-
4
-
-
0001468910
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.31.5811
-
J. A. X. Alexander, T. P. Orlando, D. Rainer, and P. M. Tedrow, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.31.5811 31, 5811 (1985).
-
(1985)
Phys. Rev. B
, vol.31
, pp. 5811
-
-
Alexander, J.A.X.1
Orlando, T.P.2
Rainer, D.3
Tedrow, P.M.4
-
5
-
-
4243786428
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.52.1637
-
P. M. Tedrow, J. T. Kucera, D. Rainer, and T. P. Orlando, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.52.1637 52, 1637 (1984).
-
(1984)
Phys. Rev. Lett.
, vol.52
, pp. 1637
-
-
Tedrow, P.M.1
Kucera, J.T.2
Rainer, D.3
Orlando, T.P.4
-
8
-
-
0031273831
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.79.4242
-
I. L. Aleiner and B. L. Altshuler, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.79.4242 79, 4242 (1997).
-
(1997)
Phys. Rev. Lett.
, vol.79
, pp. 4242
-
-
Aleiner, I.L.1
Altshuler, B.L.2
-
11
-
-
84918110772
-
-
ADPHAH 0001-8732 10.1080/00018737300101369
-
P. Fulde, Adv. Phys. ADPHAH 0001-8732 10.1080/00018737300101369 22, 667 (1973).
-
(1973)
Adv. Phys.
, vol.22
, pp. 667
-
-
Fulde, P.1
-
12
-
-
27144500674
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.95.066804
-
F. Giazotto, F. Taddei, R. Fazio, and F. Beltram, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.95.066804 95, 066804 (2005)
-
(2005)
Phys. Rev. Lett.
, vol.95
, pp. 066804
-
-
Giazotto, F.1
Taddei, F.2
Fazio, R.3
Beltram, F.4
-
13
-
-
36349033381
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.76.184518
-
F. Giazotto, F. Taddei, P. D'Amico, R. Fazio, and F. Beltram, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.76.184518 76, 184518 (2007)
-
(2007)
Phys. Rev. B
, vol.76
, pp. 184518
-
-
Giazotto, F.1
Taddei, F.2
D'Amico, P.3
Fazio, R.4
Beltram, F.5
-
14
-
-
41549141748
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.77.132501
-
F. Giazotto and F. Taddei, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.77.132501 77, 132501 (2008).
-
(2008)
Phys. Rev. B
, vol.77
, pp. 132501
-
-
Giazotto, F.1
Taddei, F.2
-
17
-
-
0006409296
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.73.1412
-
W. Wu and P. W. Adams, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.73.1412 73, 1412 (1994).
-
(1994)
Phys. Rev. Lett.
, vol.73
, pp. 1412
-
-
Wu, W.1
Adams, P.W.2
-
18
-
-
3543099749
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.9.266
-
A. M. Clogston, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.9. 266 9, 266 (1962).
-
(1962)
Phys. Rev. Lett.
, vol.9
, pp. 266
-
-
Clogston, A.M.1
-
19
-
-
0001855662
-
-
APPLAB 0003-6951 10.1063/1.1777362
-
B. S. Chandrasekhar, Appl. Phys. Lett. APPLAB 0003-6951 10.1063/1.1777362 1, 7 (1962).
-
(1962)
Appl. Phys. Lett.
, vol.1
, pp. 7
-
-
Chandrasekhar, B.S.1
-
20
-
-
0000813265
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.74.610
-
W. Wu and P. W. Adams, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.74.610 74, 610 (1995).
-
(1995)
Phys. Rev. Lett.
, vol.74
, pp. 610
-
-
Wu, W.1
Adams, P.W.2
-
22
-
-
28844485138
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.95.167001
-
X. S. Wu, P. W. Adams, and G. Catelani, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.95.167001 95, 167001 (2005)
-
(2005)
Phys. Rev. Lett.
