## Abstract

We recently demonstrated how quantitative X-ray phase contrast imaging may be performed with laboratory sources using the coded aperture technique. This technique required the knowledge of system parameters such as, for example, the source focal spot size and distances between elements of the imaging system. The method also assumes that the absorbing regions of the apertures are perfectly absorbing. In this paper we demonstrate how quantitative imaging can be performed without knowledge of individual system parameters and with partially absorbing apertures. We also show that this method is analogous to that employed in analyser based imaging which uses the rocking curve of an analyser crystal.

© 2013 Optical Society of America

## 1. Introduction

Coded aperture X-ray phase contrast imaging (CAXPCI) [1] was initially inspired by the synchrotron method known as analyser based imaging (ABI). ABI develops contrast using the rocking curve of an analyser crystal [2]. Algorithms were developed to extract sample phase and absorption from images taken on two opposing sides of the analyser crystal rocking curve [3, 4]. Algorithms employing a variety of assumptions about the sample and imaging system, and later, for more general systems were subsequently developed [5–8]. Although this technique has been demonstrated using a laboratory source [9], it is generally restricted to synchrotron sources due to the narrow band of energies selected by the two crystals employed in the imaging system.

The restriction to synchrotron sources for applications not compatible with long exposure times motivated several people to develop alternative methods of performing X-ray phase contrast imaging (XPCI) using laboratory sources [1, 10–12]. It is beyond the scope of this paper to review the substantial number of contributions to this field, however we direct readers to a review on the subject [13] for such an account. One such contribution resulted from initial experiments performed using the SYRMEP beamline of the Elettra synchrotron radiation facility in operation in Trieste [14], an experiment directly inspired by analyser based imaging. Although initially demonstrated using synchrotron radiation, the technique was soon demonstrated using laboratory sources [1]. Recently this technique has been extended to a quantitative method for both laboratory [15] and synchrotron sources [16].

The CAXPCI system is schematised in Fig. 1(a) where all parameters are defined in the figure caption. Phase contrast images are obtained by adjusting the position of A_{1} with respect to A_{2} such that the beams formed by A_{1} illuminate the edges of the A_{2}. A_{2} is initially aligned with the detector pixels and remains stationary thereafter. Higher resolution images may be obtained by scanning the sample in the *ξ* direction as indicated in Fig. 1(b). CAXPCI imaging can be performed with synchrotron radiation [16] or laboratory sources [15]. The is no limit on the spectral width of the source so long as the apertures are thick enough to generate contrast in the detected signal, in the absence of a sample, which exceeds the noise. The focal spot size should not exceed the pixel size of the detector [17]. The system has recently been shown to have sensitivity which is at least comparable to that of grating interferometry [18], the only other system to offer high phase sensitivity when employing a laboratory source. The difference between grating interferometry and CAXPCI has been discussed in detail previously [17]. However, we note that the main difference is that CAXPCI employs the edge illumination principle where the edges of the sensitive region of a pixel are illuminated by X-ray beams. This means that CAXPCI doesn’t make use of Talbot’s self-imaging phenomenon and doesn’t employ phase stepping of the detector aperture.

The existing quantitative method [15] was developed from a wave optical model of the CAXPCI system which took into account the principal system parameters such as source focal spot size and aperture dimensions and spacing. This technique thus requires such system parameters to be known to a reasonable degree of accuracy. However, some system parameters such as, for example, the source focal spot and spectrum are difficult to measure on a regular basis. It would be much more convenient if the effect of all system parameters could be aggregated into a single series of measurements, thus forming a simple method of calibrating the imaging system. We present such a method in this paper whereby a measurement, analogous to the rocking curve in ABI, is performed which forms the basis of the algorithm used to obtain quantitative phase measurements. We shall call this measurement the translation curve (TC) in order to distinguish it from the rocking curve used in ABI. We shall show in this paper how the measured TC may be used to perform quantitative phase imaging in a more general manner than our previously developed method.

