%0 Journal Article
%@holdercode {isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S}
%@nexthigherunit 8JMKD3MGPCW/3ETR8EH
%@archivingpolicy denypublisher denyfinaldraft24
%@dissemination PORTALCAPES; COMPENDEX.
%X When present-day bar antennas reach the standard quantum limit, cosmic rays are expected to become a significant source of noise. In this work. we estimate the influences of single hadrons and muons on such detectors and compare them to those expected for a hypothetical CuAl detector, since next generation resonant-mass detectors are being considered to have antennas made with this material.
%8 Jan.
%N 1-2
%T Cosmic-ray noise and gravitational wave antennas at the quantum limit
%K  raios cósmicos, ruido, ondas gravitacionais, detectores, gravitational waves, cosmic rays, noise, detectors.
%@secondarytype PRE PI
%@usergroup administrator
%@usergroup jefferson
%@group DAS-INPE-MCT-BR
%@secondarykey INPE-8710-PRE/4440
%F 9701
%@issn 0168-9002
%2 sid.inpe.br/iris@1905/2005/08.02.21.52.20
%B Nuclear Instruments and Methods in Physics Research A
%@versiontype publisher
%P 175-179
%4 sid.inpe.br/iris@1905/2005/08.02.21.52.18
%@documentstage not transferred
%D 2001
%V 457
%A Magalhães, Nadja Simão,
%A Aguiar, Odylio Denys de,
%A Frajuca, Carlos,
%A Marinho Jr., Rubens de Melo,
%@area CEA