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C. David, IEEE Conference, Rome, 21.10.2004 LMN LMN SLS SLS Phase Contrast X-Ray Radiography and Tomography Based on a Grating Interferometer C. David, T. Weitkamp, A. Diaz Laboratory 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
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Page 1: LMN

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

Page 2: LMN

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

Page 3: LMN

C. David, IEEE Conference, Rome, 21.10.2004

Improving contrast

Source Sample Detector

Page 4: LMN

C. David, IEEE Conference, Rome, 21.10.2004

Improving contrast

Source Sample Detector

efficiency, size, resolution

Page 5: LMN

C. David, IEEE Conference, Rome, 21.10.2004

Improving contrast

Source Sample Detector

spectrum, power, coherence

efficiency, size, resolution

Page 6: LMN

C. David, IEEE Conference, Rome, 21.10.2004

Improving contrast

Source Sample Detector

spectrum, power, coherence

efficiency, size, resolution

contrast mechanism

Page 7: LMN

C. David, IEEE Conference, Rome, 21.10.2004

Phase contrast vs. amplitude contrast

n = 1 – + i

x-rays

Page 8: LMN

C. David, IEEE Conference, Rome, 21.10.2004

Phase contrast vs. amplitude contrast

n = 1 – + i

x-rays

Page 9: LMN

C. David, IEEE Conference, Rome, 21.10.2004

Phase contrast vs. amplitude contrast

n = 1 – + i

x-rays

Page 10: LMN

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

Page 11: LMN

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

Page 12: LMN

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

+

Page 13: LMN

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

+

Page 14: LMN

C. David, IEEE Conference, Rome, 21.10.2004

Hard x-ray interferometry

Bonse-Hart Interferometer (since 1965)

detector

Object

Page 15: LMN

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

Page 16: LMN

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

Page 17: LMN

C. David, IEEE Conference, Rome, 21.10.2004

Propagation methods – edge contrast

Page 18: LMN

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

Page 19: LMN

C. David, IEEE Conference, Rome, 21.10.2004

50 nm

Grating x-ray interferometry

Page 20: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

s

Grating x-ray interferometry

Page 21: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

s

Grating x-ray interferometry

Page 22: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

interference pattern

s

Grating x-ray interferometry

Page 23: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

analyzer amplitude grating

interference pattern

camera

Grating x-ray interferometry

Page 24: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

interference pattern

analyzer amplitude grating

Moiré fringes

camera

Grating x-ray interferometry

Page 25: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

analyzer amplitude grating

interference pattern

camera

Grating x-ray interferometry

Page 26: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

analyzer amplitude grating

interference pattern

camera

Grating x-ray interferometry

Page 27: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

analyzer amplitude grating

interference pattern

camera

Grating x-ray interferometry

Page 28: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

analyzer amplitude grating

interference pattern

camera

Grating x-ray interferometry

Page 29: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

analyzer amplitude grating

interference pattern

camera

Grating x-ray interferometry

Page 30: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

analyzer amplitude grating

interference pattern

camera

Grating x-ray interferometry

Page 31: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

analyzer amplitude grating

interference pattern

camera

Grating x-ray interferometry

Page 32: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

analyzer amplitude grating

interference pattern

camera

Grating x-ray interferometry

Page 33: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

analyzer amplitude grating

interference pattern

camera

Grating x-ray interferometry

Page 34: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

analyzer amplitude grating

interference pattern

camera

Grating x-ray interferometry

Page 35: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

analyzer amplitude grating

interference pattern

camera

Grating x-ray interferometry

Page 36: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

analyzer amplitude grating

interference pattern

camera

Grating x-ray interferometry

Page 37: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

analyzer amplitude grating

interference pattern

phase object

camera

Grating x-ray interferometry

Page 38: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

analyzer amplitude grating

interference pattern

phase object

camera

Grating x-ray interferometry

Page 39: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

analyzer amplitude grating

interference pattern

phase object

camera

Grating x-ray interferometry

Page 40: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

analyzer amplitude gratingphase object

interference pattern

camera

Grating x-ray interferometry

Page 41: LMN

C. David, IEEE Conference, Rome, 21.10.2004

beam-splitter phase grating

analyzer amplitude grating

interference pattern

phase object

camera

Grating x-ray interferometry

Page 42: LMN

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

Page 43: LMN

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

Page 44: LMN

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

Page 45: LMN

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

Page 46: LMN

C. David, IEEE Conference, Rome, 21.10.2004

Absorption contrast andedge contrast

Interferometric phase contrast

Page 47: LMN

C. David, IEEE Conference, Rome, 21.10.2004

Absorption contrast andedge contrast

Interferometric phase contrast

Differential phase contrast

Page 48: LMN

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

Page 49: LMN

C. David, IEEE Conference, Rome, 21.10.2004

Edge contrast vs. Interferometric contrast

Non-interferometric

Absorption andEdge contrast

Tomogram

Projection0.5mm

Page 50: LMN

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

Page 51: LMN

C. David, IEEE Conference, Rome, 21.10.2004

0.5mm

Page 52: LMN

C. David, IEEE Conference, Rome, 21.10.20041mm

0.5 mm

Page 53: LMN

C. David, IEEE Conference, Rome, 21.10.20041mm

0.5 mm

Page 54: LMN

C. David, IEEE Conference, Rome, 21.10.2004

Polychromatic radiation

Page 55: LMN

C. David, IEEE Conference, Rome, 21.10.2004

camera

beam-splitter phase grating

analyzer amplitude grating

interference pattern

phase object

λ1

Polychromatic radiation

Page 56: LMN

C. David, IEEE Conference, Rome, 21.10.2004

camera

beam-splitter phase grating

analyzer amplitude grating

interference pattern

phase object

λ1

λ2

Polychromatic radiation

Page 57: LMN

C. David, IEEE Conference, Rome, 21.10.2004

camera

beam-splitter phase grating

analyzer amplitude grating

interference pattern

phase object

λ1

λ2

Polychromatic radiation

Page 58: LMN

C. David, IEEE Conference, Rome, 21.10.2004

camera

beam-splitter phase grating

analyzer amplitude grating

interference pattern

phase object

λ1

λ2

Polychromatic radiation

Page 59: LMN

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:

Page 60: LMN

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:

Page 61: LMN

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

Page 62: LMN

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

Page 63: LMN

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

Page 64: LMN

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

Page 65: LMN

C. David, IEEE Conference, Rome, 21.10.2004

Pink-beam phase tomography

Page 66: LMN

C. David, IEEE Conference, Rome, 21.10.2004

Required transverse coherence

Page 67: LMN

C. David, IEEE Conference, Rome, 21.10.2004

s camera

d

Required transverse coherence

Page 68: LMN

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

Page 69: LMN

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

Page 70: LMN

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

Page 71: LMN

C. David, IEEE Conference, Rome, 21.10.2004

Summary

Page 72: LMN

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

Page 73: LMN

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 :

Page 74: LMN

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

Page 75: LMN

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

Page 76: LMN

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


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