Photon counting distributions for interacting laser modes

Photon counting distributions for interacting laser modes

V,-~t~rr,,~. ~mb¢~ I OPTICS COMMUNICATIONS September 1973 PHOTON COUNTING DISTRIBUTIONS FOR I N T E R A C T ~ G LASER MODES W. WONNEBERGERand J. LE...

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V,-~t~rr,,~. ~mb¢~ I

OPTICS COMMUNICATIONS

September 1973

PHOTON COUNTING DISTRIBUTIONS FOR I N T E R A C T ~ G LASER MODES W. WONNEBERGERand J. LEMPERT Fakult~t fiir PhysOt der Universit~t, ~'eiburg i. Br.. Germany Received 5 June 1973

T'he pholtm tour ling distributions obtahted from the beta-distribution for the intensity of interacting waves are ~ - , ~ _ , ~ to de~o'ibe tt, e inten~W fluctuations in a single laser mode which is intensity-coupled to other equivalent : ~ , ~ s c,f a rnultimoce laser. Numerical results are given for a twe-mode laser including dead-time corrections for ¢x = ~ . ~ counting-inter,,ai- dead-time ratios.

amplatude fluctu~tiom of a single laser mode setim~led from the output of a multhnode laser differ from tlhoR of a single mode laser (cf. [1 ]) due to interac~ bet~x.en the modes. In ref. 121 it was predicted and experimentally verified ~ a t for a nonresonant feedback laser an in~e~D mte~acti~ between the modes thermalizes ea
than one for a laser far above fllreshold. For N~n ,ON m ~, 1, Q(~,) factorizes into ( 1 +aX) -Nm. Therefore, the N m investigated modes appear thermal and independent in spite of the fact that all modes are statistically dependent. For N m ~ N m , the strong correlations between the modes enter in an analogous manner as described in [21 for N m ~, 1. Eq. (2), therefore, interpolates between these extremes. In the original derivation [3] 9f eq. (2), starting from a specific interaction model, one should have N m ~ 10. However, eq. (2), being associated with the beta-distribution, physically is a good ,oproxhnation for all values o f N m provided i'-.2, m~- ,aable to Fred at some instant of time the mean tot;' output intensity (/max) = Nma already in the N~ moies investigated. This situation is effectively ruled out as long as

((zX/)2>= N

m ( N m -- N m ) a 2

/(Nm +

I)

(l)

~--.|

'~ (/max-/) 2 = ( N ~here : , is the scaled intensity [5] of the lath mode, th* ~nerating funcuon Q(M = ( e x p ( - L 0 > may be eva~aared and is shown in eq. (2):

tF:

(2)

m -

Nm)2a 2

giving (Nm -

+ 1).

(3)

This condition restricts the possible combinations of N m and N m values. The precise form of the interaction

Here. 1F~ ~ the confluent hypergeometric function. The p~lmpmg parameter a [5] is usually much larger

associated with eq. (2) under such nonasymptotic conditions is not known at present. It is expected to be

OPTICS COMMUNICATIONS

Volume 9, number 1

some type of intensity interaction with "cut off" between equivalent modes. We propose to use eq. (2) for the description of the amplitude fluctuations in a sLngle laser mode of (say) a five-mode laser with normal multimode interaction which excludes mode locking. For a combination like ( N m = 1, N m = 5) eq. (2) predicts substantially different results compared to the thermal case as well as to the amplitude stabilized case. These differences are most easily seen in photon counting experiments [6-9]. Therefore, we have computed numerical results for the expected photon counting distribution of a single laser mode coupled to four other iasing modes. For N m = 1, the recurrence relation for the counting probability p(n, T < %) (counting interval T smaller than intensity correlation time ¢c) associated with eq. (2) reads (cf. [3]):

p(n_l)_Nm + n - 1 +Nm(n ) p(n) Nm(, >

n+ 1 Nm(n)P(n+ l). (4)