## 2. Theory

#### 2.1. Derivation of expression for the translation curve

In this section we develop a forward model which allows the detector pixel signal to be calculated taking into account the salient system parameters. This formula is then used to obtain an expression for the TC of the system. We begin by mathematically defining the transmission function of the apertures as:

*i*takes the value 1 or 2 in correspondence with the apertures A

_{1}and A

_{2}respectively.

*μ*is the energy dependent linear absorption coefficient of the absorbing material used to form the apertures (generally gold),

_{ca}*T*is the thickness of the absorbing material and

_{i}*η*is the fraction of each aperture period which is non-absorbing. The sample is modelled by a multiplicative complex transparency function:

_{i}*μ*is the linear absorption coefficient of the sample,

*k*is the wave number,

*ϕ*(

*x*) = ∫

*(*

_{𝒪}δ*x*,

*z*)d

*z*,

*δ*is the refractive index decrement of the sample and

*𝒪*is the extent of the sample.

*ϕ*and

*μ*both depend upon the photon energy, however, we develop the mathematical model by considering first a single energy before integrating over the source spectrum. Note also that the sample is assumed to satisfy the projection approximation, meaning that the sample is sufficiently thin and that inhomogeneities are large compared with the wavelength [19]. In this context, one criterion for being sufficiently thin is that the thickness is much less than z

_{so}[20] although Paganin [21] presents a thorough discussion of this subject.

We now proceed to calculate the signal detected by each pixel assuming a monochromatic point source. We shall generalise to an extended, polychromatic source later. By applying the paraxial approximation to the Fresnel-Kirchhoff diffraction integral, we follow a previous publication [16] in evaluating the complex amplitude incident upon the detector aperture as

*U*

_{0}is defined implicitly by noting that the point source is assumed to emit a spherical wave, prior to applying the paraxial approximation, of the form

*U*

_{0}exp(

*ikr*)/

*r*where

*r*is the distance from the source.

Without loss of generality, we consider the signal of the pixel bound by |*x*| < *P*/2. Then the signal detected by this pixel is given by

*T*(

*x*) as

*ϕ*is thus the derivative of

_{x}*ϕ*with respect to

*x*and corresponds to the angle by which a ray is refracted by the sample. It is important to note that the coded aperture technique, like grating interferometry, measures refraction angle which, when multiplied by the wavenumber, yields the phase gradient. To avoid confusion arising due to the choice of wavenumber when employing a polychromatic source, we shall principally analyse refraction angle rather for the remainder of this paper.

In order to proceed, we substitute *T̃*(*x*) for *T*(*x*) into Eq. (3) and apply the stationary phase approximation in a manner similar to previous publications [16, 22]. The first order asymptotic solution to Eq. (3) is thus given by:

*S*(

*x*), at the target and the source spectrum and detector characteristics can be represented by a weighting

_{s}*σ*(

*E*), the detector signal for an extended, polychromatic source may be obtained as [22]:

*S*applies only to

*𝒯*

_{1}since, formally, the argument

*x*of

*𝒯*

_{1}is written as

*x*+

*x*z

_{s}_{od}/z

_{so}where

*x*is a position within the source focal spot [22]. Since

_{s}*x*only appears in the argument of

_{s}*𝒯*

_{1}, the convolution with

*S*applies only to

*𝒯*

_{1}. As a final step, we note that it is possible to consider the polychromatic system as being equivalent to a monochromatic system at an equivalent or effective energy, to a good degree of accuracy [23]. We note also that this assumption was integral to one of the first demonstrations of quantitative phase imaging with polychromatic sources using a grating interferometer [11]. As a result we simplify Eq. (9) further to

*μ̄*and

*ϕ̄*for brevity. We have now derived the key theoretical result of this paper. To further elucidate this result, consider Eq. (10) in the absence of a sample, which we write as:

_{x}*I*

_{TC}denotes the TC as it is obtained by translating the pre-sample aperture with respect to the detector aperture. We can then relate the pixel signal obtained with a sample in place to the TC as:

*μ̄*and

*ϕ̄*.

