WO2006131235A1 - Interferometer for quantative phase contrast imaging and tomography with an incoherent polychromatic x-ray source - Google Patents
Interferometer for quantative phase contrast imaging and tomography with an incoherent polychromatic x-ray source Download PDFInfo
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- G01N23/00—Investigating or analysing materials by the use of wave or particle radiation, e.g. X-rays or neutrons, not covered by groups G01N3/00 – G01N17/00, G01N21/00 or G01N22/00
- G01N23/02—Investigating or analysing materials by the use of wave or particle radiation, e.g. X-rays or neutrons, not covered by groups G01N3/00 – G01N17/00, G01N21/00 or G01N22/00 by transmitting the radiation through the material
- G01N23/04—Investigating or analysing materials by the use of wave or particle radiation, e.g. X-rays or neutrons, not covered by groups G01N3/00 – G01N17/00, G01N21/00 or G01N22/00 by transmitting the radiation through the material and forming images of the material
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- G21K2207/005—Methods and devices obtaining contrast from non-absorbing interaction of the radiation with matter, e.g. phase contrast
Definitions
- the present invention relates to an interferometer for X-rays , in particular hard X-rays, for obtaining quantitative phase contrast images and measuring wavefront shapes.
- the cross section for absorption which gener- ates the contrast in conventional radiography, is usually much smaller than that for elastic scattering.
- the elastic scattering causes a phase shift of the wave passing through matter. If, for example, 17.5-keV x-rays (which are commonly applied for mammography) pass through a 50-um-thick sheet of biological tissue, the attenuation will only be a fraction of a percent, while the phase shift is close to ⁇ .
- the possibility to record the phase shift of x-rays opens the potential for greatly enhanced contrast and, in consequence, reduction of the applied x-ray dose. Reduction of the dose is desirable i) because of health risks for patients exposed to x-rays, and ii) because of the reduced exposure times .
- phase variations in the radiation behind the sample were developed in the past years. They can be classified into interferometric methods, techniques using an analyzer crystal, and free-space propagation methods. These methods differ in the nature of the signal recorded, the experimental setup, and the requirements on the illuminating radiation (especially its spatial coherence and monochromaticity) . Although some of them yield excellent results for specific problems, none is very widely used. In particular, none of them has so far found medical diagnostics applications, which require a large field of view of many centimeters, the efficient use of broadband radiation as provided by laboratory x-ray generators and a reasonably compact setup. In addition to medical applications, any investigation of low contrast objects, e.g., in biology or materials science could benefit from exploiting phase contrast. It should be mentioned that an object embedded in a matrix of the same absorption coefficient is completely invisible in absorption contrast, while for the same sample significant differences in phase shift may occur.
- the phase of a wave cannot be measured directly, so any conversion of a phase shift into an intensity modulation has to depend on interference of two (or more) waves.
- the waves need to have a well-defined phase relation in time and space, i.e. sufficient temporal (longitudinal) coherence and spatial (transverse) coherence.
- the commercial impact of an invention in context with radiography will greatly depend on whether an x-ray tube is suitable as radiation source or whether the method is restricted to use at synchrotron radiation facilities because of the required degree of coherence.
- a thorough understanding of the relevant terms and relations is essential to appreciate the advantages of the interferometer set-up according to the present invention.
- Temporal coherence is related to the monochromaticity of the ra- diation.
- the longitudinal coherence length is ⁇ 2 / ⁇ .
- these beams only have a well-defined phase relation if the difference in optical path lengths is shorter than the longitudinal coherence length. While for visible laser light ⁇ 2 / ⁇ can extend over many meters, it is only in the order of a micron at hard x-ray wavelengths even when a crystal monochromator ( ⁇ / ⁇ « 10 4 ; is used.
- Spatial coherence is related to the size and distance of the source.
- an intrinsically incoherent and chaotic source e.g. a light bulb or a conventional x-ray tube
- transverse size c emitting at a wavelength ⁇
- the wave-front phase difference between two points lying in a plane normal to the optical axis and separated by a distance r is well defined only if the condition r ⁇ - 1/c is fulfilled.
- interference effects such as those used in the grating-based interferometers can only occur when the coherence length is approximately equal to or larger than the relevant length scale of the diffraction aperture or phase mask.
- the transverse coherence length at a distance of 1 m from the source is again in the order of only one micron.
