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Neutron Scattering

Neutron Scattering - JuSER - Forschungszentrum Jülich

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1 . <strong>Neutron</strong> Sources<br />

Harald Conrad<br />

1 .1 Introductory remarks<br />

Slow neutrons are a virtually unique probe for the investigation of structure and dynamics of<br />

condensed matter and biomolecules . <strong>Neutron</strong>s are called slow, if their kinetic energy is below<br />

1 keV. As the first neutrons used as microscopic probes were generated in nuclear reactors,<br />

historic terms like thermal neutrons are also frequently used in the classification of neutrons .<br />

In reactor physics the term thermal is used to distinguish these neutrons, which sustain the<br />

nuclear chain reaction, from the fart fission neutrons with energies of several MeV . Thermal<br />

neutrons, i.e . with an average kinetic energy of - 25 meV, are of particular interest in the<br />

context of this course . They are in thermal equilibrium with an adequate slowing down medium<br />

(moderator) like graphite, light or heavy water at ambient temperature (kBT - 25 meV) .<br />

With the availability of cryogenic moderators, cold neutrons ( = 3 meV) became important<br />

in recent decades, too . Strictly speaking, cold or so called trot neutrons ( = 200 meV) have<br />

to bc considered as thermal, too, because these are neutron gases in thermal equilibrium with<br />

a moderator at a particular temperature . Cold neutrons are in equilibrium with a cryogenic<br />

moderator, e .g . liquid hydrogen at 20 K or solid methane at liquid nitrogen temperature, 77 K .<br />

Hot neutrons are those in equilibrium with e .g . a graphite block heated to 2000 K, say .<br />

These trot neutrons and the even more energetic, so called epithermal neutrons (E > 1 eV)<br />

may in the future gain importance for scattering experiments, in particular with respect to<br />

pulsed accelerator driven neutron sources (sec below). But it is important to realize that there<br />

are no primary sources known, which directly deliver neutrons in the relevant energy range of<br />

typically 10 -3 eV < E < 1 eV . All existing sources emit primary neutrons with energies of<br />

about 10 6 eV or above and we are left with the difficult task to reduce the neutron energy<br />

between 6 and 9 orders of magnitude (moderation) .<br />

1 .2 Free <strong>Neutron</strong>s<br />

Free neutrons are unstable (half life about 12 minutes) . As a nuclear constituent they are stable,<br />

though, and as bound particles virtually ubiquitous, except in light hydrogen. So, the only<br />

means of generating free neutrons are nuclear reactions . There is a variety of possible reactions,<br />

mostly forced ones, although spontaneous neutron emission is known to exist as well. A

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