, vol.95
, pp. 167001
-
-
Wu, X.S.1
Adams, P.W.2
Catelani, G.3
-
23
-
-
33144467617
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.73.020503
-
G. Catelani, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.73.020503 73, 020503 (R) (2006).
-
(2006)
Phys. Rev. B
, vol.73
, pp. 020503
-
-
Catelani, G.1
-
24
-
-
0004287161
-
-
edited by R. D. Parks (Dekker, New York
-
K. Maki, in Superconductivity, edited by, R. D. Parks, (Dekker, New York, 1969), Chap..
-
(1969)
Superconductivity
-
-
Maki, K.1
-
26
-
-
0001710612
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.51.1378
-
W. Wu, R. G. Goodrich, and P. W. Adams, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.51.1378 51, 1378 (1995).
-
(1995)
Phys. Rev. B
, vol.51
, pp. 1378
-
-
Wu, W.1
Goodrich, R.G.2
Adams, P.W.3
-
27
-
-
33750438202
-
-
SSCOA4 0038-1098 10.1016/0038-1098(67)90514-5
-
P. Fulde, Solid State Commun. SSCOA4 0038-1098 10.1016/0038-1098(67) 90514-5 5, 181 (1967).
-
(1967)
Solid State Commun.
, vol.5
, pp. 181
-
-
Fulde, P.1
-
28
-
-
33750482588
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.74.144519
-
X. S. Wu, P. W. Adams, and G. Catelani, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.74.144519 74, 144519 (2006).
-
(2006)
Phys. Rev. B
, vol.74
, pp. 144519
-
-
Wu, X.S.1
Adams, P.W.2
Catelani, G.3
-
29
-
-
52949142695
-
-
This estimate of ξ is obtained using the value of the mean free path ℓ reported in Ref. via ξ ≃√ξ0ℓ, where ξ0 =hvF/pi;Δo and vF is the Fermi velocity. To further support this estimate we note that a separate measurement of the perpendicular critical field for a similarly prepared 6 nm thick film gives ξ≃56 nm (here we use Hc⊥ = φ0 /2π ξ2 with φ0 the flux quantum).
-
This estimate of ξ is obtained using the value of the mean free path ℓ reported in Ref. via ξ ≃√ξ0ℓ, where ξ0 =hvF/pi;Δo and vF is the Fermi velocity. To further support this estimate we note that a separate measurement of the perpendicular critical field for a similarly prepared 6 nm thick film gives ξ≃56 nm (here we use Hc⊥ = φ0 /2π ξ2 with φ0 the flux quantum).
-
-
-
-
30
-
-
0342743940
-
-
See, e.g., PRLTAO 0031-9007 10.1103/PhysRevLett.41.1509
-
See, e.g., R. C. Dynes, V. Narayanamurti, and J. P. Garno, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.41.1509 41, 1509 (1978)
-
(1978)
Phys. Rev. Lett.
, vol.41
, pp. 1509
-
-
Dynes, R.C.1
Narayanamurti, V.2
Garno, J.P.3
-
31
-
-
3343023226
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.53.2437
-
R. C. Dynes, J. P. Garno, G. B. Hertel, and T. P. Orlando, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.53.2437 53, 2437 (1984).
-
(1984)
Phys. Rev. Lett.
, vol.53
, pp. 2437
-
-
Dynes, R.C.1
Garno, J.P.2
Hertel, G.B.3
Orlando, T.P.4
-
32
-
-
1642276420
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.92.056804
-
J. P. Pekola, T. T. Heikkila, A. M. Savin, J. T. Flyktman, F. Giazotto, and F. W. J. Hekking, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.92. 056804 92, 056804 (2004).
-
(2004)
Phys. Rev. Lett.
, vol.92
, pp. 056804
-
-
Pekola, J.P.1
Heikkila, T.T.2
Savin, A.M.3
Flyktman, J.T.4
Giazotto, F.5
Hekking, F.W.J.6
-
33
-
-
52949126940
-
-
For example, no broadening is used in the upper panel curve-including it would slightly suppress the peaks' magnitude. Due to their interdependence, however, different values for c and Γ ≠ 0 could also satisfactorily fit the data.
-
For example, no broadening is used in the upper panel curve-including it would slightly suppress the peaks' magnitude. Due to their interdependence, however, different values for c and Γ ≠ 0 could also satisfactorily fit the data.
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