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We present a novel source of dark energy, which is motivated by the prevalence of hidden sectors in string theory models and is consistent with all of the proposed swampland conjectures.
1901
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2015
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2015
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2006
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S. A. Abel, C.-S. Chu, J. Jaeckel, and V. V. Khoze, “SUSY breaking by a metastable ground state: Why the early universe preferred the non-supersymmetric vacuum,” JHEP
2007
Cited alongside, same era.
S. Kachru, L. McAllister, and R. Sundrum, “Sequestering in String Theory,” JHEP
2007
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J. L. Feng, H. Tu, and H.-B. Yu, “Thermal Relics in Hidden Sectors,” JCAP
2008
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2008
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2009
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2010
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2016
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J. Maltz and L. Susskind, “de Sitter Space as a Resonance,” Phys. Rev. Lett
2017
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W. L. Freedman, “Cosmology at a Crossroads,” Nat. Astron
2017
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2017
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Particle Data Group
2018
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U. H. Danielsson and T. Van Riet, “What if string theory has no de Sitter vacua?,” Int. J. Mod. Phys
2018
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2018
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D. Curtin, P. Meade, and H. Ramani, “Thermal Resummation and Phase Transitions,” Eur. Phys. J
2018
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2018
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2018
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2018
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2019
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M. C. David Marsh, “The Swampland, Quintessence and the Vacuum Energy,” Phys. Lett
2019
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C. Han, S. Pi, and M. Sasaki, “Quintessence Saves Higgs Instability,” Phys. Lett
2019
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2019
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2019
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G. Dvali, C. Gomez, and S. Zell, “Quantum Breaking Bound on de Sitter and Swampland,” Fortsch. Phys
2019
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2019
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