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C. David, IEEE Conference, Rome, 21.10.2004
LMNLMN
SLSSLS
Phase Contrast X-Ray Radiography and Tomography Based on a Grating Interferometer
C. David, T. Weitkamp, A. DiazLaboratory for Micro- and Nanotechnology (LMN), Paul Scherrer Institut, Switzerland
F. Pfeiffer, M. Stampanoni, J.F. van der Veen Swiss Light Source (SLS), Paul Scherrer Institut, Switzerland
C. David, IEEE Conference, Rome, 21.10.2004
X-rays for medical imaging
• Minimizing the radiation dose is an important issue – especially in mammography
• low absorption contrast => large dose required to obtain sufficiently good S/N
• low applied photon energy (Mo anodes) • screening submits a large number of healthy patients to radiation dose
C. David, IEEE Conference, Rome, 21.10.2004
Improving contrast
Source Sample Detector
C. David, IEEE Conference, Rome, 21.10.2004
Improving contrast
Source Sample Detector
efficiency, size, resolution
C. David, IEEE Conference, Rome, 21.10.2004
Improving contrast
Source Sample Detector
spectrum, power, coherence
efficiency, size, resolution
C. David, IEEE Conference, Rome, 21.10.2004
Improving contrast
Source Sample Detector
spectrum, power, coherence
efficiency, size, resolution
contrast mechanism
C. David, IEEE Conference, Rome, 21.10.2004
Phase contrast vs. amplitude contrast
n = 1 – + i
x-rays
C. David, IEEE Conference, Rome, 21.10.2004
Phase contrast vs. amplitude contrast
n = 1 – + i
x-rays
C. David, IEEE Conference, Rome, 21.10.2004
Phase contrast vs. amplitude contrast
n = 1 – + i
x-rays
C. David, IEEE Conference, Rome, 21.10.2004
Phase contrast vs. amplitude contrast
Example:• 20 keV• Organic sample (polymer, biological, medical…) .• 50 m thickness
n = 1 – + i
x-rays
C. David, IEEE Conference, Rome, 21.10.2004
Phase contrast vs. amplitude contrast
Example:• 20 keV• Organic sample (polymer, biological, medical…) .• 50 m thickness only 0.2 % absorption, but - phase shift
n = 1 – + i
x-rays
C. David, IEEE Conference, Rome, 21.10.2004
Phase contrast vs. amplitude contrast
Example:• 20 keV• Organic sample (polymer, biological, medical…) .• 50 m thickness only 0.2 % absorption, but - phase shift
n = 1 – + i
x-rays
+
C. David, IEEE Conference, Rome, 21.10.2004
Phase contrast vs. amplitude contrast
Example:• 20 keV• Organic sample (polymer, biological, medical…) .• 50 m thickness only 0.2 % absorption, but - phase shift much higher contrast less dose required
n = 1 – + i
x-rays
+
C. David, IEEE Conference, Rome, 21.10.2004
Hard x-ray interferometry
Bonse-Hart Interferometer (since 1965)
detector
Object
C. David, IEEE Conference, Rome, 21.10.2004
Hard x-ray interferometry
Bonse-Hart Interferometer (since 1965)
detector
• Object beam and reference beam are generated by Bragg reflections on thin Si crystals
• The interference of both beams gives a phase image
Object
C. David, IEEE Conference, Rome, 21.10.2004
Hard x-ray interferometry
Bonse-Hart Interferometer (since 1965)
detector
• optical path length difference needs to be stable to a fraction of a wavelengths
picometer stability required
cannot be scaled up
• Object beam and reference beam are generated by Bragg reflections on thin Si crystals
• The interference of both beams gives a phase image
Object
C. David, IEEE Conference, Rome, 21.10.2004
Propagation methods – edge contrast
C. David, IEEE Conference, Rome, 21.10.2004
• phase shift greatly enhances contrast of edges
• can be used to retrieve phase information
• requires high degree of transverse coherence (i.e. small source size)
• cannot be scaled up to large fields of view (required detector resolution)
Propagation methods – edge contrast
C. David, IEEE Conference, Rome, 21.10.2004
50 nm
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
s
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
s
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
interference pattern
s
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
analyzer amplitude grating
interference pattern
camera
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
interference pattern
analyzer amplitude grating
Moiré fringes
camera
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
analyzer amplitude grating
interference pattern
camera
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
analyzer amplitude grating
interference pattern
camera
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
analyzer amplitude grating
interference pattern
camera
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
analyzer amplitude grating
interference pattern
camera
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
analyzer amplitude grating
interference pattern
camera
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
analyzer amplitude grating
interference pattern
camera
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
analyzer amplitude grating
interference pattern
camera
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
analyzer amplitude grating
interference pattern
camera
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
analyzer amplitude grating
interference pattern
camera
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
analyzer amplitude grating
interference pattern
camera
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
analyzer amplitude grating
interference pattern
camera
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
analyzer amplitude grating
interference pattern
camera
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
analyzer amplitude grating
interference pattern
phase object
camera
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
analyzer amplitude grating
interference pattern
phase object
camera
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
analyzer amplitude grating
interference pattern
phase object
camera
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
analyzer amplitude gratingphase object
interference pattern
camera
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
beam-splitter phase grating
analyzer amplitude grating
interference pattern
phase object
camera
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
Differential phase contrast imaging!
