Future observations of cosmic microwave background (CMB) polarisation have the potential to answer some of the most fundamental questions of modern physics and cosmology. In this paper, we list the requirements for a future CMB polarisation survey addressing these scientific objectives, and discuss the design drivers of the CORE space mission proposed to ESA in answer to the "M5" call for a medium-sized mission. The rationale and options, and the methodologies used to assess the mission's performance, are of interest to other future CMB mission design studies. CORE is designed as a near-ultimate CMB polarisation mission which, for optimal complementarity with ground-based observations, will perform the observations that are known to be essential to CMB polarisation scienceand cannot be obtained by any other means than a dedicated space mission.

Delabrouille, J., de Bernardis, P., Bouchet, F., Achúcarro, A., Ade, P., Allison, R., et al. (2018). Exploring cosmic origins with CORE: survey requirements and mission design. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS(4) [10.1088/1475-7516/2018/04/014].

Exploring cosmic origins with CORE: survey requirements and mission design

DE GASPERIS, GIANCARLO;MAZZOTTA, PASQUALE;VITTORIO, NICOLA;
2018-04-05

Abstract

Future observations of cosmic microwave background (CMB) polarisation have the potential to answer some of the most fundamental questions of modern physics and cosmology. In this paper, we list the requirements for a future CMB polarisation survey addressing these scientific objectives, and discuss the design drivers of the CORE space mission proposed to ESA in answer to the "M5" call for a medium-sized mission. The rationale and options, and the methodologies used to assess the mission's performance, are of interest to other future CMB mission design studies. CORE is designed as a near-ultimate CMB polarisation mission which, for optimal complementarity with ground-based observations, will perform the observations that are known to be essential to CMB polarisation scienceand cannot be obtained by any other means than a dedicated space mission.
5-apr-2018
Pubblicato
Rilevanza internazionale
Articolo
Esperti anonimi
Settore FIS/05 - ASTRONOMIA E ASTROFISICA
English
astro-ph.IM; astro-ph.IM; astro-ph.CO
http://arxiv.org/abs/1706.04516v1
Delabrouille, J., de Bernardis, P., Bouchet, F., Achúcarro, A., Ade, P., Allison, R., et al. (2018). Exploring cosmic origins with CORE: survey requirements and mission design. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS(4) [10.1088/1475-7516/2018/04/014].
Delabrouille, J; de Bernardis, P; Bouchet, F; Achúcarro, A; Ade, P; Allison, R; Arroja, F; Artal, E; Ashdown, M; Baccigalupi, C; Ballardini, M; Banday, A; Banerji, R; Barbosa, D; Bartlett, J; Bartolo, N; Basak, S; Baselmans, J; Basu, K; Battistelli, E; Battye, R; Baumann, D; Benoît, A; Bersanelli, M; Bideaud, A; Biesiada, M; Bilicki, M; Bonaldi, A; Bonato, M; Borrill, J; Boulanger, F; Brinckmann, T; Brown, M; Bucher, M; Burigana, C; Buzzelli, A; Cabass, G; Cai, Z; Calvo, M; Caputo, A; Carvalho, C; Casas, F; Castellano, G; Catalano, A; Challinor, A; Charles, I; Chluba, J; Clements, D; Clesse, S; Colafrancesco, S; Colantoni, I; Contreras, D; Coppolecchia, A; Crook, M; D'Alessandro, G; D'Amico, G; da Silva, A; de Avillez, M; DE GASPERIS, G; De Petris, M; de Zotti, G; Danese, L; Désert, F; Desjacques, V; Di Valentino, E; Dickinson, C; Diego, J; Doyle, S; Durrer, R; Dvorkin, C; Eriksen, H; Errard, J; Feeney, S; Fernández Cobos, R; Finelli, F; Forastieri, F; Franceschet, C; Fuskeland, U; Galli, S; Génova Santos, R; Gerbino, M; Giusarma, E; Gomez, A; González Nuevo, J; Grandis, S; Greenslade, J; Goupy, J; Hagstotz, S; Hanany, S; Handley, W; Henrot Versillé, S; Hernández Monteagudo, C; Hervias Caimapo, C; Hills, M; Hindmarsh, M; Hivon, E; Hoang, D; Hooper, D; Hu, B; Keihänen, E; Keskitalo, R; Kiiveri, K; Kisner, T; Kitching, T; Kunz, M; Kurki Suonio, H; Lagache, G; Lamagna, L; Lapi, A; Lasenby, A; Lattanzi, M; Le Brun, A; Lesgourgues, J; Liguori, M; Lindholm, V; Lizarraga, J; Luzzi, G; Macìas Pérez, J; Maffei, B; Mandolesi, N; Martin, S; Martinez Gonzalez, E; Martins, C; Masi, S; Massardi, M; Matarrese, S; Mazzotta, P; Mccarthy, D; Melchiorri, A; Melin, J; Mennella, A; Mohr, J; Molinari, D; Monfardini, A; Montier, L; Natoli, P; Negrello, M; Notari, A; Noviello, F; Oppizzi, F; O'Sullivan, C; Pagano, L; Paiella, A; Pajer, E; Paoletti, D; Paradiso, S; Partridge, R; Patanchon, G; Patil, S; Perdereau, O; Piacentini, F; Piat, M; Pisano, G; Polastri, L; Polenta, G; Pollo, A; Ponthieu, N; Poulin, V; Prêle, D; Quartin, M; Ravenni, A; Remazeilles, M; Renzi, A; Ringeval, C; Roest, D; Roman, M; Roukema, B; Rubino Martin, J; Salvati, L; Scott, D; Serjeant, S; Signorelli, G; Starobinsky, A; Sunyaev, R; Tan, C; Tartari, A; Tasinato, G; Toffolatti, L; Tomasi, M; Torrado, J; Tramonte, D; Trappe, N; Triqueneaux, S; Tristram, M; Trombetti, T; Tucci, M; Tucker, C; Urrestilla, J; Väliviita, J; Van de Weygaert, R; Van Tent, B; Vennin, V; Verde, L; Vermeulen, G; Vielva, P; Vittorio, N; Voisin, F; Wallis, C; Wandelt, B; Wehus, I; Weller, J; Young, K; Zannoni, M; For, T
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