Extended gravity cosmography
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In this paper, the success and the shortcomings of the ΛCDM model, based on cosmography, are discussed and a review of the model's performance is presented. But the model is not considered as a sort of a model-independent approach to tackle the dark energy/modified gravity problem.Abstract:
Cosmography can be considered as a sort of a model-independent approach to tackle the dark energy/modified gravity problem. In this review, the success and the shortcomings of the ΛCDM model, based...read more
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Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
Elcio Abdalla,G. F. Abell'an,Amin Aboubrahim,Adriano Agnello,Ozgur Akarsu,Yashar Akrami,George Alestas,Daniel Aloni,Luca Amendola,Luis A. Anchordoqui,Richard I. Anderson,Nikki Arendse,Marika Asgari,Mario Ballardini,Vernon Barger,Spyros Basilakos,R. C. Batista,Elia S. Battistelli,Richard A. Battye,Micol Benetti,David Benisty,Asher Berlin,P. de Bernardis,Emanuele Berti,Bohdan Bidenko,Simon Birrer,John P. Blakeslee,Kimberly K. Boddy,Clecio R. Bom,Alexander Bonilla,Nicolas Borghi,F. R. Bouchet,Matteo Braglia,Thomas Buchert,E. Buckley-Geer,Erminia Calabrese,Robert R. Caldwell,David Camarena,Salvatore Capozziello,Stefano Casertano,Geoff C. F. Chen,Jens Chluba,Angela Chen,Hsin-Yu Chen,Anton Chudaykin,Michele Cicoli,Craig J. Copi,Frederic Courbin,Francis-Yan Cyr-Racine,Bozena Czerny,Maria Giovanna Dainotti,Guido D'Amico,Anne-Christine Davis,Javier P'erez,Jaume Haro,Jacques Delabrouille,Peter B. Denton,Suhail Dhawan,Keith R. Dienes,E. Di Valentino,Pu Du,Dominique Eckert,Celia Escamilla-Rivera,A. Fert'e,Fabio Finelli,Pablo Fosalba,Wendy L. Freedman,Noemi Frusciante,Enrique Gaztanaga,William Giarè,Elena Giusarma,Adria G'omez-Valent,Will Handley,Ian Harrison,Luke Hart,Dhiraj Kumar Hazra,Alan Heavens,Asta Heinesen,Hendrik Hildebrandt,Jessica C Hill,Natalie B. Hogg,Daniel E. Holz,Deanna C. Hooper,Nikoo Hosseininejad,Dragan Huterer,Mustapha Ishak,Mikhail M. Ivanov,Andrew H. Jaffe,In Sung Jang,Karsten Jedamzik,Raul Jimenez,Melissa Joseph,Shahab Joudaki,Marc Kamionkowski,Tanvi Karwal,Lavrentios Kazantzidis,Ryan E. Keeley,Michael Klasen,Eiichiro Komatsu,Léon V. E. Koopmans,Suresh Kumar,Luca Lamagna,Ruth Lazkoz,Chung-Chi Lee,Julien Lesgourgues,Jackson Levi Said,Tiffany R. Lewis,Benjamin L'Huiller,Matteo Lucca,Roy Maartens,Lucas M. Macri,Danny Marfatia,Valerio Marra,Carlos Martins,Silvia Masi,Sabino Matarrese,Arindam Mazumdar,Alessandro Melchiorri,Olga Mena,Laura Mersini-Houghton,James B. Mertens,Dinko Milaković,Yuto Minami,V. Miranda,Cristian Moreno-Pulido,Michele Ennio Maria Moresco,David F. Mota,Emil Mottola,Simone Mozzon,J. Muir,Ankan Mukherjee,Suvodip Mukherjee,Pavel Naselsky,Pran Nath,Savvas Nesseris,Florian Niedermann,Alessio Notari,Rafael C. Nunes,Eoin 'O Colg'ain,Kayla A. Owens,Emre Ozulker,Francesco Paresce,Andronikos Paliathanasis,Antonella Palmese,Supriya Pan,Daniela Paoletti,S. E. Perez Bergliaffa,Leadros Perivolaropoulos,Dominic W. Pesce,Valeria Pettorino,Oliver H. E. Philcox,Levon Pogosian,Vivian Poulin,Gaspard Poulot,Marco Roveri,Mark J. Reid,F. Renzi,Adam G. Riess,V. I. Sabla,Paolo Salucci,Vincenzo Salzano,Emmanuel N. Saridakis,Bangalore Suryanarayana Sathyaprakash,Martin Schmaltz,N. Schoneberg,Daniel Scolnic,Anjan A. Sen,Neelima Sehgal,Arman Shafieloo,Mohammmad Mahdi Sheikh-Jabbari,Joseph Silk,Alessandra Silvestri,Foteini Skara,Martin S. Sloth,Marcelle Soares-Santos,Joan Solà Peracaula,Yu-Yang Songsheng,Jorge F. Soriano,Denitsa Staicova,Glenn D. Starkman,István Szapudi,E. Teixera,Brooks Thomas,Tommaso Treu,E. Trott,Carsten van de Bruck,Jose Alberto Vazquez,Licia Verde,Luca Visinelli,Deng Wang,Jian-Min Wang,Shao-Jiang Wang,Richard Watkins,Scott Watson,John K. Webb,Neal Weiner,Amanda Weltman,Samuel J. Witte,Radosław Wojtak,Anil Kumar Yadav,Weiqiang Yang,Gong-Bo Zhao,Miguel Zumalac'arregui +202 more
TL;DR: In this paper , the authors focus on the 5.0σ tension between the Planck CMB estimate of the Hubble constant H0 and the SH0ES collaboration measurements and discuss the importance of trying to fit a full array of data with a single model.
