Optical third-harmonic generation using ultrashort laser pulses
Journal Article
·
· Physical Review. A
- Department of Physics, University of Texas at Austin, 1 University Station C1600, Austin, Texas 78712-0264 (United States)
- Center for Nano and Molecular Science and Technology and Texas Materials Institute, University of Texas at Austin, Building ETC, Room 8.102, Campus Mail Code C2201, Austin, Texas 78712-1063 (United States)
To better predict optical third-harmonic generation (THG) in transparent dielectrics, we model a typical ultrashort pulsed Gaussian beam, including both group velocity mismatch and phase mismatch of the fundamental and harmonic fields. We find that competition between the group velocity mismatch and phase mismatch leads to third-harmonic generation that is sensitive only to interfaces. In this case, the spatial resolution is determined by the group velocity walk-off length. THG of modern femtosecond lasers in optical solids is a bulk process, without a surface susceptibility, but bears the signature of a surface enhancement effect in z-scan measurements. We demonstrate the accuracy of the model, by showing the agreement between the predicted spectral intensity and the measured third-harmonic spectrum from a thin sapphire crystal.
- OSTI ID:
- 20717857
- Journal Information:
- Physical Review. A, Journal Name: Physical Review. A Journal Issue: 6 Vol. 71; ISSN 1050-2947; ISSN PLRAAN
- Country of Publication:
- United States
- Language:
- English
Similar Records
Third-harmonic generation from a simple air-dielectric interface
Optical third-harmonic generation at interfaces
Pulse shaping and processing by cascaded third-harmonic generation in quasiperiodic optical superlattices
Conference
·
Sat Dec 30 23:00:00 EST 1995
·
OSTI ID:437551
Optical third-harmonic generation at interfaces
Journal Article
·
Tue Oct 31 23:00:00 EST 1995
· Physical Review A
·
OSTI ID:147639
Pulse shaping and processing by cascaded third-harmonic generation in quasiperiodic optical superlattices
Journal Article
·
Fri Oct 01 00:00:00 EDT 2004
· Physical Review. A
·
OSTI ID:20646456