Design study of a Laue lens for nuclear...
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research papers
J. Appl. Cryst. (2015). 48, 125–137 doi:10.1107/S1600576714026235 125
Journal of
AppliedCrystallography
ISSN 1600-5767
Received 8 August 2014
Accepted 29 November 2014
# 2015 International Union of Crystallography
Design study of a Laue lens for nuclear medicine
Gianfranco Paterno, Valerio Bellucci, Riccardo Camattari and Vincenzo Guidi*
Department of Physics and Earth Sciences, University of Ferrara, Via Saragat 1/c, 44122 Ferrara and
INFN Section of Ferrara, Italy. Correspondence e-mail: [email protected]
A Laue lens is an ensemble of crystals capable of focusing, through diffraction in
transmission geometry, a fraction of the photons emitted by an X- or �-ray
source onto a small area of a detector. The present study facilitates a thorough
understanding of the effect of each system parameter on the efficiency, the
resolution and the field of view of the lens. In this way, the structure and the size
of the crystals can be set to achieve a compact lens capable of providing a high-
resolution image of the radioactivity distribution lying inside a restricted region
of a patient’s body. As an application, a Laue lens optimized at 140.5 keV, the �-
line emitted by 99mTc, has been designed. The lens is composed of ten rings of
Ge crystals with curved diffracting planes and focuses the photons onto a
detector 50 cm apart from the source with 1.16 � 10�5 efficiency and 0.2 mm
resolution. The combination of these two important figures of merit makes the
proposed device better performing than pinhole single photon emission
computed tomography, which is the technique employed for top-resolution
images in nuclear medicine. Finally, the imaging capability of the designed lens
has been tested through simulations performed with a custom-made Monte
Carlo code.
1. IntroductionThe techniques of diagnostic nuclear medicine, namely scin-
tigraphy, single photon emission computed tomography
(SPECT) and positron emission tomography (PET), represent
some of the best methods for medical imaging (Bushberg et al.,
2002). While X-ray-based computed tomography (CT) and
magnetic resonance imaging (MRI) provide accurate images
of anatomical districts, diagnostic nuclear medicine permits
the analysis of some metabolic processes and an early recog-
nition of tumour masses. More specifically, in a CT examina-
tion, the patient’s body is irradiated through an external X-ray
beam emitted by an X-ray tube capable of rotating around the
bed. Since the absorbtion of X-rays by tissues basically
depends on their density, morphological imaging can be
performed by detecting the unabsorbed radiation through a
detector positioned behind the patient. In nuclear medicine, a
molecule directly involved in a specific metabolic process is
marked with a short-lived radioactive atom. Such compounds,
called radiopharmaceuticals or radiotracers, are given,
generally by injection, to the patient and accumulate in a
specific organ or anatomical district. The most used radio-
tracers are shown in Table 1. They are � emitters for scinti-
graphy and SPECT and �þ emitters for PET. In the PET case,
positrons annihilate with electrons producing two 511 keV
back-to-back photons. Therefore, with both kinds of radio-
tracers, a concentration map of the metabolic activity, i.e. a
functional imaging, can be obtained by detecting the emitted
photons. The performances of scintigraphy and SPECT are
heavily influenced by the collimator positioned before the
detector and used to discriminate the direction of the photons.
This element leads to a trade-off between efficiency and
spatial resolution. Typical values for resolution of conven-
tional SPECT and PET are 5–15 and 3–5 mm, respectively. In
the PET case there is an intrinsic limitation due to the path of
the positrons within the tissue before their annihilation
(Rahmim & Zaidi, 2008). If a resolution close to 1 mm is
required, pinhole SPECT is typically employed (Beekman &
van der Have, 2007). Nevertheless, this technique allows the
investigation of a limited region and shows a resolution–effi-
ciency trade-off. Therefore, the conventional techniques suffer
from low spatial resolution and low signal-to-noise ratio for a
small radioactive source, e.g. a tumour in an initial stage of
development.
The image resolution and quality can be increased by using
an efficient focusing device. Since the real part of the index of
refraction of all materials is approximately equal to one for
high-energy photons, the use of common optical elements is
prevented (Authier, 2001).
The desired effect can be obtained by using a Laue lens,
namely a device that exploits diffraction in crystals to
concentrate a large number of photons onto a small area of a
detector. These optics were initially studied for the realization
of a high-energy telescope (Smither, 1982) and subsequently
have also been proposed for use in nuclear medicine (Smither
& Roa, 2000). Fig. 1 schematically shows the configuration of a
diagnostic system exploiting a Laue lens.
Some prototypes of Laue lens for nuclear medicine have
already been realized (Roa et al., 2005). However, they
provide at the most the same image resolution achievable with
conventional PET. Thus, there is the need to further improve
the lens performance in such a way that its clinical use can
actually become convenient.
In this paper we present a detailed study and the design
principles for a Laue lens when, like in nuclear medicine, a
monochromatic �-ray source is employed. The proposed
method allows high-resolution images of small radioactive
sources to be obtained. The resolution can be one order of
magnitude better than the level attainable in conventional
nuclear medicine examinations.
2. High-energy radiation diffraction in crystals
2.1. Basic concepts
A Laue lens is based on X- or �-ray diffraction, which is a
coherent effect carried out by parallel atomic planes within a
crystalline material. Incident photons interact elastically with
the electrons of the lattice atoms and deviate from their
trajectory. Reflected waves interfere constructively, giving rise
to a diffracted beam, provided that their paths through the
crystal lead to a phase shift that is a multiple of the wave-
length. This condition occurs if Bragg’s law is satisfied:
2dhkl sin �B ¼ �; ð1Þ
where dhkl is the spacing between atomic planes, �B the angle
subtended by the incoming �-ray trajectory and the diffracting
lattice planes, and � the wavelength of the radiation. The
Bragg angle, �B, depends on the orientation of the lattice
planes. For a cubic crystal, such as Cu, GaAs, Si or Ge, the
spacing between the planes can be expressed as
dhkl ¼a
ðh2 þ k2 þ l2Þ1=2; ð2Þ
where a is the lattice constant of the crystal and h, k, l are the
Miller indices of the planes. Since � ¼ hpc=E, where hp is
Planck’s constant, c the speed of light in vacuum and E the
energy of the radiation, by combining equations (1) and (2), it
follows that
sin �B ¼hpcðh2 þ k2 þ l2Þ
1=2
2aE: ð3Þ
Two diffraction geometries are possible. In the first case, called
Bragg (reflection) geometry and depicted in Fig. 2(a), the
diffracted beam emerges from the same crystal surface on
which the incident beam impinges. Conversely, in the Laue
(transmission) geometry, depicted in Fig. 2(b), the diffracted
beam emerges from the surface opposite to that onto which
the incident beam impinges. For high-energy photons, such as
those emitted by a radiotracer, the Bragg angle is very small
and the crystal has to be large to diffract even a small-size
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126 Gianfranco Paterno et al. � A Laue lens for nuclear medicine J. Appl. Cryst. (2015). 48, 125–137
Figure 1Schematic representation of a nuclear diagnostic system equipped with aLaue lens. A fraction of the �-rays emitted by the radiotracer localized ina specific area of the patient’s body are focused onto the detector throughdiffraction in the crystals of the lens.
