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We consider cosmological models in which dark matter feels a fifth force mediated by the dark energy scalar field, also known as coupled dark energy.
An evolution free test for non-zero cosmological constant
Charles Alcock and Bohdan Paczyński · 1979
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Power Law Inflation
F. Lucchin and S. Matarrese · 1985
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Clustering in real space and in redshift space
Nick Kaiser · 1987
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Cosmology and the Fate of Dilatation Symmetry
C. Wetterich · 1988
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Power Spectrum Analysis of Three-Dimensional Redshift Surveys
Hume A. Feldman, Nick Kaiser, and John A. Peacock · 1994
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The Cosmon model for an asymptotically vanishing time dependent cosmological ’constant’
Christof Wetterich · 1995
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Measuring the galaxy power spectrum with future redshift surveys
Max Tegmark, Andrew Hamilton, Michael Strauss, Michael Vogeley, and Alexander Szalay · 1998
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Galaxy clustering determined from numerical cosmological simulations
Adrian Jenkins, C. S. Frenk, F. R. Pearce, P. A. Thomas, J. M. Colberg, S. D. M. White, H. M. P. Couchman, J. A. Peacock, G. Efstathiou, and A. H. Nelson · 1999
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Coupled quintessence
Luca Amendola · 2000
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Efficient Computation of CMB anisotropies in closed FRW models
Antony Lewis, Anthony Challinor, and Anthony Lasenby · 2000
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Stable clustering, the halo model and non-linear cosmological power spectra
R. E. Smith, J. A. Peacock, A. Jenkins, S. D. M. White, C. S. Frenk, F. R. Pearce, P. A. Thomas, G. Efstathiou, and H. M. P. Couchman · 2003
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A test of general relativity using radio links with the Cassini spacecraft
B. Bertotti, L. Iess, and P. Tortora · 2003
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Linear and non-linear perturbations in dark energy models
Luca Amendola · 2004
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Coupled dark energy: Parameter constraints from N-body simulations
A.V. Maccio, C. Quercellini, R. Mainini, L. Amendola, and S.A. Bonometto · 2004
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Skewness as a test of the equivalence principle
Luca Amendola and Claudia Quercellini · 2004
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N-body simulations for coupled dark energy: halo mass function and density profiles
Andrea V. Macciò, Claudia Quercellini, Roberto Mainini, Luca Amendola, and Silvio A. Bonometto · 2004
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Redshift-space distortions, pairwise velocities, and nonlinearities
Román Scoccimarro · 2004
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The Confrontation between general relativity and experiment
Clifford M. Will · 2005
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The cosmological simulation code GADGET-2
Volker Springel · 2005
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Baryonic acoustic oscillations in simulated galaxy redshift surveys
Hee-Jong Seo and Daniel J. Eisenstein · 2005
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Mass functions in coupled Dark Energy models
Roberto Mainini and Silvio Bonometto · 2006
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Probing dark energy with the shear-ratio geometric test
A. N. Taylor, T. D. Kitching, D. J. Bacon, and A. F. Heavens · 2006
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Improved forecasts for the baryon acoustic oscillations and cosmological distance scale
Hee-Jong Seo and Daniel J. Eisenstein · 2007
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Flowing with Time: a New Approach to Nonlinear Cosmological Perturbations
Massimo Pietroni · 2008
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Coupled and Extended Quintessence: theoretical differences and structure formation
Valeria Pettorino and Carlo Baccigalupi · 2008
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Concentration, spin and shape of dark matter haloes as a function of the cosmological model: WMAP
Andrea V. Macciò, Aaron A. Dutton, and Frank C. van den Bosch · 2008
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An ideal mass assignment scheme for measuring the Power Spectrum with FFTs
Weiguang Cui, Lei Liu, Xiaohu Yang, Yu Wang, Longlong Feng, and Volker Springel · 2008
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Accurate estimators of power spectra in N
Stéphane Colombi, Andrew Jaffe, Dmitri Novikov, and Christophe Pichon · 2008
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Nonlinear structure formation and the acoustic scale
Hee-Jong Seo, Ethan R. Siegel, Daniel J. Eisenstein, and Martin White · 2008
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Hydrodynamical N-body simulations of coupled dark energy cosmologies
Marco Baldi, V. Pettorino, G. Robbers, and V. Springel · 2009
Cited alongside, same era.
Constraint on coupled dark energy models from observations
Jun-Qing Xia · 2009
Cited alongside, same era.
