-
1
-
-
58249112255
-
-
10.1038/nature07644
-
T. Kondo, R. Khasanov, T. Takeuchi, J. Schmalian, and A. Kaminski, Nature (London) 457, 296 (2009). 10.1038/nature07644
-
(2009)
Nature (London)
, vol.457
, pp. 296
-
-
Kondo, T.1
Khasanov, R.2
Takeuchi, T.3
Schmalian, J.4
Kaminski, A.5
-
2
-
-
35948999286
-
-
10.1038/nature06219
-
W. S. Lee, Nature (London) 450, 81 (2007). 10.1038/nature06219
-
(2007)
Nature (London)
, vol.450
, pp. 81
-
-
Lee, W.S.1
-
4
-
-
0030169494
-
-
10.1103/PhysRevLett.76.4841;
-
D. S. Marshall, Phys. Rev. Lett. 76, 4841 (1996) 10.1103/PhysRevLett.76. 4841
-
(1996)
Phys. Rev. Lett.
, vol.76
, pp. 4841
-
-
Marshall, D.S.1
-
5
-
-
0029951157
-
-
10.1038/382051a0;
-
H. Ding, Nature (London) 382, 51 (1996) 10.1038/382051a0
-
(1996)
Nature (London)
, vol.382
, pp. 51
-
-
Ding, H.1
-
6
-
-
0039224686
-
-
10.1126/science.273.5273.325;
-
A. G. Loeser, Science 273, 325 (1996) 10.1126/science.273.5273.325
-
(1996)
Science
, vol.273
, pp. 325
-
-
Loeser, A.G.1
-
7
-
-
33745782185
-
-
10.1038/nphys334
-
A. Kanigel, Nat. Phys. 2, 447 (2006). 10.1038/nphys334
-
(2006)
Nat. Phys.
, vol.2
, pp. 447
-
-
Kanigel, A.1
-
9
-
-
69549124309
-
-
10.1126/science.1176369
-
J. Lee, Science 325, 1099 (2009). 10.1126/science.1176369
-
(2009)
Science
, vol.325
, pp. 1099
-
-
Lee, J.1
-
10
-
-
50649124272
-
-
10.1038/nature07243
-
Y. Kohsaka, Nature (London) 454, 1072 (2008). 10.1038/nature07243
-
(2008)
Nature (London)
, vol.454
, pp. 1072
-
-
Kohsaka, Y.1
-
11
-
-
67650215690
-
-
10.1126/science.1174338
-
A. Pushp, Science 324, 1689 (2009). 10.1126/science.1174338
-
(2009)
Science
, vol.324
, pp. 1689
-
-
Pushp, A.1
-
12
-
-
0037933404
-
-
10.1103/PhysRevLett.90.197004
-
D. G. Hawthorn, Phys. Rev. Lett. 90, 197004 (2003). 10.1103/PhysRevLett. 90.197004
-
(2003)
Phys. Rev. Lett.
, vol.90
, pp. 197004
-
-
Hawthorn, D.G.1
-
13
-
-
33751073198
-
-
10.1103/PhysRevLett.97.207001
-
N. Doiron-Leyraud, Phys. Rev. Lett. 97, 207001 (2006). 10.1103/PhysRevLett.97.207001
-
(2006)
Phys. Rev. Lett.
, vol.97
, pp. 207001
-
-
Doiron-Leyraud, N.1
-
14
-
-
18144382642
-
-
10.1103/PhysRevLett.94.147004
-
M. Sutherland, Phys. Rev. Lett. 94, 147004 (2005). 10.1103/PhysRevLett. 94.147004
-
(2005)
Phys. Rev. Lett.
, vol.94
, pp. 147004
-
-
Sutherland, M.1
-
15
-
-
29844438971
-
-
10.1103/PhysRevB.72.214511
-
C. Proust, K. Behnia, R. Bel, D. Maude, and S. I. Vedeneev, Phys. Rev. B 72, 214511 (2005). 10.1103/PhysRevB.72.214511
-
(2005)
Phys. Rev. B
, vol.72
, pp. 214511
-
-
Proust, C.1
Behnia, K.2
Bel, R.3
Maude, D.4
Vedeneev, S.I.5
-
16
-
-
0000132646
-
-
10.1103/PhysRevB.62.1270
-
A. C. Durst and P. A. Lee, Phys. Rev. B 62, 1270 (2000). 10.1103/PhysRevB.62.1270
-
(2000)
Phys. Rev. B
, vol.62
, pp. 1270
-
-
Durst, A.C.1
Lee, P.A.2
-
18
-
-
0019592467
-
-
10.1080/00018738100101407
-
A. G. Aronov, Y. M. Gal'perin, V. L. Gurevich, and V. I. Kozub, Adv. Phys. 30, 539 (1981). 10.1080/00018738100101407
-
(1981)
Adv. Phys.