Figure 2Diffraction geometries. (a) Bragg geometry: the diffracted beam emergesfrom the same crystal surface on which the incident beam impinges. (b)Laue geometry: the diffracted beam emerges from the surface opposite tothat on which the incident beam impinges.
Table 1Typical radioisotopes used in diagnostic nuclear medicine.
Nuclide Radiotracer Decay mode Decay product T1=2 E� (keV) SPECT/PET Usage
99mTc NaTcO4 IT 99Tc 6.02 h 140.5 SPECT General purpose67Ga Ga citrate, Ga nitrate EC 67Zn 78.3 h 93, 185, 300 SPECT Tumour imaging111In I salts EC 111Cd 67.8 h 171, 245 SPECT Brain study, intestinal disturbances123I NaI EC 67Te 13.2 h 159 SPECT Thyroid study201Tl Tl salts EC 201Hg 73.1 h 135, 167 SPECT Diagnosis of coronary artery disease18F FDG, F-DOPA �þ 18O 109.8 min 511 PET Oncology, neurology15O O2, CO2, CO �þ 15N 2.03 min 511 PET Neurology11C CO2, CO, HCN, CH3I �þ 11B 20.38 min 511 PET Cardiology13N NH3 �þ 13C 9.96 min 511 PET Cardiology
beam. For this reason, the Laue geometry represents a more
convenient choice.
The diffracted beam intensity depends on the crystal
features and can be obtained from the dynamical theory or
from the kinematic theory of diffraction (Zachariasen, 1945).
The dynamical theory, as developed by Darwin, takes into
account the interaction of X-rays with matter by solving
recurrence equations that describe the balance of partially
transmitted and partially reflected waves at each lattice plane
(Darwin, 1914a,b). On the other hand, the kinematic theory
assumes that each photon is scattered only once. The total
diffracted amplitude is simply obtained by adding the indivi-
dual amplitudes diffracted by each diffracting centre, taking
into account only the geometrical phase differences between
them and neglecting the interaction of the radiation with
matter. Even if the kinematic theory is less rigorous than the
dynamical theory, it gives correct results when a thin perfect
crystal or a highly curved crystal is considered. An exhaustive
treatment of the subject, in both perfect and distorted crystals,
can be found in specialized books (Authier, 2001) or in review
articles (Authier & Malgrange, 1998; Authier, 2006; Batterman
& Cole, 1964). Here we recall only the concepts that are
relevant to the study of the lens.
The reflectivity of a crystal is defined as the ratio of the
diffracted beam intensity over the incident beam intensity.
Instead, diffraction efficiency is defined as the ratio of the
diffracted beam intensity over the transmitted beam intensity
when no diffraction occurs.
For radiation of energy E and a crystal with lattice planes
ðhklÞ, equation (3) provides the incidence angle � at which
diffraction occurs. Actually, both kinematic and dynamical
theories predict a range around the Bragg angle �B for which
the intensity of the diffracted beam is different from zero. If
we consider a perfect crystal under Laue symmetrical
geometry,1 the rocking curve, i.e. the reflectivity (or the
diffraction efficiency) plotted as a function of �� ¼ � � �B,
shows a narrow peak. Its width at half-maximum (FWHM) is
called the Darwin width �,
� ¼ 2dhkl=�0: ð4Þ
Here �0 is defined as the extinction length
�0 ¼�Vc cos �B
re�jCjjFhklj; ð5Þ
Vc being the volume of the crystal elementary cell (Vc ¼ a3 for
a cubic cell), re the classical electron radius, C the polarization
factor and Fhkl the structure factor. For an unpolarized beam,
the polarization factor is C ¼ ð1þ cos2 �BÞ=2. The structure
factor quantifies the scattering efficiency of an elementary cell
of the crystal, by taking into account the repartition of elec-
trons in space and the vibration of lattice ions via the so-called
Debye–Waller factor (Halloin & Bastie, 2005).
For the context of this article, typical values for � are of the
order of 100. Furthermore, because of the re-diffraction of the
beam, the reflectivity of a thick flat crystal is fixed at 1/2. A
crystal can be regarded as thick if T0 � �0, T0 being the
thickness of the crystal traversed by radiation. Since in our
case �0 is small, this condition is almost always fulfilled. The
integrated reflectivity is the integral of a rocking curve over
the range of incidence angles. Since the integrated reflectivity
is very poor for a flat perfect crystal, different types of crystals
have been considered by the scientific community for the
realization of a Laue lens. Their features are summarized in
the next subsection.
