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<strong>European</strong> <strong>Synchrotron</strong> Radi<strong>at</strong>ion Facility Long-Term Str<strong>at</strong>egy 7 July 2006<br />

4. Beamlines, Experimental, <strong>Scientific</strong> and Computer Infrastructure and<br />

Instrument<strong>at</strong>ion Developments<br />

4.1 Introduction: optics and nano-focusing<br />

<strong>New</strong> science is <strong>the</strong> driving force behind <strong>the</strong> ESRF’s long-term str<strong>at</strong>egy. A common<br />

fe<strong>at</strong>ure of <strong>the</strong> new science summarised in Section 2.3 is <strong>the</strong> need for ever-smaller<br />

beams of extremely high brilliance This trend towards nano-sized beams constitutes<br />

<strong>the</strong> logical evolution of a trend which has been evident from <strong>the</strong> early days of ESRF<br />

oper<strong>at</strong>ion. In <strong>the</strong> ESRF Found<strong>at</strong>ion Phase Report (Red Book) it was expected th<strong>at</strong> a<br />

“micro-focusing beamline” could deliver a beam size of ~30 µm and th<strong>at</strong> most<br />

beamlines would oper<strong>at</strong>e with a beam of about 1 mm dimension. Today, <strong>the</strong> limiting<br />

capability of <strong>the</strong> “micro-focusing” beamlines is to deliver X-ray beams of less than<br />

100 nanometre, but this performance remains far from routine. A “standard” beamline<br />

oper<strong>at</strong>es routinely with sub-millimetre beams. The pressure from scientists and users<br />

to have routine beams of 10 µm or less (down to 1 µm) is enormous. The reasons for<br />

this are multiple and reflect many facets of <strong>the</strong> scientific case outlined in Section 2.<br />

For example <strong>the</strong>y are needed:<br />

• to study small crystals of all m<strong>at</strong>erials, protein crystals, novel m<strong>at</strong>erials, nanostructures,<br />

quantum confined structures;<br />

• to investig<strong>at</strong>e efficiently samples in extreme and exotic <strong>the</strong>rmodynamic<br />

conditions; pressures up to 3 Mbar; temper<strong>at</strong>ures up to 5000 K and down to <strong>the</strong><br />

sub-Kelvin region; magnetic fields up to 50 Tesla; combin<strong>at</strong>ions of such<br />

conditions;<br />

• to develop advanced techniques, such as coherent X-ray sc<strong>at</strong>tering and<br />

spectroscopy and, more generally, to combine imaging techniques with X-ray<br />

sc<strong>at</strong>tering and absorption techniques to develop new X-ray methodologies.<br />

Recent work performed by teams of ESRF scientists and external collabor<strong>at</strong>ors has<br />

demonstr<strong>at</strong>ed a world leading performance in focussing X-ray beams of about 20<br />

keV to less than 50 nm, using ei<strong>the</strong>r a dynamically bent graded multilayer device or<br />

an assembly of compound refractive lenses. In order to implement efficient focusing<br />

options in <strong>the</strong> sub-micron region on generic beamlines providing stability and<br />

comp<strong>at</strong>ibility with sophistic<strong>at</strong>ed sample environment equipment, it is necessary to<br />

construct optical devices capable of very large source demagnific<strong>at</strong>ion, in <strong>the</strong> range 1<br />

in 1000 to 1 in 10,000. These requirements pose a number of new challenges. Not<br />

only <strong>the</strong> optical quality of reflecting and refracting devices must be outstanding, but<br />

also <strong>the</strong> temper<strong>at</strong>ure and vibr<strong>at</strong>ion stability of <strong>the</strong> experimental environment must<br />

s<strong>at</strong>isfy extremely demanding criteria.<br />

The “long” beamlines to enable <strong>the</strong>se demagnific<strong>at</strong>ion r<strong>at</strong>ios need to be sensibly<br />

longer than a typical ESRF beamline, which is ~ 50 m, extendable to a maximum<br />

length of 70 m. In fact, with a 1:1000 demagnific<strong>at</strong>ion <strong>at</strong> 50 m from <strong>the</strong> source, only<br />

50 mm would be available between <strong>the</strong> centre of <strong>the</strong> optical device to <strong>the</strong> focal spot.<br />

This could be increased to a much more comfortable value of 120 mm if <strong>the</strong> beamline<br />

length could be extended to 120 m. The possibility to have a secondary source can<br />

be a key parameter for <strong>the</strong> improvement of <strong>the</strong> stability and <strong>the</strong> overall control of <strong>the</strong><br />

critical parts of an experiment using very small beams. This option, if implemented<br />

efficiently, also requires a beamline <strong>at</strong> least twice as long as th<strong>at</strong> typically possible<br />

today. Already, as part of <strong>the</strong> ESRF’s Medium Term <strong>Scientific</strong> Plan, two pilot nano-<br />

20

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