camera
beam-splitter phase grating
analyzer amplitude grating
interference pattern
phase object
Grating x-ray interferometry
C. David, IEEE Conference, Rome, 21.10.2004
4 µm4 µm 4 µm
Phase grating (silicon, p = 4 µm)
•Si-110 wet-etched•Depth of structures chosen so that
phase shift is π no zeroth order
The gratings
C. David, IEEE Conference, Rome, 21.10.2004
4 µm4 µm 4 µm
Absorption grating (Au in silicon, q = 2 µm)
•Au in gaps of Si grating•Grown electrochemically•Period is half that of the phase grating
The gratings
Phase grating (silicon, p = 4 µm)
4 µm4 µm
•Si-110 wet-etched•Depth of structures chosen so that
phase shift is π no zeroth order
C. David, IEEE Conference, Rome, 21.10.2004
polystyrene spheres Ø 100 and 200 µm
Photon energy: 12.4 keVp = 4 µm q = 2 µm
BM 5, ESRF, Dec. 2002
C. David, IEEE Conference, Rome, 21.10.2004
Absorption contrast andedge contrast
Interferometric phase contrast
C. David, IEEE Conference, Rome, 21.10.2004
Absorption contrast andedge contrast
Interferometric phase contrast
Differential phase contrast
C. David, IEEE Conference, Rome, 21.10.2004
Absorption contrast andedge contrast
Can be integrated to yield projected phase shift of sample
Suited for tomographic reconstruction
Interferometric phase contrast
Differential phase contrast Phase contrast
C. David, IEEE Conference, Rome, 21.10.2004
Edge contrast vs. Interferometric contrast
Non-interferometric
Absorption andEdge contrast
Tomogram
Projection0.5mm
C. David, IEEE Conference, Rome, 21.10.2004
Interferometric phase contrastNon-interferometric
Phase gradientAbsorption andEdge contrast Phase
Tomogram
Projection Projection
Tomogram
Projection
ID19, ESRF, June 200414.4 keV
0.5mm
Edge contrast vs. Interferometric contrast
C. David, IEEE Conference, Rome, 21.10.2004
0.5mm
C. David, IEEE Conference, Rome, 21.10.20041mm
0.5 mm
C. David, IEEE Conference, Rome, 21.10.20041mm
0.5 mm
C. David, IEEE Conference, Rome, 21.10.2004
Polychromatic radiation
C. David, IEEE Conference, Rome, 21.10.2004
camera
beam-splitter phase grating
analyzer amplitude grating
interference pattern
phase object
λ1
Polychromatic radiation
C. David, IEEE Conference, Rome, 21.10.2004
camera
beam-splitter phase grating
analyzer amplitude grating
interference pattern
phase object
λ1
λ2
Polychromatic radiation
C. David, IEEE Conference, Rome, 21.10.2004
camera
beam-splitter phase grating
analyzer amplitude grating
interference pattern
phase object
λ1
λ2
Polychromatic radiation
C. David, IEEE Conference, Rome, 21.10.2004
camera
beam-splitter phase grating
analyzer amplitude grating
interference pattern
phase object
λ1
λ2
Polychromatic radiation
C. David, IEEE Conference, Rome, 21.10.2004
Pink-beam phase tomography
• SLS wiggler• No monochromator• Zr absorption filter 100 µm• Camera scintillator YAG:
Y absorption edge at 17.0 keVacts as high-pass filter
• Mean energy E = 17.5 keVBandwidth ΔE ≈ 1 keV
Beam conditioning:
C. David, IEEE Conference, Rome, 21.10.2004
Pink-beam phase tomography
Three fibers• Polyamide Ø 225 µm• Boron Ø 200 µm, core: W Ø 10 µm• PBT Ø 190 µm
• SLS wiggler• No monochromator• Zr absorption filter 100 µm• Camera scintillator YAG:
Y absorption edge at 17.0 keVacts as high-pass filter
• Mean energy E = 17.5 keVBandwidth ΔE ≈ 1 keV
Beam conditioning:
Sample:
C. David, IEEE Conference, Rome, 21.10.2004
Pink-beam phase tomography
