| 1. Identity statement | |
| Reference Type | Journal Article |
| Site | mtc-m16.sid.inpe.br |
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identifier | 6qtX3pFwXQZGivnJVY/M2gKM |
| Repository | sid.inpe.br/mtc-m16@80/2006/08.01.18.46 (restricted access) |
| Last Update | 2006:08.01.18.46.13 (UTC) administrator |
| Metadata Repository | sid.inpe.br/mtc-m16@80/2006/08.01.18.46.14 |
| Metadata Last Update | 2018:06.05.01.16.54 (UTC) administrator |
| Secondary Key | INPE-13923--PRE/9103 |
| ISSN | 1742-6588 |
| Citation Key | AraújoMira:2006:StFoRa |
| Title | The star formation rate density and the stochastic background of gravitational waves  |
| Year | 2006 |
| Access Date | 2024, Apr. 23 |
| Secondary Type | PRE PI |
| Number of Files | 1 |
| Size | 90 KiB |
| 2. Context | |
| Author | 1 Araújo, José Carlos Neves de 2 Miranda, Oswaldo Duarte |
| Resume Identifier | 1 8JMKD3MGP5W/3C9JHGK 2 8JMKD3MGP5W/3C9JJ2G |
| Group | 1 DAS-INPE-MCT-BR 2 DAS-INPE-MCT-BR |
| Affiliation | 1 Instituto Nacional de Pesquisas Espaciais, Divisão de Astrosífica (INPE.DAS) 2 Instituto Nacional de Pesquisas Espaciais, Divisão de Astrosífica (INPE.DAS) |
| Journal | Journal of Physics: Conference Series |
| Volume | 32 |
| Pages | 323-326 |
| History (UTC) | 2006-08-01 18:46:14 :: simone -> administrator :: 2012-07-17 12:47:32 :: administrator -> banon :: 2006 2012-09-27 18:28:26 :: banon -> administrator :: 2006 2018-06-05 01:16:54 :: administrator -> marciana :: 2006 |
| 3. Content and structure | |
| Is the master or a copy? | is the master |
| Content Stage | completed |
| Transferable | 1 |
| Content Type | External Contribution |
| Abstract | There is in the literature a number of papers addressing the stochastic background of gravitational waves (GWs) generated by an ensemble of astrophysical sources. The main ingredient in such studies is the so called star formation rate density (SFRD), which gives the density of stars formed per unit time. Some authors argue, however, that there is, in the equation that determines the amplitude of the stochastic background of GWs, an additional (1 + z) term dividing the SFRD, which would account for the effect of cosmic expansion onto the time variable. We argue here that the inclusion of this additional term is wrong. In order to clarify where the inclusion of the (1 + z) term is really necessary, we briefly discuss the calculation of event rates in the study of GRBs (gamma ray bursts) from cosmological origin. . |
| Area | CEA |
| Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > The star formation... |
| 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 | The star formation rate density.pdf |
| User Group | administrator banon simone |
| 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/banon/2003/08.15.17.40 |
| 6. Notes | |
| Empty Fields | alternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi e-mailaddress electronicmailaddress format isbn keywords label lineage mark mirrorrepository month nextedition notes number 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 | |