_{x}#### 2.2. Design of system parameters to enable quantitative imaging

So far we have shown how a sample phase gradient, sample absorption and position of the pre-sample aperture affect the pixel signal. Now we show how this relationship may be inverted. Since we intend to determine two quantities, two measurements are required which correspond to different values of Δ*ξ*, the values of which we now derive. Our strategy is to obtain two values of Δ*ξ* which will enable the absorption term to be factored out of Eq. (10). In particular, we acquire two images, *I*_{1} and *I*_{2} corresponding to two positions of the pre-sample aperture, Δ*ξ*_{1} and Δ*ξ*_{2} respectively. In order to extract the absorption term from sum of *I*_{1} and *I*_{2} we must thus find Δ*ξ*_{1} and Δ*ξ*_{2} which results in

_{od}

*ϕ̄*(0) varies. We thus seek values of Δ

_{x}*ξ*

_{1}and Δ

*ξ*

_{2}which minimises |

*F*′(z

_{od}

*ϕ̄*(0))| everywhere. Within the domain

_{x}*x*∈ [−

*P*/2,

*P*/2],

*𝒯̄*

_{1}′(

*x*) is well approximated by

*𝒯̄*

_{1}′(

*x*) =

*δ*(

*x*+

*η*

_{1}

*P*/2) −

*δ*(

*x*−

*η*

_{1}

*P*/2), where in this case,

*δ*refers to Dirac’s delta function. Thus our task reduces to minimising the expression:

*x*̃

_{1/2}= z

_{od}

*ϕ̄*(0) +

_{x}*x*−

*M*Δ

*ξ*

_{1/2}+

*η*

_{1}

*P*/2. This expression cannot be made equal to zero in general. In order to proceed we assume only that

*S*(

*x*) is symmetric about

_{s}*x*= 0 and that it has its maximum value at

_{s}*x*= 0. By noting that the convolution operator results in four shifted and scaled replicas of

_{s}*S*, we select Δ

*ξ*

_{1}and Δ

*ξ*

_{2}such that two of them cancel and the other are shifted principally to where

*𝒯̄*

_{2}(

*x*) has a small magnitude. The symmetry of these two criteria dictates a choice of Δ

*ξ*

_{1}= −Δ

*ξ*

_{2}and equating −

*δ*(

*x̃*

_{1}−

*η*

_{1}

*P*/2) +

*δ*(

*x̃*

_{2}+

*η*

_{1}

*P*/2) = 0 gives the result Δ

*ξ*

_{2}=

*η*

_{1}

*P*/(2

*M*) = Δ

*ξ*

_{0}which is in agreement with our previous inversion technique [15] and thus defines the quantity Δ

*ξ*

_{0}.

As a final step before deriving the inversion formulae we show that |*I*_{TC}′(Δ*ξ*)| is maximised at Δ*ξ* = ±Δ*ξ*_{0}. To proceed we note that *I*_{TC}′(Δ*ξ*) is given by

*S*, only that it is centred and maximised on

*x*= 0, we conclude that |

_{s}*I*

_{TC}′(Δ

*ξ*)| is indeed maximised at Δ

*ξ*= ±Δ

*ξ*

_{0}since this maximises the overlap between one of the

*S*terms with the

*𝒯̄*

_{2}(

*x*) term and minimises the overlap with the other.

