The Photonics Project is a set of web based calculation tools for educational and analytical use. The tools are primarily Python based notebooks that execute as Web based Apps to the user, not requiring any programming knowledge or installation of any software. There will also be some tools showing full mathematical notation that are MathCad based and require the free MathCad plug in. The calculations primarily follow from equations as presented in the Infrared and Electro-Optical Systems textbook by Ron Driggers et al (second edition). They encompass a suite of Radiometric, Optical, and other photonic functionality. Further efforts are ongoing including an active imaging and photonics devices pages. Like Python itself, the site is open to suggestions and collaboration from users and submission of further tools and functionalities. And totally free of charge to all users.
KEYWORDS: Photon counting, Picture Archiving and Communication System, Photodetectors, Interferometers, Time correlated photon counting, Beam splitters, Single photon, Signal detection
Quantum sensing and metrology is the application of non-classical resources to the measurement of physical quantities with precision or accuracy beyond that allowed by classical physics. For many years non-classical resources such as atomic energy quantization, Josephson Effect, and Quantum Hall Effect have been used to define the fundamental units of time, voltage, and resistance, respectively. In recent years non-classical resources such as quantum squeezing and entanglement have been exploited to expand the range of physical phenomena measured with unprecedented precision or accuracy. We summarize some of the recent research on advanced quantum sensing and metrology and discuss our analyses of photon-added coherent states (PACS) of light. These analyses take into account imperfect photon addition and detection processes and show that PACS enable beyond-classical signal-to-noise ratio for photon counting even in cases where the probability of intended photon addition is 80%. We also show that there remains undiscovered fundamental properties of PACS related to their production and implementation.
Antimony-based Interband Cascade (IC) photodetectors are emerging as viable candidates for highperformance infrared applications, especially at high operating temperatures. In our previous IC detector designs using InAs/GaSb Type-II superlattices, the quantum efficiency was relatively low as the designs were optimized for high signal to noise ratio. Here we report our recent development of low-noise mid-IR IC photodetectors with high external quantum efficiency. By adopting IC detectors with thicker absorber designs, the quantum efficiency of these mid-IR IC detectors has been increased up to 35%. These IC devices continue to have low-dark current and high temperature operations. Some further analysis on the device characteristics is also presented.
An optimized long-wavelength two-color quantum well IR photodetector (QWIP) device structure has been designed. This device structure was grown on a three-inch semi- insulating GaAs substrate by molecule beam epitaxy (MBE). This wafer was processed into several 640 X 486 format monolithically integrated 8-9 and 14-15 micrometers two-color QWIP focal plane arrays (FPAs). These FPAs were then hybridized to 640 X 486 silicon CMOS readout multiplexers. A thinned FPA hybrid was integrated into a liquid helium cooled dewar to perform electrical and optical characterization and to demonstrate simultaneous two-color imagery. The 8-9 micrometers detectors in the FPA have shown background limited performance (BLIP) at 70 K operating temperature, at 300 K background with f/2 cold stop. The 14-15 micrometers detectors of the FPA have reached BLIP at 40 K operating temperature at the same background conditions. In this paper we discuss the performance of this long-wavelength dualband QWIP FPA in quantum efficiency, detectivity, noise equivalent temperature difference, uniformity, and operability.
Typical quantum well infrared photodetectors (QWIPs) exhibit rather narrow spectral bandwidth of 1 to 2 micrometer. For certain applications, such as spectroscopy, sensing of a broader range of infrared radiation is highly desirable. In this work, we report the design of five broadband (BB-) QWIPs sensitive over the 7 to 14 micrometer spectral range. Three n- type BB-QWIPs consisting of three, four, and five quantum wells of different thickness and/or composition in a unit cell, which are then repeated 20 times for the three and four quantum wells (QW) devices and 3 times for the five QWs device to create the BB-QWIP structures, are demonstrated. The three- well n-type InxGa1-xAs/AlyGa1-yAs BB-QWIP is designed to have a response peak at 10 micrometer, with a FWHM bandwidth that varies with the applied bias. A maximum bandwidth of (Delta) (lambda) /(lambda) p equals 21% was obtained for this device at Vb equals -2 V. The four- well n-type InxGa1-xAs/GaAs BB-QWIP not only exhibits a very large responsivity of 2.31 A/W at 10.3 micrometer and Vb equals +4.5 V, but also achieves a broader bandwidth of (Delta) (lambda) /(lambda) p equals 29% than the three-well device. The five-well n-type InxGa1- xAs/GaAs BB-QWIP has achieved a FWHM bandwidth of (Delta) (lambda) /(lambda) p equals 28% at Vb equals 1.75 V. In addition, two p-type InxGa1-xAs/GaAs BB-QWIPs with variable well thickness and composition, sensitive in the 7 - 14 micrometer spectral range, are also demonstrated. The variable composition p-type BB-QWIP has a very large FWHM bandwidth of (Delta) (lambda) /(lambda) p equals 48% at Vb equals -1.5 V and T equals 40 K. The variable thickness p- type BB-QWIP was found to have an even broader FWHM bandwidth of (Delta) (lambda) /(lambda) p equals 63% at Vb equals 1.1 V and T equals 40 K, with a corresponding peak responsivity of 25 mA/W at 10.2 micrometer. The results reveal that p-type BB- QWIPs have a broader and flatter spectral bandwidth but lower responsivity than that of n-type BB-QWIPs under similar operating conditions.
