-
1
-
-
0030146149
-
-
10.1103/PhysRevLett.76.4250
-
E. Beaurepaire, J.-C. Merle, A. Daunois, and J.-Y. Bigot, Phys. Rev. Lett. 76, 4250 (1996). 10.1103/PhysRevLett.76.4250
-
(1996)
Phys. Rev. Lett.
, vol.76
, pp. 4250
-
-
Beaurepaire, E.1
Merle, J.-C.2
Daunois, A.3
Bigot, J.-Y.4
-
3
-
-
24144444305
-
-
10.1007/3-540-40907-6-8
-
G. P. Zhang, W. Hübner, E. Beaurepaire, and J.-Y. Bigot, Top. Appl. Phys. 83, 245 (2002). 10.1007/3-540-40907-6-8
-
(2002)
Top. Appl. Phys.
, vol.83
, pp. 245
-
-
Zhang, G.P.1
Hübner, W.2
Beaurepaire, E.3
Bigot, J.-Y.4
-
4
-
-
19444377818
-
-
10.1103/PhysRevLett.93.077401;
-
J.-Y. Bigot, L. Guidoni, E. Beaurepaire, and P. N. Saeta, Phys. Rev. Lett. 93, 077401 (2004) 10.1103/PhysRevLett.93.077401
-
(2004)
Phys. Rev. Lett.
, vol.93
, pp. 077401
-
-
Bigot, J.-Y.1
Guidoni, L.2
Beaurepaire, E.3
Saeta, P.N.4
-
5
-
-
27744595862
-
-
10.1103/PhysRevLett.94.237601;
-
M. Vomir, L. H. F. Andrade, L. Guidoni, E. Beaurepaire, and J.-Y. Bigot, Phys. Rev. Lett. 94, 237601 (2005) 10.1103/PhysRevLett.94.237601
-
(2005)
Phys. Rev. Lett.
, vol.94
, pp. 237601
-
-
Vomir, M.1
Andrade, L.H.F.2
Guidoni, L.3
Beaurepaire, E.4
Bigot, J.-Y.5
-
6
-
-
63549124117
-
-
10.1103/PhysRevLett.102.117201;
-
I. Radu, G. Woltersdorf, M. Kiessling, A. Melnikov, U. Bovensiepen, J.-U. Thiele, and C. H. Back, Phys. Rev. Lett. 102, 117201 (2009) 10.1103/PhysRevLett.102.117201
-
(2009)
Phys. Rev. Lett.
, vol.102
, pp. 117201
-
-
Radu, I.1
Woltersdorf, G.2
Kiessling, M.3
Melnikov, A.4
Bovensiepen, U.5
Thiele, J.-U.6
Back, C.H.7
-
7
-
-
12944272136
-
-
10.1103/PhysRevLett.85.844;
-
B. Koopmans, M. van Kampen, J. T. Kohlhepp, and W. J. M. de Jonge, Phys. Rev. Lett. 85, 844 (2000) 10.1103/PhysRevLett.85.844
-
(2000)
Phys. Rev. Lett.
, vol.85
, pp. 844
-
-
Koopmans, B.1
Van Kampen, M.2
Kohlhepp, J.T.3
De Jonge, W.J.M.4
-
8
-
-
34848910821
-
-
10.1038/nmat1985;
-
C. Stamm, T. Kachel, N. Pontius, R. Mitzner, T. Quast, K. Holldack, S. Khan, C. Lupulescu, E. F. Aziz, M. Wietstruk, H. A. Dürr, and W. Eberhardt, Nature Mater. 6, 740 (2007) 10.1038/nmat1985
-
(2007)
Nature Mater.
, vol.6
, pp. 740
-
-
Stamm, C.1
Kachel, T.2
Pontius, N.3
Mitzner, R.4
Quast, T.5
Holldack, K.6
Khan, S.7
Lupulescu, C.8
Aziz, E.F.9
Wietstruk, M.10
Dürr, H.A.11
Eberhardt, W.12
-
9
-
-
57949098937
-
-
10.1038/nmat2341
-
G. M. Müller, J. Walowski, M. Djordjevic, G. X. Miao, A. Gupta, A. V. Ramos, K. Gehrke, V. Moshnyaga, K. Samwer, J. Schmalhorst, A. Thomas, A. Hütten, G. Reiss, J. S. Moodera, and M. Münzenberg, Nature Mater. 8, 56 (2009). 10.1038/nmat2341
-
(2009)
Nature Mater.
