Built on

L. Perenon, J. Bel, R. Maartens, and A. de la Cruz-Dombriz, “Optimising growth of structure constraints on modified gravity,” JCAP
Original
1901
Earlier work this paper cites.
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,” Mon. Not. Roy. Astron. Soc
Original
1901
Earlier work this paper cites.
M. Raveri, “Reconstructing Gravity on Cosmological Scales,” Phys. Rev. D
Original
1902
Earlier work this paper cites.
G. Brando, F. T. Falciano, E. V. Linder, and H. E. S. Velten, “Modified gravity away from a Λ \Lambda CDM background,” JCAP
Original
1904
Earlier work this paper cites.
R. Arjona, W. Cardona, and S. Nesseris, “Designing Horndeski and the effective fluid approach,” Phys. Rev. D
Original
1904
Earlier work this paper cites.
S. Melville and J. Noller, “Positivity in the Sky: Constraining dark energy and modified gravity from the UV,” Phys. Rev. D
Original
1904
Earlier work this paper cites.
N. Frusciante and L. Perenon, “Effective field theory of dark energy: A review,” Phys. Rept
Original
1907
Earlier work this paper cites.
E. Bellini, I. Sawicki, and M. Zumalacárregui, “hi_class: Background Evolution, Initial Conditions and Approximation Schemes,” JCAP
Original
1909
Earlier work this paper cites.
A. Bonilla, R. D’Agostino, R. C. Nunes, and J. C. N. de Araujo, “Forecasts on the speed of gravitational waves at high z z ,” JCAP
Original
1910
Earlier work this paper cites.
P. Creminelli, G. Tambalo, F. Vernizzi, and V. Yingcharoenrat, “Dark-Energy Instabilities induced by Gravitational Waves,” arXiv:1910.14035 [gr-qc]
Original
1910
Earlier work this paper cites.
S. Arai, P. Karmakar, and A. Nishizawa, “Cosmological evolution of viable models in the generalized scalar-tensor theory,” Phys. Rev. D
Original
1912
Earlier work this paper cites.
D. N. Limber, “The Analysis of Counts of the Extragalactic Nebulae in Terms of a Fluctuating Density Field. II,” Astrophys. J
1954
Earlier work this paper cites.
G. W. Horndeski, “Second-order scalar-tensor field equations in a four-dimensional space,” Int. J. Theor. Phys
1974
Earlier work this paper cites.
N. Kaiser, “Weak gravitational lensing of distant galaxies,” Astrophys. J
1992
Earlier work this paper cites.
N. Kaiser, “Weak lensing and cosmology,” Astrophys. J
1998
Earlier work this paper cites.
J. J. Condon, W. D. Cotton, E. W. Greisen, Q. F. Yin, R. A. Perley, G. B. Taylor, and J. J. Broderick, “The NRAO VLA Sky survey,” Astron. J
1998
Earlier work this paper cites.
J. Noller, “Cosmological constraints on dark energy in light of gravitational wave bounds,” Phys. Rev. D
Original
2001
Earlier work this paper cites.
F. Calore, A. Cuoco, T. Regimbau, S. Sachdev, and P. D. Serpico, “Cross-correlating galaxy catalogs and gravitational waves: a tomographic approach,” Phys. Rev. Res
Original
2002
Earlier work this paper cites.
P. Fosalba, E. Gaztanaga, and F. Castander, “Detection of the ISW and SZ effects from the CMB-galaxy correlation,” Astrophys. J. Lett
2003
Earlier work this paper cites.
J. Kennedy and L. Lombriser, “Positivity bounds on reconstructed Horndeski models,” Phys. Rev. D
Original
2003
Earlier work this paper cites.
K. M. Huffenberger, U. Seljak, and A. Makarov, “Sunyaev-Zeldovich effect in WMAP and its effect on cosmological parameters,” Phys. Rev. D
2004
Earlier work this paper cites.
N. Afshordi, Y.-S. Loh, and M. A. Strauss, “Cross - correlation of the Cosmic Microwave Background with the 2MASS galaxy survey: Signatures of dark energy, hot gas, and point sources,” Phys. Rev. D
2004
Earlier work this paper cites.
