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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnK2Y/Nicf6
Repositorysid.inpe.br/mtc-m17@80/2006/11.28.12.41   (restricted access)
Last Update2006:11.28.12.45.27 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m17@80/2006/11.28.12.41.37
Metadata Last Update2018:06.05.03.44.05 (UTC) administrator
Secondary KeyINPE-14363-PRE/9450
ISSN0378-4371
Citation KeyAbramoSodrSouz:2006:AnLoCM
TitleAnomalies in the low CMB multipoles and extended foregrounds
Year2006
Access Date2024, Apr. 28
Secondary TypePRE PI
Number of Files1
Size920 KiB
2. Context
Author1 Abramo, L. Raul
2 Sodré Júnior, Laerte
3 Souza, Carlos Alexandre Wuensche de
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JGQK
Group1
2
3 DAS-INPE-MCT-BR
Affiliation1 Instituto de Física, Universidade de São Paulo
2 Departamento de Astronomia, Instituto Astronômico e Geofísico, Universidade de São Paulo
3 Instituto Nacional de Pesquisas Espaciais (INPE)
JournalPhysica A: Statistical Mechanics and its Applications
Volume74
History (UTC)2006-11-28 12:45:27 :: simone -> administrator ::
2008-06-29 02:28:46 :: administrator -> simone ::
2008-11-04 18:42:37 :: simone -> banon ::
2010-05-17 19:10:27 :: banon -> administrator ::
2012-11-24 01:39:06 :: administrator -> simone :: 2006
2013-02-20 15:19:51 :: simone -> administrator :: 2006
2018-06-05 03:44:05 :: administrator -> marciana :: 2006
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractWe discuss how an extended foreground of the cosmic microwave background (CMB) can account for the anomalies in the low multipoles of the CMB anisotropies. The distortion needed to account for the anomalies is consistent with a cold spot with the spatial geometry of the local supercluster (LSC) and a temperature quadrupole of order T2 2 50 K2. If this hypothetic foreground is subtracted from the CMB data, the amplitude of the quadrupole ( 2) is substantially increased, and the statistically improbable alignment of the quadrupole with the octopole ( 3) is substantially weakened, increasing dramatically the likelihood of the cleaned maps. By placing the foreground on random locations and then computing the likelihood of the cleaned maps we can estimate the most likely place for this foreground. Although the 1-year WMAP data clearly points the location of this hypothetical foreground to the LSC or its specular image (i.e., the vicinity of the poles of the cosmic dipole axis), the three-year data seems to point to these locations as well as the north ecliptic pole. We show that this is consistent with the symmetries of the cosmic quadrupole. We also discuss a possible mechanism that could have generated this foreground: the thermal Sunyaev-Zeldovich effect caused by hot electrons in the LSC. We argue that the temperature and density of the hot gas which are necessary to generate such an effect, though in the upper end of the expected range of values, are marginally consistent with present observations of the X-ray background of spectral distortions of the CMB.
AreaCEA
Arrangementurlib.net > DMA > Anomalies in the...
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4. Conditions of access and use
Languageen
Target FileAnomalies in the low CMB.pdf
User Groupadministrator
banon
simone
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; PORTALCAPES; COMPENDEX.
Host Collectionlcp.inpe.br/ignes/2004/02.12.18.39
cptec.inpe.br/walmeida/2003/04.25.17.12
6. Notes
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7. Description control
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