@Article{DiValentinoAAAAAABBBBBBBCCCCCCCCBPDDEFFFFGGGHHHHHHHIJKKKKLLLMMMMMMMMMMMMNNNPPPPPPPPRRSSSSSSSSSPBVVWWWYY:2021:HuCoTe,
author = "Di Valentino, Eleonora and Anchordoqui, Luis A. and Akarsu, Ozgur
and Ali-Haimoud, Yacine and Amendola, Luca and Arendse, Nikki and
Asgari, Marika and Ballardini, Mario and Basilakos, Spyros and
Battistelli, Elia and Benetti, Micol and Birrer, Simon and
Bouchet, Francois R. and Bruni, Marco and Calabrese, Erminia and
Camarena, David and Capozziello, Salvatore and Chen, Angela and
Chluba, Jens and Chudaykin, Anton and Colgain, Eoin O. and
Cyr-Racine, Francis-Yan and de Bernardis, Paolo and Perez, Javier
de Cruz and Delabrouille, Jacques and Dunkley, Jo and
Escamilla-Rivera, Celia and Ferte, Agnes and Finelli, Fabio and
Freedman, Wendy and Frusciante, Noemi and Giusarma, Elena and
Gomez-Valent, Adria and Guy, Julien and Handley, Will and
Harrison, Ian and Hart, Luke and Heavens, Alan and Hildebrandt,
Hendrik and Holz, Daniel and Huterer, Dragan and Ivanov, Mikhail
M. and Joudaki, Shahab and Kamionkowski, Marc and Karwal, Tanvi
and Knox, Lloyd and Kumar, Suresh and Lamagna, Luca and
Lesgourgues, Julien and Lucca, Matteo and Marra, Valerio and Masi,
Silvia and Matarrese, Sabino and Mazumdar, Arindam and Melchiorri,
Alessandro and Mena, Olga and Mersini-Houghton, Laura and Miranda,
Vivian and Moreno-Pulido, Cristian and Mota, David F. and Muir,
Jessica and Mukherjee, Ankan and Niedermann, Florian and Notari,
Alessio and Nunes, Rafael da Costa and Pace, Francesco and
Paliathanasis, Andronikos and Palmese, Antonella and Pan, Supriya
and Paoletti, Daniela and Pettorino, Valeria and Piacentini,
Francesco and Poulin, Vivian and Raveri, Marco and Riess, Adam G.
and Salzano, Vincenzo and Saridakis, Emmanuel N. and Sen, Anjan A.
and Shafieloo, Arman and Shajib, Anowar J. and Silk, Joseph and
Silvestri, Alessandra and Sloth, Martin S. and Smith, Tristan L.
and Peracaula, Joan Sola and van de Bruck, Carsten and Verde,
Licia and Visinelli, Luca and Wandelta, Benjamin D. and Wang, Deng
and Wang, Jian-Min and Yadav, Anil K. and Yang, Weiqiang",
affiliation = "Univ Manchester, JBCA, Manchester, Lancs, England. and CUNY, New
York, NY 10021 USA. and Istanbul Tech Univ, Istanbul, Turkey. and
NYU, New York, NY USA. and Heidelberg Univ, Heidelberg, Germany.
and Niels Bohr Inst, DARK, Copenhagen, Denmark. and Univ
Edinburgh, Edinburgh, Midlothian, Scotland. and Alma Mater
Studiorum Univ Bologna, Bologna, Italy. and Acad Athens, Athens,
Greece.; Nat Observ Athens, Athens, Greece. and Sapienza Univ
Roma, Rome, Italy.; Ist Nazl Fis Nucl, Sez Roma, Rome, Italy. and
Univ Napoli Federico II, Naples, Italy.; Ist Nazl Fis Nucl, Sez
Napoli, Naples, Italy. and Stanford Univ, Stanford, CA 94305 USA.
