-
2
-
-
0001578550
-
-
Ser. A
-
M. V. Berry and M. Tabor, Proc. R. Soc. London, Ser. A 356, 375 (1977); S. W. McDonald and A. N. Kaufman, Phys. Rev. Lett. 42, 1189 (1979); E. Haller, H. Köppel, and L. S. Cederbaum, ibid. 52, 1665 (1984).
-
(1977)
Proc. R. Soc. London
, vol.356
, pp. 375
-
-
Berry, M.V.1
Tabor, M.2
-
3
-
-
29444438626
-
-
M. V. Berry and M. Tabor, Proc. R. Soc. London, Ser. A 356, 375 (1977); S. W. McDonald and A. N. Kaufman, Phys. Rev. Lett. 42, 1189 (1979); E. Haller, H. Köppel, and L. S. Cederbaum, ibid. 52, 1665 (1984).
-
(1979)
Phys. Rev. Lett.
, vol.42
, pp. 1189
-
-
McDonald, S.W.1
Kaufman, A.N.2
-
4
-
-
3743106429
-
-
M. V. Berry and M. Tabor, Proc. R. Soc. London, Ser. A 356, 375 (1977); S. W. McDonald and A. N. Kaufman, Phys. Rev. Lett. 42, 1189 (1979); E. Haller, H. Köppel, and L. S. Cederbaum, ibid. 52, 1665 (1984).
-
(1984)
Phys. Rev. Lett.
, vol.52
, pp. 1665
-
-
Haller, E.1
Köppel, H.2
Cederbaum, L.S.3
-
5
-
-
0002495103
-
-
Indeed, one can show that given a system with energy level repulsion, a chaotic classical spectrum emerges in the correspondence limit if one utilizes the semiclassical theory for hyperbolic systems. See, J. Wilkie and P. Brumer, Phys. Rev. A 55, 27, 43 (1997).
-
(1997)
Phys. Rev. A
, vol.55
, pp. 27
-
-
Wilkie, J.1
Brumer, P.2
-
7
-
-
0001253559
-
-
R. L. Sundberg, E. Abramson, J. L. Kinsey, and R. W. Field, J. Chem. Phys. 83, 466 (1985); Y. Chen, S. Halle, D. M. Jonas, J. L. Kinsey, and R. W. Field, J. Opt. Soc. Am. B 7, 1805 (1990).
-
(1985)
J. Chem. Phys.
, vol.83
, pp. 466
-
-
Sundberg, R.L.1
Abramson, E.2
Kinsey, J.L.3
Field, R.W.4
-
8
-
-
84975661824
-
-
R. L. Sundberg, E. Abramson, J. L. Kinsey, and R. W. Field, J. Chem. Phys. 83, 466 (1985); Y. Chen, S. Halle, D. M. Jonas, J. L. Kinsey, and R. W. Field, J. Opt. Soc. Am. B 7, 1805 (1990).
-
(1990)
J. Opt. Soc. Am. B
, vol.7
, pp. 1805
-
-
Chen, Y.1
Halle, S.2
Jonas, D.M.3
Kinsey, J.L.4
Field, R.W.5
-
10
-
-
0000216706
-
-
G. Sitja and J. P. Pique, Phys. Rev. Lett. 73, 232 (1994). Long range correlations in this reference are obtained by time smoothing a stick spectrum. This method is totally unreliable and often misleading, see Ref. 8.
-
(1994)
Phys. Rev. Lett.
, vol.73
, pp. 232
-
-
Sitja, G.1
Pique, J.P.2
-
13
-
-
3743133363
-
-
L. Leviandier, M. Lombardi, R. Jost, and J. P. Pique, Phys. Rev. Lett. 56, 2449 (1986); J. P. Pique, Y. Chen, R. W. Field, and J. L. Kinsey, ibid. 58, 475 (1987). See, however, Ref. 8, where we make clear the limitations of the procedure adopted in the latter paper.
-
(1986)
Phys. Rev. Lett.
, vol.56
, pp. 2449
-
-
Leviandier, L.1
Lombardi, M.2
Jost, R.3
Pique, J.P.4
-
14
-
-
3743137684
-
-
L. Leviandier, M. Lombardi, R. Jost, and J. P. Pique, Phys. Rev. Lett. 56, 2449 (1986); J. P. Pique, Y. Chen, R. W. Field, and J. L. Kinsey, ibid. 58, 475 (1987). See, however, Ref. 8, where we make clear the limitations of the procedure adopted in the latter paper.
-
(1987)
Phys. Rev. Lett.
