Built on

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.
E. Ó Colgáin, “A hint of matter underdensity at low z?,” JCAP 09
Original
1903
Earlier work this paper cites.
V. de Sainte Agathe, C. Balland, H. du Mas des Bourboux, N. G. Busca, M. Blomqvist, J. Guy, J. Rich, A. Font-Ribera, M. M. Pieri and J. E. Bautista, et al
Original
1904
Earlier work this paper cites.
M. Blomqvist, H. du Mas des Bourboux, N. G. Busca, V. de Sainte Agathe, J. Rich, C. Balland, J. E. Bautista, K. Dawson, A. Font-Ribera and J. Guy, et al
Original
1904
Earlier work this paper cites.
D. Camarena and V. Marra, “Local determination of the Hubble constant and the deceleration parameter,” Phys. Rev. Res. 2
Original
1906
Earlier work this paper cites.
L. Verde, T. Treu and A. G. Riess, “Tensions between the Early and the Late Universe,” Nature Astron. 3
Original
1907
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.
G. ’t Hooft, “Dimensional reduction in quantum gravity,” Conf. Proc. C 930308
1993
Earlier work this paper cites.
A. G. Riess et al
1998
Earlier work this paper cites.
A. G. Cohen, D. B. Kaplan and A. E. Nelson, “Effective field theory, black holes, and the cosmological constant,” Phys. Rev. Lett. 82
1999
Earlier work this paper cites.
S. Perlmutter et al
1999
Earlier work this paper cites.
M. Chevallier and D. Polarski, “Accelerating universes with scaling dark matter,” Int. J. Mod. Phys. D 10
2001
Earlier work this paper cites.
G. Benevento, W. Hu and M. Raveri, “Can Late Dark Energy Transitions Raise the Hubble constant?,” Phys. Rev. D 101
Original
2002
Earlier work this paper cites.
E. V. Linder, “Exploring the expansion history of the universe,” Phys. Rev. Lett. 90
2003
Earlier work this paper cites.
W. M. Dai, Y. Z. Ma and H. J. He, “Reconciling Hubble Constant Discrepancy from Holographic Dark Energy,” Phys. Rev. D 102
Original
2003
Earlier work this paper cites.
E. Di Valentino, A. Melchiorri and J. Silk, “Cosmic Discordance: Planck and luminosity distance data exclude LCDM,” Astrophys. J. Lett. 908
Original
2003
Earlier work this paper cites.
M. Li, “A Model of holographic dark energy,” Phys. Lett. B 603
2004
Earlier work this paper cites.
Q. G. Huang and M. Li, “The Holographic dark energy in a non-flat universe,” JCAP 08
2004
Earlier work this paper cites.
Q. G. Huang and Y. G. Gong, “Supernova constraints on a holographic dark energy model,” JCAP 08
2004
Earlier work this paper cites.
S. D. H. Hsu, “Entropy bounds and dark energy,” Phys. Lett. B 594
2004
Earlier work this paper cites.

Similar

D. Pavon and W. Zimdahl, “Holographic dark energy and cosmic coincidence,” Phys. Lett. B 628
2005
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B. Wang, Y. g. Gong and E. Abdalla, “Transition of the dark energy equation of state in an interacting holographic dark energy model,” Phys. Lett. B 624
2005
Cited alongside, same era.
E. N. Saridakis, “Barrow holographic dark energy,” Phys. Rev. D 102
Original
2005
Cited alongside, same era.
X. Zhang and F. Q. Wu, “Constraints on holographic dark energy from Type Ia supernova observations,” Phys. Rev. D 72
2005
Cited alongside, same era.
E. Di Valentino, A. Mukherjee and A. A. Sen, “Dark Energy with Phantom Crossing and the H 0 H_{0} tension,” [arXiv:2005.12587 [astro-ph.CO]]
Original
2005
Cited alongside, same era.

Then

L. P. Chimento, M. I. Forte and M. G. Richarte, “Self-interacting holographic dark energy,” Mod. Phys. Lett. A 28
Original
2013
Later among the works it cites.
L. P. Chimento, M. G. Richarte and I. E. Sánchez García, “Interacting dark sector with variable vacuum energy,” Phys. Rev. D 88
Original
2013
Later among the works it cites.
M. Li, X. D. Li, Y. Z. Ma, X. Zhang and Z. Zhang, “Planck Constraints on Holographic Dark Energy,” JCAP 09
Original
2013
Later among the works it cites.
V. A. Rubakov, “The Null Energy Condition and its violation,” Usp. Fiz. Nauk 184
Original
2014
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

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2021

A Critique of Holographic Dark Energy

Colgáin, Eoin Ó, Sheikh-Jabbari, M. M.

Understand

Observations restrict the parameter space of Holographic Dark Energy (HDE) so that a turning point in the Hubble parameter $H(z)$ is inevitable.

Concretely, cosmic microwave background (CMB), baryon acoustic oscillations (BAO) and Type Ia supernovae (SNE) data put the turning point in the future, but removing SNE results in an observational turning point at positive redshift.
From the perspective of theory, not only does the turning point violate the Null Energy Condition (NEC), but as we argue, it may be interpreted as an evolution of the Hubble constant $H_0$ with redshift, which is at odds with the very FLRW framework within which data has been analysed.
Tellingly, neither of these are problems for the flat $\Lambda$CDM model, and a direct comparison of fits further disfavours HDE relative to flat $\Lambda$CDM.