- an inter- ferometer for X-rays for obtaining quantitative phase contrast images
- an X-ray source preferably a standard polychromatic X-ray source
- a diffractive optical element preferably in transmission ge- ometry, that acts as a beam splitter
- a position-sensitive detector with spatially modulated detection sensitivity. This modulation acts as an analyzer for the interference pattern formed by the beam splitter; it can be integrated in the detector or separate from it.
- This interferometer unifies all the requested requirements in using only a conventional X-ray source instead of a synchrotron source and in using only two different grating structures, one for diffracting the x-rays having passed through the object to be investigated, and the other one for delivering the spatially modulated detection sensitivity.
- the beam splitter is a phase grating, that is, a line grating or a two- dimensionalIy structured grating with low X-ray absorption, but considerable X-ray phase shift, preferably with a phase shift of ⁇ or odd multiples thereof.
- the phase grating may be made by deep etching into silicon or a polymer.
- the modulation of the detector sensitivity can be achieved by a one- or two-dimensional grating structure with high X-ray absorption contrast, placed immediately in front of the detector.
- This analyzer grating may serve as an anti-scatter grid, or an anti-scatter grid can be used as the analyzer grat- ing.
- the absorption grating can be made by deposition of a heavy metal into the gaps of a low-absorbing structure.
- the distance between beam splitter and analyzer is chosen to be an odd fractional Talbot distance, given by the equation
- phase shift of the beam-splitter grating and the distance between beam splitter and analyzer can be adapted to a photon energy corresponding to an emission line of the X- ray generator used as the source.
- a mechanism can be included to vary the angular orientation around the optical axis of the beam splitter with respect to the analyzer.
- a one- or two-dimensional phase stepping scan can be implemented by lateral transverse movement of the radia- tion source and/or an aperture located in front of the radiation source, and/or of the beam splitter, and/or of the analyzer, and/or by a tilt of the interferometer with respect to the X-ray source.
- the detector can be designed as being position-sensitive in two dimensions, whereby the lateral dimensions of the beam splitter and the analyzer cover a significant portion of the active area of the detector.
- a collimator can be placed between the source and the beam splitter that limits the spatial extent of the illuminating X rays to a fan beam; a line- array detector and a mechanism can be comprised that allows a linear scan of the sample relative to the rest of the apparatus, perpendicular to the opening angle of the fan.
- This array of a sources may be generated by an aperture mask with line- or dot- shaped openings.
- the array of sources is generated by electron optics that creates an array of electron line or dot foci on the anode of the X-ray source. This can be achieved i.e.
- the array of sources can be generated by using an X-ray source comprising an anode which is structured either topographically or has assem- bled in a mosaic manner from different materials.
- means for rotating the sample relatively to the remaining components can be comprised in order to perform data collection for a tomography scan.
- the scanning techniques can be carried out by implementing an analysis procedure for phase-stepping scan data that comprises the steps of calculating for each ele- ment of the detector the Fourier transform or at least one Fourier component of the intensity curve measured in the element, and then retaining the phase of one or more Fourier components as a signal for further processing.
- an analysis procedure can be implemented for phase- stepping scan data that comprises the steps of fitting for each element of the detector the intensity curve measured in the element to an intensity curve modeled or measured separately without the beam distortions under study, where at least one of the fit parameters is the shift of the curve along the position axis of the scan.
- Figure 1 a schematical view on a two-grating interferometer according to the present invention
- Figure 2 a schematical view on Talbot self-imaging of a linear phase grating and moire fringe formation using the interferometer according to Figure 1;
- Figure 3 a schematic view on Moire interferometry
- Figure 4 a schematic view on the principles of the phase stepping technique used with the interferometer according to figure 1;
- Figure 5 tomography images obtained with phase stepping interferometry FIG. 5
- Figure 6 a schematic view on four different options to obtain phase stepping movement for the two grating interferometer according to Figure 1;
- Figure 7 a schematic view on the cone-beam problem and a number of solutions for it;
- Figure 8 a schematic view of a two grating interferometer implemented in a scanning x-ray imaging system, whereby two possible orientations of the grating lines with respect to the fan beam are shown,-
- Figure 10 a schematic view on a grating interferometer with an array of line sources
- Figure 11 a schematic view on a grating interferometer with a source grating
- Figure 12 X-ray images of a test sample containing aluminum and plastic spheres, recorded with polychromatic radiation from a standard laboratory x-ray source.
