-
1
-
-
0033248448
-
-
RMPHAT 0034-6861 10.1103/RevModPhys.71.1
-
A.-C. J. Weiner, V. S. Bagnato, S. Zilio, and P. S. Julienne, Rev. Mod. Phys. RMPHAT 0034-6861 10.1103/RevModPhys.71.1 71, 1 (1999).
-
(1999)
Rev. Mod. Phys.
, vol.71
, pp. 1
-
-
Weiner, A.-C.J.1
Bagnato, V.S.2
Zilio, S.3
Julienne, P.S.4
-
2
-
-
33144478901
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.73.011402
-
M. Taglieber, A.-C. Voigt, F. Henkel, S. Fray, T. W. Hänsch, and K. Dieckmann, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.73.011402 73, 011402 (2006).
-
(2006)
Phys. Rev. A
, vol.73
, pp. 011402
-
-
Taglieber, M.1
Voigt, A.-C.2
Henkel, F.3
Fray, S.4
Hänsch, T.W.5
Dieckmann, K.6
-
3
-
-
77951713045
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.81.043637
-
F. M. Spiegelhalder, A. Trenkwalder, D. Naik, G. Kerner, E. Wille, G. Hendl, F. Schreck, and R. Grimm, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.81.043637 81, 043637 (2010).
-
(2010)
Phys. Rev. A
, vol.81
, pp. 043637
-
-
Spiegelhalder, F.M.1
Trenkwalder, A.2
Naik, D.3
Kerner, G.4
Wille, E.5
Hendl, G.6
Schreck, F.7
Grimm, R.8
-
4
-
-
2542434477
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.92.153001
-
A. J. Kerman, J. M. Sage, S. Sainis, Thomas Bergeman, and David DeMille, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.92.153001 92, 153001 (2004).
-
(2004)
Phys. Rev. Lett.
, vol.92
, pp. 153001
-
-
Kerman, A.J.1
Sage, J.M.2
Sainis, S.3
Bergeman, T.4
Demille, D.5
-
5
-
-
33749185074
-
-
JPAPEH 0953-4075 10.1088/0953-4075/39/19/S13
-
S. D. Kraft, P. Staanum, J. Lange, L. Vogel, R. Wester, and M. Weidemüller, J. Phys. B JPAPEH 0953-4075 10.1088/0953-4075/39/19/S13 39, S993 (2006).
-
(2006)
J. Phys. B
, vol.39
, pp. 993
-
-
Kraft, S.D.1
Staanum, P.2
Lange, J.3
Vogel, L.4
Wester, R.5
Weidemüller, M.6
-
6
-
-
59249093791
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.102.020405
-
A.-C. Voigt, M. Taglieber, L. Costa, T. Aoki, W. Wieser, T. W. Hänsch, and K. Dieckmann, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.102.020405 102, 020405 (2009).
-
(2009)
Phys. Rev. Lett.
, vol.102
, pp. 020405
-
-
Voigt, A.-C.1
Taglieber, M.2
Costa, L.3
Aoki, T.4
Wieser, W.5
Hänsch, T.W.6
Dieckmann, K.7
-
7
-
-
4243517992
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.62.030702
-
S. D. Gensemer, P. L. Gould, P. J. Leo, E. Tiesinga, and C. J. Williams, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.62.030702 62, 030702 (2000).
-
(2000)
Phys. Rev. A
, vol.62
, pp. 030702
-
-
Gensemer, S.D.1
Gould, P.L.2
Leo, P.J.3
Tiesinga, E.4
Williams, C.J.5
-
8
-
-
0001306220
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.63.957
-
A. Gallagher and D. E. Pritchard, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.63.957 63, 957 (1989).
-
(1989)
Phys. Rev. Lett.
, vol.63
, pp. 957
-
-
Gallagher, A.1
Pritchard, D.E.2
-
9
-
-
0000485245
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.63.961
-
D. Sesko, T. Walker, C. Monroe, A. Gallagher, and C. Wieman, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.63.961 63, 961 (1989).
-
(1989)
Phys. Rev. Lett.
