-
1
-
-
41349119565
-
-
PLEEE8 1063-651X 10.1103/PhysRevE.70.066142
-
E. Cuansing and Hisao Nakanishi, Phys. Rev. E PLEEE8 1063-651X 10.1103/PhysRevE.70.066142, 70, 066142 (2004).
-
(2004)
Phys. Rev. e
, vol.70
, pp. 066142
-
-
Cuansing, E.1
Nakanishi, H.2
-
3
-
-
5544255958
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.44.9926
-
Th. Koslowski and W. von Niessen, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.44.9926 44, 9926 (1991).
-
(1991)
Phys. Rev. B
, vol.44
, pp. 9926
-
-
Koslowski, Th.1
Von Niessen, W.2
-
4
-
-
0000199476
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.53.R16125
-
R. Berkovits and Y. Avishai, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.53.R16125 53, R16125 (1996).
-
(1996)
Phys. Rev. B
, vol.53
, pp. 16125
-
-
Berkovits, R.1
Avishai, Y.2
-
5
-
-
26144433204
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.42.673
-
E. Abrahams, P. W. Anderson, D. C. Licciardello, and T. V. Ramakrishnan, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.42.673 42, 673 (1979).
-
(1979)
Phys. Rev. Lett.
, vol.42
, pp. 673
-
-
Abrahams, E.1
Anderson, P.W.2
Licciardello, D.C.3
Ramakrishnan, T.V.4
-
6
-
-
33244490523
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.73.045118
-
N. Goldenfeld and R. Haydock, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.73.045118 73, 045118 (2006).
-
(2006)
Phys. Rev. B
, vol.73
, pp. 045118
-
-
Goldenfeld, N.1
Haydock, R.2
-
8
-
-
0010150536
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.30.1612
-
T. Odagaki and K. C. Chang, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.30.1612 30, 1612 (1984).
-
(1984)
Phys. Rev. B
, vol.30
, pp. 1612
-
-
Odagaki, T.1
Chang, K.C.2
-
9
-
-
4244169869
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.30.2238
-
V. Srivastava and M. Chaturvedi, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.30.2238 30, 2238 (1984).
-
(1984)
Phys. Rev. B
, vol.30
, pp. 2238
-
-
Srivastava, V.1
Chaturvedi, M.2
-
13
-
-
0035994639
-
-
PSSBBD 0370-1972 10.1002/1521-3951(200203)230:1<249::AID-PSSB249>3. 0.CO;2-G
-
G. Hałda, A. Kolek, and A. W. Stadler, Phys. Status Solidi B PSSBBD 0370-1972 10.1002/1521-3951(200203)230:1<249::AID-PSSB249>3.0.CO;2- G 230, 249 (2002).
-
(2002)
Phys. Status Solidi B
, vol.230
, pp. 249
-
-
Hałda, G.1
Kolek, A.2
Stadler, A.W.3
-
14
-
-
0000097507
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.45.1074
-
Y. Avishai and J. M. Luck, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.45.1074 45, 1074 (1992).
-
(1992)
Phys. Rev. B
, vol.45
, pp. 1074
-
-
Avishai, Y.1
Luck, J.M.2
-
16
-
-
0001227039
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.44.4685
-
C. M. Soukoulis and G. S. Grest, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.44.4685 44, 4685 (1991).
-
(1991)
Phys. Rev. B
, vol.44
, pp. 4685
-
-
Soukoulis, C.M.1
Grest, G.S.2
-
18
-
-
0001390732
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.49.3190
-
M. Inui, S. A. Trugman, and E. Abrahams, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.49.3190 49, 3190 (1994).
-
(1994)
Phys. Rev. B
, vol.49
, pp. 3190
-
-
Inui, M.1
Trugman, S.A.2
Abrahams, E.3
-
19
-
-
36649033463
-
-
PHYADX 0378-4371 10.1016/j.physa.2007.10.002
-
E. Cuansing and Hisao Nakanishi, Physica A PHYADX 0378-4371 10.1016/j.physa.2007.10.002, 387, 806 (2008).
-
(2008)
Physica A
, vol.387
, pp. 806
-
-
Cuansing, E.1
Nakanishi, H.2
-
20
-
-
0000254815
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.43.721
-
G. J. Dolan and D. D. Osheroff, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.43.721 43, 721 (1979).
-
(1979)
Phys. Rev. Lett.
