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D. Andriot, “Open problems on classical de Sitter solutions,” Fortsch. Phys
Original
1902
Earlier work this paper cites.
F. Carta, J. Moritz, and A. Westphal, “Gaugino condensation and small uplifts in KKLT,” JHEP
Original
1902
Earlier work this paper cites.
E. Palti, “The Swampland: Introduction and Review,” Fortsch. Phys
Original
1903
Earlier work this paper cites.
E. Hardy and S. Parameswaran, “Thermal Dark Energy,” Phys. Rev. D
Original
1907
Earlier work this paper cites.
A. Lewis, “GetDist: a Python package for analysing Monte Carlo samples,” arXiv:1910.13970 [astro-ph.IM]
Original
1910
Earlier work this paper cites.
H. Akaike, “A New Look at the Statistical Model Identification,” IEEE Transactions on Automatic Control
1974
Earlier work this paper cites.
K. Choi, “String or M theory axion as a quintessence,” Phys. Rev. D
2000
Earlier work this paper cites.
M. Chevallier and D. Polarski, “Accelerating universes with scaling dark matter,” Int. J. Mod. Phys. D
2001
Earlier work this paper cites.
A. Lewis and S. Bridle, “Cosmological parameters from CMB and other data: A Monte Carlo approach,” Phys. Rev
2002
Earlier work this paper cites.
E. V. Linder, “Exploring the expansion history of the universe,” Phys. Rev. Lett
2003
Earlier work this paper cites.
J. E. Kim and H. P. Nilles, “A Quintessential axion,” Phys. Lett. B
2003
Earlier work this paper cites.
A. R. Liddle, “How many cosmological parameters?,” Mon. Not. Roy. Astron. Soc
2004
Earlier work this paper cites.
B. Valeixo Bento, D. Chakraborty, S. L. Parameswaran, and I. Zavala, “Dark Energy in String Theory,” PoS
Original
2005
Earlier work this paper cites.
J. E. Kim, H. P. Nilles, and M. Peloso, “Completing natural inflation,” JCAP
2005
Earlier work this paper cites.
J. Torrado and A. Lewis, “Cobaya: Code for Bayesian Analysis of hierarchical physical models,” JCAP
Original
2005
Earlier work this paper cites.
N. Arkani-Hamed, L. Motl, A. Nicolis, and C. Vafa, “The String landscape, black holes and gravity as the weakest force,” JHEP
2007
Earlier work this paper cites.
H. Ooguri and C. Vafa, “On the Geometry of the String Landscape and the Swampland,” Nucl. Phys. B
2007
Earlier work this paper cites.
S. Dutta and R. J. Scherrer, “Hilltop Quintessence,” Phys. Rev. D
Original
2008
Earlier work this paper cites.
S. Dimopoulos, S. Kachru, J. McGreevy, and J. G. Wacker, “N-flation,” JCAP
2008
Earlier work this paper cites.
P. Sikivie, “Axion Cosmology,” Lect. Notes Phys
2008
Earlier work this paper cites.
T. Chiba, “Slow-Roll Thawing Quintessence,” Phys. Rev. D
Original
2009
Earlier work this paper cites.
N. Kaloper and L. Sorbo, “Where in the String Landscape is Quintessence,” Phys. Rev. D
Original
2009
Earlier work this paper cites.
A. Arvanitaki, S. Dimopoulos, S. Dubovsky, N. Kaloper, and J. March-Russell, “String Axiverse,” Phys. Rev. D
Original
2010
Earlier work this paper cites.

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N. Schöneberg, L. Vacher, J. D. F. Dias, M. M. C. D. Carvalho, and C. J. A. P. Martins, “News from the Swampland — constraining string theory with astrophysics and cosmology,” JCAP
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2023
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Original
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Closest in time.
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2024

Cosmological tests of quintessence in quantum gravity

Bhattacharya, Sukannya, Borghetto, Giulia, Malhotra, Ameek et al.

