The present invention relates in general to high-energy radiation detectors, and in particular it relates to radiation detectors based on direct-gap semiconductor scintillator wafers, endowed with an epitaxial photodiode on a surface thereof.
Referring now to
Referring now to
To better understand the collection of photons in the integrated-pixel architecture, it has been noted that the propagation of scintillating radiation in the body of n-doped InP scintillator is diffusive, as shown by the research in room temperature experiments. Most of the scintillation photons reaching the detectors surface are not photons directly generated by the electrons and holes at the site of the gamma particle interaction, but photons that have been re-absorbed and re-emitted a multiple number of times. The motion of light form the initial interaction site to the detector is a random and characterized by a mean free path of about λ=100 μm (in the samples of doping n=6·1018 cm−3 at room temperature). The corresponding diffusion coefficient of light can be estimated as D=λ2/τ≈105 cm2/s, where τ=(Bn)−1≈1 ns is the radiative recombination time and B≈1.2×10−10 cm3/s is the radiative recombination constant in InP. This estimate justifiably assumes that light propagation between the absorption/re-emission sites is practically instantaneous.
To estimate the illumination area by an interaction event that occurs a distance h deep into the scintillator, the diffusion equation has been solved for the density of photons N({right arrow over (r)},t):
with the boundary condition, N(z=0,t)=0, of absorbing detector surface and the initial condition N({right arrow over (r)},t=0)=N0δ({right arrow over (r)}−{right arrow over (r)}0), where {right arrow over (r)}0=(0,0,−h). Using the known Green's function of the diffusion equation (1), it was found the resultant flux density j({right arrow over (r)},t) [cm−2 s−1] through the detector surface (the boundary plane) in the form of
It has been observed that the flux density decays radially from the epicenter as a Gaussian function of width d=√{square root over (Dt)}. For the total pulse duration T=h2/2D=v·τ, where v is the average number of the absorption/re-emission events, we have d=√{square root over (2DT)}=h≈λ√{square root over (T/τ)}=λ√{square root over (v)}. In the experiments at room temperature, h≈300 μm and v≈10, so that the Gaussian width of the flux distribution is about 3λ≈h. Both estimates, d=h and d=λ√{square root over (v)} give roughly the same width.
In the above-discussed prior art, all embodiments of the scintillator, the capacitance of the epitaxial PIN diode has been determined by the volume of its charge collection, and therefore it scales with the area of the pixel. Thus, there has been a need for a new architecture that provides a substantially smaller capacitance for same collection volume, the architecture which provides substantially higher pixel sensitivity.
One aspect of the invention relates to the composition of the scintillator body which addresses an essential issue of how to make the semiconductor transparent at wavelengths of its own fundamental interband emission. This emission wavelengths constitutes the scintillation spectrum of the radiation detector. For one of the embodiments of InP, the scintillation spectrum is within a relatively narrow band near 920 nm. The semiconductor is made relatively transparent to this radiation by doping it heavily with donor impurities, so as to introduce the so-called Burstein (or Moss-Burstein) shift between the emission and the absorption spectra. For the purposes of the invention, the term “heavy doping” means “degenerately doped with shallow donors” and specifies the doping as being so heavy that the Fermi energy counted from the bottom of semiconductor conduction band is larger than the operating temperature of the detector expressed in energy units. Because of the heavy doping, the edge of absorption is blue-shifted relative to the emission edge by the carrier Fermi energy. This quantum effect is called the Burstein shift. It underlies operation of many prior art semiconductor lasers. The transparency of semiconductor body to its own radiation helps delivering the scintillating photons, generated by high energy radiation deep inside the semiconductor wafer, to the surface of the wafer.
