-
1
-
-
7444220645
-
-
10.1126/science.1102896
-
K. S. Novoselov, A. K. Geim, S. V. Morozov, D. Jiang, Y. Zhang, S. V. Dubonos, I. V. Grigorieva, and A. A. Firsov Science 306, 666 (2004). 10.1126/science.1102896
-
(2004)
Science
, vol.306
, pp. 666
-
-
Novoselov, K.S.1
Geim, A.K.2
Morozov, S.V.3
Jiang, D.4
Zhang, Y.5
Dubonos, S.V.6
Grigorieva, I.V.7
Firsov, A.A.8
-
2
-
-
27744534165
-
-
10.1038/nature04233
-
K. S. Novoselov, A. K. Geim, S. V. Morozov, D. Jiang, M. I. Katsnelson, I. V. Grigorieva, S. V. Dubonos, and A. A. Firsov, Nature (London) 438, 197 (2005). 10.1038/nature04233
-
(2005)
Nature (London)
, vol.438
, pp. 197
-
-
Novoselov, K.S.1
Geim, A.K.2
Morozov, S.V.3
Jiang, D.4
Katsnelson, M.I.5
Grigorieva, I.V.6
Dubonos, S.V.7
Firsov, A.A.8
-
4
-
-
59949098337
-
-
10.1103/RevModPhys.81.109
-
A. H. Castro Neto, F. Guinea, N. M. R. Peres, K. S. Novoselov, and A. K. Geim, Rev. Mod. Phys. 81, 109 (2009). 10.1103/RevModPhys.81.109
-
(2009)
Rev. Mod. Phys.
, vol.81
, pp. 109
-
-
Castro Neto, A.H.1
Guinea, F.2
Peres, N.M.R.3
Novoselov, K.S.4
Geim, A.K.5
-
5
-
-
85013962866
-
-
edited by T. Makarova and F. Palacios (Elsevier, Amsterdam
-
Carbon Based Magnetism, edited by, T. Makarova, and, F. Palacios, (Elsevier, Amsterdam, 2006).
-
(2006)
Carbon Based Magnetism
-
-
-
6
-
-
34648843377
-
-
10.1103/PhysRevB.76.115423
-
H. Amara, S. Latil, V. Meunier, P. Lambin, and J. C. Charlier, Phys. Rev. B 76, 115423 (2007). 10.1103/PhysRevB.76.115423
-
(2007)
Phys. Rev. B
, vol.76
, pp. 115423
-
-
Amara, H.1
Latil, S.2
Meunier, V.3
Lambin, P.4
Charlier, J.C.5
-
7
-
-
0042208346
-
-
10.1103/PhysRevLett.91.017202
-
P. O. Lehtinen, A. S. Foster, A. Ayuela, A. Krasheninnikov, K. Nordlund, and R. M. Nieminen, Phys. Rev. Lett. 91, 017202 (2003). 10.1103/PhysRevLett.91. 017202
-
(2003)
Phys. Rev. Lett.
, vol.91
, pp. 017202
-
-
Lehtinen, P.O.1
Foster, A.S.2
Ayuela, A.3
Krasheninnikov, A.4
Nordlund, K.5
Nieminen, R.M.6
-
9
-
-
64049105752
-
-
10.1103/PhysRevLett.102.126807
-
A. V. Krasheninnikov, P. O. Lehtinen, A. S. Foster, P. Pyykkö, and R. M. Nieminen, Phys. Rev. Lett. 102, 126807 (2009). 10.1103/PhysRevLett.102. 126807
-
(2009)
Phys. Rev. Lett.
, vol.102
, pp. 126807
-
-
Krasheninnikov, A.V.1
Lehtinen, P.O.2
Foster, A.S.3
Pyykkö, P.4
Nieminen, R.M.5
-
10
-
-
79051470664
-
-
10.1209/0295-5075/80/67007
-
N. M. R. Peres, F. D. Klironomos, S.-W. Tsai, J. R. Santos, J. M. B. Lopes dos Santos, and A. H. Castro Neto, Europhys. Lett. 80, 67007 (2007). 10.1209/0295-5075/80/67007
-
(2007)
Europhys. Lett.
