| Literature DB >> 28273922 |
Hui Xiong1, Benoit Mignolet2, Li Fang3, Timur Osipov4, Thomas J A Wolf5, Emily Sistrunk5,6, Markus Gühr5,7, Francoise Remacle2, Nora Berrah8.
Abstract
The interaction of gas phase endohedral fullerene Ho3N@C80 with intense (0.1-5 × 1014 W/cm2), short (30 fs), 800 nm laser pulses was investigated. The power law dependence of Ho3N@C80q+, q = 1-2, was found to be different from that of C60. Time-dependent density functional theory computations revealed different light-induced ionization mechanisms. Unlike in C60, in doped fullerenes, the breaking of the cage spherical symmetry makes super atomic molecular orbital (SAMO) states optically active. Theoretical calculations suggest that the fast ionization of the SAMO states in Ho3N@C80 is responsible for the n = 3 power law for singly charged parent molecules at intensities lower than 1.2 × 1014 W/cm2.Entities:
Year: 2017 PMID: 28273922 PMCID: PMC5427842 DOI: 10.1038/s41598-017-00124-9
Source DB: PubMed Journal: Sci Rep ISSN: 2045-2322 Impact factor: 4.379
Figure 1Mass/charge spectra of Ho3N@C80 ionized with laser pulses of 800 nm, 30 fs pulse duration and an intensity of 4 × 1014 W/cm2.
Figure 2Comparison of the ion yield dependence on peak intensity for the ionization of Ho3N@C80 q+ (q = 1, 2) (filled symbols) and C60 q+ (q = 1, 2) (open symbols). The Ho3N@C80 q+ results are extracted from data in Fig. 1 and the yields of Ho3N@C80 with a charge q = 1 is multiplied by 5. The C60 data are from ref. 40 and the C60 + yield was multiplied by 2 for clarity.
Measured power laws for HoN3@C80 and for C60 [40] ion charge states.
| Charge state q | q = 1+ | q = 2+ |
|---|---|---|
| C60 | 5 | 8 |
| Ho3N@C80 | 3.0 (±0.1) | 5.7 (±0.5) |
Figure 3(a) Dyson orbitals of a typical valence state, s SAMO, p SAMO and d SAMO states of Ho3N@C80 with an isocontour of 0.002|e|/Å. (b) Charge density of the Dyson orbitals of panel a. (c) Density of SAMO states as a function of the excitation energy. The electronic states and Dyson orbitals have been computed in TDDFT at the LC-BLYP/6–31G(d) + ECP56MWB/7s6p5d for Ho + Bq (6–31(6+)G(d)) level for Ho3N@C80’s lowest energy isomer shown in the inset.
Computed binding energies, photoionization lifetimes (in fs) for a field intensity of 1013 and 1014 W/cm2 and transition dipole moments (μtrans) between the ground and excited states shown in Fig. 3.
| Excitation energy(eV) | Photoionization lifetime (fs) | μtrans (au) | ||||
|---|---|---|---|---|---|---|
| 1013 W/cm2 | 1014 W/cm2 | Ho3N@C80 | C60 | C80 | ||
| Valence (ES 67) | 4.25 | 351.03 | 39.00 | 1.19 | 1.55 | 1.47 |
|
| 4.98 | 2.00 | 0.22 | 0.66 | 0.00 | 0.02 |
|
| 5.23 | 1.49 | 0.13 | 0.69 | 0.00 | 0.30 |
|
| 5.60 | 1.56 | 0.17 | 0.49 | 0.00 | 0.29 |
The photoionization lifetimes are computed for the ionization of an electron with a kinetic energy of 0.2 eV. For comparison, the computed transition dipole moments of the valence (with an excitation energy around 4.25 eV), s, p and d SAMO states are also given for C60 and C80.
Figure 4Photoionization lifetime (field intensity of 1013 W/cm2) for a set of representative SAMO and valence states, plotted as a function of the kinetic energy of electron ionized from the SAMO or valence states. Amongst the valence states, some are isoenergetic with the SAMO states (see S.I. for details).