2.2. Mosaic crystals
Unlike an ideal crystal, a real crystal presents imperfections
due to its growth conditions, and it can be better modelled
through the Darwin model (Halloin & Bastie, 2005). This
model, known also as the mosaic model, regards the crystal as
an ensemble of microscopic ideal crystals. The crystallites are
slightly misaligned with respect to each other according to an
angular distribution, which is usually a Gaussian function:
Wð��Þ ¼1
ð2�Þ1=2�exp���2
2�2: ð6Þ
The FWHM of this distribution m ¼ 2ð2 log 2Þ1=2� is the
mosaicity of the crystal. The reflectivity, under symmetric
Laue conditions, is expressed by
R ¼ 12 ½1� expð2T0Þ�
1=2 expð�T0= cos �BÞ; ð7Þ
T0 being the thickness traversed by the beam, the linear
absorption coefficient of the crystal and
¼ Wð��ÞQ: ð8Þ
Q is the integrated intensity diffracted by an individual crys-
tallite per unit of thickness. From the dynamical theory of
diffraction, Q can be written as
Q ¼�2ddhk
�20 cos �B
f ðAÞ: ð9Þ
Under the small-angle approximation, which is valid above
100 keV, the function f ðAÞ can be written as
f ðAÞ ¼2I0ð2AÞ
2A: ð10Þ
I0 is the integral, from 0 to 2A, of the zero-order Bessel
function. A is defined as
A ¼�t0
�0 cos �B
; ð11Þ
t0 being the thickness of the crystallites. f ðAÞ is approximately
1, which is its maximum value, when t0 � �0, namely when
the kinematic theory tends to the dynamical theory.
The reflectivity of a mosaic crystal is the product of two
terms. The first one is the diffraction efficiency of the crystal;
the second one takes into account the absorption of the beam.
As can be seen by equation (7), the reflectivity peaks at
�� ¼ 0. The peak height is at most 1/2 as in the case of a
perfect crystal.
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J. Appl. Cryst. (2015). 48, 125–137 Gianfranco Paterno et al. � A Laue lens for nuclear medicine 127
1 In Laue symmetrical geometry, the angle between the lattice plane and thecrystal surface is exactly 90�.
The FWHM of the rocking curve, �, is proportional to the
mosaicity of the crystal and can be written as
� ¼ m� ln � 1
� ln 12 1þ expð��Þ½ �� �� �
ln 2
� �; ð12Þ
where � is a dimensionless coefficient given by
� ¼ 4�2 ln 2
�
� 1=2dhklT0
�20m
: ð13Þ
Even though the peak reflectivity is at most 1/2, a mosaic
crystal with large mosaicity (it can be several tens of arcse-
conds) may exhibit a large integrated reflectivity. For this
reason, such crystals were chosen for the realization of the first
prototypes of Laue lens for nuclear medicine (Smither & Roa,
2000; Roa et al., 2005).
2.3. Curved diffracting planes crystals
Another type of crystal is the so-called curved diffracting
planes (CDP) crystal. In a CDP crystal, a stress induces a
curvature in the whole lattice structure according to the elastic
properties of the material. Owing to the curvature, the crystal
possesses an angular dispersion of the lattice planes. The
continuous change in the orientation of the lattice planes
prevents re-diffraction inside the crystal and the reflectivity
limit of 50% disappears (Fig. 3). Thus, CDP crystals have the
potential to achieve better performance with respect to both
perfect and mosaic crystals.
There are many ways to fabricate a curved diffracting plane.
The easiest one is by means of an external device (holder) that
applies a bending moment to the crystal (Carassiti et al., 2010).
This method has been in use for decades for the realization of
high-efficiency monochromators employed in synchrotron
high-energy X-ray beamlines (Schulze et al., 1998; Suortti et
al., 1997). However, the use of a holder implies additional
weight and space occupation. These problems represent a
severe limitation to the use of such a crystal as a component of
a Laue lens for both satellite-borne and medical applications.
Thus, the crystal curvature is required to be self-standing. For
this purpose, various methods have been proposed. One is by
applying a thermal gradient perpendicular to the considered
diffracting planes of a perfect crystal (Smither et al., 2005).
Another is by growing a two-component crystal whose
composition varies along the crystal growth axis (Keitel et al.,
1999). A self-standing curvature can be also obtained by
depositing a coating or by grinding (Ferrari et al., 2013) or
grooving a face of the crystal (Bellucci et al., 2011; Camattari,
Guidi et al., 2013).
In the grooving method, the grooves, manufactured on the
surface of the crystal by means of a diamond saw, produce
dislocations and partial amorphizations in the surrounding
regions, which are hence compressed and prevented from
relaxation. Such strain deforms the whole crystal and induces
a net curvature. This method has been proved to be simple,
economical and highly reproducible (Camattari, Battelli et al.,
2013; Camattari, Paterno, Battelli et al., 2014). All of these
features are very important when one has to deal with several
samples as in the case of a Laue lens. The drawback using the
grooving method is the decrease in integrated reflectivity due
to the removed material and to the mosaicization of a portion
of the crystal (Camattari, Paterno, Bellucci & Guidi, 2014).
A new method to produce a self-standing CDP crystal
without losing efficiency is carbon fiber deposition onto a
mono-crystal. Some promising results have been already
achieved and further studies are under development
(Camattari, Dolcini et al., 2014).
Diffraction in curved crystals can be studied through the
Takagi–Taupin equations (Takagi, 1969; Taupin, 1964). They
are hyperbolic partial derivative equations obtained from
Maxwell’s equations in a deformed periodic medium. In the
general case, these equations cannot be solved explicitly and a
numerical approach has to be used. Alternatively, for a slightly
curved crystal, the so-called PPK theory can be adopted. This
theory, based on geometrical optics principles, has been
developed independently by Penning & Polder (1961) and by
Kato (1963). In the PPK theory the distortion of the
diffracting planes is described by the strain gradient �,
� ¼�0
cos2 �B
@2ðh uÞ
@s0@sh
; ð14Þ
where s0 and sh are unit vectors parallel to the incident and to
the diffracted beams, respectively. h is the reciprocal lattice
vector of the reflection hkl and u the displacement vector. If
the curvature of a crystal is uniform, the strain gradient
assumes the simpler form
� ¼�
T0�=2; ð15Þ
� being the angular distribution of the lattice planes, T0 the
thickness of the crystal and � the Darwin width given by
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128 Gianfranco Paterno et al. � A Laue lens for nuclear medicine J. Appl. Cryst. (2015). 48, 125–137
Figure 3Diffraction in CDP and perfect crystals. (a) In a CDP crystal, because ofthe continuous change of the incident angle, re-diffraction is prevented.(b) In a perfect crystal the beam is reflected many times, limiting thereflectivity to 50%.
equation (4). The angular distribution of the lattice plane is
directly proportional to the crystal curvature. Indeed, it is
� ¼ T0=Rcurv; ð16Þ
where Rcurv is the radius of curvature of the crystal.
