“…For odd CNTs, increasing the diameter decreases the difference energy positions and a broadened peak is observed instead of two distinct peaks. For example, in (12,1) CNT, these peaks are located at energies 3.88 eV and 3.93 eV and they move to 3.87 eV and 3.89 eV in (12,11) CNT. We reached two main conclusions from our observation.…”
Section: Optical Propertiesmentioning
confidence: 99%
“…Increasing the distance between them is due to the increasing of the magnetic field. Figure 9 shows optical spectra for (10,3), (11,1) and (12,2) CNTs in different axial magnetic fields (up to 200 T) in the infrared region, respectively. Their spectra do not show clear splitting below the 30 T, while at higher magnetic fields above 30 T, each peak is divided into two distinct peaks (e.g., peaks E 11+ and E 11À ) with the splitting energy DE ð1Þ ¼ E cv 11þ À E cv 11À .…”
Section: Optical Propertiesmentioning
confidence: 99%
“…This is in agreement with previous theoretical and experimental studies. 21 (8,7), (10,6), (11,1), (10,3), (12,2) and (11,4) CNTs is 6, 5.9, 5.7, 5.77, 5.75 and 5.82, respectively. which is in agreement with previous studies.…”
Section: Optical Propertiesmentioning
confidence: 99%
“…5,6 By adding other parameters such as next-neighbor hopping integral, overlap and on-site energy, the 1NN-TB model can be completed and the values obtained from this model will be improved for graphene and CNTs. 4,[7][8][9][10][11][12] To calculate the optical properties of CNTs, the electronic transitions between VHSs in the DOS should be determined. 13 Semiconducting SWCNTs are already candidates for photovoltaic applications, 14 opto-electronics 15 and molecular electronics.…”
We have applied a third nearest-neighbor tight binding model to investigate the optical properties of CNTs in terms of radius, chirality and magnetic field. The optical spectrum of CNTs depends strongly on the radius and chirality in the infrared region in contrast to the middle energy region. The dependence of E 22 /E 11 on the radius and chirality from optical peak positions and band structure is similar. In the infrared region, by applying the magnetic field, the optical peak splitting rates show well-expressed radius and chirality dependence and family behaviors.
“…For odd CNTs, increasing the diameter decreases the difference energy positions and a broadened peak is observed instead of two distinct peaks. For example, in (12,1) CNT, these peaks are located at energies 3.88 eV and 3.93 eV and they move to 3.87 eV and 3.89 eV in (12,11) CNT. We reached two main conclusions from our observation.…”
Section: Optical Propertiesmentioning
confidence: 99%
“…Increasing the distance between them is due to the increasing of the magnetic field. Figure 9 shows optical spectra for (10,3), (11,1) and (12,2) CNTs in different axial magnetic fields (up to 200 T) in the infrared region, respectively. Their spectra do not show clear splitting below the 30 T, while at higher magnetic fields above 30 T, each peak is divided into two distinct peaks (e.g., peaks E 11+ and E 11À ) with the splitting energy DE ð1Þ ¼ E cv 11þ À E cv 11À .…”
Section: Optical Propertiesmentioning
confidence: 99%
“…This is in agreement with previous theoretical and experimental studies. 21 (8,7), (10,6), (11,1), (10,3), (12,2) and (11,4) CNTs is 6, 5.9, 5.7, 5.77, 5.75 and 5.82, respectively. which is in agreement with previous studies.…”
Section: Optical Propertiesmentioning
confidence: 99%
“…5,6 By adding other parameters such as next-neighbor hopping integral, overlap and on-site energy, the 1NN-TB model can be completed and the values obtained from this model will be improved for graphene and CNTs. 4,[7][8][9][10][11][12] To calculate the optical properties of CNTs, the electronic transitions between VHSs in the DOS should be determined. 13 Semiconducting SWCNTs are already candidates for photovoltaic applications, 14 opto-electronics 15 and molecular electronics.…”
We have applied a third nearest-neighbor tight binding model to investigate the optical properties of CNTs in terms of radius, chirality and magnetic field. The optical spectrum of CNTs depends strongly on the radius and chirality in the infrared region in contrast to the middle energy region. The dependence of E 22 /E 11 on the radius and chirality from optical peak positions and band structure is similar. In the infrared region, by applying the magnetic field, the optical peak splitting rates show well-expressed radius and chirality dependence and family behaviors.
“…However, first principle and numerical tight-binding calculations show that only armchair CNTs (n = m) are truly metallic. [19][20][21] All other tubes from the specified category have a small curvature-induced band gap that ranges from ≈ 2 − 50 meV depending on the tube diameter and chirality.…”
Interband transitions in narrow-gap carbon nanotubes and graphene nanoribbons We use the robust nearest-neighbour tight-binding approximation to study on the same footing interband dipole transitions in narrow-bandgap carbon nanotubes and graphene nanoribbons. It is demonstrated that curvature effects in metallic singlewalled carbon nanotubes and edge effects in gapless graphene nanoribbons not only open up bang gaps, which typically correspond to THz frequencies, but also result in a giant enhancement of the probability of optical transitions across these gaps. Moreover, the matrix element of the velocity operator for these transitions has a universal value (equal to the Fermi velocity in graphene) when the photon energy coincides with the band-gap energy. Upon increasing the excitation energy, the transition matrix element first rapidly decreases (for photon energies remaining in the THz range but exceeding two band gap energies it is reduced by three orders of magnitude), and thereafter it starts to increase proportionally to the photon frequency. A similar effect occurs in an armchair carbon nanotube with a band gap opened and controlled by a magnetic field applied along the nanotube axis. There is a direct correspondence between armchair graphene nanoribbons and single-walled zigzag carbon nanotubes. The described sharp photon-energy dependence of the transition matrix element together with the van Hove singularity at the band gap edge of the considered quasi-one-dimensional systems make them promising candidates for active elements of coherent THz radiation emitters. The effect of Pauli blocking of low-energy interband transitions caused by residual doping can be suppressed by creating a population inversion using high-frequency (optical) excitation.
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