Precision dispersion compensation for ultra-broadband bi-photons using a prism-pair with negative separation
Yaakov Shaked, Shai Yefet, Avi Pe
The Brewster prism-pair is a major tool for dispersion control that produces tuned negative dispersion even when the prisms material has positive dispersion. We present a complementary technique for obtaining overall positive dispersion even when the material dispersion is negative, which is most useful for applications in the infrared, where the majority of the optical materials have negative dispersion. By adding a telescope between the prisms that images the first prism beyond the location of the second one, an effectively negative separation between the prisms can be obtained. This ability to flip the sign of the angular dispersion between the prisms provides a powerful new knob to the prism-pair system and allows higher degree of dispersion compensation. We demonstrate a prism-pair configuration, where both the 2nd and 4th order dispersion are compensated in the 1400-2400nm range, designed for a quantum optics experiment with ultra-broadband bi-photons. c 2014 Optical Society of America OCIS codes: 140.7090, 230.5480 Since the introduction of the Brewster prism-pair as a mechanism for dispersion control [1], it became a major tool for tuned dispersion compensation in ultrafast optical systems. Specifically, a prism-pair is commonly used to compensate for second-order dispersion (group delay dispersion - GDD). The angular dispersion that is created by the separation between the prisms tips always introduces negative GDD, even when the prisms material produces positive GDD. Thus, any negative dispersion can be achieved by the appropriate separation between the prisms; and tuned dispersion can be achieved by controlling the amount of prism material in the beam.
•Mar 10, 2014•0 citations