The status of the Brazilian spherical detector

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
Rok vydání:	2002
Předmět:	Physics Gravitational-wave observatory Physics and Astronomy (miscellaneous) Gravitational wave business.industry Bandwidth (signal processing) Detector Testbed Graviton Astrophysics Particle detector Optics Measuring instrument business
Zdroj:	Classical and Quantum Gravity. 19:1949-1953
ISSN:	1361-6382 0264-9381
DOI:	10.1088/0264-9381/19/7/397
Popis:	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 feature a sensitivity better than h = 10?21 Hz?1/2 at the 3.0?3.4 kHz bandwidth, and to work not only as a detector, but also as a testbed for the development of new technologies. Here we present the status of this detector.
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_________::a2178606054806e53a0f7a668098ce1f https://doi.org/10.1088/0264-9381/19/7/397 Zobrazit plný text záznamu