Built on

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.
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.
D. Grin, M. A. Amin, V. Gluscevic, R. Hlǒzek, D. J. E. Marsh, V. Poulin et al., Gravitational probes of ultra-light axions , 1904.09003
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.
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.
K. Abazajian, G. Addison, P. Adshead, Z. Ahmed, S. W. Allen, D. Alonso et al., CMB-S4 Science Case, Reference Design, and Project Plan , arXiv e-prints (2019) arXiv:1907.04473 [ 1907.04473 ]
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.
J. Sakstein, H. Desmond and B. Jain, Screened Fifth Forces Mediated by Dark Matter–Baryon Interactions: Theory and Astrophysical Probes , Phys. Rev. D100
Original
1907
Earlier work this paper cites.
H. Desmond, B. Jain and J. Sakstein, Local resolution of the Hubble tension: The impact of screened fifth forces on the cosmic distance ladder , Phys. Rev. D100
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.
K. Dutta, A. Roy, Ruchika, A. A. Sen and M. M. Sheikh-Jabbari, Cosmology with low-redshift observations: No signal for new physics , Phys. Rev. D100
Original
1908
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.
J. Halverson, C. Long, B. Nelson and G. Salinas, Towards string theory expectations for photon couplings to axionlike particles , Phys. Rev. D100
Original
1909
Earlier work this paper cites.
L. M. Capparelli, R. R. Caldwell and A. Melchiorri, Cosmic Birefringence Test of the Hubble Tension , 1909.04621
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.
P. Lemos, F. Köhlinger, W. Handley, B. Joachimi, L. Whiteway and O. Lahav, Quantifying Suspiciousness Within Correlated Data Sets , 1910.07820
Original
1910
Earlier work this paper cites.
C. S. Kochanek, Over-constrained Gravitational Lens Models and the Hubble Constant , Mon. Not. Roy. Astron. Soc. 493
Original
1911
Earlier work this paper cites.
J. Sakstein and M. Trodden, Early dark energy from massive neutrinos – a natural resolution of the Hubble tension , 1911.11760
Original
1911
Earlier work this paper cites.
K. V. Berghaus and T. Karwal, Thermal Friction as a Solution to the Hubble Tension , 1911.06281
Original
1911
Earlier work this paper cites.
S. Alexander, E. McDonough, A. Pullen and B. Shapiro, Physics Beyond The Standard Model with Circular Polarization in the CMB and CMB-21cm Cross-Correlation , JCAP 2001
Original
1911
Earlier work this paper cites.
I. L. Padilla et al., Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: A Measurement of Circular Polarization at 40 GHz , 1911.00391
Original
1911
Earlier work this paper cites.
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
Earlier work this paper cites.
M. Raveri, G. Zacharegkas and W. Hu, Quantifying concordance of correlated cosmological data sets , 1912.04880
Original
1912
Earlier work this paper cites.

Similar

R. D. Peccei and H. R. Quinn, CP Conservation in the Presence of Instantons , Phys. Rev. Lett. 38
1977
Cited alongside, same era.
F. Wilczek, Problem of Strong P P and T T Invariance in the Presence of Instantons , Phys. Rev. Lett. 40
1978
Cited alongside, same era.
S. Weinberg, A New Light Boson? , Phys. Rev. Lett. 40
1978
Cited alongside, same era.
M. S. Turner, Coherent scalar-field oscillations in an expanding universe , Phys. Rev. D 28
1983
Cited alongside, same era.
N. Kaiser, Clustering in real space and in redshift space , MNRAS 227
1987
Cited alongside, same era.
A. Gelman and D. B. Rubin, Inference from Iterative Simulation Using Multiple Sequences , Statist. Sci. 7
1992
Cited alongside, same era.

Then

M. Montero, A. M. Uranga and I. Valenzuela, Transplanckian axions!? , JHEP 08
Original
2015
Later among the works it cites.
T. Rudelius, Constraints on Axion Inflation from the Weak Gravity Conjecture , JCAP 1509
Original
2015
Later among the works it cites.
T. Rudelius, On the Possibility of Large Axion Moduli Spaces , JCAP 1504
Original
2015
Later among the works it cites.
A. J. Ross, L. Samushia, C. Howlett, W. J. Percival, A. Burden and M. Manera, The clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at z = 0.15 z=0.15 , Mon. Not. Roy. Astron. Soc. 449
Original
2015
Later among the works it cites.
A. B. Mantz, A. von der Linden, S. W. Allen, D. E. Applegate, P. L. Kelly, R. G. Morris et al., Weighing the giants - IV. Cosmology and neutrino mass , MNRAS 446

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Reading the bibliography…

2020

Early Dark Energy Does Not Restore Cosmological Concordance

Hill, J. Colin, McDonough, Evan, Toomey, Michael W. et al.

Understand

Current cosmological data exhibit a tension between inferences of the Hubble constant, $H_0$, derived from early and late-universe measurements.

One proposed solution is to introduce a new component in the early universe, which initially acts as "early dark energy" (EDE), thus decreasing the physical size of the sound horizon imprinted in the cosmic microwave background (CMB) and increasing the inferred $H_0$.
Previous EDE analyses have shown this model can relax the $H_0$ tension, but the CMB-preferred value of the density fluctuation amplitude, $\sigma_8$, increases in EDE as compared to $\Lambda$CDM, increasing tension with large-scale structure (LSS) data.
We show that the EDE model fit to CMB and SH0ES data yields scale-dependent changes in the matter power spectrum compared to $\Lambda$CDM, including $10\%$ more power at $k = 1~h$/Mpc.

