@Article{BortoliFrajAgui:2018:ScMiCa,
author = "Bortoli, F. S. and Frajuca, C. and Aguiar, Odylio Denys de",
affiliation = "{Instituto Federal de S{\~a}o Paulo (IFSP)} and {Instituto
Federal de S{\~a}o Paulo (IFSP)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)}",
title = "Schenberg microwave cabling seismic isolation",
journal = "Journal of Physics: Conference Series",
year = "2018",
volume = "957",
number = "1",
pages = "e012013",
month = "mar.",
note = "{12th Edoardo Amaldi Conference on Gravitational Waves (AMALDI
12)}",
abstract = "SCHENBERG is a resonant-mass gravitational wave detector with a
frequency about 3.2 kHz. Its spherical antenna, weighing 1.15
metric ton, is connected to the external world by a system which
must attenuate seismic noise. When a gravitational wave passes the
antenna vibrates, its motion is monitored by transducers. These
parametric transducers uses microwaves carried by coaxial cables
that are also connected to the external world, they also carry
seismic noise. In this analysis the system was modeled using
finite element method. This work shows that the addition of masses
along these cables can decrease this noise, so that this noise is
below the thermal noise of the detector when operating at 50 mK.",
doi = "10.1088/1742-6596/957/1/012013",
url = "http://dx.doi.org/10.1088/1742-6596/957/1/012013",
issn = "1742-6588",
language = "en",
targetfile = "bortoli_schenberg.pdf",
urlaccessdate = "27 abr. 2024"
}