-
1
-
-
0346688981
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.91.223001
-
M. Takamoto and H. Katori, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.91.223001 91, 223001 (2003).
-
(2003)
Phys. Rev. Lett.
, vol.91
, pp. 223001
-
-
Takamoto, M.1
Katori, H.2
-
2
-
-
33845328481
-
-
SCIEAS 0036-8075 10.1126/science.1133732
-
M. M. Boyd, T. Zelevinsky, A. D. Ludlow, S. M. Foreman, S. Blatt, T. Ido, and J. Ye, Science SCIEAS 0036-8075 10.1126/science.1133732 314, 1430 (2006).
-
(2006)
Science
, vol.314
, pp. 1430
-
-
Boyd, M.M.1
Zelevinsky, T.2
Ludlow, A.D.3
Foreman, S.M.4
Blatt, S.5
Ido, T.6
Ye, J.7
-
4
-
-
27144545346
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.95.083003
-
C. W. Hoyt, Z. W. Barber, C. W. Oates, T. M. Fortier, S. A. Diddams, and L. Hollberg, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.95.083003 95, 083003 (2005).
-
(2005)
Phys. Rev. Lett.
, vol.95
, pp. 083003
-
-
Hoyt, C.W.1
Barber, Z.W.2
Oates, C.W.3
Fortier, T.M.4
Diddams, S.A.5
Hollberg, L.6
-
5
-
-
4444360622
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.91.040404
-
Y. Takasu, K. Maki, K. Komori, T. Takano, K. Honda, M. Kumakura, T. Yabuzaki, and Y. Takahashi, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.91.040404 91, 040404 (2003).
-
(2003)
Phys. Rev. Lett.
, vol.91
, pp. 040404
-
-
Takasu, Y.1
Maki, K.2
Komori, K.3
Takano, T.4
Honda, K.5
Kumakura, M.6
Yabuzaki, T.7
Takahashi, Y.8
-
6
-
-
33846397097
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.98.030401
-
T. Fukuhara, Y. Takasu, M. Kumakura, and Y. Takahashi, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.98.030401 98, 030401 (2007).
-
(2007)
Phys. Rev. Lett.
, vol.98
, pp. 030401
-
-
Fukuhara, T.1
Takasu, Y.2
Kumakura, M.3
Takahashi, Y.4
-
7
-
-
33847349776
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.98.093001
-
J. R. Guest, N. D. Scielzo, I. Ahmad, K. Bailey, J. P. Greene, R. J. Holt, Z. T. Lu, T. P. O'Connor, and D. H. Potterveld, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.98.093001 98, 093001 (2007).
-
(2007)
Phys. Rev. Lett.
, vol.98
, pp. 093001
-
-
Guest, J.R.1
Scielzo, N.D.2
Ahmad, I.3
Bailey, K.4
Greene, J.P.5
Holt, R.J.6
Lu, Z.T.7
O'Connor, T.P.8
Potterveld, D.H.9
-
8
-
-
18144375980
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.94.160401
-
A. Griesmaier, J. Werner, S. Hensler, J. Stuhler, and T. Pfau, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.94.160401 94, 160401 (2005).
-
(2005)
Phys. Rev. Lett.
, vol.94
, pp. 160401
-
-
Griesmaier, A.1
Werner, J.2
Hensler, S.3
Stuhler, J.4
Pfau, T.5
-
9
-
-
33645808696
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.96.143005
-
J. J. McClelland and J. L. Hanssen, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.96.143005 96, 143005 (2006).
-
(2006)
Phys. Rev. Lett.
, vol.96
, pp. 143005
-
-
McClelland, J.J.1
Hanssen, J.L.2
-
10
-
-
0003544506
-
-
NSRDS-NBS, Washington: National Bureau of Standards, U.S. Department of Commerce
-
W. C. Martin, R. Zalubas, and L. Hagan, Atomic Energy Levels-The Rare-Earth Elements (NSRDS-NBS, Washington: National Bureau of Standards, U.S. Department of Commerce, 1978).
