Cosmic crystallography with a pullback


Autoria(s): Fagundes, Helio V.; Gausmann, Evelise
Contribuinte(s)

Universidade Estadual Paulista (UNESP)

Data(s)

27/05/2014

27/05/2014

18/10/1999

Resumo

We present a modified version of the cosmic crystallography method, especially useful for testing closed models of negative spatial curvature. The images of clusters of galaxies in simulated catalogs are 'pulled back' to the fundamental domain before the set of distances is calculated. © 1999 Published by Elsevier Science B.V. All rights reserved.

Formato

235-239

Identificador

http://dx.doi.org/10.1016/S0375-9601(99)00647-7

Physics Letters, Section A: General, Atomic and Solid State Physics, v. 261, n. 5-6, p. 235-239, 1999.

0375-9601

http://hdl.handle.net/11449/65863

10.1016/S0375-9601(99)00647-7

WOS:000083334400002

2-s2.0-0347875984

Idioma(s)

eng

Relação

Physics Letters, Section A: General, Atomic and Solid State Physics

Direitos

closedAccess

Tipo

info:eu-repo/semantics/article