-
1
-
-
4043165940
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.81.742
-
Tin-Lun Ho, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.81.742 81, 742 (1998).
-
(1998)
Phys. Rev. Lett.
, vol.81
, pp. 742
-
-
Ho, T.1
-
2
-
-
4043170275
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.80.2027
-
D. M. Stamper-Kurn, M. R. Andrews, A. P. Chikkatur, S. Inouye, H.-J. Miesner, J. Stenger, and W. Ketterle, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.80.2027 80, 2027 (1998).
-
(1998)
Phys. Rev. Lett.
, vol.80
, pp. 2027
-
-
Stamper-Kurn, D.M.1
Andrews, M.R.2
Chikkatur, A.P.3
Inouye, S.4
Miesner, H.-J.5
Stenger, J.6
Ketterle, W.7
-
3
-
-
0032569802
-
-
NATUAS 0028-0836 10.1038/24567
-
J. Stenger, S. Inouye, D. M. Stamper-Kurn, H.-J. Miesner, A. P. Chikkatur, and W. Ketterle, Nature (London) NATUAS 0028-0836 10.1038/24567 396, 345 (1998).
-
(1998)
Nature (London)
, vol.396
, pp. 345
-
-
Stenger, J.1
Inouye, S.2
Stamper-Kurn, D.M.3
Miesner, H.-J.4
Chikkatur, A.P.5
Ketterle, W.6
-
4
-
-
0037424183
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.90.090401
-
A. Görlitz, T. L. Gustavson, A. E. Leanhardt, R. Löw, A. P. Chikkatur, S. Gupta, S. Inouye, D. E. Pritchard, and W. Ketterle, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.90.090401 90, 090401 (2003).
-
(2003)
Phys. Rev. Lett.
, vol.90
, pp. 090401
-
-
Görlitz, A.1
Gustavson, T.L.2
Leanhardt, A.E.3
Löw, R.4
Chikkatur, A.P.5
Gupta, S.6
Inouye, S.7
Pritchard, D.E.8
Ketterle, W.9
-
5
-
-
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
-
6
-
-
0035804232
-
-
NATUAS 0028-0836 10.1038/35051038
-
A. Sorensen, L.-M. Duan, J. I. Cirac, and P. Zoller, Nature (London) NATUAS 0028-0836 10.1038/35051038 409, 63 (2001).
-
(2001)
Nature (London)
, vol.409
, pp. 63
-
-
Sorensen, A.1
Duan, L.-M.2
Cirac, J.I.3
Zoller, P.4
-
7
-
-
0036508702
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.65.033619
-
L.-M. Duan, J. I. Cirac, and P. Zoller, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.65.033619 65, 033619 (2002).
-
(2002)
Phys. Rev. A
, vol.65
, pp. 033619
-
-
Duan, L.-M.1
Cirac, J.I.2
Zoller, P.3
-
8
-
-
34247493853
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.50.67
-
D. J. Wineland, J. J. Bollinger, W. M. Itano, and D. J. Heinzen, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.50.67 50, 67 (1994).
-
(1994)
Phys. Rev. A
, vol.50
, pp. 67
-
-
Wineland, D.J.1
Bollinger, J.J.2
Itano, W.M.3
Heinzen, D.J.4
-
9
-
-
11144240517
-
-
APBOEM 0946-2171 10.1007/s00340-004-1664-6
-
H. Schmaljohann, M. Erhard, J. Kronjager, K. Sengstock, and K. Bongs, Appl. Phys. B: Lasers Opt. APBOEM 0946-2171 10.1007/s00340-004-1664-6 79, 1001 (2004).
-
(2004)
Appl. Phys. B: Lasers Opt.
, vol.79
, pp. 1001
-
-
Schmaljohann, H.1
Erhard, M.2
Kronjager, J.3
Sengstock, K.4
Bongs, K.5
-
10
-
-
2542441991
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.92.140403
-
M.-S. Chang, C. D. Hamley, M. D. Barrett, J. A. Sauer, K. M. Fortier, W. Zhang, L. You, and M. S. Chapman, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.92.140403 92, 140403 (2004).
-
(2004)
Phys. Rev. Lett.
, vol.92
, pp. 140403
-
-
Chang, M.-S.1
Hamley, C.D.2
Barrett, M.D.3
Sauer, J.A.4
Fortier, K.M.5
Zhang, W.6
You, L.7
Chapman, M.S.8
-
11
-
-
33645785439
-
-
ZZZZZZ 1745-2473
-
M. S. Chang, Q. Qin, W. X. Zhang, L. You, and M. S. Chapman, Nat. Phys. ZZZZZZ 1745-2473 1, 111 (2005).
-
(2005)
Nat. Phys.
, vol.1
, pp. 111
-
-
Chang, M.S.1
Qin, Q.2
Zhang, W.X.3
You, L.4
Chapman, M.S.5
-
12
-
-
4043110992
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.81.5257
-
C. K. Law, H. Pu, and N. P. Bigelow, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.81.5257 81, 5257 (1998).
-
(1998)
Phys. Rev. Lett.
, vol.81
, pp. 5257
-
-
Law, C.K.1
Pu, H.2
Bigelow, N.P.3
-
13
-
-
0000306645
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.60.1463
-
H. Pu, C. K. Law, S. Raghavan, J. H. Eberly, and N. P. Bigelow, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.60.1463 60, 1463 (1999).
-
(1999)
Phys. Rev. A
, vol.60
, pp. 1463
-
-
Pu, H.1
Law, C.K.2
Raghavan, S.3
Eberly, J.H.4
Bigelow, N.P.5
-
14
-
-
42549158147
-
-
arXiv:cond-mat/0608732.
-
R. B. Diener and T. L. Ho, e-print arXiv:cond-mat/0608732.
-
-
-
Diener, R.B.1
Ho, T.L.2
-
15
-
-
28844503832
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.72.043614
-
C. G. Bao and Z. B. Li, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.72.043614 72, 043614 (2005).
-
(2005)
Phys. Rev. A
, vol.72
, pp. 043614
-
-
Bao, C.G.1
Li, Z.B.2
-
17
-
-
40849124063
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.77.023614
-
Z. Li, C. Bao, and J. Katriel, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.77.023614 77, 023614 (2008).
-
(2008)
Phys. Rev. A
, vol.77
, pp. 023614
-
-
Li, Z.1
Bao, C.2
Katriel, J.3
-
19
-
-
42549158605
-
-
note
-
For the case N0 =N-M and M=N/4, the evolution is well approximated by Eq. 11. Hence, the frequency of oscillation [as shown in Fig. 3] is essentially determined by cos [4 (Sa +3/2+ kmax) τ], where Sa + kmax is the location of the peak of O N0, μ M,S against S [refer to Fig. 1]. It was found numerically that in this case Sa + kmax 0.66N. On the other hand, the strength J can be evaluated under the Thomas-Fermi limit. When N=1000,6000, and 3× 105 R 87 b atoms are trapped in an isotropic harmonic potential with ω=514.5, then the frequency is 0.79, 1.61, and 7.69 Hz, respectively. The latter is close to the frequency given in Fig. 1 of Ref.. Incidentally, 514.5= (ωx ωy ωz) 1/3, where the three ω are those used in the experiment of Ref..
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