| 1. Identity statement | |
| Reference Type | Journal Article |
| Site | mtc-m16.sid.inpe.br |
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identifier | 6qtX3pFwXQZ3r59YDa/H2oRQ |
| Repository | sid.inpe.br/iris@1916/2005/08.01.17.07 (restricted access) |
| Last Update | 2006:06.05.13.47.29 (UTC) administrator |
| Metadata Repository | sid.inpe.br/iris@1916/2005/08.01.17.07.29 |
| Metadata Last Update | 2018:06.05.01.16.07 (UTC) administrator |
| Secondary Key | INPE-13047-PRE/8317 |
| ISSN | 0264-9381 |
| Citation Key | AraujoMiraAgui:2005:DeFmUn |
| Title | Detectability of f-mode unstable neutron stars by the Schenberg spherical antenna  |
| Year | 2005 |
| Month | May |
| Access Date | 2024, Apr. 28 |
| Secondary Type | PRE PI |
| Number of Files | 1 |
| Size | 96 KiB |
| 2. Context | |
| Author | 1 Araujo, José Carlos Neves de 2 Miranda, Oswaldo Duarte 3 Aguiar, Odylio Denys de |
| Resume Identifier | 1 8JMKD3MGP5W/3C9JHGK 2 8JMKD3MGP5W/3C9JJ2G 3 8JMKD3MGP5W/3C9JJ2A |
| Group | 1 DAS-INPE-MCT-BR |
| Affiliation | 1 Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica 2 3 |
| Journal | Classical and Quantum Gravity |
| Volume | 22 |
| Number | 10 |
| Pages | S471-S477 Sp. Iss. SI |
| History (UTC) | 2006-06-05 13:47:29 :: sergio -> administrator :: 2006-09-28 22:30:02 :: administrator -> sergio :: 2008-01-07 12:52:53 :: sergio -> administrator :: 2008-06-10 22:39:34 :: administrator -> marciana :: 2011-05-26 00:03:36 :: marciana -> administrator :: 2018-06-05 01:16:07 :: administrator -> marciana :: 2005 |
| 3. Content and structure | |
| Is the master or a copy? | is the master |
| Content Stage | completed |
| Transferable | 1 |
| Content Type | External Contribution |
| Keywords | GAMMA-RAY BURSTS RADIO PULSARS EVOLUTION DETECTOR ORIGIN |
| Abstract | The Brazilian spherical antenna (Schenberg) is planned to detect high frequency gravitational waves (GWs) ranging from 3.0 kHz to 3.4 kHz. There is a host of astrophysical sources capable of being detected by the Brazilian antenna, namely: core collapse in supernova events; (proto)neutron stars undergoing hydrodynamical instability; f-mode unstable neutron stars, caused by quakes and oscillations; excitation of the first quadrupole normal mode of 4-9 solar mass black holes; coalescence of neutron stars and/or black holes; exotic sources such as bosonic or strange matter stars rotating at 1.6 kHz; and inspiralling of mini black-hole binaries. We here address our study in particular to neutron stars, which could well become f-mode unstable producing therefore GWs. We estimate, for this particular source of GWs, the event rates that in principle can be detected by Schenberg and by the Dutch Mini-Grail antenna. |
| Area | CEA |
| Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Detectability of f-mode... |
| 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 | araujo-detectabiblity.pdf |
| User Group | administrator sergio |
| Visibility | shown |
| Copy Holder | SID/SCD |
| Archiving Policy | denypublisher denyfinaldraft12 |
| Read Permission | deny from all and allow from 150.163 |
| Update Permission | transferred to sergio |
| 5. Allied materials | |
| Next Higher Units | 8JMKD3MGPCW/3ETR8EH |
| Dissemination | WEBSCI; PORTALCAPES; COMPENDEX. |
| Host Collection | sid.inpe.br/banon/2003/08.15.17.40 |
| 6. Notes | |
| Empty Fields | alternatejournal archivist callnumber copyright creatorhistory descriptionlevel doi e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype |
| 7. Description control | |
| e-Mail (login) | marciana |
| update | |