Built on

E.V. Linder, No Run Gravity, JCAP 1907, 034 (2019) [arXiv:1903.02010]
Original
1903
Earlier work this paper cites.
G. W. Horndeski, Second-order scalar-tensor field equations in a four-dimensional space, Int. J. Theor. Phys. 10 (1974) 363
1974
Earlier work this paper cites.
A. Gelman and D. B. Rubin, Inference from Iterative Simulation Using Multiple Sequences, Statist. Sci. 7 (1992) 457
1992
Earlier work this paper cites.
M.J. Francis, G.F. Lewis, E.V. Linder, Power Spectra to 1% Accuracy between Dynamical Dark Energy Cosmologies, Mon. Not. Roy. Astron. Soc. 380, 1079 (2007) [arXiv:0704.0312]
Original
2007
Earlier work this paper cites.
S. Ho, C. Hirata, N. Padmanabhan, U. Seljak and N. Bahcall, Phys. Rev. D 78, 043519 (2008) [arXiv:0801.0642]
Original
2008
Earlier work this paper cites.
C. Deffayet, X. Gao, D. A. Steer and G. Zahariade, From k-essence to generalised Galileons, Phys. Rev. D84 (2011) 064039 [1103.3260]
2011
Earlier work this paper cites.
F. Beutler et al., The 6dF Galaxy Survey: z ≈ 0 z\approx 0 measurements of the growth rate and σ 8 \sigma_{8} , Mon. Not. R. Astron. Soc. 423, 3430 (2012) [arXiv:1204.4725]
Original
2012
Earlier work this paper cites.
C. Blake et al., The WiggleZ Dark Energy Survey: Joint measurements of the expansion and growth history at z < 1 z<1 , Mon. Not. R. Astron. Soc. 425, 405 (2012) [arXiv:1204.3674]
Original
2012
Earlier work this paper cites.
G. Gubitosi, F. Piazza, and F. Vernizzi, The effective field theory of dark energy, J. Cosmol. Astropart. Phys. 02 (2013) 032 [arXiv:1210.0201]
Original
2013
Earlier work this paper cites.
J. K. Bloomfield, E. E. Flanagan, M. Park, and S. Watson, Dark energy or modified gravity? An effective field theory approach, J. Cosmol. Astropart. Phys. 08 (2013) 010 [arXiv:1211.7054]
Original
2013
Earlier work this paper cites.
J. Gleyzes, D. Langlois, F. Piazza, and F. Vernizzi, Essential building blocks of dark energy, J. Cosmol. Astropart. Phys. 08 (2013) 025 [arXiv:1304.4840]
Original
2013
Earlier work this paper cites.
C. Blake et al., Galaxy And Mass Assembly (GAMA): improved cosmic growth measurements using multiple tracers of large-scale structure, Mon. Not. R. Astron. Soc. 436, 3089 (2013) [arXiv:1309.5556]
Original
2013
Earlier work this paper cites.
S. de la Torre et al., The VIMOS Public Extragalactic Redshift Survey (VIPERS). Galaxy clustering and redshift-space distortions at z ≈ 0.8 z\approx 0.8 in the first data release, Astron. Astroph. 557, 54 (2013) [arXiv:1303.2622]
Original
2013
Earlier work this paper cites.
B. Audren, J. Lesgourgues, K. Benabed and S. Prunet, Conservative Constraints on Early Cosmology: an illus- tration of the Monte Python cosmological parameter in- ference code, JCAP 1302, 001 (2013) doi:10.1088/1475- 7516/2013/02/001 [arXiv:1210.7183]
Original
2013
Earlier work this paper cites.

Similar

Then

J. Renk, M. Zumalacárregui, F. Montanari and A. Barreira, Galileon gravity in light of ISW, CMB, BAO and H0 data, JCAP 1710 (2017) 020 [1707.02263]
2017
Later among the works it cites.
E. Di Valentino, A. Melchiorri, E.V. Linder, J. Silk, Constraining Dark Energy Dynamics in Extended Parameter Space, Phys. Rev. D 96, 023523 (2017) [arXiv:1704.00762]
Original
2017
Later among the works it cites.
H. Hildebrandt et al., KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing, Mon. Not. R. Astron. Soc. 465, 1454 (2017) [arXiv:1606.05338]
Original
2017
Later among the works it cites.
S. Joudaki et al., KiDS-450 + 2dFLenS: Cosmological parameter constraints from weak gravitational lensing tomography and overlapping redshift-space galaxy clustering, Mon. Not. R. Astron. Soc. 474, 4894 (2017) [arXiv:1707.06627]
Original
2017
Later among the works it cites.

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2019

Modified Gravity Away from a $\Lambda$CDM Background

Brando, Guilherme, Falciano, Felipe T., Linder, Eric V. et al.

Understand

Within the effective field theory approach to cosmic acceleration, the background expansion can be specified separately from the gravitational modifications.

We explore the impact of modified gravity in a background different from a cosmological constant plus cold dark matter ($\Lambda$CDM) on the stability and cosmological observables, including covariance between gravity and expansion parameters.
In No Slip Gravity the more general background allows more gravitational freedom, including both positive and negative Planck mass running.
We examine the effects on cosmic structure growth, as well as showing that a viable positive integrated Sachs-Wolfe effect crosscorrelation easily arises from this modified gravity theory.