Built on

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.
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.
D. Grin, M. A. Amin, V. Gluscevic, R. Hlǒzek, D. J. E. Marsh, V. Poulin et al., Gravitational probes of ultra-light axions , 1904.09003
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.
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.
K. Abazajian, G. Addison, P. Adshead, Z. Ahmed, S. W. Allen, D. Alonso et al., CMB-S4 Science Case, Reference Design, and Project Plan , arXiv e-prints (2019) arXiv:1907.04473 [ 1907.04473 ]
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.
J. Sakstein, H. Desmond and B. Jain, Screened Fifth Forces Mediated by Dark Matter–Baryon Interactions: Theory and Astrophysical Probes , Phys. Rev. D100
Original
1907
Earlier work this paper cites.
H. Desmond, B. Jain and J. Sakstein, Local resolution of the Hubble tension: The impact of screened fifth forces on the cosmic distance ladder , Phys. Rev. D100
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.
K. Dutta, A. Roy, Ruchika, A. A. Sen and M. M. Sheikh-Jabbari, Cosmology with low-redshift observations: No signal for new physics , Phys. Rev. D100
Original
1908
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.
J. Halverson, C. Long, B. Nelson and G. Salinas, Towards string theory expectations for photon couplings to axionlike particles , Phys. Rev. D100
Original
1909
Earlier work this paper cites.
L. M. Capparelli, R. R. Caldwell and A. Melchiorri, Cosmic Birefringence Test of the Hubble Tension , 1909.04621
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.
P. Lemos, F. Köhlinger, W. Handley, B. Joachimi, L. Whiteway and O. Lahav, Quantifying Suspiciousness Within Correlated Data Sets , 1910.07820
Original
1910
Earlier work this paper cites.
C. S. Kochanek, Over-constrained Gravitational Lens Models and the Hubble Constant , Mon. Not. Roy. Astron. Soc. 493
Original
1911
Earlier work this paper cites.
J. Sakstein and M. Trodden, Early dark energy from massive neutrinos – a natural resolution of the Hubble tension , 1911.11760
Original
1911
Earlier work this paper cites.
K. V. Berghaus and T. Karwal, Thermal Friction as a Solution to the Hubble Tension , 1911.06281
Original
1911
Earlier work this paper cites.
S. Alexander, E. McDonough, A. Pullen and B. Shapiro, Physics Beyond The Standard Model with Circular Polarization in the CMB and CMB-21cm Cross-Correlation , JCAP 2001
Original
1911
Earlier work this paper cites.
I. L. Padilla et al., Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: A Measurement of Circular Polarization at 40 GHz , 1911.00391
Original
1911
Earlier work this paper cites.
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
Earlier work this paper cites.
M. Raveri, G. Zacharegkas and W. Hu, Quantifying concordance of correlated cosmological data sets , 1912.04880
Original
1912
Earlier work this paper cites.

Similar

R. D. Peccei and H. R. Quinn, CP Conservation in the Presence of Instantons , Phys. Rev. Lett. 38
1977
Cited alongside, same era.
F. Wilczek, Problem of Strong P P and T T Invariance in the Presence of Instantons , Phys. Rev. Lett. 40
1978
Cited alongside, same era.
S. Weinberg, A New Light Boson? , Phys. Rev. Lett. 40
1978
Cited alongside, same era.
M. S. Turner, Coherent scalar-field oscillations in an expanding universe , Phys. Rev. D 28
1983
Cited alongside, same era.
N. Kaiser, Clustering in real space and in redshift space , MNRAS 227
1987
Cited alongside, same era.
A. Gelman and D. B. Rubin, Inference from Iterative Simulation Using Multiple Sequences , Statist. Sci. 7
1992
Cited alongside, same era.

Then

M. Montero, A. M. Uranga and I. Valenzuela, Transplanckian axions!? , JHEP 08
Original
2015
Later among the works it cites.
T. Rudelius, Constraints on Axion Inflation from the Weak Gravity Conjecture , JCAP 1509
Original
2015
Later among the works it cites.
T. Rudelius, On the Possibility of Large Axion Moduli Spaces , JCAP 1504
Original
2015
Later among the works it cites.
A. J. Ross, L. Samushia, C. Howlett, W. J. Percival, A. Burden and M. Manera, The clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at z = 0.15 z=0.15 , Mon. Not. Roy. Astron. Soc. 449
Original
2015
Later among the works it cites.
A. B. Mantz, A. von der Linden, S. W. Allen, D. E. Applegate, P. L. Kelly, R. G. Morris et al., Weighing the giants - IV. Cosmology and neutrino mass , MNRAS 446

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. J. Fixsen, E. S. Cheng, J. M. Gales, J. C. Mather, R. A. Shafer and E. L. Wright, The Cosmic Microwave Background Spectrum from the Full COBE FIRAS Data Set , ApJ 473

1996

Cited alongside, same era.

K. Blum, E. Castorina and M. Simonović, Could quasar lensing time delays hint to cored dark matter halos, instead of H 0 H_{0} tension? , 2001.07182

Original

2001

Cited alongside, same era.

D. W. Pesce et al., The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints , Astrophys. J. 891

Original

2001

Cited alongside, same era.

W. L. Freedman, B. F. Madore, T. Hoyt, I. S. Jang, R. Beaton, M. G. Lee et al., Calibration of the Tip of the Red Giant Branch (TRGB) , 2002.01550

Original