-
1
-
-
18144375250
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.94.090405
-
Y.J. Wang, Phys. Rev. Lett. 94, 090405 (2005). PRLTAO 0031-9007 10.1103/PhysRevLett.94.090405
-
(2005)
Phys. Rev. Lett.
, vol.94
, pp. 090405
-
-
Wang, Y.J.1
-
2
-
-
0141973598
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.91.080401
-
M.P.A. Jones, Phys. Rev. Lett. 91, 080401 (2003). PRLTAO 0031-9007 10.1103/PhysRevLett.91.080401
-
(2003)
Phys. Rev. Lett.
, vol.91
, pp. 080401
-
-
Jones, M.P.A.1
-
3
-
-
0033546505
-
-
EULEEJ 0295-5075 10.1209/epl/i1999-00404-8
-
C. Henkel and M. Wilkens, Europhys. Lett. 47, 414 (1999). EULEEJ 0295-5075 10.1209/epl/i1999-00404-8
-
(1999)
Europhys. Lett.
, vol.47
, pp. 414
-
-
Henkel, C.1
Wilkens, M.2
-
4
-
-
0347699521
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.76.4500
-
H. Ito, Phys. Rev. Lett. 76, 4500 (1996). PRLTAO 0031-9007 10.1103/PhysRevLett.76.4500
-
(1996)
Phys. Rev. Lett.
, vol.76
, pp. 4500
-
-
Ito, H.1
-
5
-
-
0000402006
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.55.3684
-
M.J. Renn, Phys. Rev. A 55, 3684 (1997). PLRAAN 1050-2947 10.1103/PhysRevA.55.3684
-
(1997)
Phys. Rev. A
, vol.55
, pp. 3684
-
-
Renn, M.J.1
-
6
-
-
0033316032
-
-
JOBOFD 1464-4266 10.1088/1464-4266/1/4/307
-
R.G. Dall, J. Opt. B 1, 396 (1999). JOBOFD 1464-4266 10.1088/1464-4266/1/ 4/307
-
(1999)
J. Opt. B
, vol.1
, pp. 396
-
-
Dall, R.G.1
-
7
-
-
4243890730
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.61.033411
-
D. Müller, Phys. Rev. A 61, 033411 (2000). PLRAAN 1050-2947 10.1103/PhysRevA.61.033411
-
(2000)
Phys. Rev. A
, vol.61
, pp. 033411
-
-
Müller, D.1
-
8
-
-
0033520334
-
-
SCIEAS 0036-8075 10.1126/science.285.5433.1537
-
R.F. Cregan, Science 285, 1537 (1999). SCIEAS 0036-8075 10.1126/science.285.5433.1537
-
(1999)
Science
, vol.285
, pp. 1537
-
-
Cregan, R.F.1
-
9
-
-
33749066122
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.97.023603
-
S. Ghosh, Phys. Rev. Lett. 97, 023603 (2006). PRLTAO 0031-9007 10.1103/PhysRevLett.97.023603
-
(2006)
Phys. Rev. Lett.
, vol.97
, pp. 023603
-
-
Ghosh, S.1
-
10
-
-
17444398658
-
-
OPEXFF 1094-4087 10.1364/OPEX.13.001457
-
M. Wegmüller, Opt. Express 13, 1457 (2005). At 860 nm, linearly polarized input light always gives a clean, roughly Gaussian mode. OPEXFF 1094-4087 10.1364/OPEX.13.001457
-
(2005)
Opt. Express
, vol.13
, pp. 1457
-
-
Wegmüller, M.1
-
11
-
-
34547239724
-
-
JPAMA4 0022-3700 10.1088/0022-3700/2/5/313
-
D.J. Croucher and J.L. Clark, J. Phys. B JPAMA4 0022-3700 2, 603 (1969); 10.1088/0022-3700/2/5/313
-
(1969)
J. Phys. B
, vol.2
, pp. 603
-
-
Croucher, D.J.1
Clark, J.L.2
-
13
-
-
0035331807
-
-
with van der Waals constants and polarizabilities from PLRAAN 1050-2947 10.1103/PhysRevA.63.052704
-
with van der Waals constants and polarizabilities from A. Derevianko, J.F. Babb, and A. Dalgarno, Phys. Rev. A 63, 052704 (2001); PLRAAN 1050-2947 10.1103/PhysRevA.63.052704
-
(2001)
Phys. Rev. A
, vol.63
, pp. 052704
-
-
Derevianko, A.1
Babb, J.F.2
Dalgarno, A.3
-
14
-
-
0001437377
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.59.4708
-
E. Hult, Phys. Rev. B PRBMDO 0163-1829 59, 4708 (1999). 10.1103/PhysRevB.59.4708
-
(1999)
Phys. Rev. B
, vol.59
, pp. 4708
-
-
Hult, E.1
-
15
-
-
3042709248
-
-
PLRAAN 1050-2947 10.1103/PhysRevA.69.053411
-
T. Takekoshi, Phys. Rev. A 69, 053411 (2004). This is the 5P3/2→continuum cross section. Almost all of the excited atoms are in 5P3/2, as verified by trying 476 nm light instead of 458 nm light. PLRAAN 1050-2947 10.1103/PhysRevA.69.053411
-
(2004)
Phys. Rev. A
, vol.69
, pp. 053411
-
-
Takekoshi, T.1
-
16
-
-
0346621532
-
-
APPCDL 0721-7269 10.1007/BF00325375
-
M. Kasevich and S. Chu, Appl. Phys. B APPCDL 0721-7269 54, 321 (1992). 10.1007/BF00325375
-
(1992)
Appl. Phys. B
, vol.54
, pp. 321
-
-
Kasevich, M.1
Chu, S.2
|