Built on

A. Zucca, L. Pogosian, A. Silvestri and G.-B. Zhao, MGCAMB with massive neutrinos and dynamical dark energy , JCAP 05
Original
1901
Earlier work this paper cites.
F. Gerardi, M. Martinelli and A. Silvestri, Reconstruction of the Dark Energy equation of state from latest data: the impact of theoretical priors , JCAP 07
Original
1902
Earlier work this paper cites.
M. Ishak et al., Modified Gravity and Dark Energy models Beyond w ⁡ ( z ) w(z) CDM Testable by LSST , 1905.09687
Original
1905
Earlier work this paper cites.
Supernova Search Team
1998
Earlier work this paper cites.
Supernova Cosmology Project
1999
Earlier work this paper cites.
M. Chevallier and D. Polarski, Accelerating universes with scaling dark matter , Int. J. Mod. Phys. D 10
2001
Earlier work this paper cites.
A. Lewis and S. Bridle, Cosmological parameters from CMB and other data: a Monte- Carlo approach , Phys. Rev. D66
2002
Earlier work this paper cites.
E.V. Linder, Exploring the expansion history of the universe , Phys. Rev. Lett. 90
Original
2003
Earlier work this paper cites.
G.-B. Zhao et al., The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: a multi-tracer analysis in Fourier space for measuring the cosmic structure growth and expansion rate , 2007.09011
Original
2007
Earlier work this paper cites.
Y. Wang et al., The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR16 luminous red galaxy and emission line galaxy samples: cosmic distance and structure growth measurements using multiple tracers in configuration space , 2007.09010
Original
2007
Earlier work this paper cites.
J. Hou et al., The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the Quasar Sample in configuration space between redshift 0.8 and 2.2 , Mon. Not. Roy. Astron. Soc. 500
Original
2007
Earlier work this paper cites.
H. du Mas des Bourboux et al., The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Baryon acoustic oscillations with Lyman- α \alpha forests , 2007.08995
Original
2007
Earlier work this paper cites.
J.E. Bautista et al., The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic correlation function between redshifts 0.6 and 1 , Mon. Not. Roy. Astron. Soc. 500
Original
2007
Earlier work this paper cites.
A. de Mattia et al., The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum between redshift 0.6 and 1.1 , Mon. Not. Roy. Astron. Soc. 501
Original
2007
Earlier work this paper cites.
R. Neveux et al., The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from the anisotropic power spectrum of the quasar sample between redshift 0.8 and 2.2 , Mon. Not. Roy. Astron. Soc. 499
Original
2007
Earlier work this paper cites.
L. Amendola, M. Kunz and D. Sapone, Measuring the dark side (with weak lensing) , JCAP 0804
Original
2008
Earlier work this paper cites.
E. Bertschinger and P. Zukin, Distinguishing Modified Gravity from Dark Energy , Phys. Rev. D78
Original
2008
Earlier work this paper cites.
A. Silvestri and M. Trodden, Approaches to Understanding Cosmic Acceleration , Rept. Prog. Phys. 72
Original
2009
Earlier work this paper cites.

Similar

G.-B. Zhao, L. Pogosian, A. Silvestri and J. Zylberberg, Searching for modified growth patterns with tomographic surveys , Phys. Rev. D79
Original
2009
Cited alongside, same era.
R.G. Crittenden, L. Pogosian and G.-B. Zhao, Investigating dark energy experiments with principal components , JCAP 0912
2009
Cited alongside, same era.
L. Pogosian, A. Silvestri, K. Koyama and G.-B. Zhao, How to optimally parametrize deviations from General Relativity in the evolution of cosmological perturbations? , Phys. Rev. D81
Original
2010
Cited alongside, same era.
C. Garcia-Quintero, M. Ishak and O. Ning, Current constraints on deviations from General Relativity using binning in redshift and scale , JCAP 12
Original
2010
Cited alongside, same era.
A. Hojjati, L. Pogosian and G.-B. Zhao, Testing gravity with CAMB and CosmoMC , JCAP 1108

Then

L. Amendola, M. Kunz, M. Motta, I.D. Saltas and I. Sawicki, Observables and unobservables in dark energy cosmologies , Phys. Rev. D 87
Original
2013
Later among the works it cites.
Euclid Theory Working Group
Original
2013
Later among the works it cites.
E. Bellini and I. Sawicki, Maximal freedom at minimum cost: linear large-scale structure in general modifications of gravity , JCAP 1407
Original
2014
Later among the works it cites.
B. Hu, M. Raveri, N. Frusciante and A. Silvestri, Effective Field Theory of Cosmic Acceleration: an implementation in CAMB , Phys. Rev. D89
Original
2014
Later among the works it cites.
M. Raveri, B. Hu, N. Frusciante and A. Silvestri, Effective Field Theory of Cosmic Acceleration: constraining dark energy with CMB data , Phys. Rev. D90

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

Reading the bibliography…

2021

Principal reconstructed modes of dark energy and gravity

Raveri, Marco, Pogosian, Levon, Martinelli, Matteo et al.

Understand

Recently, in [1], we presented the first combined non-parametric reconstruction of the three time-dependent functions that capture departures from the standard cosmological model, $\Lambda$CDM, in the expansion history and gravitational effects on matter and light from the currently available combination of the background and large scale structure data.

The reconstruction was performed with and without a theory-informed prior, built on the general Horndeski class of scalar-tensor theories, that correlates the three functions.
In this work, we perform a decomposition of the prior and posterior covariances of the three functions to determine the structure of the modes that are constrained by the data relative to the Horndeski prior.
We find that the combination of all data can constrain 15 combined eigenmodes of the three functions with respect to the prior.