243 research outputs found
The Dyer-Roeder distance-redshift relation in inhomogeneous universes
Using Monte-Carlo methods, we determine the best-fit value of the homogeneity
parameter alpha in the Dyer-Roeder distance-redshift relation for a variety of
redshifts, inhomogeneity models and cosmological parameter values. The relation
between alpha and the fraction of compact objects, f_p, is found to be
approximately linear. This relation can be parametrized with reasonable
accuracy for all cases treated in this paper by alpha = a*f_p, where a = 0.6.Comment: 5 pages, 10 figures, submitted to Phys.Rev.
Impact of symmetron screening on the Hubble tension: new constraints using cosmic distance ladder data
Fifth forces are ubiquitous in modified theories of gravity. To be compatible
with observations, such a force must be screened on solar-system scales but may
still give a significant contribution on galactic scales. If this is the case,
the fifth force can influence the calibration of the cosmic distance ladder,
hence changing the inferred value of the Hubble constant . In this paper,
we analyze symmetron screening and show that it generally increases the Hubble
tension. On the other hand, by doing a full statistical analysis, we show that
cosmic distance ladder data are able to constrain the theory to a level
competitive with solar-system tests -- currently the most constraining tests of
the theory. For the standard coupling case, the constraint on the symmetron
Compton wavelength is . Thus,
distance ladder data constitutes a novel and powerful way of testing this, and
similar, types of theories.Comment: 11 pages, 9 figures. Comments are welcom
Probing a scale dependent gravitational slip with galaxy strong lensing systems
Observations of galaxy-scale strong gravitational lensing systems enable
unique tests of departures from general relativity at the kpc-Mpc scale. In
this work, the gravitational slip parameter , measuring the
amplitude of a hypothetical fifth force, is constrained using 130 elliptical
galaxy lens systems. We implement a lens model with a power-law total mass
density and a deprojected De Vaucouleurs luminosity density, favored over a
power-law luminosity density. To break the degeneracy between the lens velocity
anisotropy, , and the gravitational slip, we introduce a new prior on
the velocity anisotropy based on recent dynamical data. For a constant
gravitational slip, we find in agreement
with general relativity at the 68\% confidence level. Introducing a Compton
wavelength , effectively screening the fifth force at small and
large scales, the best fit is obtained for Mpc and
. A local minimum is found at
Mpc and . We conclude
that there is no evidence in the data for a significant departure from general
relativity and that using accurate assumptions and having good constraints on
the lens galaxy model is key to ensure reliable constraints on the
gravitational slip.Comment: 12 pages, 5 figure
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