, vol.80
, pp. 67007
-
-
Peres, N.M.R.1
Klironomos, F.D.2
Tsai, S.-W.3
Santos, J.R.4
Lopes Dos Santos, J.M.B.5
Castro Neto, A.H.6
-
12
-
-
33947639578
-
-
10.1103/PhysRevB.75.125425
-
T. O. Wehling, A. V. Balatsky, M. I. Katsnelson, A. I. Lichtenstein, K. Scharnberg, and R. Wiesendanger, Phys. Rev. B 75, 125425 (2007). 10.1103/PhysRevB.75.125425
-
(2007)
Phys. Rev. B
, vol.75
, pp. 125425
-
-
Wehling, T.O.1
Balatsky, A.V.2
Katsnelson, M.I.3
Lichtenstein, A.I.4
Scharnberg, K.5
Wiesendanger, R.6
-
13
-
-
57149129871
-
-
10.1103/PhysRevB.78.195420
-
E. J. G. Santos, A. Ayuela, S. B. Fagan, J. Mendes Filho, D. L. Azevedo, A. G. Souza Filho, and D. Sanchez-Portal, Phys. Rev. B 78, 195420 (2008). 10.1103/PhysRevB.78.195420
-
(2008)
Phys. Rev. B
, vol.78
, pp. 195420
-
-
Santos, E.J.G.1
Ayuela, A.2
Fagan, S.B.3
Mendes Filho, J.4
Azevedo, D.L.5
Souza Filho, A.G.6
Sanchez-Portal, D.7
-
14
-
-
44949134855
-
-
10.1002/smll.200700929
-
Y. Gan, L. Sun, and F. Banhart, Small 4, 587 (2008). 10.1002/smll. 200700929
-
(2008)
Small
, vol.4
, pp. 587
-
-
Gan, Y.1
Sun, L.2
Banhart, F.3
-
16
-
-
3342899450
-
-
10.1103/PhysRevLett.62.1201
-
E. H. Lieb, Phys. Rev. Lett. 62, 1201 (1989). 10.1103/PhysRevLett.62.1201
-
(1989)
Phys. Rev. Lett.
, vol.62
, pp. 1201
-
-
Lieb, E.H.1
-
18
-
-
0037171091
-
-
10.1088/0953-8984/14/11/302
-
J. M. Soler, Emilio Artacho, Julian D. Gale, Alberto García, Javier Junquera, Pablo Ordejón, and Daniel Sánchez-Portal, J. Phys.: Condens. Matter 14, 2745 (2002). 10.1088/0953-8984/14/11/302
-
(2002)
J. Phys.: Condens. Matter
, vol.14
, pp. 2745
-
-
Soler, J.M.1
Artacho, E.2
Gale, J.D.3
García, A.4
Junquera, J.5
Ordejón, P.6
Sánchez-Portal, D.7
-
21
-
-
12844286241
-
-
10.1103/PhysRevB.47.558
-
G. Kresse and J. Hafner, Phys. Rev. B 47, 558 (1993). 10.1103/PhysRevB.47.558
-
(1993)
Phys. Rev. B
, vol.47
, pp. 558
-
-
Kresse, G.1
Hafner, J.2
-
23
-
-
33645731298
-
-
10.1103/PhysRevB.73.144103
-
M. Ushiro, K. Uno, T. Fujikawa, Y. Sato, K. Tohji, F. Watari, W. J. Chun, Y. Koike, and K. Asakura, Phys. Rev. B 73, 144103 (2006). 10.1103/PhysRevB.73. 144103
-
(2006)
Phys. Rev. B
, vol.73
, pp. 144103
-
-
Ushiro, M.1
Uno, K.2
Fujikawa, T.3
Sato, Y.4
Tohji, K.5
Watari, F.6
Chun, W.J.7
Koike, Y.8
Asakura, K.9
-
24
-
-
33747586347
-
-
10.1038/nature04971
-
D. Kitchen, Anthony Richardella, Jian-Ming Tang, Michael E. Flatté, and Ali Yazdani, Nature (London) 442, 436 (2006). 10.1038/nature04971
-
(2006)
Nature (London)
, vol.442
, pp. 436
-
-
Kitchen, D.1
Richardella, A.2
Tang, J.3
Flatté, M.E.4
Yazdani, A.5
-
25
-
-
77955155506
-
-
Only Co has a partially occupied band, related to the impurity, at the Fermi energy composed mostly by pz C character. In contrast, the band character at Fermi energy for Fe is mainly 3d and Ni substitutionals is mainly sp C from the C neighbors
-
Only Co has a partially occupied band, related to the impurity, at the Fermi energy composed mostly by p z C character. In contrast, the band character at Fermi energy for Fe is mainly 3 d and Ni substitutionals is mainly s p C from the C neighbors.
-
-
-
-
26
-
-
48949087936
-
-
10.1103/PhysRevB.70.125422;
-
M. Khantha, N. A. Cordero, L. M. Molina, J. A. Alonso, and L. A. Girifalco, Phys. Rev. B 70, 125422 (2004) 10.1103/PhysRevB.70.125422
-
(2004)
Phys. Rev. B
, vol.70
, pp. 125422
-
-
Khantha, M.1
Cordero, N.A.2
Molina, L.M.3
Alonso, J.A.4
Girifalco, L.A.5
-
28
-
-
51849164491
-
-
10.1063/1.2966373
-
Y. Sanchez-Paisal, D. Sanchez-Portal, N. Garmendia, R. Muñoz, I. Obieta, J. Arbiol, L. Calvo-Barrio, and A. Ayuela, Appl. Phys. Lett. 93, 053101 (2008). 10.1063/1.2966373
-
(2008)
Appl. Phys. Lett.
