Joachim Kopp — Research Activities
Student: Dr. Einstein, aren't these the same questions as last year's final exam?
Dr. Einstein: Yes; But this year the answers are different.
We study theoretical extensions of the Standard Model of Particle Physics
that attempt to answer some of the most fundamental questions of modern
particle physics, astrophysics, and cosmology:
- What is the nature of Dark Matter?
- How is the electroweak gauge symmetry broken?
- Why are there three generations of elementary particles?
- What determines the patterns among particle masses and mixing
angles?
- ...
While many theoretical ideas exist to solve at least some of these problems,
ultimate answers can only be provided by experiments. Our work therefore
strongly emphasizes phenomenology, i.e. the observable consequences of the
theories we study. We are particularly interested in three broad classes of
experiments.
DARK MATTER SEARCHES.
The existence of Dark
Matter — evidenced by a variety of astrophysical and cosmological
observations — is perhaps the strongest hint for the incompleteness of
the Standard Model of particle physics. The nature of dark matter, however,
remains a mystery. Fortunately, experiments are rapidly improving and can thus
test the parameter space of the most promising theoretical models. They do this
by searching for dark matter interactions with atomic nuclei or
electrons in a terrestrial detector, by looking for the annihilation or
decay products of dark matter in high-energy cosmic rays, and by studying
the impact of dark matter on the evolution of the Universe as a whole.
However, exploiting the experimental results to their full extent requires
strong theoretical efforts as well. We use experimental data to constrain
theories of dark matter, and as a guideline for developing novel and improved
theories of dark matter. This requires a deep understanding of the particle
physics aspects of dark matter, but also of astrophysical concepts and of the
physics of the early Universe.
NEUTRINOS.
Our understanding of neutrinos has skyrocketed in
the past two decades. Neutrino physics today is a precision science that has
the potential to teach us a lot about the origin of the observed mass and
mixing patterns among elementary particles. Moreover, being electrically
neutral, neutrinos are the only Standard Model fermions that can mix with new
particles that are uncharged under the Standard Model gauge group. An important
example for such new particles are sterile neutrinos,
which in turn could be related to the Dark Matter in the Universe.
When studying neutrino phenomenology, we focus in particular on neutrino
oscillations, the periodic conversion of one neutrino flavor into another.
On the one hand, we investigate the quantum mechanical underpinnings of this
phenomenon, for instance the coherence
conditions required for neutrino oscillations to occur. On the other hand, we
make detailed predictions that can be tested in present or future neutrino
oscillation experiments, we study how these experiments can distinguish between
different theoretical frameworks, and we compare our predictions to
experimental data. Our main tools are analytical calculations as well as
numerical simulations such as
GLoBES, which we use and develop as needed.
COLLIDERS, in particular the flagship of particle physics, the
Large
Hadron Collider (LHC).
Virtually all extensions of the Standard Model involve
new particles beyond the three known families of quarks and
leptons, the SU(3) x
SU(2) x U(1) gauge
bosons, and the Higgs boson. If these
new particles are not too heavy, they can be produced at the
LHC,
and they can be observed in the
ATLAS and
CMS detectors. Moreover, new
particles can
alter the behavior of Standard Model particles such as neutral
mesons, which are studied with great precision by
LHCb.
Our work in collider physics involves predicting production cross sections and
decay rates for new particles, developing search strategies, validating these
search strategies with realistic numerical simulations, and, wherever possible,
using real data to constrain the theoretical models we study.
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