Broadband Photoconductive Sampling in Gallium Phosphide
Source abstract
Abstract
Abstract Direct measurements of the electric field of light enable new observations of light–matter interactions. In the near‐infrared and visible spectral ranges, this typically relies on techniques that exploit nonlinearities in gases or solids, which limits their sensitivity. Here, a method for the detection of broadband near‐infrared fields spanning more than one octave from 110 to 220 THz based on linear absorption in a semiconductor is demonstrated. This technique, which avoids complex vacuum setups and works under ambient conditions, employs linear photoconductive sampling (LPS) in gallium phosphide. Simulations reveal that the response function of LPS is concerned with the intensity envelope of the gate field, in contrast to electro‐optic sampling, relaxing the stringent temporal requirements on the gate pulse.
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Research context
OpenAlex topics: Terahertz technology and applications · Laser-Matter Interactions and Applications · Spectroscopy Techniques in Biomedical and Chemical Research
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Division of Attosecond Physics Max Planck Institute of Quantum Optics 85748 Garching Germany
Department of Physics Ludwig‐Maximilians‐Universität 85748 Garching Germany
PULSE Institute SLAC National Accelerator Laboratory Menlo Park CA 94025 USA
Applied Physics Department Stanford University Stanford CA 94305 USA
Funding
H2020 European Research Council · Deutsche Forschungsgemeinschaft · Air Force Office of Scientific Research · U.S. Department of Energy · Office of Science
References (42)
Show source-provided references
1. 10.1038/nature1765010.1038/nature17650 ↗
2. 10.1103/RevModPhys.81.16310.1103/RevModPhys.81.163 ↗
3. 10.1038/nature0227710.1038/nature02277 ↗
4. 10.1126/science.114285510.1126/science.1142855 ↗
5. 10.1038/nature0622910.1038/nature06229 ↗
6. 10.1038/nature1172010.1038/nature11720 ↗
7. 10.1038/s41586-019-1333-x10.1038/s41586-019-1333-x ↗
8. 10.1103/PhysRevLett.117.09300110.1103/PhysRevLett.117.093001 ↗
9. 10.1126/science.aao473110.1126/science.aao4731 ↗
10. 10.1038/s41567-020-0887-810.1038/s41567-020-0887-8 ↗
11. 10.1038/nphys412910.1038/nphys4129 ↗
12. 10.1126/science.abb097910.1126/science.abb0979 ↗
13. 10.2533/chimia.2022.52010.2533/chimia.2022.520 ↗
14. 10.1063/1.9348510.1063/1.93485 ↗
15. 10.1063/1.180823210.1063/1.1808232 ↗
16. 10.1063/1.12360110.1063/1.123601 ↗
17. 10.1038/nphoton.2015.26910.1038/nphoton.2015.269 ↗
18. 10.1038/s41467-022-28699-610.1038/s41467-022-28699-6 ↗
19. 10.1038/s41467-019-14268-x10.1038/s41467-019-14268-x ↗
20. 10.1364/OPTICA.5.00040210.1364/OPTICA.5.000402 ↗
21. 10.1364/PRJ.42091610.1364/PRJ.420916 ↗
22. 10.1038/s41566-021-00924-610.1038/s41566-021-00924-6 ↗
23. 10.1038/s41566-021-00792-010.1038/s41566-021-00792-0 ↗
24. 10.1364/OPTICA.45961210.1364/OPTICA.459612 ↗
25. 10.1364/OPTICA.39884610.1364/OPTICA.398846 ↗
26. 10.1364/OPTICA.41143410.1364/OPTICA.411434 ↗
27. 10.1063/1.8807910.1063/1.88079 ↗
28. 10.1364/AO.36.00785310.1364/AO.36.007853 ↗
29. 10.1063/1.176831310.1063/1.1768313 ↗
30. 10.1049/ip-opt:2002026210.1049/ip-opt:20020262 ↗
31. 10.1143/JJAP.47.822110.1143/JJAP.47.8221 ↗
32. 10.1038/s41467-022-29252-110.1038/s41467-022-29252-1 ↗
33. 10.1007/BF0133945510.1007/BF01339455 ↗
34. 10.1364/OPTICA.39526510.1364/OPTICA.395265 ↗
35. 10.1103/PhysRev.134.A162810.1103/PhysRev.134.A1628 ↗
36. 10.1103/PhysRevLett.127.08740110.1103/PhysRevLett.127.087401 ↗
37. Keldysh L. V. · J. Exp. Theor. Phys. · 1965 · 20 · 1307
38. 10.1103/PhysRevLett.78.328210.1103/PhysRevLett.78.3282 ↗
39. 10.1103/PhysRevLett.102.22640110.1103/PhysRevLett.102.226401 ↗
40. The elk code http://elk.sourceforge.io (accessed: June 2022).
41. 10.1364/JOSAB.16.00120410.1364/JOSAB.16.001204 ↗
42. 10.1063/1.314361310.1063/1.3143613 ↗