#### 2.3. Derivation of inversion formulae

We are now ready to derive the inversion formulae. In particular, we form images

*ξ*

_{0}is chosen such that I

_{TC}(−Δ

*ξ*

_{0}− z

_{od}

*ϕ̄*/

_{x}*M*) + I

_{TC}(Δ

*ξ*

_{0}− z

_{od}

*ϕ̄*/

_{x}*M*) is approximately constant, and thus approximately equal to 2I

_{TC}(Δ

*ξ*

_{0}), which allows ∫

*d*

_{𝒪}μ̄*z*to be found according to:

*ϕ̄*, we note that without making any further approximations, that the quantity Î

_{x}_{Δ}/Î

_{Σ}depends only upon Δ

*ξ*

_{0}and z

_{od}

*ϕ̄*. We then form the function using the reference TC:

_{x}_{Δ}

*= [−*

_{ξ}*a*,

*a*] for some positive real

*a*, is chosen to ensure that

*f*is injective. Then, any image data Î

_{Δ}/Î

_{Σ}with values within the range Ω

_{O}can be related to a sample refraction angle,

*ϕ̄*, by inverting

_{x}*f*. This inversion technique is valid for a wider range of refraction angles than the existing CAXPCI inversion method. This is because the current method requires fewer assumptions and is based upon a single measured quantity, the TC.

It is, however, possible to obtain a linear inversion formula valid for smaller refraction angles. By expanding I_{R} and I_{L} in a Taylor series and again making the approximation I_{TC} (−Δ*ξ*_{0} − z_{od}*ϕ̄ _{x}*/

*M*) + I

_{TC}(Δ

*ξ*

_{0}− z

_{od}

*ϕ̄*/

_{x}*M*) ≈ 2I

_{TC}(Δ

*ξ*

_{0}), gives

_{TC}is approximately zero in the vicinity of Δ

*ξ*

_{0}, since it was shown that the first derivative of I

_{TC}is minimised at Δ

*ξ*

_{0}. Eq. (22) can then be manipulated to reveal the sample refraction angle image as:

_{TC}(Δ

*ξ*

_{0})/I′

_{TC}(Δ

*ξ*

_{0}) is known from the experimentally measured TC.

## 3. Experimental example

The TC of the system is measured routinely whenever the pre-sample aperture is aligned with the detector aperture. An experimentally acquired TC is plotted in Fig. 2 using our laboratory CAXPCI system which has system parameters z_{so} ≈1.6m and z_{od} ≈0.4m. These quantities are approximate since the apertures and detector are initially placed in these positions and an alignment procedure is used to accurately position them. The pre-sample aperture, A_{1}, has period p_{1}=134*μ*m and pixel width P=85*μ*m. The detector aperture A_{2} has a period of 83.5*μ*m to allow it to be placed in front of the detector. The width of the transmitting regions of *A*_{1} and *A*_{2} are 16*μ*m and 20*μ*m respectively. The quantity Δ*ξ* refers to the displacement of A_{1} from the position of perfect alignment with A_{2}. Note that in practice, every second pixel was skipped to minimise detector pixel cross talk. We employed a Rigaku 007HF X-ray tube generator operated at 35 kVp/25 mA with a rotating Mo target, an Anrad SMAM flat panel detector and the gratings were fabricated by Creatv Microtech (Potomac, Maryland, USA). The TC was acquired by taking the average over all pixels for each displacement of the pre-sample aperture. Note that the measured data points are unequally spaced as two separate measurements have been combined and one of the measurements was acquired only for negative values of Δ*ξ*. The fitted curve was found by fitting a fourth order Fourier cosine series thus assuming symmetry about Δ*ξ* = 0. We showed in Sec. (2.2) that Δ*ξ*_{0} should be chosen to be equal to half of the width of the transmitting region of the pre-sample aperture, which is 8*μ*m in our experimental system. Figure 3 shows plots of I_{L}, I_{R} and I_{Σ} for the sampled TC which shows that I_{Σ} is indeed flat for a range of values of Δ*ξ _{s}* = z

_{od}

*ϕ̄*. We can, however, show using the experimentally acquired TC, that the selected value of Δ

_{x}*ξ*

_{0}results in I

_{Σ}being maximally flat over a range of values of Δ

*ξ*. In order to show this we define a measure of flatness as:

_{s}_{Δξs}= [−5 × 10

^{−6}, 5 × 10

^{−6}] m was chosen to accommodate extreme values measured experimentally [16]. The maximum, minimum and mean values were found using the fitted TC.

