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20022014
most citedCosmological Constraints from the SDSS Luminous Red Galaxies

1.4k citations

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45 papers · 1 filter

gr-qc20066 cited

The evolution of tensor perturbations in scalar-tensor theories of gravity

Sante Carloni, Peter K. S. Dunsby

The evolution equations for tensor perturbations in a generic scalar tensor theory of gravity are presented. Exact solution are given for a specific class of theories and Friedmann…

astro-ph200630 cited

HST and Optical Observations of Three Pulsating Accreting White Dwarfs in Cataclysmic Variables

Paula Szkody, Anjum Mukadam, Boris T. Gaensicke +8

Ultraviolet observations using the Solar Blind Channel on the Hubble Space Telescope provide light curves and low resolution spectra of three pulsating white dwarfs in the cataclys…

gr-qc2006695 cited

The cosmological gravitational wave background from primordial density perturbations

Kishore N. Ananda, Chris Clarkson, David Wands

We discuss the gravitational wave background generated by primordial density perturbations evolving during the radiation era. At second-order in a perturbative expansion, density f…

gr-qc200630 cited

A dynamical system approach to higher order gravity

Sante Carloni, Peter K. S. Dunsby

The dynamical system approach has recently acquired great importance in the investigation on higher order theories of gravity. In this talk I review the main results and I give bri…

gr-qc200624 cited

Gauge invariant perturbations of Scalar-Tensor Cosmologies: The vacuum case

Sante Carloni, Peter K. S. Dunsby, Claudio Rubano

The covariant gauge invariant perturbation theory of scalar cosmological perturbations is developed for a general Scalar-Tensor Friedmann-Lemaitre-Robertson-Walker cosmology in a v…

gr-qc20061 cited

Group classification of the Sachs equations for a radiating axisymmetric, non-rotating, vacuum space-time

Nail H. Ibragimov, Ewald J. H. Wessels, George F. R. Ellis

We carry out a Lie group analysis of the Sachs equations for a time-dependent axisymmetric non-rotating space-time in which the Ricci tensor vanishes. These equations, which are th…