-
2
-
-
27144466781
-
-
and references therein
-
M. Fleischhauer, A. Imamoglu, and J. P. Marangos, Rev. Mod. Phys. 77, 633 (2005), and references therein.
-
(2005)
Rev. Mod. Phys.
, vol.77
, pp. 633
-
-
Fleischhauer, M.1
Imamoglu, A.2
Marangos, J.P.3
-
3
-
-
77951576765
-
-
and references therein
-
K. Hammerer, A. S. Sorensen, and E. S. Polzik, Rev. Mod. Phys. 82, 1041 (2010), and references therein.
-
(2010)
Rev. Mod. Phys.
, vol.82
, pp. 1041
-
-
Hammerer, K.1
Sorensen, A.S.2
Polzik, E.S.3
-
4
-
-
72449212274
-
-
and references therein
-
A. I. Lvovsky, B. C. Sanders, and W. Tittel, Nat. Photon. 3, 706 (2009), and references therein.
-
(2009)
Nat. Photon.
, vol.3
, pp. 706
-
-
Lvovsky, A.I.1
Sanders, B.C.2
Tittel, W.3
-
5
-
-
27144501475
-
-
R. Santra, E. Arimondo, T. Ido, C. H. Greene, and J. Ye, Phys. Rev. Lett. 94, 173002 (2005).
-
(2005)
Phys. Rev. Lett.
, vol.94
, pp. 173002
-
-
Santra, R.1
Arimondo, E.2
Ido, T.3
Greene, C.H.4
Ye, J.5
-
6
-
-
33845371031
-
-
T. Zanon-Willette, A. D. Ludlow, S. Blatt, M. M. Boyd, E. Arimondo, and J. Ye, Phys. Rev. Lett. 97, 233001 (2006).
-
(2006)
Phys. Rev. Lett.
, vol.97
, pp. 233001
-
-
Zanon-Willette, T.1
Ludlow, A.D.2
Blatt, S.3
Boyd, M.M.4
Arimondo, E.5
Ye, J.6
-
7
-
-
18244397453
-
-
T. Hong, C. Cramer, W. Nagourney, and E. N. Fortson, Phys. Rev. Lett. 94, 050801 (2005).
-
(2005)
Phys. Rev. Lett.
, vol.94
, pp. 050801
-
-
Hong, T.1
Cramer, C.2
Nagourney, W.3
Fortson, E.N.4
-
13
-
-
18444400235
-
-
A. Peng, M. Johnsson, W. P. Bowen, P. K. Lam, H.-A. Bachor, and J. J. Hope, Phys. Rev. A 71, 033809 (2005).
-
(2005)
Phys. Rev. A
, vol.71
, pp. 033809
-
-
Peng, A.1
Johnsson, M.2
Bowen, W.P.3
Lam, P.K.4
Bachor, H.-A.5
Hope, J.J.6
-
14
-
-
28844503198
-
-
I. Friedler, D. Petrosyan,M. Fleischhauer, and G. Kurizki, Phys. Rev. A 72, 043803 (2005).
-
(2005)
Phys. Rev. A
, vol.72
, pp. 043803
-
-
Friedler, I.1
Petrosyan, D.2
Fleischhauer, M.3
Kurizki, G.4
-
15
-
-
0037595505
-
-
C. Ottaviani, D. Vitali, M. Artoni, F. Cataliotti, and P. Tombesi, Phys. Rev. Lett. 90, 197902 (2003).
-
(2003)
Phys. Rev. Lett.
, vol.90
, pp. 197902
-
-
Ottaviani, C.1
Vitali, D.2
Artoni, M.3
Cataliotti, F.4
Tombesi, P.5
-
16
-
-
19644401228
-
-
S. Rebić, D. Vitali, C. Ottaviani, P. Tombesi, M. Artoni, F. Cataliotti, and R. Corbalán, Phys. Rev. A 70, 032317 (2004).
-
(2004)
Phys. Rev. A
, vol.70
, pp. 032317
-
-
Rebić, S.1
Vitali, D.2
Ottaviani, C.3
Tombesi, P.4
Artoni, M.5
Cataliotti, F.6
Corbalán, R.7
-
18
-
-
33746656801
-
-
C. Hang, Y. Li, L. Ma, and G. Huang, Phys. Rev. A 74, 012319 (2006).
-
(2006)
Phys. Rev. A
, vol.74
, pp. 012319
-
-
Hang, C.1
Li, Y.2
Ma, L.3
Huang, G.4
-
19
-
-
34547298790
-
-
If the group velocity of a light pulse is reduced by a factor of F from the speed of light in vacuum, the phase-shift operation will be a factor of F slower
-
If the group velocity of a light pulse is reduced by a factor of F from the speed of light in vacuum, the phase-shift operation will be a factor of F slower [L. Deng and M. G. Payne, Phys. Rev. Lett. 98, 253902 (2007).].
-
(2007)
Phys. Rev. Lett.
, vol.98
, pp. 253902
-
-
Deng, L.1
Payne, M.G.2
-
27
-
-
42449097667
-
-
K. J. Jiang, L. Deng, E.W. Hagley, and M. G. Payne, Phys. Rev. A 77, 045804 (2008).
-
(2008)
Phys. Rev. A
, vol.77
, pp. 045804
-
-
Jiang, K.J.1
Deng, L.2
Hagley, E.W.3
Payne, M.G.4
-
31
-
-
78649591514
-
-
note
-
Due to the symmetric configuration of the system, the linear and nonlinear susceptibilities of both the probe and signal fields are almost equal [see Eq. (5)]. Hence, the curves plotted in Fig. 3 are valid for both the probe and signal fields.
-
-
-
-
32
-
-
3843146888
-
-
Q. A. Turchette, C. J. Hood, W. Lange, H. Mabuchi, and H. J. Kimble, Phys. Rev. Lett. 75, 4710 (1995).
-
(1995)
Phys. Rev. Lett.
, vol.75
, pp. 4710
-
-
Turchette, Q.A.1
Hood, C.J.2
Lange, W.3
Mabuchi, H.4
Kimble, H.J.5
-
34
-
-
65649122327
-
-
M. Bajcsy, S. Hofferberth, V. Balic, T. Peyronel, M. Hafezi, A. S. Zibrov, V. Vuletic, and M. D. Lukin, Phys. Rev. Lett. 102, 203902 (2009).
-
(2009)
Phys. Rev. Lett.
, vol.102
, pp. 203902
-
-
Bajcsy, M.1
Hofferberth, S.2
Balic, V.3
Peyronel, T.4
Hafezi, M.5
Zibrov, A.S.6
Vuletic, V.7
Lukin, M.D.8
-
35
-
-
42449097667
-
-
The lead time is typically about 10% of c. Thus the device transient time can be estimated quite accurately by using the free-space speed of light
-
The lead time is typically about 10% of c. Thus the device transient time can be estimated quite accurately by using the free-space speed of light [K. J. Jiang, L. Deng, E.W. Hagley, and M. G. Payne, Phys. Rev. A 77, 045804 (2008).].
-
(2008)
Phys. Rev. A
, vol.77
, pp. 045804
-
-
Jiang, K.J.1
Deng, L.2
Hagley, E.W.3
Payne, M.G.4
-
36
-
-
77955681438
-
-
K.-P. Marzlin, Z.-B. Wang, S. A. Moiseev, and B. C. Sanders, J. Opt. Soc. B 27, A36 (2010).
-
(2010)
J. Opt. Soc. B
, vol.27
-
-
Marzlin, K.-P.1
Wang, Z.-B.2
Moiseev, S.A.3
Sanders, B.C.4
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