, vol.93
, pp. 053101
-
-
Sanchez-Paisal, Y.1
Sanchez-Portal, D.2
Garmendia, N.3
Muñoz, R.4
Obieta, I.5
Arbiol, J.6
Calvo-Barrio, L.7
Ayuela, A.8
-
29
-
-
77955155249
-
-
When we could stabilize a FM solution, it lies at higher energy, around 0.2 eV above the PM one
-
When we could stabilize a FM solution, it lies at higher energy, around 0.2 eV above the PM one.
-
-
-
-
30
-
-
0032179596
-
-
10.1016/S0039-6028(98)00622-0
-
K. F. Kelly and N. J. Halas, Surf. Sci. 416, L1085 (1998). 10.1016/S0039-6028(98)00622-0
-
(1998)
Surf. Sci.
, vol.416
, pp. 1085
-
-
Kelly, K.F.1
Halas, N.J.2
-
31
-
-
0001277852
-
-
10.1126/science.244.4904.559
-
H. A. Mizes and J. S. Foster, Science 244, 559 (1989). 10.1126/science.244.4904.559
-
(1989)
Science
, vol.244
, pp. 559
-
-
Mizes, H.A.1
Foster, J.S.2
-
32
-
-
34447550598
-
-
10.1126/science.1142882
-
G. M. Rutter, J. N. Crain, N. P. Guisinger, T. Li, P. N. First, and J. A. Stroscio, Science 317, 219 (2007). 10.1126/science.1142882
-
(2007)
Science
, vol.317
, pp. 219
-
-
Rutter, G.M.1
Crain, J.N.2
Guisinger, N.P.3
Li, T.4
First, P.N.5
Stroscio, J.A.6
-
33
-
-
0000530417
-
-
10.1103/PhysRevLett.84.4910
-
P. Ruffieux, O. Groning, P. Schwaller, L. Schlapbach, and P. Groning, Phys. Rev. Lett. 84, 4910 (2000). 10.1103/PhysRevLett.84.4910
-
(2000)
Phys. Rev. Lett.
, vol.84
, pp. 4910
-
-
Ruffieux, P.1
Groning, O.2
Schwaller, P.3
Schlapbach, L.4
Groning, P.5
-
34
-
-
47749146955
-
-
10.1103/PhysRevLett.101.037203
-
O. V. Yazyev, Phys. Rev. Lett. 101, 037203 (2008). 10.1103/PhysRevLett. 101.037203
-
(2008)
Phys. Rev. Lett.
, vol.101
, pp. 037203
-
-
Yazyev, O.V.1
-
35
-
-
36348983181
-
-
10.1103/PhysRevB.76.184430
-
S. Saremi, Phys. Rev. B 76, 184430 (2007). 10.1103/PhysRevB.76.184430
-
(2007)
Phys. Rev. B
, vol.76
, pp. 184430
-
-
Saremi, S.1
-
36
-
-
29644435690
-
-
10.1103/PhysRevB.72.155121
-
M. A. H. Vozmediano, M. P. Lopez-Sancho, T. Stauber, and F. Guinea, Phys. Rev. B 72, 155121 (2005). 10.1103/PhysRevB.72.155121
-
(2005)
Phys. Rev. B
, vol.72
, pp. 155121
-
-
Vozmediano, M.A.H.1
Lopez-Sancho, M.P.2
Stauber, T.3
Guinea, F.4
-
37
-
-
77955158470
-
-
) AB configuration, respectively. These values have to be compared with the ∼0.5eV spin splitting of the Cosub defect. All those AB systems with gaps larger than 0.4 eV are found to converge to PM solutions
-
) A B configuration, respectively. These values have to be compared with the ∼ 0.5 eV spin splitting of the Co s u b defect. All those A B systems with gaps larger than 0.4 eV are found to converge to PM solutions.
-
-
-
-
39
-
-
33847768178
-
-
10.1103/PhysRevB.75.125408
-
O. V. Yazyev and L. Helm, Phys. Rev. B 75, 125408 (2007). 10.1103/PhysRevB.75.125408
-
(2007)
Phys. Rev. B
, vol.75
, pp. 125408
-
-
Yazyev, O.V.1
Helm, L.2
-
42
-
-
42649110687
-
-
10.1103/PhysRevB.77.134114
-
Yang Lei, S. A. Shevlin, W. Zhu, and Z. X. Guo, Phys. Rev. B 77, 134114 (2008). 10.1103/PhysRevB.77.134114
-
(2008)
Phys. Rev. B
, vol.77
, pp. 134114
-
-
Lei, Y.1
Shevlin, S.A.2
Zhu, W.3
Guo, Z.X.4
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