Cosmology intertwined III: fσ8 and S8

The standard Λ Cold Dark Matter cosmological model provides a wonderful fit to current cosmological data, but a few statistically significant tensions and anomalies were found in the latest data analyses. While these anomalies could be due to the presence of systematic errors in the experiments, the...

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Published inAstroparticle physics Vol. 131
Main Authors Di Valentino, Eleonora, Anchordoqui, Luis A., Akarsu, Özgür, Ali-Haimoud, Yacine, Amendola, Luca, Arendse, Nikki, Asgari, Marika, Ballardini, Mario, Basilakos, Spyros, Battistelli, Elia, Benetti, Micol, Birrer, Simon, Bouchet, François R., Bruni, Marco, Calabrese, Erminia, Camarena, David, Capozziello, Salvatore, Chen, Angela, Chluba, Jens, Chudaykin, Anton, Colgáin, Eoin Ó, Cyr-Racine, Francis-Yan, de Bernardis, Paolo, de Cruz Pérez, Javier, Delabrouille, Jacques, Dunkley, Jo, Escamilla-Rivera, Celia, Ferté, Agnès, Finelli, Fabio, Freedman, Wendy, Frusciante, Noemi, Giusarma, Elena, Gómez-Valent, Adrià, Handley, Will, Harrison, Ian, Hart, Luke, Heavens, Alan, Hildebrandt, Hendrik, Holz, Daniel, Huterer, Dragan, Ivanov, Mikhail M., Joudaki, Shahab, Kamionkowski, Marc, Karwal, Tanvi, Knox, Lloyd, Kumar, Suresh, Lamagna, Luca, Lesgourgues, Julien, Lucca, Matteo, Marra, Valerio, Masi, Silvia, Matarrese, Sabino, Mazumdar, Arindam, Melchiorri, Alessandro, Mena, Olga, Mersini-Houghton, Laura, Miranda, Vivian, Moreno-Pulido, Cristian, Mota, David F., Muir, Jessica, Mukherjee, Ankan, Niedermann, Florian, Notari, Alessio, Nunes, Rafael C., Pace, Francesco, Paliathanasis, Andronikos, Palmese, Antonella, Pan, Supriya, Paoletti, Daniela, Pettorino, Valeria, Piacentini, Francesco, Poulin, Vivian, Raveri, Marco, Riess, Adam G., Salzano, Vincenzo, Saridakis, Emmanuel N., Sen, Anjan A., Shafieloo, Arman, Shajib, Anowar J., Silk, Joseph, Silvestri, Alessandra, Sloth, Martin S., Smith, Tristan L., Solà Peracaula, Joan, van de Bruck, Carsten, Verde, Licia, Visinelli, Luca, Wandelt, Benjamin D., Wang, Deng, Wang, Jian-Min, Yadav, Anil K., Yang, Weiqiang
Format Journal Article
LanguageEnglish
Published Elsevier B.V 01.09.2021
Subjects
cosmological parameters
cosmological tensions
cosmological tensions
cosmological parameters
Online AccessGet full text
ISSN0927-6505
1873-2852
DOI10.1016/j.astropartphys.2021.102604

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Abstract The standard Λ Cold Dark Matter cosmological model provides a wonderful fit to current cosmological data, but a few statistically significant tensions and anomalies were found in 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 between Planck data and weak lensing measurements and redshift surveys, in the value of the matter energy density Ωm and the amplitude σ8 (or the growth rate fσ8) of cosmic structure. We list a few promising models for solving this tension, and discuss the importance of trying to fit multiple cosmological datasets with complete physical models, rather than fitting individual datasets with a few handpicked theoretical parameters.
AbstractList The standard Λ Cold Dark Matter cosmological model provides a wonderful fit to current cosmological data, but a few statistically significant tensions and anomalies were found in 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 between Planck data and weak lensing measurements and redshift surveys, in the value of the matter energy density Ωm and the amplitude σ8 (or the growth rate fσ8) of cosmic structure. We list a few promising models for solving this tension, and discuss the importance of trying to fit multiple cosmological datasets with complete physical models, rather than fitting individual datasets with a few handpicked theoretical parameters.
ArticleNumber 102604
Author Delabrouille, Jacques
Dunkley, Jo
Giusarma, Elena
Mukherjee, Ankan
Saridakis, Emmanuel N.
Benetti, Micol
Poulin, Vivian
Basilakos, Spyros
Karwal, Tanvi
Chudaykin, Anton
Harrison, Ian
Pan, Supriya
Muir, Jessica
Pace, Francesco
Kamionkowski, Marc
Mersini-Houghton, Laura
Salzano, Vincenzo
Silk, Joseph
Camarena, David
Shafieloo, Arman
van de Bruck, Carsten
Ali-Haimoud, Yacine
de Cruz Pérez, Javier
Lamagna, Luca
Solà Peracaula, Joan
Ballardini, Mario
Battistelli, Elia
Mena, Olga
Ivanov, Mikhail M.
Bruni, Marco
Asgari, Marika
Hildebrandt, Hendrik
Melchiorri, Alessandro
de Bernardis, Paolo
Escamilla-Rivera, Celia
Frusciante, Noemi
Masi, Silvia
Knox, Lloyd
Nunes, Rafael C.
Paliathanasis, Andronikos
Wang, Jian-Min
Chluba, Jens
Moreno-Pulido, Cristian
Amendola, Luca
Hart, Luke
Mazumdar, Arindam
Raveri, Marco
Miranda, Vivian
Smith, Tristan L.
Palmese, Antonella
Huterer, Dragan
Akarsu, Özgür
Ferté, Agnès
Lucca, Matteo
Calabrese, Erminia
Matarrese, Sabino
Wandelt, Benjamin D.
Capozziello, Salvatore
Yang, Weiqiang
Sloth, Martin S.
Shajib, Anowar J.
Wang, Deng
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Snippet The standard Λ Cold Dark Matter cosmological model provides a wonderful fit to current cosmological data, but a few statistically significant tensions and...
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SourceType Publisher
SubjectTerms cosmological parameters
cosmological tensions
Title Cosmology intertwined III: fσ8 and S8
URI https://dx.doi.org/10.1016/j.astropartphys.2021.102604
Volume 131
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