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Assuming that the universe contains a dark energy fluid with a constant linear equation of state and a constant sound speed, we study the prospects of detecting dark energy perturbations using CMB data from Planck, cross-correlated with galaxy distribution maps from a survey like LSST.
C.-P. Ma and E. Bertschinger, “Cosmological perturbation theory in the synchronous and conformal Newtonian gauges,” Astrophys. J
1995
Earlier work this paper cites.
W. Hu, “Structure Formation with Generalized Dark Matter,” Astrophys. J
1998
Earlier work this paper cites.
M. Bucher, K. Moodley, and N. Turok, “The general primordial cosmic perturbation,” Phys. Rev
2000
Earlier work this paper cites.
A. Lewis, A. Challinor, and A. Lasenby, “Efficient computation of CMB anisotropies in closed FRW models,” Astrophys. J
2000
Earlier work this paper cites.
R. Dave, R. R. Caldwell and P. J. Steinhardt, “Sensitivity of the cosmic microwave background anisotropy to initial conditions in quintessence cosmology,” Phys. Rev. D 66
2002
Earlier work this paper cites.
A. Lewis and S. Bridle, “Cosmological parameters from CMB and other data: a Monte- Carlo approach,” Phys. Rev
2002
Earlier work this paper cites.
S. DeDeo, R. R. Caldwell, and P. J. Steinhardt, “Effects of the sound speed of quintessence on the microwave background and large scale structure,” Phys. Rev
2003
Earlier work this paper cites.
J. Weller and A. M. Lewis, “Large Scale Cosmic Microwave Background Anisotropies and Dark Energy,” Mon. Not. Roy. Astron. Soc
2003
Earlier work this paper cites.
M. Doran, C. M. Muller, G. Schafer, and C. Wetterich, “Gauge-invariant initial conditions and early time perturbations in quintessence universes,” Phys. Rev
2003
Earlier work this paper cites.
T. Okamoto and W. Hu, “CMB Lensing Reconstruction on the Full Sky,” Phys. Rev
2003
Earlier work this paper cites.
R. Bean and O. Doré, “Probing dark energy perturbations: the dark energy equation of state and speed of sound as measured by WMAP,” Phys. Rev
2004
Earlier work this paper cites.
W. Hu and R. Scranton, “Measuring Dark Energy Clustering with CMB-Galaxy Correlations,” Phys. Rev
2004
Earlier work this paper cites.
S. Hannestad, “Constraints on the sound speed of dark energy,” Phys. Rev
2005
Cited alongside, same era.
P.-S. Corasaniti, T. Giannantonio, and A. Melchiorri, “Constraining dark energy with cross-correlated CMB and Large Scale Structure data,” Phys. Rev
2005
Cited alongside, same era.
M. Takada, “Can A Galaxy Redshift Survey Measure Dark Energy Clustering?,” Phys. Rev
2006
Cited alongside, same era.
D. Pietrobon, A. Balbi and D. Marinucci, “Integrated Sachs-Wolfe effect from the cross-correlation of WMAP 3 year and NVSS: new results and constraints on dark energy,” Phys. Rev
2006
Cited alongside, same era.
L. Perotto, J. Lesgourgues, S. Hannestad, H. Tu, and Y. Y. Y. Wong, “Probing cosmological parameters with the CMB: Forecasts from full Monte Carlo simulations,” JCAP
2006
Cited alongside, same era.
E. Bertschinger and P. Zukin, “Distinguishing Modified Gravity from Dark Energy,” 2008, 0801.2431
2008
Later among the works it cites.
A. Torres-Rodriguez, C. M. Cress, and K. Moodley, “Covariance of dark energy parameters and sound speed constraints from large HI surveys,” 2008, 0804.2344
2008
Later among the works it cites.
2008
Later among the works it cites.
G. Ballesteros and A. Riotto, “Parameterizing the Effect of Dark Energy Perturbations on the Growth of Structures,” Phys. Lett
2008
Later among the works it cites.
J. Lesgourgues, W. Valkenburg, and E. Gaztanaga, “Constraining neutrino masses with the ISW-galaxy correlation function,” Phys. Rev
2008
Later among the works it cites.
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J. Lesgourgues, L. Perotto, S. Pastor, and M. Piat, “Probing neutrino masses with CMB lensing extraction,” Phys. Rev
2006
Cited alongside, same era.
M. Kunz and D. Sapone, “Dark energy versus modified gravity,” Phys. Rev. Lett
2007
Cited alongside, same era.
J.-Q. Xia, Y.-F. Cai, T.-T. Qiu, G.-B. Zhao, and X. Zhang, “Constraints on the sound speed of dynamical dark energy,” 2007, astro-ph/0703202
2007
Cited alongside, same era.
D. F. Mota, J. R. Kristiansen, T. Koivisto, and N. E. Groeneboom, “Constraining Dark Energy Anisotropic Stress,” 2007, 0708.0830
2007
Cited alongside, same era.
A. Torres-Rodriguez and C. M. Cress, “Constraining the Nature of Dark Energy using the SKA,” Mon. Not. Roy. Astron. Soc
2007
Cited alongside, same era.
M. LoVerde, L. Hui, and E. Gaztanaga, “Magnification-Temperature Correlation: the Dark Side of ISW Measurements,” Phys. Rev
2007
Cited alongside, same era.
P. Creminelli, G. D’Amico, J. Norena, and F. Vernizzi, “The Effective Theory of Quintessence: the w < < -1 Side Unveiled,” JCAP
2009
Later among the works it cites.
D. Sapone, M. Kunz, and M. Kunz, “Fingerprinting Dark Energy,” Phys. Rev
2009
Later among the works it cites.
2009
Later among the works it cites.
R. de Putter, D. Huterer, and E. V. Linder, “Measuring the Speed of Dark: Detecting Dark Energy Perturbations,” 2010, 1002.1311
2010
Closest in time.
2010
Closest in time.
M. Martinelli, L. L. Honorez, A. Melchiorri, and O. Mena, “Future CMB cosmological constraints in a dark coupled universe,” 2010, 1004.2410
2010
Closest in time.