Another aspect of the invention concerns how to ensure the collection of the scintillating photons in photodetector. External detectors are inefficient for the following reason. Owing to the high refractive index of semiconductors, e.g., n=3.3 for InP, most of the scintillating photons will not escape from the semiconductor, but suffer a complete internal reflection. Only those photons that are incident on the InP-air interface within a narrow cone sin θ<1/n off the perpendicular to the interface, have a chance to escape from the semiconductor. The escape cone accommodates only about 2% of isotropic scintillation, signifying the inefficiency of collection. It is essential to provide the scintillator wafer with an epitaxial photodetector that has a substantially similar or even higher refractive index. Such epitaxial photodetector is most conveniently implemented as PIN photodiode. In principle one can use a single photodiode over the entire area of the chip, but for a chip of large area this may introduce a large capacitance that is difficult to handle by a readout circuitry. Even for a chip having an area of 1 mm×1 mm (1 mm2), the typical capacitance of a PIN diode would be about 50 pF. Such a high value of diode capacitance presents stringent and hard-to-meet requirements to the readout circuitry. Separation of 1,000 electron-hole pairs on such a capacitor produces a voltage of about 3.2 μV, which is difficult to measure due to noise. This limits the sensitivity of the 1 mm2 photodetector PIN diode. To achieve higher sensitivity it is possible to use smaller-area independently contacted diodes forming a two-dimensional (2D) array of pixels. Each of the small-area diodes has a proportionally smaller capacitance, which is beneficial from the standpoint of noise, but it also receives a smaller share of the scintillation flux generated deep inside the scintillator.
As to still another aspect of the invention, it would be highly desirable to implement a PIN diode that collects light from the same area but has a substantially lower capacitance, so that the sensitivity threshold would be much lower.
A still further aspect of the invention relates to the three dimensional (3D) pixellation of the scintillator response. A stack of individually contacted two dimensional (2D) pixellated semiconductor slabs forms a 3D array of radiation detectors. A gamma photon incident on such an array, undergoes several Compton interactions depositing varying amounts of energy Li in pixels with coordinates (xi, yi, zi), where zi describes the position in the stack of the slab with a responding (“firing”) pixel and (xi, yi) are 2D coordinates of the firing pixel in that slab. Thus, each incident photon produces a cluster of firing pixels that reports their positions and the amount of energy deposited. The information reported enables one to estimate both the incident photon energy and the direction to the source.
A reasonable figure of merit (FoM) for the pixel performance is the ratio of expected number of photons incident of the pixel's PIN diode in response to the typical Compton interaction that occurred within the volume of said pixel, to the capacitance of the pixel's diode. In the prior art design, at least for small enough pixels, both parameters in the FoM scale with the diode area and hence their ratio remains approximately constant. Thus, it is an essential aspect of the present invention to improve said FoM and thus to enhance the signal to noise ratio. This is accomplished by substantially lowering the capacitance of the pixel's PIN diode, while keeping the same volume of absorption (the depleted region of the PIN structure) and therefore keep in the same typical number of absorbed scintillation photons.
Referring now to
The total area of the collector contacts 12 is much smaller than the area of the diode and the contacts are spaced from each other by the distance 2s. Such distance should be not too large so that the travel time of holes over the distance s is much smaller than the lifetime of holes in the intrinsic region. All contacts 12 are connected together by thin metallic lines (not shown in
In the embodiment of
The diode capacitance is a key parameter that governs the noise in the front-end amplifier circuit, which is mainly associated with the thermal and flicker noise of the input MOS transistor. The input MOS transistor dominates the noise introduced by the readout electronics due to signal amplification in the preamplifier stage. Hence its optimization provides optimal sensitivity.
As illustrated in
The limitations on the spacing of the collector contacts arise from the following considerations. Firstly, the speed of response required of the PIN diode. The travel time of minority carriers must be shorter than the allowed integration time τint for the diode. For PIN diodes employed in optical communication this would be very restrictive limitation. However, for PIN diodes employed in imaging arrays, the integration time may be longer than 10 μs, perhaps as long as 1 ms and even longer.