This equation permits convenient numerical evaluation ofp(n). For a realistic experimental situation, the counting interval T must be rather small, presumably T ~ 10 -7 see. Since the minimum dead time of the photon counter will be about 10 -8 see, dead-time corrections must be included in the evaluation of eq. (4). The theory of dead-time corrections for nonparalyzable counters in the case T < r e has been given by B6dard [ lO]. According to his work, the corrected distribution function p(n, T, r, (n)c) (r dead time, (n)c corrected mean number of counts) for n >_ l is given by

p(n, T, r,
f ., 0

For n = 0, P(/) is the with Q(~) defined in

#

"fin, ~ =/" ,ix x n- t e-X.

,~n-l)_7(n+l,~n) n!

)

(6)

o

The quantity l~n Is def'med in eq. (7): ~n = a T / ( l

(7)

-nr/T) - vnl.

The coefficient a measures the quantum efficien~v of the detector. Note, that

(n)= vO(1)-=-(n)0 and in addition, we def'me

n = vn (I). One would like to expressp(n. T, ¢, (n) c) solely in terms of uncorrected distribution functions p(n, T, 0, (n)) for appropriately chosen mean values (n). This is accompit~ed by the following transformations:

~,(n, ~) = vn f dx x n - l e-~X 0 =p

Uging the generating function Q(~)= (exp(-M)), one obtains

p(n, T, r, (n)c) n-I

- v("n -- Il ) ! (_vn_, a ) Pn

d/P(/) 7_ " , (n-i)!

Sepmmber t973

l -Q(X) x ) [ ~=,,,,_~

rl

(5)

one has of course p(0, T, r) = p(0, T, 0). intensity distribution function associated and 7 is the incomplete gamma-function eq. (6):

The n-fold derivatives are evaluated as follows. With

(-valax),, f(x) - ~ . l one has (!/,~)[nl = vnn! x-Cn~I).

Volume 9, number 1

OPTICS COMMUNICATIONS

September 1973

Table 1 Photon counting distributions p (n) for a single mode of a five-mode laser with intensity mode coupling. The distributions p (n) are derived from the beta-distribution for the mode intensity and corrected for several ratios of short counting interval T to dead time r. (n >is the uneon-~ted number of mean counts. 4 .

.

.

.

.

.

5 .

6 -

7

8

_

_

9 .

.

.

.

.

.

10 .

.

.

.

.

.

.

.

.

0

0.1424

0.1697

0.1894

0.2040

0.2152

0.2242

0.2315

1

0.1957

0.2053

0.2106

0.2137

0.2157

0.2171

0.2180

2

0.2696

0.2391

0.2222

0.2113

0.2037

0.1981

0.1938

3

0.3042

0.2387

0.2053

0.1856

0.1728

0.1637

0.1570

4

0.0881

0.1354

0.1346

0.1271

0.1201

0.1144

0.1099

0.0118

0.0369

0.0514

0.0576

0.0601

0.0609

0.0010

0.0068

0.0140

0.0195

0.0234

0.0001

0.0009

0.0028

0,0051

0.0000

0.0001

0.0004

0.0000

0.0000

5 6 •7 8

9 10

0.0000

(n>

4.996

4.442

3.868

3.288

Using tS~ relation, the following identity is valid: M

(Q(]k)I~k)[nl= m= 0~ pmm, (~)

~k-(m+l' Q(~k)[n-ml.

According to Mandel's formula [ 11 ]:

[n-ml t = (n-m)! p(n-m, T, O, (n )n) ,

Q(~,) l~=pn

(8)

one, therefore, ends up with the relation r/

p(n, 7, r, (n)c) = m~0 p(n-m, T, O, (n)n) n-1

- ~_t p ( n - m - l , T , O , (n>n l)" (9) rrt---'0 With the definition 2~ l = 0, this relation is valid for all 0 ~
3.081

