CV Lattes
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Ministério da Ciência, Tecnologia e Inovação (Brasil). Instituto Nacional de Pesquisas Espaciais (INPE) (Institutional affiliation from the last research proposal) Birthplace: Brazil
graduation at Bacharelado Em Física from Pontifícia Universidade Católica de São Paulo (1988), master's at Astronomy from Universidade de São Paulo (1992) and doctorate at Astronomy from Universidade de São Paulo (1997). Has experience in Astronomy, focusing on Cosmology, acting on the following subjects: cosmologia, ondas gravitacionais, detectores de ondas gravitacionais, buracos negros and formação de estruturas. (Source: Lattes Curriculum)
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We propose to investigate a number of research problems relevant to the detection and analysis of gravitational wave (GW) signals observable by space-based interferometers. The LaserInterferometer Space Antenna (LISA) project and the Antenna for Mid-Band InterferometricGravitational wave Observations (AMIGO) mission are expected to uncover a wealth of information about the Universe throug…
The fact that Dark Matter interacts very weakly to Standard Model implies in many difficulties in searching for it. Therefore, any situation which could put in evidence DM signatures is of great interest. The interactions between DM and SM particles are proportional to the density of the particle it interacts with. So, this suggests that we could study DM matter presence nearby astronomic…
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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 t…
In this post-doctoral project we study the possible signatures generated by non-singular models in Quantum Cosmology on the Cosmic Microwave Background Radiation (CMB). We shall study CMB anisotropies generated not only by primordial Gravitational Waves (PGW), but by curvature perturbations induced by these non-singular models as well. Also, we shall investigate the possible non-gaussiani…
| 5 / 4 | Completed research grants |
| 8 / 2 | Completed scholarships in Brazil |
| 1 / 0 | Completed scholarships abroad |
| 14 / 6 | All research grants and scholarships |
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