Neutron Scattering - JUWEL - Forschungszentrum Jülich
Neutron Scattering - JUWEL - Forschungszentrum Jülich
Neutron Scattering - JUWEL - Forschungszentrum Jülich
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RESEDA 11<br />
The neutrons are counted in 3 He detectors. RESEDA uses four points of an echo group<br />
to analyze the polarization. These four points are separated by a π/2-rotation of the spin<br />
phase. The measured signals do not necessarily correspond to the exact maximum or<br />
minimum of the amplitude. Nevertheless this method allows to obtain the polarization<br />
in a short measurement time with good statistics and without knowing the exact phase<br />
of the neutron spin.<br />
The measurements of the phase of the neutron spin may be disturbed by external<br />
magnetic stray fields. Therefore, the spectrometer arms and sample region of RESEDA<br />
is surrounded by a double Mu-metal shielding (very high permeability of μr ≫ 10000)<br />
which compensates small stray fields.<br />
4.2 The samples under study<br />
At RESEDA, quasi-elastic dynamics in the spin echo time range 1.5 ps to 2 ns is<br />
routinely studied. In the laboratory course, two samples will be used. A standard<br />
elastically scattering sample is used to verify the operation of the instrument, and, in<br />
particular, to check the polarization of the spin rotation signal and the spin echo signal.<br />
The quasi-elastic measurements are performed on a magnetically scattering sample<br />
which exhibits helical magnetic ordering (figure 8) below the temperature of 28.5 K.<br />
The quasi-elastic dynamics are studied slightly above this temperature.<br />
Figure 8: Schematic magnetic ordering structure of MnSi below 28.5 K. The spins form a helix with<br />
wavelength λ (therefore the name „helical phase“). a is the lattice spacing of the MnSi crystal.<br />
5 Preparatory Exercises<br />
1. Read this instruction carefully.<br />
2. Calculate the energy and velocity of the neutrons accessible at RESEDA (cold<br />
source!). Calculate the time the neutrons need to pass the spectrometer arms<br />
(total length 8 m).<br />
3. Look up the typical value of the earth‘s magnetic field. Calculate the precession<br />
frequency of the neutron spin in this field (gyromagnetic ratio!). Conclude with<br />
2. on the spin phase accumulated at RESEDA, if there was no mu-metal<br />
shielding.