The rocking curve of a curved crystal follows a rectangular
distribution with width �. The height of the plateau, which
corresponds to the peak reflectivity, depends on the curvature
of the diffracting planes as well. In the general case, reflectivity
cannot be expressed in a closed form. However, for a highly
curved crystal there exists an extension of the PPK theory that
provides the reflectivity under Laue symmetric condition for
diffraction (Malgrange, 2002). It holds that
R ¼ 1� exp��2dhkl
�20
T0
�
� � �exp �
T0
cos �B
� : ð17Þ
A crystal can be regarded as highly curved when the following
condition for the strain gradient is met:
�>�c ¼ �=ð2�0Þ: ð18Þ
Such a condition is fulfilled if the radius of curvature of the
diffracting planes Rcurv is smaller than the critical value
Rcurvc¼ 4�0=��.
If Rcurv >Rcurvc, a multi-lamellar model can be used for the
calculation of the crystal diffraction efficiency (Boeuf et al.,
1978). A multi-lamellar model that takes into account the re-
diffraction of the beam is reported by Bellucci, Guidi et al.
(2013). Such a model merges the results provided by equation
(17) for highly curved crystals with the results provided by the
dynamical theory for flat thick crystals.
In Fig. 4 the rocking curves for a mosaic and a CDP crystal
with the same angular acceptance are compared. The peak
reflectivity of a CDP crystal, as calculated by equation (17),
does not suffer from the 50% limitation. Hence, CDP crystals
can have a very high integrated reflectivity, making them very
good candidates for the realization of a Laue lens.
3. Design principles of the lens
The design principles of a Laue lens for astrophysics have
been well defined in the literature (see for instance Lund,
1992; Frontera & Von Ballmoos, 2010; Bellucci, Camattari &
Guidi, 2013). Even though the requirements of a lens for
nuclear medicine and a lens for astrophysics are the same, the
design approach differs significantly. In the astrophysical case,
the polychromatic hard X- or �-rays come from very distant
sources and can be considered to be parallel when they
impinge on the crystals of the lens. Conversely, in the medical
case one has to deal with a monochromatic and divergent
beam, since � photons are emitted in any direction by the
radioactive source lying inside the patient’s body.
3.1. Geometry of the system
A lens composed of concentric rings of crystals is shown in
Fig. 5(a). It lies at a distance LS from a �-ray point source and
LD from a detector. LS and LD are called the object distance
and image distance, respectively. With an appropriate design,
the lens can focus the photons toward the image point OD,
providing a point-to-point imaging.
First, the energy E of the monochromatic source and the
object distance LS have to be set. Then, the lens geometry can
be determined. The lens is formed by N rings, each of them
exploiting a different set of crystalline planes and/or a
different crystalline material. The crystals of each ring are
assumed to be identical. To obtain the diffraction of the
photons, the radius of the jth ring, rj, has to be set according to
LS ¼rj
tanð�Bj� �jÞ
; ð19Þ
where �j is the angle between the crystal axis and the lens axis
(see Fig. 5b). The photons diffracted by each crystal are
focused toward the point OD if the image distance is set to
LD ¼rj
tanð�Bjþ �jÞ
: ð20Þ
Under the small-angle approximation, tan �Bj’ sin �Bj
’ �Bj,
it is possible to obtain the same equation as for thin lenses in
visible optics (Smither et al., 1995):
1
LS
þ1
LD
¼1
f; ð21Þ
where f is the focal length of the lens, namely the distance from
the ring to the focus for a distant source,
f ¼rj
tanð2�BjÞ: ð22Þ
The source-to-detector distance, LS þ LD, is minimum when
�j ¼ 0, namely when the crystals are perfectly aligned with the
lens axis. Since the system should be as compact as possible,
hereinafter we will assume that this condition is fulfilled.
Moreover, we will always use the small-angle approximation.
Therefore, it follows that
rj=�Bj¼ LD ¼ LS: ð23Þ
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J. Appl. Cryst. (2015). 48, 125–137 Gianfranco Paterno et al. � A Laue lens for nuclear medicine 129
Figure 4Rocking curves for a mosaic and a CDP Ge crystal with the samethickness T0 = 1 mm and acceptance � = 200 0 and using (111) latticeplanes to diffract 140.5 keV photons. (a) CDP crystal with radius ofcurvature Rcurv = 10.3 m. (b) Mosaic crystal with mosaicity m = 13.60 0.
By combining equations (23) and (3), the radius of the jth ring
can be written as
rj ¼hpc
2a
LS
Eðh2þ k2þ l2Þ
1=2: ð24Þ
Therefore, once the material and the lattice plane ðhklÞ used
for a ring have been set, the ring radius is determined. The
higher the Miller indices, the larger the ring radius. For the
arrangement of the crystals in each ring, we assume the
polygonal arrangement that best approximates the ring, i.e.
the polygon inscribed in the circle with radius ðrj � Lrj=2Þ=
cosð�=njÞ. To determine the number of crystals in each ring,
the tangential length Ltjand the radial length Lrj
have to be
set. The latter has been already shown in Fig. 5(b), while Ltjis
the size of the side orthogonal to the plane of the figure. The
number of crystals in each ring, nj, turns out to be
nj ¼ �
arctanLtj
2rj � Lrj
!: ð25Þ
Not all the lattice planes ðhklÞ can be selected for a given
material and size because different crystals would occupy
approximately the same position in the lens. This limitation
becomes more severe as LS decreases.
3.2. Efficiency calculation
The type and thickness of the crystals have to be set to
optimize the lens performance. An important figure of merit is
the lens efficiency. It is defined as the ratio between the
number of photons with energy E diffracted per second by the
lens and the number of photons with energy E emitted per
second by the source. The latter quantity is given by the
product of the source activity and the probability of emission
of the considered �-line. Even though the lens efficiency is a
dimensionless quantity, it can be expressed in counts per
second per becquerel, which is the unit of measurement used
in nuclear medicine. Indeed, the number of counts per second
of the signal on the detector is equal to the number of photons
diffracted per second by the lens, provided that the air
absorption is neglected, an ideal detector is considered, and
the counts due to the background and to the not coherently
scattered photons are subtracted. Furthermore, in nuclear
medicine the ratio described above is often called sensitivity.
