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The observed galaxy bispectrum from single-field inflation in the squeezed limit
(IOP Publishing, 2018)
Using the consistency relation in Fourier space, we derive the observed galaxy bispectrum from
single- eld in
ation in the squeezed limit, in which one of the three modes has a wavelength much
longer than the other two. ...
Clustering of quintessence on horizon scales and its imprint on HI intensity mapping
(IOP Science, 2013)
Quintessence can cluster only on horizon scales. What is the effect on the observed matter distribution? To answer this, we need a relativistic approach that goes beyond the standard Newtonian
calculation and deals properly ...
Testing gravity using large-scale redshift-space distortions
(Oxford University Press, 2013)
We use luminous red galaxies from the Sloan Digital Sky Survey (SDSS) II to test
the cosmological structure growth in two alternatives to the standard cold dark matter
( CDM)+general relativity (GR) cosmological model. ...
Matter bispectrum in cubic Galileon cosmologies
(IOP Science, 2013)
In this paper we obtain the bispectrum of dark matter density perturbations in
the frame of covariant cubic Galileon theories. This result is obtained by means of a semi-
analytic approach to second-order perturbations ...
Probing the imprint of interacting dark energy on very large scales
(American Physical Society, 2015)
The observed galaxy power spectrum acquires relativistic corrections from light-cone effects, and these corrections grow on very large scales. Future galaxy surveys in optical, infrared and radio bands will probe increasingly ...
Cosmology on the largest scales with the SKA
(Proceedings of Science, 2014)
The study of the Universe on ultra-large scales is one of the major science cases for the Square
Kilometre Array (SKA). The SKA will be able to probe a vast volume of the cosmos, thus representing
a unique instrument, ...