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1973
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2018

The Swampland, Quintessence and the Vacuum Energy

Marsh, M. C. David

Understand

It has recently been conjectured that string theory does not admit de Sitter vacua, and that quintessence explains the current epoch of accelerated cosmic expansion.

A proposed, key prediction of this scenario is time-varying couplings in the dark sector, induced by the evolving quintessence field.
We note that cosmological models with varying couplings suffer from severe problems with quantum corrections, beyond those shared by all quintessence models.
The vacuum energy depends on all masses and couplings of the theory, and even small variations of parameters can lead to overwhelmingly large corrections to the effective potential.

Built on

S. R. Coleman and E. J. Weinberg, Phys. Rev. D7
1973
Earlier work this paper cites.
S. Weinberg, Phys. Rev. D7
1973
Earlier work this paper cites.
J. Iliopoulos, C. Itzykson, and A. Martin, Les Houches School 1976:0115 , Rev. Mod. Phys. 47
1975
Earlier work this paper cites.
B. Zumino, Nucl. Phys. B89
1975
Earlier work this paper cites.
M. T. Grisaru, M. Rocek, and A. Karlhede, Phys. Lett. 120B
1983
Earlier work this paper cites.
S. Ferrara, C. Kounnas, and F. Zwirner, Nucl. Phys. B429
1995
Earlier work this paper cites.
T. Banks, M. Dine, and M. R. Douglas, Phys. Rev. Lett. 88
2002
Earlier work this paper cites.
J. F. Donoghue, JHEP 03
2003
Earlier work this paper cites.
B. Wang, E. Abdalla, F. Atrio-Barandela, and D. Pavon, Rept. Prog. Phys. 79
Original
2016
Earlier work this paper cites.
G. D’Amico, T. Hamill, and N. Kaloper, Phys. Rev. D94
Original
2016
Earlier work this paper cites.
S. Ferrara and A. Van Proeyen, Fortsch. Phys. 64
Original
2016
Earlier work this paper cites.