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Differences between scalar field and scalar density field solutions

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 01 Jan 2012Embargo end date: 01 Jan 2007 Turkey Publisher:Canadian Science PublishingJournal:Canadian Journal of Physics, volume 90, pages 91-95 (issn: 0008-4204, eissn: 1208-6045, Copyright policy )
Authors: Sert I.; Pirinççiog˜lu N.;

doi: 10.1139/p11-146 , 10.48550/arxiv.gr-qc/0701160

arXiv: http://arxiv.org/abs/gr-qc/0701160

handle: 11454/18982

Differences between scalar field and scalar density field solutions

Abstract

Differences between scalar field and scalar density solutions are explored using a Robertson–Walker (RW) metric, and a nonrelativistic Hamiltonian is derived for a scalar density field in the post-newtonian approximation. The results are compared with those of a scalar field. The expanding universe in a RW metric and a post-newtonian solution of the Klein–Gordon equation are discussed separately.

Country
Turkey
Related Organizations
Keywords

FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), General Relativity and Quantum Cosmology

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
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bronze