Built on

K. L. Pandey, T. Karwal, and S. Das, Alleviating the H 0 H_{0} and σ 8 \sigma_{8} anomalies with a decaying dark matter model, JCAP 07
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.
P. Agrawal, F.-Y. Cyr-Racine, D. Pinner, and L. Randall, Rock ’n’ Roll Solutions to the Hubble Tension (2019), arXiv:1904.01016 [astro-ph.CO]
Original
1904
Earlier work this paper cites.
D. Hooper, G. Krnjaic, and S. D. McDermott, Dark Radiation and Superheavy Dark Matter from Black Hole Domination, JHEP 08
Original
1905
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. D 100
Original
1905
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.
K. C. Wong et al. , H0LiCOW – XIII. A 2.4 per cent measurement of H0 from lensed quasars: 5.3 σ \sigma tension between early- and late-Universe probes, Mon. Not. Roy. Astron. Soc. 498
Original
1907
Earlier work this paper cites.
W. L. Freedman et al. , The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch (2019), arXiv:1907.05922 [astro-ph.CO]
Original
1907
Earlier work this paper cites.
L. Verde, T. Treu, and A. Riess, Tensions between the Early and the Late Universe (2019) arXiv:1907.10625 [astro-ph.CO]
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. D 100
Original
1907
Earlier work this paper cites.
N. Aghanim et al. (Planck), Planck 2018 results. V. CMB power spectra and likelihoods, Astron. Astrophys. 641
Original
1907
Earlier work this paper cites.
C. D. Huang, A. G. Riess, W. Yuan, L. M. Macri, N. L. Zakamska, S. Casertano, P. A. Whitelock, S. L. Hoffmann, A. V. Filippenko, and D. Scolnic, Hubble Space Telescope Observations of Mira Variables in the Type Ia Supernova Host NGC 1559: An Alternative Candle to Measure the Hubble Constant (2019), arXiv:1908.10883 [astro-ph.CO]
Original
1908
Earlier work this paper cites.
L. Knox and M. Millea, Hubble constant hunter’s guide, Phys. Rev. D 101
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. D 101
Original
1908
Earlier work this paper cites.
M. Escudero and S. J. Witte, A CMB search for the neutrino mass mechanism and its relation to the Hubble tension, Eur. Phys. J. C 80
Original
1909
Earlier work this paper cites.
J. Sakstein and M. Trodden, Early Dark Energy from Massive Neutrinos as a Natural Resolution of the Hubble Tension, Phys. Rev. Lett. 124
Original
1911
Earlier work this paper cites.
J. Alcaniz, N. Bernal, A. Masiero, and F. S. Queiroz, Light Dark Matter: A Common Solution to the Lithium and H 0 {H_{0}} Problems (2019), arXiv:1912.05563 [astro-ph.CO]
Original
1912
Earlier work this paper cites.
P. Motloch and W. Hu, Lensinglike tensions in the P l a n c k Planck legacy release, Phys. Rev. D 101
Original
1912
Earlier work this paper cites.
S. Weinberg, Goldstone Bosons as Fractional Cosmic Neutrinos, Phys. Rev. Lett. 110
Original
1971
Earlier work this paper cites.
F. Lucchin and S. Matarrese, Power Law Inflation, Phys. Rev. D 32
1985
Earlier work this paper cites.
J. Halliwell, Scalar Fields in Cosmology with an Exponential Potential, Phys. Lett. B 185
1987
Earlier work this paper cites.
Q. Shafi and C. Wetterich, Inflation From Higher Dimensions, Nucl. Phys. B 289
1987
Earlier work this paper cites.
B. Ratra and P. Peebles, Cosmological Consequences of a Rolling Homogeneous Scalar Field, Phys. Rev. D 37
1988
Earlier work this paper cites.
A. Burd and J. D. Barrow, Inflationary Models with Exponential Potentials, Nucl. Phys. B 308
1989
Earlier work this paper cites.
A. Gelman and D. B. Rubin, Inference from Iterative Simulation Using Multiple Sequences, Statist. Sci. 7
1992
Earlier work this paper cites.
C. Wetterich, An asymptotically vanishing time dependent cosmological ’constant’, Astron. Astrophys. 301
1995
Earlier work this paper cites.
C.-P. Ma and E. Bertschinger, Cosmological perturbation theory in the synchronous and conformal Newtonian gauges, Astrophys. J. 455
1995
Earlier work this paper cites.
P. G. Ferreira and M. Joyce, Cosmology with a primordial scaling field, Phys. Rev. D 58
1998
Earlier work this paper cites.
E. J. Copeland, A. R. Liddle, and D. Wands, Exponential potentials and cosmological scaling solutions, Phys. Rev. D 57
1998
Earlier work this paper cites.
P. J. Steinhardt, L.-M. Wang, and I. Zlatev, Cosmological tracking solutions, Phys. Rev. D 59
1999
Earlier work this paper cites.
A. Lewis, A. Challinor, and A. Lasenby, Efficient computation of CMB anisotropies in closed FRW models, Astrophys. J. 538
2000
Earlier work this paper cites.