, vol.8
, pp. 56
-
-
Müller, G.M.1
Walowski, J.2
Djordjevic, M.3
Miao, G.X.4
Gupta, A.5
Ramos, A.V.6
Gehrke, K.7
Moshnyaga, V.8
Samwer, K.9
Schmalhorst, J.10
Thomas, A.11
Hütten, A.12
Reiss, G.13
Moodera, J.S.14
Münzenberg, M.15
-
10
-
-
0342918645
-
-
10.1103/PhysRevLett.85.3025;
-
G. P. Zhang and W. Hübner, Phys. Rev. Lett. 85, 3025 (2000) 10.1103/PhysRevLett.85.3025
-
(2000)
Phys. Rev. Lett.
, vol.85
, pp. 3025
-
-
Zhang, G.P.1
Hübner, W.2
-
11
-
-
0041111027
-
-
10.1103/PhysRevB.58.R5920;
-
W. Hübner and G. P. Zhang, Phys. Rev. B 58, R5920 (1998) 10.1103/PhysRevB.58.R5920
-
(1998)
Phys. Rev. B
, vol.58
, pp. 5920
-
-
Hübner, W.1
Zhang, G.P.2
-
14
-
-
28644439448
-
-
10.1103/PhysRevB.71.165108
-
A. Vernes and P. Weinberger, Phys. Rev. B 71, 165108 (2005). 10.1103/PhysRevB.71.165108
-
(2005)
Phys. Rev. B
, vol.71
, pp. 165108
-
-
Vernes, A.1
Weinberger, P.2
-
15
-
-
34547463502
-
-
10.1103/PhysRevLett.99.047601
-
C. D. Stanciu, F. Hansteen, A. V. Kimel, A. Kirilyuk, A. Tsukamoto, A. Itoh, and Th. Rasing, Phys. Rev. Lett. 99, 047601 (2007). 10.1103/PhysRevLett. 99.047601
-
(2007)
Phys. Rev. Lett.
, vol.99
, pp. 047601
-
-
Stanciu, C.D.1
Hansteen, F.2
Kimel, A.V.3
Kirilyuk, A.4
Tsukamoto, A.5
Itoh, A.6
Rasing, Th.7
-
17
-
-
67650799834
-
-
10.1038/nphys1315
-
G. P. Zhang, W. Hübner, G. Lefkidis, Y. Bai, and T. F. George, Nat. Phys. 5, 499 (2009). 10.1038/nphys1315
-
(2009)
Nat. Phys.
, vol.5
, pp. 499
-
-
Zhang, G.P.1
Hübner, W.2
Lefkidis, G.3
Bai, Y.4
George, T.F.5
-
18
-
-
65149102696
-
-
10.1103/PhysRevB.79.140401;
-
D. Steiauf and M. Fähnle, Phys. Rev. B 79, 140401 (R) (2009) 10.1103/PhysRevB.79.140401
-
(2009)
Phys. Rev. B
, vol.79
, pp. 140401
-
-
Steiauf, D.1
Fähnle, M.2
-
19
-
-
33746709694
-
-
10.1103/PhysRev.96.266;
-
R. J. Elliott, Phys. Rev. 96, 266 (1954) 10.1103/PhysRev.96.266
-
(1954)
Phys. Rev.
, vol.96
, pp. 266
-
-
Elliott, R.J.1
-
20
-
-
2842586600
-
-
10.1016/S0081-1947(08)60259-3
-
Y. Yafet, Solid State Phys. 14, 1 (1963) 10.1016/S0081-1947(08)60259-3
-
(1963)
Solid State Phys.
, vol.14
, pp. 1
-
-
Yafet, Y.1
-
21
-
-
0037433312
-
-
A paper by Koopmans suggests that the total amount of angular-momentum transfer is limited by the number of photons involved in the laser field. For details, see, 10.1088/0953-8984/15/5/324
-
A paper by Koopmans suggests that the total amount of angular-momentum transfer is limited by the number of photons involved in the laser field. For details, see B. Koopmans, M. van Kampen, and W. J. M. deJonge, J. Phys.: Condens. Matter 15, S723 (2003). 10.1088/0953-8984/15/5/324
-
(2003)
J. Phys.: Condens. Matter
, vol.15
, pp. 723
-
-
Koopmans, B.1
Van Kampen, M.2
Dejonge, W.J.M.3
-
23
-
-
55749086225
-
-
10.1103/PhysRevLett.101.187203
-
G. P. Zhang, Phys. Rev. Lett. 101, 187203 (2008). 10.1103/PhysRevLett. 101.187203
-
(2008)
Phys. Rev. Lett.
