Computation of schenberg response function by using finite element modelling

Detalhes bibliográficos
Autor(a) principal: Frajuca, C.
Data de Publicação: 2016
Outros Autores: Bortoli, F. S., Magalhaes, N. S. [UNIFESP]
Tipo de documento: Artigo de conferência
Idioma: eng
Título da fonte: Repositório Institucional da UNIFESP
Texto Completo: http://repositorio.unifesp.br/handle/11600/49354
http://dx.doi.org/10.1088/1742-6596/716/1/012016
Resumo: Schenberg is a detector of gravitational waves resonant mass type, with a central frequency of operation of 3200 Hz. Transducers located on the surface of the resonating sphere, according to a distribution half-dodecahedron, are used to monitor a strain amplitude. The development of mechanical impedance matchers that act by increasing the coupling of the transducers with the sphere is a major challenge because of the high frequency and small in size. The objective of this work is to study the Schenberg response function obtained by finite element modeling (FEM). Finnaly, the result is compared with the result of the simplified model for mass spring type system modeling verifying if that is suitable for the determination of sensitivity detector, as the conclusion the both modeling give the same results.
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spelling Frajuca, C.Bortoli, F. S.Magalhaes, N. S. [UNIFESP]2019-01-21T10:29:44Z2019-01-21T10:29:44Z201611th Edoardo Amaldi Conference On Gravitational Waves (AMALDI 11). Bristol, v. 716, p. UNSP 012016, 2016.1742-6588http://repositorio.unifesp.br/handle/11600/49354http://dx.doi.org/10.1088/1742-6596/716/1/012016WOS000386960500016.pdf10.1088/1742-6596/716/1/012016WOS:000386960500016Schenberg is a detector of gravitational waves resonant mass type, with a central frequency of operation of 3200 Hz. Transducers located on the surface of the resonating sphere, according to a distribution half-dodecahedron, are used to monitor a strain amplitude. The development of mechanical impedance matchers that act by increasing the coupling of the transducers with the sphere is a major challenge because of the high frequency and small in size. The objective of this work is to study the Schenberg response function obtained by finite element modeling (FEM). Finnaly, the result is compared with the result of the simplified model for mass spring type system modeling verifying if that is suitable for the determination of sensitivity detector, as the conclusion the both modeling give the same results.Sao Paulo Federal Institute Rua Pedro Vicente 625, 01109-010 Sao Paulo, SP, BrazilFederal University of Sao Paulo, Department of Exact and Earth Sciences Rua Sao Nicolau 120, 09913-030 Diadema, SP, BrazilFederal University of Sao Paulo, Department of Exact and Earth Sciences Rua Sao Nicolau 120, 09913-030 Diadema, SP, BrazilWeb of ScienceUNSP 012016engUniv Federal Ceara, Centro Ciencias Agrarias11th Edoardo Amaldi Conference On Gravitational Waves (AMALDI 11)Gravitational-Wave AntennaComputation of schenberg response function by using finite element modellinginfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UNIFESPinstname:Universidade Federal de São Paulo (UNIFESP)instacron:UNIFESPORIGINALWOS000386960500016.pdfapplication/pdf1929936${dspace.ui.url}/bitstream/11600/49354/1/WOS000386960500016.pdff76e1468d28a6d733b682596a5cd1432MD51open accessTEXTWOS000386960500016.pdf.txtWOS000386960500016.pdf.txtExtracted texttext/plain12227${dspace.ui.url}/bitstream/11600/49354/8/WOS000386960500016.pdf.txtcaf91704705ddad38e8c8e951c86e7a2MD58open accessTHUMBNAILWOS000386960500016.pdf.jpgWOS000386960500016.pdf.jpgIM Thumbnailimage/jpeg5171${dspace.ui.url}/bitstream/11600/49354/10/WOS000386960500016.pdf.jpg4ec0b1ea584fccce216dc5bda3ea5d76MD510open access11600/493542023-06-05 19:41:39.42open accessoai:repositorio.unifesp.br:11600/49354Repositório InstitucionalPUBhttp://www.repositorio.unifesp.br/oai/requestopendoar:34652023-06-05T22:41:39Repositório Institucional da UNIFESP - Universidade Federal de São Paulo (UNIFESP)false
dc.title.en.fl_str_mv Computation of schenberg response function by using finite element modelling
title Computation of schenberg response function by using finite element modelling
spellingShingle Computation of schenberg response function by using finite element modelling
Frajuca, C.
Gravitational-Wave Antenna
title_short Computation of schenberg response function by using finite element modelling
title_full Computation of schenberg response function by using finite element modelling
title_fullStr Computation of schenberg response function by using finite element modelling
title_full_unstemmed Computation of schenberg response function by using finite element modelling
title_sort Computation of schenberg response function by using finite element modelling
author Frajuca, C.
author_facet Frajuca, C.
Bortoli, F. S.
Magalhaes, N. S. [UNIFESP]
author_role author
author2 Bortoli, F. S.
Magalhaes, N. S. [UNIFESP]
author2_role author
author
dc.contributor.author.fl_str_mv Frajuca, C.
Bortoli, F. S.
Magalhaes, N. S. [UNIFESP]
dc.subject.eng.fl_str_mv Gravitational-Wave Antenna
topic Gravitational-Wave Antenna
description Schenberg is a detector of gravitational waves resonant mass type, with a central frequency of operation of 3200 Hz. Transducers located on the surface of the resonating sphere, according to a distribution half-dodecahedron, are used to monitor a strain amplitude. The development of mechanical impedance matchers that act by increasing the coupling of the transducers with the sphere is a major challenge because of the high frequency and small in size. The objective of this work is to study the Schenberg response function obtained by finite element modeling (FEM). Finnaly, the result is compared with the result of the simplified model for mass spring type system modeling verifying if that is suitable for the determination of sensitivity detector, as the conclusion the both modeling give the same results.
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dc.identifier.citation.fl_str_mv 11th Edoardo Amaldi Conference On Gravitational Waves (AMALDI 11). Bristol, v. 716, p. UNSP 012016, 2016.
dc.identifier.uri.fl_str_mv http://repositorio.unifesp.br/handle/11600/49354
http://dx.doi.org/10.1088/1742-6596/716/1/012016
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identifier_str_mv 11th Edoardo Amaldi Conference On Gravitational Waves (AMALDI 11). Bristol, v. 716, p. UNSP 012016, 2016.
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10.1088/1742-6596/716/1/012016
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