and CNRS, Inst Astrophys Paris, Paris, France.; Sorbonne Univ,
Paris, France. and Inst Cosmol \& Gravitat, Portsmouth, Hants,
England.; Ist Nazl Fis Nucl, Sez Trieste, Trieste, Italy. and
Cardiff Univ, Cardiff, Wales. and Univ Fed Espirito Santo,
Vitoria, ES, Brazil. and Univ Napoli Federico II, Naples, Italy.;
Ist Nazl Fis Nucl, Sez Napoli, Naples, Italy. and Univ Michigan,
Ann Arbor, MI 48109 USA. and Univ Manchester, JBCA, Manchester,
Lancs, England. and Inst Nucl Res, Dubna, Russia. and Asia Pacific
Ctr Theoret Phys, Seoul, South Korea. and Univ New Mexico,
Albuquerque, NM 87131 USA. and Sapienza Univ Roma, Rome, Italy.;
Ist Nazl Fis Nucl, Sez Roma, Rome, Italy. and Univ Barcelona, Dept
FQA, Barcelona, Spain.; Univ Barcelona, ICCUB, Barcelona, Spain.
and CNRS IN2P3, Lab APC, Paris, France.; CEA IRFU, Saclay,
France.; UST, Hefei, Peoples R China. and Princeton Univ,
Princeton, NJ 08544 USA. and Univ Nacl Autonoma Mexico, ICN,
Mexico City, DF, Mexico. and CALTECH, JPL, Pasadena, CA USA. and
INAF OAS Bologna, Bologna, Italy.; Ist Nazl Fis Nucl, Sez Bologna,
Bologna, Italy. and Univ Chicago, Chicago, IL 60637 USA. and Inst
Astrofis \& Ciencias Espaco, Lisbon, Portugal. and Michigan
Technol Univ, Houghton, MI 49931 USA. and Heidelberg Univ,
Heidelberg, Germany. and Lawrence Berkeley Natl Lab, Berkeley, CA
USA. and Univ Cambridge, Cambridge, England. and Univ Manchester,
JBCA, Manchester, Lancs, England. and Univ Manchester, JBCA,
Manchester, Lancs, England. and Imperial Coll London, ICIC,
London, England. and Ruhr Univ Bochum, Bochum, Germany. and Univ
Chicago, Chicago, IL 60637 USA. and Univ Michigan, Ann Arbor, MI
48109 USA. and NYU, New York, NY USA. and Univ Oxford, Oxford,
England.; Univ Waterloo, Waterloo, ON, Canada. and Johns Hopkins
Univ, Baltimore, MD USA. and Univ Penn, Philadelphia, PA 19104
USA. and Univ Calif Davis, Davis, CA USA. and BITS Pilani, Pilani
Campus, Pilani, Rajasthan, India. and Sapienza Univ Roma, Rome,
Italy.; Ist Nazl Fis Nucl, Sez Roma, Rome, Italy. and Rhein
Westfal TH Aachen, Aachen, Germany. and Univ Libre Bruxelles,
Brussels, Belgium. and Univ Fed Espirito Santo, Vitoria, ES,
Brazil. and Sapienza Univ Roma, Rome, Italy.; Ist Nazl Fis Nucl,
Sez Roma, Rome, Italy. and Univ Padua, Padua, Italy.; Ist Nazl Fis
Nucl, Sez Padova, Padua, Italy. and IIT Kharagpur, Ctr Theoret
Studies, Kharagpur, W Bengal, India. and Sapienza Univ Roma, Rome,
Italy.; Ist Nazl Fis Nucl, Sez Roma, Rome, Italy. and CSIC UV,
IFIC, Barcelona, Spain. and Univ N Carolina, Chapel Hill, NC 27515
USA. and Univ Arizona, Tucson, AZ 85721 USA. and Univ Barcelona,
Dept FQA, Barcelona, Spain.; Univ Barcelona, ICCUB, Barcelona,
Spain. and Univ Oslo, Oslo, Norway. and Stanford Univ, KIPAC,
Stanford, CA 94305 USA. and Jamia Millia Islamia, New Delhi,
India. and Univ Southern Denmark, CP3 Origins, Aarhus, Denmark.
