THE ROLE OF DARK MATTER INTERACTION IN GALAXY CLUSTERS


Autoria(s): Oliveira, Carlos Eduardo Pellicer de; Ferreira, Elisa G. M.; Guariento, Daniel C.; Costa, André Alencar da; Graef, Leila Lobato; Coelho, Andréa Vila Nova; Abdalla, Elcio
Contribuinte(s)

UNIVERSIDADE DE SÃO PAULO

Data(s)

21/10/2013

21/10/2013

2012

Resumo

We consider a toy del to analyze the consequences of dark matter interaction with a dark energy background on the overall rotation of galaxy clusters and the misalignment between their dark matter and baryon distributions when compared to ACDM predictions. The interaction parameters are found via a genetic algorithm search. The results obtained suggest that interaction is a basic phenomenon whose effects are detectable even in simple models of galactic dynamics.

FAPESP

CNPq

Identificador

MODERN PHYSICS LETTERS A, SINGAPORE, v. 27, n. 26, supl. 1, Part 1, pp. 11232-11240, AUG 30, 2012

0217-7323

http://www.producao.usp.br/handle/BDPI/35241

10.1142/S0217732312501441

http://dx.doi.org/10.1142/S0217732312501441

Idioma(s)

eng

Publicador

WORLD SCIENTIFIC PUBL CO PTE LTD

SINGAPORE

Relação

MODERN PHYSICS LETTERS A

Direitos

closedAccess

Copyright WORLD SCIENTIFIC PUBL CO PTE LTD

Palavras-Chave #COSMOLOGY #GALAXY CLUSTERS #DARK MATTER #DARK ENERGY #OBSERVATIONAL CONSTRAINTS #ENERGY-MODEL #UNIVERSE #PARAMETERS #ALIGNMENT #HALOS #MODELO ENERGÉTICO #FÍSICA NUCLEAR #FÍSICA, PARTÍCULAS E CAMPOS #PHYSICS, NUCLEAR #PHYSICS, PARTICLES & FIELDS #PHYSICS, MATHEMATICAL
Tipo

article

original article

publishedVersion