Zobrazeno 1 - 5
of 5
pro vyhledávání: '"G. C. Catella"'
Autor:
G. C. Catella, Robert S. Feigelson, D. Perlov, Larry E. Halliburton, Wei Hong, K. T. Stevens, Roger K. Route
Publikováno v:
Journal of Applied Physics. 94:2510-2515
Electron paramagnetic resonance (EPR) has been used to investigate point defects in single crystals of β-BaB2O4 (commonly referred to as BBO). An irradiation with x rays at 77 K produces two dominant EPR spectra, one electronlike and the other holel
Autor:
M. Yan, Natalia Zaitseva, K. T. Stevens, N. Y. Garces, G. C. Catella, J. J. DeYoreo, Larry E. Halliburton, J. R. Luken
Publikováno v:
Applied Physics Letters. 75:1503-1505
The intrinsic “self-trapped” hole center in KD2PO4 crystals has been identified using electron paramagnetic resonance and electron-nuclear double resonance. These defects, labeled [D2PO4]o centers, can be formed at 77 K by irradiating with either
Autor:
C. L. Marquardt, D. G. Cooper, P. A. Budni, M. G. Knights, K. L. Schepler, R. DeDomenico, G. C. Catella
Publikováno v:
Optical Society of America Annual Meeting.
The 2-μm pumped AgGaSe2 OPO is currently limited to outputs below 1 W and pulse recognition frequencies of a few kilohertz, apparently because of thermal lensing. Conflicting values for K and dn/dT and the lack of accurate 2-μm absorption data have
Autor:
D G Cooper, Roger K. Route, L R Shiozawa, G. C. Catella, R. C. Eckardt, J R Hietanen, Robert S. Feigelson, Charles L. Marquardt
Publikováno v:
Applied Optics. 32:3948
We report new experimental results on the spectral, thermal, and orientational characteristics of stoichiometry-dependent mid-IR absorption in AgGaSe(2) crystals. In currently available material, this absorption poses an obstacle to the power scaling
Autor:
S. Velsko, G. C. Kennedy, Leslie F. Warren, G. C. Catella, Christopher A. Ebbers, Mark S. Webb, Henry O. Marcy
Publikováno v:
Applied Optics. 31:5051
The linear and second-order nonlinear optical properties of single-crystal zinc tris(thiourea) sulfate, or ZTS, are determined. The deduced nonlinear coefficients are |d(31)| = 0.31, |d(32)| = 0.35, and |d(33)| = 0.23 pm/V compared with a |d(14)| val