- the basis of the present invention is the two-grating interferometer as it is shown in figure 1. It comprises the following components: an x-ray source XS (e.g. a stationary or rotating anode with a typical electron energy in the range of 10 to 100 keV, or any other X-ray source) , an optional set of appropriate filters F, an object O, a beam splitter phase grating Gl, an analyzer amplitude grating G2, and a spatially resolving x-ray detector D.
- the source XS provides some degree of spatial coherence at least in one direction perpendicular to the optical axis A.
- the anode material should be chosen to have appropriate lines in the energy range well suited for the specific application.
- these could be Nb, Mo, Rh, Pd, Ag, which have K-emission lines in the 15 to 25-keV region.
- the energy would be in the range of 5-10 keV (e.g. a Cu anode) .
- the spectrum of the source XS may be filtered to reduce the source bandwidth. The coherence requirements are defined in more detail further below.
- the beam splitter grating Gl with a period pi should be constructed such that it divides the incoming beam essentially into the two first diffraction orders .
- the conditions for this are that the grating lines have little absorption and shift the phase of the radiation passing through the grating lines by an odd multiple of ⁇ , and that the width of the phase-shifting structures is close to half of the grating period, i.e., that the grating has a duty cycle close to 0.5.
- the angle between the two diffracted beams is so small that they overlap almost completely.
- the diffracted beams interfere and form linear periodic fringe patterns in planes perpendicular to the optical axis A at a distance d downstream of Gl.
- the period of the interference pattern is equal to
- the period of the interference fringes is about half of the period of Gl. Neither the period nor the lateral position of these fringes depends on the wavelength of the radiation used. Perturbations of the incident ⁇ wave front, such as those induced by refraction on a phase ob- ject in the beam, lead to local displacement of the fringes.
- a fundamental idea for the operation of the grating-based interferometer described here is to detect the positions of the fringes and determine from these the shape of the wave front.
- an analyzer grating G2 with absorbing lines and the same periodicity p2 and orientation as the fringes is placed in the detection plane, immediately before the detector.
- the transmission of the absorber lines should be as low as possible, and the width of the absorber lines should be close to the width of the gaps in between them (duty cycle close to 0.5) to give optimum performance.
- This analyzer grating G2 acts as a transmission mask for the detector D and transforms local fringe position into signal intensity variation.
- the detected intensity signal contains quantitative information about the phase shift induced by the object 0. At least three methods can be applied to extract this phase information:
- a local distortion of the interference fringes will cause a change in the local transmission proportional to fringe distortion.
- a phase object introduced upstream of the gratings will cause a distortion of the transmitted wave front that in turn will cause a distortion of the interference fringe pattern. It can be shown, that this distortion is proportional to the derivative of the phase shift induced by the object O.
- the recorded image is therefore a differential phase contrast image. If required, a phase contrast image can be obtained by integration of the dif ⁇ ferential phase contrast image in the direction perpendicular to the grating lines.
- the recorded image contains possible absorption contrast and contrast from diffraction of edges inside the object 0. Both are difficult to distinguish from the (differential) phase contrast contribution, ii)
- the method requires an exact alignment of the interference pattern with respect to the analyzer grating lines over the whole field of view. This may be difficult to obtain especially for large fields of view, and even impossible when either the interference fringes or the grating lines are distorted due to mechanical imperfections of the set-up or fabrication errors of the gratings .
- the fringes are displaced with respect to the plane wave parallel to the optical axis (Fig. 2c, d) .
- the moire fringes are inclined (Fig. 2f) . From the local positi- ons of the moire-fringe maxima or from the local moire-fringe inclination, the derivative of the wave-front phase profile can be obtained relatively simply.
- the relationship between the lateral moire-fringe displacement ⁇ y and the wavefront phase 0 is
- FIG. 3 shows an example of experimental data and a preliminary analysis.
- the choice of the inclination angle a of the two gratings is determined by a tradeoff between spatial resolution and sensitivity.
- the spatial resolution in the direction normal to the moire fringes cannot be much better than one moire-fringe period P 1n . Since Pm decreases with increasing a (Eq. 2), stronger tilt means better spatial resolution. But Eq. 3 shows that the sensitivity decreases with increasing tilt, i.e., for a given phase gradient the moire fringes are less displaced for stronger a.
