-
1
-
-
3442881546
-
-
10.1103/PhysRevLett.53.2449
-
G. W. Semenoff, Phys. Rev. Lett. 53, 2449 (1984). 10.1103/PhysRevLett.53. 2449
-
(1984)
Phys. Rev. Lett.
, vol.53
, pp. 2449
-
-
Semenoff, G.W.1
-
2
-
-
39649102203
-
-
Springer, Berlin
-
A. Jorio, G. Dresselhaus, and M. S. Dresselhaus, Carbon Nanotubes: Advanced Topics in the Synthesis, Structure, Properties, and Applications (Springer, Berlin, 2008).
-
(2008)
Carbon Nanotubes: Advanced Topics in the Synthesis, Structure, Properties, and Applications
-
-
Jorio, A.1
Dresselhaus, G.2
Dresselhaus, M.S.3
-
4
-
-
59949098337
-
-
10.1103/RevModPhys.81.109
-
A. H. Castro Neto, Rev. Mod. Phys. 81, 109 (2009). 10.1103/RevModPhys.81. 109
-
(2009)
Rev. Mod. Phys.
, vol.81
, pp. 109
-
-
Castro Neto, A.H.1
-
5
-
-
1642407592
-
-
10.1016/j.cplett.2004.02.034
-
A. Grüneis, Chem. Phys. Lett. 387, 301 (2004). 10.1016/j.cplett. 2004.02.034
-
(2004)
Chem. Phys. Lett.
, vol.387
, pp. 301
-
-
Grüneis, A.1
-
8
-
-
4043108064
-
-
10.1103/PhysRevB.66.035412
-
S. Reich, Phys. Rev. B 66, 035412 (2002). 10.1103/PhysRevB.66.035412
-
(2002)
Phys. Rev. B
, vol.66
, pp. 035412
-
-
Reich, S.1
-
9
-
-
0000234091
-
-
10.1103/PhysRevB.60.13339
-
S. Kazaoui, Phys. Rev. B 60, 13339 (1999). 10.1103/PhysRevB.60.13339
-
(1999)
Phys. Rev. B
, vol.60
, pp. 13339
-
-
Kazaoui, S.1
-
10
-
-
70249110391
-
-
10.1126/science.1176112
-
N. M. Gabor, Science 325, 1367 (2009). 10.1126/science.1176112
-
(2009)
Science
, vol.325
, pp. 1367
-
-
Gabor, N.M.1
-
11
-
-
0031504972
-
-
10.1143/JPSJ.66.1066
-
T. Ando, J. Phys. Soc. Jpn. 66, 1066 (1997). 10.1143/JPSJ.66.1066
-
(1997)
J. Phys. Soc. Jpn.
, vol.66
, pp. 1066
-
-
Ando, T.1
-
13
-
-
1642585814
-
-
10.1103/PhysRevLett.92.077402
-
C. D. Spataru, Phys. Rev. Lett. 92, 077402 (2004). 10.1103/PhysRevLett. 92.077402
-
(2004)
Phys. Rev. Lett.
, vol.92
, pp. 077402
-
-
Spataru, C.D.1
-
14
-
-
18244392180
-
-
10.1126/science.1110265
-
F. Wang, Science 308, 838 (2005). 10.1126/science.1110265
-
(2005)
Science
, vol.308
, pp. 838
-
-
Wang, F.1
-
15
-
-
19644401335
-
-
10.1103/PhysRevLett.93.157402
-
H. Zhao and S. Mazumdar, Phys. Rev. Lett. 93, 157402 (2004). 10.1103/PhysRevLett.93.157402
-
(2004)
Phys. Rev. Lett.
, vol.93
, pp. 157402
-
-
Zhao, H.1
Mazumdar, S.2
-
16
-
-
33749650943
-
-
10.1103/PhysRevB.74.155411
-
S. Uryu and T. Ando, Phys. Rev. B 74, 155411 (2006). 10.1103/PhysRevB.74. 155411
-
(2006)
Phys. Rev. B
, vol.74
, pp. 155411
-
-
Uryu, S.1
Ando, T.2
-
18
-
-
34547562388
-
-
10.1021/nl070260f
-
J. Shaver, Nano Lett. 7, 1851 (2007). 10.1021/nl070260f
-
(2007)
Nano Lett.
, vol.7
, pp. 1851
-
-
Shaver, J.1
-
19
-
-
50249123415
-
-
10.1103/PhysRevLett.101.087402
-
A. Srivastava, Phys. Rev. Lett. 101, 087402 (2008). 10.1103/PhysRevLett. 101.087402
-
(2008)
Phys. Rev. Lett.
, vol.101
, pp. 087402
-
-
Srivastava, A.1
-
21
-
-
15544375926
-
-
10.1126/science.1072631
-
M. J. O'Connell, Science 297, 593 (2002). 10.1126/science.1072631
-
(2002)
Science
, vol.297
, pp. 593
-
-
O'Connell, M.J.1
-
24
-
-
77955161606
-
-
The theoretical value of r|| for randomly oriented dipoles is 0.4, while some possible processes such as light scattering or exciton migration could be expected to reduce the anisotropy in the real case. To take these effects into account, we assigned the maximum value of observed anisotropy in lower-energy range near E11 to r||
-
The theoretical value of r || for randomly oriented dipoles is 0.4, while some possible processes such as light scattering or exciton migration could be expected to reduce the anisotropy in the real case. To take these effects into account, we assigned the maximum value of observed anisotropy in lower-energy range near E 11 to r ||.
-
-
-
-
25
-
-
34247403724
-
-
10.1103/PhysRevLett.98.167406
-
J. Lefebvre and P. Finnie, Phys. Rev. Lett. 98, 167406 (2007). 10.1103/PhysRevLett.98.167406
-
(2007)
Phys. Rev. Lett.
, vol.98
, pp. 167406
-
-
Lefebvre, J.1
Finnie, P.2
-
26
-
-
0037147175
-
-
10.1126/science.1078727
-
S. M. Bachilo, Science 298, 2361 (2002). 10.1126/science.1078727
-
(2002)
Science
, vol.298
, pp. 2361
-
-
Bachilo, S.M.1
-
27
-
-
77955132362
-
-
Since (8, 6) and (12, 1) SWNTs have almost the same E11, one cannot distinguish ET (-) of both species only from the PL and PLE spectra. We assigned ET (-) of them so that ET (-), ΔT, peak widths and the intensity ratio in Fig. are along with the tendency (family pattern) of other chiral indices
-
Since (8, 6) and (12, 1) SWNTs have almost the same E 11, one cannot distinguish E T (-) of both species only from the PL and PLE spectra. We assigned E T (-) of them so that E T (-), Δ T, peak widths and the intensity ratio in Fig. are along with the tendency (family pattern) of other chiral indices.
-
-
-
-
28
-
-
34648825474
-
-
10.1103/PhysRevB.76.115420
-
S. Uryu and T. Ando, Phys. Rev. B 76, 115420 (2007). 10.1103/PhysRevB.76. 115420
-
(2007)
Phys. Rev. B
, vol.76
, pp. 115420
-
-
Uryu, S.1
Ando, T.2
-
29
-
-
70349690185
-
-
10.1143/JPSJ.78.104703
-
T. Ando, J. Phys. Soc. Jpn. 78, 104703 (2009). 10.1143/JPSJ.78.104703
-
(2009)
J. Phys. Soc. Jpn.
, vol.78
, pp. 104703
-
-
Ando, T.1
|