% IMPORTANT: The following is UTF-8 encoded. This means that in the presence
% of non-ASCII characters, it will not work with BibTeX 0.99 or older.
% Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or
% “biber”.
@MASTERSTHESIS{Smitmanns:907315,
author = {Smitmanns, Hendrik},
title = {{M}easurements of {T}ransitions between {D}ifferent
{H}yperfine {S}tructure {S}ubstates of {H}ydrogen using a
{S}ona {T}ransition {U}nit},
school = {RWTH Aachen},
type = {Masterarbeit},
reportid = {FZJ-2022-01958},
pages = {71},
year = {2022},
note = {Masterarbeit, RWTH Aachen, 2022},
abstract = {Nuclear spin polarization and its phenomena have been
studied since the early days of quantum mechanics. Today, in
particular, nuclear spin polarized hydrogenand deuterium are
used in many ways, e.g. as target material or in the form of
polarized beams. One way of measuring the polarization of
such a beam is the Lambshiftpolarimeter. In an experiment
conducted at the Institut für Kernphysik of the
Forschungszentrum Jülich to study the influence of a Sona
transition unit on thepolarization of a nuclear
spin-polarized hydrogen beam, unexpected oscillations of the
occupation numbers of different hyperfine substates of
hydrogen atoms as a functionof the magnetic field were
discovered. The oscillations are induced within the Sona
transition unit, which allows an exchange of the occupation
numbers of the alpha 1 andbeta3 states by reversing the
direction of the magnetic field defining the quantization
axis.The transition energies between the different substates
were in the range of only a few neV. In order to investigate
this phenomenon further, a similar experiment is set up in
Jülich which allows measuring these oscillations of the
occupation numbers of metastable $2S_1/2$ hydrogen as well
as the recording of the thereby produced spectra of the two
alpha states. In addition, an analysis method is developed
and applied to determine the energies of the transitions
that occur between the different substates. The aim of the
method is to measure these transition energies with an
accuracy that allows the QED corrections to the classical
Breit-Rabi formula to be detected.},
cin = {IKP-2 / PGI-6 / IKP-4},
cid = {I:(DE-Juel1)IKP-2-20111104 / I:(DE-Juel1)PGI-6-20110106 /
I:(DE-Juel1)IKP-4-20111104},
pnm = {612 - Cosmic Matter in the Laboratory (POF4-612)},
pid = {G:(DE-HGF)POF4-612},
typ = {PUB:(DE-HGF)19},
url = {https://juser.fz-juelich.de/record/907315},
}