| Zugriffsnummer | 37640 |
| Dokumenttyp | Zeitschriftenartikel |
| Sprache | Englisch |
| Titel | Generalized complex Swift-Hohenberg equation for optical parametric oscillators parametric oscillators |
| Autor(in); Institution |
S.aacute.nchez-Morcillo, Víctor J.; Departament d’Òptica, Universitat de València, Burjassot, SPAIN
Rold.aacute.n, Eugenio; Departament d’Òptica, Universitat de València, Burjassot, SPAIN
Valc.aacute.rcel, Germ.aacute.n J. de; Departament d’Òptica, Universitat de València, Burjassot, SPAIN
Staliunas, Kestutis; 4.33, Zeit- und Frequenzübertragung, PTB-Braunschweig
|
| Quelle/Jahr | Physical Review A: 56 (1997), 4, 3237 - 3244 |
| ISSN | 1050-2947 (PRINT) ; 1094-1622 (ONLINE) |
| DOI | |
| Verlag | College Park, Md.: American Physical Society |
| Klassifikationscode | PACS: 42.65.Sf ; PACS: 42.65.Yj ; PACS: 47.32.Cc |
| Zusammenfassung | A generalized complex Swift-Hohenberg equation including diffraction and nonlinear resonance terms is derived for spatially extended nondegenerate optical parametric oscillators (OPOs) with flat end mirrors. For vanishing pump detuning this equation becomes the complex Swift-Hohenberg (SH) equation valid also for lasers. Nevertheless the similarities between OPOs and lasers are limited, since the diffractive character of OPOs is lost when the diffraction coefficients of signal and idler fields are equal. This manifests, e.g., in the absence of advection by traveling waves (TWs), a clear difference with lasers. When pump detuning is nonzero a nonlinear resonance develops, as it occurs in degenerate OPOs. This nonlinear resonance is essential in order to properly describe the TWs that OPOs support, and describes the bistability between TWs. This leads to the appearance of localized structures, which we also report here. |
Zitierung
S.aacute.nchez-Morcillo, V. J., Rold.aacute.n, E., Valc.aacute.rcel, G. J. D., & Staliunas, K. (1997). Generalized complex Swift-Hohenberg equation for optical parametric oscillators parametric oscillators. Physical Review A, 56(4), 3237–3244. http://doi.org/10.1103/physreva.56.3237