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1. Identity statement
Reference TypeJournal Article
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W/3UGCRU5
Repositorysid.inpe.br/plutao/2019/12.03.14.02.27   (restricted access)
Last Update2019:12.05.17.52.26 (UTC) lattes
Metadata Repositorysid.inpe.br/plutao/2019/12.03.14.02.28
Metadata Last Update2021:07.28.22.12.43 (UTC) administrator
DOI10.1088/1475-7516/2019/11/047
ISSN1475-7516
Labellattes: 1448223845901360 4 FortesMiraStecWuen:2019:PoGaRa
Citation KeyFortesMiraStecWuen:2019:PoGaRa
TitleSome implications of the leptonic annihilation of dark matter: possible galactic radio emission signatures and the excess radio flux of extragalactic origin
Year2019
Access Date2024, May 17
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size970 KiB
2. Context
Author1 Fortes, Elaine Cristina Ferreira Silva
2 Miranda, Oswaldo Duarte
3 Stecker, Floyd W.
4 Wuensche, Carlos Alexandre
Resume Identifier1
2 8JMKD3MGP5W/3C9JJ2G
Group1
2 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
3
4 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Universidade Federal do Pampa (UNIPAMPA)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Astrophysics Science Division, NASA Goddard Space Flight Center
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 elainefortes@unipampa.edu.br
2 oswaldo.miranda@inpe.br
3 floyd.w.stecker@nasa.gov
4 ca.wuensche@inpe.br
JournalJournal of Cosmology and Astroparticle Physics
Volume2019
Number11
Pages047-047
Secondary MarkA1_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA A1_ENGENHARIAS_III A1_ASTRONOMIA_/_FÍSICA B1_GEOCIÊNCIAS
History (UTC)2019-12-03 14:02:28 :: lattes -> administrator ::
2019-12-03 14:05:25 :: administrator -> lattes :: 2019
2019-12-03 17:41:33 :: lattes -> administrator :: 2019
2019-12-05 17:50:44 :: administrator -> lattes :: 2019
2019-12-05 17:52:27 :: lattes -> administrator :: 2019
2021-07-28 22:12:43 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Keywordsdark matter theory
particle acceleration
AbstractWe give theoretical predictions for the radio emission of a dark matter candidate annihilating into 2-lepton and 4-lepton final states. We then compare our results with the known radio measurements of the sky temperature as a function of the frequency. In particular, we calculate the radio emission for some dark matter candidates annihilating into intermediate bosons that subsequently decay into a 4-lepton channel with a thermal annihilation cross-section. We show that within the range of frequencies from 20 MHz to 5 GHz, this channel can produce a stronger signature than direct annihilation into leptons.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Some implications of...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target Filefortes_some.pdf
Reader Groupadministrator
lattes
Visibilityshown
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
Citing Item Listsid.inpe.br/bibdigital/2013/10.01.00.07 2
sid.inpe.br/mtc-m21/2012/07.13.14.57.32 1
DisseminationWEBSCI; PORTALCAPES.
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url usergroup versiontype
7. Description control
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