- the main advantage of moire operation of the interferometer is that pure phase information, without any unwanted absorption contrast, can be obtained from a single image.
- the main disadvantage is that the resolution in the direction parallel to the grating lines (normal to the moire fringes) is at least one order of magnitude poorer than the pixel size of the detector.
- Phase stepping - A third method that avoids the disadvantages of the approaches described above is the following: to separate the phase information from other contributions to the signal, such as absorption in the sample, inhomogeneous illumination or imperfections of the gratings, the phase-stepping approach used in visible-light interferometry was adapted to this setup. It is illustrated in Figure 4: one of the gratings is scanned along the transverse direction perpendicular to the grating lines over one period of the grating, and for every point of the scan an image is taken ( Figure 4a to d) .
- the intensity signal I(x,y) in each pixel (x,y) in the detector plane oscillates as a function of Xg ( Figure 4e) .
- the phases of the intensity oscillations in each pixel, ⁇ (x,y) ( Figure 4f) are related to the wavefront phase profile ⁇ (x,y) by
- phase profile of the object can thus be retrieved from ⁇ (x,y) by a simple one-dimensional integration, as shown in Figure 4g.
- the background phase distribution ⁇ ba c k te/y ⁇ should be measured with the object O removed from the beam and then subtracted.
- phase unwrapping is generally not necessary because the measured quantity cp, essentially the first derivative of ⁇ (Eq. 4) , will not exceed ⁇ as long as the phase gradients in the sample are not too steep.
- Figure 5 shows processed radiographs a(x,y) and ⁇ (x,y) obtained by phase stepping, the integrated phase shift ⁇ (x,y) , as well as reconstructed tomograms of both the absorption and the phase signal and a three-dimensional rendering of the tomographically reconstructed refractive index of the sample, a small spider.
- the edge-enhanced absorption image a (x,y) shows strong contrast for fine details both in projection (fig. 5a) and tomogram (fig. 5d) . But low spatial frequencies of the phase distribution are lost, so that image segmentation, i.e., the assignment of each pixel or voxel to one of the constituent materials of the sample, is not easily possible.
- the phase tomogram (fig.
- the source can be moved either mechanically or by deflecting the electron beam of the x-ray source to move the position of the electron impact on the anode.
- the movement of the source point also has a larger component along the optical axis .
- the component perpendicular to the optical axis has an effect on the phase stepping.
- the total deflection of the beam on the anode surface is in this case larger reducing the requirements on the accuracy of the electron beam movement.
- a phase-stepping scan yields, for each pixel in the detector, a series of intensity values from which different quantities can be extracted, especially the phase ⁇ of the intensity oscillation in each pi- xel, which is related to the derivative of the wavefront phase ⁇ by eq. (2), and the average intensity a over an oscillation period, which essentially corresponds to the non-interferometric X-ray image.
- phase ⁇ of the intensity oscillation in each pi- xel which is related to the derivative of the wavefront phase ⁇ by eq. (2)
- the average intensity a over an oscillation period which essentially corresponds to the non-interferometric X-ray image.
- the range of the phase stepping scan should cover (at least) one period of the oscillation.
- the optical components are usually designed such that the contrast curve (as shown, e.g., in Fig. 4e) is sinusoidal. In that case it is sufficient to take three points in a scan.
- the tangent of the phase ⁇ of the oscillation is then easily calculated by just taking the ratio of signal differences.
- the situation in the X-ray interferometer differs from the conventional one in that the shape of the contrast curve is not sinusoidal. (For the ideal case of box-profile gratings and fully coherent illumination, it would, for example, be triangular.) There are at least two ways to cope with this problem:
- phase-stepping scans with a larger number of points per oscillation period.
- the phase of the first component of the Fourier transform represents the oscillation phase ⁇ (wrapped into a half-open interval of width ⁇ ) .
- the minimum number of points in the phase-stepping scan for this type of analysis should be the number of the highest Fourier component of non-negligible intensity, plus 2.
- phase-stepping scans can be performed with few points in the scan, and the phase ⁇ determined by using the calibrated contrast curve, for example with a fitting procedure.
- the first method has the drawback of more necessary points per phase-stepping scan, but the advantage that higher Fourier components can potentially be used to extract additional informa- tion.
