Results 81 to 90 of about 683 (126)
AdS4flux vacua in type II superstrings and their domain-wall solutions
Acknowledgment ...
Kounnas, C. +3 more
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Branes with brains: exploring string vacua with deep reinforcement learning
We propose deep reinforcement learning as a model-free method for exploring the landscape of string vacua. As a concrete application, we utilize an artificial intelligence agent known as an asynchronous advantage actor-critic to explore type IIA ...
James Halverson +2 more
doaj +1 more source
Anomalous U(1)s in Type I superstring vacua
We perform a systematic string computation of the masses of anomalous U(1) gauge bosons in four-dimensional orientifold vacua, and we study their localization properties in the internal (compactified) space. We find that N=1 supersymmetric sectors yield four-dimensional contributions, localized in the whole six-dimensional internal space, while N=2 ...
Antoniadis, I., Kiritsis, E., Rizos, J.
openaire +2 more sources
Geometrical Construction of Type I Superstring Vacua
12 pages, latex, no figures; contribution to the Proceedings of the 12th Italian Conference on General Relativity and Gravitational Physics, Rome, september 23-27 ...
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The gravitational sector of 2d (0, 2) F-theory vacua
F-theory compactifications on Calabi-Yau fivefolds give rise to two-dimensional N = (0, 2) supersymmetric field theories coupled to gravity. We explore the dilaton supergravity defined by the moduli sector of such compactifications.
Craig Lawrie +2 more
doaj +1 more source
De Sitter vacua in no-scale supergravity
No-scale supergravity is the appropriate general framework for low-energy effective field theories derived from string theory. The simplest no-scale Kähler potential with a single chiral field corresponds to a compactification to flat Minkowski space ...
John Ellis +3 more
doaj +1 more source
100 years of mathematical cosmology: Models, theories and problems, Part B. [PDF]
Cotsakis S, Yefremov AP.
europepmc +1 more source
Conflicts with de Sitter Vacua in Superstring Theory
Models of our universe lack consistency at different energy scales, so we require a theory with ultraviolet (UV) completion such as string theory. A suitable candidate to model our universe in this framework is de Sitter space, a spacetime which expands and has positive curvature.
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A universal tachyon in nearly no-scale de Sitter compactifications
We investigate de Sitter solutions of N=1 $$ \mathcal{N}=1 $$ supergravity with an F-term scalar potential near a no-scale Minkowski point, as they may in particular arise from flux compactifications in string theory.
Daniel Junghans, Marco Zagermann
doaj +1 more source
Detection of early-universe gravitational-wave signatures and fundamental physics. [PDF]
Caldwell R +37 more
europepmc +1 more source