, vol.30
, pp. 539
-
-
Aronov, A.G.1
Gal'Perin, Y.M.2
Gurevich, V.L.3
Kozub, V.I.4
-
19
-
-
35949000515
-
-
10.1103/PhysRevB.76.174501
-
M. R. Norman, A. Kanigel, M. Randeria, U. Chatterjee, and J. C. Campuzano, Phys. Rev. B 76, 174501 (2007). 10.1103/PhysRevB.76.174501
-
(2007)
Phys. Rev. B
, vol.76
, pp. 174501
-
-
Norman, M.R.1
Kanigel, A.2
Randeria, M.3
Chatterjee, U.4
Campuzano, J.C.5
-
20
-
-
33344474731
-
-
10.1103/PhysRevB.71.172509
-
T.-K. Ng, Phys. Rev. B 71, 172509 (2005). 10.1103/PhysRevB.71.172509
-
(2005)
Phys. Rev. B
, vol.71
, pp. 172509
-
-
Ng, T.-K.1
-
22
-
-
68949128598
-
-
10.1103/PhysRevLett.103.076402
-
T. Senthil and P. A. Lee, Phys. Rev. Lett. 103, 076402 (2009). 10.1103/PhysRevLett.103.076402
-
(2009)
Phys. Rev. Lett.
, vol.103
, pp. 076402
-
-
Senthil, T.1
Lee, P.A.2
-
23
-
-
67349284330
-
-
10.1016/j.aop.2009.02.004
-
L. L. Hur and T. M. Rice, Ann. Phys. 324, 1452 (2009). 10.1016/j.aop.2009.02.004
-
(2009)
Ann. Phys.
, vol.324
, pp. 1452
-
-
Hur, L.L.1
Rice, T.M.2
-
25
-
-
70249146960
-
-
10.1209/0295-5075/86/37002
-
K.-Y. Yang, H.-B. Yang, P. D. Johnson, T. M. Rice, and F.-C. Zhang, EPL 86, 37002 (2009). 10.1209/0295-5075/86/37002
-
(2009)
EPL
, vol.86
, pp. 37002
-
-
Yang, K.-Y.1
Yang, H.-B.2
Johnson, P.D.3
Rice, T.M.4
Zhang, F.-C.5
-
26
-
-
77954964812
-
-
10.1103/PhysRevB.81.115129
-
Y. Qi and S. Sachdev, Phys. Rev. B 81, 115129 (2010). 10.1103/PhysRevB.81.115129
-
(2010)
Phys. Rev. B
, vol.81
, pp. 115129
-
-
Qi, Y.1
Sachdev, S.2
-
28
-
-
0032498772
-
-
10.1103/PhysRevLett.80.2193
-
X.-G. Wen and P. A. Lee, Phys. Rev. Lett. 80, 2193 (1998). 10.1103/PhysRevLett.80.2193
-
(1998)
Phys. Rev. Lett.
, vol.80
, pp. 2193
-
-
Wen, X.-G.1
Lee, P.A.2
-
30
-
-
0037101091
-
-
10.1103/PhysRevB.66.033104
-
W. Kim and J. P. Carbotte, Phys. Rev. B 66, 033104 (2002). 10.1103/PhysRevB.66.033104
-
(2002)
Phys. Rev. B
, vol.66
, pp. 033104
-
-
Kim, W.1
Carbotte, J.P.2
-
32
-
-
77956503374
-
-
For example, from Eq. the heat current in the electron basis U vth U is d dk H k, which can be rewritten in the BCS case as vth = τ 3 vf + τ 1 v2, where τ α is a Pauli matrix. This is a well-known result for d -wave superconductors (Ref.)
-
For example, from Eq. the heat current in the electron basis U v t h U is d d k H k, which can be rewritten in the BCS case as v t h = τ 3 v f + τ 1 v 2, where τ α is a Pauli matrix. This is a well-known result for d -wave superconductors (Ref.).
-
-
-
-
34
-
-
77956526492
-
-
Both particle-particle and particle-hole scattering processes are incorporated into the self energy appearing in the YRZ Green's function. So our conductivity calculation, which separately considers this Green's function within the electron-hole and electron-electron pairing scenarios, is not fully consistent with the YRZ formulation. However, since we treat the model Green's functions as though they were purely phenomonological, the calculation follows the spirit of this article
-
Both particle-particle and particle-hole scattering processes are incorporated into the self energy appearing in the YRZ Green's function. So our conductivity calculation, which separately considers this Green's function within the electron-hole and electron-electron pairing scenarios, is not fully consistent with the YRZ formulation. However, since we treat the model Green's functions as though they were purely phenomonological, the calculation follows the spirit of this article.
-
-
-
|