A (giant) void is not mandatory to explain away dark energy with a Lemaître-Tolman model

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dc.contributor.authorCélérier, M-N
dc.contributor.authorBolejko, K
dc.contributor.authorKrasiński, A
dc.date.accessioned2021-10-08T11:01:04Z
dc.date.available2021-10-08T11:01:04Z
dc.date.issued2010
dc.description.abstractContext. Lemaître-Tolman (L-T) toy models with a central observer have been used to study the effect of large scale inhomogeneities on the SN Ia dimming. Claims that a giant void is mandatory to explain away dark energy in this framework are currently dominating.
dc.identifier.apacitationCélérier, M., Bolejko, K., & Krasiński, A. (2010). A (giant) void is not mandatory to explain away dark energy with a Lemaître-Tolman model. <i>Astronomy and Astrophysics</i>, 518(4), A21 - 177. http://hdl.handle.net/11427/35080en_ZA
dc.identifier.chicagocitationCélérier, M-N, K Bolejko, and A Krasiński "A (giant) void is not mandatory to explain away dark energy with a Lemaître-Tolman model." <i>Astronomy and Astrophysics</i> 518, 4. (2010): A21 - 177. http://hdl.handle.net/11427/35080en_ZA
dc.identifier.citationCélérier, M., Bolejko, K. & Krasiński, A. 2010. A (giant) void is not mandatory to explain away dark energy with a Lemaître-Tolman model. <i>Astronomy and Astrophysics.</i> 518(4):A21 - 177. http://hdl.handle.net/11427/35080en_ZA
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.ris TY - Journal Article AU - Célérier, M-N AU - Bolejko, K AU - Krasiński, A AB - Context. Lemaître-Tolman (L-T) toy models with a central observer have been used to study the effect of large scale inhomogeneities on the SN Ia dimming. Claims that a giant void is mandatory to explain away dark energy in this framework are currently dominating. DA - 2010 DB - OpenUCT DP - University of Cape Town IS - 4 J1 - Astronomy and Astrophysics LK - https://open.uct.ac.za PY - 2010 SM - 0004-6361 SM - 1432-0746 T1 - A (giant) void is not mandatory to explain away dark energy with a Lemaître-Tolman model TI - A (giant) void is not mandatory to explain away dark energy with a Lemaître-Tolman model UR - http://hdl.handle.net/11427/35080 ER - en_ZA
dc.identifier.urihttp://hdl.handle.net/11427/35080
dc.identifier.vancouvercitationCélérier M, Bolejko K, Krasiński A. A (giant) void is not mandatory to explain away dark energy with a Lemaître-Tolman model. Astronomy and Astrophysics. 2010;518(4):A21 - 177. http://hdl.handle.net/11427/35080.en_ZA
dc.language.isoeng
dc.publisher.departmentDepartment of Mathematics and Applied Mathematics
dc.publisher.facultyFaculty of Science
dc.sourceAstronomy and Astrophysics
dc.source.journalissue4
dc.source.journalvolume518
dc.source.paginationA21 - 177
dc.source.urihttps://dx.doi.org/10.1051/0004-6361/200913581
dc.subject.othercosmology: dark energy
dc.subject.othercosmology: miscellaneous
dc.titleA (giant) void is not mandatory to explain away dark energy with a Lemaître-Tolman model
dc.typeJournal Article
uct.type.publicationResearch
uct.type.resourceJournal Article
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