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    Escamilla, Luis A.
    L’Huillier, Benjamin
    D’Agostino, Rocco
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    Banihashemi, Abdolali
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    Ghodsi, Mina
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    Mendoza, Renier
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    Olmo, Gonzalo J.
    Joudaki, Shahab
    Franco-Abellán, Guillermo
    Marques, Catarina
    Nilsson, Nils A.
    Reyhani, Masoume
    William, Anjitha John
    Pfeifer, Christian
    Sokoliuk, Oleksii
    Karčiauskas, Mindaugas
    Koivisto, Tomi
    Putten, Maurice H.P.M. van
    Lobo, Francisco S.N.
    Eckert, Dominique
    Jovanović, Predrag
    Davari, Zahra
    Padilla, Luis E.
    Shah, Rahul
    Raftogianni, Matthildi
    Correa, Carlos
    Zeynalabdi, Ismailov Nariman
    Krššák, Martin
    Le Delliou, Morgan
    Wagner, Jenny
    Caruana, Maria
    Demirci, Mehmet
    Niedermann, Florian
    Mishra, Bivudutta
    Rácz, Gábor
    Gómez-Vargas, Isidro
    Valls-Gabaud, David
    Suman, Petar
    Peracaula, Joan Solà
    Gómez-Valent, Adrià
    Saal, Margus
    Pacaud, Florian
    Fornengo, Nicolao
    Pedrotti, Davide
    Holm, Emil Brinch
    Cañas-Herrera, Guadalupe
    Koopmans, Lón V.E.
    Sultan, Abdul Malik
    Boiza, Carlos G.
    Melo, Mariana
    Brinckmann, Thejs
    Banik, Indranil
    Prat, Judit
    Benisty, David
    Chudaykin, Anton
    Regis, Marco
    Opis:
    The standard model of cosmology has provided a good phenomenological description of a wide range of observations both at astrophysical and cosmological scales for several decades. This concordance model is constructed by a universal cosmological constant and supported by a matter sector described by the standard model of particle physics and a cold dark matter contribution, as well as very early-time inflationary physics, and underpinned by gravitation through general relativity. There have always been open questions about the soundness of the foundations of the standard model. However, recent years have shown that there may also be questions from the observational sector with the emergence of differences between certain cosmological probes. In this White Paper, we identify the key objectives that need to be addressed over the coming decade together with the core science projects that aim to meet these challenges. These discordances primarily rest on the divergence in the measurement of core cosmological parameters with varying levels of statistical confidence. These possible statistical tensions may be partially accounted for by systematics in various measurements or cosmological probes but there is also a growing indication of potential new physics beyond the standard model. After reviewing the principal probes used in the measurement of cosmological parameters, as well as potential systematics, we discuss the most promising array of potential new physics that may be observable in upcoming surveys. We also discuss the growing set of novel data analysis approaches that go beyond traditional methods to test physical models. These new methods will become increasingly important in the coming years as the volume of survey data continues to increase, and as the degeneracy between predictions of different physical models grows. There are several perspectives on the divergences between the values of cosmological parameters, such as the model-independent probes in the late Universe and model-dependent measurements in the early Universe, which we cover at length. The White Paper closes with a number of recommendations for the community to focus on for the upcoming decade of observational cosmology, statistical data analysis, and fundamental physics developments.
    Dostawca treści:
    Repozytorium Uniwersytetu Jagiellońskiego
    Artykuł
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