Built on

P. Zhang, M. Liguori, R. Bean, and S. Dodelson, “Probing Gravity at Cosmological Scales by Measurements which Test the Relationship between Gravitational Lensing and Matter Overdensity,” Phys.Rev.Lett
Original
1932
Earlier work this paper cites.
G. W. Horndeski, “Second-order scalar-tensor field equations in a four-dimensional space,” Int.J.Th.Phys
1974
Earlier work this paper cites.
N. Kaiser, “Clustering in real space and in redshift space,” Mon.Not.Roy.Astron.Soc
1987
Earlier work this paper cites.
W. Hu, “Power spectrum tomography with weak lensing,” Astrophys.J
1999
Earlier work this paper cites.
R. Scoccimarro, H. Couchman, and J. A. Frieman, “The Bispectrum as a signature of gravitational instability in redshift-space,” Astrophys.J
1999
Earlier work this paper cites.
C. Armendariz-Picon, T. Damour, and V. F. Mukhanov, “k - inflation,” Phys.Lett
1999
Earlier work this paper cites.
J. Garriga and V. F. Mukhanov, “Perturbations in k-inflation,” Phys.Lett
1999
Earlier work this paper cites.
L. Amendola, “Coupled quintessence,” Phys.Rev
2000
Earlier work this paper cites.
C. Armendariz-Picon, V. F. Mukhanov, and P. J. Steinhardt, “A Dynamical solution to the problem of a small cosmological constant and late time cosmic acceleration,” Phys.Rev.Lett
2000
Earlier work this paper cites.
C. Armendariz-Picon, V. F. Mukhanov, and P. J. Steinhardt, “Essentials of k essence,” Phys.Rev
2001
Earlier work this paper cites.
D. Huterer and G. Starkman, “Parameterization of dark-energy properties: A Principal-component approach,” Phys.Rev.Lett
2003
Earlier work this paper cites.
R. R. Caldwell and M. Doran, “Dark-energy evolution across the cosmological-constant boundary,” Phys.Rev
2005
Earlier work this paper cites.
E. V. Linder, “Cosmic growth history and expansion history,” Phys.Rev
2005
Earlier work this paper cites.
E. Bertschinger, “On the Growth of Perturbations as a Test of Dark Energy,” Astrophys.J
2006
Earlier work this paper cites.
M. Kunz and D. Sapone, “Crossing the Phantom Divide,” Phys.Rev
2006
Earlier work this paper cites.
R. Kimura and K. Yamamoto, “Large Scale Structures in Kinetic Gravity Braiding Model That Can Be Unbraided,” JCAP
Original
2006
Earlier work this paper cites.
W. Hu and I. Sawicki, “A Parameterized Post-Friedmann Framework for Modified Gravity,” Phys.Rev
Original
2007
Earlier work this paper cites.
W. Hu and I. Sawicki, “Models of f(R) Cosmic Acceleration that Evade Solar-System Tests,” Phys.Rev
Original
2007
Earlier work this paper cites.

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2013

Probing Dark Energy through Scale Dependence

Motta, Mariele, Sawicki, Ignacy, Saltas, Ippocratis D. et al.

Understand

We consider the consequences of having no prior knowledge of the true dark energy model for the interpretation of cosmological observations.

The magnitude of redshift-space distortions and weak-lensing shear is determined by the metric on the geodesics of which galaxies and light propagate.
We show that, given precise enough observations, we can use these data to completely reconstruct the metric on our past lightcone and therefore to measure the scale- and time-dependence of the anisotropic stress and the evolution of the gravitational potentials in a model-independent manner.
Since both dark matter and dark energy affect the visible sector only through the gravitational field they produce, they are inseparable without a model for dark energy: galaxy bias cannot be measured and therefore the distribution of dark matter determined; the peculiar velocity of dark matter can be identified with that of the galaxies only when the equivalence principle holds.

Built on

P. Zhang, M. Liguori, R. Bean, and S. Dodelson, “Probing Gravity at Cosmological Scales by Measurements which Test the Relationship between Gravitational Lensing and Matter Overdensity,” Phys.Rev.Lett
Original
1932
Earlier work this paper cites.
G. W. Horndeski, “Second-order scalar-tensor field equations in a four-dimensional space,” Int.J.Th.Phys
1974
Earlier work this paper cites.
N. Kaiser, “Clustering in real space and in redshift space,” Mon.Not.Roy.Astron.Soc
1987
Earlier work this paper cites.
W. Hu, “Power spectrum tomography with weak lensing,” Astrophys.J
1999
Earlier work this paper cites.
R. Scoccimarro, H. Couchman, and J. A. Frieman, “The Bispectrum as a signature of gravitational instability in redshift-space,” Astrophys.J
1999
Earlier work this paper cites.
C. Armendariz-Picon, T. Damour, and V. F. Mukhanov, “k - inflation,” Phys.Lett
1999
Earlier work this paper cites.
J. Garriga and V. F. Mukhanov, “Perturbations in k-inflation,” Phys.Lett
1999
Earlier work this paper cites.
L. Amendola, “Coupled quintessence,” Phys.Rev
2000
Earlier work this paper cites.
C. Armendariz-Picon, V. F. Mukhanov, and P. J. Steinhardt, “A Dynamical solution to the problem of a small cosmological constant and late time cosmic acceleration,” Phys.Rev.Lett
2000
Earlier work this paper cites.
C. Armendariz-Picon, V. F. Mukhanov, and P. J. Steinhardt, “Essentials of k essence,” Phys.Rev
2001
Earlier work this paper cites.
D. Huterer and G. Starkman, “Parameterization of dark-energy properties: A Principal-component approach,” Phys.Rev.Lett
2003
Earlier work this paper cites.
R. R. Caldwell and M. Doran, “Dark-energy evolution across the cosmological-constant boundary,” Phys.Rev
2005
Earlier work this paper cites.
E. V. Linder, “Cosmic growth history and expansion history,” Phys.Rev
2005
Earlier work this paper cites.
E. Bertschinger, “On the Growth of Perturbations as a Test of Dark Energy,” Astrophys.J
2006
Earlier work this paper cites.
M. Kunz and D. Sapone, “Crossing the Phantom Divide,” Phys.Rev
2006
Earlier work this paper cites.
R. Kimura and K. Yamamoto, “Large Scale Structures in Kinetic Gravity Braiding Model That Can Be Unbraided,” JCAP
Original
2006
Earlier work this paper cites.
W. Hu and I. Sawicki, “A Parameterized Post-Friedmann Framework for Modified Gravity,” Phys.Rev
Original
2007
Earlier work this paper cites.
W. Hu and I. Sawicki, “Models of f(R) Cosmic Acceleration that Evade Solar-System Tests,” Phys.Rev
Original
2007
Earlier work this paper cites.