- the distance d between the two gratings can be chosen freely, although there are values of d for which the contrast is best and others for which it has a minimum (see below) .
- the sensitivity of the method increases linearly with d.
- the choice of larger d may result in a loss of spatial resolution due to penumbral blurring, as the distance between the object and the detector is increased.
- a higher degree of lateral coherence is required (see below) .
- the contrast of the interference fringes changes periodically as a function of d.
- any distance d n n P 1 2 I (8 ⁇ ) as the " ⁇ -th fractional Talbot distance” and to the planes at a distance d n from the phase grating as the "n-th fractional Talbot plane” .
- the expression above for the fractional Talbot distances has to be modified to d a n,sph. ⁇ i l d j" - ⁇ i-»-Px 2 l ⁇ &) ( 5)
- phase shift of the lines of the grating Gl depends on the photon energy due to the dispersion of the grating material.
- the condition to induce a phase shift e- qual to odd multiples of ⁇ is not strict, and a radiation within a certain energy band in the order of ⁇ 10% around the design e- nergy can be accepted.
- a deviation from ⁇ only affects the contrast - but it does not change the interference pattern qua- litatively.
- position of the Talbot planes depends on the photon energy.
- the refractive index of the object depends on the photon energy used. Nevertheless, re-constructed phase projections and tomograms will still be quantitative under the condition that the elements contained in the sample have no absorption edges in the range of the used photon energy band. In this case, all parts of the sample have the same dispersion relation, i.e. the real part of the refractive index changes with E '2 .
- the considerations of the previous sections show that the phase shift induced by the structures of the grating G2 should be close to odd multiples of ⁇ and that the distance between the grating Gl and the grating G2 should be close to an odd frac- tional Talbot distance d n , S ph.
- both, phase shift and fractional Talbot distance depend on the wavelength of the radiation used. It is therefore important that the grating structures and the distance chosen between the grating Gl and the grating G2 are matched to each other, meaning that both fulfill the conditions for the same wavelength. Moreover, it might be useful if this wavelength coincides with an emission line of the anode material of the used x-ray source. As mentioned above, the acceptable bandwidth is wide compared to other interferometric methods . In particular, it is wide enough to accept a series of emission lines (e.g. the Cu-K ⁇ i, Cu-K ⁇ 2 and Cu-K ® - lines emitting at
- the use of a smaller source will increase the spatial coherence, resulting in an improvement of the phase contrast.
- a line source can be used.
- the grating G2 comprises structures that are 5 to 10 microns thick - depending on the photon energy used -to provide sufficient x-ray absorption and that have, at the same time, widths on the order of one micron.
- the aspect ratio of the structures is therefore usually much greater than unity.
- the grating G2 can therefore also act as an anti-scatter grid.
- the anti-scatter grid of an x-ray imaging system may be used as the analyzer in a grating based interferometer, although this would require that the period of the anti-scatter grid be smaller than is the case in commonly available systems.
- the divergence angle of the x-ray beam is considerable, as the source cannot be placed at distances too far from the detector. Due to the high aspect ratio of the grating structures in the interferometer, especially of the grating G2, the beams in certain regions close to the edges of the field of view may pass through the gratings under too large angles . Only the angular component within the drawing of the lower part of figure 1 has an effect. To completely avoid this problem, the grating structures have to be bent or curved as depicted in Fig. 7a to d, or a scanning scheme with appropriate orientation of the gratings has to be applied.
- Fig. 7a illustrated a solution by bending the grating lines on a flat substrate.
- Fig. 7c) schematically depicts the grating lines being placed on a curved surface.
- Fig. 7d) shows a way that segments of a flat grating approximating the curved or bent geometry.
- a slit S placed between the source XS and the sample O generates a fan-shaped beam, and a one-dimensional line detector Di can be used, with its elements aligned to the fan.
- the two dimensional projection of the sample O is obtained by either scanning the sample through the fan- beam, or by scanning the beam across the sample and moving the line detector Di with the beam.
- the detector Di is read out at different positions during the scan and a two-dimensional image is created line by line.
- the scanning scheme has some important advantages compared to a two- dimensional setup: i) a suppression of diffuse scattering with- out an anti-scatter grid, since the slit S, together with the limited size of the source spot, acts as a collimator, ii) lower cost and higher detection efficiency of one-dimensional detectors in comparison with two-dimensional detectors.
