The ninth data release of the Sloan Digital Sky Survey: first spectroscopic data from the SDSS-III Baryon Oscillation Spectroscopic Survey

CP Ahn, R Alexandroff, CA Prieto… - The Astrophysical …, 2012 - iopscience.iop.org
ABSTRACT The Sloan Digital Sky Survey III (SDSS-III) presents the first spectroscopic data
from the Baryon Oscillation Spectroscopic Survey (BOSS). This ninth data release (DR9) of …

[HTML][HTML] General relativity and cosmology: Unsolved questions and future directions

I Debono, GF Smoot - Universe, 2016 - mdpi.com
For the last 100 years, General Relativity (GR) has taken over the gravitational theory mantle
held by Newtonian Gravity for the previous 200 years. This article reviews the status of GR in …

Constraints on local primordial non-Gaussianity from large scale structure

A Slosar, C Hirata, U Seljak, S Ho… - Journal of Cosmology …, 2008 - iopscience.iop.org
Recent work has shown that the local non-Gaussianity parameter f NL induces a scale
dependent bias, whose amplitude is growing with scale. Here we first rederive this result …

Statistical analysis of galaxy surveys–I. Robust error estimation for two-point clustering statistics

P Norberg, CM Baugh, E Gaztanaga… - Monthly Notices of the …, 2009 - academic.oup.com
We present a test of different error estimators for two-point clustering statistics, appropriate
for present and future large galaxy redshift surveys. Using an ensemble of very large dark …

Resumming cosmological perturbations via the Lagrangian picture: One-loop results in real space and in redshift space

T Matsubara - Physical Review D, 2008 - APS
We develop a new approach to study the nonlinear evolution in the large-scale structure of
the Universe both in real space and in redshift space, extending the standard perturbation …

Non-linear evolution of cosmological structures in warm dark matter models

A Schneider, RE Smith, AV Maccio… - Monthly Notices of the …, 2012 - academic.oup.com
The dark energy dominated warm dark matter (WDM) model is a promising alternative
cosmological scenario. We explore large-scale structure formation in this paradigm. We do …

First results from the XENON10 dark matter experiment at the Gran Sasso National Laboratory

J Angle, E Aprile, F Arneodo, L Baudis… - arXiv preprint arXiv …, 2007 - arxiv.org
The XENON10 experiment at the Gran Sasso National Laboratory uses a 15 kg xenon dual
phase time projection chamber (XeTPC) to search for dark matter weakly interacting …

Theoretical models of dark energy

J Yoo, Y Watanabe - International Journal of Modern Physics D, 2012 - World Scientific
Mounting observational data confirm that about 73% of the energy density consists of dark
energy which is responsible for the current accelerated expansion of the Universe. We …

Mirror dark matter: Cosmology, galaxy structure and direct detection

R Foot - International Journal of Modern Physics A, 2014 - World Scientific
A simple way to accommodate dark matter is to postulate the existence of a hidden sector.
That is, a set of new particles and forces interacting with the known particles predominantly …

Nonlocal cosmology

S Deser, RP Woodard - Physical Review Letters, 2007 - APS
We explore nonlocally modified models of gravity, inspired by quantum loop corrections, as
a mechanism for explaining current cosmic acceleration. These theories enjoy two major …