The other limitation arises from the requirement that the travel time of carriers to the nearest contact must be shorter than the lifetime of carriers, which in the depleted diode region is typically limited by the Shockley-Read-Hall generation/recombination processes associated with deep-level impurities. The rate of these process, 1/τg, can be estimated from the measured density of the dark current in our PIN diodes, governed by SRH generation,
It has been found I=10 pA in 1 mm×1 mm diodes, i.e., J=1 nA/cm2. The intrinsic carrier concentration in our quaternary InGaAsP diodes was about 7×108 cm−3 based on the known ni=1.3×107 cm−3 of InP and the fact that the bandgap of our diodes has been designed to be 100 meV narrower than that of InP. Using Eq. (3) we find τg≈20 μs.
Thus, both of the limitations will be satisfied if the travel time τtr of holes over the distance s is about 1 μs or shorter. The transport of holes to the nearest collector contact proceeds by diffusion and drift. If the distances is very large, then the potential in the middle region between any two contacts is relatively flat and the transport is by diffusion. Since drift is faster, by assuming only diffusion an upper bound estimate for τtr or equivalently, the diffusion relation s2=Dτtr gives a lower-bound estimate for s. Taking D=10 cm2/s and τtr=1 μs, we find s≈32 μm, which is certainly an underestimate. More accurate estimate can be obtained by numerical simulation, solving the drift-diffusion equation for a given electrode geometry. Thus, the collector contacts can be safely spaced by 2s≈60 μm and perhaps by as much as twice that distance.
Referring now to
It is instructive to compare the hexagonal lattice of collector contacts, illustrated in
A
1=2s2√{square root over (3)}=(3/2)b2√{square root over (3)} A14s2=2b2
Referring now to
Quantitative analysis of the capacitance requires an accurate account of the fringing fields. Capacitance between a circular disc 22 of radius r and an infinite plane electrode 24 that is distance d apart, (see
where C0 is the elementary capacitance, calculated neglecting the fringing fields,
Here ε is the relative permittivity and ε0 the vacuum permittivity. To avoid misunderstanding, the “e” in the denominator under logarithm in Eq. (4) is the Euler number, so that ln(8πr/ed)≡ln(8πr/d)−1.
Eq. (4) and similar formulae were previously compared with the results of exact numerical calculations. They found that for r/d>2, equation (4) estimates the capacitance with virtually no error and even for r/d≈1 the error is less than 2%. This should be contrasted with the original Kirchhoff formula that corresponds to the first two terms in Eq. (4) and gives over 16% error already at r/d≈2. The exact numerical calculations lie very accurately on a straight line, in the entire range 0<d/r<2 that is of interest to us in the present invention. This empirical linear approximation is extremely convenient to use and its justification can perhaps be found by an analysis similar to that due to Rao1 and valid in the large-gap limit, d>r. The accurate linear interpolation formula can be written in the form:
which can be viewed as simply a sum of the elementary capacitance C0(d)=ε0επr2/d and the proper capacitance of a disk, C(r)=ε0ε8r. For d/r=1 equation (4) yields C(d)=3.469 C0 (d) and Eq. (6) similarly gives C(d)=3.5 C0(d). Obviously, the fringing field effect should not be neglected.
It should be noted that equations (4) and (6) apply to the case when the entire half-space above the ground plane is filled with a uniform dielectric. If the space above the disc 22 has a lower permittivity than that below the disk (assuming that the dielectric layer is infinitely extended laterally below the disk), then the fringing-field effects will be somewhat reduced. The effect can be taken into account quite accurately, (see
Referring now to
This case has been considered by Chew and Kong,2 who obtained the following result:
here ε is the relative permittivity and
For ε→1 one has A→1+lnπ and we recover Eq. (4). For ε≠1, there is a linear interpolation formula, similar in spirit to Eq. (6) and due to Wheeler,3 which gives an excellent approximation to Eq. (7):
For d/r≈1 and ε≈2 the correction is rather small, but the fringe contribution to the capacitance is indeed reduced. In the case of interest, the dielectric between the plates is InGaAsP (ε≈12.8) and the space above the disc is Si3N4 (ε≈7.5). In this case, the relative εrel≈1.71 and we find from (7) and (8) that C(d)=3.0 C0(d) for d/r≈1. Thus, tangible reduction has been obtained compared to the uniform case, where for d/r≈1 we had C(d)=3.5 C0(d).