, vol.63
, pp. 961
-
-
Sesko, D.1
Walker, T.2
Monroe, C.3
Gallagher, A.4
Wieman, C.5
-
10
-
-
3142772739
-
-
EPJDF6 1434-6060 10.1140/epjd/e2004-00066-6
-
M. W. Mancini, A. R.-L. Caires, G. D. Telles, V. S. Bagnato, and L. G. Marcassa, Eur. Phys. J. D EPJDF6 1434-6060 10.1140/epjd/e2004-00066-6 30, 105 (2004).
-
(2004)
Eur. Phys. J. D
, vol.30
, pp. 105
-
-
Mancini, M.W.1
Caires, A.R.-L.2
Telles, G.D.3
Bagnato, V.S.4
Marcassa, L.G.5
-
11
-
-
78650962762
-
-
It has been pointed out that the heteronuclear loss rates are not reciprocal, i.e., one cannot a priori assume βi,j′=βj,i′.
-
It has been pointed out that the heteronuclear loss rates are not reciprocal, i.e., one cannot a priori assume β i, j ′ = β j, i ′.
-
-
-
-
12
-
-
0035280178
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.63.033406
-
G. D. Telles, W. Garcia, L. G. Marcassa, V. S. Bagnato, D. Ciampini, M. Fazzi, J. H. Müller, D. Wilkowski, and E. Arimondo, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.63.033406 63, 033406 (2001).
-
(2001)
Phys. Rev. A
, vol.63
, pp. 033406
-
-
Telles, G.D.1
Garcia, W.2
Marcassa, L.G.3
Bagnato, V.S.4
Ciampini, D.5
Fazzi, M.6
Müller, J.H.7
Wilkowski, D.8
Arimondo, E.9
-
13
-
-
4043122641
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.69.063408
-
M. E. Holmes, M. Tscherneck, P. A. Quinto-Su, and N. P. Bigelow, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.69.063408 69, 063408 (2004).
-
(2004)
Phys. Rev. A
, vol.69
, pp. 063408
-
-
Holmes, M.E.1
Tscherneck, M.2
Quinto-Su, P.A.3
Bigelow, N.P.4
-
14
-
-
0001465908
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.65.1571
-
C. Monroe, W. Swann, H. Robinson, and C. Wieman, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.65.1571 65, 1571 (1990).
-
(1990)
Phys. Rev. Lett.
, vol.65
, pp. 1571
-
-
Monroe, C.1
Swann, W.2
Robinson, H.3
Wieman, C.4
-
15
-
-
0030552763
-
-
EULEEJ 0295-5075 10.1209/epl/i1996-00512-5
-
D. Haubrich, H. Schadwinkel, F. Strauch, B. Ueberholz, R. Wynands, and D. Meschede, Europhys. Lett. EULEEJ 0295-5075 10.1209/epl/i1996-00512-5 34, 663 (1996).
-
(1996)
Europhys. Lett.
, vol.34
, pp. 663
-
-
Haubrich, D.1
Schadwinkel, H.2
Strauch, F.3
Ueberholz, B.4
Wynands, R.5
Meschede, D.6
-
16
-
-
0030544575
-
-
EULEEJ 0295-5075 10.1209/epl/i1996-00510-7
-
F. Ruschewitz, D. Bettermann, J. L. Peng, and W. Ertmer, Europhys. Lett. EULEEJ 0295-5075 10.1209/epl/i1996-00510-7 34, 651 (1996).
-
(1996)
Europhys. Lett.
, vol.34
, pp. 651
-
-
Ruschewitz, F.1
Bettermann, D.2
Peng, J.L.3
Ertmer, W.4
-
17
-
-
78650933950
-
-
The Geiger mode can be used only for photon rates which are smaller than the inverse dead time of 1/35 ns of the APD. Considering the corresponding detection setups the count rates of Rb and Cs are 108/s and 105/s, respectively, thus only allowing to operate the Cs APD in the Geiger mode.
-
The Geiger mode can be used only for photon rates which are smaller than the inverse dead time of 1/35 ns of the APD. Considering the corresponding detection setups the count rates of Rb and Cs are 10 8 /s and 10 5 /s, respectively, thus only allowing to operate the Cs APD in the Geiger mode.
