journal article·2018-12

p‐Type Doped AlAsSb/GaSb Resonant Tunneling Diode Photodetector for the Mid‐Infrared Spectral Region

Andreas Pfenning, Fabian Hartmann, Robert Weih, Monika Emmerling, Lukas Worschech, Sven Höfling

Advanced Optical Materials· Volume 6· Issue 24
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Abstract

Abstract Mid‐infrared (MIR) resonant tunneling diode (RTD) photodetectors based on a p‐type doped AlAsSb/GaSb double‐barrier quantum well (DBQW) are proposed and investigated for their optoelectronic transport properties. At room temperature, a distinct resonant tunneling current with a region of negative differential conductance is measured. The peak‐to‐valley current ratio (PVCR) is 1.51. To provide photosensitivity within the MIR spectral region, a lattice‐matched quaternary low‐bandgap GaInAsSb absorption layer with cutoff wavelength of λ = 2.77 μm is integrated near the DBQW. Under illumination with infrared light, photogenerated minority electrons within the absorption layer can drift toward the DBQW, where they accumulate and cause a shift of the current–voltage characteristics toward smaller bias voltages, which can be exploited to measure the incident MIR light power. In a tunable diode laser absorption spectroscopy experiment, the RTD photodetector is used to identify three distinct water absorption lines in the MIR close to λ = 2.61 μm. By adjusting the absorption layer doping concentration, the RTD quantum efficiency can be increased by a factor of 10, resulting in a sensitivity of S = 2.71 A W−1, which corresponds to an estimated multiplication factor of M = 8.6.
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Research context

OpenAlex topics: Semiconductor Quantum Structures and Devices · Spectroscopy and Laser Applications · Advanced Semiconductor Detectors and Materials

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

Technische Physik Physikalisches Institut and Röntgen Center for Complex Material Systems (RCCM) Universität Würzburg Am Hubland D‐97074 Würzburg Germany

SUPA School of Physics and Astronomy University of St. Andrews St. Andrews KY16 9SS UK

Funding

Bundesministerium für Bildung und Forschung

References (64)

Show source-provided references
1. 10.1063/1.165450910.1063/1.1654509 ↗
2. 10.1063/1.165506710.1063/1.1655067 ↗
3. 10.1109/5.66354110.1109/5.663541 ↗
4. 10.1103/PhysRevB.64.24533310.1103/PhysRevB.64.245333 ↗
5. 10.1103/PhysRevB.59.1021710.1103/PhysRevB.59.10217 ↗
6. 10.1103/PhysRevB.70.11532110.1103/PhysRevB.70.115321 ↗
7. 10.1143/JJAP.47.437510.1143/JJAP.47.4375 ↗
8. Suzuki S. · Appl. Phys. Lett. · 2010 · 97 · 33
9. Izumi R. · 2017
10. 10.1038/srep1951010.1038/srep19510 ↗
11. 10.1063/1.500888810.1063/1.5008888 ↗
12. 10.1186/1556-276X-8-21810.1186/1556-276X-8-218 ↗
13. 10.1021/acsnano.5b0183110.1021/acsnano.5b01831 ↗
14. 10.1063/1.10446710.1063/1.104467 ↗
15. 10.1063/1.172829010.1063/1.1728290 ↗
16. 10.3390/s13070946410.3390/s130709464 ↗
17. 10.1117/12.223727010.1117/12.2237270 ↗
18. 10.1016/j.physe.2003.08.00310.1016/j.physe.2003.08.003 ↗
19. 10.1117/12.35124910.1117/12.351249 ↗
20. 10.1103/PhysRevLett.100.23660110.1103/PhysRevLett.100.236601 ↗
21. 10.1103/PhysRevLett.107.13660310.1103/PhysRevLett.107.136603 ↗
22. 10.1103/PhysRevLett.115.03680310.1103/PhysRevLett.115.036803 ↗
23. 10.1103/PhysRevB.98.04130110.1103/PhysRevB.98.041301 ↗
24. 10.1063/1.477359310.1063/1.4773593 ↗
25. 10.1126/science.264.5158.55310.1126/science.264.5158.553 ↗
26. 10.1038/nphoton.2012.14310.1038/nphoton.2012.143 ↗
27. 10.1063/1.490732610.1063/1.4907326 ↗
28. 10.1088/0022-3727/48/12/12300110.1088/0022-3727/48/12/123001 ↗
29. 10.1063/1.481113310.1063/1.4811133 ↗
30. 10.1006/spmi.1995.101710.1006/spmi.1995.1017 ↗
31. 10.1049/el:1996006410.1049/el:19960064 ↗
32. 10.1063/1.331393410.1063/1.3313934 ↗
33. 10.1063/1.499485810.1063/1.4994858 ↗
34. 10.1063/1.10215110.1063/1.102151 ↗
35. 10.1103/PhysRevB.46.1601210.1103/PhysRevB.46.16012 ↗
36. 10.1063/1.10180110.1063/1.101801 ↗
37. 10.1063/1.11170510.1063/1.111705 ↗
38. 10.1103/PhysRevB.51.793810.1103/PhysRevB.51.7938 ↗
39. 10.1103/PhysRevB.52.R549510.1103/PhysRevB.52.R5495 ↗
40. 10.1063/1.497389410.1063/1.4973894 ↗
41. 10.1063/1.499749710.1063/1.4997497 ↗
42. Hartmann F. · Proc. SPIE · 2017 · 10403 · 1040306
43. 10.1063/1.136815610.1063/1.1368156 ↗
44. 10.1016/S0921-5107(99)00098-710.1016/S0921-5107(99)00098-7 ↗
45. 10.1088/0268-1242/26/7/07502110.1088/0268-1242/26/7/075021 ↗
46. 10.1063/1.146284410.1063/1.1462844 ↗
47. 10.1016/j.physleta.2004.09.05610.1016/j.physleta.2004.09.056 ↗
48. 10.12693/APhysPolA.110.11110.12693/APhysPolA.110.111 ↗
49. 10.1063/1.496779110.1063/1.4967791 ↗
50. 10.1103/PhysRev.92.132410.1103/PhysRev.92.1324 ↗
51. 10.1103/RevModPhys.64.75510.1103/RevModPhys.64.755 ↗
52. 10.1016/S0921-5107(01)00978-310.1016/S0921-5107(01)00978-3 ↗
53. 10.1063/1.35968310.1063/1.359683 ↗
54. 10.1063/1.483453610.1063/1.4834536 ↗
55. 10.1063/1.492942410.1063/1.4929424 ↗
56. 10.1088/0957-4484/27/35/35520210.1088/0957-4484/27/35/355202 ↗
57. 10.1063/1.11438410.1063/1.114384 ↗
58. 10.1117/12.223818910.1117/12.2238189 ↗
59. 10.1063/1.502553110.1063/1.5025531 ↗
60. 10.1109/55.49183510.1109/55.491835 ↗
61. 10.1063/1.36867710.1063/1.368677 ↗
62. 10.1103/PhysRevB.60.810510.1103/PhysRevB.60.8105 ↗
63. 10.1063/1.501901910.1063/1.5019019 ↗
64. 10.1016/j.jqsrt.2017.06.03810.1016/j.jqsrt.2017.06.038 ↗