, vol.101
, pp. 187203
-
-
Zhang, G.P.1
-
24
-
-
50449103121
-
-
10.1103/PhysRevB.78.052407
-
G. P. Zhang and T. F. George, Phys. Rev. B 78, 052407 (2008). 10.1103/PhysRevB.78.052407
-
(2008)
Phys. Rev. B
, vol.78
, pp. 052407
-
-
Zhang, G.P.1
George, T.F.2
-
26
-
-
49249109521
-
-
10.1103/PhysRevLett.101.066402
-
M. Pickel, A. B. Schmidt, F. Giesen, J. Braun, J. Minár, H. Ebert, M. Donath, and M. Weinelt, Phys. Rev. Lett. 101, 066402 (2008). 10.1103/PhysRevLett.101.066402
-
(2008)
Phys. Rev. Lett.
, vol.101
, pp. 066402
-
-
Pickel, M.1
Schmidt, A.B.2
Giesen, F.3
Braun, J.4
Minár, J.5
Ebert, H.6
Donath, M.7
Weinelt, M.8
-
27
-
-
0036496827
-
-
10.1103/PhysRevB.65.104429
-
T. Kampfrath, R. G. Ulbrich, F. Leuenberger, M. Münzenberg, B. Sass, and W. Felsch, Phys. Rev. B 65, 104429 (2002). 10.1103/PhysRevB.65.104429
-
(2002)
Phys. Rev. B
, vol.65
, pp. 104429
-
-
Kampfrath, T.1
Ulbrich, R.G.2
Leuenberger, F.3
Münzenberg, M.4
Sass, B.5
Felsch, W.6
-
28
-
-
0003930336
-
-
One should not confuse the variational method with perturbation theory. See the variational method in, Dover, New York
-
One should not confuse the variational method with perturbation theory. See the variational method in A. Messiah, Quantum Mechanics (Dover, New York, 1999), Chap. No., p. 762; see the perturbation method in Chapters XVI and XVII in the same book.
-
(1999)
Quantum Mechanics
, pp. 762
-
-
Messiah, A.1
-
29
-
-
0003417617
-
-
Karlheinz Schwarz, Technische Universität Wien, Austria
-
P. Blaha, K. Schwarz, G. K. H. Madsen, D. Kvasnicka, and J. Luitz, WIEN2K, An Augmented Plane Wave Plus Local Orbitals Program for Calculating Crystal Properties (Karlheinz Schwarz, Technische Universität Wien, Austria, 2001).
-
(2001)
WIEN2K, An Augmented Plane Wave Plus Local Orbitals Program for Calculating Crystal Properties
-
-
Blaha, P.1
Schwarz, K.2
Madsen, G.K.H.3
Kvasnicka, D.4
Luitz, J.5
-
30
-
-
65249183481
-
-
10.1063/1.3058704;
-
T. Hartenstein, G. Lefkidis, W. Hübner, G. P. Zhang, and Y. Bai, J. Appl. Phys. 105, 07D305 (2009) 10.1063/1.3058704
-
(2009)
J. Appl. Phys.
, vol.105
-
-
Hartenstein, T.1
Lefkidis, G.2
Hübner, W.3
Zhang, G.P.4
Bai, Y.5
-
31
-
-
42149139142
-
-
10.1063/1.2837248
-
G. P. Zhang, Y. Bai, W. Hübner, G. Lefkidis, and T. F. George, J. Appl. Phys. 103, 07B113 (2008). 10.1063/1.2837248
-
(2008)