Understand

We use a suite of the most recent cosmological observations to test models of dynamical dark energy motivated by quantum gravity.

Specifically, we focus on hilltop quintessence scenarios, able to satisfy theoretical constraints from quantum gravity.
We discuss their realisation based on axions, their supersymmetric partners, and Higgs-like string constructions, including dynamical mechanisms to set up initial conditions at the hilltops.
We also examine a specific parameterisation for dynamical dark energy suitable for hilltop quintessence.

Built on

D. Andriot, “Open problems on classical de Sitter solutions,” Fortsch. Phys
Original
1902
Earlier work this paper cites.
F. Carta, J. Moritz, and A. Westphal, “Gaugino condensation and small uplifts in KKLT,” JHEP
Original
1902
Earlier work this paper cites.
E. Palti, “The Swampland: Introduction and Review,” Fortsch. Phys
Original
1903
Earlier work this paper cites.
E. Hardy and S. Parameswaran, “Thermal Dark Energy,” Phys. Rev. D
Original
1907
Earlier work this paper cites.
A. Lewis, “GetDist: a Python package for analysing Monte Carlo samples,” arXiv:1910.13970 [astro-ph.IM]
Original
1910
Earlier work this paper cites.
H. Akaike, “A New Look at the Statistical Model Identification,” IEEE Transactions on Automatic Control
1974
Earlier work this paper cites.
K. Choi, “String or M theory axion as a quintessence,” Phys. Rev. D
2000
Earlier work this paper cites.
M. Chevallier and D. Polarski, “Accelerating universes with scaling dark matter,” Int. J. Mod. Phys. D
2001
Earlier work this paper cites.
A. Lewis and S. Bridle, “Cosmological parameters from CMB and other data: A Monte Carlo approach,” Phys. Rev
2002
Earlier work this paper cites.
E. V. Linder, “Exploring the expansion history of the universe,” Phys. Rev. Lett
2003
Earlier work this paper cites.
J. E. Kim and H. P. Nilles, “A Quintessential axion,” Phys. Lett. B
2003
Earlier work this paper cites.
A. R. Liddle, “How many cosmological parameters?,” Mon. Not. Roy. Astron. Soc
2004
Earlier work this paper cites.
B. Valeixo Bento, D. Chakraborty, S. L. Parameswaran, and I. Zavala, “Dark Energy in String Theory,” PoS
Original
2005
Earlier work this paper cites.
J. E. Kim, H. P. Nilles, and M. Peloso, “Completing natural inflation,” JCAP
2005
Earlier work this paper cites.
J. Torrado and A. Lewis, “Cobaya: Code for Bayesian Analysis of hierarchical physical models,” JCAP
Original
2005
Earlier work this paper cites.
N. Arkani-Hamed, L. Motl, A. Nicolis, and C. Vafa, “The String landscape, black holes and gravity as the weakest force,” JHEP
2007
Earlier work this paper cites.
H. Ooguri and C. Vafa, “On the Geometry of the String Landscape and the Swampland,” Nucl. Phys. B
2007
Earlier work this paper cites.
S. Dutta and R. J. Scherrer, “Hilltop Quintessence,” Phys. Rev. D
Original
2008
Earlier work this paper cites.
S. Dimopoulos, S. Kachru, J. McGreevy, and J. G. Wacker, “N-flation,” JCAP
2008
Earlier work this paper cites.
P. Sikivie, “Axion Cosmology,” Lect. Notes Phys
2008
Earlier work this paper cites.
T. Chiba, “Slow-Roll Thawing Quintessence,” Phys. Rev. D
Original
2009
Earlier work this paper cites.
N. Kaloper and L. Sorbo, “Where in the String Landscape is Quintessence,” Phys. Rev. D
Original
2009
Earlier work this paper cites.
A. Arvanitaki, S. Dimopoulos, S. Dubovsky, N. Kaloper, and J. March-Russell, “String Axiverse,” Phys. Rev. D
Original
2010
Earlier work this paper cites.