Cosmic microwave background bispectrum from active models of structure formation

Mostrar todas las versiones(4)

We propose a method for a numerical computation of the angular bispectrum of the cosmic microwave background (CMB) anisotropies arising from active models such as cosmic topological defects, using a modified Boltzmann code based on CMBFAST. The method does not use CMB sky maps and requires moderate...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Gangui, A., Pogosian, L., Winitzki, S.
Formato: JOUR
Materias:
anisotropy
article
astronomy
calculation
methodology
model
physics
signal detection
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_05562821_v64_n4_p_Gangui
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

Ejemplares similares

Ejemplares similares