Thus, for our purposes, the two terms are considered as
synonyms.
The efficiency of the lens is strictly related to the integrated
reflectivity of the crystals that compose the lens. Let us
consider Fig. 6, which sketches a crystal in a generic ring. The
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130 Gianfranco Paterno et al. � A Laue lens for nuclear medicine J. Appl. Cryst. (2015). 48, 125–137
Figure 5Schematic representation of the geometry of the system. (a) A pointsource is positioned at OS, the lens is placed at a distance LS from thesource and a detector, centred at OD, is at a distance LD from the lens. Ageneric ring of the lens is highlighted; OCij ¼ rj is the radius of the ring.The crystals of each ring are assumed to be identical. (b) A detail of thecrystal i in the ring j. T0j
is the thickness of the crystal traversed bythe photons. �j is the angle between the crystal axis and the lens axis. Inour calculation, we assume that �j ¼ 0.
Figure 6Schematic representation of a crystal in a generic ring (not to scale).OC ¼ r is the radius of the ring. The crystal diffracts the photons emittedwith a polar angle � within the range ½�B ��=2; �B þ�=2�, where � isthe crystal acceptance.
crystal diffracts only the photons emitted with a polar angle �belonging to the interval ½�B ��=2; �B þ�=2�. � is the
angular acceptance of the crystal and is considered to be equal
to the FWHM of its rocking curve. This is exact if a CDP
crystal is considered but is only an approximation for a mosaic
crystal. Likewise, the integrated reflectivity of a mosaic crystal
is considered to be simply the product of the peak reflectivity
and the angular acceptance, as in the case of a CDP crystal.
These approximations allow us to develop our analytical
calculation in the same way for both types of crystal.
It should be noted that not all the crystal volume diffracts
the photons emitted by a point source. Equivalently, not all the
surface on which the photons impinge acts as a collecting area.
Since OSQ ¼ OSO�QO ¼ LS � T0=2 ’ LS, by considering
the two triangles dOSQEOSQE and dOSQBOSQB, it can be calculated that
AE ¼ EB ¼ �=2LS. Therefore, the collecting area of the
crystal is LS�Lt. Since �LS <Lr, the collecting area is lower
than the geometric area LrLt. The collecting area of each ring
is equal to the number of crystals nj times their collecting area:
Acj¼ njLS�jLtj
: ð26Þ
The effective area of each ring is defined as the collecting area
of the ring times the reflectivity of the crystals. The effective
area of the lens is the sum of the effective area of the N rings:
Aeff ¼PNj¼1
Aeffj¼PNj¼1
AcjRj; ð27Þ
Rj being the peak reflectivity of the crystals in the jth ring.
If _NSNS is the number of � photons per second emitted by the
point source, the photon flux on the lens is �L ¼_NSNS=4�L2
S.
Hence, the number of photons per second diffracted by the
lens is _NDND ¼ �LAeff. Therefore, the efficiency of the lens can
be written as
" ¼_NDND
_NSNS
¼Aeff
4�L2S
¼1
4�L2S
XN
j¼1
AcjRj: ð28Þ
It follows that
" ¼1
2
XN
j¼1
njLtj
2�LS
�jRj ¼1
2
XN
j¼1
njLtj
2�rj
�Bj�jRj: ð29Þ
Since
njLtj
2�rj
’ 1; ð30Þ
we obtain
" ¼PNj¼1
"j ¼12
PNj¼1
�Bj�jRj: ð31Þ
The efficiency of a ring is approximately given by
"j ¼12 �Bj
�jRj: ð32Þ
In a first approximation, "j does not depend on LS or on nj or
on the surface on which the photons impinge. Indeed, by
raising the object distance, a larger number of crystals can be
arranged in each ring. Thus, an increase in Aeff can be
obtained. However, this gain is approximately compensated
for by the decrease in the photon flux hitting the lens.
Conversely, "j depends on the Bragg angle, on the acceptance
and on the thickness of the crystals. For a ring of crystals of a
given material and a given set of lattice planes, �j and T0jare
two free parameters that can be chosen to maximize the effi-
ciency of the ring.
To proceed further in the analysis, highly curved crystals are
considered. In this case, the efficiency of a generic ring
assumes the form (neglecting the subscript j)
" ¼1
2�B� 1� exp
��2dhkl
�20
T0
�
� � �exp�T0
cos �B
� : ð33Þ
The efficiency depends linearly on �B. However, by equation
(3) it follows that a higher value of the Bragg angle implies
higher indices and hence a higher value of �0, leading to a
decrease in the ring efficiency. For this reason, the outermost
rings in the lens give a small contribution to the overall effi-
ciency. As a result, it is not convenient to increase the number
of rings over a certain value, which depends on the specific
case. Otherwise, there would be only an increase in the lens
complexity without an appreciable increase in the lens effi-
ciency.
Fig. 7 plots the efficiency at 140.5 keV of a ring exploiting
the (111) planes of Ge crystals.
The acceptance has to be as high as possible to maximize
the efficiency of the ring. Moreover, for each value of �, there
is a relatively narrow range of thickness T0 for which the
efficiency attains its maximum value.
Another parameter that is generally used to quantify the
diffraction capability in the whole lens, especially those for
astrophysics, is the lens diffraction efficiency, which has not to
be confused with the crystals’ diffraction efficiency. The lens
diffraction efficiency is defined as the ratio between the
number of photons per second diffracted by the lens _NDND and
number of photons per second incident on the lens _NLNL. It turns
out that
research papers
J. Appl. Cryst. (2015). 48, 125–137 Gianfranco Paterno et al. � A Laue lens for nuclear medicine 131
Figure 7Normalized efficiency at 140.5 keV of a ring exploiting the (111) planes ofGe crystals as a function of the thickness and the acceptance of thecrystals. The solid black lines plot the optimum thickness as a function ofthe acceptance �.