High performance long-wavelength GaAs/AlxGa1-xAs quantum well infrared photodetectors for low background applications have been demonstrated. This is the first theoretical analysis of quantum well infrared photodetectors for low background applications and the detectivity D* of 6 X 1013 cm(root)Hz/W has been achieved at T equals 40 K with 2 X 109 photons/cm2/sec background. In addition, this paper describes the demonstration of mid- wavelength/long-wavelength dualband quantum well infrared photodetectors and long-wavelength/very long-wavelength dualband quantum well infrared photodetectors in 4 - 26 micrometer wavelength region.
We report a two-stack indirect-barrier (IB-) GaAs/Al0.55Ga0.45As quantum well infrared photodetector (QWIP) for mid-wavelength infrared (MWIR) and a voltage-tunable In0.05Ga0.95As/GaAs/Al0.19Ga0.81As triple-coupled (TC-) QWIP for long-wavelength infrared (LWIR) detection. We also investigate the performance dependence of this stacked QWIP with different quantum well periods (20-period and 40- period). The peak responsivity of the 20-period stacked-QWIP at zero bias (PV mode) was found to be 30 mA/W at (lambda) p equals 4.3 micrometer and T equals 40 K. The maximum peak responsivity (PC mode) was found to be 0.25 A/W at (lambda) p equals 4.3 micrometer, Vb equals -4 V, and T equals 40 K for the 20-period MWIR IB-QWIP. For the LWIR TC- QWIP, the peak wavelength due to (E1 yields E3) transition shifts from 10 micrometer to 9.4 micrometer as bias voltage changes from 5 to 7 V and from 9 to 14 V for 20-period and 40 period devices, respectively. A peak responsivity of 0.16 A/W was obtained at (lambda) p equals 9.4 micrometer, Vb equals 7 V, and T equals 40 K for the 20-period TC- QWIP. The results show that simultaneous detection of IR radiation at both the MWIR and LWIR bands can be achieved at Vb greater than or equal to 7 V or Vb less than or equal to -5 V for the 20-period stacked QWIP. It is shown that this two-stack QQWIP can be used as a wavelength-tunable IR detector for the MWIR and LWIR bands.
A high sensitivity triple-coupled quantum well infrared photodetector (TC-QWIP) based on high strain InGaAs/AlGaAs/InGaAs material system has been demonstrated. It consists of a high strain Si-doped In0.25Ga0.75As quantum well and two undoped thin Al0.11Ga0.89As/In0.12Ga0.88As quantum wells (QWs) separated by a thick Al0.11Ga0.89As barrier layer. We also investigate the performance dependence of this QWIP with two different numbers of quantum well periods (5- and 10-period). Two response peaks at 9.5 micrometer and 7 micrometer were observed under different negative bias conditions, which are attributed to the transitions from the ground state to the second excited states and the continuum states, respectively. Spectral responsivities of 2.77 A/W and 1.55 A/W and the BLIP detectivities of 2.24 X 1010 cm-Hz1/2/W and 1.68 X 1010 cm-Hz1/2/W were obtained at Vb equals -3 V and (lambda) p equals 9.6 micrometer with 45 degree facet illumination and normal incidence illumination, respectively, for the 5-period device. As to the 10-period device, spectral responsivities of 2.7 A/W and 1.05 A/W and the BLIP detectivities of 2.21 X 1010 cm-Hz1/2/W and 1.38 X 1010 cm-Hz1/2/W were obtained at Vb equals -5 V and (lambda) p equals 9.6 micrometer with 45 degree facet illumination and normal incidence illumination, respectively, for this device. This represents the highest normal incidence response ever reported for a QWIP operating at 9.6 micrometer peak wavelength. Based on the responsivity and detectivity data the minimum detectable photon flux for this new device is found to be 1.08 X 1011 and 1.09 X 1011 cm-2s-1 for the 5-period and 10- period devices, respectively, at (lambda) p equals 9.6 micrometer, bandwidth equals 1 micrometer, and FOV equals 180 degrees. Thus, the HS-TC-QWIP reported here is capable for lower background IR imaging array applications.
