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  Probing non-Riemannian spacetime geometry

Puetzfeld, D., & Obukhov, Y. N. (2008). Probing non-Riemannian spacetime geometry. Physics Letters A, 372(45), 6711-6717. doi:10.1016/j.physleta.2008.09.041.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-6D8F-9 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-6D94-C
Genre: Journal Article

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0708.1926v2OJ.pdf (Publisher version), 260KB
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 Creators:
Puetzfeld, Dirk1, Author              
Obukhov, Yuri N.2, Author
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, Golm, DE, ou_24013              
2External Organizations, ou_persistent22              

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Free keywords: gr-qc astro-ph
 Abstract: The equations of motion for matter in non-Riemannian spacetimes are derived via a multipole method. It is found that only test bodies with microstructure couple to the non-Riemannian spacetime geometry. Consequently it is impossible to detect spacetime torsion with the satellite experiment Gravity Probe B, contrary to some recent claims in the literature.

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 Dates: 2008-10-30
 Publication Status: Published online
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 Identifiers: DOI: 10.1016/j.physleta.2008.09.041
eDoc: 390581
arXiv: 0708.1926
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Title: Physics Letters A
Source Genre: Journal
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Pages: - Volume / Issue: 372 (45) Sequence Number: - Start / End Page: 6711 - 6717 Identifier: ISSN: 0375-9601