"D ¼_NDND
_NLNL
¼Aeff
AL
; ð34Þ
where AL ¼PN
j¼1 njLtjLrj
is the geometric area of the lens.
3.3. Point spread function calculation
The point spread function (PSF), i.e. the system response to
a point-like source, is the physical quantity that fully char-
acterizes an imaging system. Indeed, the image of an extended
source is obtained by the convolution of its spatial distribution
and the PSF of the system (Webb, 1988). The PSF of the
system is given by the convolution of the PSF of each indivi-
dual element that contributes to the formation of the image. In
our case, only the lens and the detector contribute to the
formation of the image. Thus, for an ideal detector, the PSF of
the system coincides with the PSF of the lens. The spatial
resolution of the system is defined as the FWHM of its PSF.
This quantity affects the capability to distinguish small details
of the image and hence has to be as small as possible.
An ideal situation would be if the crystals, other than
possessing the curvature of the planes of diffraction, were bent
to perfectly fit in the ring in which they are positioned. In this
case, a perfect focusing onto a single point could be achieved.
Unfortunately, owing to the mechanical stiffness of the crys-
tals, this condition cannot be met and each crystal focuses only
in its scattering plane.2 Therefore, on the image plane, where
the detector is positioned, the distribution function of the
incoming photons is spread out around the centre OD. This
spread, and hence the lens resolution, depends on several
parameters.
If the lens is composed of highly curved crystals disposed
under Laue symmetric geometry, the photon trajectories and
their distribution on the detector can be calculated. Because of
the variation of the lattice plane orientation due to the
curvature, a photon penetrates into the crystal until the zone
where the Bragg condition is reached. Such a zone is narrow
enough that the photon trajectory undergoes a kink
(Malgrange, 2002). Therefore, each photon is diffracted only
once and then proceeds along its trajectory undergoing
normal absorption. These are the conditions provided by the
kinematic theory.
Let us consider the situation sketched in Fig. 8. A photon
impinges on the surface of a crystal with azimuthal angle equal
to zero. The coordinates of the diffraction point can be
calculated as
yD ¼ 0; ð35Þ
zD ¼ �T0
���; ð36Þ
xD ¼ ���T0
�� � LS
� : ð37Þ
The distance of the arrival point of the photons on the
detector, with respect to OD, turns out to be
xDET ¼ rþ xD � ðLD � zDÞð�B ���Þ; ð38Þ
where r is the radius of the ring to which the crystal belongs
and �� ¼ � � �B. Since LD ¼ LS, by considering all the
possible values for the polar angle �, the image obtained on
the detector is a line of width j2T0�B � 2�LSj. Owing to the
focusing effect provided by curved diffracting planes, this
value is lower than the radial size of the crystal Lr. Further-
more, including in our analysis the photon azimuthal angle, it
is possible to see that a point source produces a rectangle with
sides j2T0�B � 2�LSj and 2Lt as an image of each crystal. The
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132 Gianfranco Paterno et al. � A Laue lens for nuclear medicine J. Appl. Cryst. (2015). 48, 125–137
Figure 8Schematic representation of diffraction in a highly curved crystal underLaue symmetric geometry. The kink of the trajectory is due to the largevariation of the lattice plane orientation over a distance equal to theextinction length.
2 The scattering plane is defined by the normal vector of the diffracting latticeplanes and the incoming beam direction. In the perpendicular direction theradiation propagates in a straight line (Stockmeier & Magerl, 2008).
PSF of the lens can be estimated by taking into account such
contributions for all crystals in each ring. In the next section a
specific lens will be considered and its PSF shown. The FWHM
of the PSF depends on the object distance, on the Bragg angle
of each ring, and on the thickness and the acceptance of the
crystals. Conversely, the tails of the PSF are basically deter-
mined by the tangential size of the crystals.
The PSF can also be calculated if the lens is composed of
mosaic crystals (Halloin, 2005). In this case, the width of the
image spot is at least equal to the radial size of the crystals Lr
and becomes larger, owing to the so-called mosaic defocusing,
as LS increases over the value 2 lnð2Þ½ �1=2
Lr=m, m being the
mosaicity of the crystals (Halloin & Bastie, 2005). Therefore,
the image resolution attainable with a lens composed of CDP
crystals is much better than for a lens composed of mosaic
crystals.
A parameter that combines the efficiency and focusing
capability of a lens is the focusing factor G. It is defined as
(Frontera & Von Ballmoos, 2010)
G ¼ fphAeff=AD; ð39Þ
Aeff being the effective area of the lens and AD the area of the
spot on the detector that contains a fraction fph of photons
reflected by the lens.
3.4. Field of view estimation
The field of view (FOV) of the lens is the portion of space
within which a source has to lie so that it can be correctly
reproduced on the image plane. This issue can be precisely
addressed by a numerical simulation. However, an estimation
can be performed as follows. Let us consider a Laue lens
composed of crystals of the same type and size. Let us also
assume that Lr Lt. If a point source is positioned at OS, the
lens provides a point-to-point imaging with a blur given by the
lens resolution. If the point source is moved away from OS, the
lens diffracts the photons with no efficiency loss or increase in
blurring only if the transaxial displacement is lower than
approximately Lr=2. Beyond this distance, diffraction may not
occur for some polar angles within the nominal acceptance
range. Indeed, through a modified version of equation (37)
which includes the source shift and the azimuthal angle
contribution (not reported here), it is possible to calculate that
the diffraction point lies outside the crystal. Since the lens
transaxial FOV is approximately given by the radial size of the
crystals, there is a trade-off between the need for small Lr (to
enable diffraction from all the desired planes) and the need
for a large value of Lr (to magnify the transaxial FOV). The
axial FOV of the lens is far broader than the transaxial one.
Indeed, it is approximately equal to �1LS=�B1, �B1
being very
small.
3.5. Response of the lens versus energy
A lens designed for a specific monochromatic source can be
used with different sources as well. Equation (24) settles a
proportionality relationship between E and LS. Thus, if the
source energy changes, the object and the image distances
have to be set accordingly. However, the lens efficiency and
resolution change as well.
The efficiency worsens at high energy. Indeed, the crystal
thickness should be increased to maintain a high value of
reflectivity. Furthermore, even if one considers the optimum
thickness, the lower Bragg angle leads to an increase in �0 and
hence to a decrease in diffraction efficiency at high energy.
