Built on

R. Jimenez, A. Cimatti, L. Verde, M. Moresco, and B. Wandelt, The local and distant Universe: stellar ages and H 0 H_{0}
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
Original
1903
Earlier work this paper cites.
P. Agrawal, F.-Y. Cyr-Racine, D. Pinner, and L. Randall, Rock ’n’ Roll Solutions to the Hubble Tension
Original
1904
Earlier work this paper cites.
S. Alexander and E. McDonough, Axion-Dilaton Destabilization and the Hubble Tension
Original
1904
Earlier work this paper cites.
I. n. Zubeldia and A. Challinor, Cosmological constraints from Planck galaxy clusters with CMB lensing mass bias calibration
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
Original
1905
Earlier work this paper cites.
W. L. K. Wu et al., A Measurement of the Cosmic Microwave Background Lensing Potential and Power Spectrum from 500 deg 2 of SPTpol Temperature and Polarization Data
Original
1905
Earlier work this paper cites.
L. Verde, T. Treu, and A. G. Riess, Tensions between the Early and the Late Universe
Original
1907
Earlier work this paper cites.
L. Visinelli, S. Vagnozzi, and U. Danielsson, Revisiting a negative cosmological constant from low-redshift data
Original
1907
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
Original
1908
Earlier work this paper cites.
L. Knox and M. Millea, Hubble constant hunter’s guide
Original
1908
Earlier work this paper cites.
F. Niedermann and M. S. Sloth, New early dark energy
Original
1910
Earlier work this paper cites.
A. Lewis, GetDist: a Python package for analysing Monte Carlo samples
Original
1910
Earlier work this paper cites.
M. Asgari et al., KiDS+VIKING-450 and DES-Y1 combined: Mitigating baryon feedback uncertainty with COSEBIs
Original
1910
Earlier work this paper cites.
J. Sakstein and M. Trodden, Early Dark Energy from Massive Neutrinos as a Natural Resolution of the Hubble Tension
Original
1911
Earlier work this paper cites.
H.-H. Li, G. Ye, Y. Cai, and Y.-S. Piao, Trans-Planckian censorship of multistage inflation and dark energy
Original
1911
Earlier work this paper cites.
P. Motloch and W. Hu, Lensinglike tensions in the P l a n c k Planck legacy release
Original
1912
Earlier work this paper cites.
J. M. Maldacena, The Large N limit of superconformal field theories and supergravity
1998
Earlier work this paper cites.
R. Bousso and J. Polchinski, Quantization of four form fluxes and dynamical neutralization of the cosmological constant
2000
Earlier work this paper cites.
A. G. Riess, The Expansion of the Universe is Faster than Expected
Original
2001
Earlier work this paper cites.
G. Ye and Y.-S. Piao, Is the Hubble tension a hint of AdS phase around recombination?
Original
2001
Earlier work this paper cites.
M.-Z. Lyu, B. S. Haridasu, M. Viel, and J.-Q. Xia, H 0 H_{0} Reconstruction with Type Ia Supernovae, Baryon Acoustic Oscillation and Gravitational Lensing Time-Delay
Original
2001
Earlier work this paper cites.
M. Zumalacarregui, Gravity in the Era of Equality: Towards solutions to the Hubble problem without fine-tuned initial conditions
Original
2003
Earlier work this paper cites.
J. C. Hill, E. McDonough, M. W. Toomey, and S. Alexander, Early dark energy does not restore cosmological concordance
Original
2003
Earlier work this paper cites.
VIRGO Consortium
2003
Earlier work this paper cites.
G. D’Amico, L. Senatore, and P. Zhang, Limits on w w CDM from the EFTofLSS with the PyBird code
Original
2003
Earlier work this paper cites.
A. Chudaykin, D. Gorbunov, and N. Nedelko, Combined analysis of Planck and SPTPol data favors the early dark energy models
Original
2004
Earlier work this paper cites.
Y.-S. Piao, Can the universe experience many cycles with different vacua?
2004
Earlier work this paper cites.