Referring now to
The capacitance introduced by the metal runners 44 is a function of the runner width a, the thickness dox and relative permittivity εox of the interlevel dielectric 42 and the connection geometry. Minimizing the total length of the metal runners for a given collector contact array will not bring substantial results. However, it is worth noting that for the square lattice, the length of the runners 44 will be shorter than for the honeycomb structures. This is especially so, if the spacing s is kept constant. It has already been noted in connection with
It follows from Eq.(10) that for the same value of b, the hexagonal lattice is again preferable from the consideration of the shortest runner length. Previously, in connection with
The reason or a potential reduction of the runner length is primarily to minimize the parasitic capacitance due to the runner. In analogy with Eqs. (6) and (9), the parasitic capacitance can again be estimated as a sum of two contributions, an elementary parallel-plate capacitor of area aL, where a is the width of the runner, and the proper capacitance of the long wire. The former contribution is taken neglecting the fringing field, and is of the form.
The wire capacitance is approximately given by
The estimate of capacitance reduction is now presented in the instance of a preferred embodiment of the present invention, namely the design of a pixel for the epitaxial photoreceiver disposed on the surface of a semiconductor scintillator. This could be useful for either the cleaved-pixel or integrated-pixel designs, discussed in connection with the prior art arrangements illustrated in
For concreteness, estimates will be made for a pixel of area 1 mm×1 mm. If the p contact formed a continuous plate, the capacitance of such a diode, CCont Plate, implemented in InP with the depleted region d≈2 μm, would be about 50 pF. Instead we have the p contact in the form of an array of small discs of diameter 2r separated by the distance 2s.
The scintillator material is InP and the epitaxial photoreceiver is InGaAsP alloy of bandgap about 100 meV smaller than that of InP, so that the interband emission of InP is fully absorbed in the PIN diode. To estimate the capacitance we need to know the permittivity of the quaternary In1−xGaxAsyp1−y alloy lattice-matched to InP. The lattice-matched condition is important because otherwise dislocations will have a detrimental effect on the photoreceiver performance. For lattice-matched compositions (x=0.454y) the alloy bandgap can be determined4 by an interpolation according to Vegard's law EG(y)=1.35−0.72y+0.12y2, and the desired bandgap value EGPh=1.24 eV is achieved with x=0.07 and y=0.16. The permittivity of the quaternary alloy can be determined by a similar Vegard's interpolation,
ε(x,y)=(1−x)yεInAs+(1−x)(1−y)εInP+xyεGaAs+x(1−y)εGaP. (12)
using the literature values of the relative permittivity of binary semiconductors, εInAs=15.15, εInP=12.5, εGaAs=12.9, and εGaP=11.1, we find that for the quaternary alloy of interest the relative permittivity is εInGaAsP=12.82. We assume that the space above the discs is filled with silicon nitride, εSi
Consider, exemplarily, r=2 μm≈d and s=30 μm with honeycomb arrangement of the disc array. The reduced capacitance of the disc array is given by Eq. (9) times the ratio of disc area to the unit cell area,
The parasitic capacitance, due to the metallic runner of width a=2 μm over an interlevel dielectric (assumed SiO2, relative permittivity εox=3.9) of not too large thickness dox≈2 μm, will be estimated using Eq. (11a) and Eq. (10) for hexagonal lattice. This yields
It has been observed that both contributions are similar in magnitude and combined indicate a reduction by a factor of 25 over the continuous plate pixel. This is a conservative estimate based on the disc spacing limited by diffusion only. Taking into account drift will increase the possible spacing to at least a factor of 2. Therefore, it is expected that the technique will allow the fabrication of PIN diode pixel of 1 mm2 area with C≈1 pF, which is a 50-fold reduced capacitance, compared to that of a continuous 1 mm2 plate.
