12.01.2013 Views

Neutron Scattering - JUWEL - Forschungszentrum Jülich

Neutron Scattering - JUWEL - Forschungszentrum Jülich

Neutron Scattering - JUWEL - Forschungszentrum Jülich

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

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.

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!