Three fibers• Polyamide Ø 225 µm• Boron Ø 200 µm, core: W Ø 10 µm• PBT Ø 190 µm
Sample:
Edge contrast
C. David, IEEE Conference, Rome, 21.10.2004
Pink-beam phase tomography
Three fibers• Polyamide Ø 225 µm• Boron Ø 200 µm, core: W Ø 10 µm• PBT Ø 190 µm
Sample:
Differential phase contrast
Edge contrast
C. David, IEEE Conference, Rome, 21.10.2004
Pink-beam phase tomography
Three fibers• Polyamide Ø 225 µm• Boron Ø 200 µm, core: W Ø 10 µm• PBT Ø 190 µm
Sample:
Differential phase contrast Phase contrast
Edge contrast
C. David, IEEE Conference, Rome, 21.10.2004
Pink-beam phase tomography
Three fibers• Polyamide Ø 225 µm• Boron Ø 200 µm, core: W Ø 10 µm• PBT Ø 190 µm
Sample:
Differential phase contrast Phase contrast
Edge contrast Edge contrasttomogram
Phase contrasttomogram
C. David, IEEE Conference, Rome, 21.10.2004
Pink-beam phase tomography
C. David, IEEE Conference, Rome, 21.10.2004
Required transverse coherence
C. David, IEEE Conference, Rome, 21.10.2004
s camera
d
Required transverse coherence
C. David, IEEE Conference, Rome, 21.10.2004
s camera
dIn our experiments:
E = 17.5 keV, => = 0.07nm
d = 28mm, => s = 1m
Required transverse coherence
C. David, IEEE Conference, Rome, 21.10.2004
s camera
dIn our experiments:
E = 17.5 keV, => = 0.07nm
d = 28mm, => s = 1m
Transverse coherence length c:
c = * p/s
p: source distance, e.g. 2m s: source size, e.g. 100m
Required transverse coherence
C. David, IEEE Conference, Rome, 21.10.2004
s camera
dIn our experiments:
E = 17.5 keV, => = 0.07nm
d = 28mm, => s = 1m
Transverse coherence length c:
c = * p/s = 1.4m
p: source distance, e.g. 2m s: source size, e.g. 100m
Required transverse coherence
C. David, IEEE Conference, Rome, 21.10.2004
Summary
C. David, IEEE Conference, Rome, 21.10.2004
Summary
• There is a large potential to reduce the x-ray dose in medical imaging by exploiting the phase shifting property of matter rather than the absorption
C. David, IEEE Conference, Rome, 21.10.2004
Summary
• There is a large potential to reduce the x-ray dose in medical imaging by exploiting the phase shifting property of matter rather than the absorption
• Grating interferometry offers advantages compared to other phase imaging methods :
C. David, IEEE Conference, Rome, 21.10.2004
Summary
• There is a large potential to reduce the x-ray dose in medical imaging by exploiting the phase shifting property of matter rather than the absorption
• Grating interferometry offers advantages compared to other phase imaging methods :
• Robustness • Quantitative method • Works fine at energies suitable for mammography • Requires no temporal and little spatial coherence • Has potential to be scaled up to large fields of view
C. David, IEEE Conference, Rome, 21.10.2004
AcknowledgmentsAcknowledgments
At ESRF:
P. CloetensJ. Hoszowska E. Ziegler
and many others ...
Funding: Swiss National Science Foundation European Community
Many thanks to:
At PSIE. DeckardtF. GlausB. HaasY. HemmerlingL. HeydermanM. Lange J. Lehmann D. Meister T. Neiger B. Nöhammer T. Rohbeck
C. David, IEEE Conference, Rome, 21.10.2004
AcknowledgmentsAcknowledgments
At ESRF:
P. CloetensJ. Hoszowska E. Ziegler
and many others ...
Funding: Swiss National Science Foundation European Community
Many thanks to:
At PSIE. DeckardtF. GlausB. HaasY. HemmerlingL. HeydermanM. Lange J. Lehmann D. Meister T. Neiger B. Nöhammer T. Rohbeck
Postdoc Position available