- the grating based phase contrast can also be applied to a scanning scheme, as shown in Figure 8. The advantage is that only gratings over a smaller area are required compared to a full-field imaging scheme, which will significantly reduce the cost.
- Figure 9 shows x-ray images of a test sample containing polymethylmethacrylate (PMMA, 1.5 mm diameter) and Aluminum (1.0 mm diameter) spheres.
- the detector was a fiber-coupled CCD (model "Hystar", manufacturer Photonic Science) with an effective pixel size of approximately 30 ⁇ m. The data were acquired by phase stepping with 17 steps over 1 oscillation period, with an exposure time of 50 s for each CCD frame.
- the x-ray source that consists of an array of N line sources.
- the line sources are oriented along the grating lines and the width of each source line is chosen narrow enough to provide sufficient spatial coherence in the direction perpendicular to the grating lines.
- each of the line sources is intrinsically coherent, whereas the lines can be mutually inco- herent.
- the spacing of neighboring source lines i.e. the period Po of the source array is chosen such that the shift of the interference patterns created by two neighboring virtual line sources along the direction perpendicular to the grating lines is exactly p 2 .
- the arrangement also works for source array periods that are integer multiples of po-
- the size c of the source array can be much bigger than the width s of an individual line source.
- the duty cycle DC s / po of the source array determines the degree of transverse coherence in the direction perpendicular to the interferometer grating lines.
- the interference patterns of all N virtual line sources add up incoherently (as the virtual line sources are mutually incoherent) but preserving contrast.
- a source array as described above can be obtained in various ways :
- the simplest method is to put an array of slits, i.e. an amplitude grating in front of a large x-ray source to generate an array of virtual line sources.
- a schematic view of such a set-up is shown in figure 11.
- the open fraction, or duty cycle, DC of the source grating determines the degree of spatial coherence.
- the contrast of the phase images is improved at the cost of reduced flux density.
- the considerations described in the previous sections in context with the two grating interferometer with a single source are also valid for the setup with an arrayed source.
- the possibility to perform a phase stepping scan by moving the source has to be generalized in this case: it is the entire array of sources that should be moved for phase stepping. When an array of slits is used to create the source array, then that slit-array aperture should be moved together with the source, or it may even be moved alone, with the source remaining fixed in space.
- Figure 12 shows images obtained under the similar conditions as those shown in figure 9, i.e., with a laboratory X-ray source. The important difference is that this time a source with a size of 0.8 mm x 0.4 mm was used, which is far to large to provide sufficient transverse coherence for interferometric phase contrast.
- a source with a size of 0.8 mm x 0.4 mm was used, which is far to large to provide sufficient transverse coherence for interferometric phase contrast.
- phase contrast x-ray imaging configurations particularly suited for phase contrast x-ray imaging are listed in detail. They are designed for two different applications: desktop microtomography and mammography. The latter can be implemented either with a full-field setup or a scanning setup.
- a grating based interferometer for phase contrast desktop tomography system may consist of the following components :
- Suitable anode materials include Ti, V, Cr, Mn, Fe, Co, Ni, Cu, and Ge.
- the number of pixels of the detector should be between 500x500 and 4000x4000, typically 2000x2000.
- the field of view of the detector should be between 5 and 30 mm, typically 10 mm.
- the pixel size of the detector is thus typically 5 ⁇ m x 5 ⁇ m.
- the center of the detector and the center of the source define the optical axis.
- the optical axis can be in any di- rection, but a horizontal axis is most advantageous.
- a rotatable sample holder with the axis of rotation perpendicular to the optical axis is placed between the source and the detector so that a sample can be mounted with its center of gravity close to the optical axis.
- the distance between the sample and the source is called a
- the distance between the sample and the detector is called b.
- the phase grating and the absorption grating are placed directly in front of the detector.
- the period p 2 of the analyzer grating should be chosen smaller than the detector pi- xel size, so that the spatial resolution of the detector can be fully used.
- a grating depth of 10.2 ⁇ m is required to obtain a phase shift of ⁇ .
- the intensity trans- mission of 10.2 ⁇ m of Si is 86.6 %, so that the transmission of an Si grating with that thickness and a duty cycle of 0.5 would be 93.3 %.
- PMMA polymethylmethacrylate
- the ideal grating depth is 18.7 ⁇ m.
