| 1. Identity statement | |
| Reference Type | Journal Article |
| Site | mtc-m16c.sid.inpe.br |
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identifier | 6qtX3pFwXQZ3P8SECKy/CBPab |
| Repository | sid.inpe.br/jeferson/2004/06.30.11.05 (restricted access) |
| Last Update | 2006:06.14.04.04.12 (UTC) administrator |
| Metadata Repository | sid.inpe.br/jeferson/2004/06.30.11.05.28 |
| Metadata Last Update | 2018:06.04.04.12.52 (UTC) administrator |
| Secondary Key | INPE-10788-PRE/6245 |
| ISBN/ISSN | 0264-9381 |
| ISSN | 0264-9381 |
| Citation Key | MirandaArauAgui:2004:CaBaGr |
| Title | Can a background of gravitational waves constrain the star formation history of the universe?  |
| Year | 2004 |
| Secondary Date | 20040205 |
| Month | Mar |
| Access Date | 2024, Apr. 28 |
| Secondary Type | PRE PI |
| Number of Files | 1 |
| Size | 108 KiB |
| 2. Context | |
| Author | 1 Miranda, Oswaldo Duarte 2 Araujo, Jose Carlos Neves de 3 Aguiar, Odylio Denys de |
| Resume Identifier | 1 8JMKD3MGP5W/3C9JJ2G 2 8JMKD3MGP5W/3C9JHGK 3 8JMKD3MGP5W/3C9JJ2A |
| Group | 1 DAS-INPE-MCT-BR |
| Affiliation | 1 Instituto Tecnológico de Aeronáutica - Departamento de Física 2 Instituto Nacional de Pesquisas Espaciais - Divisão de Astrofísica |
| e-Mail Address | oswaldo@fis.ita.br |
| Journal | Classical and Quantum Gravity |
| Volume | 21 |
| Number | 5 |
| Pages | S557-S562 |
| History (UTC) | 2007-03-05 21:29:48 :: 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 | alpha forest population enrichment density gravitational wave |
| Abstract | In general, the history of star formation of the universe is obtained from hydrodynamical simulations in a _-CDM cosmology. On the other hand, a complete study of the formation of the first objects and the feedback effects on the ambient medium produced by them, is not still possible with the present numerical approaches. However, formation of stars at different redshifts can produce a stochastic background of gravitational waves in the VIRGO and LIGO frequency band and so the detection of this background could directly be used to obtain information about the star formation rate density of the Universe. Here, we use the Press–Schechter formalism to calculate the comoving abundance of halos and themass contained within the collapsed objects of a given mass range. Then, we study, in particular for a pair of advanced LIGO observatories, what limits could be imposed on the fraction of baryons converted into stars within halos that collapse at redshifts 5 < z < 30. |
| Area | CEA |
| Arrangement | urlib.net > Produção anterior à 2021 > DIDAS > Can a 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 | Can a background of gravitational waves.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 |
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