Non-linear power spectrum including massive neutrinos: the time-RG flow approach
The codecs project: a publicly available suite of cosmological N-body simulations for interacting dark energy models
Marco Baldi · 2012
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The halo mass function in interacting Dark Energy models
Weiguang Cui, Marco Baldi, and Stefano Borgani · 2012
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Dark Energy Simulations
Marco Baldi · 2012
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Constraints on coupled dark energy using CMB data from WMAP and SPT
Valeria Pettorino, Luca Amendola, Carlo Baccigalupi, and Claudia Quercellini · 2012
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Cosmological non-linearities as an effective fluid
Daniel Baumann, Alberto Nicolis, Leonardo Senatore, and Matias Zaldarriaga · 2012
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Julien Lesgourgues, Sabino Matarrese, Massimo Pietroni, and Antonio Riotto · 2009
Cited alongside, same era.
The Coyote Universe. I. Precision determination of the nonlinear matter power spectrum
Katrin Heitmann, Martin White, Christian Wagner, Salman Habib, and David Higdon · 2010
Cited alongside, same era.
The coyote universe. III. simulation suite and precision emulator for the nonlinear matter power spectrum
Earl Lawrence, Katrin Heitmann, Martin White, David Higdon, Christian Wagner, Salman Habib, and Brian Williams · 2010
Cited alongside, same era.
Cosmological Non-Linearities as an Effective Fluid
Daniel Baumann, Alberto Nicolis, Leonardo Senatore, and Matias Zaldarriaga · 2010
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Clarifying spherical collapse in coupled dark energy cosmologies
Nico Wintergerst and Valeria Pettorino · 2010
Cited alongside, same era.
Time-dependent couplings in the dark sector: from background evolution to non-linear structure formation
Marco Baldi · 2010
Cited alongside, same era.
Spherical collapse model in dark energy cosmologies
F. Pace, J. C. Waizmann, and M. Bartelmann · 2010
Cited alongside, same era.
Sylvain de la Torre and Luigi Guzzo · 2012
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Toward More Realistic Forecasting of Dark Energy Constraints from Galaxy Redshift Surveys
Yun Wang, Chia-Hsun Chuang, and Christopher M. Hirata · 2012
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Neutrino masses and cosmological parameters from a Euclid-like survey: Markov Chain Monte Carlo forecasts including theoretical errors
Benjamin Audren, Julien Lesgourgues, Simeon Bird, Martin G Haehnelt, and Matteo Viel · 2013
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Testing modified gravity with Planck: the case of coupled dark energy
Valeria Pettorino · 2013
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The Coyote Universe Extended: Precision Emulation of the Matter Power Spectrum
Katrin Heitmann, Earl Lawrence, Juliana Kwan, Salman Habib, and David Higdon · 2014
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Shankar Agarwal, Filipe B. Abdalla, Hume A. Feldman, Ofer Lahav, and Shaun A. Thomas · 2014
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Cosmological Leverage from the Matter Power Spectrum in the Presence of Baryon and Nonlinear Effects
Jannis Bielefeld, Dragan Huterer, and Eric V. Linder · 2014
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Analytic model for the matter power spectrum, its covariance matrix, and baryonic effects
Irshad Mohammed and Uros Seljak · 2014
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Edoardo Carlesi, Alexander Knebe, Geraint F. Lewis, Scott Wales, and Gustavo Yepes · 2014
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On the observability of coupled dark energy with cosmic voids
P. M. Sutter, Edoardo Carlesi, Benjamin D. Wandelt, and Alexander Knebe · 2014
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Paolo Creminelli, Jérôme Gleyzes, Lam Hui, Marko Simonović, and Filippo Vernizzi · 2014
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Cosmic microwave background constraints on coupled dark matter
Sophie C. F. Morris and Anne M. Green · 2014
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Review of Particle Physics
K. A. Olive et al · 2014
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Hydrodynamical simulations of coupled and uncoupled quintessence models - I. Halo properties and the cosmic web
E. Carlesi, A. Knebe, G. F. Lewis, S. Wales, and G. Yepes · 2014
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Alessandro Manzotti, Marco Peloso, Massimo Pietroni, Matteo Viel, and Francisco Villaescusa-Navarro · 2014
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Breaking the spell of Gaussianity: forecasting with higher order Fisher matrices
Elena Sellentin, Miguel Quartin, and Luca Amendola · 2014
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Effects of Coupled Dark Energy on the Milky Way and its Satellites
C. Penzo, A. V. Macciò, M. Baldi, L. Casarini, and J. Oñorbe · 2015
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Planck 2015 results. XIV. Dark energy and modified gravity
Planck Collaboration · 2015
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Atom-interferometry constraints on dark energy
Paul Hamilton, Matt Jaffe, Philipp Haslinger, Quinn Simmons, Holger Müller, and Justin Khoury · 2015
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Atom-interferometry constraints on dark energy
P. Hamilton, M. Jaffe, P. Haslinger, Q. Simmons, H. Müller, and J. Khoury · 2015
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Planck 2015 results. XIII. Cosmological parameters
P.A.R. Ade et al · 2015
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