On the void explanation of the Cold Spot
Ver/ Abrir
Registro completo
Mostrar el registro completo DCAutoría
Marcos Caballero, Airam Eduardo; Fernández Cobos, Raúl
; Martínez González, Enrique; Vielva Martínez, Patricio
Fecha
2016-06Derechos
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society, ©2016 The authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Publicado en
Monthly Notices of the Royal Astronomical Society, 2016, 460(1), L15-L19
Editorial
Oxford University Press
Enlace a la publicación
Palabras clave
Methods: data analysis
Cosmic background radiation
Resumen/Abstract
The integrated Sachs–Wolfe (ISW) contribution induced on the cosmic microwave background by the presence of a supervoid as the one detected by Szapudi et al. (2015) is reviewed in this letter in order to check whether it could explain the Cold Spot (CS) anomaly. Two different models, previously used for the same purpose, are considered to describe the matter density profile of the void: a top hat function and a compensated profile produced by a Gaussian potential. The analysis shows that, even enabling ellipticity changes or different values for the dark-energy equation of state parameter ω, the ISW contribution due to the presence of the void does not reproduce the properties of the CS.
Colecciones a las que pertenece
- D15 Artículos [850]
- D15 Proyectos de Investigación [162]
- D52 Artículos [1345]
- D52 Proyectos de investigación [432]







