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Mikael von Strauss

Researcher at Institut d'Astrophysique de Paris

Publications -  32
Citations -  2425

Mikael von Strauss is an academic researcher from Institut d'Astrophysique de Paris. The author has contributed to research in topics: Massive gravity & Graviton. The author has an hindex of 23, co-authored 32 publications receiving 2236 citations. Previous affiliations of Mikael von Strauss include Stockholm University & Royal Institute of Technology.

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Beyond $\Lambda$CDM: Problems, solutions, and the road ahead

TL;DR: There is a persistent interest in extending cosmology beyond the standard model, $\Lambda$CDM as discussed by the authors, motivated by a range of apparently serious theoretical issues, involving such questions as the cosmological constant problem, the particle nature of dark matter, the validity of general relativity on large scales, the existence of anomalies in the CMB and on small scales, and the predictivity and testability of the inflationary paradigm.
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Cosmological Solutions in Bimetric Gravity and their Observational Tests

TL;DR: In this article, the general cosmological evolution equations for a classically consistent theory of bimetric gravity were obtained and their analytic solutions were demonstrated to generically allow for a cosmic evolution.
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Recent developments in bimetric theory

TL;DR: In this paper, a review is dedicated to recent progress in the development of classical, in-teracting, massive spin-2 theories, with a focus on ghost-free bimetric theory.
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Proof of consistency of nonlinear massive gravity in the Stückelberg formulation

TL;DR: In this paper, the absence of the Boulware-deser ghost in the Stuckelberg formulation of nonlinear massive gravity was shown to be consistent with existing consistency proofs.
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Cosmological Solutions in Bimetric Gravity and their Observational Tests

TL;DR: In this article, the general cosmological evolution equations for a classically consistent theory of bimetric gravity were obtained and their analytic solutions were demonstrated to generically allow for a cosmic evolution starting out from a matter dominated FLRW universe while relaxing towards a de Sitter (anti-de Sitter) phase at late cosmic time.