Similar

M. Braglia, W. T. Emond, F. Finelli, A. E. Gumrukcuoglu, and K. Koyama, Unified framework for early dark energy from α \alpha -attractors
Original
2005
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Ruchika, K. Dutta, A. Mukherjee, and A. A. Sen, Observational Constraints on Axion(s) with a Cosmological Constant
Original
2005
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M. M. Ivanov, E. McDonough, J. C. Hill, M. Simonović, M. W. Toomey, S. Alexander, and M. Zaldarriaga, Constraining Early Dark Energy with Large-Scale Structure
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2006
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2006
Cited alongside, same era.
C. Heymans et al., KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints

Then

J. L. Bernal, L. Verde, and A. G. Riess, The trouble with H 0 H_{0}
Original
2016
Later among the works it cites.
M. Moresco, L. Pozzetti, A. Cimatti, R. Jimenez, C. Maraston, L. Verde, D. Thomas, A. Citro, R. Tojeiro, and D. Wilkinson, A 6% measurement of the Hubble parameter at z ∼ 0.45 z\sim 0.45 : direct evidence of the epoch of cosmic re-acceleration
Original
2016
Later among the works it cites.
H. Gil-Marín et al., The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies
Original
2016
Later among the works it cites.
Y. Cai, Y. Wan, H.-G. Li, T. Qiu, and Y.-S. Piao, The Effective Field Theory of nonsingular cosmology
Original
2017
Later among the works it cites.

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2021

Testing AdS early dark energy with Planck, SPTpol and LSS data

Jiang, Jun-Qian, Piao, Yun-Song

Understand

The Hubble tension might be resolved by injecting a new energy component, called Early Dark Energy (EDE), prior to recombination.

An Anti-de Sitter (AdS) phase around recombination can make the injected energy decay faster, which thus allows a higher EDE fraction (so larger $H_0$) while prevents degrading the CMB fit.
In this work, we test the AdS-EDE model with CMB and Large-Scale Structure (LSS) data.
Our CMB dataset consists of low-$\ell$ part of Planck TT spectrum and SPTpol polarization and lensing measurements, since this dataset predicts the CMB lensing effect consistent with $\Lambda$CDM expectation.

Built on

R. Jimenez, A. Cimatti, L. Verde, M. Moresco, and B. Wandelt, The local and distant Universe: stellar ages and H 0 H_{0}
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
Original
1903
Earlier work this paper cites.
P. Agrawal, F.-Y. Cyr-Racine, D. Pinner, and L. Randall, Rock ’n’ Roll Solutions to the Hubble Tension
Original
1904
Earlier work this paper cites.
S. Alexander and E. McDonough, Axion-Dilaton Destabilization and the Hubble Tension
Original
1904
Earlier work this paper cites.
I. n. Zubeldia and A. Challinor, Cosmological constraints from Planck galaxy clusters with CMB lensing mass bias calibration
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
Original
1905
Earlier work this paper cites.
W. L. K. Wu et al., A Measurement of the Cosmic Microwave Background Lensing Potential and Power Spectrum from 500 deg 2 of SPTpol Temperature and Polarization Data
Original
1905
Earlier work this paper cites.
L. Verde, T. Treu, and A. G. Riess, Tensions between the Early and the Late Universe
Original
1907
Earlier work this paper cites.
L. Visinelli, S. Vagnozzi, and U. Danielsson, Revisiting a negative cosmological constant from low-redshift data
Original
1907
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
Original
1908
Earlier work this paper cites.
L. Knox and M. Millea, Hubble constant hunter’s guide
Original
1908
Earlier work this paper cites.
F. Niedermann and M. S. Sloth, New early dark energy
Original
1910
Earlier work this paper cites.
A. Lewis, GetDist: a Python package for analysing Monte Carlo samples
Original
1910
Earlier work this paper cites.
M. Asgari et al., KiDS+VIKING-450 and DES-Y1 combined: Mitigating baryon feedback uncertainty with COSEBIs
Original
1910
Earlier work this paper cites.
J. Sakstein and M. Trodden, Early Dark Energy from Massive Neutrinos as a Natural Resolution of the Hubble Tension
Original
1911
Earlier work this paper cites.
H.-H. Li, G. Ye, Y. Cai, and Y.-S. Piao, Trans-Planckian censorship of multistage inflation and dark energy
Original
1911
Earlier work this paper cites.
P. Motloch and W. Hu, Lensinglike tensions in the P l a n c k Planck legacy release
Original
1912
Earlier work this paper cites.
J. M. Maldacena, The Large N limit of superconformal field theories and supergravity
1998
Earlier work this paper cites.
R. Bousso and J. Polchinski, Quantization of four form fluxes and dynamical neutralization of the cosmological constant
2000
Earlier work this paper cites.
A. G. Riess, The Expansion of the Universe is Faster than Expected
Original
2001
Earlier work this paper cites.
G. Ye and Y.-S. Piao, Is the Hubble tension a hint of AdS phase around recombination?
Original
2001
Earlier work this paper cites.
M.-Z. Lyu, B. S. Haridasu, M. Viel, and J.-Q. Xia, H 0 H_{0} Reconstruction with Type Ia Supernovae, Baryon Acoustic Oscillation and Gravitational Lensing Time-Delay
Original
2001
Earlier work this paper cites.
M. Zumalacarregui, Gravity in the Era of Equality: Towards solutions to the Hubble problem without fine-tuned initial conditions
Original
2003
Earlier work this paper cites.
J. C. Hill, E. McDonough, M. W. Toomey, and S. Alexander, Early dark energy does not restore cosmological concordance
Original
2003
Earlier work this paper cites.
VIRGO Consortium
2003
Earlier work this paper cites.
G. D’Amico, L. Senatore, and P. Zhang, Limits on w w CDM from the EFTofLSS with the PyBird code
Original
2003
Earlier work this paper cites.
A. Chudaykin, D. Gorbunov, and N. Nedelko, Combined analysis of Planck and SPTPol data favors the early dark energy models
Original
2004
Earlier work this paper cites.
Y.-S. Piao, Can the universe experience many cycles with different vacua?
2004
Earlier work this paper cites.