*ε*(Δ

*ξ*

_{0}) is plotted in Fig. 4 which shows that it exhibits a minimum value in the vicinity of Δ

*ξ*

_{0}as expected.

Another important factor which influences the choice of Δ*ξ*_{0} is the sensitivity to sample refraction angles. Figure 5 shows a plot of the derivative of the curve fitted to the experimentally observed TC data. This plot verifies the result obtained in Sec. (2.2), that the optimal values of the derivative of the TC appear in the vicinity of Δ*ξ* = ±Δ*ξ*_{0}. A similar approach was employed by Diemoz *et al.*[24] for the case of grating interferometry. In particular, rather than phase stepping the detector grating, the pre-sample and detector gratings were offset by an amount which maximised the change in pixel signal for a given change to offset between the gratings. In their method, they make use of a principal analogous to the TC but, instead of separating phase and absorption, obtain a single image containing a well described combination of phase and absorption information. This technique carries the advantage that a single acquisition is acquired per angle of rotation when performing CT imaging.

The accuracy of Eq. (23) depends significantly on how constant the derivative of the TC is in the vicinity of Δ*ξ*_{0}. Figure 6 shows how this derivative varies over a region which corresponds to a sample refraction angle satisfying |*ϕ _{x}*| < 10

^{−5}rad/m. The derivative of the rocking curve varies by at most approximately 15% over this range. Whilst this maximum error would be experienced only for extreme refraction angles, as explained in Sec. (2.3), it is possible to derive a refraction angle inversion formula without making such an assumption. Figure 7 shows a plot of I

_{Δ}/I

_{Σ}versus Δ

*ξ*for the experimental system being considered, using the fitted TC plotted in Fig. 2. The plot shows that, in order to uniquely determine Δ

_{s}*ξ*from an observed value of Î

_{s}_{Δ}/Î

_{Σ}, it is necessary to restrict the domain of Δ

*ξ*to |Δ

_{s}*ξ*| ≲ 0.011 mm which implicitly restricts the observable refraction angles to the range |

_{s}*ϕ̄*| ≲ 0.034 rad/mm. The refraction angle may be extracted from an observed value of Î

_{x}_{Δ}/Î

_{Σ}by numerically determining, from Fig. 7, the value of Δ

*ξ*to which it corresponds. This numerical inversion may be performed very accurately and efficiently.

_{s}## 4. Examples and analysis

In this section we analyse the TC refraction angle retrieval method and show some examples of how it may be applied. In particular, we show how the TC method differs from that previously published for the experimental system considered in Sec. (3) using some experimentally acquired images. We also perform some numerical simulations to demonstrate the improvement offered by the TC method.

We begin by comparing the TC refraction angle extraction algorithm with that published previously, derived analytically and based upon the assumption of perfectly absorbing apertures. In particular, we have previously published [15] a phase extraction algorithm which extracts the refraction angle according to the formula:

_{d}is the full width at half maximum of the beams projected onto the detector aperture. Figure 8 shows a comparison between the analytic inversion formulae and those obtained using the TC plotted in Fig. 7. All of the plots relate to the system used to obtain the TC plotted in Fig. 2.

*σ*

_{d}was found to be approximately 12.5

*μ*m by determining the focal spot size which gave the best match between calculated and measured TCs. The TC approach should, in general, predict a refraction angle greater or equal in magnitude compared with the analytic method, since the TC method implicitly takes account of the partial absorption by the apertures.

