1. Identity statement | |
Reference Type | Journal Article |
Site | marte3.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 6qtX3pFwXQZ3r59YCT/H37Pn |
Repository | sid.inpe.br/iris@1905/2005/08.02.21.57 (restricted access) |
Last Update | 2013:03.20.17.34.41 (UTC) jefferson |
Metadata Repository | sid.inpe.br/iris@1905/2005/08.02.21.57.38 |
Metadata Last Update | 2018:06.06.03.54.05 (UTC) administrator |
Secondary Key | INPE-8770-PRE/4493 |
ISSN | 0378-4371 |
Label | 9731 |
Citation Key | AraujoMiraAgui:2000:StBaGr |
Title | Stochastic background of gravitational waves |
Year | 2000 |
Secondary Date | 20010419 |
Access Date | 2024, May 02 |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 1115 KiB |
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2. Context | |
Author | 1 Araujo, José Carlos Neves de 2 Miranda, Oswaldo Duarte 3 Aguiar, Odylio Denys de |
Group | 1 DAS-INPE-MCT-BR 2 DAS-INPE-MCT-BR 3 DAS-INPE-MCT-BR |
Journal | Physica A: Statistical Mechanics and its Applications |
Volume | 61 |
Number | 12 |
Pages | 4015-1-4015-6 |
History (UTC) | 2008-06-09 16:45:38 :: administrator -> banon :: 2010-05-17 19:09:08 :: banon -> administrator :: 2013-03-20 17:34:04 :: administrator -> jefferson :: 2000 2013-03-20 17:34:43 :: jefferson -> administrator :: 2000 2018-06-06 03:54:05 :: administrator -> marciana :: 2000 |
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3. Content and structure | |
Is the master or a copy? | is the master |
Content Stage | completed |
Transferable | 1 |
Content Type | External Contribution |
Version Type | publisher |
Keywords | ASTROFÍSICA emissão fontes processos estocásticos ondas gravitacionais explosões gravitational waves bursts sources emission stochastic processes |
Abstract | A continuous stochastic background of gravitational waves (GWs)for burst sources is produced if the mean time interval between the occurrence of bursts is smaller than the average time duration of a single burst at the emission, i.e., the so-called duty cycle must be greater than one. To evaluate the background of GWs produced by an ensemble of sources, during their formation, for example, one needs to know the average energy flux emitted during the formation of a single object and the formation rate of such objects as well. In many cases the energy flux emitted during an event of production of GWs is not known in detail; only characteristic values for the dimensionless amplitude and frequencies are known. Here we present a shortcut to calculate stochastic backgrounds of GWs produced from cosmological sources. For this approach it is not necessary to know in detail the energy flux emitted at each frequency. Knowing the characteristic values for the "lumped" dimensionless amplitude and frequency we show that it is possible to calculate the stochastic background of GWs produced by an ensemble of sources. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Stochastic background of... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | there are no files |
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4. Conditions of access and use | |
Target File | USING STANDARD SYSTE -.pdf |
User Group | administrator banon jefferson |
Visibility | shown |
Archiving Policy | denypublisher denyfinaldraft24 |
Read Permission | deny from all and allow from 150.163 |
Update Permission | not transferred |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/3ETR8EH |
Dissemination | WEBSCI; PORTALCAPES; COMPENDEX. |
Host Collection | sid.inpe.br/banon/2001/04.03.15.36 |
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6. Notes | |
Empty Fields | affiliation alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel doi e-mailaddress electronicmailaddress format isbn language lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url |
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7. Description control | |
e-Mail (login) | marciana |
update | |
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