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PHYS01200804001 Sohrab Abbas - Homi Bhabha National Institute

PHYS01200804001 Sohrab Abbas - Homi Bhabha National Institute

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to record the first neutron diffraction pattern from a macroscopic grating of 200 m period. The<br />

transverse coherence length of 175 m (FWHM) extracted from the analysis of this pattern is the<br />

greatest achieved to date for Å wavelength neutrons.<br />

A magnetic air prism between the monochromator and analyser Bragg prisms can separate the upand<br />

down-spin components of the neutron beam, thus providing a polarised SUSANS facility [166-<br />

168].<br />

As indicated in Chapter 4, one can produce even tighter neutron collimation by employing other<br />

Bragg reflections, asymmetry and apex angles. The monochromator and analyser Bragg prisms<br />

characterised in Chapter 4 can be used to produce a sharper neutron beam by employing higher<br />

order reflections. This Bragg prism pair operating near {333} Bragg incidence of 1.75 Å neutrons<br />

can achieve a 0.065 arcsec wide rocking curve. The transverse coherence length of 525 μm<br />

(FWHM) of this beam will facilitate SUSANS studies down to 3x10 -7 Å -1 and characterise<br />

agglomerates up to 450 μm in size. A magnetic air prism between the monochromator and sample<br />

would then yield a Polarised submicro-Å -1 SUSANS facility.<br />

One may envisage tightening the neutron collimation further with Bragg prisms operating at still<br />

smaller wavelengths. However, there are practical limits such as the mechanical stability of the<br />

apparatus, the minimum rotation step achievable for the goniometer and the inherent weakness of<br />

neutron sources in terms of flux. Only when the next generation neutron sources like Inertial<br />

Confinement Fusion based or advanced pulsed sources, becomes operational, may Bragg prisms be<br />

able to deliver sufficiently strong neutron beam with extremely narrow angular profiles.<br />

However, with X-rays, these novel Bragg prisms can produce sharper angular profiles than neutron<br />

beams as photon flux available currently is many orders of magnitude greater compared to<br />

neutrons.<br />

121

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