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Wed 28 Nov
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Mathis Manzel
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Fixational eye movements and random walks
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Statistics are an important tool in many fields of
physics. They can not only be found in calculations regarding huge
ensembles of particles (e.g. gases) but also describing random movements
of small objects in more microscopic invironments (e.g. diffusion).
Methods like mean square displacement or autocorrelation functions help us
to better understand the nature of such random movements. In order to
focus on objects of interest, the human eye exhibits fixational eye
movments (FEMs) with sub- and superdiffusive movement patterns. These can
be described via self avoiding walk simulations to provide a better
understanding of their origin.
Literature:
Carl J.J. Herrmann et al.,
"A self-avoiding walk with neural
delays as a model of fixational eye movements",
Sci. Rep. 7, 12958 (2017).
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Wed 05 Dec
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Simon Schöll
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CO2's contribution to the Earth's greenhouse effect — a simple estimation
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The climate change and fake news on its scientific background are among the
biggest problems humanity faces in the beginning of the 21st century. In this
talk the contribution of CO2 to the natural greenhouse effect and the
direct warming by doubling the atmospheric CO2 concentration (without
taking feedbacks into account) will be estimated based on physical laws and
basic mathematics.
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, 306 (2012).
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Wed 05 Dec
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Julius Eberhard
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Two Einstein results from the Jarzynski equality
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When disturbing a thermally equilibrated system in an irreversible way, the
second law of thermodynamics is usually expressed as an inequality. The
difference of free energy before and after the disturbance will remain smaller
than the average work necessary to create the disturbance. Hence, the Jarzynski
equality may provide a surprise by introducing an equal sign relating simple
functions of free energy differences and nonequilibrium work amounts. Its
validity and scaling constraints are illustrated by deriving from the equality
two findings of Einstein: first, the relation between diffusion coefficient,
temperature, and drag coefficient in Brownian motion, and second, the necessity
for stimulated emission in light-absorbing two-state systems.
Literature:
F. Gittes,
"Two famous results of Einstein derived from the Jarzynski equality",
Am. J. Phys. 86(1), 31–35 (2018).
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Wed 12 Dec
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Marie Zeller
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The apparent "super-Carnot" efficiency of hurricanes:
Nature's steam engine versus the steam locomotive
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The thermodynamics of a hurricane is presented in comparison of that of a
normal steam engine. The paper states a hurricane has "super-Carnot"
efficiency and this is consistent with the 2nd law of thermodynamics. How
this is (or is not) possible will be calculated and discussed.
Literature:
Jack Denur, "The apparent 'super-Carnot' efficiency of hurricanes:
Nature's steam engine versus the steam locomotive",
Am. J. Phys. 79(6), 631–43 (2010).
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Wed 12 Dec
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Erich Ohlhäuser
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Quantum entanglement with Freedman's inequality
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In 1935, eight years after the Copenhagen interpretation (1927)
A. Einstein, B. Podolski and N. Rosen published a paper
where they showed that the quantum mechanical description
of physical reality is not complete. That conclusion rested
on the seemingly reasonable assumptions of locality and realism.
Almost thirty years later, in 1964, Bell showed theoretically
that quantum mechanics cannot be real and local at the same time,
so that one of the assumptions must be wrong.
Only eight years later, the first Bell inequality ever tested
was the simple version derived by S. Freedman.
By using the Freedman's inequality, students can contradict
the philosophical assumption of local realism
in correlated photon experiments.
Literature:
J. Brody and C. Selton,
"Quantum entanglement with Freedman's inequality",
Am. J. Phys. 86, 412–16 (2018).
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Wed 19 Dec
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Oliver Franke
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Power spectral density of a single Brownian trajectory
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Usually stochastic trajectories are studied in terms of their mean
squared
displacements. An alternative evaluation is based on the power spectral
density (PSD). The paper analyzes what information on the PSD can be
extracted from a single trajectory for a finite observation time. The
authors have mathematically proven that the scaling exponent for the
frequency-dependence of the ensemble-averaged PSD can be already
obtained
from a single trajectory for continuous-time Brownian motion. The
distribution of its amplitude is calculated exactly identifying the
appropriate frequency window. They show that the diffusion coefficient
can
be extracted by averaging over a small number of trajectories. These
analytical results are verified by numerical simulations and
experiments.