Journal ArticleDOI
Snowmass2021 - Letter of interest cosmology intertwined II: The hubble constant tension
Eleonora Di Valentino,Luis A. Anchordoqui,Özgür Akarsu,Yacine Ali-Haïmoud,Luca Amendola,Nikki Arendse,Marika Asgari,Mario Ballardini,Spyros Basilakos,Elia S. Battistelli,Micol Benetti,Simon Birrer,François R. Bouchet,Marco Bruni,Erminia Calabrese,David Camarena,Salvatore Capozziello,Angela Chen,Jens Chluba,Anton Chudaykin,Eoin Ó Colgáin,Francis-Yan Cyr-Racine,Paolo de Bernardis,Javier de Cruz Pérez,Jacques Delabrouille,Jo Dunkley,Celia Escamilla-Rivera,Agnès Ferté,Fabio Finelli,Wendy L. Freedman,Noemi Frusciante,Elena Giusarma,Adrià Gómez-Valent,Julien Guy,Will Handley,Ian Harrison,Luke Hart,Alan Heavens,Hendrik Hildebrandt,Daniel E. Holz,Dragan Huterer,Mikhail M. Ivanov,Shahab Joudaki,Shahab Joudaki,Marc Kamionkowski,Tanvi Karwal,Lloyd Knox,Suresh Kumar,Luca Lamagna,Julien Lesgourgues,Matteo Lucca,Valerio Marra,Silvia Masi,Sabino Matarrese,Arindam Mazumdar,Alessandro Melchiorri,Olga Mena,Laura Mersini-Houghton,Vivian Miranda,Cristian Moreno-Pulido,David F. Mota,J. Muir,Ankan Mukherjee,Florian Niedermann,Alessio Notari,Rafael C. Nunes,Francesco Pace,Andronikos Paliathanasis,Antonella Palmese,Supriya Pan,Daniela Paoletti,Valeria Pettorino,F. Piacentini,Vivian Poulin,Marco Raveri,Adam G. Riess,Vincenzo Salzano,Emmanuel N. Saridakis,Anjan A. Sen,Arman Shafieloo,Anowar J. Shajib,Joseph Silk,Joseph Silk,Alessandra Silvestri,Martin S. Sloth,Tristan L. Smith,Joan Solà Peracaula,Carsten van de Bruck,Licia Verde,Luca Visinelli,Benjamin D. Wandelt,Deng Wang,Jian-Min Wang,Anil Kumar Yadav,Weiqiang Yang +94 more
TL;DR: In this article, the authors focus on the 4.4σ tension between the Planck estimate of the Hubble constant H0 and the SH0ES collaboration measurements and discuss how the next decade's experiments will be crucial.
Journal ArticleDOI
Energy conditions in f(R) gravity
TL;DR: The null and strong energy conditions in this framework are derived from Raychaudhuri's equation along with the requirement that gravity is attractive, whereas the weak and dominant energy conditions are stated from a comparison with the energy conditions that can be obtained in a direct approach via an effective energy-momentum tensor for f(R) gravity.
Journal ArticleDOI
Kinematic reconstructions of extended theories of gravity at small and intermediate redshifts
TL;DR: In this paper, the authors focus on two classes of extended theories, i.e., the f(R, G) and f(r, G)-gravity, by calibrating the shapes of their curves through some of the most suitable dark energy parameterizations, XCDM, CPL, WP.
Journal ArticleDOI
A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension
TL;DR: In this article, the authors proposed a phenomenological emergent dark energy model where dark energy has no effective presence in the past and emerges at the later times, and showed that the model can satisfy different combinations of cosmological observations at low and high redshifts.
References
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