CV Lattes
Instituto Federal de Educação, Ciência e Tecnologia de São Paulo (IFSP). Campus São Paulo (Institutional affiliation from the last research proposal) Birthplace: Brazil
Graduate in Mechanics at São Carlos Federal University (1986), Graduate in Physics at Sao Paulo University (1987), master's in Sciences at Sao Paulo University (1992) and Ph.D. in Sciences at São Paulo University de São Paulo (1996). . Habilitation in Stelar astrophysics, compact objects and cosmology by the Federal University of Sao Paulo. More areas of Expertise: 1. Electromechanical Instrumentation 2. Relativity and Gravitation 3. Particles and Fields 4. Vocational Education. Has experience in Electric Engineering, focusing on Electromechanical Instrumentation, acting mainly in gravitational waves detectors. Main Management and Administrative Positions: Institution Brasilia Federal Institute: 08/2009 - 02/2010 PostGraduation and Research Pro-Rector; 03/2009 - 07/2009 UnderGraduation Pro-Rector 03/2009 and 02/2010 Substitute Rector. Currently in a position of Full-Professor at Rio Grande Federal University, forme Full-Professor atSao Paulo Federal Institute, with a fellowship in research in Mechanics, Naval, Oceanics and Airspace Engineering from the National Council for Research. Referee for the Classical and Quantum Gravity and Journal of Physics:Conference Series. Member of the editorial board of the journals: Journal of Gravity and Sinergia (ISSN: 2177-451X) and editor of the Sinergia for two years. My score in the researchgate (47.47) is higher than 97.5% of ResearchGate members'. (Source: Lattes Curriculum)
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| TITULO |
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| VEICULO: TITULO (DATA) |
| VEICULO: TITULO (DATA) |
It is being built in the Physics Institute of Sao Paulo University a resonant-mass spherical gravitational wave detector that will be part of a detection network with a similar one being built in The Nederlands. The goal of such detector is to reach a sensitivity , in h, of 10-21, in frequencies close to 3200 Hz with a band of 200 Hz. The expected sensitivity of each detector will be clos…
(Only some records are available in English at this moment)
LISA is a project of an interferometric gravitational wave detector to be assembled in space, so the abbreviature LISA means Laser Interferometer Space Antenna. The LISA function is to find wavelength fluctuations in the sides of an equilateral triangle with side-length of 5x106km shaped by spaceships in each vertex of the triangle. The goal of this work is to re-elaborate a noise model f…
| 8 / 8 | Completed research grants |
| 1 / 1 | Completed scholarships in Brazil |
| 1 / 0 | Completed scholarships abroad |
| 10 / 9 | All research grants and scholarships |
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