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PreprintarXiv licencearXiv

The Disordered Universe 2025: Features in a Λ>0 Universe

Abstract

A complete understanding of cosmology, from its earliest epoch all the way to the current dark energy dominated era, requires the development of a mathematical framework that incorporates quantum features in an expanding universe. Such a framework, alongside a description of the underlying degrees of freedom, is so far lacking. Several of the pertinent challenges and puzzles already arise upon considering even the most idealised model of an expanding universe --- the de Sitter spacetime and fluctuations thereof. In these lectures, we review some elementary ideas of the de Sitter physics, passing through the representation theory of the de Sitter group, aspects of canonical quantum gravity, all the way to attempts in describing quasi-local features. Throughout, we highlight open problems that motivate ongoing efforts to understand quantum gravity and cosmology in universes with Λ>0. These notes are based on a series of lectures held during the La Ricotta Summer School: The Disordered Universe 2025 from 21 July to 1 August 2025.

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BibTeX
@misc{brian2026disordered,
  title = {{The Disordered Universe 2025: Features in a $Λ>0$ Universe}},
  author = {Samuel Brian and Yakov Landau and Tommaso Marini and Daniel McLoughlin and Polina Petriakova and Rajat Sharma and Dionysios Anninos and Paolo Benincasa and Guilherme Leite Pimentel},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.37117},
  eprint = {2610.37117},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.37117},
}
RIS
TY  - UNPB
TI  - The Disordered Universe 2025: Features in a Λ>0 Universe
AU  - Samuel Brian
AU  - Yakov Landau
AU  - Tommaso Marini
AU  - Daniel McLoughlin
AU  - Polina Petriakova
AU  - Rajat Sharma
AU  - Dionysios Anninos
AU  - Paolo Benincasa
AU  - Guilherme Leite Pimentel
PY  - 2026
DA  - 2026/10/27
PB  - arXiv
DO  - 10.48550/arxiv.2610.37117
UR  - https://arxiv.org/abs/2610.37117
AB  - A complete understanding of cosmology, from its earliest epoch all the way to the current dark energy dominated era, requires the development of a mathematical framework that incorporates quantum features in an expanding universe. Such a framework, alongside a description of the underlying degrees of freedom, is so far lacking. Several of the pertinent challenges and puzzles already arise upon considering even the most idealised model of an expanding universe --- the de Sitter spacetime and fluctuations thereof. In these lectures, we review some elementary ideas of the de Sitter physics, passing through the representation theory of the de Sitter group, aspects of canonical quantum gravity, all the way to attempts in describing quasi-local features. Throughout, we highlight open problems that motivate ongoing efforts to understand quantum gravity and cosmology in universes with Λ>0. These notes are based on a series of lectures held during the La Ricotta Summer School: The Disordered Universe 2025 from 21 July to 1 August 2025.
ER  -