Such a decrease is stronger than the increase in the absorption
factor and, as a result, the reflectivity decreases.
The shape of the lens PSF also changes with energy. Indeed,
it depends on LS and on the Bragg angles of each ring and, in
turn, these physical quantities vary with energy. As will be
shown in the next section, there is an energy range within
which the resolution assumes its best value. However, this
condition leads to a smaller fraction of photons enclosed by a
circle with diameter equal to the FWHM of the PSF.
4. High-resolution lens
In order to estimate the performance of a Laue lens designed
with the method described above, we will now work out a
practical case. In particular, we will design a lens to focus the
140.5 keV photons emitted by a point source of 99mTc located
0.25 m from the lens.
4.1. Lens features
The selection of the crystals that compose the lens heavily
affects the properties of the lens itself. We consider a lens
composed of ten rings of CDP Ge crystals whose transaxial
size is 1.0 � 0.5 mm. Furthermore, we take under considera-
tion crystals with a radius of curvature of 11.5 m. This value is
achievable through the grooving method, creating 16 grooves,
320 mm deep and 150 mm wide, on the largest face of the
crystal. The removed material would be about 30%. However,
taking into account the mosaicization that could occur in some
portions of the crystals and that not all the volume of the
crystals is required to diffract the photons emitted by a point
source, the decrease in lens efficiency can be estimated to be
20%. Since the crystals do not necessarily have to be fabri-
cated through the grooving method, the reduction factor is not
taken into account and a general treatment is kept.
In the previous section we showed that each ring should be
composed of crystals with different thicknesses. However, in
this case, the optimum thickness does not change very much
from one ring to another. Thus, for the sake of simplicity, we
set the thickness of all the crystals to be 5.0 mm. Their angular
acceptance turns out to be 9000. Finally, we consider a
symmetric Laue geometry and a perfect crystal alignment. The
features of the lens are summarized in Table 2.
For each ring, the lattice planes, the radius and the number
of crystals exploited are listed in Table 3.
By using such diffracting planes, the lens assumes the
geometry whose front view is depicted in Fig. 9. The lens is
very compact, having a diameter of 27 mm. Thus, it would be
easy to move it to perform the scan of a restricted area.
Through equation (29), the lens efficiency turns out to be
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J. Appl. Cryst. (2015). 48, 125–137 Gianfranco Paterno et al. � A Laue lens for nuclear medicine 133
1:16� 10�5, which is lower than the levels for SPECT and
PET and is indeed comparable to that of pinhole SPECT. The
efficiency of the proposed lens is also of the same order of
magnitude if compared with the already realized prototypes
(Smither & Roa, 2000; Roa et al., 2005).
By application of the method expounded in the previous
section, the PSF of the lens can be calculated. It is a function of
the two coordinates on the image (detector) planes. However,
owing to the nearly perfect cylindrical symmetry of the lens, a
cross section along any axis can be considered. Fig. 10 shows
the cross section of the PSF along the X axis.
The majority of the photons are focused near to the image
point OD. Indeed, the FWHM of the curve is 0.20 mm and the
number of diffracted photons enclosed by a circle whose
diameter is 0.20 mm turns out to be 42%. Furthermore, a spot
of 0.92 mm contains 80% of the diffracted photons. Fig. 11
plots the fraction of diffracted photons, fph, enclosed by a
circle of increasing diameter dfph.
Owing to the focusing power of the lens, a very low blur in
the image of a point source is guaranteed. A resolution of
0.20 mm would be an outstanding performance for a tech-
nique in nuclear medicine. This value is one order of magni-
tude better than that obtainable with PET and it can be only
approached by some pinhole SPECTs, but in such cases, the
efficiency would be far lower than for the lens described here.
The lens performance at 140.5 keV is summarized in Table 4.
Finally, the efficiency and the resolution of the lens as a
function of energy are shown in Figs. 12 and 13 respectively.
As explained in the previous section, the efficiency decreases
monotonically at high energy owing to the decrease in
reflectivity of the crystals.
The PSF of the lens varies versus energy because of the
variation of LS and of the Bragg angle relative to each ring.
When the condition for best resolution occurs, a smaller
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134 Gianfranco Paterno et al. � A Laue lens for nuclear medicine J. Appl. Cryst. (2015). 48, 125–137
Figure 9Front view of the designed lens. The largest side of the crystals is thetangential side Lt. The radial side is Lr, while the thickness T0 traversedby the photons is in the direction perpendicular to the plane of the figure.
Figure 10Cross section of the lens PSF along the X axis of the image plane.
Table 3Rings of the lens.
Ring Lattice planes Number of crystals Radius (mm)
1 (111) 19 3.382 (220) 33 5.523 (311) 39 6.474 (400) 47 7.805 (331) 51 8.506 (422) 58 9.567 (511) 62 10.148 (440) 67 11.049 (620) 76 12.3510 (444) 83 13.53
Figure 11Fraction of the diffracted photons enclosed by a circle of increasingdiameter.
Table 2Lens features.
E (keV) 140.5LS (m) 0.25LD (m) 0.25N 10Crystals Ge (CDP)T0 (mm) 5.0Lt (mm) 1.0Lr (mm) 0.5Rcurv (m) 11.5� (0 0) 90
fraction of diffracted photons is enclosed by a circle with
diameter equal to the FWHM of the PSF. Furthermore, the
diameter of a circle enclosing 80% of diffracted photons is
larger.
It can be argued that the lens is still usable when other
monochromatic sources are considered. Naturally, the best
performance is achieved at the energy for which the lens has
been designed.
4.2. Simulations
In order to obtain in-depth knowledge about the imaging
properties of the lens, several Monte Carlo simulations have
been performed through a custom-made code named
LAUENM. The code, which is implemented in the MATLAB
language (The MathWorks Inc., Natick, MA, USA), enables
one to design the lens and to simulate the overall diffraction
process. The lens can be composed of crystals of different
material and different structure (CDP or mosaic). The code is
modular and each module deals with a particular task. A
specific module manages the photon source, which can take
various shapes and activity distributions. The photons are
emitted randomly in direction. A module works out the lens
geometry starting from the input parameters set by the user.