S. Boughn and R. Crittenden, “A Correlation of the cosmic microwave sky with large scale structure,” Nature
2004
Earlier work this paper cites.
C. Burrage and J. Dombrowski, “Constraining the cosmological evolution of scalar-tensor theories with local measurements of the time variation of G,” JCAP
Original
2004
Earlier work this paper cites.
D. B. Thomas, “Cosmological gravity on all scales: simple equations, required conditions, and a framework for modified gravity,” Phys. Rev. D
Original
2004
Earlier work this paper cites.
L. Heisenberg, J. Noller, and J. Zosso, “Horndeski under the quantum loupe,” JCAP
Original
2004
Earlier work this paper cites.
P. Vielva, E. Martinez-Gonzalez, and M. Tucci, “WMAP and NVSS cross-correlation in wavelet space: ISW detection and dark energy constraints,” Mon. Not. Roy. Astron. Soc
2006
Earlier work this paper cites.
A. Cabre, E. Gaztanaga, M. Manera, P. Fosalba, and F. Castander, “Cross-correlation of wmap 3rd year and the sdss dr4 galaxy survey: new evidence for dark energy,” Mon. Not. Roy. Astron. Soc
2006
Earlier work this paper cites.
T. Giannantonio, R. G. Crittenden, R. C. Nichol, R. Scranton, G. T. Richards, A. D. Myers, R. J. Brunner, A. G. Gray, A. J. Connolly, and D. P. Schneider, “A high redshift detection of the integrated Sachs-Wolfe effect,” Phys. Rev. D
2006
Earlier work this paper cites.
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. D
2006
Earlier work this paper cites.
T. Baker and I. Harrison, “Constraining Scalar-Tensor Modified Gravity with Gravitational Waves and Large Scale Structure Surveys,” JCAP
Original
2007
Earlier work this paper cites.
A. Cabre, P. Fosalba, E. Gaztanaga, and M. Manera, “Error analysis in cross-correlation of sky maps: Application to the ISW detection,” Mon. Not. Roy. Astron. Soc
2007
Earlier work this paper cites.
J. D. McEwen, P. Vielva, M. P. Hobson, E. Martinez-Gonzalez, and A. N. Lasenby, “Detection of the integrated Sachs–Wolfe effect and corresponding dark energy constraints made with directional spherical wavelets,” Mon. Not. Roy. Astron. Soc
2007
Earlier work this paper cites.
A. Rassat, K. Land, O. Lahav, and F. B. Abdalla, “Cross-correlation of 2MASS and WMAP3: Implications for the Integrated Sachs-Wolfe effect,” Mon. Not. Roy. Astron. Soc
2007
Earlier work this paper cites.
J. Noller, L. Santoni, E. Trincherini, and L. G. Trombetta, “Scalar-tensor cosmologies without screening,” JCAP
Original
2008
Earlier work this paper cites.
A. de la Cruz-Dombriz, A. Dobado, and A. L. Maroto, “On the evolution of density perturbations in f(R) theories of gravity,” Phys. Rev. D
Original
2008
Earlier work this paper cites.
A. Raccanelli, A. Bonaldi, M. Negrello, S. Matarrese, G. Tormen, and G. De Zotti, “A reassessment of the evidence of the Integrated Sachs-Wolfe effect through the WMAP-NVSS correlation,” Mon. Not. Roy. Astron. Soc
Original
2008
Earlier work this paper cites.
S. Ho, C. Hirata, N. Padmanabhan, U. Seljak, and N. Bahcall, “Correlation of CMB with large-scale structure: I. ISW Tomography and Cosmological Implications,” Phys. Rev. D
Original
2008
Earlier work this paper cites.
T. Giannantonio, R. Scranton, R. G. Crittenden, R. C. Nichol, S. P. Boughn, A. D. Myers, and G. T. Richards, “Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications,” Phys. Rev. D
Original
2008
Earlier work this paper cites.
M. LoVerde and N. Afshordi, “Extended Limber Approximation,” Phys. Rev. D
Original
2008
Earlier work this paper cites.
J.-Q. Xia, M. Viel, C. Baccigalupi, and S. Matarrese, “The High Redshift Integrated Sachs-Wolfe Effect,” JCAP
Original
2009
Earlier work this paper cites.

