| 1. Identity statement | |
| Reference Type | Journal Article |
| Site | mtc-m16c.sid.inpe.br |
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identifier | 6qtX3pFwXQZ3P8SECKy/CBVid |
| Repository | sid.inpe.br/jeferson/2004/06.30.15.53 (restricted access) |
| Last Update | 2006:06.14.04.04.24 (UTC) administrator |
| Metadata Repository | sid.inpe.br/jeferson/2004/06.30.15.53.50 |
| Metadata Last Update | 2018:06.04.04.12.52 (UTC) administrator |
| Secondary Key | INPE-10781-PRE/6238 |
| ISBN/ISSN | 0264-9381 |
| ISSN | 0264-9381 |
| Citation Key | CostaAguiMaga:2004:ReBrGr |
| Title | Response of the Brazilian gravitational wave detector to signals from a black hole ringdown  |
| Year | 2004 |
| Secondary Date | 20040210 |
| Month | Mar. |
| Access Date | 2024, Apr. 28 |
| Secondary Type | PRE PI |
| Number of Files | 1 |
| Size | 202 KiB |
| 2. Context | |
| Author | 1 Costa, César Augusto 2 Aguiar, Odylio Denys de 3 Magalhães, Nadja Simão |
| Resume Identifier | 1 2 8JMKD3MGP5W/3C9JJ2A |
| Group | 1 DAS-INPE-MCT-BR |
| Affiliation | 1 Instituto Nacional de Pesquisas Espaciais - Divisão de Astrofísica 2 Instituto Tecnológico de Aeronáutica - Departamento de Física |
| e-Mail Address | cesar@das.inpe.br |
| Journal | Classical and Quantum Gravity |
| Volume | 21 |
| Number | 5 Sp. Iss. |
| Pages | S827-S832 |
| History (UTC) | 2007-03-05 21:29:52 :: administrator -> marciana :: 2008-07-23 17:14:28 :: marciana -> administrator :: 2018-06-04 04:12:52 :: administrator -> marciana :: 2004 |
| 3. Content and structure | |
| Is the master or a copy? | is the master |
| Content Stage | completed |
| Transferable | 1 |
| Content Type | External Contribution |
| Keywords | mass antenna coalescences sensitivity merger gravitational wave schemberg model black hole |
| Abstract | It is assumed that a black hole can be disturbed in such a way that a ringdown gravitational wave would be generated. This ringdown waveform is well understood and is modelled as an exponentially damped sinusoid. In this work, we use this kind of waveform to study the performance of the SCHENBERG gravitationalwave detector. This first realistic simulationwill help us to develop strategies for the signal analysis of this Brazilian detector. We calculated the signal-to-noise ratio as a function of frequency for the simulated signals and obtained results that show that SCHENBERG is expected to be sensitive enough to detect this kind of signal up to a distance of ~20 kpc. |
| Area | CEA |
| Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Response of the... |
| doc Directory Content | access |
| source Directory Content | there are no files |
| agreement Directory Content | there are no files |
| 4. Conditions of access and use | |
| Language | en |
| Target File | Response of the Brazilian gravitational wave detector.pdf |
| User Group | administrator marciana valdirene |
| Visibility | shown |
| Copy Holder | SID/SCD |
| Archiving Policy | denypublisher denyfinaldraft12 |
| Read Permission | deny from all and allow from 150.163 |
| 5. Allied materials | |
| Next Higher Units | 8JMKD3MGPCW/3ETR8EH |
| Dissemination | WEBSCI; PORTALCAPES; COMPENDEX. |
| Host Collection | sid.inpe.br/mtc-m18@80/2008/03.17.15.17 |
| 6. Notes | |
| Empty Fields | alternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi electronicmailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype |
| 7. Description control | |
| e-Mail (login) | marciana |
| update | |