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Testing fundamental gravity and validating gravitational waveforms

Processo: 14/50259-3
Linha de fomento:Auxílio à Pesquisa - Regular
Vigência: 01 de março de 2015 - 28 de fevereiro de 2017
Área do conhecimento:Ciências Exatas e da Terra - Física
Convênio/Acordo: University of Birmingham
Pesquisador responsável:Riccardo Sturani
Beneficiário:Riccardo Sturani
Pesq. responsável no exterior: Alberto Vecchio
Instituição no exterior: University of Birmingham, Inglaterra
Instituição-sede: Instituto de Física Teórica (IFT). Universidade Estadual Paulista (UNESP). Campus de São Paulo. São Paulo , SP, Brasil
Vinculado ao auxílio:12/14132-3 - Análise das ondas gravitacionais, AP.JP
Assunto(s):Gravidade  Ondas gravitacionais 


The gravitational wave astronomy era will start in a few years time, with the most likely candidate source for repeated detection being coalescing binaries made of compact objects like neutron stars and stellar mass black holes. However, for earth-based detectors like LIGO and Virgo the signals are buried deeply within the instrumental noise, thus a detailed knowledge of the signal itself is necessary in order to enhance detection probability and ensure an accurate measure of the source parameters. At the moment there not exist a single waveform model that can be used for ali physical sources, and it is of primary importance for reliable measurements of the source physical parameters to understand the relative performances of the various analytical waveforms. We intend to investigate how the discrepancy between the available analytic waveforms describing the binary system coalescence aftect: the detection, the parameter estimation and the confidence with which detection and parameter estimation can be achieved. We plan to utilise the knowledge acquired with this investigation to eventually develop methods to correct for the observed discrepancies. (AU)

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