Galaxy clusters, type Ia supernovae and the fine structure constant

As is well known, measurements of the Sunyaev-Zeldovich effect can be combined with observations of the X-ray surface brightness of galaxy clusters to estimate the angular diameter distance to these structures. In this paper, we show that this technique depends on the fine structure constant, α. The...

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Detalles Bibliográficos
Autor principal:	Landau, Susana J.
Publicado:	2016
Materias:	galaxy clusters modified gravity supernovas
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14757516_v2016_n8_p_Holanda http://hdl.handle.net/20.500.12110/paper_14757516_v2016_n8_p_Holanda
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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