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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/46MLNJB
Repositorysid.inpe.br/mtc-m21d/2022/04.14.12.15   (restricted access)
Last Update2022:04.14.12.15.55 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2022/04.14.12.15.55
Metadata Last Update2023:01.03.16.46.04 (UTC) administrator
DOI10.1007/s13538-021-01014-2
ISSN0103-9733
Citation KeyEvangelista:2022:StBaGr
TitleStochastic Background of Gravitational Waves Generated by Black Hole MACHO Binaries in the Galaxy
Year2022
MonthJune
Access Date2024, May 14
Type of Workjournal article
Secondary TypePRE PN
Number of Files1
Size2631 KiB
2. Context
AuthorEvangelista, Edgard de Freitas Diniz
GroupDIAST-CGCE-INPE-MCTI-GOV-BR
AffiliationInstituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Addressedgard.inpe@gmail.com
JournalBrazilian Journal of Physics
Volume52
Number3
Pagese91
Secondary MarkB1_INTERDISCIPLINAR B1_GEOCIÊNCIAS B1_ENGENHARIAS_IV B1_ENGENHARIAS_III B1_CIÊNCIAS_AGRÁRIAS_I B1_BIODIVERSIDADE B1_ASTRONOMIA_/_FÍSICA B2_ODONTOLOGIA B2_MATERIAIS B2_FARMÁCIA B2_ENGENHARIAS_II B2_ECONOMIA B2_CIÊNCIA_DA_COMPUTAÇÃO B3_MEDICINA_II B3_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA B3_CIÊNCIAS_AMBIENTAIS B3_BIOTECNOLOGIA B4_QUÍMICA B4_ENSINO B4_CIÊNCIAS_BIOLÓGICAS_III B4_CIÊNCIAS_BIOLÓGICAS_II B4_CIÊNCIAS_BIOLÓGICAS_I
History (UTC)2022-04-14 12:15:55 :: simone -> administrator ::
2022-04-14 12:15:56 :: administrator -> simone :: 2022
2022-04-14 12:16:11 :: simone -> administrator :: 2022
2023-01-03 16:46:04 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsDark Matter
Galaxy
Gravitational Waves
MACHO
Stochastic Background
AbstractThe interest in gravitational waves (GW) has increased since the recent detections of such signals announced by the LIGO Scientific Collaboration and the Virgo Collaboration. On the other hand, also interesting is the study of the stochastic backgrounds of GW (SBGW), which could in principle be generated by a variety of sources and astrophysical processes; particularly, in the present paper we are concerned with the SBGW from MACHO binaries in the Galaxy. In our scheme, we take into account only MACHOs which are black holes (BHMACHOs) and are located up to 50 kpc from the center of the Galaxy. Our spectra, which are calculated in the scenarios with Ω h2= 0.1 and Ω h2= 1.0 , are parameterized by the fraction of the Galaxys dark halo mass which is in the form of BHMACHOs and are compared with some results found in the literature. Besides, we investigate in what situations the backgrounds are above the sensitivity curves of the Laser Interferometer Space Antenna (LISA), Einstein Telescope (ET), Advanced Virgo (AdV) and Advanced Laser Interferometer Gravitational-Wave Observatory Plus (LIGO A+).
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Stochastic Background of...
doc Directory Contentaccess
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4. Conditions of access and use
Languageen
Target FileEvangelista2022_Article_StochasticBackgroundOfGravitat.pdf
User Groupsimone
Reader Groupadministrator
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Visibilityshown
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
DisseminationWEBSCI; PORTALCAPES; SCIELO; SCOPUS.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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