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DES, LIGO Scientific, Virgo
Original
1901
Earlier work this paper cites.
R. Akeson, L. Armus, E. Bachelet, V. Bailey, L. Bartusek, A. Bellini et al., The Wide Field Infrared Survey Telescope: 100 Hubbles for the 2020s , arXiv e-prints (2019) arXiv:1902.05569 [ 1902.05569 ]
Original
1902
Earlier work this paper cites.
A. G. Riess, S. Casertano, W. Yuan, L. M. Macri and D. Scolnic, Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond Λ \Lambda CDM , Astrophys. J. 876
Original
1903
Earlier work this paper cites.
N. Kaloper, Dark Energy, H 0 H_{0} and Weak Gravity Conjecture , Int. J. Mod. Phys. D28
Original
1903
Earlier work this paper cites.
M. Blomqvist et al., Baryon acoustic oscillations from the cross-correlation of Ly α \alpha absorption and quasars in eBOSS DR14 , Astron. Astrophys. 629
Original
1904
Earlier work this paper cites.
P. Agrawal, F.-Y. Cyr-Racine, D. Pinner and L. Randall, Rock ’n’ Roll Solutions to the Hubble Tension , 1904.01016
Original
1904
Earlier work this paper cites.
S. Alexander and E. McDonough, Axion-Dilaton Destabilization and the Hubble Tension , Phys. Lett. B797
Original
1904
Earlier work this paper cites.
M.-X. Lin, G. Benevento, W. Hu and M. Raveri, Acoustic Dark Energy: Potential Conversion of the Hubble Tension , Phys. Rev. D100
Original
1905
Earlier work this paper cites.
H. Kondo, H. Miyatake, M. Shirasaki, N. Sugiyama and A. J. Nishizawa, Weak Lensing Measurement of Filamentary Structure with the SDSS BOSS and Subaru Hyper Suprime-Cam Data , 1905.08991
Original
1905
Earlier work this paper cites.
A. Cuceu, J. Farr, P. Lemos and A. Font-Ribera, Baryon Acoustic Oscillations and the Hubble Constant: Past, Present and Future , JCAP 10
Original
1906
Earlier work this paper cites.
L. Verde, T. Treu and A. G. Riess, Tensions between the Early and the Late Universe , in Nature Astronomy 2019 , 2019, 1907.10625 , DOI
Original
1907
Earlier work this paper cites.
K. C. Wong et al., H0LiCOW XIII. A 2.4% measurement of H 0 H_{0} from lensed quasars: 5.3 σ 5.3\sigma tension between early and late-Universe probes , 1907.04869
Original
1907
Earlier work this paper cites.
N. Schöneberg, J. Lesgourgues and D. C. Hooper, The BAO+BBN take on the Hubble tension , JCAP 10
Original
1907
Earlier work this paper cites.
A. Chudaykin and M. M. Ivanov, Measuring neutrino masses with large-scale structure: Euclid forecast with controlled theoretical error , JCAP 11
Original
1907
Earlier work this paper cites.
Planck Collaboration, N. Aghanim, Y. Akrami, M. Ashdown, J. Aumont, C. Baccigalupi et al., Planck 2018 results. V. CMB power spectra and likelihoods , arXiv e-prints (2019) arXiv:1907.12875 [ 1907.12875 ]
Original
1907
Earlier work this paper cites.
C. D. Huang, A. G. Riess, W. Yuan, L. M. Macri, N. L. Zakamska, S. Casertano et al., Hubble Space Telescope Observations of Mira Variables in the Type Ia Supernova Host NGC 1559: An Alternative Candle to Measure the Hubble Constant , 1908.10883
Original
1908
Earlier work this paper cites.
L. Knox and M. Millea, Hubble constant hunter’s guide , Phys. Rev. D101
Original
1908
Earlier work this paper cites.
T. L. Smith, V. Poulin and M. A. Amin, Oscillating scalar fields and the Hubble tension: a resolution with novel signatures , Phys. Rev. D101
Original
1908
Earlier work this paper cites.
A. Heinesen, C. Blake and D. L. Wiltshire, Quantifying the accuracy of the Alcock-Paczy&nacute;ski scaling of baryon acoustic oscillation measurements , JCAP 2001
Original
1908
Earlier work this paper cites.
M. M. Ivanov, M. Simonović and M. Zaldarriaga, Cosmological Parameters from the BOSS Galaxy Power Spectrum , 1909.05277
Original
1909
Earlier work this paper cites.
G. D’Amico, J. Gleyzes, N. Kokron, D. Markovic, L. Senatore, P. Zhang et al., The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure , 1909.05271
Original
1909
Earlier work this paper cites.
T. Tröster, A. G. Sánchez, M. Asgari, C. Blake, M. Crocce, C. Heymans et al., Cosmology from large-scale structure. Constraining Λ \Lambda CDM with BOSS , A&A 633
Original
1909
Earlier work this paper cites.
T. Colas, G. D’amico, L. Senatore, P. Zhang and F. Beutler, Efficient Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure , 1909.07951
Original
1909
Earlier work this paper cites.
T. Tröster et al., Cosmology from large-scale structure: Constraining Λ \Lambda CDM with BOSS , Astron. Astrophys. 633
Original
1909
Earlier work this paper cites.
F. Niedermann and M. S. Sloth, New Early Dark Energy , 1910.10739
Original
1910
Earlier work this paper cites.
A. Lewis, GetDist: a Python package for analysing Monte Carlo samples , arXiv e-prints (2019) arXiv:1910.13970 [ 1910.13970 ]
Original
1910
Earlier work this paper cites.

