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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnK2Y/Qzax9
Repositorysid.inpe.br/mtc-m17@80/2007/06.26.16.39   (restricted access)
Last Update2007:11.09.14.10.19 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m17@80/2007/06.26.16.39.45
Metadata Last Update2018:06.05.03.34.25 (UTC) administrator
Secondary KeyINPE-14861-PRE/9775
ISSN0001-7701
Citation KeyAraújoMira:2007:SoGaDi
TitleA solution for galactic disks with Yukawian gravitational potential
Year2007
MonthJune
Access Date2024, Apr. 28
Secondary TypePRE PI
Number of Files1
Size147 KiB
2. Context
Author1 Araújo, José Carlos Neves de
2 Miranda, Oswaldo Duarte
Resume Identifier1
2 8JMKD3MGP5W/3C9JJ2G
Group1 DAS-INPE-MCT-BR
2 DAS-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 jcarlos@das.inpe.br
2 oswaldo@das.inpe.br
JournalGeneral Relativity and Gravitation
Volume39
Number6
Pages777-784
History (UTC)2007-11-09 14:10:19 :: simone -> administrator ::
2012-10-23 23:55:18 :: administrator -> simone :: 2007
2013-02-20 15:20:00 :: simone -> administrator :: 2007
2018-06-05 03:34:25 :: administrator -> marciana :: 2007
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsEXTENDED ROTATION CURVES
MODIFIED DYNAMICS
SPIRAL GALAXIES
CLUSTER
AbstractWe present a new solution for the rotation curves of galactic disks with gravitational potential of the Yukawa type. We follow the technique employed by Toomre in 1963 in the study of galactic disks in the Newtonian theory. This new solution allows an easy comparison between the Newtonian solution and the Yukawian one. Therefore, constraints on the parameters of theories of gravitation can be imposed, which in the weak field limit reduce to Yukawian potentials. We then apply our formulae to the study of rotation curves for a zero-thickness exponential disk and compare it with the Newtonian case studied by Freeman in 1970. As an application of the mathematical tool developed here, we show that in any theory of gravity with a massive graviton (this means a gravitational potential of the Yukawa type), a strong limit can be imposed on the mass (m(g)) of this particle. For example, in order to obtain a galactic disk with a scale length of b similar to 10 kpc, we should have a massive graviton of m(g) << 10(-59)g. This result is much more restrictive than those inferred from solar system observations.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > A solution for...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target Filea solution for galactic.pdf
User Groupadministrator
simone
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft12
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
e-Mail (login)marciana
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