1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m16b.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 6qtX3pFwXQZGivnK2Y/Qzax9 |
Repository | sid.inpe.br/mtc-m17@80/2007/06.26.16.39 (restricted access) |
Last Update | 2007:11.09.14.10.19 (UTC) administrator |
Metadata Repository | sid.inpe.br/mtc-m17@80/2007/06.26.16.39.45 |
Metadata Last Update | 2018:06.05.03.34.25 (UTC) administrator |
Secondary Key | INPE-14861-PRE/9775 |
ISSN | 0001-7701 |
Citation Key | AraújoMira:2007:SoGaDi |
Title | A solution for galactic disks with Yukawian gravitational potential |
Year | 2007 |
Month | June |
Access Date | 2024, May 11 |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 147 KiB |
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2. Context | |
Author | 1 Araújo, José Carlos Neves de 2 Miranda, Oswaldo Duarte |
Resume Identifier | 1 2 8JMKD3MGP5W/3C9JJ2G |
Group | 1 DAS-INPE-MCT-BR 2 DAS-INPE-MCT-BR |
Affiliation | 1 Instituto Nacional de Pesquisas Espaciais (INPE) 2 Instituto Nacional de Pesquisas Espaciais (INPE) |
Author e-Mail Address | 1 jcarlos@das.inpe.br 2 oswaldo@das.inpe.br |
Journal | General Relativity and Gravitation |
Volume | 39 |
Number | 6 |
Pages | 777-784 |
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 |
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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 |
Keywords | EXTENDED ROTATION CURVES MODIFIED DYNAMICS SPIRAL GALAXIES CLUSTER |
Abstract | We 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. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > A solution for... |
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 | |
Language | en |
Target File | a solution for galactic.pdf |
User Group | administrator simone |
Visibility | shown |
Copy Holder | SID/SCD |
Archiving Policy | denypublisher denyfinaldraft12 |
Read Permission | deny from all and allow from 150.163 |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/3ETR8EH |
Dissemination | WEBSCI; PORTALCAPES; COMPENDEX. |
Host Collection | lcp.inpe.br/ignes/2004/02.12.18.39 cptec.inpe.br/walmeida/2003/04.25.17.12 |
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6. Notes | |
Empty Fields | alternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage doi e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype |
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7. Description control | |
e-Mail (login) | marciana |
update | |
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