The refraction angle retrieval curves in Fig. 8 reveal that the full and approximate TC methods are equivalent for small refraction angles yet diverge strongly for large refraction angles. This will lead to the approximate TC method underestimating refraction angles. This phenomenon results from the partial transmission of X-rays through the apertures as is demonstrated by the remaining plots in Fig. 8. In particular, the full analytic method (Eq. (25)) and the ideal TC methods coincide. The ideal TC inversion curve was obtained from a simulated TC for the case of perfectly absorbing apertures. The approximate analytic curve (Eq. (26)) departs only slightly from the full analytic curve.

We now present an example showing how three of the refraction angle inversion relationships in Fig. 8 result in different values of refraction angle in an experimental case. We used the experimental system for which the TC in Fig. 2 was obtained, to image a titanium wire of radius 125*μ*m. Images were taken at a total of 16 sub-pixel object positions in order to increase spatial resolution. Each such image had an 8.75 second exposure time. We selected this sample due to its very high value of *δ* throughout the source spectrum, even though it is also highly absorbing. High values of *δ* causes high values of |Î_{Δ}/Î_{Σ}| to be measured which is where the greatest difference between the three inversion formulae occurs. We have also shown, for reference, the theoretical refraction angle at the estimated mean energy of the spectrum (18keV). We do not expect the experimentally acquired results to match this profile due to beam hardening which results from absorption by the wire [25]. The main point of these plots is to show an experimental case where the full TC inversion formula is required for accuracy in order to account for large refraction angles. This difference arises because the linearity of the TC breaks down for large separations between the pre-sample and detector apertures. We also imaged aluminium, sapphire, polyetheretherketone and boron wires but these samples did not result in a difference between the full and approximate TC refraction angles. The expected refraction angle in Fig. 9 can only be calculated with accurate knowledge of the source and detector spectral responses and the sample absorption [25]. In light of this and in order to further demonstrate the advantages of the TC inversion method we now present some numerical simulations.

We modelled the experimental system considered in Sec. (3) using an estimated spectrum as plotted in Fig. 10 and assuming that the Anrad SMAM flat panel detector is energy integrating with photon weighting directly proportional to photon energy. We also assumed that the source has a focal spot with a FWHM of 60*μ*m. All other system parameters are as described in Sec. (3). We considered a polyetheretherketone (PEEK) fiber of radius 100*μ*m, assumed to have chemical composition C_{19}O_{3}H_{18} and density 1.3 gm/cm^{3}. The refractive index data was obtained theoretically [26] which is also plotted in Fig. 10. Note that we use *β* to refer to the imaginary part of refractive index. The refractive index for the gold apertures was also calculated from theory [26]. The simulation method is described fully in previous publications [17, 22] however it takes as its starting point Eq. (3) which is evaluated numerically for a range of photon energies within the spectrum. The values of *T* and *𝒯*_{1} are calculated according to photon energy. As such, the simulation is accurate to within the approximations of the paraxial Fresnel-Kirchhoff diffraction integral and the projection approximation as discussed in Sec. (2.1). Each refraction angle was calculated at 51 sample points by scanning the object to increase spatial resolution. This was only for the purposes of numerical comparison, to ensure that the integrated refraction angle did not experience artefacts resulting from the integration.

We have performed simulations for both the polychromatic and monochromatic cases, however, assuming a 60*μ*m FWHM focal spot in both cases. The monochromatic simulation serves to demonstrate that the TC technique performs very accurate quantitative phase retrieval in a scenario when phase is well defined. When a polychromatic source is employed, the concept of phase is ambiguous since it implies an averaging of phase. Furthermore, any such measured phase will depend on the source, aperture, detector and sample spectral properties [25].

Figure 11(a) shows the calculated TC for the polychromatic case for aperture gold thicknesses of 10, 20, 40 and 80*μ*m respectively. We note that no significant variation in calculated TC or retrieved refraction angle was observed for aperture gold thicknesses exceeding 80*μ*m. Figure 11(b) shows the calculated TC for the monochromatic case at the spectrum mean energy of 18keV. The two simulations assume the same source power density. Figure 11(c) shows the refraction angle retrieval relationship, Eq. (21), corresponding to the polychromatic TCs of Fig. 11a) and Fig. 11(d) shows the retrieval relationship corresponding to the monochromatic TCs of Fig. 11b). The two cases are similar, but not identical. In particular, we note that in the poly-chromatic case, thicker gold is required to achieve the ideal refraction angle relationship where there is insignificant transmission through the apertures.

