Accès ouvert déclaré
2019
preprint
Astro2020 Science White Paper: Dark Energy and Modified Gravity
Anže Slosar, Kevork N. Abazajian, Zeeshan Ahmed, David Alonso, Mustafa A. Amin, Behzad Ansarinejad, Robert Armstrong, J. Asorey, Arturo Avelino, S. Àvila, Carlo Baccigalupi, M. Ballardini, Kevin Bandura, Nicholas Battaglia, Amy N. Bender, Charles Bennett, Bradford Benson, Florian Beutler, F. Bianchini, Maciej Bilicki, Colin Bischoff, Andrea Biviano, Jonathan Blazek, Lindsey Bleem, A. Bolton, J. Richard Bond, Julian Borrill, Sownak Bose, A. Boucaud, F. R. Bouchet, Elizabeth Buckley-Geer, Philip Bull, Zheng Cai, John E. Carlstrom, Francisco J. Castander, Emanuele Castorina, A. Challinor, Tzu-Ching Chang, J. Chaves-Montero, Nora Elisa Chisari, Douglas Clowe, Johan Comparat, Asantha Cooray, Rupert A.C. Croft, Francis-Yan Cyr-Racine, Guido D'Amico, T. M. Davis, Kyle Dawson, Marcel Demarteau, Arjun Dey, Olivier Dore, Duan Yutong, Joanna Dunkley, Cora Dvorkin, Alexander Eggemeier, Eisenstein, Daniel, J. Ellison, Alexander van Engelen, Stephanie Escoffier, Giulio Fabbian, Simone Ferraro, Pedro G. Ferreira, Andreu Font-Ribera, Simon Foreman, Pablo Fosalba, Oliver Friedrich, Juan Garcıa-Bellido, M. Gerbino, Mandeep S.S. Gill, Vera Gluscevic, Satya Gontcho A. Gontcho, K. M. Górski, Daniel Gruen, Jon E. Gudmundsson, N. Gupta, Julien Guy, Shaul Hanany, Will Handley, César Hernández-Aguayo, J. Colin Hill, Christopher M. Hirata, Renée Hložek, Gilbert Holder, Dragan Huterer, Mustapha Ishak, Tesla Jeltema, Saurabh W. Jha, J. Cohen-Tanugi, Bradley Johnson, Marc Kamionkowski, Kirit S. Karkare, Ryan E.Keeley, Rishi Khatri, David Kirkby, Theodore Kisner, Jean-Paul Kneib, Lloyd Knox, Savvas M. Koushiappas, Ely D. Kovetz, Kazuya Koyama, Elisabeth Krause, Benjamin L’Huillier, Ofer Lahav, Massimiliano Lattanzi, Danielle Leonard, Michael Levi, M. Liguori, Anja von der Linden, Marilena Loverde, Zarija Lukić, Axel de la Macorra, Mathew Madhavacheril, Andres Plazas, Alessio Spurio Mancini, Marc Manera, Adam Mantz, Paul Martini, Kiyoshi Masui, Jeff Mcmahon, P. Daniel Meerburg, James Mertens, Joel Meyers, Surhud More, Pavel Motloch, Suvodip Mukherjee, Julian B. Muñoz, Adam D. Myers, Johanna Nagy, Nathalie Palanque-Delabrouille, Laura Newburgh, Jeffrey A. Newman, Michael D. Niemack, Gustavo Niz, A. Nomerotski, P. O’Connor, Lyman Page, A. Palmese, Mariana Penna-Lima, Will J. Percival, Francesco Piacentni, Matthew M. Pieri, E. Pierpaoli, Levon Pogosian, Abhishek Prakash, Clement Pryke, Giuseppe Puglisi, Radek Stompor, Marco Raveri, Christian L. Reichardt, Jason Rhodes, Steven Rodney, Benjamin Rose, Ashley J. Ross, Graziano Rossi, John Ruhl, Benjamin Saliwanchik, Lado Samushia, Javier Sanchez, Misao Sasaki, Emmanuel Schaan, David J. Schlegel, Marcel Schmittfull, Michael Schubnell, Douglas Scott, Neelima Sehgal, Leonardo Senatore, Hee-Jong Seo, Arman Shafieloo, Huanyuan Shan, Blake D. Sherwin, Feng Shi, Sara Simon, Anže Slosar, Suzanne Staggs, Glenn Starkman, Albert Stebbins, Aritoki Suzuki, Eric R. Switzer, Peter Timbie, Andrew J. Tolley, Matthieu Tristram, Mark Trodden, M.A. Troxel, Cora Uhlemann, Caterina Umilta, L. Arturo Urenña-López, Eleonora Di Valentino, M. Vargas-Magana, Abigail Vieregg, C. W. Walter, Yi Wang, Scott Watson, Martin White, Nathan Whitehorn, W.L.K. Wu, Wenting Xu, Siavash Yasini, Matias Zaldarriaga, Gong-Bo Zhao, Yi Zheng, Hong-Ming Zhu, Ningfeng Zhu, Joe Zuntz
8Citations signalées, ce qui n’est pas une note de qualité
47Institutions déclarées
12Pays d’affiliation déclarés
Rattachement africain : us, gb, kr, es, Afrique du Sud, au, pl, it, ch, ca, fr, ru.
Niveau de preuve : code pays fourni par la source.
Le résumé fourni par la source
Despite two decades of tremendous experimental and theoretical progress, the riddle of the accelerated expansion of the Universe remains to be solved. On the experimental side, our understanding of the possibilities and limitations of the major dark energy probes has evolved; here we summarize the major probes and their crucial challenges. On the theoretical side, the taxonomy of explanations for the accelerated expansion rate is better understood, providing clear guidance to the relevant observables. We argue that: i) improving statistical precision and systematic control by taking more data, supporting research efforts to address crucial challenges for each probe, using complementary methods, and relying on cross-correlations is well motivated; ii) blinding of analyses is difficult but ever more important; iii) studies of dark energy and modified gravity are related; and iv) it is crucial that R&D for a vibrant dark energy program in the 2030s be started now by supporting studies and technical R&D that will allow embryonic proposals to mature. Understanding dark energy, arguably the biggest unsolved mystery in both fundamental particle physics and cosmology, will remain one of the focal points of cosmology in the forthcoming decade.
Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.
Le contrôle bibliographique ouvert
Aucun DOI disponible pour le contrôle Crossref.
Les institutions déclarées
Une affiliation ne permet pas de déduire la nationalité d’un auteur.
Les sujets associés
Cosmology and Gravitation TheoriesGalaxies: Formation, Evolution, PhenomenaDark Matter and Cosmic Phenomena