, vol.43
, pp. 721
-
-
Dolan, G.J.1
Osheroff, D.D.2
-
21
-
-
0000383309
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.44.1153
-
D. J. Bishop, D. C. Tsui, and R. C. Dynes, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.44.1153 44, 1153 (1980).
-
(1980)
Phys. Rev. Lett.
, vol.44
, pp. 1153
-
-
Bishop, D.J.1
Tsui, D.C.2
Dynes, R.C.3
-
22
-
-
36149046984
-
-
JPSOAW 0022-3719 10.1088/0022-3719/13/33/005
-
M. J. Uren, R. A. Davies, and M. Papper, J. Phys. C JPSOAW 0022-3719 10.1088/0022-3719/13/33/005 13, L985 (1980).
-
(1980)
J. Phys. C
, vol.13
, pp. 985
-
-
Uren, M.J.1
Davies, R.A.2
Papper, M.3
-
23
-
-
4243615171
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.50.8039
-
S. V. Kravchenko, G. V. Kravchenko, J. E. Furneaux, V. M. Pudalov, and M. D'Iorio, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.50.8039 50, 8039 (1994).
-
(1994)
Phys. Rev. B
, vol.50
, pp. 8039
-
-
Kravchenko, S.V.1
Kravchenko, G.V.2
Furneaux, J.E.3
Pudalov, V.M.4
D'Iorio, M.5
-
24
-
-
18344376980
-
-
PRBMDO 0163-1829 10.1103/PhysRevB.51.7038
-
S. V. Kravchenko, W. E. Mason, G. E. Bowker, J. E. Furneaux, V. M. Pudalov, and M. D'Iorio, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.51.7038 51, 7038 (1995).
-
(1995)
Phys. Rev. B
, vol.51
, pp. 7038
-
-
Kravchenko, S.V.1
Mason, W.E.2
Bowker, G.E.3
Furneaux, J.E.4
Pudalov, V.M.5
D'Iorio, M.6
-
26
-
-
44949093814
-
-
edited by N. P. Ong and R. N. Bhatt (Princeton University Press, Princeton, NJ
-
M. P. Sarachik, in More is Different: Fifty Years of Condensed Matter Physics, edited by, N. P. Ong, and, R. N. Bhatt, (Princeton University Press, Princeton, NJ, 2001), pp. 42-43.
-
(2001)
More Is Different: Fifty Years of Condensed Matter Physics
, pp. 42-43
-
-
Sarachik, M.P.1
-
30
-
-
44949205821
-
-
note
-
For exponential and power laws, the motivation comes from a picture where the transmission arises from overlapping wave functions. Then the overlap integral will decay exponentially with the distance if the wave functions are themselves exponential. It will decay by a power law if they are power-law or long-ranged. The motivation for fitting to an exponential plus a constant offset to test for delocalization can be understood by a simple analogy to, say, the correlation function of an Ising model below Tc. If there were finite order (transmission, here), then there would be a constant offset. Except for this "order", the correlation should behave very similarly to the "disordered" phase since the critical correlation of the fluctuations should only occur at Tc and not for T< Tc or T> Tc. That is, if we subtract the offset, the remainder should decay the same way as it does above Tc, i.e., exponentially. Of course, in our problem, this analogy may not be true and some sort of residual long-range correlations may still exist after subtracting the offset, which might require a power-law plus offset instead. However, our first guess would be to use an exponential plus offset.
-
-
-
|