Similar

R. R. Caldwell, An introduction to quintessence, Braz. J. Phys. 30
2000
Cited alongside, same era.
D. Pesce et al. , The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints, Astrophys. J. Lett. 891
Original
2001
Cited alongside, same era.
G. Ye and Y.-S. Piao, Is the Hubble tension a hint of AdS phase around recombination?, Phys. Rev. D 101
Original
2001
Cited alongside, same era.
O. H. Philcox, M. M. Ivanov, M. Simonović, and M. Zaldarriaga, Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0, JCAP 05
Original
2002
Cited alongside, same era.
G. Benevento, W. Hu, and M. Raveri, Can Late Dark Energy Transitions Raise the Hubble constant?, Phys. Rev. D 101
Original

Then

E. Di Valentino, A. Melchiorri, and J. Silk, Reconciling Planck with the local value of H 0 H_{0} in extended parameter space, Phys. Lett. B 761
Original
2016
Later among the works it cites.
S. Kumar and R. C. Nunes, Probing the interaction between dark matter and dark energy in the presence of massive neutrinos, Phys. Rev. D 94
Original
2016
Later among the works it cites.
J. L. Bernal, L. Verde, and A. G. Riess, The trouble with H 0 H_{0} , JCAP 10
Original
2016
Later among the works it cites.
J. Lesgourgues, G. Marques-Tavares, and M. Schmaltz, Evidence for dark matter interactions in cosmological precision data?, JCAP 02
Original
2016
Later among the works it cites.
T. Karwal and M. Kamionkowski, Dark energy at early times, the Hubble parameter, and the string axiverse, Phys. Rev. D 94

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2021

No H_0 Assistance from Assisted Quintessence

Sabla, Vivian I., Caldwell, Robert R.

Understand

Early dark energy, as a proposed solution to the Hubble tension, faces an additional "why now" problem.

Why should dark energy emerge just prior to recombination, billions of years before the onset of cosmic acceleration? Assisted quintessence explains this connection by positing that multiple scaling fields build up over time to drive the present-day cosmic acceleration.
In this framework, early dark energy is inevitable.
Yet, we show that scaling also leads to the demise of the scenario: the same feature that solves the coincidence problem then spoils a concordance of the Hubble constant inferred from the cosmic microwave background with that from the local distance ladder.

Built on

K. L. Pandey, T. Karwal, and S. Das, Alleviating the H 0 H_{0} and σ 8 \sigma_{8} anomalies with a decaying dark matter model, JCAP 07
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.
P. Agrawal, F.-Y. Cyr-Racine, D. Pinner, and L. Randall, Rock ’n’ Roll Solutions to the Hubble Tension (2019), arXiv:1904.01016 [astro-ph.CO]
Original
1904
Earlier work this paper cites.
D. Hooper, G. Krnjaic, and S. D. McDermott, Dark Radiation and Superheavy Dark Matter from Black Hole Domination, JHEP 08
Original
1905
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. D 100
Original
1905
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.
K. C. Wong et al. , H0LiCOW – XIII. A 2.4 per cent measurement of H0 from lensed quasars: 5.3 σ \sigma tension between early- and late-Universe probes, Mon. Not. Roy. Astron. Soc. 498
Original
1907
Earlier work this paper cites.
W. L. Freedman et al. , The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch (2019), arXiv:1907.05922 [astro-ph.CO]
Original
1907
Earlier work this paper cites.
L. Verde, T. Treu, and A. Riess, Tensions between the Early and the Late Universe (2019) arXiv:1907.10625 [astro-ph.CO]
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. D 100
Original
1907
Earlier work this paper cites.
N. Aghanim et al. (Planck), Planck 2018 results. V. CMB power spectra and likelihoods, Astron. Astrophys. 641
Original
1907
Earlier work this paper cites.
C. D. Huang, A. G. Riess, W. Yuan, L. M. Macri, N. L. Zakamska, S. Casertano, P. A. Whitelock, S. L. Hoffmann, A. V. Filippenko, and D. Scolnic, Hubble Space Telescope Observations of Mira Variables in the Type Ia Supernova Host NGC 1559: An Alternative Candle to Measure the Hubble Constant (2019), arXiv:1908.10883 [astro-ph.CO]
Original
1908
Earlier work this paper cites.
L. Knox and M. Millea, Hubble constant hunter’s guide, Phys. Rev. D 101
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. D 101
Original
1908
Earlier work this paper cites.
M. Escudero and S. J. Witte, A CMB search for the neutrino mass mechanism and its relation to the Hubble tension, Eur. Phys. J. C 80
Original
1909
Earlier work this paper cites.
J. Sakstein and M. Trodden, Early Dark Energy from Massive Neutrinos as a Natural Resolution of the Hubble Tension, Phys. Rev. Lett. 124
Original
1911
Earlier work this paper cites.
J. Alcaniz, N. Bernal, A. Masiero, and F. S. Queiroz, Light Dark Matter: A Common Solution to the Lithium and H 0 {H_{0}} Problems (2019), arXiv:1912.05563 [astro-ph.CO]
Original
1912
Earlier work this paper cites.
P. Motloch and W. Hu, Lensinglike tensions in the P l a n c k Planck legacy release, Phys. Rev. D 101
Original
1912
Earlier work this paper cites.
S. Weinberg, Goldstone Bosons as Fractional Cosmic Neutrinos, Phys. Rev. Lett. 110
Original
1971
Earlier work this paper cites.
F. Lucchin and S. Matarrese, Power Law Inflation, Phys. Rev. D 32
1985
Earlier work this paper cites.
J. Halliwell, Scalar Fields in Cosmology with an Exponential Potential, Phys. Lett. B 185
1987
Earlier work this paper cites.
Q. Shafi and C. Wetterich, Inflation From Higher Dimensions, Nucl. Phys. B 289
1987
Earlier work this paper cites.
B. Ratra and P. Peebles, Cosmological Consequences of a Rolling Homogeneous Scalar Field, Phys. Rev. D 37
1988
Earlier work this paper cites.
A. Burd and J. D. Barrow, Inflationary Models with Exponential Potentials, Nucl. Phys. B 308
1989
Earlier work this paper cites.
A. Gelman and D. B. Rubin, Inference from Iterative Simulation Using Multiple Sequences, Statist. Sci. 7
1992
Earlier work this paper cites.
C. Wetterich, An asymptotically vanishing time dependent cosmological ’constant’, Astron. Astrophys. 301
1995
Earlier work this paper cites.
C.-P. Ma and E. Bertschinger, Cosmological perturbation theory in the synchronous and conformal Newtonian gauges, Astrophys. J. 455
1995
Earlier work this paper cites.
P. G. Ferreira and M. Joyce, Cosmology with a primordial scaling field, Phys. Rev. D 58
1998
Earlier work this paper cites.
E. J. Copeland, A. R. Liddle, and D. Wands, Exponential potentials and cosmological scaling solutions, Phys. Rev. D 57
1998
Earlier work this paper cites.
P. J. Steinhardt, L.-M. Wang, and I. Zlatev, Cosmological tracking solutions, Phys. Rev. D 59
1999
Earlier work this paper cites.
A. Lewis, A. Challinor, and A. Lasenby, Efficient computation of CMB anisotropies in closed FRW models, Astrophys. J. 538
2000
Earlier work this paper cites.

