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@ARTICLE{Lenisa:838665,
author = {Lenisa, Paolo and Rathmann, Frank},
title = {{COSY} {P}repares the {F}irst {M}easurement of the
{D}euteron {E}lectric {D}ipole {M}oment},
journal = {Nuclear physics news},
volume = {27},
number = {3},
issn = {1050-6896},
address = {London [u.a.]},
publisher = {Taylor $\&$ Francis},
reportid = {FZJ-2017-07233},
pages = {10 - 13},
year = {2017},
abstract = {One of the most intriguing questions in cosmology and
perhaps in all of physics is: “Why is there so much matter
in the Universe and so little antimatter?” Until today,
there is no evidence for any primordial antimatter within
our galaxy or even beyond. There is no indication for any
form of co-existence of matter and antimatter in clusters or
galaxies within our Universe. Hence, it is usually concluded
that our visible Universe is made entirely of matter and is
intrinsically matter non-symmetric. According to the
combined Standard Models of cosmology and particle physics
it is expected that at the end of the inflationary
epoch—following the Big Bang—the number of particles and
antiparticles were in extreme balance, yet somehow the laws
of physics contrived to act differently on matter and
antimatter in order to generate the current imbalance.
Interestingly, one of the necessary physics mechanisms
required for such effects—namely CP-violation—is very
small in the Standard Model (SM) of particle physics and
thus is only able to account for a tiny fraction of the
actual asymmetry.},
cin = {IKP-2 / JARA-FAME},
ddc = {530},
cid = {I:(DE-Juel1)IKP-2-20111104 / $I:(DE-82)080023_20140620$},
pnm = {612 - Cosmic Matter in the Laboratory (POF3-612) / srEDM -
Search for electric dipole moments using storage rings
(694340)},
pid = {G:(DE-HGF)POF3-612 / G:(EU-Grant)694340},
experiment = {EXP:(DE-Juel1)JEDI-20170712},
typ = {PUB:(DE-HGF)16},
doi = {10.1080/10619127.2017.1317175},
url = {https://juser.fz-juelich.de/record/838665},
}