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Peer-reviewedCC BY-NC-ND 4.0Astroparticle Physics

Cosmology intertwined III: fσ8 and S8

80 more authors

60 listed; 92 in total.

Abstract

The standard Λ Cold Dark Matter cosmological model provides a wonderful fit to current cosmological data, but a few tensions and anomalies became statistically significant with the latest data analyses. While these anomalies could be due to the presence of systematic errors in the experiments, they could also indicate the need for new physics beyond the standard model. In this Letter of Interest we focus on the tension of the Planck data with weak lensing measurements and redshift surveys, about the value of the matter energy density Ωm, and the amplitude or rate of the growth of structure (σ8,fσ8). We list a few interesting models for solving this tension, and we discuss the importance of trying to fit with a single model a full array of data and not just one parameter at a time.

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BibTeX
@article{valentino2026cosmology,
  title = {{Cosmology intertwined III: fσ8 and S8}},
  author = {Eleonora Di Valentino and Luis A. Anchordoqui and Özgür Akarsu and Yacine Ali-Haimoud and Luca Amendola and Nikki Arendse and Marika Asgari and Mario Ballardini and Spyros Basilakos and Elia Battistelli and Micol Benetti and Simon Birrer and François R. Bouchet and Marco Bruni and Erminia Calabrese and David Camarena and Salvatore Capozziello and Angela Chen and Jens Chluba and Anton Chudaykin and Eoin Ó Colgáin and Francis-Yan Cyr-Racine and Paolo de Bernardis and Javier de Cruz Pérez and Jacques Delabrouille and Jo Dunkley and Celia Escamilla-Rivera and Agnès Ferté and Fabio Finelli and Wendy Freedman and Noemi Frusciante and Elena Giusarma and Adrià Gómez-Valent and Will Handley and Ian Harrison and Luke Hart and Alan Heavens and Hendrik Hildebrandt and Daniel Holz and Dragan Huterer and Mikhail M. Ivanov and Shahab Joudaki and Marc Kamionkowski and Tanvi Karwal and Lloyd Knox and Suresh Kumar and Luca Lamagna and Julien Lesgourgues and Matteo Lucca and Valerio Marra and Silvia Masi and Sabino Matarrese and Arindam Mazumdar and Alessandro Melchiorri and Olga Mena and Laura Mersini-Houghton and Vivian Miranda and Cristian Moreno-Pulido and David F. Mota and Jessica Muir},
  journal = {Astroparticle Physics},
  year = {2026},
  month = sep,
  doi = {10.1016/j.astropartphys.2021.102604},
  eprint = {2008.11285},
  archivePrefix = {arXiv},
  url = {https://hal.science/hal-02939996v1},
  note = {CC BY-NC-ND 4.0},
}
RIS
TY  - JOUR
TI  - Cosmology intertwined III: fσ8 and S8
AU  - Eleonora Di Valentino
AU  - Luis A. Anchordoqui
AU  - Özgür Akarsu
AU  - Yacine Ali-Haimoud
AU  - Luca Amendola
AU  - Nikki Arendse
AU  - Marika Asgari
AU  - Mario Ballardini
AU  - Spyros Basilakos
AU  - Elia Battistelli
AU  - Micol Benetti
AU  - Simon Birrer
AU  - François R. Bouchet
AU  - Marco Bruni
AU  - Erminia Calabrese
AU  - David Camarena
AU  - Salvatore Capozziello
AU  - Angela Chen
AU  - Jens Chluba
AU  - Anton Chudaykin
AU  - Eoin Ó Colgáin
AU  - Francis-Yan Cyr-Racine
AU  - Paolo de Bernardis
AU  - Javier de Cruz Pérez
AU  - Jacques Delabrouille
AU  - Jo Dunkley
AU  - Celia Escamilla-Rivera
AU  - Agnès Ferté
AU  - Fabio Finelli
AU  - Wendy Freedman
AU  - Noemi Frusciante
AU  - Elena Giusarma
AU  - Adrià Gómez-Valent
AU  - Will Handley
AU  - Ian Harrison
AU  - Luke Hart
AU  - Alan Heavens
AU  - Hendrik Hildebrandt
AU  - Daniel Holz
AU  - Dragan Huterer
AU  - Mikhail M. Ivanov
AU  - Shahab Joudaki
AU  - Marc Kamionkowski
AU  - Tanvi Karwal
AU  - Lloyd Knox
AU  - Suresh Kumar
AU  - Luca Lamagna
AU  - Julien Lesgourgues
AU  - Matteo Lucca
AU  - Valerio Marra
AU  - Silvia Masi
AU  - Sabino Matarrese
AU  - Arindam Mazumdar
AU  - Alessandro Melchiorri
AU  - Olga Mena
AU  - Laura Mersini-Houghton
AU  - Vivian Miranda
AU  - Cristian Moreno-Pulido
AU  - David F. Mota
AU  - Jessica Muir
PY  - 2026
DA  - 2026/09/29
JO  - Astroparticle Physics
DO  - 10.1016/j.astropartphys.2021.102604
UR  - https://hal.science/hal-02939996v1
AB  - The standard Λ Cold Dark Matter cosmological model provides a wonderful fit to current cosmological data, but a few tensions and anomalies became statistically significant with the latest data analyses. While these anomalies could be due to the presence of systematic errors in the experiments, they could also indicate the need for new physics beyond the standard model. In this Letter of Interest we focus on the tension of the Planck data with weak lensing measurements and redshift surveys, about the value of the matter energy density Ω_m, and the amplitude or rate of the growth of structure (σ_8,fσ_8). We list a few interesting models for solving this tension, and we discuss the importance of trying to fit with a single model a full array of data and not just one parameter at a time.
SN  - 0927-6505
SN  - 1873-2852
ER  -