Built on

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.
E. Ó Colgáin, “A hint of matter underdensity at low z?,” JCAP 09
Original
1903
Earlier work this paper cites.
V. de Sainte Agathe, C. Balland, H. du Mas des Bourboux, N. G. Busca, M. Blomqvist, J. Guy, J. Rich, A. Font-Ribera, M. M. Pieri and J. E. Bautista, et al
Original
1904
Earlier work this paper cites.
M. Blomqvist, H. du Mas des Bourboux, N. G. Busca, V. de Sainte Agathe, J. Rich, C. Balland, J. E. Bautista, K. Dawson, A. Font-Ribera and J. Guy, et al
Original
1904
Earlier work this paper cites.
D. Camarena and V. Marra, “Local determination of the Hubble constant and the deceleration parameter,” Phys. Rev. Res. 2
Original
1906
Earlier work this paper cites.
L. Verde, T. Treu and A. G. Riess, “Tensions between the Early and the Late Universe,” Nature Astron. 3
Original
1907
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.
G. ’t Hooft, “Dimensional reduction in quantum gravity,” Conf. Proc. C 930308
1993
Earlier work this paper cites.
A. G. Riess et al
1998
Earlier work this paper cites.
A. G. Cohen, D. B. Kaplan and A. E. Nelson, “Effective field theory, black holes, and the cosmological constant,” Phys. Rev. Lett. 82
1999
Earlier work this paper cites.
S. Perlmutter et al
1999
Earlier work this paper cites.
M. Chevallier and D. Polarski, “Accelerating universes with scaling dark matter,” Int. J. Mod. Phys. D 10
2001
Earlier work this paper cites.
G. Benevento, W. Hu and M. Raveri, “Can Late Dark Energy Transitions Raise the Hubble constant?,” Phys. Rev. D 101
Original
2002
Earlier work this paper cites.
E. V. Linder, “Exploring the expansion history of the universe,” Phys. Rev. Lett. 90
2003
Earlier work this paper cites.
W. M. Dai, Y. Z. Ma and H. J. He, “Reconciling Hubble Constant Discrepancy from Holographic Dark Energy,” Phys. Rev. D 102
Original
2003
Earlier work this paper cites.
E. Di Valentino, A. Melchiorri and J. Silk, “Cosmic Discordance: Planck and luminosity distance data exclude LCDM,” Astrophys. J. Lett. 908
Original
2003
Earlier work this paper cites.
M. Li, “A Model of holographic dark energy,” Phys. Lett. B 603
2004
Earlier work this paper cites.
Q. G. Huang and M. Li, “The Holographic dark energy in a non-flat universe,” JCAP 08
2004
Earlier work this paper cites.
Q. G. Huang and Y. G. Gong, “Supernova constraints on a holographic dark energy model,” JCAP 08
2004
Earlier work this paper cites.
S. D. H. Hsu, “Entropy bounds and dark energy,” Phys. Lett. B 594
2004
Earlier work this paper cites.

Similar

D. Pavon and W. Zimdahl, “Holographic dark energy and cosmic coincidence,” Phys. Lett. B 628
2005
Cited alongside, same era.
B. Wang, Y. g. Gong and E. Abdalla, “Transition of the dark energy equation of state in an interacting holographic dark energy model,” Phys. Lett. B 624
2005
Cited alongside, same era.
E. N. Saridakis, “Barrow holographic dark energy,” Phys. Rev. D 102
Original
2005
Cited alongside, same era.
X. Zhang and F. Q. Wu, “Constraints on holographic dark energy from Type Ia supernova observations,” Phys. Rev. D 72
2005
Cited alongside, same era.
E. Di Valentino, A. Mukherjee and A. A. Sen, “Dark Energy with Phantom Crossing and the H 0 H_{0} tension,” [arXiv:2005.12587 [astro-ph.CO]]
Original
2005
Cited alongside, same era.

Then

L. P. Chimento, M. I. Forte and M. G. Richarte, “Self-interacting holographic dark energy,” Mod. Phys. Lett. A 28
Original
2013
Later among the works it cites.
L. P. Chimento, M. G. Richarte and I. E. Sánchez García, “Interacting dark sector with variable vacuum energy,” Phys. Rev. D 88
Original
2013
Later among the works it cites.
M. Li, X. D. Li, Y. Z. Ma, X. Zhang and Z. Zhang, “Planck Constraints on Holographic Dark Energy,” JCAP 09
Original
2013
Later among the works it cites.
V. A. Rubakov, “The Null Energy Condition and its violation,” Usp. Fiz. Nauk 184
Original
2014
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

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. Eisenstein et al

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Z. Chang, F. Q. Wu and X. Zhang, “Constraints on holographic dark energy from x-ray gas mass fraction of galaxy clusters,” Phys. Lett. B 633

2006

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R. G. Cai, “A Dark Energy Model Characterized by the Age of the Universe,” Phys. Lett. B 657

Original

2007

Cited alongside, same era.

X. Zhang and F. Q. Wu, “Constraints on Holographic Dark Energy from Latest Supernovae, Galaxy Clustering, and Cosmic Microwave Background Anisotropy Observations,” Phys. Rev. D 76

2007

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C. Gao, F. Wu, X. Chen and Y. G. Shen, “A Holographic Dark Energy Model from Ricci Scalar Curvature,” Phys. Rev. D 79

Original

2009

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N. J. Secrest, S. von Hausegger, M. Rameez, R. Mohayaee, S. Sarkar and J. Colin, “A Test of the Cosmological Principle with Quasars,” [arXiv:2009.14826 [astro-ph.CO]]

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2009

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X. Zhang, “Holographic Ricci dark energy: Current observational constraints, quintom feature, and the reconstruction of scalar-field dark energy,” Phys. Rev. D 79

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2009

Cited alongside, same era.

Original

2015