-
(1978)
Atomic Energy Levels-The Rare-Earth Elements
-
-
Martin, W.C.1
Zalubas, R.2
Hagan, L.3
-
11
-
-
85010174907
-
-
OPEXFF 1094-4087
-
H. Y. Ban, M. Jacka, J. L. Hanssen, J. Reader, and J. J. McClelland, Opt. Express OPEXFF 1094-4087 13, 3185 (2005).
-
(2005)
Opt. Express
, vol.13
, pp. 3185
-
-
Ban, H.Y.1
Jacka, M.2
Hanssen, J.L.3
Reader, J.4
McClelland, J.J.5
-
12
-
-
33745228426
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.73.064502
-
J. J. McClelland, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.73. 064502 73, 064502 (2006).
-
(2006)
Phys. Rev. A
, vol.73
, pp. 064502
-
-
McClelland, J.J.1
-
13
-
-
4644363219
-
-
NATUAS 0028-0836 10.1038/nature02938
-
C. I. Hancox, S. C. Doret, M. T. Hummon, L. Luo, and J. M. Doyle, Nature (London) NATUAS 0028-0836 10.1038/nature02938 431, 281 (2004).
-
(2004)
Nature (London)
, vol.431
, pp. 281
-
-
Hancox, C.I.1
Doret, S.C.2
Hummon, M.T.3
Luo, L.4
Doyle, J.M.5
-
14
-
-
33845728533
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.74.063416
-
J. L. Hanssen, J. J. McClelland, E. A. Dakin, and M. Jacka, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.74.063416 74, 063416 (2006).
-
(2006)
Phys. Rev. A
, vol.74
, pp. 063416
-
-
Hanssen, J.L.1
McClelland, J.J.2
Dakin, E.A.3
Jacka, M.4
-
15
-
-
33846349112
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.75.012304
-
J. H. Wesenberg, K. Molmer, L. Rippe, and S. Kroll, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.75.012304 75, 012304 (2007).
-
(2007)
Phys. Rev. A
, vol.75
, pp. 012304
-
-
Wesenberg, J.H.1
Molmer, K.2
Rippe, L.3
Kroll, S.4
-
16
-
-
4043179280
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.67.3483
-
T. E. Barrett, S. W. Dapore-Schwartz, M. D. Ray, and G. P. Lafyatis, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.67.3483 67, 3483 (1991).
-
(1991)
Phys. Rev. Lett.
, vol.67
, pp. 3483
-
-
Barrett, T.E.1
Dapore-Schwartz, S.W.2
Ray, M.D.3
Lafyatis, G.P.4
-
18
-
-
0028513874
-
-
APDOEM 0946-2171 10.1007/BF01081396
-
M. Drewsen, Ph. Laurent, A. Nadir, G. Santarelli, A. Clairon, Y. Castin, D. Grison, and C. Salomon, Appl. Phys. B APDOEM 0946-2171 10.1007/BF01081396 59, 283 (1994).
-
(1994)
Appl. Phys. B
, vol.59
, pp. 283
-
-
Drewsen, M.1
Laurent, Ph.2
Nadir, A.3
Santarelli, G.4
Clairon, A.5
Castin, Y.6
Grison, D.7
Salomon, C.8
-
19
-
-
0037595581
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.90.193002
-
X. Xu, T. H. Loftus, J. W. Dunn, C. H. Greene, J. L. Hall, A. Gallagher, and J. Ye, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.90.193002 90, 193002 (2003).
-
(2003)
Phys. Rev. Lett.