Similar

G. T. Richards, A. D. Myers, A. G. Gray, R. N. Riegel, R. C. Nichol, R. J. Brunner, A. S. Szalay, D. P. Schneider, and S. F. Anderson, “Efficient Photometric Selection of Quasars from the Sloan Digital Sky Survey: II. ~1,000,000 Quasars from Data Release Six,” Astrophys. J. Suppl
Original
2009
Cited alongside, same era.
S. Joudaki, P. G. Ferreira, N. A. Lima, and H. A. Winther, “Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory,” arXiv:2010.15278 [astro-ph.CO]
Original
2010
Cited alongside, same era.
T. Kobayashi, M. Yamaguchi, and J. Yokoyama, “Generalized G-inflation: Inflation with the most general second-order field equations,” Prog. Theor. Phys
Original
2011
Cited alongside, same era.
C. Deffayet, X. Gao, D. A. Steer, and G. Zahariade, “From k-essence to generalised Galileons,” Phys. Rev
Original
2011
Cited alongside, same era.

Then

P. Creminelli and F. Vernizzi, “Dark Energy after GW170817 and GRB170817A,” Phys. Rev. Lett
Original
2017
Later among the works it cites.
J. Sakstein and B. Jain, “Implications of the Neutron Star Merger GW170817 for Cosmological Scalar-Tensor Theories,” Phys. Rev. Lett
Original
2017
Later among the works it cites.
J. M. Ezquiaga and M. Zumalacárregui, “Dark Energy After GW170817: Dead Ends and the Road Ahead,” Phys. Rev. Lett
Original
2017
Later among the works it cites.
T. Baker, E. Bellini, P. G. Ferreira, M. Lagos, J. Noller, and I. Sawicki, “Strong constraints on cosmological gravity from GW170817 and GRB 170817A,” Phys. Rev. Lett
Original
2017
Later among the works it cites.
E. V. Linder, “Challenges in connecting modified gravity theory and observations,” Phys. Rev

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2024

Constraining dark energy with the integrated Sachs-Wolfe effect

Seraille, Emeric, Noller, Johannes, Sherwin, Blake D.

Understand

We use the integrated Sachs-Wolfe (ISW) effect, by now detectable at $\sim 5\sigma$ within the context of $\Lambda{}$CDM cosmologies, to place strong constraints on dynamical dark energy theories.

Working within an effective field theory framework for dark energy we find that including ISW constraints from galaxy-CMB cross-correlations significantly strengthens existing large-scale structure constraints, yielding bounds consistent with $\Lambda{}$CDM and approximately reducing the viable parameter space by $\sim 70\%$.
This is a direct consequence of ${\cal O}(1)$ changes induced in these cross-correlations by otherwise viable dark energy models, which we discuss in detail.
We compute constraints by adapting the $\Lambda{}$CDM ISW likelihood from [1] for dynamical dark energy models using galaxy data from 2MASS, WISE $\times$ SuperCOSMOS, SDSS-DR12, QSOs and NVSS, CMB data from Planck 18, and BAO and RSD large scale structure measurements from BOSS and 6dF.

