E. Buffagni, C. Ferrari, L. Zanotti, A. Zappettini

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E. Buffagni, C. Ferrari, L. Zanotti, A. Zappettini IMEM-CNR Institute, Parma (Italy)

1. Laue lenses for hard x-ray astronomy 2. Mosaic crystals 3. GaAs crystals 4. X-ray diffraction characterization 5. Artificial mosaic crystals 6. Conclusions Channeling 2010 Ferrara, October 3-8 2

1. Laue lenses for hard x-ray astronomy Hard x-rays: E > 60 kev Bragg law: very small incident angle NO OK H. Halloin and P. Bastie, Exp. Astron. 20 (2005) 151 Channeling 2010 Ferrara, October 3-8 3

1. Laue lenses for hard x-ray astronomy Spherical shape with radius R Focal length f=r/2 Crystal tiles, as small as possible, with lattice planes perpendicular to the front surface Resolution a few tens of arcsec Fundamental requirement a few tens of arcsec of angular acceptance D. Pellicciotta et al., IEEE Trans. Nucl. Sci. 53 (2006) 253 Channeling 2010 Ferrara, October 3-8 4

1. Laue lenses for hard x-ray astronomy Perfect crystal FWHM ~ 0.06 arcsec Ge 400 diffraction at 500 kev r e = electronic radius = wavelength F H = structure factor d = lattice spacing V = crystal cell volume To improve the collection efficiency MOSAIC CRYSTALS can be used Channeling 2010 Ferrara, October 3-8 5

2. Mosaic crystals Crystal made of microscopic perfect crystal domains (crystallites) slightly misoriented with respect to each other Mosaic spread Bandwidth diffracted by the crystal Channeling 2010 Ferrara, October 3-8 6

3. GaAs crystals Grown by using the Liquid Encapsulated Czochralsky (LEC) technique The same crystal structure (fcc), lattice spacing, and electron density of Ge crystals Spontaneous mosaicity, that can be controlled by changing growth parameters Channeling 2010 Ferrara, October 3-8 7

4. X-ray diffraction characterization by means of a high resolution X-Pert Pro Philips diffractometer Cu anode Perfect GaAs crystal FWHM(004) = 15.8 arcsec CuK 1 =0.15405 nm Channeling 2010 Ferrara, October 3-8 8

4. X-ray diffraction characterization Sample: slice cut along the growth axis of a GaAs ingot 004 diffraction profiles Channeling 2010 Ferrara, October 3-8 9

4. X-ray diffraction characterization Sample: slice cut along the growth axis of a GaAs ingot Mosaic spread Central zone (from -20 to 20 mm) with nearly constant value: ~ 18 arcsec Channeling 2010 Ferrara, October 3-8 10

4. X-ray diffraction characterization Sample: wafer cut perpendicularly to the growth axis of a GaAs ingot 004 diffraction profiles -20 mm 20 mm Channeling 2010 Ferrara, October 3-8 11

4. X-ray diffraction characterization Sample: wafer cut perpendicularly to the growth axis of a GaAs ingot Mosaic spread -20 mm 20 mm follows the typical W shape of the dislocation density Channeling 2010 Ferrara, October 3-8 12

4. X-ray diffraction characterization Mosaic spread obtained from rocking curves collected near the centre of wafers cut at different heights of ingots grown in different conditions sample N 096: Cr-doped samples N 183, 193, 206, MB: undoped stoichiometric samples N 190, 191: As-rich Growth conditions and doping may affect the mosaic spread Channeling 2010 Ferrara, October 3-8 13

5. Artificial mosaic crystals A complementary strategy to increase the Darwin width of the diffraction curve can be the use of artificial mosaic crystals: STACKS OF CURVED CRYSTALS High diffraction efficiency Broad energy bandwidth R. K. Smither et al., Exp. Astron. 20 (2005) 201 Stack of curved crystals Channeling 2010 Ferrara, October 3-8 14

5. Artificial mosaic crystals The curvature is obtained by introducing a compressive stress on the crystal surface by damaging it with fine sand paper compressive strain curvature Stoney formula Thickness t Angular acceptance Analyzed materials: Si crystals GaAs crystals It is possible to check the crystal curvature monitoring the angular shift of the rocking curves Channeling 2010 Ferrara, October 3-8 15

5. Artificial mosaic crystals After a treatment of three hours with sand paper Shift ~ 0.006 Shift ~ 0.05 Channeling 2010 Ferrara, October 3-8 16

5. Artificial mosaic crystals <R> ~ 58 m y x Channeling 2010 Ferrara, October 3-8 17

5. Artificial mosaic crystals Si doped Dislocation free sample FWHM = 15 arcsec After a treatment of 10 minutes with sand paper Rocking curves collected along two perpendicular direction y x Channeling 2010 Ferrara, October 3-8 18

6. Conclusions GaAs is suitable for hard x-ray Laue lens due to its mosaic structure It is possible to tailor the mosaic structure by adjusting the growth conditions or introducing dopants The mosaic spread measured in different GaAs crystals varies between 10 and 40 arcsec An alternative optical element for the Laue lens made of a stack of curved crystals is proposed Nearly spherical curvature can be obtained in Si and GaAs samples by introducing a crystal surface damage Channeling 2010 Ferrara, October 3-8 19

Thank you for your attention Channeling 2010 Ferrara, October 3-8 20

GaAs As first approximation the diffraction efficiency is linked to the electronic density (in figure) H. Halloin, Exp. Astron. 20 (2005) 171 Channeling 2010 Ferrara, October 3-8 21

Growth parameters boron oxide thickness of 15 mm argon counter pressure of 20 atm thermal gradient at solid/liquid interface in the range of 30-50 C pulling rate of 10 mm/h growth direction: <100> Schematic of LEC growth Channeling 2010 Ferrara, October 3-8 22

Low angle grain boundaries Channeling 2010 Ferrara, October 3-8 23

= extinction length = Darwin width Variation of the angle of incidence on reflecting planes due to the distortion Condition for application of geometrical optics If we define In a distorted crystal the transition from the dynamical to the kinematical diffraction theory can be driven also by the distortion dynamical C. Malgrange, Cryst. Res. Technol. 37 (2002) 7 decreasing wavelength decreasing structure factor kinematical Channeling 2010 Ferrara, October 3-8 24

Channeling 2010 Ferrara, October 3-8 25

5. Artificial mosaic crystals Mosaic crystal After a treatment of 5 minutes with sand paper from 0 up to 25 arcsec <R> ~ 8 m t = 1 cm ~ 4 minutes of arc Channeling 2010 Ferrara, October 3-8 26