1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m16c.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 6qtX3pFwXQZ3P8SECKy/CDaAz |
Repository | sid.inpe.br/jeferson/2004/07.02.16.31 (restricted access) |
Last Update | 2006:06.14.04.07.30 (UTC) administrator |
Metadata Repository | sid.inpe.br/jeferson/2004/07.02.16.31.44 |
Metadata Last Update | 2018:06.04.04.12.52 (UTC) administrator |
Secondary Key | INPE-10795-PRE/6251 |
ISBN/ISSN | 0264-9381 |
ISSN | 0264-9381 |
Citation Key | AraujoMiraAgui:2004:GrWaBa |
Title | Gravitational wave background from stellar black holes in a scenario of structure formation. |
Year | 2004 |
Month | Mar. |
Access Date | 2024, Apr. 27 |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 65 KiB |
|
2. Context | |
Author | 1 Araujo, Jose 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 Instituto Tecnológico de Aeronáutica - Departamento de Física |
e-Mail Address | jcarlos@das.inpe.br |
Journal | Classical and Quantum Gravity |
Volume | 21 |
Number | 5 |
Pages | S545-S549 |
History (UTC) | 2007-03-05 21:29:54 :: administrator -> marciana :: 2008-05-02 16:20:25 :: 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 | STARS. Gravitational wave background black hele |
Abstract | We study the generation of a stochastic gravitational wave (GW) background produced from a population of core-collapse supernovae, which form black holes in scenarios of structure formation. In particular, we take into account in the present paper the history of star formation derived by Springel & Hernquist, who employed hydrodynamic simulations of structure formation in a lambda cold dark matter (LCDM) cosmology. In addition, and contrary to previous studies, we consider the effect of taking into account different values of the ? parameter, the fraction of the progenitor mass which forms the black hole. Different values of ? imply different frequency bands for the GWs produced. Because the sensitivity of the GW detectors depends on the frequency of the GWs, it is worth studying the influence of ? on the detection of the background considered here. We then study the detectability of the GW background produced in scenarios such as those studied here and discuss what astrophysical informationcould be obtained from a positive – or even negative – detection of such a putative background. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Gravitational wave background... |
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 | Gravitational Wave Background1.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 secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype |
|
7. Description control | |
e-Mail (login) | marciana |
update | |
|