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 …
explain how the results of this 20-year endeavor could point to the fact that string theory …
Snowmass white paper: the cosmological bootstrap
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 study of the statistics of primordial fluctuations from consistency with unitarity, locality and …
The string landscape, the swampland, and the missing corner
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 …
compactifications. We then explain how this motivates the notion of the swampland and …
The landscape, the swampland and the era of precision cosmology
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 …
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 …
Assuming thermal equilibrium, we use the quantum Ryu–Takayanagi or island formula to …
De sitter space
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 …
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 …
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 …
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 …
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
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 …
Yang-Mills gauge groups SO (p, 6− p)(p= 0, 1, 2, 3), physical global symmetry SU (1, 1), and …