Literature: Diego Krapf et al.,
"Power spectral density of a single
Brownian trajectory: what one can and cannot learn from it",
New J. Phys. 20, 023029 (2018).
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Wed 09 Jan
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Max Pritzkuleit
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Gravitational waves without general relativity
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In 2015, the LIGO and VIRGO detectors observed
for the first time gravitational waves
emitted by two merging black holes. Einstein
predicted the existence of gravitational waves using his theory of
general relativity, but other suggestions had been made
before. In the paper, the properties of
gravitational waves emitted by orbiting binary objects are calculated
using analogies with electromagnetic radiation, as a physicist might
have done prior to 1915. The calculations are using Newtonian
mechanics, electromagnetic theory and the technique of retarded time.
The results will be compared with the observed signal.
Literatur:
R. C. Hilborn, "Gravitational waves from orbiting binaries
without general relativity", Am. J. Phys. 86(3),
186 (2018).
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Wed 09 Jan
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Maximilian Mattern
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Quantum anomalies in Bose-Einstein condensates
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One of the most powerful methods in physics is based on symmetries and
groups. The analysis of the symmetry group of the Hamilton operator
often predicts the physical behavior of the system. When this symmetry is
violated, the dynamics of the system change and a (quantum) anomaly
occurs. We analyse a two-dimensional gas in a harmonic potential with a
delta-function interaction potential. In classical and in quantum
mechanics, such a trapped gas shows a collective oscillation,
a so-called
"breathing mode" at exactly twice the trap frequency. This is
justified by an underlying symmetry group isomorphic to the
two-dimensional Lorentz group SO(2,1). The careful further study of the
particle interaction requires a regularization that breaks the
scale invariance of the Hamilton operator. This shifts the breathing
frequency by about one percent, indicating a quantum anomaly.
Literatur:
L. P. Pitaevskii and A. Rosch,
"Breathing modes and hidden symmetry of trapped atoms
in two dimensions", Phys. Rev. A 55, R853 (1997);
M. Olshanii, H. Perrin and V. Lorent,
"Example of a Quantum Anomaly in the Physics of Ultracold Gases",
Phys. Rev. Lett. 105, 095302 (2010).
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Thu 10 Jan
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Sara Vitali
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Simple models of complex chaotic systems
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The study of nonlinear dynamics has blossomed in the past few
decades and it has
been developed and used extensively, with many different
applications.
In this talk the basic concepts of the theory of
nonlinear dynamical systems will be
presented, starting from the definition of an ordinary
differential equation/dynamical system and
the linearization about a fixed point, ending with the
definition of chaos.
Apart from the mathematical theory behind the topic,
I will also emphasize the
possibility of application of this theory through
different examples.
Literature:
Steven H. Strogratz, "Nonlinear dynamics and chaos",
Perseus (1985).
J. C. Sprott, "Simple models of complex chaotic systems",
Am. J. Phys. 76, 474 (2008)
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Thu 17 Jan
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S. Marzieh Hosseini
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Vacuum catastrophe and the cosmological constant problem
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According to Quantum field Theory (QFT), empty space is not really empty and contains zero-point fluctuations. This results in a large energy density for the vacuum which should have gravitational effects.
By using Quantum theory, I will discuss this issue for the electromagnetic field and also briefly for other fields.
In addition, one of the important manifestations of vacuum energy will be shown, the Casimir effect which demonstrates that the energy density of the vacuum is real.
At the end, by using classical gravitational theory and also observations, I will estimate an upper limit of the energy density in the Universe which is less than predicted from QFT by 120 orders of magnitude.
Literatur: Ronald J. Adler, Brenden Casey, and Ovid C. Jacob,
"Vacuume catastrophe: an elementary exposition of the cosmological constant problem",
American Journal of Physics, 63(7), 620-26 (1995).
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Thu 17 Jan
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Özgün Adebali
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Moon-induced Gaps in Planetary Rings
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The rings of Saturn were first observed in 1655. They are separated by
gaps the largest of which is called the Cassini Division. It is thought
they originate from the disintegration of moons of Saturn, perhaps by
scattering with comets or asteroids. In this talk, a non-linear diffusion
model for gaps in planetary rings is developed. By looking at the
gravitational scattering of the ring particles and an embedded moon, the
density profile around the moon is examined. The models are applied to the
gaps of the moons Pan and Daphnis which are located in the outer A ring of
Saturn.
