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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/47CHQ68
Repositorysid.inpe.br/mtc-m21d/2022/08.02.13.22   (restricted access)
Last Update2022:08.02.13.25.10 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2022/08.02.13.22.32
Metadata Last Update2023:01.03.16.46.11 (UTC) administrator
DOI10.1016/j.jheap.2022.04.002
ISSN2214-4048
Label20220802
Citation KeyAbdallaAAAAAAAAAAAABBBBBBBBBBBBBBBBBBBBBBCCCCCCCCCCCCCCCDDDCHDDDDDDEEFFFFFGGGGHHHHHHHHHHHHHIIJJJJJJKKKKKKKKLLLLLLLLMMMMMMMMMMMMMMMMMMMMMMMNNNNNNCOÖPPPPPPPPPPPPPRRRRSSSSSSSSSSSSSSSSSSSSSSSTTTTBVVVWWWWWWWWWWYYZZ:2022:RePaPh
TitleCosmology intertwined: A review of the particle physics, astrophysics, and cosmology associated with the cosmological tensions and anomalies
Year2022
MonthJune
Access Date2024, May 14
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size10254 KiB
2. Context
Author  1 Abdalla, Elcio
  2 Abellán, Guillermo Franco
  3 Aboubrahim, Amin
  4 Agnello, Adriano
  5 Akarsu, Özgür
  6 Akrami, Yashar
  7 Alestas, George
  8 Aloni, Daniel
  9 Amendola, Luca
 10 Anchordoqui, Luis A.
 11 Anderson, Richard I.
 12 Arendse, Nikki
 13 Asgari, Marika
 14 Ballardini, Mario
 15 Barger, Vernon
 16 Basilakos, Spyros
 17 Batista, Ronaldo C.
 18 Battistelli, Elia S.
 19 Battye, Richard
 20 Benetti, Micol
 21 Benisty, David
 22 Berlin, Asher
 23 de Bernardis, Paolo
 24 Berti, Emanuele
 25 Bidenko, Bohdan
 26 Birrer, Simon
 27 Blakeslee, John P.
 28 Boddy, Kimberly K.
 29 Bom, Clecio R.
 30 Bonilla, Alexander
 31 Borghi, Nicola
 32 Bouchet, François R.
 33 Braglia, Matteo
 34 Buchert, Thomas
 35 Buckley-Geer, Elizabeth
 36 Calabrese, Erminia
 37 Caldwell, Robert R.
 38 Camarena, David
 39 Capozziello, Salvatore
 40 Casertano, Stefano
 41 Chen, Geoff C. -F.
 42 Chluba, Jens
 43 Chen, Angela
 44 Chen, Hsin-Yu
 45 Chudaykin, Anton
 46 Cicoli, Michele
 47 Copi, Craig J.
 48 Courbin, Fred
 49 Cyr-Racine, Francis-Yan
 50 Czerny, Bo|ena
 51 Dainotti, Maria
 52 D'Amico, Guido
 53 Davis, Anne-Christine
 54 de Cruz Pérez, Javier
 55 de Haro, Jaume
 56 Delabrouille, Jacques
 57 Denton, Peter B.
 58 Dhawan, Suhail
 59 Dienes, Keith R.
 60 Di Valentino, Eleonora
 61 Du, Pu
 62 Eckert, Dominique
 63 Escamilla-Rivera, Celia
 64 Ferté, Agnès
 65 Finelli, Fabio
 66 Fosalba, Pablo
 67 Freedman, Wendy L.
 68 Frusciante, Noemi
 69 Gaztañaga, Enrique
 70 Giarè, William
 71 Giusarma, Elena
 72 Gómez-Valent, AdriÃ
 73 Handley, Will
 74 Harrison, Ian
 75 Hart, Luke
 76 Hazra, Dhiraj Kumar
 77 Heavens, Alan
 78 Heinesen, Asta
 79 Hildebrandt, Hendrik
 80 Hill, J. Colin
 81 Hogg, Natalie B.
 82 Holz, Daniel E.
 83 Hooper, Deanna C.
 84 Hosseininejad, Nikoo
 85 Huterer, Dragan
 86 Ishak, Mustapha
 87 Ivanov, Mikhail M.
 88 Jaffe, Andrew H.
 89 Jang, In Sung
 90 Jedamzik, Karsten
 91 Jimenez, Raul
 92 Joseph, Melissa
 93 Joudaki, Shahab
 94 Kamionkowski, Marc
 95 Karwal, Tanvi
 96 Kazantzidis, Lavrentios
 97 Keeley, Ryan E.
 98 Klasen, Michael
 99 Komatsu, Eiichiro
100 Koopmans, Léon V. E.
101 Kumar, Suresh
102 Lamagna, Luca
103 Lazkoz, Ruth
104 Lee, Chung-Chi
105 Lesgourgues, Julien
106 Levi Said, Jackson
107 Lewis, Tiffany R.
108 L'Huillier, Benjamin
109 Lucca, Matteo
110 Maartens, Roy
111 Macri, Lucas M.
112 Marfatia, Danny
113 Marra, Valerio
114 Martins, Carlos J. A. P.
115 Masi, Silvia
116 Matarrese, Sabino
117 Mazumdar, Arindam
118 Melchiorri, Alessandro
119 Mena, Olga
120 Mersini-Houghton, Laura
121 Mertens, James
122 Milakovi, Dinko
123 Minami, Yuto
124 Miranda, Vivian
125 Moreno-Pulido, Cristian
126 Moresco, Michele
127 Mota, David F.
128 Mottola, Emil
129 Mozzon, Simone
130 Muir, Jessica
131 Mukherjee, Ankan
132 Mukherjee, Suvodip
133 Naselsky, Pavel
134 Nath, Pran
135 Nesseris, Savvas
136 Niedermann, Florian
137 Notari, Alessio
138 Nunes, Rafael da Costa
139 Colgáin, Eoin Ó
140 Owens, Kayla A.
141 Özülker, Emre
142 Pace, Francesco
143 Paliathanasis, Andronikos
144 Palmese, Antonella
145 Pan, Supriya
146 Paoletti, Daniela
147 Perez Bergliaffa, Santiago E.
148 Perivolaropoulos, Leandros
149 Pesce, Dominic W.