Referring now to
The traditional design of readout circuits is based on the assumption that the dominant noise sources are the shot noise of the detector and noise (thermal and flicker noise) of the input MOS transistor. The input MOS transistor dominates the noise introduced by the readout electronics due to signal amplification in the preamplifier stage. Hence its optimization provides optimal sensitivity.
For the optimal pulse shaping with the shaper time constant τ, the calculated equivalent noise charge (ENC) is given by
where CDET and CMOS are the capacitances of the photodetector and the MOS transistor, respectively, ILK is the leakage current and gm is the transistor transconductance. Here, ath, ash and af are dimensionless integration constants (of order unity) and Kf is the 1/f noise coefficient. The ENC quantifies sensitivity of the electrical readout circuitry in terms of the charge at the output of the detector that would produce a voltage signal at the output of the readout electronics equal to the noise contribution of both the detector and electronics.
Equation (15) shows the importance of the photodetector diode area in the noise budget. The shot noise contribution directly scales with the leakage current and the input MOS transistor noise directly scales with the detector capacitance. The design parameter is the shaper time constant, τ, which inversely scales the thermal noise contribution of the input transistor and directly scales the shot noise contribution of the detector. The shorter τ reduces the shot noise but exacts a penalty from thermal noise for increasing bandwidth.
In the traditional design, both the leakage current and the detector capacitance are expected to scale directly with the area. Smaller area would reduce both terms in the equivalent noise charge and this has been the main motivation of the present invention in pursuing the integrated prior art pixel design. The integrated-pixel detector design with 100-fold smaller pixel area leads to a dramatically lower limit of the detectable charge per pixel. However, the useful signal is also expected to be reduced (albeit by a smaller amount) because the scintillation photons, generated by a single gamma interaction a distance h away from the surface of detectors, will be shared by a number pixels within the area of about h2, as discussed in connection with Eqs. (1) and (2). Still another trade-off, involved in the integrated-pixel design, is rooted in the fact that each pixel must contain the electrical readout circuitry. With the decreasing detector size, the area becomes an important design parameter that has to be included into optimization of the input transistor.
In contrast, in the low-capacitance disk-array pixel, the reduction of capacitance occurs independently of dark current. One must therefore revise the approach to noise analysis, by taking the dark current as constant, while scaling the diode capacitance. The analysis must be carried in two steps. First, one must optimize the integration time (i.e., the shaper time constant, τ). As the capacitance is reduced, the shot noise form the PIN diode dark current stays the same, because the diode collection volume remains constant, while the amplifier noise, both thermal and flicker, are reduced with the diode capacitance. Therefore, the smaller the capacitance the shorter should be the integration time. Second, one evaluates the ENC for the optimum τ.
Such an analysis was carried out5 for an exemplary PIN diode of 1 mm2 pixel area. For the continuous plate pixel architecture, such a diode has a capacitance of approximately C=50 pF and the leakage current of ILK=10 pA at 1V reverse bias. Varying the capacitance C downward while keeping ILK constant, it was found that the optimum integration time scales down from about 22 μs at C=50 pF to about 2 μs at C=2 pF.
The value of 2 pF corresponds to the conservative estimates of Eqs. (13) and (14). The ENC is thereby reduced from about 250 electrons at 50 pF to about 50 electrons at 2 pF. Lowering the detectable charge to as low as 50 electrons in a 1 mm2 pixel is a dramatic improvement of the photo-detection system for the semiconductor scintillator.
The exceptional sensitivity resulting from the capacitance reduction—with no reduction in the collection volume—should be useful for a variety of imaging systems that must be sensitive to low levels of radiation.
