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Cosmology with the Laser Interferometer Space Antenna / LISA Cosmology Working Group Collaboration
The Laser Interferometer Space Antenna (LISA) has two scientific objectives of cosmological focus: to probe the expansion rate of the universe, and to understand stochastic gravitational-wave backgrounds and their implications for early universe and particle physics, from the MeV to the Planck scale. However, the range of potential cosmological applications of gravitational wave observations extends well beyond these two objectives. [...]
arXiv:2204.05434; LISA CosWG-22-03; FERMILAB-PUB-22-349-SCD.- 2023-08-28 - 176 p. - Published in : Living Rev. Relativ. 26 (2023) 5 Fulltext: 2204.05434 - PDF; jt - PDF; Fulltext from Publisher: PDF; External link: Fermilab Library Server

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New horizons for fundamental physics with LISA / LISA Collaboration
The Laser Interferometer Space Antenna (LISA) has the potential to reveal wonders about the fundamental theory of nature at play in the extreme gravity regime, where the gravitational interaction is both strong and dynamical. In this white paper, the Fundamental Physics Working Group of the LISA Consortium summarizes the current topics in fundamental physics where LISA observations of GWs can be expected to provide key input. [...]
arXiv:2205.01597.- 2022-06-30 - 116 p. - Published in : Living Rev. Relativ. 25 (2022) 4 Fulltext: 2205.01597 - PDF; document - PDF;

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Dark Energy / Zumalacárregui, Miguel (speaker)
2022 - 1725. Conferences & Workshops; Second EuCAPT Annual Symposium External links: Talk details; Event details In : Second EuCAPT Annual Symposium

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Unveiling the gravitational universe at $\mu$-Hz frequencies / Sesana, Alberto (Milan Bicocca U.) ; Korsakova, Natalia (Cote d'Azur Observ., Nice) ; Sedda, Manuel Arca (U. Heidelberg (main)) ; Baibhav, Vishal (Johns Hopkins U. (main)) ; Barausse, Enrico (SISSA, Trieste) ; Barke, Simon (U. Florida, Gainesville (main)) ; Berti, Emanuele (Johns Hopkins U. (main)) ; Bonetti, Matteo (Milan Bicocca U.) ; Capelo, Pedro R. (U. Zurich (main)) ; Caprini, Chiara (APC, Paris) et al.
We propose a space-based interferometer surveying the gravitational wave (GW) sky in the milli-Hz to $\mu$-Hz frequency range. By the 2040s', the $\mu$-Hz frequency band, bracketed in between the Laser Interferometer Space Antenna (LISA) and pulsar timing arrays, will constitute the largest gap in the coverage of the astrophysically relevant GW spectrum. [...]
arXiv:1908.11391.- 2021-09-04 - 28 p. - Published in : Exp. Astron. 51 (2021) 1333-1383 Fulltext: 1908.11391 - PDF; document - PDF;

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Dark Energy in light of Multi-Messenger Gravitational-Wave astronomy / Ezquiaga, Jose María (Madrid, IFT) ; Zumalacárregui, Miguel (BCCP, Berkeley ; IPhT, Saclay)
Gravitational waves (GWs) provide a new tool to probe the nature of dark energy (DE) and the fundamental properties of gravity. We review the different ways in which GWs can be used to test gravity and models for late-time cosmic acceleration. [...]
arXiv:1807.09241; IFT-UAM-CSIC-18-83; CERN-TH-2018-172.- 2018-12-04 - 34 p. - Published in : Front. Astron. Space Sci. 5 (2018) 44 Fulltext: PDF;

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Talk and Discussion on Constraints on PBHs from gravitational lensing of SNe / Zumalacarregui, Miguel (speaker)
2018 - 6577. TH institutes; Primordial versus Astrophysical Origin of Black Holes External links: Talk details; Event details In : Primordial versus Astrophysical Origin of Black Holes

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