Literatur: F. Grätz, M. Seiß & F. Spahn,
"Formation of Moon-induced Gaps in Dense Planetary Rings:
Application to the Rings of Saturn",
The Astrophysical Journal, 862(2), 157 (2018).
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The 24 Jan
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G. Mátyás Szabó
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Nonlinear Newtonian Gravity and Black Holes
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General relativity is a very important field for understanding how the universe works on a fundamental level. Simplified models (such as nonlinear Newtonian gravity) are often used in courses and textbooks to make it conceptually easier to grasp and less computationally intensive, even though they are ultimately flawed. The goal of this talk is to present an example of such a simplified model in action. Using a nonlinear version of Newtonian gravity that allows for black holes to exist, upper limits are derived on how much a black hole can be charged via bombardment by high- or low-energy charged particles. The result is then compared to the one obtained using general relativity, and the differences are reflected upon.
Literature: Michael R. R. Good, "On a nonlinear Newtonian gravity and charging a black hole",
Am. J. Phys. 86(6), 453-59 (2018).
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Thu 24 Jan
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Robin Schmidt
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Hyperbolic Meta-Materials and the Purcell Effect
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Nanofabricated Hyperbolic Media give rise to interesting new physics because of their unique way of interacting with light. For example, having a hyperbolic dispersion relation they offer an increased amount of decay channels compared to the vacuum for emitters in their immediate environment, effectively increasing its rate of emission. This effect is called the Purcell Effect.
In this lecture I will give an overview about the theory of metamaterials and their properties and applications. Also I will show how Fermi's Golden Rule can be used to understand how the engineering of the density of states can produce enhanced photon sources that emit in a highly directional fashion.
Literature:
Zubin Jacob, Igor I. Smolyaninov, Evgenii E. Narimanov,
"Broadband Purcell effect: Radiative decay engineering with
metamaterials", Appl. Phys. Lett. 100, 181105 (2012).
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Wed 30 Jan
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Mitali Damle
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Bell's Theorem and Causality
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The laws of Quantum Mechanics (QM) allow for correlations between particles that have no equivalent in the classical world. Experiments based on spatially separated particles seem to predict "spooky actions at a distance". Bell's theorem give a precise limit between predictions from a Classical Mechanics and that from QM, stating that "The predictions of QM cannot be reproduced by any locally causal realistic description". The assumption that causality and QM hold both true simultaneously leads to contradictions with Relativity. An attempt is made to relieve the tension between QM, causality and Relativity by considering the implications of a retro-causal toy model, which appears to violate causality in the "past", rather than "at a distance".
Literature:
N. Argaman, "Bell's theorem and the causal arrow of time,"
Am. J. Phys. 78, 1007-13 (2010).
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Thu 31 Jan
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Georg Filatow
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Bronstein's Quantisation of weak gravitational Fields
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Die Physik kann man in verschiedene Gebiete aufteilen, darin ist die Gravitation eine
der vier Wechselwirkungen, die sich mit der Anziehung zwischen Massen beschäftigt.
Durch das Quantisieren wurde aus der klassischen Physik die Quantenphysik, mit
deren Hilfe verschiedene Effekte korrekt beschrieben oder vorhergesagt werden können
(Energieniveaus von Atomen, Welle-Teilchen-Dualismus). Eine Verbindung zwischen
Quantenphysik und Gravitationstheorie ist erstrebenswert, aber bislang noch Gegenstand
der Forschung.
M. Bronstein hat bereits im Jahr 1936 die Einstein'sche Gravitationstheorie für schwache
Felder quantisiert. Im Vortrag diskutieren wir ein paar Formeln und stellen ein Gedankenexperiment
vor, das sich mit der Messung von Gravitationsfeldern beschäftigt. Zum Schluss bringen wir
eine "Quanten-Herleitung" des Newtonschen Gravitationsgesetzes.
Matvei Bronstein, "Quantentheorie Schwacher Gravitationsfelder",
Physikalische Zeitschrift d. Sowjetunion 9, 140-57 (1936)
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