150 Pettorino, Valeria
151 Philcox, Oliver H. E.
152 Pogosian, Levon
153 Poulin, Vivian
154 Poulot, Gaspard
155 Raveri, Marco
156 Reid, Mark J.
157 Renzi, Fabrizio
158 Riess, Adam G.
159 Sabla, Vivian I.
160 Salucci, Paolo
161 Salzano, Vincenzo
162 Saridakis, Emmanuel N.
163 Sathyaprakash, Bangalore S.
164 Schmaltz, Martin
165 Schöneberg, Nils
166 Scolnic, Dan
167 Sen, Anjan A.
168 Sehgal, Neelima
169 Shafieloo, Arman
170 Sheikh-Jabbari, M. M.
171 Silk, Joseph
172 Silvestri, Alessandra
173 Skara, Foteini
174 Sloth, Martin S.
175 Soares-Santos, Marcelle
176 Solà Peracaula, Joan
177 Songsheng, Yu-Yang
178 Soriano, Jorge F.
179 Staicova, Denitsa
180 Starkman, Glenn D.
181 Szapudi, István
182 Teixeira, Elsa M.
183 Thomas, Brooks
184 Treu, Tommaso
185 Trott, Emery
186 van de Bruck, Carsten
187 Vazquez, J. Alberto
188 Verde, Licia
189 Visinelli, Luca
190 Wang, Deng
191 Wang, Jian-Min
192 Wang, Shao-Jiang
193 Watkins, Richard
194 Watson, Scott
195 Webb, John K.
196 Weiner, Neal
197 Weltman, Amanda
198 Witte, Samuel J.
199 Wojtak, RadosBaw
200 Yadav, Anil Kumar
201 Yang, Weiqiang
202 Zhao, Gong-Bo
203 Zumalacárregui, Miguel
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138 DIAST-CGCE-INPE-MCTI-GOV-BR
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138 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address  1
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138 rafadcnunes@gmail.com
JournalJournal of High Energy Astrophysics
Volume34
Pages49-211
History (UTC)2022-08-02 13:22:32 :: administrator -> simone ::
2022-08-02 13:25:19 :: simone -> administrator :: 2022
2023-01-03 16:46:11 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractThe standard Λ Cold Dark Matter (ΛCDM) cosmological model provides a good description of a wide range of astrophysical and cosmological data. However, there are a few big open questions that make the standard model look like an approximation to a more realistic scenario yet to be found. In this paper, we list a few important goals that need to be addressed in the next decade, taking into account the current discordances between the different cosmological probes, such as the disagreement in the value of the Hubble constant H0, the σ8S8 tension, and other less statistically significant anomalies. While these discordances can still be in part the result of systematic errors, their persistence after several years of accurate analysis strongly hints at cracks in the standard cosmological scenario and the necessity for new physics or generalisations beyond the standard model. In this paper, we focus on the 5.0σ tension between the Planck CMB estimate of the Hubble constant H0 and the SH0ES collaboration measurements. After showing the H0 evaluations made from different teams using different methods and geometric calibrations, we list a few interesting new physics models that could alleviate this tension and discuss how the next decade's experiments will be crucial. Moreover, we focus on the tension of the Planck CMB 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 proposed for alleviating this tension, and we discuss the importance of trying to fit a full array of data with a single model and not just one parameter at a time. Additionally, we present a wide range of other less discussed anomalies at a statistical significance level lower than the H0S8 tensions which may also constitute hints towards new physics, and we discuss possible generic theoretical approaches that can collectively explain the non-standard nature of these signals. Finally, we give an overview of upgraded experiments and next-generation space missions and facilities on Earth that will be of crucial importance to address all these open questions.
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Target File1-s2.0-S2214404822000179-main.pdf
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Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/bibdigital/2022/04.03.17.52 3
DisseminationSCOPUS
Host Collectionurlib.net/www/2021/06.04.03.40
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