, vol.58
, pp. 475
-
-
Pique, J.P.1
Chen, Y.2
Field, R.W.3
Kinsey, J.L.4
-
15
-
-
0347281051
-
-
H. Bitto, S. Derler, and J. R. Huber, Chem. Phys. Lett. 162, 291 (1989); S. Derler, H. Bitto, and J. R. Huber, Chem. Phys. 169, 275 (1993).
-
(1989)
Chem. Phys. Lett.
, vol.162
, pp. 291
-
-
Bitto, H.1
Derler, S.2
Huber, J.R.3
-
16
-
-
21144482944
-
-
H. Bitto, S. Derler, and J. R. Huber, Chem. Phys. Lett. 162, 291 (1989); S. Derler, H. Bitto, and J. R. Huber, Chem. Phys. 169, 275 (1993).
-
(1993)
Chem. Phys.
, vol.169
, pp. 275
-
-
Derler, S.1
Bitto, H.2
Huber, J.R.3
-
20
-
-
85033169386
-
-
M.Sc. thesis, University of Toronto
-
J. Wilkie, M.Sc. thesis, University of Toronto, 1990.
-
(1990)
-
-
Wilkie, J.1
-
22
-
-
85033166874
-
-
note
-
Insufficient averaging makes us concerned about the correlation holes observed in Ref. 11. Only three of fifteen sets of spectra; with ∼5 spectra in each set, displayed evidence of correlation holes. Our experience (Ref. 14) suggests that such features might well arise from insufficient averaging.
-
-
-
-
24
-
-
3743078676
-
-
reprinted in Ref. 17
-
C. E. Porter, Nucl. Phys. 40, 167 (1963) (reprinted in Ref. 17).
-
(1963)
Nucl. Phys.
, vol.40
, pp. 167
-
-
Porter, C.E.1
-
25
-
-
11744315517
-
-
These billiard systems consist of a particle confined to either a circle or stadium shaped region by infinite walls. They are effective examples of regular and chaotic behavior. See, e.g., R. D. Taylor and P. Brumer, Discuss. Faraday Soc. 75, 117 (1983).
-
(1983)
Discuss. Faraday Soc.
, vol.75
, pp. 117
-
-
Taylor, R.D.1
Brumer, P.2
-
28
-
-
3743127771
-
-
X.-P. Jiang and P. Brumer, J. Chem. Phys. 94, 5833 (1991); Chem. Phys. Lett. 180, 222 (1991).
-
(1991)
Chem. Phys. Lett.
, vol.180
, pp. 222
-
-
-
29
-
-
85033166304
-
-
ψ(a,b;z) is difficult to compute for the z values in Eq. (58). We found it easier to numerically perform the integral in Eq. (50)
-
ψ(a,b;z) is difficult to compute for the z values in Eq. (58). We found it easier to numerically perform the integral in Eq. (50).
-
-
-
-
31
-
-
85033188102
-
-
N(t) corresponds to using a square envelope for the electric field of the laser
-
N(t) corresponds to using a square envelope for the electric field of the laser.
-
-
-
-
32
-
-
0003158074
-
-
R. D. Levine, Adv. Chem. Phys. 70, 53 (1987); Th. Zimmermann, H. Köppel, and L. S. Cederbaum, J. Chem. Phys. 91, 3934 (1989).
-
(1987)
Adv. Chem. Phys.
, vol.70
, pp. 53
-
-
Levine, R.D.1
-
33
-
-
36549097271
-
-
R. D. Levine, Adv. Chem. Phys. 70, 53 (1987); Th. Zimmermann, H. Köppel, and L. S. Cederbaum, J. Chem. Phys. 91, 3934 (1989).
-
(1989)
J. Chem. Phys.
, vol.91
, pp. 3934
-
-
Zimmermann, Th.1
Köppel, H.2
Cederbaum, L.S.3
-
34
-
-
85033181836
-
-
note
-
2(t) must be evaluated for the new distribution. The rest of the equations in this paper can easily be modified to include the new damping factors, and the analysis of the fluorescence signal can then be carried out as described.
-
-
-
-
36
-
-
85033176258
-
-
In the event that a poor fit is obtained, other distributions of the radiative linewidths must be considered (Refs. 25,26)
-
In the event that a poor fit is obtained, other distributions of the radiative linewidths must be considered (Refs. 25,26).
-
-
-
-
37
-
-
85033162436
-
-
Software and references available from William Goffe at (http:// emlab.berkeley.edu/Software/abstracts/goffe895.html).
-
-
-
Goffe, W.1
|