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Synergies with the cosmic microwave background radiation

AutorDiego, José María ; Hernández-Monteagudo, C.; Herranz, D. ; Martínez-González, Enrique ; Rubiño-Martín, J. A.; Vielva, P.
Fecha de publicación2015
EditorSociedad Española de Astronomía
CitaciónThe Spanish Square Kilometre Array White Book: 20-28 (2015)
ResumenThe Cosmic Microwave Background (CMB), just like the HI 21 cm radiation, constitutes a privileged witness of the evolution of our universe during and after the epoch of reionization. This parallelism between the two radiation fields is also reflected in the fact that cosmological events leave different (but often complementary) signatures on both photon fields. In fact, there exists a number of physical channels of interaction between the CMB radiation with electrons, atoms, ions and gravitational potentials during and after the epoch of reionization: these strongly motivate a joint study of the CMB and future HI 21 cm data. In this context, we also highlight the existing parallelism between problems addressed in CMB analysis and problems foreseen in future HI 21 cm observations, in many of which the Spanish cosmological community has been deeply involved during the last decade.
URIhttp://hdl.handle.net/10261/141412
ISBN978-84-606-8955-3
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