We first explain how the numerical results are analysed. As previously discussed, the system results in a measurement of refraction angle, *ϕ̄ _{x}*. In this example we consider the object to have a circular cross section and so within the support of the object,

*ϕ̄*is given by $\overline{\varphi}=2\overline{\delta}\sqrt{{R}^{2}-{x}^{2}}$ where, as usual, overlines are used to denote quantities averaged over the spectrum. Spatial variation is thus contained within the function which describes the shape of the object. In what follows, we plot the integrated refraction angle,

*ϕ̄*= ∫

*ϕ̄*d

_{x}*x*which enables

*δ̄*to be determined since the shape function is known. The integrated refraction angle can be used to obtain an measurement of integrated phase through multiplication by an effective wavenumber.

Figure 12 shows the integrated refraction angle for the polychromatic ((a) and (c)) and monochromatic ((b) and (d)) cases and using the TC refraction angle retrieval ((a) and (b)) and the approximate linear method Eq. (26) ((c) and (d)). The integrated refraction angle, calculated analytically, at the spectrum mean energy has also been plotted. We note that only in case b) do all integrated refraction angles match the analytic profile. Agreement should be expected in this case since it has not been necessary to assume the existence of an effective energy for the spectrum in order to obtain Eq. (10). In both c) and d), the approximate linear method results in a large variation between measured integrated refraction angle for the different aperture thicknesses, although we note that in the monochromatic case, the solution is very close to the analytic case for the 80*μ*m thick apertures. Both the approximate linear cases exhibit wide variation simply because the method doesn’t take into account X-ray transmission through the apertures. The polychromatic case returns a generally greater phase change than the monochromatic simply because the average value of *δ* across the spectrum is greater than *δ* at the mean energy of the spectrum. The plots in Fig. 12(a), however, demonstrate the main result of this paper. Here we see a much smaller variation in the integrated refraction angle as aperture thickness varies. This shows that the TC method reduces the impact of the system’s spectral properties on the measured refraction angle. In order to more thoroughly analyse the results plotted in a) we present the values of *δ̄* measured for each aperture thickness in Table 1. We expect the predicted value of *δ̄* to converge towards the value of *δ* averaged over the spectrum, ie, *δ _{ave}* = ∫

*δ*(

*E*)

*σ*(

*E*)d

*E*= 1.16×10

^{−6}. Whilst this value is within the range of predicted values of

*δ̄*, the values do not converge to this value. This error arises due to the approximation that the system has an effective energy made in order to simplify Eq. (9) to Eq. (10).

## 5. Conclusions

We have demonstrated a new quantitative technique for measuring X-ray refraction angle and absorption using the coded aperture method with a laboratory source. The quantitative technique requires knowledge of only the so-called translation curve which is obtained by recording the detector signal as the pre-sample aperture is translated relative to the detector aperture. The translation curve is measured routinely when the system is aligned.

We showed that the new technique is more accurate for measuring larger refraction angles and also is more accurate in the case where the apertures are only partially absorbing. We compared the new technique with that previously used which assumed that the apertures were perfectly absorbing. We showed that the new method is significantly more accurate in the case of partially absorbing apertures. Finally, we showed that the proposed technique measures an average value of refraction angle based upon the sample’s value of *δ* averaged over the spectrum, rather than, for example, measuring *δ* at the average energy of the spectrum.

## Acknowledgments

This work was funded by the UK Engineering and Physical Sciences Research Council ( EP/G004250/1 and EP/I021884/1). P.M. is currently supported by a Discovery Early Career Research Award from the Australian Research Council ( DE120101331).

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