Similar

C. S. Kochanek, Over-constrained Gravitational Lens Models and the Hubble Constant , Mon. Not. Roy. Astron. Soc. 493
Original
1911
Cited alongside, same era.
J. Sakstein and M. Trodden, Early dark energy from massive neutrinos – a natural resolution of the Hubble tension , 1911.11760
Original
1911
Cited alongside, same era.
K. V. Berghaus and T. Karwal, Thermal Friction as a Solution to the Hubble Tension , 1911.06281
Original
1911
Cited alongside, same era.
M. M. Ivanov, M. Simonović and M. Zaldarriaga, Cosmological Parameters and Neutrino Masses from the Final Planck and Full-Shape BOSS Data , 1912.08208
Original
1912
Cited alongside, same era.
R. D. Peccei and H. R. Quinn, CP Conservation in the Presence of Instantons , Phys. Rev. Lett. 38

Then

A. Chudaykin, M. M. Ivanov and M. Simonović, CLASS-PT: non-linear perturbation theory extension of the Boltzmann code CLASS , 2004.10607
Original
2004
Later among the works it cites.
A. Chudaykin, D. Gorbunov and N. Nedelko, Combined analysis of Planck and SPTPol data favors the early dark energy models , 2004.13046
Original
2004
Later among the works it cites.
R. M. Neal, Taking Bigger Metropolis Steps by Dragging Fast Variables , arXiv Mathematics e-prints (2005) math/0502099 [ math/0502099 ]
2005
Later among the works it cites.
F. Niedermann and M. S. Sloth, Resolving the Hubble Tension with New Early Dark Energy , 2006.06686
Original
2006
Later among the works it cites.
S. Birrer, A. J. Shajib, A. Galan, M. Millon, T. Treu, A. Agnello et al., TDCOSMO IV: Hierarchical time-delay cosmography – joint inference of the Hubble constant and galaxy density profiles , arXiv e-prints (2020) arXiv:2007.02941 [ 2007.02941 ]

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2020

Constraining Early Dark Energy with Large-Scale Structure

Ivanov, Mikhail M., McDonough, Evan, Hill, J. Colin et al.

Understand

An axion-like field comprising $\sim 10\%$ of the energy density of the universe near matter-radiation equality is a candidate to resolve the Hubble tension; this is the "early dark energy" (EDE) model.

However, as shown in Hill et al.
(2020), the model fails to simultaneously resolve the Hubble tension and maintain a good fit to both cosmic microwave background (CMB) and large-scale structure (LSS) data.
Here, we use redshift-space galaxy clustering data to sharpen constraints on the EDE model.