Quantum well infrared photodetector (QWIP) technology has developed rapidly in the past decade culminating in the demonstration of large format focal plane arrays. Most of the efforts so far have been on tactical applications in which an increased operating temperature is the major objective. For strategic applications with a cold background and a faint target, low temperature operation is required. Under these conditions, improving the conversion efficiency (quantum efficiency times gain) is very important for QWIPs to collect sufficient signal. Simplified QWIP (S-QWIP) structures with increased optical gains have been demonstrated. In this presentation, experimental results of several S-QWIPs will be given. The properties of simplified QWIPs will be examined at low temperatures with a low background and a faint target. Results of a computer simulation with an unresolved target will be discussed.
One of the simplest device realizations of the classic particle-in-the-box problem of basic quantum mechanics is the Quantum Well Infrared Photodetector (QWIP). In this paper we discuss the optimization of the detector design, material growth and processing that has culminated in realization of 15 micron cutoff 128 X 128 QWIP focal plane array camera, hand-held and palmsize 256 X 256 long-wavelength QWIP cameras and 648 X 480 long-wavelength camera, holding forth great promise for myriad applications in 6 - 25 micron wavelength range in science, medicine, defense and industry. In addition, we present the recent developments in broadband QWIPs, mid-wavelength/long-wavelength dualband QWIPs, long- wavelength/very long-wavelength dualband QWIPs, and high quantum efficiency QWIPs for low background applications in 4 - 26 micrometer wavelength region for NASA and DOD applications.
Quantum well infrared photodetectors (QWIPs) have emerged as a viable contender for many remote sensing applications, even in the space environment where low background fluxes are involved. There are, however, several issues that still need to be resolved in order to achieve optimum performance at low operating temperatures. One important issue is the dark current, which is dominated by Fowler-Nordheim and trap-assisted tunneling in this regime. In order to decrease the dark current of QWIPs at low temperatures, we are investigating these mechanisms to better understand them. Our preliminary investigations have uncovered another possible problem; offsets in the I-V characteristics which could impair the compatibility of a QWIP array with a readout circuit. In this paper we discuss these design issues.
Quantum well and superlattice IR detectors have recently become visible contenders for many military applications. In this paper we present an overview of the issues related to quantum well and superlattice IR detectors and discuss in detail, the issues related to the application of these detectors for space missions.
In this paper we present an experimental investigation of the performance of GaAs/AlGaAs multiple quantum well photodetectors. The purpose of this exercise was to independently evaluate and verify the responsivity of the GaAs/AlGaAs quantum well infrared photodetectors developed at the Industrial Microelectronics Center in Sweden. These devices use 2D gratings to couple radiation into the detectors and a cladding layer to enhance the coupling of radiation. The devices were of two types: those optimized for high detectivity, and those optimized for high quantum efficiency. The tests performed on these devices included measurement of optical responsivity vs. bias, spectral response, Detectivity (D*), and measurement of cross-talk between pixels. Several interesting observations were made during the investigation and will be reported in the paper.
The past decade has seen extensive development of strategic IR focal plane arrays, with the result that surveillance, tracking, and interceptor sensors are a much more credible force for national and theater defense. Investment in IR detector materials, especially HgCdTe, has resulted in breakthrough improvements in array sensitivity, uniformity, and size, making these materials viable for the vital strategic defense systems currently envisioned for deployment. Development of silicon impurity band conductor detector arrays has resulted in arrays for the very long-wave IR that approach theoretical limits for performance in the surveillance applications of tomorrow. Programs for the development of readout circuitry have allowed array sizes to increase dramatically, while permitting longer operational lifetimes in space radiation environments with reduced electronics noise. Efforts under these development programs to cut array costs, while improving yield and performance, are preparing us for programs to manufacture the number required at a cost that will allow the surveillance system to be affordable. This paper presents an overview of space sensor missions, technical progress from recently completed programs, status of ongoing efforts, and speculation about development needs and directions for the future.
We introduce charge accumulation in quantum wells through the use of a nonlinear Schrodinger equation. Looking first at infinite and finite square wells allows us to calculate the new energy spectrum including the separate effects of a biasing electric field and charge accumulation. This gives us insight into the new resonant tunneling energies that arise due to the quasibound states being shifted by either the external field or the reaction field built up through the accumulation of charge. Using a double barrier potential, we calculate the transmission coefficient with and without the external bias field and then with charge accumulation. To study the tunneling dynamics, we first start with a single barrier in an infinite well and discover a fractal-like character to the probability for finding an electron wavepacket in one side of the structure. Finally we numerically integrate the full time- dependent nonlinear Schrodinger equation with various barrier potentials to obtain the dynamics of a wavepacket incident on the structures.
Neutron irradiation produces defects in silica glass which could lead to permanent loss in transmission of signals through an optical fiber made from this material. This paper reports on a study aimed at gaining a deeper understanding of the nature of damage caused by neutron irradiation to silica glass optical fibers operating at 1.3//m and 1.55/im. The data obtained so far indicates that the radiation induced damage has less effect on the transmission at 1.3//m than on the transmission at 1.55/im. The implications of this significant observation, and the details of the experimental techniques utilised in this study will be discussed in this paper.
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