Built on

A. Spurio Mancini, F. Köhlinger, B. Joachimi, V. Pettorino, B. M. Schäfer, R. Reischke, E. van Uitert, S. Brieden, M. Archidiacono, and J. Lesgourgues, KiDS + GAMA: constraints on horndeski gravity from combined large-scale structure probes
Original
1901
Earlier work this paper cites.
K. Markovic, B. Bose, and A. Pourtsidou, Assessing non-linear models for galaxy clustering I: unbiased growth forecasts from multipole expansion
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1904
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N. E. Chisari et al
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1905
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B. Bose, A. Pourtsidou, K. Markovič, and F. Beutler, Assessing non-linear models for galaxy clustering II: model validation and forecasts for Stage IV surveys
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1905
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L. Verde, T. Treu, and A. G. Riess, Tensions between the Early and the Late Universe
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1907
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F. N. Chamings, A. Avgoustidis, E. J. Copeland, A. M. Green, and A. Pourtsidou, Understanding the suppression of structure formation from dark matter-dark energy momentum coupling
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1912
Earlier work this paper cites.
E. J. Copeland, M. Sami, and S. Tsujikawa, Dynamics of dark energy
1936
Earlier work this paper cites.
L. Guzzo et al
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1944
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B. Jain and E. Bertschinger, Second-Order Power Spectrum and Nonlinear Evolution at High Redshift
1994
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R. R. Caldwell, R. Dave, and P. J. Steinhardt, Cosmological imprint of an energy component with general equation of state
1998
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D. J. Eisenstein and W. Hu, Baryonic features in the matter transfer function
1998
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R. Scoccimarro, H. M. P. Couchman, and J. A. Frieman, The Bispectrum as a Signature of Gravitational Instability in Redshift Space
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L. Amendola, Coupled quintessence
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E. Jones, T. Oliphant, P. Peterson, et al
2001
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F. Bernardeau, S. Colombi, E. Gaztanaga, and R. Scoccimarro, Large scale structure of the universe and cosmological perturbation theory
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P. J. E. Peebles and B. Ratra, The Cosmological Constant and Dark Energy
2003
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T. Nishimichi, G. D’Amico, M. M. Ivanov, L. Senatore, M. Simonović, M. Takada, M. Zaldarriaga, and P. Zhang, Blinded challenge for precision cosmology with large-scale structure: results from effective field theory for the redshift-space galaxy power spectrum
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2003
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A. Gómez-Valent, V. Pettorino, and L. Amendola, Update on coupled dark energy and the H 0 H_{0} tension
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2004
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A. Chudaykin, M. M. Ivanov, O. H. E. Philcox, and M. Simonović, Nonlinear perturbation theory extension of the Boltzmann code CLASS
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S. Nojiri and S. D. Odintsov, Introduction to modified gravity and gravitational alternative for dark energy
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A. Eggemeier, R. Scoccimarro, M. Crocce, A. Pezzotta, and A. G. Sánchez, Testing one-loop galaxy bias: Power spectrum
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2021

Interacting dark energy from redshift-space galaxy clustering

Carrilho, Pedro, Moretti, Chiara, Bose, Benjamin et al.

Understand

Interacting dark energy models have been proposed as attractive alternatives to $\Lambda$CDM.

Forthcoming Stage-IV galaxy clustering surveys will constrain these models, but they require accurate modelling of the galaxy power spectrum multipoles on mildly non-linear scales.
In this work we consider a dark scattering model with a simple 1-parameter extension to $w$CDM - adding only $A$, which describes a pure momentum exchange between dark energy and dark matter.
We then provide a comprehensive comparison of three approaches of modeling non-linearities, while including the effects of this dark sector coupling.

