Noise properties of preamplifier to be used with LN2-cooled HgCdTe photodetector
https://doi.org/10.32362/2500316X-2025-13-1-122-135
EDN: OABDBH
Abstract
Objectives. Photoresistors based on a solid solution of mercury–cadmium–tellurium (MCT) have been used in infrared (IR) technology for over 60 years. They can have a sensitivity range in the wavelength region from 1 μm to 15 μm, depending on Hg1−xCdxTe composition. The resistance of photosensitive MCT elements is (depending on their area) tens of Ohms, and for such a resistor the thermodynamically expected Nyquist noise is less than 1 nV/√Hz. Modern semiconductor technologies ensure a high level of quality of both photodetectors and input stages of integrated circuits for amplifying the signal from them. The aim of this work is to study the noise properties of the electronic unit developed for joint operation with a liquid nitrogen cooled MCT-photodetector.
Methods. An analog input-output digital signal processor card P25M (Innovative, Inc., USA) was used to measure and accumulate the noise spectra of the signal in the frequency range 0–1 MHz. The card has four 16-bit ADCs of sampling rate up to 25MSpS, a Spartan-3 field-programmable gate array controlling them, a TMS320C6713 processor, and RAM, in order to transmit the collected digital data to the motherboard through a common PCI-X slot. The spectra of the received data were calculated using the fast Fourier transform algorithm with subsequent averaging of the square of the amplitude for all spectral components.
Results. The noise properties of comparatively modern integrated circuits currently used for this task were considered. The noise density spectra of the first stage (ADA4898-2), the second stage (AD8034), and bias current sources (AD8397 and LT3009) were measured. It was found that the spectral density of the input noise of the operational amplifier ADA4898-2 is comparable to the Nyquist (thermodynamically expected) noise of a 20–100-Ohm resistor corresponding to the resistance of the photosensitive element. This means that the selected operational amplifier is ideal for resolving the technical problem discussed herein. Meanwhile, it was also established that the noise spectrum of the LT3009, ADR510 voltage and current stabilizer integrated circuits contains a noticeable drift component with a spectral density of “pink noise” 1/f α (f – frequency, α ≈ 1).
Conclusions. It was shown that the spectral noise density of the electronic components, reduced to the input of the device, is several times lower than the noise density of the photodetector used.
About the Authors
Dmitry V. KazantsevRussian Federation
Dmitry V. Kazantsev, Dr. Sci. (Phys.-Math.), Senior Researcher; Professor, Faculty of Physics,
53, Leninskii pr., Moscow, 119991;
21/5, Staraya Basmannaya ul., Moscow, 101000.
Scopus AuthorID: 6603178750.
Competing Interests:
The authors declare no conflicts of interest.
Elena A. Kazantseva
Russian Federation
Elena A. Kazantseva, Senior Lecturer, Higher Mathematics Department, Institute of Cybersecurity and Digital Technologies,
78, Vernadskogo pr., Moscow, 119454.
Scopus AuthorID: 57219932826.
Competing Interests:
The authors declare no conflicts of interest.
