@InProceedings{AraújoCoelLadiCost:2022:GrWaPu,
author = "Ara{\'u}jo, Jos{\'e} Carlos Neves de and Coelho, Jaziel G. and
Ladislau, Samantha Monaliza and Costa, Cesar Augusto",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and
{Universidade Tecnol{\'o}gica Federal do Paran{\'a} (UTFPR)} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)}",
title = "Gravitational waves from pulsars due to their magnetic
ellipticity",
booktitle = "Proceedings...",
year = "2022",
pages = "1539",
organization = "MG15. Meeting on General Relativity",
note = "{Setores de Atividade: Pesquisa e desenvolvimento
cient{\'{\i}}fico.}",
keywords = "Pulsars, Estrela de Neutrons.",
abstract = "We discuss some aspects of de Araujo, Coelho and Costa 1,2
concerning the role of a time dependent magnetic ellipticity on
the pulsars braking indices and on the putative gravitational
waves (GWs) these objects can emit. Since only nine of more than
2000 known pulsars have accurately measured braking indices, it is
of interest to extend this study to all known pulsars, in
particular as regards GW generation. In summary, our results show
a pessimistic prospect for the detection of GWs generated by these
pulsars, even for advanced detectors such as aLIGO and AdVirgo,
and the planned Einstein Telescope, would not be able to detect
these pulsar, if the ellipticity has magnetic origin.",
conference-location = "University of Rome La Sapienza",
conference-year = "2018",
doi = "10.1142/9789811258251_0226",
url = "http://dx.doi.org/10.1142/9789811258251_0226",
isbn = "9789811258244",
label = "lattes: 6217296674061205 1 AraujoCoelLadiCost:2022:GrWaPu",
language = "en",
targetfile = "1906.00774.pdf",
urlaccessdate = "12 maio 2024"
}