| Grant number: | 11/12909-8 |
| Support Opportunities: | Regular Research Grants |
| Start date: | November 01, 2011 |
| End date: | October 31, 2013 |
| Field of knowledge: | Physical Sciences and Mathematics - Astronomy - Extragalactic Astrophysics |
| Principal Investigator: | Diego Antonio Falceta Gonçalves |
| Grantee: | Diego Antonio Falceta Gonçalves |
| Host Institution: | Escola de Artes, Ciências e Humanidades (EACH). Universidade de São Paulo (USP). São Paulo , SP, Brazil |
| City of the host institution: | São Paulo |
Abstract
The intergalactic medium is composed by rarefied hot plasma, considered non-collisional in many cases, with complex dynamics. It is known that this plasma is also magnetized. However, the dynamics of magnetized non-collisional plasmas is not fully understood. In this work we will evaluate the role of plasma instabilities in the intergalactic medium. In particular, we will study the amplification of the magnetic energy, and the correlation lengths of the field lines, as well as the particle acceleration under these instabilities and the synchrotron and gamma emissions related. These models will be compared to the observations. Also, we will continue the study on AGN jets and their role on the dynamics of the intergalactic medium, as well as in the suppression of cooling flows. (AU)
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