2.931

2.817

positive it must be replaced by zero and the associated uncorrected counting distribution is p(n) = 5n, O" Using eqs. (4) and (9), numerical results were computed for N m = 5, (n)c = 2000, and several values for the ratio T/¢ of counting interval T to dead time r. They are given in table 1. For comparison, the corresponding values for a thermal (or thermalized [6, 12]) mode are given in table 2. The Bose-Einstein counting distribution appropriate for this case was simulated by settingN m = IO s in eq. (4). It is seen, that the counting distribution of a single laser mode intensity.coupled to only four other equivalent modes is similar to the Bose-Einstein distribution in contrast to the case of a single "free" laser mode for which the appropriate counting distri. bution is similar to the Poisson distribution [ l ]. In order to use the X2 statistical test to discriminate experimentally between the two cases in tables 1 and 2, a sufficiently large number of samples is necessary. This number should be of the order 104.

Volume 9, number 1

OPTICS COMMUNICATIONS

September 1973

Table 2 IPhoton counting disUibutions p (n) of a thermal light mode during short counting interval T. The distributions p (n) include dea6 time corrections for several ratios of counting interval T to dead time ~-. (n) is the uncorrected number of mean counts. _

4

.

..

.

.

.

.

.

.

.

.

.

.

5

.

. .

.

.

.

.

.

6 .

.

.

.

.

.

.

.

.

.

.

.

.

.

..

7 .

.

.

~

.

.

.

.

.

.

.

.

.

.

.

.

9 ..

8 ,

10 .

.

.

.

.

.

.

.

.

.

.

.

0

0.1546

0.1841

0.2056

0.2217

0.2343

0~244 3

0.2524

1

0.1978

0.2070

0.2120

0.2149

0.2167

0.2179

0.2188

2

0.2530

0.2244

0.2083

0.1979

0.1906

0.1~52

0.1811

3

0.2821

0.2168

0.1853

0.1671

0.1552

0.1468

0.1406

4

0.1125

0.1446

0.1322

0.1201

0.1113

0.1048

0.0998

0.0231

0.0530

0.0625

0.0640

0.0633

0.0621

0.0036

0.0153

0.0242

0.0290

0.0314

0.0005

0.0037

0.0079

0.0114

0.0000

0.0008

0.0023

0.0000

0.0001

5 6 7 8

9 0 (n )

, .

,

,

_

0.0000 5.504

4.086

3.868

Acknowledgements The authors are indebted to Dr. J. Herrington and Dr. W. Wettling for helpful discussions.

References [ 1] M. Sargent !I1 and M.O. Scully, in: Laser Handbook, F.T. Arecchi and E.O. Schulz-DuBois, eds. (NorthHolland, Amsterdam, 1972), oh. A2, p. 45, H. Haken, ibid., ch. A3, p. 115; F.T. Arecchi and V. Degiorgio, ibid., ch. AS, p. 191. [2] R.V. Ambartsumyan, P.G. K~yukov, V.S. Letokhov, and Yu.A. Matveets, Zh. Eksp. Teor. Fiz. 53 (1967) 1955 (JETP 26 (1968) 1109).

3.512

3.269

3.094

2.962

[3] W. Wonneberger and J. Lempert, Phys. Letters 43A (1973) 75 and Z. Naturforsch. 28a (1973) 762. [4] W. Brunner and H. Paul, Ann. Physik 23 (1969) 152 and 384. tSl H. Risken, Z, Phys. 186 (1965) 85. [61 F.T. Arecchi, Phys. Re,,,. Letters 15 (1965) 912. [7] C. Freed and H.A. Haus, Phys. Rev. Letters 15 (1965) 943. [Sl W.A. Smith and J.A. Armstrong, Phys. Rev. Letters 16 (1966) 1169. 191 F.T. Azecchi and V. Degiorgio in ref. [ 1 ]. [to] G. B~dard, Proc. Phys. Soc. 90 (1967) 131. 111] L. Mandel, Proc. Phys. Soc. 72 (1958) 1037. 112] W. Martienssen and E. Spiller, Am. J. Phys. 32 (1964) 919.