It has been discussed hereinabove that the present invention provides a semiconductor photodiode having an active region which consists substantially of the first epitaxial semiconductor region 66, the base second epitaxial semiconductor region 64, and the third semiconductor region 78. The first semiconductor region is also provided with an arrangement or means for providing electrical contact thereto. The first semiconductor region 66 can be in the form of an emitter layer having a first type of conductivity. The second or base epitaxial semiconductor region 64 comprises a semiconductor layer which is in contact with the emitter layer 66. As to the third semiconductor region 78, it is arranged so as to be in contact with the base region 64 and comprises a plurality of separated collector regions 62 of a second conductivity type. The photodiode also includes a low capacitance conducting arrangement or means 76 for providing electrical contacts to all collector regions 62. The collector regions 62 are spaced apart from each other in the lateral direction of the semiconductor diode by the distance which is substantially greater than the width of the respective regions. It should be noted however, such distance is substantially short, so that travel time by the carriers of the second conductivity type from the farthest point between the collection regions to the nearest collection region being shorter than the life time of the carriers in the base region 66. The conducting arrangement 78/76 has capacitance which is lower than the combined capacitance of all collector regions 62. The emitter layer 66 of the first conductivity type is n-type conductivity layer, whereas the separated collector regions 62 of the second conductivity type are associated with respective holes. In one embodiment of the invention the collector regions 62 is an array which can be in the form of a honeycomb lattice. The collector regions 62 can be also formed having configuration of substantially circular disks.
The lower-capacitance conducting arrangement for providing electrical contacts to the collector regions 62 comprises a plurality of metallic runners 76 which are separated in the longitudinal direction of the semiconductor diode from the third semiconductor region 78 by an interlevel dielectric layer 72. In one embodiment of the invention the width of the runners 76 is less than the diameter of the respective collector regions 62. The lower-capacitance arrangement for providing electrical contacts to all collector regions further comprises via holes 75 in the interlevel dielectric layer 72. The via holes 75 are adapted to accommodate metal blogs 77 provided to link the collector regions 62 with the metallic runners 76,78.
The epitaxial PIN diode designs are shown in
Referring now to
Surface leakage is a known problem and it had been encountered and resolved in the prior art in the implementation of InGaAs avalanche photodiodes (APD) for optical telecommunications. In such devices the low dark current requirement is essential, similar to that of the invention. Initially, a preferred approach has been to avoid placing the cleaved surface under voltage. According to the present invention, to circumvent the problem of surface leakage, the pixel design has been changed, so that the surface is no longer under bias. The diodes produced in this way have a good performance from the standpoint of dark current. The reverse-bias leakage current, interpreted in terms of Eq. (3), corresponds to the carrier lifetime of 20 μs. Interpreted in terms of the Shockley-Read-Hall process, this implies a very low concentration NT<1013 cm−3 of deep-level traps in the depletion region of the diode. These fabrication principles will be described in the preferred embodiment of the method of the invention for manufacturing of the disk-array pixel, presented below.
The preferred fabrication sequence for manufacturing of the disk-array pixel in accordance with the method of the present invention is schematically illustrated in
The cross-section view of the structure after the diffusion step is illustrated in
Referring now to
Nevertheless the use lift-off technique is preferred for this operation. To do this, the structure is covered with the second dielectric layer 79, made of Si3N4 for example. The layer 79 is then patterned with the mask M2 in such a manner that holes 67 are produced concentric with the holes 65 of the M1 mask, but having smaller diameter. In the lift-off technique, p-metal is deposited while the resist is still on and then removed everywhere except in the above-mentioned holes 67. The same mask M1 can be used in this operation. However, it is preferable to use a different mask M2 having slightly smaller diameter features. This is because metal contacts 74 should only cover the p+ diffused regions 62 and the smaller-diameter features of the M2 mask mitigate the possible misalignment of the metal contacts.
The next step of the method of the invention is illustrated in
A further step of the method, illustrated in
Finally, by bonding or using solder or indium bumps, a contact pad for contacting the pixel is being provided. The metal pad is schematically shown by a dashed circle on the mask M4 (see
THIS NON-PROVISIONAL APPLICATION CLAIMS PRIORITY UNDER 35 USC 119 (e) OF U.S. PROVISIONAL APPLICATION SER. NO. 61/072,229 FILED BY DR. SERGE LURYI ON MAR. 28, 2008.
Number | Date | Country | |
---|---|---|---|
61072229 | Mar 2008 | US |