Built on

L. Perenon, J. Bel, R. Maartens, and A. de la Cruz-Dombriz, “Optimising growth of structure constraints on modified gravity,” JCAP
Original
1901
Earlier work this paper cites.
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,” Mon. Not. Roy. Astron. Soc
Original
1901
Earlier work this paper cites.
M. Raveri, “Reconstructing Gravity on Cosmological Scales,” Phys. Rev. D
Original
1902
Earlier work this paper cites.
G. Brando, F. T. Falciano, E. V. Linder, and H. E. S. Velten, “Modified gravity away from a Λ \Lambda CDM background,” JCAP
Original
1904
Earlier work this paper cites.
R. Arjona, W. Cardona, and S. Nesseris, “Designing Horndeski and the effective fluid approach,” Phys. Rev. D
Original
1904
Earlier work this paper cites.
S. Melville and J. Noller, “Positivity in the Sky: Constraining dark energy and modified gravity from the UV,” Phys. Rev. D
Original
1904
Earlier work this paper cites.
N. Frusciante and L. Perenon, “Effective field theory of dark energy: A review,” Phys. Rept
Original
1907
Earlier work this paper cites.
E. Bellini, I. Sawicki, and M. Zumalacárregui, “hi_class: Background Evolution, Initial Conditions and Approximation Schemes,” JCAP
Original
1909
Earlier work this paper cites.
A. Bonilla, R. D’Agostino, R. C. Nunes, and J. C. N. de Araujo, “Forecasts on the speed of gravitational waves at high z z ,” JCAP
Original
1910
Earlier work this paper cites.
P. Creminelli, G. Tambalo, F. Vernizzi, and V. Yingcharoenrat, “Dark-Energy Instabilities induced by Gravitational Waves,” arXiv:1910.14035 [gr-qc]
Original
1910
Earlier work this paper cites.
S. Arai, P. Karmakar, and A. Nishizawa, “Cosmological evolution of viable models in the generalized scalar-tensor theory,” Phys. Rev. D
Original
1912
Earlier work this paper cites.
D. N. Limber, “The Analysis of Counts of the Extragalactic Nebulae in Terms of a Fluctuating Density Field. II,” Astrophys. J
1954
Earlier work this paper cites.
G. W. Horndeski, “Second-order scalar-tensor field equations in a four-dimensional space,” Int. J. Theor. Phys
1974
Earlier work this paper cites.
N. Kaiser, “Weak gravitational lensing of distant galaxies,” Astrophys. J
1992
Earlier work this paper cites.
N. Kaiser, “Weak lensing and cosmology,” Astrophys. J
1998
Earlier work this paper cites.
J. J. Condon, W. D. Cotton, E. W. Greisen, Q. F. Yin, R. A. Perley, G. B. Taylor, and J. J. Broderick, “The NRAO VLA Sky survey,” Astron. J
1998
Earlier work this paper cites.
J. Noller, “Cosmological constraints on dark energy in light of gravitational wave bounds,” Phys. Rev. D
Original
2001
Earlier work this paper cites.
F. Calore, A. Cuoco, T. Regimbau, S. Sachdev, and P. D. Serpico, “Cross-correlating galaxy catalogs and gravitational waves: a tomographic approach,” Phys. Rev. Res
Original
2002
Earlier work this paper cites.
P. Fosalba, E. Gaztanaga, and F. Castander, “Detection of the ISW and SZ effects from the CMB-galaxy correlation,” Astrophys. J. Lett
2003
Earlier work this paper cites.
J. Kennedy and L. Lombriser, “Positivity bounds on reconstructed Horndeski models,” Phys. Rev. D
Original
2003
Earlier work this paper cites.
K. M. Huffenberger, U. Seljak, and A. Makarov, “Sunyaev-Zeldovich effect in WMAP and its effect on cosmological parameters,” Phys. Rev. D
2004
Earlier work this paper cites.
N. Afshordi, Y.-S. Loh, and M. A. Strauss, “Cross - correlation of the Cosmic Microwave Background with the 2MASS galaxy survey: Signatures of dark energy, hot gas, and point sources,” Phys. Rev. D
2004
Earlier work this paper cites.
