38 research outputs found
A gauge theoretic approach to elasticity with microrotations
We formulate elasticity theory with microrotations using the framework of
gauge theories, which has been developed and successfully applied in various
areas of gravitation and cosmology. Following this approach, we demonstrate the
existence of particle-like solutions. Mathematically this is due to the fact
that our equations of motion are of Sine-Gordon type and thus have soliton type
solutions. Similar to Skyrmions and Kinks in classical field theory, we can
show explicitly that these solutions have a topological origin.Comment: 15 pages, 1 figure; revised and extended version, one extra page;
revised and extended versio
Observational Constraints on Teleparallel Dark Energy
We use data from Type Ia Supernovae (SNIa), Baryon Acoustic Oscillations
(BAO), and Cosmic Microwave Background (CMB) observations to constrain the
recently proposed teleparallel dark energy scenario based on the teleparallel
equivalent of General Relativity, in which one adds a canonical scalar field,
allowing also for a nonminimal coupling with gravity. Using the power-law, the
exponential and the inverse hyperbolic cosine potential ansatzes, we show that
the scenario is compatible with observations. In particular, the data favor a
nonminimal coupling, and although the scalar field is canonical the model can
describe both the quintessence and phantom regimes.Comment: 19 pages, 6 figures, version accepted by JCA
Phase-Space analysis of Teleparallel Dark Energy
We perform a detailed dynamical analysis of the teleparallel dark energy
scenario, which is based on the teleparallel equivalent of General Relativity,
in which one adds a canonical scalar field, allowing also for a nonminimal
coupling with gravity. We find that the universe can result in the
quintessence-like, dark-energy-dominated solution, or to the stiff dark-energy
late-time attractor, similarly to standard quintessence. However, teleparallel
dark energy possesses an additional late-time solution, in which dark energy
behaves like a cosmological constant, independently of the specific values of
the model parameters. Finally, during the evolution the dark energy
equation-of-state parameter can be either above or below -1, offering a good
description for its observed dynamical behavior and its stabilization close to
the cosmological-constant value.Comment: 23 pages, 4 figures, 5 tables, version published at JCA
Disseminated mucormycosis of an immunocompromised multiple myeloma patient: impact of biopsy of extramedullary tumours in refractory multiple myeloma
Maximal symmetry and metric-affine f(R) gravity
The affine connection in a space-time with a maximally symmetric spatial
subspace is derived using the properties of maximally symmetric tensors. The
number of degrees of freedom in metric-affine gravity is thereby considerably
reduced while the theory allows spatio-temporal torsion and remains non-metric.
The Ricci tensor and scalar are calculated in terms of the connection and the
field equations derived for the Einstein-Hilbert as wells as for f(R)
Lagrangians. By considering specific forms of f(R), we demonstrate that the
resulting Friedmann equations in Palatini formalism without torsion and
metric-affine formalism with maximal symmetry are in general different in the
presence of matter.Comment: 7 page
Existence of relativistic stars in f(T) gravity
We examine the existence of relativistic stars in f(T) modified gravity and
explicitly construct several classes of static perfect fluid solutions. We
derive the conservation equation from the complete f(T) gravity field equations
and present the differences with its teleparallel counterpart. Firstly, we
choose the tetrad field in the diagonal gauge and study the resulting field
equations. Some exact solutions are explicitly constructed and it is noted that
these solutions have to give a constant torsion scalar. Next, we choose a non
diagonal tetrad field which results in field equations similar to those of
general relativity. For specific models we are able to construct exact
solutions of these field equations. Among those new classes of solutions, we
find negative pressure solutions, and an interesting class of polynomial
solutions.Comment: 19 pages; substantially revised and extended version, off diagonal
tetrad discussion adde
Varying constants, Gravitation and Cosmology
Fundamental constants are a cornerstone of our physical laws. Any constant
varying in space and/or time would reflect the existence of an almost massless
field that couples to matter. This will induce a violation of the universality
of free fall. It is thus of utmost importance for our understanding of gravity
and of the domain of validity of general relativity to test for their
constancy. We thus detail the relations between the constants, the tests of the
local position invariance and of the universality of free fall. We then review
the main experimental and observational constraints that have been obtained
from atomic clocks, the Oklo phenomenon, Solar system observations, meteorites
dating, quasar absorption spectra, stellar physics, pulsar timing, the cosmic
microwave background and big bang nucleosynthesis. At each step we describe the
basics of each system, its dependence with respect to the constants, the known
systematic effects and the most recent constraints that have been obtained. We
then describe the main theoretical frameworks in which the low-energy constants
may actually be varying and we focus on the unification mechanisms and the
relations between the variation of different constants. To finish, we discuss
the more speculative possibility of understanding their numerical values and
the apparent fine-tuning that they confront us with.Comment: 145 pages, 10 figures, Review for Living Reviews in Relativit
Schnelleres Aufwachenverhalten bei Frauen im Vergleich zu Männern nach EEG geführter Propofolsedierung im Rahmen der Koloskopie Erste prospektive Beobachtungstudie zu geschlechtsspezifischen Unterschieden zu Propofoldosis und Aufwachzeit
Hippocampal cannabinoid-1 receptor upregulation upon endothelin-B receptor deficiency: A neuroprotective substitution effect ?
Endothelin (ETB)-receptors mediate anti-apoptotic actions. Lack of functional ETB-receptors leads to increased neuronal apoptosis in the hippocampus. The increased apoptosis must be compensated by other mechanisms, however, as ETB-deficient rats display normal overall brain morphology. To illuminate on brain plasticity in ETB-receptor deficiency, we studied the expression and function of another neuroprotective system, the cannabinoid CB1-receptors, in ETB-deficient hippocampus. We show that CB1 expression in hippocampus increases postnatally in all rats but that the increase in CB1-receptor expression is significantly higher in ETB-deficient compared to wildtype littermates. Neuronal apoptosis decreases during brain maturation but remains on a significantly higher level in the ETB-deficient compared to wildtype dentate. When investigating survival of hippocampal neurons in culture, we found significant protection against hypoxia-induced cell death with CB1-analogs (noladin, (9-tetrahydrocannabinol) only in ETB-deficient neurons. We suggest that CB1-receptor upregulation in the ETB-mutant hippocampus reflects an attempt to compensate for the lack of ETB-receptors
