@Article{LiccardoLeMaAgFrBoCo:2023:DeStSe,
author = "Liccardo, Vincenzo and Lenzi, C. H. and Marinho Junior, R. M. and
Aguiar, Odylio Denys de and Frajuca, C. and Bortoli, F. da Silva
and Costa, Cesar Augusto",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Tecnol{\'o}gico de Aeron{\'a}utica (ITA)} and {Instituto
Tecnol{\'o}gico de Aeron{\'a}utica (ITA)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {} and {} and
{Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "The design strain sensitivity of the schenberg spherical resonant
antenna for gravitational waves",
journal = "Scientific Reports",
year = "2023",
volume = "13",
number = "1",
pages = "e17706",
month = "Dec.",
abstract = "The main purpose of this study is to review the Schenberg resonant
antenna transfer function and to recalculate the antenna design
strain sensitivity for gravitational waves. We consider the
spherical antenna with six transducers in the semi dodecahedral
configuration. When coupled to the antenna, the transducer-sphere
system will work as a mass-spring system with three masses. The
first one is the antenna effective mass for each quadrupole mode,
the second one is the mass of the mechanical structure of the
transducer first mechanical mode and the third one is the
effective mass of the transducer membrane that makes one of the
transducer microwave cavity walls. All the calculations are done
for the degenerate (all the sphere quadrupole mode frequencies
equal) and non-degenerate sphere cases. We have come to the
conclusion that the ultimate sensitivity of an advanced version of
Schenberg antenna (aSchenberg) is around the standard quantum
limit (although the parametric transducers used could, in
principle, surpass this limit). However, this sensitivity, in the
frequency range where Schenberg operates, has already been
achieved by the two aLIGOs in the O3 run, therefore, the only
reasonable justification for remounting the Schenberg antenna and
trying to place it in the sensitivity of the standard quantum
limit would be to detect gravitational waves with another physical
principle, different from the one used by laser interferometers.
This other physical principle would be the absorption of the
gravitational wave energy by a resonant mass like Schenberg.",
doi = "10.1038/s41598-023-43808-1",
url = "http://dx.doi.org/10.1038/s41598-023-43808-1",
issn = "2045-2322",
language = "en",
targetfile = "s41598-023-43808-1.pdf",
urlaccessdate = "16 jun. 2024"
}