Built on

E.V. Linder, No Run Gravity, JCAP 1907, 034 (2019) [arXiv:1903.02010]
Original
1903
Earlier work this paper cites.
G. W. Horndeski, Second-order scalar-tensor field equations in a four-dimensional space, Int. J. Theor. Phys. 10 (1974) 363
1974
Earlier work this paper cites.
A. Gelman and D. B. Rubin, Inference from Iterative Simulation Using Multiple Sequences, Statist. Sci. 7 (1992) 457
1992
Earlier work this paper cites.
M.J. Francis, G.F. Lewis, E.V. Linder, Power Spectra to 1% Accuracy between Dynamical Dark Energy Cosmologies, Mon. Not. Roy. Astron. Soc. 380, 1079 (2007) [arXiv:0704.0312]
Original
2007
Earlier work this paper cites.
S. Ho, C. Hirata, N. Padmanabhan, U. Seljak and N. Bahcall, Phys. Rev. D 78, 043519 (2008) [arXiv:0801.0642]
Original
2008
Earlier work this paper cites.
C. Deffayet, X. Gao, D. A. Steer and G. Zahariade, From k-essence to generalised Galileons, Phys. Rev. D84 (2011) 064039 [1103.3260]
2011
Earlier work this paper cites.
F. Beutler et al., The 6dF Galaxy Survey: z ≈ 0 z\approx 0 measurements of the growth rate and σ 8 \sigma_{8} , Mon. Not. R. Astron. Soc. 423, 3430 (2012) [arXiv:1204.4725]
Original
2012
Earlier work this paper cites.
C. Blake et al., The WiggleZ Dark Energy Survey: Joint measurements of the expansion and growth history at z < 1 z<1 , Mon. Not. R. Astron. Soc. 425, 405 (2012) [arXiv:1204.3674]
Original
2012
Earlier work this paper cites.
G. Gubitosi, F. Piazza, and F. Vernizzi, The effective field theory of dark energy, J. Cosmol. Astropart. Phys. 02 (2013) 032 [arXiv:1210.0201]
Original
2013
Earlier work this paper cites.
J. K. Bloomfield, E. E. Flanagan, M. Park, and S. Watson, Dark energy or modified gravity? An effective field theory approach, J. Cosmol. Astropart. Phys. 08 (2013) 010 [arXiv:1211.7054]
Original
2013
Earlier work this paper cites.
J. Gleyzes, D. Langlois, F. Piazza, and F. Vernizzi, Essential building blocks of dark energy, J. Cosmol. Astropart. Phys. 08 (2013) 025 [arXiv:1304.4840]
Original
2013
Earlier work this paper cites.
C. Blake et al., Galaxy And Mass Assembly (GAMA): improved cosmic growth measurements using multiple tracers of large-scale structure, Mon. Not. R. Astron. Soc. 436, 3089 (2013) [arXiv:1309.5556]
Original
2013
Earlier work this paper cites.
S. de la Torre et al., The VIMOS Public Extragalactic Redshift Survey (VIPERS). Galaxy clustering and redshift-space distortions at z ≈ 0.8 z\approx 0.8 in the first data release, Astron. Astroph. 557, 54 (2013) [arXiv:1303.2622]
Original
2013
Earlier work this paper cites.
B. Audren, J. Lesgourgues, K. Benabed and S. Prunet, Conservative Constraints on Early Cosmology: an illus- tration of the Monte Python cosmological parameter in- ference code, JCAP 1302, 001 (2013) doi:10.1088/1475- 7516/2013/02/001 [arXiv:1210.7183]
Original
2013
Earlier work this paper cites.

Similar

Then

J. Renk, M. Zumalacárregui, F. Montanari and A. Barreira, Galileon gravity in light of ISW, CMB, BAO and H0 data, JCAP 1710 (2017) 020 [1707.02263]
2017
Later among the works it cites.
E. Di Valentino, A. Melchiorri, E.V. Linder, J. Silk, Constraining Dark Energy Dynamics in Extended Parameter Space, Phys. Rev. D 96, 023523 (2017) [arXiv:1704.00762]
Original
2017
Later among the works it cites.
H. Hildebrandt et al., KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing, Mon. Not. R. Astron. Soc. 465, 1454 (2017) [arXiv:1606.05338]
Original
2017
Later among the works it cites.
S. Joudaki et al., KiDS-450 + 2dFLenS: Cosmological parameter constraints from weak gravitational lensing tomography and overlapping redshift-space galaxy clustering, Mon. Not. R. Astron. Soc. 474, 4894 (2017) [arXiv:1707.06627]
Original
2017
Later among the works it cites.

Beyond the bibliography

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

Open on alphaXiv

alphaXiv is searching for related work…

Original

2015

Cited alongside, same era.

E. V. Linder, G. Sengör and S. Watson, Is the Effective Field Theory of Dark Energy Effective?, JCAP 1605 (2016) 053 [arXiv:1512.06180]

Original

2016

Cited alongside, same era.

J. Renk, M. Zumalacárregui and F. Montanari, Gravity at the horizon: on relativistic effects, CMB-LSS correlations and ultra-large scales in Horndeski’s theory, JCAP 1607 (2016) 040 [1604.03487]

2016

Cited alongside, same era.

N. Aghanim, et al., Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters, Astron. Astrophys. 594 (2016) A11. arXiv:1507.02704, doi:10.1051/0004-6361/201526926

Original

2016

Cited alongside, same era.

P. A. R. Ade, et al., Planck 2015 results. XV. Gravitational lensing, Astron. Astrophys. 594 (2016) A15. arXiv:1502.01591, doi:10.1051/0004-6361/201525941

Original

2016

Cited alongside, same era.

B. Abbott et al. (Virgo, LIGO Scientific), Phys. Rev. Lett. 119, 161101 (2017)

2017