S. Boughn and R. Crittenden, “A Correlation of the cosmic microwave sky with large scale structure,” Nature
2004
Earlier work this paper cites.
C. Burrage and J. Dombrowski, “Constraining the cosmological evolution of scalar-tensor theories with local measurements of the time variation of G,” JCAP
Original
2004
Earlier work this paper cites.
D. B. Thomas, “Cosmological gravity on all scales: simple equations, required conditions, and a framework for modified gravity,” Phys. Rev. D
Original
2004
Earlier work this paper cites.
L. Heisenberg, J. Noller, and J. Zosso, “Horndeski under the quantum loupe,” JCAP
Original
2004
Earlier work this paper cites.
P. Vielva, E. Martinez-Gonzalez, and M. Tucci, “WMAP and NVSS cross-correlation in wavelet space: ISW detection and dark energy constraints,” Mon. Not. Roy. Astron. Soc
2006
Earlier work this paper cites.
A. Cabre, E. Gaztanaga, M. Manera, P. Fosalba, and F. Castander, “Cross-correlation of wmap 3rd year and the sdss dr4 galaxy survey: new evidence for dark energy,” Mon. Not. Roy. Astron. Soc
2006
Earlier work this paper cites.
T. Giannantonio, R. G. Crittenden, R. C. Nichol, R. Scranton, G. T. Richards, A. D. Myers, R. J. Brunner, A. G. Gray, A. J. Connolly, and D. P. Schneider, “A high redshift detection of the integrated Sachs-Wolfe effect,” Phys. Rev. D
2006
Earlier work this paper cites.
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. D
2006
Earlier work this paper cites.
T. Baker and I. Harrison, “Constraining Scalar-Tensor Modified Gravity with Gravitational Waves and Large Scale Structure Surveys,” JCAP
Original
2007
Earlier work this paper cites.
A. Cabre, P. Fosalba, E. Gaztanaga, and M. Manera, “Error analysis in cross-correlation of sky maps: Application to the ISW detection,” Mon. Not. Roy. Astron. Soc
2007
Earlier work this paper cites.
J. D. McEwen, P. Vielva, M. P. Hobson, E. Martinez-Gonzalez, and A. N. Lasenby, “Detection of the integrated Sachs–Wolfe effect and corresponding dark energy constraints made with directional spherical wavelets,” Mon. Not. Roy. Astron. Soc
2007
Earlier work this paper cites.
A. Rassat, K. Land, O. Lahav, and F. B. Abdalla, “Cross-correlation of 2MASS and WMAP3: Implications for the Integrated Sachs-Wolfe effect,” Mon. Not. Roy. Astron. Soc
2007
Earlier work this paper cites.
J. Noller, L. Santoni, E. Trincherini, and L. G. Trombetta, “Scalar-tensor cosmologies without screening,” JCAP
Original
2008
Earlier work this paper cites.
A. de la Cruz-Dombriz, A. Dobado, and A. L. Maroto, “On the evolution of density perturbations in f(R) theories of gravity,” Phys. Rev. D
Original
2008
Earlier work this paper cites.
A. Raccanelli, A. Bonaldi, M. Negrello, S. Matarrese, G. Tormen, and G. De Zotti, “A reassessment of the evidence of the Integrated Sachs-Wolfe effect through the WMAP-NVSS correlation,” Mon. Not. Roy. Astron. Soc
Original
2008
Earlier work this paper cites.
S. Ho, C. Hirata, N. Padmanabhan, U. Seljak, and N. Bahcall, “Correlation of CMB with large-scale structure: I. ISW Tomography and Cosmological Implications,” Phys. Rev. D
Original
2008
Earlier work this paper cites.
T. Giannantonio, R. Scranton, R. G. Crittenden, R. C. Nichol, S. P. Boughn, A. D. Myers, and G. T. Richards, “Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications,” Phys. Rev. D
Original
2008
Earlier work this paper cites.
M. LoVerde and N. Afshordi, “Extended Limber Approximation,” Phys. Rev. D
Original
2008
Earlier work this paper cites.
J.-Q. Xia, M. Viel, C. Baccigalupi, and S. Matarrese, “The High Redshift Integrated Sachs-Wolfe Effect,” JCAP
Original
2009
Earlier work this paper cites.

