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Numerical simulation of Supermassive black holes population and its role into the universe reionization

Grant number: 12/21877-5
Support type:Scholarships in Brazil - Post-Doctorate
Effective date (Start): January 01, 2013
Effective date (End): December 31, 2015
Field of knowledge:Physical Sciences and Mathematics - Physics
Principal Investigator:Oswaldo Duarte Miranda
Grantee:Eduardo dos Santos Pereira
Home Institution: Instituto Nacional de Pesquisas Espaciais (INPE). Ministério da Ciência, Tecnologia, Inovações e Comunicações (Brasil). São José dos Campos , SP, Brazil

Abstract

For the study of the Universe evolution and its structures, like galaxies and galaxies clusters, the junction of many areas of physics/astrophysics are necessary. As example we can cite a new astronomical a cosmological window that will be opened with the first detection of the gravitacional waves. These waves are space-time perturbation that propagate, into the General Relativity, with the speed of light. Promising source of gravitational waves is into the process of growing of super-massive black holes, by accretion of by fusion of these objects. Beyond the gravitational waves signature, the growing of super-massive black holes within pre-galactics objects, like mini-quasers, can having an important role into the Universer reionization, it is possible that these objects have left a signature into the cosmic microwave background radiation. Within this context, the present project propose the study of super-massive black holes evolution and its role for the Universe reionization. Also, we have the intention to do the same test for cosmological models with different states-equation for dark energy, in particular, the standard model with cosmological constant, and Chaplygin gas. (AU)

Scientific publications
(References retrieved automatically from Web of Science and SciELO through information on FAPESP grants and their corresponding numbers as mentioned in the publications by the authors)
PEREIRA, EDUARDO S.; MIRANDA, OSWALDO D. The role of the dark matter haloes on the cosmic star formation rate. NEW ASTRONOMY, v. 41, p. 48-52, NOV 2015. Web of Science Citations: 0.
GUEDES, M. R. G.; PEREIRA, E. S.; CECATTO, J. R. Wavelet analysis of CME, X-ray flare, and sunspot series. Astronomy & Astrophysics, v. 573, JAN 2015. Web of Science Citations: 5.
PEREIRA, EDUARDO S.; MIRANDA, OSWALDO D. Accretion history of active black holes from type 1 AGN. ASTROPHYSICS AND SPACE SCIENCE, v. 352, n. 2, p. 801-807, AUG 2014. Web of Science Citations: 0.

Please report errors in scientific publications list by writing to: cdi@fapesp.br.