Group
information
We study
the cosmos
through
numerical
simulations
and
computational
modeling.
Our
research
spans
multiple
physical
scales,
addressing
key
questions
in:
-
Cosmology:
exploring
the
large-scale
structure
of
the
universe,
dark
matter,
and
the
formation
and
evolution
of
galaxies.
-
Galactic
Dynamics
and
Structure:
investigating
the
formation
and
evolution
of
galaxies,
their
rotation
curves,
star
formation,
and
stellar
feedback.
-
Interstellar
Medium
(ISM)
and
Molecular
Clouds:
modeling
the
turbulent,
magnetized
gas
that
gives
birth
to
stars,
including
the
role
of
gravity,
magnetic
fields,
and
stellar
feedback.
-
Star
Formation:
studying
the
gravitational
collapse
of
dense
cores
within
molecular
clouds,
fragmentation
processes,
and
accretion
phenomena.
-
Protoplanetary
Discs:
simulating
the
dynamics
and
evolution
of
discs
around
young
stars,
including
planet-disk
interactions,
migration,
and
disc
fragmentation.
To tackle
these
complex,
multi-scale
problems,
we employ
a suite of
advanced
numerical
tools,
including
AREPO,
FLASH,
Gadget,
FARGO3D, and
Torch. These
codes
allow us
to
simulate
hydrodynamics,
magnetohydrodynamics,
gravity,
and
radiation
with high
resolution
and
physical
realism.
As a
group, we
are
committed
to
contribute
actively
to the
international
scientific
community.
Through
collaboration
and
rigorous
numerical
experimentation,
we aim to
study the
complex
physical
processes
that shape
our
universe.
Welcome to
our
webpage,
where the
wonders of
the
universe
come alive
through
the power
of
computation!