%0 Journal Article
%4 sid.inpe.br/plutao/2014/12.01.12.20
%2 sid.inpe.br/plutao/2014/12.01.12.20.16
%@doi 10.1093/mnrasl/slu124
%@issn 1745-3925
%F lattes: 9300685610267922 1 MoraesMira:2014:PrStSt
%T Probing strange stars with advanced gravitational wave detectors
%D 2014
%9 journal article
%A Moraes, Pedro Henrique Ribeiro da Silva,
%A Miranda, Oswaldo Duarte,
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%B Royal Astronomical Society. Monthly Notices. Letters
%V 445
%N 1
%P L11-L15
%K ondas gravitacionais, sistemas binários emitindo ondas gravitacionais, estrelas estranhas.
%X When a neutron star is squeezed to huge densities, it can be converted to a strange star. Using the event/year rate of a neutron starstrange star binary system, we show that the operational phase of advanced gravitational wave detectors might show some evidence that such strange stars do exist. Moreover, we argue that such a system could be a plausible progenitor to GRB 051103 and GRB 070201. In the last run of the Laser Interferometer Gravitational-Wave Observatory (LIGO), no gravitational wave signal was found for these gamma-ray bursts, and a conclusive explanation for this needs to be found.
%@language en
%3 MNRAS-2014-Moraes-L11-5.pdf