part (induced di- chroism of amplification) tends on the con- trary to decrease its stability by increa- sing the gain on the other axis. This ani- sotropy depends strongly on the structure of the lasing levels. Now it can be seen that, depending on the respective strength of the opposite effects c and d, the bista-

bility range will be a complicated function of the light intensity. However when the intensity increases the saturated index tends to 1 and the c effect on the quality

factor decreases while the d effect or di- chroism increases. As a results the polari- zation flip will occur sooner and the bis- tability range decreases according to the experimental results shown in figure 2.

REFERENCES

[1] Stephan G. and Hugon D., Phys. Rev.

Lett. 55, (1985) 703

[2] Culshaw W. and Kannelaud J., Phys. Rev.

141, (1966) 237

[3] Stephan G., Le Naour R. and Le Floch A., Phys. Rev. A17, (1978) 733

[4] Hugon D., 3rd cycle thesis, Rennes (1982).

[5] Sargent III M., Scully M.L. and Lamb Jr.

W.E., Laser Physics, (Addison-Wesley, London) 1974, P. 101 eq. 14 and 15.

[6] Lamb’s formulation has the advantage to separate clearly gain and losses. An alternative method consists in writing :

$$ Q-1xy = c/d03C9 {1 - Ra |Ry| cos 03B8xy

$$ exp(-2 kiy d)}

with the gain exp $$ (-2 kiyd) included in

Qxy. This method leads to the same con-

clusions.

[7] Supercripts r and i stand respectively

vely for "real part of" and "imaginary

part of".

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