- the intensity transmis- sion of such a grating would be 99.3 % (for a duty cycle of 0.5).
- the use of other polymers would result in similar figures.
- For the absorption grating if gold is used as the material, a thickness of 6 ⁇ m would ensure an absorption of more than 90 %, and 12 ⁇ m thickness would result in more than 99 % of absorption in the grating lines.
- a grating based interferometer for a phase contrast full-field digital mammography (FFDM) system could consist of the following components :
- Anode materials could be Nb, Mo, Rh, Pd, or Ag.
- the design of the entire apparatus can be based on that of common (absorption-contrast) FFDM systems, with the source array, beam splitter and analyzer as new, different elements .
- a filter of Pd or Rh or another material with an x-ray ab- sorption edge in the 23-30 keV energy range and a thickness between 20 and 100 ⁇ m, typically 50 ⁇ m may be used to suppress unwanted parts of the spectrum.
- a gantry with compression paddle as commonly used in mammography screening systems comprises a two-dimensional digital flat-panel x-ray detector, placed at a distance of 0.5-1.0 m from the source, just below (i.e., downstream of) the gantry.
- 1.0 m as the distance was used.
- the field of view of the detector should be not much smaller than (200 mm) 2 ', preferably around 240 x 300 mm 2 ' (i.e., the size of the largest commonly used film cassette in conventional mammography) .
- the pixel size of the detector is typically between 50 and 100 ⁇ m in each dimension, so that the detec- tor has between (2500) 2 and (5000) 2 pixels. (These are the characteristics of most commercially available detectors for FFDM.) Here, a pixel size of 70 ⁇ m is assumed.
- p 2 3 ⁇ m (period of the analyzer grating)
- pi 8.4 ⁇ m (period of the phase grating)
- po 26.6 ⁇ m (spacing of the virtual line sources).
- the total size of the source array should, with these parameters, not exceed 0.4 mm, i.e., the maximum number of virtual line sources is 15.
- phase grating if nickel is used as the material, the thickness required to achieve a phase shift of ⁇ is 7.7 ⁇ m, resulting in an average intensity transmission of 92.6 % (for a duty cycle of 0.5).
- the analyzer grating if made of gold, should have a minimum thickness of 20 ⁇ m, which yields absorption of 90 % in the grating lines .
- the source material, distances and grating periods can be chosen similar or identical to the FFDM example above.
- the following items would be different or additional with respect to the FFDM setup: • A first collimator (one slit or a sequence of slits), made of a strongly absorbing material, should be mounted between the source and the object position. Together with the spots of an arrayed virtual source, this collimator defines a fan-shaped beam. • A second collimator slit, made of a strongly absorbing material, should be mounted just above (i.e., upstream of) the interferometer gratings .
- the detector can be a line-array detector, for example a direct-detection detector.
- the detector elements should ha- ve non-square shape, with a size between 25 and 100 ⁇ m
- the collimator slits, the interferometer gratings and the detector should be parallel to each other.
- the lines of the interferometer gratings should be parallel to the fan- opening plane .
- the collimators and the detector can be rotated around the source array, perpendicular to the fan-opening plane, over an angular range large enough to cover one dimension of the field of view mentioned in the FFDM setup. For the acquisition of a mammogram, these components will be scanned to- gether .
- phase grating is four times more efficient. Nonetheless, for a number of applications where these drawbacks can be tolerated and/or where a phase grating is not available, the use of an absorption grating as beam splitter can make sense.
- n ' n p ⁇ 2 / ⁇ for a plane illuminating wave and /- « constructive l-n-p ⁇ IA for a spherical wave, which replaces Equation (5) .
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Publication number | Publication date |
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CN101257851B (en) | 2011-06-15 |
US7889838B2 (en) | 2011-02-15 |
CA2610934A1 (en) | 2006-12-14 |
CN101257851A (en) | 2008-09-03 |
US20090092227A1 (en) | 2009-04-09 |
AU2006257026B2 (en) | 2010-03-04 |
EP1887936B1 (en) | 2013-12-25 |
JP5162453B2 (en) | 2013-03-13 |
EP1887936A1 (en) | 2008-02-20 |
AU2006257026A1 (en) | 2006-12-14 |
JP2008545981A (en) | 2008-12-18 |
CA2610934C (en) | 2014-09-30 |
EP1731099A1 (en) | 2006-12-13 |
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