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Wed 06 Nov
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Alexandre Gillet
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Clustering in granular matter
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Excited granular matter driven by external forces is a rich
pattern-forming system. It exists in numerous form from microscopic
particles to macroscopic gravels. Granular systems with high density
exhibit interesting properties such as clustering instability. In
dissipative granular gases where collisions are inelastic, particles tend
to form dense clusters. A slight variation of density, pressure or
temperature leads to this peculiar physical process. Particle
interactions,
i.e. collisions, combined with gravity may lead to cluster formation.
The talk discusses how the temperature has an impact on the density
fluctuation in the system and how the nature of the particle collisions is
changing as the temperature decreases.
Literature:
M.X. Lim, A. Souslov, V. Vitelli, and H. M. Jaeger,
"Cluster formation by acoustic forces",
Nature Phys. 15, 460–64 (2019);
I. Goldhirsch, G. Zanetti,
"Clustering Instability in Dissipative Gases",
Phys. Rev. Lett. 70, 1619–22 (1993).
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Wed 13 Nov
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Marian Dawidczak
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Six easy roads to the Planck scale
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The Planck length is a fundamental minimum to the classical concept of
spacetime. Beyond this scale the nature of spacetime must be reconsidered
since quantum effects cannot be neglected anymore. These properties are
responsible for why the Planck scale has an important role in present and
future theories of quantum spacetime and quantum gravity.
This talk uses elementary, heuristic and plausible arguments to find the
Planck scale in 6 different thought experiments.
Literature:
Ronald J. Adler,
"Six easy roads to the Planck scale",
Am. J. Phys. 78 (9), 925–32 (2010).
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Wed 20 Nov
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Ida Sigusch
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Simple estimation of CO2 contribution to the greenhouse effect
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The topic of climate change, especially global warming, has gained more awareness in
popular and scientific discussions during the last decades. Derrek J. Wilson and Julio Gea-Banacloche
worked out a model for a simple estimation of the contribution of CO2 to the greenhouse effect. The
main indicator for the impact is the so called "climate sensitivity", which gives the increase in temperature caused by a doubling of the concentration of CO2, under the main
assumption of no feedbacks. The evaluation of this simple model is done in two steps.
The first step is to give an upper bound for the climate sensitivity based on photons
performing a random walk in the atmosphere. In the second step, the calculation is done using
the radiative transfer equation and therefore the molecular absorption spectrum has to be taken into
account. The second model is to be found in fairly good agreement with currently accepted values.
Literature:
Derrek J. Wilson and Julio Gea-Banacloche,
"Simple model to estimate the contribution of atmospheric CO2 to the
Earth's greenhouse effect",
Am. J. Phys. 80 (4), 306–15 (2012).
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Wed 11 Dec
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Jann Winkler
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Fixational Eye Movements and Random Walks
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Small and jerky movements of the eye (so called Microsaccades),
while we are fixing an object,
are essential for high acuity vision. These movements can be
considered as a stochastic process and are described by models
of anomalous diffusion.
In previous analyses of experimental data, it was found that the
mean-squared-displacement on long time-scales shows oscillations.
To explain these,
Hermann, Metzler and Engbert propose a new model that
combines a self-avoiding random walk with neuronal time-delay.
Literature: C.J.J. Herrmann, R. Metzler, and R. Engbert,
"A self-avoiding walk with neural delays as a model of
fixational eye movements",
Sci. Rep. 7, 12958 (2017).
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Wed 08 Jan
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Nina Kunert
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Gravitational waves without general relativity
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The recent observations of gravitational waves have excited the physic
community and the general public. However, to many physicists, the tensor
formalism used in general relativity to formalize gravitational waves seem
rather challenging. Using analogies with the vector based theory of
electromagnetism, Robert C. Hilborn presents a relatively simple model of
gravitational wave radiation emitted by orbiting binaries. This model is
able to describe the detected gravitational wave form observed by the
LIGO-VIRGO observatories and predicted from numerical GR calculations
except for wave forms that result from the final ring-down moments of a
binary merger.
Literature: Robert C. Hilborn,
"Gravitational waves from orbiting
binaries without general relativity",
Am. J. Phys. 86 (3), 186–97 (2018).
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Wed 22 Jan
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Jan Kutschera
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Twisted light and longitudinal field components
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Light can be described as a transverse wave. The electric field of a
light beam can oscillate in a direction perpendicular to the beam
axis, but can also
rotate around it. There are two forms of rotation. One results
from the photon spin which is related to the (circular) polarization of
the beam, it determines the spin angular momentum of light
(SAM). The other is obtained from the wavefront of the light beam and
determines its orbital angular momentum (OAM). In special shaped or
inhomogenous light fields the electric field can also have longitudinal
components. This is for example the case in twisted light where the
wavefronts are helical due to a nonzero OAM and where spin and orbital angular
momentum are antiparallel to each other.
Longitudinal field components are usually neglected for light-matter
interaction in the paraxial approximation.
Quinteiro et al. compare a twisted light model
with experimental data of quadrupole transitions excited
in trapped ions to prove the
relevance of longitudinal field components.
Literature:
G. F. Quinteiro, Ferdinand Schmidt-Kaler and Christian T. Schmiegelow,
"Twisted-Light-Ion Interaction: The Role of Longitudinal Fields",
Phys. Rev. Lett. 119 (2017) 253203.
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