and Univ Barcelona, ICCUB, Barcelona, Spain. and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and Univ Manchester, JBCA,
Manchester, Lancs, England. and DUT, Durban, South Africa.; UACh,
Santiago, Chile. and Fermilab Natl Accelerator Lab, POB 500,
Batavia, IL 60510 USA. and Presidency Univ, Kolkata, India. and
INAF OAS Bologna, Bologna, Italy.; Ist Nazl Fis Nucl, Sez Bologna,
Bologna, Italy. and Univ Paris, Univ Paris Saclay, CNRS, CEA,AIM,
Paris, France. and Sapienza Univ Roma, Rome, Italy.; Ist Nazl Fis
Nucl, Sez Roma, Rome, Italy. and CNRS, LUPM, Paris, France.; Univ
Montpellier, Montpellier, France. and Univ Penn, Philadelphia, PA
19104 USA. and Johns Hopkins Univ, Baltimore, MD USA. and Univ
Szczecin, Szczecin, Poland. and Natl Observ Athens, Athens,
Greece. and Jamia Millia Islamia, New Delhi, India. and Korea
Astron \& Space Sci Inst KASI, Daejeon, South Korea. and Univ
Calif Los Angeles, Los Angeles, CA USA. and Johns Hopkins Univ,
Baltimore, MD USA.; Sorbonne Univ, IAP, Paris, France.; CNRS,
Paris, France. and Leiden Univ, Leiden, Netherlands. and Univ
Southern Denmark, CP3 Origins, Aarhus, Denmark. and Swarthmore
Coll, Swarthmore, PA 19081 USA. and Univ Barcelona, Dept FQA,
Barcelona, Spain.; Univ Barcelona, ICCUB, Barcelona, Spain. and
Univ Sheffield, Sheffield, S Yorkshire, England. and Univ
Barcelona, ICREA, Icrea, Spain. and Univ Amsterdam, GRAPPA,
Amsterdam, Netherlands. and Sorbonne Univ, IAP, Paris, France.;
CNRS, Paris, France.; CCA, Oakland, CA USA. and Chinese Acad Sci,
Natl Astron Observ, Beijing, Peoples R China. and Chinese Acad
Sci, Key Lab Particle Astrophys, IHEP, Beijing, Peoples R China.
and United Coll Engn \& Res, Gn, India. and Liaoning Normal Univ,
Dalian, Peoples R China.",
title = "Snowmass2021-Letter of interest cosmology intertwined II: The
hubble constant tension",
journal = "Astroparticle Physics",
year = "2021",
volume = "131",
month = "Sep.",
abstract = "The current cosmological probes have provided a fantastic
confirmation of the standard A Cold Dark Matter cosmological
model, which has been constrained with unprecedented accuracy.
However, with the increase of the experimental sensitivity, a few
statistically significant tensions between different independent
cosmological datasets emerged. While these tensions can be in part
the result of systematic errors, the persistence after several
years of accurate analysis strongly hints at cracks in the
standard cosmological scenario and the need for new physics. In
this Letter of Interest we will focus on the 4.4 sigma - tension
between the Planck estimate of the Hubble constant H-0 and the
SH0ES collaboration measurements. After showing the H-0
evaluations made from different teams using different methods and
geometric calibrations, we will list a few interesting models of
new physics that could solve this tension and discuss how the next
decade's experiments will be crucial. (C) 2021 Elsevier B.V. All
rights reserved.",
doi = "10.1016/j.astropartphys.2021.102605",
url = "http://dx.doi.org/10.1016/j.astropartphys.2021.102605",
issn = "0927-6505",
label = "20210623",
language = "en",
targetfile = "valentino_iii.pdf",
urlaccessdate = "20 maio 2024"
}