Built on

A. Spurio Mancini, F. Köhlinger, B. Joachimi, V. Pettorino, B. M. Schäfer, R. Reischke, E. van Uitert, S. Brieden, M. Archidiacono, and J. Lesgourgues, KiDS + GAMA: constraints on horndeski gravity from combined large-scale structure probes
Original
1901
Earlier work this paper cites.
K. Markovic, B. Bose, and A. Pourtsidou, Assessing non-linear models for galaxy clustering I: unbiased growth forecasts from multipole expansion
Original
1904
Earlier work this paper cites.
N. E. Chisari et al
Original
1905
Earlier work this paper cites.
B. Bose, A. Pourtsidou, K. Markovič, and F. Beutler, Assessing non-linear models for galaxy clustering II: model validation and forecasts for Stage IV surveys
Original
1905
Earlier work this paper cites.
L. Verde, T. Treu, and A. G. Riess, Tensions between the Early and the Late Universe
Original
1907
Earlier work this paper cites.
L. Knox and M. Millea, Hubble constant hunter’s guide
Original
1908
Earlier work this paper cites.
T. Tröster et al
Original
1909
Earlier work this paper cites.
A. Lewis, GetDist: a Python package for analysing Monte Carlo samples
Original
1910
Earlier work this paper cites.
F. N. Chamings, A. Avgoustidis, E. J. Copeland, A. M. Green, and A. Pourtsidou, Understanding the suppression of structure formation from dark matter-dark energy momentum coupling
Original
1912
Earlier work this paper cites.
E. J. Copeland, M. Sami, and S. Tsujikawa, Dynamics of dark energy
1936
Earlier work this paper cites.
L. Guzzo et al
Original
1944
Earlier work this paper cites.
B. Jain and E. Bertschinger, Second-Order Power Spectrum and Nonlinear Evolution at High Redshift
1994
Earlier work this paper cites.
R. R. Caldwell, R. Dave, and P. J. Steinhardt, Cosmological imprint of an energy component with general equation of state
1998
Earlier work this paper cites.
D. J. Eisenstein and W. Hu, Baryonic features in the matter transfer function
1998
Earlier work this paper cites.
R. Scoccimarro, H. M. P. Couchman, and J. A. Frieman, The Bispectrum as a Signature of Gravitational Instability in Redshift Space
1999
Earlier work this paper cites.
L. Amendola, Coupled quintessence
2000
Earlier work this paper cites.
A. Lewis, A. Challinor, and A. Lasenby, Efficient computation of CMB anisotropies in closed FRW models
2000
Earlier work this paper cites.
E. Jones, T. Oliphant, P. Peterson, et al
2001
Earlier work this paper cites.
F. Bernardeau, S. Colombi, E. Gaztanaga, and R. Scoccimarro, Large scale structure of the universe and cosmological perturbation theory
2002
Earlier work this paper cites.
P. J. E. Peebles and B. Ratra, The Cosmological Constant and Dark Energy
2003
Earlier work this paper cites.
T. Nishimichi, G. D’Amico, M. M. Ivanov, L. Senatore, M. Simonović, M. Takada, M. Zaldarriaga, and P. Zhang, Blinded challenge for precision cosmology with large-scale structure: results from effective field theory for the redshift-space galaxy power spectrum
Original
2003
Earlier work this paper cites.
A. Gómez-Valent, V. Pettorino, and L. Amendola, Update on coupled dark energy and the H 0 H_{0} tension
Original
2004
Earlier work this paper cites.
A. Chudaykin, M. M. Ivanov, O. H. E. Philcox, and M. Simonović, Nonlinear perturbation theory extension of the Boltzmann code CLASS
Original
2004
Earlier work this paper cites.
S. Nojiri and S. D. Odintsov, Introduction to modified gravity and gravitational alternative for dark energy
2006
Earlier work this paper cites.
A. Eggemeier, R. Scoccimarro, M. Crocce, A. Pezzotta, and A. G. Sánchez, Testing one-loop galaxy bias: Power spectrum
Original
2006
Earlier work this paper cites.
C. Heymans et al
Original
2007
Earlier work this paper cites.
J. D. Hunter, Matplotlib: A 2d graphics environment
2007
Earlier work this paper cites.
E. Di Valentino et al
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2008
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E. Di Valentino et al
Original
2008
Earlier work this paper cites.
R. Bean, E. E. Flanagan, I. Laszlo, and M. Trodden, Constraining interactions in cosmology’s dark sector
2008
Earlier work this paper cites.
A. Vikhlinin et al
Original
2009
Earlier work this paper cites.
J.-Q. Xia, Constraint on coupled dark energy models from observations
Original
2009
Earlier work this paper cites.

Similar

K. A. Malik and D. Wands, Cosmological perturbations
Original
2009
Cited alongside, same era.
P. McDonald and A. Roy, Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS
Original
2009
Cited alongside, same era.
G. Caldera-Cabral, R. Maartens, and B. M. Schaefer, The Growth of Structure in Interacting Dark Energy Models
Original
2009
Cited alongside, same era.
E. Di Valentino and O. Mena, A fake Interacting Dark Energy detection?
Original
2009
Cited alongside, same era.
T. P. Sotiriou and V. Faraoni, f(R) Theories Of Gravity
Original
2010

Then

F. Beutler, H.-J. Seo, S. Saito, C.-H. Chuang, A. J. Cuesta, D. J. Eisenstein, H. Gil-Marín, J. N. Grieb, N. Hand, F.-S. Kitaura, and et al., The clustering of galaxies in the completed sdss-iii baryon oscillation spectroscopic survey: anisotropic galaxy clustering in fourier space
2016
Later among the works it cites.
F. Simpson, C. Blake, J. A. Peacock, I. Baldry, J. Bland-Hawthorn, A. Heavens, C. Heymans, J. Loveday, and P. Norberg, Galaxy and mass assembly: Redshift space distortions from the clipped galaxy field
Original
2016
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A. Pourtsidou and T. Tram, Reconciling CMB and structure growth measurements with dark energy interactions
Original
2016
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J. Lesgourgues, G. Marques-Tavares, and M. Schmaltz, Evidence for dark matter interactions in cosmological precision data?
Original
2016
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