Abstract
The standard A 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 Omega(m), and the amplitude sigma(8) (or the growth rate f sigma(8)) 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. (C) 2021 Elsevier B.V. All rights reserved.
Original language | English |
---|---|
Article number | 102604 |
Journal | Astroparticle Physics |
Volume | 131 |
Number of pages | 6 |
ISSN | 0927-6505 |
DOIs | |
Publication status | Published - Sep 2021 |
Keywords
- cosmological tensions
- cosmological parameters
- RUNNING VACUUM
- COSMIC SHEAR
- DARK ENERGY
- PLANCK
- CONSTRAINTS
- CFHTLENS
- CONCORDANCE
- SYSTEMATICS
- CATALOG
- GROWTH
Access to Document
Cite this
- APA
- Standard
- Harvard
- Vancouver
- Author
- BIBTEX
- RIS
Cosmology intertwined III : fσ8 and S8. / Di Valentino, Eleonora; Anchordoqui, Luis A.; Akarsu, Ozgur; Ali-Haimoud, Yacine; Amendola, Luca; Arendse, Nikki; Asgari, Marika; Ballardini, Mario; Basilakos, Spyros; Battistelli, Elia; Benetti, Micol; Birrer, Simon; Bouchet, Francois R.; Bruni, Marco; Calabrese, Erminia; Camarena, David; Capozziello, Salvatore; Chen, Angela; Chluba, Jens; Chudaykin, Anton; Colgain, Eoin O.; Cyr-Racine, Francis-Yan; de Bernardis, Paolo; Perez, Javier de Cruz; Delabrouille, Jacques; Dunkley, Jo; Escamilla-Rivera, Celia; Ferte, Agnes; Finelli, Fabio; Freedman, Wendy; Frusciante, Noemi; Giusarma, Elena; Gomez-Valent, Adria; 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.; Sola, Joan; van de Bruck, Carsten; Verde, Licia; Visinelli, Luca; Wandelt, Benjamin D.; Wang, Deng; Wang, Jian-Min; Yadav, Anil K.; Yang, Weiqiang.
In: Astroparticle Physics, Vol. 131, 102604, 09.2021.Research output: Contribution to journal › Journal article › Research › peer-review
}
TY - JOUR
T1 - Cosmology intertwined III
T2 - fσ8 and S8
AU - Di Valentino, Eleonora
AU - Anchordoqui, Luis A.
AU - Akarsu, Ozgur
AU - Ali-Haimoud, Yacine
AU - Amendola, Luca
AU - Arendse, Nikki
AU - Asgari, Marika
AU - Ballardini, Mario
AU - Basilakos, Spyros
AU - Battistelli, Elia
AU - Benetti, Micol
AU - Birrer, Simon
AU - Bouchet, Francois R.
AU - Bruni, Marco
AU - Calabrese, Erminia
AU - Camarena, David
AU - Capozziello, Salvatore
AU - Chen, Angela
AU - Chluba, Jens
AU - Chudaykin, Anton
AU - Colgain, Eoin O.
AU - Cyr-Racine, Francis-Yan
AU - de Bernardis, Paolo
AU - Perez, Javier de Cruz
AU - Delabrouille, Jacques
AU - Dunkley, Jo
AU - Escamilla-Rivera, Celia
AU - Ferte, Agnes
AU - Finelli, Fabio
AU - Freedman, Wendy
AU - Frusciante, Noemi
AU - Giusarma, Elena
AU - Gomez-Valent, Adria
AU - Handley, Will
AU - Harrison, Ian
AU - Hart, Luke
AU - Heavens, Alan
AU - Hildebrandt, Hendrik
AU - Holz, Daniel
AU - Huterer, Dragan
AU - Ivanov, Mikhail M.
AU - Joudaki, Shahab
AU - Kamionkowski, Marc
AU - Karwal, Tanvi
AU - Knox, Lloyd
AU - Kumar, Suresh
AU - Lamagna, Luca
AU - Lesgourgues, Julien
AU - Lucca, Matteo
AU - Marra, Valerio
AU - Masi, Silvia
AU - Matarrese, Sabino
AU - Mazumdar, Arindam
AU - Melchiorri, Alessandro
AU - Mena, Olga
AU - Mersini-Houghton, Laura
AU - Miranda, Vivian
AU - Moreno-Pulido, Cristian
AU - Mota, David F.
AU - Muir, Jessica
AU - Mukherjee, Ankan
AU - Niedermann, Florian
AU - Notari, Alessio
AU - Nunes, Rafael C.
AU - Pace, Francesco
AU - Paliathanasis, Andronikos
AU - Palmese, Antonella
AU - Pan, Supriya
AU - Paoletti, Daniela
AU - Pettorino, Valeria
AU - Piacentini, Francesco
AU - Poulin, Vivian
AU - Raveri, Marco
AU - Riess, Adam G.
AU - Salzano, Vincenzo
AU - Saridakis, Emmanuel N.
AU - Sen, Anjan A.
AU - Shafieloo, Arman
AU - Shajib, Anowar J.
AU - Silk, Joseph
AU - Silvestri, Alessandra
AU - Sloth, Martin S.
AU - Smith, Tristan L.
AU - Sola, Joan
AU - van de Bruck, Carsten
AU - Verde, Licia
AU - Visinelli, Luca
AU - Wandelt, Benjamin D.
AU - Wang, Deng
AU - Wang, Jian-Min
AU - Yadav, Anil K.
AU - Yang, Weiqiang
PY - 2021/9
Y1 - 2021/9
N2 - The standard A 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 Omega(m), and the amplitude sigma(8) (or the growth rate f sigma(8)) 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. (C) 2021 Elsevier B.V. All rights reserved.
AB - The standard A 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 Omega(m), and the amplitude sigma(8) (or the growth rate f sigma(8)) 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. (C) 2021 Elsevier B.V. All rights reserved.
KW - cosmological tensions
KW - cosmological parameters
KW - RUNNING VACUUM
KW - COSMIC SHEAR
KW - DARK ENERGY
KW - PLANCK
KW - CONSTRAINTS
KW - CFHTLENS
KW - CONCORDANCE
KW - SYSTEMATICS
KW - CATALOG
KW - GROWTH
U2 - 10.1016/j.astropartphys.2021.102604
DO - 10.1016/j.astropartphys.2021.102604
M3 - Journal article
VL - 131
JO - Astroparticle Physics
JF - Astroparticle Physics
SN - 0927-6505
M1 - 102604
ER -