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Observational probes of cosmic acceleration

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TLDR
In this article, the authors present extensive forecasts for constraints on the dark energy equation of state and parameterized deviations from General Relativity, achievable with Stage III and Stage IV experimental programs that incorporate supernovae, BAO, weak lensing, and cosmic microwave background data.
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This article is published in Physics Reports.The article was published on 2013-09-10 and is currently open access. It has received 1253 citations till now. The article focuses on the topics: Dark energy & Lambda-CDM model.

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Model-independent Curvature Determination from Gravitational-Wave Standard Sirens and Cosmic Chronometers

TL;DR: In this paper, the spatial curvature of a GW source is estimated in a model-independent way by comparing the distances from future GW sources and current cosmic-chronometer observations.
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Nonlinear spherical perturbations in Quintessence Models of Dark Energy

TL;DR: In this article, the response of quintessence dark energy to non-linear perturbations in dark matter is studied. And the authors find that dark energy perturbation remains localised and does not diffuse out to larger scales.
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Reconstruction with velocities

TL;DR: Zhu et al. as mentioned in this paper used radial velocities measured from the cosmic microwave background observation through the kinematic Sunyaev-Zeldovich effect to improve performance near the boundary.
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Searching for the Evidence of Dynamical Dark Energy

TL;DR: In this paper, the authors search for the evidence of dynamical dark energy (DDE) using the "Joint Light-curve Analysis" (JLA) Type Ia supernovae (SNe Ia) sample, the 30 latest cosmic chronometer data points (H(z)), Planck's shift parameter from cosmic microwave background (CMB) anisotropies, the 156 latest HII galaxy measurements and 79 calibrated gamma-ray bursts (GRBs).
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Cosmology of viscous holographic f(G) gravity and consequences in the framework of quintessence scalar field

TL;DR: In this paper, the reconstruction schemes for the f(G) gravity in the framework of bulk viscosity and holographic background evolution by considering the universe filled b... are presented.
References
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The relationship between infrared, optical, and ultraviolet extinction

TL;DR: In this article, the average extinction law over the 3.5 micron to 0.125 wavelength range was derived for both diffuse and dense regions of the interstellar medium. And the validity of the law over a large wavelength interval suggests that the processes which modify the sizes and compositions of grains are stochastic in nature.
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