Similar

M. Braglia, W. T. Emond, F. Finelli, A. E. Gumrukcuoglu, and K. Koyama, Unified framework for early dark energy from α \alpha -attractors
Original
2005
Cited alongside, same era.
Ruchika, K. Dutta, A. Mukherjee, and A. A. Sen, Observational Constraints on Axion(s) with a Cosmological Constant
Original
2005
Cited alongside, same era.
M. M. Ivanov, E. McDonough, J. C. Hill, M. Simonović, M. W. Toomey, S. Alexander, and M. Zaldarriaga, Constraining Early Dark Energy with Large-Scale Structure
Original
2006
Cited alongside, same era.
G. D’Amico, L. Senatore, P. Zhang, and H. Zheng, The Hubble Tension in Light of the Full-Shape Analysis of Large-Scale Structure Data
Original
2006
Cited alongside, same era.
C. Heymans et al., KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints

Then

J. L. Bernal, L. Verde, and A. G. Riess, The trouble with H 0 H_{0}
Original
2016
Later among the works it cites.
M. Moresco, L. Pozzetti, A. Cimatti, R. Jimenez, C. Maraston, L. Verde, D. Thomas, A. Citro, R. Tojeiro, and D. Wilkinson, A 6% measurement of the Hubble parameter at z ∼ 0.45 z\sim 0.45 : direct evidence of the epoch of cosmic re-acceleration
Original
2016
Later among the works it cites.
H. Gil-Marín et al., The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies
Original
2016
Later among the works it cites.
Y. Cai, Y. Wan, H.-G. Li, T. Qiu, and Y.-S. Piao, The Effective Field Theory of nonsingular cosmology
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

2007

Cited alongside, same era.

H. Ooguri and C. Vafa, On the Geometry of the String Landscape and the Swampland

2007

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E. Di Valentino et al., Snowmass2021 - Letter of interest cosmology intertwined II: The hubble constant tension

Original

2008

Cited alongside, same era.

G. Ye and Y.-S. Piao, T 0 T_{0} censorship of early dark energy and AdS vacua

Original

2008

Cited alongside, same era.

R. Calderón, R. Gannouji, B. L’Huillier, and D. Polarski, Negative cosmological constant in the dark sector?

Original

2008

Cited alongside, same era.

M.-X. Lin, W. Hu, and M. Raveri, Testing H 0 H_{0} in Acoustic Dark Energy with Planck and ACT Polarization

Original

2009

Cited alongside, same era.

R. Murgia, G. F. Abellán, and V. Poulin, Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies

Original

2009

Cited alongside, same era.

T. L. Smith, V. Poulin, J. L. Bernal, K. K. Boddy, M. Kamionkowski, and R. Murgia, Early dark energy is not excluded by current large-scale structure data

Original

2009

Cited alongside, same era.

S. Vagnozzi, E. Giusarma, O. Mena, K. Freese, M. Gerbino, S. Ho, and M. Lattanzi, Unveiling ν \nu secrets with cosmological data: neutrino masses and mass hierarchy

Original

2017

Later among the works it cites.

D. M. Scolnic et al., The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample

Original

2018

Later among the works it cites.

L. Amendola et al., Cosmology and fundamental physics with the Euclid satellite

Original

2018

Later among the works it cites.

V. Poulin, T. L. Smith, T. Karwal, and M. Kamionkowski, Early Dark Energy Can Resolve The Hubble Tension