References
1. Norton P. HgCdTe infrared detectors. Opto-Electron. Rev. 2002;10(3):159–174.
2. Kopytko M., Rogalski A. New insights into the ultimate performance of HgCdTe photodiodes. Sensors and Actuators A: Physical. 2022;339:113511. doi: 10.1016/j.sna.2022.113511
3. Józwikowska A., Józwikowski K., Rogalski A. Performance of mercury cadmium telluride photoconductive detectors. Infrared Phys. 1991;31(6):543–554. doi: 10.1016/0020-0891(91)90141-2
4. Rogalski A. Commentary on the Record-Breaking Performance of Low-Dimensional Solid Photodetectors. ACS Photonics. 2023;10(3):647–653. doi: 10.1021/acsphotonics.2c01672
5. Kulchitsky N.A., Naumov A.B., Startsev V.V. Cooled IR photodetectors based on cadmium-mercury-tellurium: current status and development prospects. Elektronika: nauka, tekhnologiya, biznes = Electronics: Science, Technology, Business. 2020;6(197):114–121 (in Russ.). https://doi.org/10.22184/1992-4178.2020.197.6.114.121
6. Hansen G.L., Schmit J.L., Casselman T.N. Energy gap versus alloy composition and temperature in Hg1−xCdxTe. J. App. Phys. 1982;53(10):7099–7101. https://doi.org/10.1063/1.330018
7. Lawson W., Nielsen S., Putley E., Young A. Preparation and properties of HgTe and mixed crystals of HgTe–CdTe. J. Phys. Chem. Solids. 1959;9(3–4):325–329. https://doi.org/10.1016/0022-3697(59)90110-6
8. Schmit J.L., Stelzer E.L. Temperature and Alloy Compositional Dependences of the Energy Gap of Hg1−xCdxTe. J. Appl. Phys. 1969;40(12):4865–4869. https://doi.org/10.1063/1.1657304
9. Scott M.W. Energy Gap in Hg1−xCdxTe by Optical Absorption. J. Appl. Phys. 1969;40(10):4077–4081. https://doi.org/10.1063/1.1657147
10. Elliott C., Melngailis J., Harman T., Kafalas J., Kernan W. Pressure Dependence of the Carrier Concentrations in p-Type Alloys of Hg1−xCdxTe at 4.2 and 77°K. Phys. Rev. B. 1972;5(8):2985. https://doi.org/10.1103/PhysRevB.5.2985
11. McCombe B.D., Wagner R.J., Prinz G.A. Far-Infrared Observation of Electric-Dipole-Excited Electron-Spin Resonance in Hg1−xCdxTe. Phys. Rev. Lett. 1970;25(2):87–90. https://doi.org/10.1103/PhysRevLett.25.87
12. Xin W., Zhong W., Shi Y., Shi Y., Jing J., Xu T., Guo J., Liu W., Li Y., Liang Z., Xin X., Cheng J., Hu W., Xu H., Liu Y. Low-Dimensional-Materials-Based Photodetectors for Next-Generation Polarized Detection and Imaging. Adv. Mater. 2024;36(7):2306772. https://doi.org/10.1002/adma.202306772
13. Xue X., Chen M., Luo Y., Qin T., Tang X., Hao Q. High-operating-temperature mid-infrared photodetectors via quantum dot gradient homojunction. Light: Sci. Appl. 2023;12(1):2. https://doi.org/10.1038/s41377-022-01014-0
14. Agarwal H., Nowakowski K., Forrer A., Principi A., Bertini R., Batlle-Porro S., Reserbat-Plantey A., Prasad P., Vistoli L., Watanabe K., Taniguchi T., Bachtold A., Scalari G., Krishna Kumar R., Koppens F.H.L. Ultra-broadband photoconductivity in twisted graphene heterostructures with large responsivity. Nat. Photon. 2023;17(12):1047–1053. https://doi.org/10.1038/s41566-023-01291-0
15. Lau J.A., Verma V.B., Schwarzer D., Wodtke A.M. Superconducting single-photon detectors in the mid-infrared for physical chemistry and spectroscopy. Chem. Soc. Rev. 2023;52:921–941. https://doi.org/10.1039/d1cs00434d
16. Rogalski A. HgCdTe infrared detector material: history, status and outlook. Rep. Prog. Phys. 2005;68(10):2267. http://doi.org/10.1088/0034-4885/68/10/R01
17. Kimchi J., Frederick J.R., Wong T.T.S. Low-frequency noise in photoconductive HgCdTe detectors. Proc. SPIE. 1996;2812. 12 p. https://doi.org/10.1117/12.254098
18. Johnson J.B. The Schottky Effect in Low Frequency Circuits. Phys. Rev. 1925;26(1):71–85. https://doi.org/10.1103/PhysRev.26.71
19. Schottky W. Small-Shot Effect and Flicker Effect. Phys. Rev. 1926;28(1):74–103. https://doi.org/10.1103/PhysRev.28.74
20. Dutta P., Horn P.M. Low-frequency fluctuations in solids: 1/f noise. Rev. Mod. Phys. 1981;53(3):497–516. https://doi.org/10.1103/RevModPhys.53.497
21. Voss R.F., Clarke J. 1/f noise in music and speech. Nature. 1975;258(5533):317. https://doi.org/10.1038/258317a0
22. Press W.H. Flicker noises in astronomy and elsewhere. Comments Astrophys. 1978;7(4):103–119.
23. Milotti E. 1/f noise: a pedagogical review. 2002; ArXiV_0204033v1. https://arxiv.org/pdf/physics/0204033
24. Rytov S.M. Vvedenie v statisticheskuyu radiofiziku. Chast’ 1. Sluchainye protsessy (Introduction to Statistical Radiophysics. Part 1. Random Processes). Moscow: Nauka; 1976. 496 p. (in Russ.).