The main processing module manages the interaction of the
photons with the crystals and calculates the arrival point of the
photons on the detector. Finally, a post-processing module,
taking into account the detector features, computes the
obtained image and all the figures of merit regarding the lens.
Fig. 14 depicts the simulated lens PSF and a comparison
with the PSF calculated through the
analytical method described in the
previous section. An ideal detector with
100% efficiency and 40 � 40 mm pixel
size is considered.
The PSF is a narrow distribution
peaked at OD. It is also possible to
notice a very good agreement between
simulation and analytical calculation.
In order to investigate the FOV of the
lens, the lens efficiency is recorded as a
function of the position of the point
source. In particular, the source is
moved along a transaxial direction and
along the axial direction, namely along
the axes xS and zS of a frame centred at
OS. Fig. 15 plots the normalized lens
efficiency as a function of xS and zS. It is possible to recognize
that within a transaxial distance equal to 0.25 mm from OS
there is no efficiency decrease. This distance corresponds to
Lr=2. The axial distance within which there is no efficiency
decrease is approximately equal to 4.0 mm, which corresponds
to �1LS=2�B1. It is worth noting that over these distances the
response does not vanish but undergoes a progressive loss
accompanied by an increase in the photon spread. This affects
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J. Appl. Cryst. (2015). 48, 125–137 Gianfranco Paterno et al. � A Laue lens for nuclear medicine 135
Figure 12Efficiency of the lens as a function of source energy.
Figure 13Characteristic parameters of the lens PSF as a function of the sourceenergy. Red circles joined by a red solid line plot the resolution of the lens(mm). Green crosses joined by a green dot–dashed line plot the fractionof photons (%) enclosed by a circle whose diameter is equal to theFWHM of the lens PSF. Blue squares joined by a blue dotted line plot thediameter of the circle (mm) that encloses 80% of diffracted photons.
Table 4Lens performance at 140.5 keV.
Number of crystals 535Lens diameter (cm) 2.7Filling factor (%) 46Diffraction efficiency (%) 3.4Efficiency 1:16� 10�5
Resolution (mm) 0.20fph (%) 42d80% (mm) 0.92G80% 9
Figure 14(a) Simulated lens PSF. (b) Comparison of the simulated and calculated PSF cross section along thedetector X axis.
the ability to obtain a correct image of the source. Hence, the
FOV of the lens has to be considered limited to the value
within which the normalized efficiency is 1, to be capable of
reconstructing the image of an extended source.
Fig. 16 summarizes the images obtained when various
source configurations are considered, provided that the
background and the not coherently scattered photons are
neglected. Fig. 16(a) plots the image obtained in the nominal
configuration, i.e. with the point source
positioned at OS. Fig. 16(b) plots the
image related to a point source posi-
tioned at yS =�0.2 mm, which is a point
inside the FOV of the lens. It can be
seen that an exact image of the source is
reproduced on the detector. Fig. 16(c)
plots the image related to a point source
positioned at xS = +0.4 mm, a point
outside the FOV of the lens as defined
above. In this case it is still possible to
recognize that the peak of the photon
distribution is centred at X = +0.4 mm.
However, there is a broadening of the
peak and an asymmetry in the tails,
which are much more extended in the
opposite direction with respect to the
source shift and are almost absent in the
perpendicular direction. This asymmetry makes it very diffi-
cult to reconstruct the image when an extended source is
considered. In Fig. 16(d) the point source is moved 10 mm
axially with respect to OS; thus it is outside the FOV. Because
the part of the crystal closer to the lens axis diffracts hardly
any photons, a central hole appears, making image recon-
struction impossible. In Fig. 16(e) two point sources with
different activity are considered. One is centred at OS and the
other, having an activity equal to one-half that of the former, is
moved 0.25 mm along xS. Both the sources are perfectly
resolved and the difference in activity is perceptible. Indeed,
both the sources are inside the FOV and are separated by a
distance larger than the spatial resolution. Finally, Fig. 16( f)
shows the image of a circular source with a radius of 0.32 mm,
which is correctly reproduced.
5. Conclusions
The design principles of a diagnostic imaging system based on
a Laue lens have been presented. CDP crystals represent the
best choice for the composition of the lens because of their
high integrated reflectivity and the ability to fabricate them in
a reproducible manner. By properly selecting the size of the
crystals, a lens with good efficiency and high resolution can be
obtained. In particular, such a system attains the best resolu-
tion among diagnostic techniques used in nuclear medicine.
The transaxial FOV of the lens is limited by the radial size of
the crystals and ranges within 0.3–5 mm. However, by moving
the lens, it would be possible to perform a high-resolution scan
over a restricted region of interest (alternatively, the lens
could be maintained in a fixed position and the bed moved).
The obtained image may help specialists to gain a better
understanding of some metabolic processes or to recognize
more accurately the extension and the position of a tumour
mass in an early stage of evolution. Generally speaking, the
lens could be used in those cases where the results of a
conventional diagnostic examination are doubtful. Owing to
the compactness of the lens, it would be possible to make use
of a high number of identical lenses to observe the same point,
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136 Gianfranco Paterno et al. � A Laue lens for nuclear medicine J. Appl. Cryst. (2015). 48, 125–137
Figure 15(a) Normalized lens efficiency as a function of xS and zS. (b) Contour of the normalized lensefficiency.
Figure 16Image on the detector with various source configurations. (a) Point sourcepositioned at OS. (b) Point source moved 0.2 mm transversely (along yS)with respect to OS. (c) Point source moved 0.4 mm transversely (along xS)with respect to OS. (d) Point source moved 10 mm axially (along zS) withrespect to OS. (e) Two point sources of different activity are considered,one at OS and the second, having an activity equal to one-half that of theformer, moved 0.25 mm along xS. ( f ) Circular source with a radius of0.32 mm.
obtaining an amplification of the lens efficiency. In this way,
the high-resolution scan could be performed immediately
after a conventional SPECT examination without the need for
a new injection of the radiotracer.
We acknowledge partial support by the LOGOS project of
INFN and the SPINNER project of Emilia-Romagna region.
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