J. Appl. Phys.
, vol.103
-
-
Zhang, G.P.1
Bai, Y.2
Hübner, W.3
Lefkidis, G.4
George, T.F.5
-
32
-
-
0034664595
-
-
For other methods to compute the dipole transition matrix in solids, please refer to, 10.1103/PhysRevB.62.7998;
-
For other methods to compute the dipole transition matrix in solids, please refer to G. F. Bertsch, J.-I. Iwata, A. Rubio, and K. Yabana, Phys. Rev. B 62, 7998 (2000) 10.1103/PhysRevB.62.7998
-
(2000)
Phys. Rev. B
, vol.62
, pp. 7998
-
-
Bertsch, G.F.1
Iwata, J.-I.2
Rubio, A.3
Yabana, K.4
-
33
-
-
34547607921
-
-
in edited by K. M. Rabe, C. H. Ahn, and J.-M. Triscone (Springer-Verlag, Berlin, 10.1007/978-3-540-34591-6-2;
-
R. Resta and D. Vanderbilt, in Physics of Ferroelectrics: a Modern Perspective, edited by, K. M. Rabe,,, C. H. Ahn,, and, J.-M. Triscone, (Springer-Verlag, Berlin, 2007), pp. 31-68 10.1007/978-3-540-34591-6-2
-
(2007)
Physics of Ferroelectrics: A Modern Perspective
, pp. 31-68
-
-
Resta, R.1
Vanderbilt, D.2
-
35
-
-
0001462282
-
-
10.1103/PhysRevLett.80.1800
-
R. Resta, Phys. Rev. Lett. 80, 1800 (1998). 10.1103/PhysRevLett.80.1800
-
(1998)
Phys. Rev. Lett.
, vol.80
, pp. 1800
-
-
Resta, R.1
-
38
-
-
0001235317
-
-
We have not included the relativistic corrections in the momentum operator as Wang and Callaway have already pointed out that the matrix element is small [, 10.1103/PhysRevB.9.4897
-
We have not included the relativistic corrections in the momentum operator as Wang and Callaway have already pointed out that the matrix element is small [C. S. Wang and J. Callaway, Phys. Rev. B 9, 4897 (1974)]. 10.1103/PhysRevB.9.4897
-
(1974)
Phys. Rev. B
, vol.9
, pp. 4897
-
-
Wang, C.S.1
Callaway, J.2
-
39
-
-
77954740389
-
-
Note that the coefficients are spin-orbit coupling dependent. As a result, the transition-matrix element contains the mixed spin-up and spin-down components. One should not confuse the following three matrices: (a) the matrix formed within the LAPW basis, (b) the matrix formed within the spin-polarized basis, and (c) the matrix formed within the spin-polarized basis with the presence of spin-orbit coupling
-
Note that the coefficients are spin-orbit coupling dependent. As a result, the transition-matrix element contains the mixed spin-up and spin-down components. One should not confuse the following three matrices: (a) the matrix formed within the LAPW basis, (b) the matrix formed within the spin-polarized basis, and (c) the matrix formed within the spin-polarized basis with the presence of spin-orbit coupling.
-
-
-
-
40
-
-
77954706526
-
-
There is no intrinsic limitation in our scheme. As far as the DFT works, the scheme will work. If the laser is too strong and melts the sample then our scheme will break down as does the experimental one. We only consider the electron dynamics and work on the time scale of several hundred femtoseconds before the phonon is strongly activated. We can not use temperature concept during the laser excitation: temperature is a statistical concept and should not be used within a few hundred fs
-
There is no intrinsic limitation in our scheme. As far as the DFT works, the scheme will work. If the laser is too strong and melts the sample then our scheme will break down as does the experimental one. We only consider the electron dynamics and work on the time scale of several hundred femtoseconds before the phonon is strongly activated. We can not use temperature concept during the laser excitation: temperature is a statistical concept and should not be used within a few hundred fs.
-
-
-
-
41
-
-
77954736584
-
-
The small magnetization change is due to a weak laser field used in our simulation. If we use a strong laser, the demagnetization will of course be larger. There are two reasons why we choose a weak laser. First, when excited with a weak laser field, all the states, that make substantial magnetic contribution will make substantial contributions to the magnetic changes when the laser field becomes strong. But the other way around is not necessarily true. We use linearly polarized light in the present work. In metals, polarity does not play a big role since the orbital moment is small. Since our sample is a metal, there is no big effect on the results, which is already known from experiments. The laser affects the system through the second term as explained in our paper (Ref.)
-
The small magnetization change is due to a weak laser field used in our simulation. If we use a strong laser, the demagnetization will of course be larger. There are two reasons why we choose a weak laser. First, when excited with a weak laser field, all the states, that make substantial magnetic contribution will make substantial contributions to the magnetic changes when the laser field becomes strong. But the other way around is not necessarily true. We use linearly polarized light in the present work. In metals, polarity does not play a big role since the orbital moment is small. Since our sample is a metal, there is no big effect on the results, which is already known from experiments. The laser affects the system through the second term as explained in our paper (Ref.).
-
-
-
|