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S. Tsujikawa, “Quintessence: A Review,” Class. Quant. Grav
Original
1961
Earlier work this paper cites.
A. A. Starobinsky, “A New Type of Isotropic Cosmological Models Without Singularity,” Phys. Lett
1980
Earlier work this paper cites.
A. H. Guth, “The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems,” Phys. Rev
1981
Earlier work this paper cites.
A. D. Linde, “A New Inflationary Universe Scenario: A Possible Solution of the Horizon, Flatness, Homogeneity, Isotropy and Primordial Monopole Problems,” Phys. Lett
1982
Earlier work this paper cites.
A. Albrecht and P. J. Steinhardt, “Cosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking,” Phys. Rev. Lett
1982
Earlier work this paper cites.
R. R. Caldwell, R. Dave, and P. J. Steinhardt, “Cosmological imprint of an energy component with general equation of state,” Phys. Rev. Lett
1998
Earlier work this paper cites.
K. Choi, “String or M theory axion as a quintessence,” Phys. Rev
Original
2000
Earlier work this paper cites.
S. Hellerman, N. Kaloper, and L. Susskind, “String theory and quintessence,” JHEP
2001
Earlier work this paper cites.
T. Banks, M. Dine, P. J. Fox, and E. Gorbatov, “On the possibility of large axion decay constants,” JCAP
2003
Earlier work this paper cites.

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2018

Agrawal, Prateek, Obied, Georges, Steinhardt, Paul J. et al.

We study constraints imposed by two proposed string Swampland criteria on cosmology.

These criteria involve an upper bound on the range traversed by scalar fields as well as a lower bound on $|\nabla_{\phi} V|/V$ when $V >0$.
We find that inflationary models are generically in tension with these two criteria.
Applying these same criteria to dark energy in the present epoch, we find that specific quintessence models can satisfy these bounds and, at the same time, satisfy current observational constraints.

S. Tsujikawa, “Quintessence: A Review,” Class. Quant. Grav
Original
1961
Earlier work this paper cites.
A. A. Starobinsky, “A New Type of Isotropic Cosmological Models Without Singularity,” Phys. Lett
1980
Earlier work this paper cites.
A. H. Guth, “The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems,” Phys. Rev
1981
Earlier work this paper cites.
A. D. Linde, “A New Inflationary Universe Scenario: A Possible Solution of the Horizon, Flatness, Homogeneity, Isotropy and Primordial Monopole Problems,” Phys. Lett
1982
Earlier work this paper cites.
A. Albrecht and P. J. Steinhardt, “Cosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking,” Phys. Rev. Lett
1982
Earlier work this paper cites.
R. R. Caldwell, R. Dave, and P. J. Steinhardt, “Cosmological imprint of an energy component with general equation of state,” Phys. Rev. Lett
1998
Earlier work this paper cites.
K. Choi, “String or M theory axion as a quintessence,” Phys. Rev
Original
2000
Earlier work this paper cites.
S. Hellerman, N. Kaloper, and L. Susskind, “String theory and quintessence,” JHEP
2001
Earlier work this paper cites.
T. Banks, M. Dine, P. J. Fox, and E. Gorbatov, “On the possibility of large axion decay constants,” JCAP
2003
Earlier work this paper cites.

N. Kaloper, “Cosmological horizons, quintessence and string theory,” Prog. Theor. Phys. Suppl
2003
Cited alongside, same era.
E. Silverstein and D. Tong, “Scalar speed limits and cosmology: Acceleration from D-cceleration,” Phys. Rev
2004
Cited alongside, same era.
H. Ooguri and C. Vafa, “On the Geometry of the String Landscape and the Swampland,” Nucl. Phys
2007
Cited alongside, same era.
N. Arkani-Hamed, L. Motl, A. Nicolis, and C. Vafa, “The String landscape, black holes and gravity as the weakest force,” JHEP
2007
Cited alongside, same era.
E. Silverstein and A. Westphal, “Monodromy in the CMB: Gravity Waves and String Inflation,” Phys. Rev
Original
2008
Cited alongside, same era.