What if string theory has no de Sitter vacua?

UH Danielsson, TV Riet - International Journal of Modern Physics D, 2018 - World Scientific
We present a brief overview of attempts to construct de Sitter vacua in string theory and
explain how the results of this 20-year endeavor could point to the fact that string theory …

Snowmass white paper: the cosmological bootstrap

D Baumann, D Green, A Joyce, E Pajer… - SciPost Physics …, 2024 - scipost.org
This white paper summarizes recent progress in the cosmological bootstrap, an approach to
the study of the statistics of primordial fluctuations from consistency with unitarity, locality and …

The string landscape, the swampland, and the missing corner

TD Brennan, F Carta, C Vafa - arxiv preprint arxiv:1711.00864, 2017 - arxiv.org
We give a brief overview of the string landscape and techniques used to construct string
compactifications. We then explain how this motivates the notion of the swampland and …

The landscape, the swampland and the era of precision cosmology

Y Akrami, R Kallosh, A Linde… - Fortschritte der …, 2019 - Wiley Online Library
We review the advanced version of the KKLT construction and pure de Sitter supergravity,
involving a nilpotent multiplet, with regard to various conjectures that de Sitter state cannot …

Pure de Sitter space and the island moving back in time

W Sybesma - Classical and Quantum Gravity, 2021 - iopscience.iop.org
Observers in de Sitter space can only access the space up to their cosmological horizon.
Assuming thermal equilibrium, we use the quantum Ryu–Takayanagi or island formula to …

De sitter space

M Spradlin, A Strominger, A Volovich - … Session LXXVI, 30 July–31 August …, 2002 - Springer
These lectures present an elementary discussion of some background material relevant to
the problem of de Sitter quantum gravity. The first two lectures discuss the classical …

Partial masslessness of higher spins in (A) dS

S Deser, A Waldron - Nuclear Physics B, 2001 - Elsevier
Massive spin s⩾ 3/2 fields can become partially massless in cosmological backgrounds. In
the plane spanned by m2 and Λ, there are lines where new gauge invariances permit …

Timelike T-duality, de Sitter space, large N gauge theories and topological field theory

CM Hull - Journal of High Energy Physics, 1998 - iopscience.iop.org
T-Duality on a timelike circle does not interchange IIA and IIB string theories, but takes the
IIA theory to a type IIB∗ theory and the IIB theory to a type IIA∗ theory. The type II∗ theories …

Gauge invariances and phases of massive higher spins in (anti-) de Sitter space

S Deser, A Waldron - Physical Review Letters, 2001 - APS
Abstract The (m 2, Λ) plane of spin s> 1 massive fields in (anti-) de Sitter space backgrounds
is shown to consist of separate phases, divided by lines of novel “partially massless” gauge …

Compact and non-compact gauged supergravity theories in five dimensions

M Günaydin, LJ Romans, NP Warner - Nuclear Physics B, 1986 - Elsevier
We give a detailed construction of gauged N= 8 supergravity theories in five dimensions with
Yang-Mills gauge groups SO (p, 6− p)(p= 0, 1, 2, 3), physical global symmetry SU (1, 1), and …