TripleSpec Update TripleSpec Update TripleSpec Update TripleSpec Update TripleSpec Update TripleSpec Update TripleSpec Update Detector Characterization The performance of detectors can be characterized in terms of: Responsivity -- the number of amps (electrons) out for a Watt of incident power For G=1 and =1 R∝ 1 I nj ∝ A 1 R Noise Equivalent Power (NEP) -- The amount of incident power needed to produce a signal equal to the RMS noise. Detectivity (D) - The inverse of NEP (for those who don't golf). Normalized Detectivity (D*) -- D divided by sqrt(detector area) this provides a more geometry independent assessment of detector performance since, for Johnson noise limited performance, R∝ 1 A I nj ∝ 1 R Extrinsic Semiconductors Introducing an impurity into an intrinsic semiconductor can introduce energy states with very small bandgaps relative to the intrinsic conduction (donors) or valence (acceptors) bands. At room temperatures doping creates a well-controlled population of conducting electrons/holes – semiconductor devices. At cryogenic temperatures (kT <<< bandgap energy) dopants create bound states/conduction levels with small energy difference – long wavelength detectors. Extrinsic Semiconductor Detectors Doping levels must be low (1016 cm−3 ) in order to avoid dark conduction due to ''hopping''. Requires centimeter thick detector layers to obtain necessary absorption for good quantum efficiency. Stressed Photoconductors Even extrinsic semiconductors have large bandgaps relative to the energy of a 200um photon (0.005 eV) Mechanical stress can weaken the bond of an acceptor (hole) in a p-type extrinsic material. The Spitzer 160um array is constructed with discrete stressed Ge:Ga detectors. http://fifils.mpe-garching.mpg.de/pics/det/spect-resp.gif http://mips.as.arizona.edu/MIPS/ http://fifils.mpe-garching.mpg.de/detector.html Stressed Photoconductors Even extrinsic semiconductors have large bandgaps relative to the energy of a 200um photon (0.005 eV) Mechanical stress can weaken the bond of an acceptor (hole) in a p-type extrinsic material. The Spitzer 160um array is constructed with discrete stressed Ge:Ga detectors. http://mips.as.arizona.edu/MIPS/ Stressed Photoconductors Even extrinsic semiconductors have large bandgaps relative to the energy of a 200um photon (0.005 eV) Mechanical stress can weaken the bond of an acceptor (hole) in a p-type extrinsic material. The Spitzer 160um array is constructed with discrete stressed Ge:Ga detectors. http://mips.as.arizona.edu/MIPS/ Blocked Impurity Band (BIB) Extrinsic Photoconductors In order to avoid “hopping” (valence band conduction) doping levels must be kept low in biased extrinsic semiconductors. At these low doping levels, physical thickness must be large to obtain good quantum efficiency. Large arrays become impractical due to detector size. If a heavily doped layer, however, is insulated from conducting leads hopping is avoided. Blocked Impurity Band detectors (BIB's) provide the best of both worlds. An undoped (''insulating'') layer thwarts conduction through the device in the heavily doped impurity band. The applied bias... Photons can still promote carriers to the conduction band of the intrinsic material BIBs in Space Arsenic doped Silicon (Si:As) BIB detectors provide high quantum efficiency in array formats as large as 1024x1024 Quantum efficiency can be close to 100% Dark currents range from 10,000 e-/s at 10K to 10 e-/s at 6K Spitzer IRS uses 128x128 Si:As (520um) and Si:Sb (18-38um) BIB arrays. Spitzer MIPS 24um is a 128x128 Si:As BIB WISE (2009 launch) will use two 1024x1024 Si:As BIB arrays for its 12 and 23um imaging channels. DRS Technologies BIB Arrays BIBs in Space Arsenic doped Silicon (Si:As) BIB detectors provide high quantum efficiency in array formats as large as 1024x1024 Quantum efficiency can be close to 100% Dark currents range from 10,000 e-/s at 10K to 10 e-/s at 6K Spitzer IRS uses 128x128 Si:As (520um) and Si:Sb (18-38um) BIB arrays. Spitzer MIPS 24um is a 128x128 Si:As BIB WISE (2009 launch) will use two 1024x1024 Si:As BIB arrays for its 12 and 23um imaging channels. DRS Technologies BIB Arrays Short Wavelength Infrared Arrays: InSb as a (poor) Photoconductor Indium Antimonide (InSb) is a particularly attractive intrinsic semiconductor for near-infrared detection (bandgap -> 5.5um) 7 5 2 −1 −1 Given =10 ; =10 cm V s in this material. G = 10 −2 V l 2 InSb will break down at about 1V, so the thickness of such a detector would have to be 1mm in order to achieve G=1. Given the high carrier mobility such a thin detector would have a small resistance and, thus, large Johnson noise. At the same time, the detector would exhibit poor quantum efficiency due to (not to mention a potentially poor quantum efficiency due to a small absorption cross section. These two competing goals – thick for absorption, thin for G=1, seem to rule out this ideal material as a viable detector. HgCdTe has similar properties.... so how to make effective short wavelength detectors??? particularly for arrays... Diodes If materials with different Fermi energies are brought into contact, the Fermi levels must reach equilibrium in the two materials through the migration of carriers. This situation is achieved in practice by joining a donor doped extrinsic semiconductor (n-type) with acceptor doped material (ptype) – – Donor electrons in the n-type material find it energetically favorable to migrate into the p-type region and fill holes. This migration creates a “depletion region” at the p/n junction which is free of both donors and acceptors. Diodes If materials with different Fermi energies are brought into contact, the Fermi levels must reach equilibrium in the two materials through the migration of carriers. This situation is achieved in practice by joining a donor doped extrinsic semiconductor (n-type) with acceptor doped material (ptype) – – Donor electrons in the n-type material find it energetically favorable to migrate into the p-type region and fill holes. The displacement of charges creates a significant “contact potential” from the electric field across the depletion region Diode Behavior The depletion region has a high resistance and prevents conduction through the detector – good for minimizing Johnson noise. Placing a voltage across the diode can either enhance or degrade/eliminate the potential barrier presented by the depletion region. A diode will not conduct when a reverse bias is applied which adds to the contact potential barrier. The diode will begin to conduct when a forward bias is applied in excess of the junction potential barrier. Non-ideal Diode Behavior In reality, a small contaminant of donors exists in the p-type material and vice versa. These minority carriers create a small leakage current when the diode is reverse biased. The reverse current (Io) is proportional to the density of these contaminants. At high reverse bias tunneling can begin to add to the reverse current. Ultimately avalanche breakdown forces the junction into conduction at extreme reverse bias level. Explaining Diode Conduction Diode current vs. applied voltage bias, Vb, is given by qV b Io = I = I 0 e kT − 1 – qAD L N where A is the junction area, D is the diffusion coefficient, L is the diffusion length and N is the carrier density. How does this come about? The pn junction is a barrier of width, w, permeated by an electric field which yields a contact potential difference, Vo. One can solve the diffusion equation for carrier density through the junction under this opposing potential, yielding for the carrier density on qV np eithe side of the junction. = e kT nn o Under a bias, a carrier that makes it across the junction contributes to the current. since np is uninfluenced by Vb. q V −V qV np = e kT = n n e kT nn o b b The carriers which cross the junction must then make it through the (hostile) oppositely doped region – thus the constant dependent on diffusion. Photodiode Detection The migration/diffusion of carriers across the junction creates a region depleted of carriers an electric field across the region due to the excess of opposite type carriers on either side. An electron/hole pair created by a photon near this depletion region will be separated and swept out by the electric field if the electron can diffuse to the region before recombining. prevents rapid recombination creates a ''photocurrent'' which will flow through a wire connecting the ''p'' and ''n'' type materials the “assured” detection of the electron makes the photoconductive gain = 1 in this configuration high resistance and high gain make for an attractive detector Detection of Photocurrent