The system of neutron optics for the diffractometer E PSILON and SKAT

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The system of neutron optics for the diffractometer E PSILON and SKAT. Walther A. Bulkin Frischbutter V. Kudryashov Ch. Scheffzük F. Schilling. V. Zhuravlov A. Sirotin E. Shabalin I. Natkaniec S. Manoshin S. Kulikov A. Belushkin A. Balagurov. Thanks to:. - PowerPoint PPT Presentation

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The system of neutron optics for the diffractometer EPSILON and

SKAT

K. Walther

A. Bulkin

A. Frischbutter

V. Kudryashov

Ch. Scheffzük

F. Schilling

Thanks to:

♦V. Zhuravlov♦A. Sirotin♦E. Shabalin♦I. Natkaniec♦S. Manoshin♦S. Kulikov♦A. Belushkin♦A. Balagurov

Historical review(1):

♦1983 - reactor IBR-2 became critically♦1983 – the diffractometer NSWR, built in the

workshop of the TU Dresden, was mounted at beamline 7

♦1983 - first plans for a long flight path for an inelastic spectrometer with inverted geometry

♦1984 - idea for an additional multipurpose- instrument:

○quasi-elastic scattering

○high resolution diffraction

○texture investigation

Historical review(2):

♦1985 - sputtering of glass with Cr/Ni and production of the glass segments for both guides in the workshop of the FLNP

♦1986 - commissioning of the instrument NSWR at the long flight path

○for the multi-purpose instrument it was realised only the texture unit

♦1995 - early variant of EPSILON

♦1996 - replacement of NSWR by SKAT♦2007 - begin of the reconstruction of the

former neutron guide 7A

What do we expect from a good diffractometer?

♦Good spectral resolution♦Good spatial resolution♦High intensity♦Low background♦Good sample environment

In-pile improvements for high intensity:

♦ In order to reduce the attenuation due to absorption and scattering at this side should be built in an evacuated tube

♦ Start of the neutron guides as near as possible to the chopper

♦ built in of a guide splitter

Reduction of the background with a background chopper

♦Pulse reactor IBR works as a low power steady state reactor (≈ 100 kW)

♦Every 200 ms a high power neutron pulse is generated (≈ 1000 MW)

Background chopper(1)

♦Flight path: 102≤l1+l2≤110 m

♦resulting velocity for travelling within 200 ms 510≤v≤550 m/s

♦cut-off wavelength due to frame overlapping:

λc-o =7.75Å and 7.19Å, respectively

♦opening in the chopper disk (dist. = 5.5m) 19.4° and 18°, respectively

♦opening of the chopper 10.8 ms and 10 ms, respectively (for a beam of zero width)

Background chopper(2)

Calculations of the transmission function of the background chopper were done for:

♦“Standard” (old) mounting: chopper axis is below the entrance windows of the guides

○edges radial○edges parallel

♦“alternative” mounting: chopper axis is at the same height but aside the entrance windows○edges radial○edges parallel

Guide splitter(1)

♦All guides start closer to the moderator♦The three guides do not “disturb” each other♦at the end of the guide splitter 3 separate

neutron guides will start ♦all guides are evacuated.

Lambda-chopper(1)

♦The 7th beam line will have partial sight on the cold source

♦There is a need to have neutrons beyond the frame overlapping, both for EPSILON and SKAT

due to the large unit cells of some minerals♦Every second power pulse could be eliminated

by an additional chopper♦The back ground chopper should provide this

extended wavelength range too

Lambda-chopper(2)

Lambda-chopper(3)

Lambda-chopper(4)

Neutron guide and some fundamental mathematics

♦Neutrons are classical mechanical particles○They have a mass mo

○They have a velocity v

○They have a momentum p

Neutron guide and some fundamental mathematics(2)

♦Neutrons are waves○They have a wave length

The wave length λ is connected with the flight time t byt

llm

h

210

1

Neutron guide and some fundamental mathematics(3)

In time-of-flight diffraction patterns you see peaks in a distribution of the number of diffracted neutrons (intensity) over the wavelength for a given scattering angle ϑ.

According to BRAGG‘s law

sin2 d we get

tllm

hd

sin

11

2

1

210

Spectral Resolution

cott

t

d

d

Spectral resolution can be improved by increasing the flight path!

Neutron guides♦Classical neutron guides are based on the

phenomena „total reflection“ like fibre optics

♦Small total reflection angles in the order of minutes of arc

♦Only few minerals/elements are of interest

♦Angle of total reflection is proportional to the wavelength

♦Angle of total reflection of Ni with natural abundance of isotopes defines the value m=1.0 which corresponds αtot=0.1°

♦Ni58 corresponds m=1.2

Neutron guides(2)

♦Neutron guides are built of well aligned glass sections

♦The surface of the glass should have nearly no roughness

♦Boron glass meets the requirements♦Neutron guides for thermal neutrons are

bent in the most cases

Neutron guides(2)

♦Neutron guides are built of well aligned glass sections

♦The surface of the glass should have nearly no roughness

♦Boron glass meets the requirements♦Neutron guides for thermal neutrons are

bent in the most cases

Neutron guides(3)♦The neutron guides for EPSILON and SKAT are

built up of sections 1 m long♦The sections are 95 mm high and 50 mm wide♦The first part (within the splitter) is straight♦The next part about 80 m length is bent; radius

of curvature:13 400 m♦Bent neutron guides transport only neutrons

with a wavelength greater the critical wavelenght, which depends on the width and the radius of bending.The critical wavelength is 1.58 Å

♦In order to homogenize the flux across the section the last part are straight

Outlook and conclusion

♦After realization the new neutron guides and the chopper system there are created two high level diffractometers for long wavelength diffraction

Acknowledgment

- the BMBF Germany,

- FLNP Dubna

- Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences

- Karlsruhe Institute for Technology

for support

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