Similar

R. R. Caldwell, An introduction to quintessence, Braz. J. Phys. 30
2000
Cited alongside, same era.
D. Pesce et al. , The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints, Astrophys. J. Lett. 891
Original
2001
Cited alongside, same era.
G. Ye and Y.-S. Piao, Is the Hubble tension a hint of AdS phase around recombination?, Phys. Rev. D 101
Original
2001
Cited alongside, same era.
O. H. Philcox, M. M. Ivanov, M. Simonović, and M. Zaldarriaga, Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0, JCAP 05
Original
2002
Cited alongside, same era.
G. Benevento, W. Hu, and M. Raveri, Can Late Dark Energy Transitions Raise the Hubble constant?, Phys. Rev. D 101
Original

Then

E. Di Valentino, A. Melchiorri, and J. Silk, Reconciling Planck with the local value of H 0 H_{0} in extended parameter space, Phys. Lett. B 761
Original
2016
Later among the works it cites.
S. Kumar and R. C. Nunes, Probing the interaction between dark matter and dark energy in the presence of massive neutrinos, Phys. Rev. D 94
Original
2016
Later among the works it cites.
J. L. Bernal, L. Verde, and A. G. Riess, The trouble with H 0 H_{0} , JCAP 10
Original
2016
Later among the works it cites.
J. Lesgourgues, G. Marques-Tavares, and M. Schmaltz, Evidence for dark matter interactions in cosmological precision data?, JCAP 02
Original
2016
Later among the works it cites.
T. Karwal and M. Kamionkowski, Dark energy at early times, the Hubble parameter, and the string axiverse, Phys. Rev. D 94

Beyond the bibliography

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

Open on alphaXiv

alphaXiv is searching for related work…

2002

Cited alongside, same era.

R. Dave, R. R. Caldwell, and P. J. Steinhardt, Sensitivity of the cosmic microwave background anisotropy to initial conditions in quintessence cosmology, Phys. Rev. D 66

2002

Cited alongside, same era.

M. Malquarti and A. R. Liddle, Initial conditions for quintessence after inflation, Phys. Rev. D 66

2002

Cited alongside, same era.

A. Lewis and S. Bridle, Cosmological parameters from CMB and other data: A Monte Carlo approach, Phys. Rev. D 66

2002

Cited alongside, same era.

H. Desmond and J. Sakstein, Screened fifth forces lower the TRGB-calibrated Hubble constant too, Phys. Rev. D 102

Original

2003

Cited alongside, same era.