-
-
-
-
18
-
-
78650960240
-
-
For Rb atom numbers less than 700 the statistics is much less, and we average over about 50 traces only. However, this does not influence the analysis of the Rb-Cs interaction parameter, because this is based only on data sets with Rb atom numbers larger than or equal to 1000.
-
For Rb atom numbers less than 700 the statistics is much less, and we average over about 50 traces only. However, this does not influence the analysis of the Rb-Cs interaction parameter, because this is based only on data sets with Rb atom numbers larger than or equal to 1000.
-
-
-
-
19
-
-
78650929574
-
-
While in steady state the histograms are expected to follow a Poissonian distribution, we find that also for non-steady-state conditions our data are very well described by a Poissonian. For simplicity we therefore fit a Poissonian distribution to the data and extract its mean atom number which is shifted toward smaller values for an increasing number of Rb atoms.
-
While in steady state the histograms are expected to follow a Poissonian distribution, we find that also for non-steady-state conditions our data are very well described by a Poissonian. For simplicity we therefore fit a Poissonian distribution to the data and extract its mean atom number which is shifted toward smaller values for an increasing number of Rb atoms.
-
-
-
-
21
-
-
42549143701
-
-
JPAPEH 0953-4075 10.1088/0953-4075/41/3/035303
-
M. L. Harris, P. Tierney, and S. L. Cornish, J. Phys. B JPAPEH 0953-4075 10.1088/0953-4075/41/3/035303 41, 035303 (2008).
-
(2008)
J. Phys. B
, vol.41
, pp. 035303
-
-
Harris, M.L.1
Tierney, P.2
Cornish, S.L.3
-
22
-
-
49249091667
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.78.023610
-
H. T. Ng and S. Bose, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.78. 023610 78, 023610 (2008).
-
(2008)
Phys. Rev. A
, vol.78
, pp. 023610
-
-
Ng, H.T.1
Bose, S.2
-
23
-
-
33744819428
-
-
NJOPFM 1367-2630 10.1088/1367-2630/8/6/087
-
M. Bruderer and D. Jaksch, New J. Phys. NJOPFM 1367-2630 10.1088/1367-2630/8/6/087 8, 87 (2006).
-
(2006)
New J. Phys.
, vol.8
, pp. 87
-
-
Bruderer, M.1
Jaksch, D.2
-
24
-
-
26944465290
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.71.061401
-
M. Anderlini, E. Courtade, M. Cristiani, D. Cossart, D. Ciampini, C. Sias, O. Morsch, and E. Arimondo, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.71.061401 71, 061401 (2005).
-
(2005)
Phys. Rev. A
, vol.71
, pp. 061401
-
-
Anderlini, M.1
Courtade, E.2
Cristiani, M.3
Cossart, D.4
Ciampini, D.5
Sias, C.6
Morsch, O.7
Arimondo, E.8
-
25
-
-
35649008956
-
-
NJOPFM 1367-2630 10.1088/1367-2630/9/5/147
-
M. Haas, V. Leung, D. Frese, D. Haubrich, S. John, C. Weber, A. Rauschenbeutel, and D. Meschede, New J. Phys. NJOPFM 1367-2630 10.1088/1367-2630/9/5/147 9, 147 (2007).
-
(2007)
New J. Phys.
, vol.9
, pp. 147
-
-
Haas, M.1
Leung, V.2
Frese, D.3
Haubrich, D.4
John, S.5
Weber, C.6
Rauschenbeutel, A.7
Meschede, D.8
-
26
-
-
66049099794
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.79.042718
-
K. Pilch, A. D. Lange, A. Prantner, G. Kerner, F. Ferlaino, H.-C. Nägerl, and R. Grimm, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.79. 042718 79, 042718 (2009).
-
(2009)
Phys. Rev. A
, vol.79
, pp. 042718
-
-
Pilch, K.1
Lange, A.D.2
Prantner, A.3
Kerner, G.4
Ferlaino, F.5
Nägerl, H.-C.6
Grimm, R.7
|