Similar

G. T. Richards, A. D. Myers, A. G. Gray, R. N. Riegel, R. C. Nichol, R. J. Brunner, A. S. Szalay, D. P. Schneider, and S. F. Anderson, “Efficient Photometric Selection of Quasars from the Sloan Digital Sky Survey: II. ~1,000,000 Quasars from Data Release Six,” Astrophys. J. Suppl
Original
2009
Cited alongside, same era.
S. Joudaki, P. G. Ferreira, N. A. Lima, and H. A. Winther, “Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory,” arXiv:2010.15278 [astro-ph.CO]
Original
2010
Cited alongside, same era.
T. Kobayashi, M. Yamaguchi, and J. Yokoyama, “Generalized G-inflation: Inflation with the most general second-order field equations,” Prog. Theor. Phys
Original
2011
Cited alongside, same era.
C. Deffayet, X. Gao, D. A. Steer, and G. Zahariade, “From k-essence to generalised Galileons,” Phys. Rev
Original
2011
Cited alongside, same era.

Then

P. Creminelli and F. Vernizzi, “Dark Energy after GW170817 and GRB170817A,” Phys. Rev. Lett
Original
2017
Later among the works it cites.
J. Sakstein and B. Jain, “Implications of the Neutron Star Merger GW170817 for Cosmological Scalar-Tensor Theories,” Phys. Rev. Lett
Original
2017
Later among the works it cites.
J. M. Ezquiaga and M. Zumalacárregui, “Dark Energy After GW170817: Dead Ends and the Road Ahead,” Phys. Rev. Lett
Original
2017
Later among the works it cites.
T. Baker, E. Bellini, P. G. Ferreira, M. Lagos, J. Noller, and I. Sawicki, “Strong constraints on cosmological gravity from GW170817 and GRB 170817A,” Phys. Rev. Lett
Original
2017
Later among the works it cites.
E. V. Linder, “Challenges in connecting modified gravity theory and observations,” Phys. Rev

Beyond the bibliography

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

Open on alphaXiv

alphaXiv is searching for related work…

D. Blas, J. Lesgourgues, and T. Tram, “The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes,” JCAP

Original

2011

Cited alongside, same era.

F. X. Dupe, A. Rassat, J. L. Starck, and M. J. Fadili, “Measuring the Integrated Sachs-Wolfe Effect,” Astron. Astrophys

Original

2011

Cited alongside, same era.

E. Babichev, C. Deffayet, and G. Esposito-Farese, “Constraints on Shift-Symmetric Scalar-Tensor Theories with a Vainshtein Mechanism from Bounds on the Time Variation of G,” Phys. Rev. Lett

Original

2011

Cited alongside, same era.

R. Kimura, T. Kobayashi, and K. Yamamoto, “Observational Constraints on Kinetic Gravity Braiding from the Integrated Sachs-Wolfe Effect,” Phys. Rev. D

Original

2012

Cited alongside, same era.

T. Giannantonio, R. Crittenden, R. Nichol, and A. J. Ross, “The significance of the integrated Sachs-Wolfe effect revisited,” Mon. Not. Roy. Astron. Soc

Original

2012

Cited alongside, same era.

F. Beutler, C. Blake, M. Colless, D. H. Jones, L. Staveley-Smith, G. B. Poole, L. Campbell, Q. Parker, W. Saunders, and F. Watson, “The 6dF Galaxy Survey: z ≈ 0 z\approx 0 measurement of the growth rate and σ 8 \sigma_{8} ,” Mon. Not. Roy. Astron. Soc

Original

2012

Cited alongside, same era.

G. Gubitosi, F. Piazza, and F. Vernizzi, “The Effective Field Theory of Dark Energy,” JCAP

Original

2013

Cited alongside, same era.

J. K. Bloomfield, E. E. Flanagan, M. Park, and S. Watson, “Dark energy or modified gravity? An effective field theory approach,” JCAP

Original

2013

Cited alongside, same era.

Original

2017