Zobrazeno 1 - 10
of 83
pro vyhledávání: '"S R Furtado"'
Autor:
Mariana S. R. Furtado, Raoul Henry, Thiago Rodrigues dos Santos, Suele Aparecida Mendes Santos, Carla Ferragut
Publikováno v:
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Made available in DSpace on 2018-12-11T17:16:19Z (GMT). No. of bitstreams: 0 Previous issue date: 2018-04-01 Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq) Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP) Peri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3515dce3acf5f14c95effd4f3320ffea
Publikováno v:
Day 1 Tue, October 24, 2017.
This paper aims at evaluating the applicability of input-output analysis to local content management practices as a tool to assess the relationship between the Brazilian Government's Local Content Policy and social and economic impacts of implementat
Autor:
Odylio D. Aguiar, Juliana B. Carvalho, Claudia B. M. P. Leme, Marbey M. Mosso, Jorge A. M. Souza, S R Furtado, Vanessa P. R. Magri
Publikováno v:
Microwave and Optical Technology Letters. 56:2304-2310
This work describes a simplified procedure to measure ultralow phase-noise in microwave oscillators using the delay properties of high quality factor cavities. Measurement procedures are achieved using only one microwave source and two signals extrac
Autor:
W. de Paula, Rubens M. Marinho, Nadja S. Magalhães, J L Melo, F. S. Bortoli, C Stellati, L A Carneiro, Carlos Frajuca, E C de Rey Neto, W F Velloso, Pedro J. Castro, Odylio D. Aguiar, Nei F. Oliveira, J. Weber, S R Furtado, Giorgio Frossati, S.L.T. de Souza, C. A. Costa, Oswaldo D. Miranda, A U de Lucena, K M F Costa, A C Fauth, K L Ribeiro, Joaquim J. Barroso, J. C. N. de Araujo, L A Andrade
Publikováno v:
Classical and Quantum Gravity. 23:S239-S244
The Mario Schenberg gravitational wave detector has been constructed at its site in the Physics Institute of the University of Sao Paulo as programmed by the Brazilian Graviton Project, under the full support of FAPESP (the Sao Paulo State Foundation
Autor:
S R Furtado, Odylio D. Aguiar, A U de Lucena, Nadja S. Magalhães, K M F Costa, A C Fauth, W F Velloso, W. de Paula, C Stellati, L A Carneiro, Joaquim J. Barroso, L A Andrade, C. A. Costa, Bruno Woltzenlogel Paleo, Nei F. Oliveira, J. C. N. de Araujo, M Remy, J. Weber, E C de Rey Neto, Carlos Frajuca, K L Ribeiro, Giorgio Frossati, Pedro J. Castro, S.L.T. de Souza, Oswaldo D. Miranda, J L Melo, E S Matos, Rubens M. Marinho, F. S. Bortoli
Publikováno v:
Classical and Quantum Gravity. 22:S209-S214
The Schenberg gravitational wave detector is almost completed for operation at its site in the Physics Institute of the University of Sao Paulo, under the full support of FAPESP (the Sao Paulo State Foundation for Research Support). We have been work
Autor:
Odylio D. Aguiar, K L Ribeiro, Joaquim J. Barroso, Pedro J. Castro, M Remy, Carlos Frajuca, S R Furtado
Publikováno v:
Classical and Quantum Gravity. 21:S1225-S1229
We studied the niobium re-entrant cavity utilized by the Australian group in the Niobe gravitational wave detector. Instead of using their non-contact re-entrant cavity, we plan to change it to a closed one to be used in the parametric transducers of
Autor:
K L Ribeiro, S R Furtado, Giorgio Frossati, S.L.T. de Souza, Odylio D. Aguiar, E S Matos, Rubens M. Marinho, Nadja S. Magalhães, L A Andrade, Bruno Woltzenlogel Paleo, Lucrecia Camilo De Lima, Carlos Frajuca, Pedro J. Castro, J. C. N. de Araujo, A U de Lucena, Cecília Silva de Castro, L. Camargo Filho, K M F Costa, A C Fauth, M Remy, W. de Paula, Nei F. Oliveira, Joaquim J. Barroso, Oswaldo D. Miranda, C Stellati, E C de Rey Neto, L A Carneiro, J L Melo, J. Weber, W F Velloso, C. A. Costa
Publikováno v:
Classical and Quantum Gravity. 21:S457-S463
We are building the Schenberg gravitational wave detector at the Physics Institute of the University of Sao Paulo as programmed by the Brazilian Graviton Project. The antenna and its vibration isolation system are already built, and we have made a fi
Autor:
Odylio D. Aguiar, S R Furtado
Publikováno v:
Classical and Quantum Gravity. 19:1973-1978
The resonant-mass technique for the detection of gravitational waves may involve, in the near future, the cooling of very large masses (about 100 tons) from room temperature (300 K) to extreme cryogenic temperatures (20 mK). To cool these detectors t
Autor:
Nei F. Oliveira, Karla Beatriz M. Salles, Nadja S. Magalhães, C. A. Costa, K L Ribeiro, Odylio D. Aguiar, Luiz Alberto de Andrade, J. C. N. de Araujo, E S Matos, Rubens M. Marinho, V.G.S. Furtado, C Stellati, S R Furtado, M. T. Meliani, Walter F. Velloso, E C de Rey Neto, Giorgio Frossati, S.L.T. de Souza, L. Camargo Filho, Carlos Frajuca, J L Melo, Oswaldo D. Miranda, A C Fauth
Publikováno v:
Classical and Quantum Gravity. 19:1949-1953
The first phase of the Brazilian Graviton Project is the construction and operation of the gravitational wave detector Mario Schenberg at the Physics Institute of the University of S?o Paulo. This gravitational wave spherical antenna is planned to fe
Autor:
Odylio D. Aguiar, S R Furtado, C. L. Barucke, Jorge A. M. Souza, Marbey M. Mosso, Vanessa P. R. Magri
Publikováno v:
2013 SBMO/IEEE MTT-S International Microwave & Optoelectronics Conference (IMOC).
This work describes the development of an oscillator prototype at 10GHz that consists of a feedback loop amplifier using a Sapphire loaded cavity and a tunable cylindrical cavity filter. Measurement procedures involving a phase detector circuit techn