Kaluza-Klein-Carmeli Metric from Quaternion-Cliord Space, Lorentz’s Force, and Some Observables

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dc.creatorChristianto, Victor
dc.creatorSmarandache, Florentin
dc.date2008-04
dc.date.accessioned2013-09-02T03:36:04Z
dc.date.available2013-09-02T03:36:04Z
dc.date.issued2013-09-02
dc.descriptionIt was known for quite long time that a quaternion space can be generalized to a Clifford space, and vice versa; but how to find its neat link with more convenient metric form in the General Relativity theory, has not been explored extensively. We begin with a representation of group with non-zero quaternions to derive closed FLRW metric [1], and from there obtains Carmeli metric, which can be extended further to become 5D and 6D metric (which we propose to call Kaluza-Klein-Carmeli metric). Thereafter we discuss some plausible implications of this metric, beyond describing a galaxy’s spiraling motion and redshift data as these have been done by Carmeli and Hartnett [4, 5, 6]. In subsequent section we explain Podkletnov’s rotating disc experiment. We also note possible implications to quantum gravity. Further observations are of course recommended in order to refute or verify this proposition.
dc.formatapplication/pdf
dc.identifierhttp://scireprints.lu.lv/116/1/PP-13-19quaterniongroupCarmeli.pdf
dc.identifierChristianto, Victor and Smarandache, Florentin (2008) Kaluza-Klein-Carmeli Metric from Quaternion-Cliord Space, Lorentz’s Force, and Some Observables. Progress in Physics, vol. 2, 2008, 2 (-). pp. 144-150.
dc.identifier.urihttps://dspace.lu.lv/dspace/handle/7/1737
dc.language.isolaven_US
dc.relationhttp://scireprints.lu.lv/116/
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectQC00 Physics (General)
dc.titleKaluza-Klein-Carmeli Metric from Quaternion-Cliord Space, Lorentz’s Force, and Some Observables
dc.typeArticle
dc.typePeerReviewed
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