25. Morikawa M., Nakamichi A. A simple model for pink noise from amplitude modulations. Sci. Rep. 2023;13(1):8364. https://doi.org/10.1038/s41598-023-34816-2
26. Zenhausern F., O’Boyle M.P., Wickramasinghe H.K. Apertureless near-field optical microscope. Appl. Phys. Lett. 1994;65(13):1623–1625. http://doi.org/10.1063/1.112931
27. Zenhausern F., Martin Y., Wickramasinghe H.K. Scanning Interferometric Apertureless Microscopy: Optical Imaging at 10 Angstrom Resolution. Science. 1995;269(5227):1083–1085. https://doi.org/10.1126/science.269.5227.1083
28. Keilmann F., Hillenbrand R. Near-Field Microscopy by Elastic Light Scattering from a Tip. Philos. Trans.: Math., Phys. Eng. Sci. 2004;362(1817):787–805. https://doi.org/10.1098/rsta.2003.1347
29. Kazantsev D.V., Kazantseva E.A. A Preamplifier for a CdHgTe Photodetector. Instrum. Exp. Tech. 2020;63(1):133–138. https://doi.org/10.1134/S0020441220010194 [Original Russian Text: Kazantsev D.V., Kazantseva E.A. A Preamplifier for a CdHgTe Photodetector. Pribory i tekhnika eksperimenta. 2020;1:144–150 (in Russ.). https://doi.org/10.31857/S0032816220010218 ]
30. Shockley W. The Theory of p-n Junctions in Semiconductors and p-n Junction Transistors. Bell System Tech. J. 1949;28(3): 435–489. https://doi.org/10.1002/j.1538-7305.1949.tb03645.x
31. Kazantsev D.V., Kazantseva E.A. Digital Detection of Optical Signals in a Near-Optical-Field Microscope. Instrum. Exp. Tech. 2022;65(2):273–291. https://doi.org/10.1134/S0020441222020130 [Original Russian Text: Kazantsev D.V., Kazantseva E.A. Digital Detection of Optical Signals in a Near-Optical-Field Microscope. Pribory i tekhnika eksperimenta. 2022;2:79–98 (in Russ.). Available from URL: https://sciencejournals.ru/view-article/?j=pribory&y=2022&v=0&n=2&a=Pribory2202014Kazantsev ]
32. Cooley J.W., Tukey J.W. An algorithm for the machine calculation of complex Fourier series. Math. Comp. 1965;19(90): 297–301. https://doi.org/10.1090/S0025-5718-1965-0178586-1
33. Stephens D.R., Diggins C., Turkanis J., Cogswell J. C++ Cookbook. O’Reilly Media, Inc.; 2005. 592 p. ISBN 978-059-600761-4
Supplementary files
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1. Hg1−xCdxTe-based photodetectors photodetector placed on a substrate | |
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Type | Исследовательские инструменты | |
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Indexing metadata ▾ |
- The electronic unit for joint operation with a liquid nitrogen cooled mercury–cadmium–tellurium photodetector was developed and its noise properties were investigated.
- The noise properties of comparatively modern integrated circuits currently used for this task were considered. The noise density spectra of the first stage (ADA4898-2), the second stage (AD8034), and bias current sources (AD8397 and LT3009) were measured. It was found that the spectral density of the input noise of the operational amplifier ADA4898-2 is comparable to the Nyquist (thermodynamically expected) noise of a 20–100-Ohm resistor corresponding to the resistance of the photosensitive element. This means that the selected operational amplifier is ideal for resolving the technical problem discussed herein.
- It is shown that the spectral noise density of the electronic components, reduced to the input of the device, is several times lower than the noise density of the photodetector used.
Review
For citations:
Kazantsev D.V., Kazantseva E.A. Noise properties of preamplifier to be used with LN2-cooled HgCdTe photodetector. Russian Technological Journal. 2025;13(1):122-135. https://doi.org/10.32362/2500316X-2025-13-1-122-135. EDN: OABDBH