, vol.90
, pp. 193002
-
-
Xu, X.1
Loftus, T.H.2
Dunn, J.W.3
Greene, C.H.4
Hall, J.L.5
Gallagher, A.6
Ye, J.7
-
20
-
-
21144483170
-
-
JOBPDE 0740-3224
-
M. Walhout, J. Dalibard, S. L. Rolston, and W. D. Phillips, J. Opt. Soc. Am. B JOBPDE 0740-3224 9, 1997 (1992).
-
(1992)
J. Opt. Soc. Am. B
, vol.9
, pp. 1997
-
-
Walhout, M.1
Dalibard, J.2
Rolston, S.L.3
Phillips, W.D.4
-
21
-
-
0026979062
-
-
OPCOB8 0030-4018 10.1016/0030-4018(92)90599-M
-
J. Werner, H. Wallis, and W. Ertmer, Opt. Commun. OPCOB8 0030-4018 10.1016/0030-4018(92)90599-M 94, 525 (1992).
-
(1992)
Opt. Commun.
, vol.94
, pp. 525
-
-
Werner, J.1
Wallis, H.2
Ertmer, W.3
-
22
-
-
0000674001
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.54.2275
-
M. Walhout, U. Sterr, and S. L. Rolston, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.54.2275 54, 2275 (1996).
-
(1996)
Phys. Rev. A
, vol.54
, pp. 2275
-
-
Walhout, M.1
Sterr, U.2
Rolston, S.L.3
-
23
-
-
45849155040
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.64.031405
-
J. Stuhler, P. O. Schmidt, S. Hensler, J. Werner, J. Mlynek, and T. Pfau, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.64.031405 64, 031405 (R) (2001).
-
(2001)
Phys. Rev. A
, vol.64
, pp. 031405
-
-
Stuhler, J.1
Schmidt, P.O.2
Hensler, S.3
Werner, J.4
Mlynek, J.5
Pfau, T.6
-
24
-
-
0037965883
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.67.021401
-
D. P. Hansen, J. R. Mohr, and A. Hemmerich, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.67.021401 67, 021401 (R) (2003).
-
(2003)
Phys. Rev. A
, vol.67
, pp. 021401
-
-
Hansen, D.P.1
Mohr, J.R.2
Hemmerich, A.3
-
25
-
-
0037244671
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.67.011401
-
S. B. Nagel, C. E. Simien, S. Laha, P. Gupta, V. S. Ashoka, and T. C. Killian, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.67.011401 67, 011401 (R) (2003).
-
(2003)
Phys. Rev. A
, vol.67
, pp. 011401
-
-
Nagel, S.B.1
Simien, C.E.2
Laha, S.3
Gupta, P.4
Ashoka, V.S.5
Killian, T.C.6
-
26
-
-
36549026236
-
-
Unless otherwise noted, all uncertainties represent one standard deviation combined random and systematic uncertainty.
-
Unless otherwise noted, all uncertainties represent one standard deviation combined random and systematic uncertainty.
-
-
-
-
27
-
-
36549034660
-
-
In our image analysis, we do not account for Zeeman shifts over the spatial extent of the cloud, which are expected to alter the excited state fraction by at most 7%.
-
In our image analysis, we do not account for Zeeman shifts over the spatial extent of the cloud, which are expected to alter the excited state fraction by at most 7%.
-
-
-
-
28
-
-
36549022903
-
-
We find good fits to the magnetic trap relaxation data of Fig. 6 for a simple model in which a fraction f of initially dark (metastable) atoms relaxes to the ground state exponentially while atoms are simultaneously lost from the trap at a second exponential rate. However, this larger number of fit parameters cannot give an independent indication of both the initial dark state fraction and the metastable relaxation rate so we have only included a fit to the long-time relaxation behavior here.
-
We find good fits to the magnetic trap relaxation data of Fig. 6 for a simple model in which a fraction f of initially dark (metastable) atoms relaxes to the ground state exponentially while atoms are simultaneously lost from the trap at a second exponential rate. However, this larger number of fit parameters cannot give an independent indication of both the initial dark state fraction and the metastable relaxation rate so we have only included a fit to the long-time relaxation behavior here.
-
-
-
|