Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2697
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dc.contributor.authorSivaram, C-
dc.date.accessioned2008-07-16T06:00:25Z-
dc.date.available2008-07-16T06:00:25Z-
dc.date.issued1993-08-
dc.identifier.citationAstronomy and Astrophysics, Vol. 275, No. 1, pp. 37 - 38en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2248/2697-
dc.description.abstractRecently a new type of gravitational coupling due to a gravo-inductive force field generated by mass currents was introduced to account for constant rotation velocities at large distances from galactic cores. It is pointed out that the exact analogy with electromagnetism assumed in postulating this force would for reason of consistency imply a vanishingly small coupling rather than the anomalously large coupling required. The gravo-inductive radiation is compared with gravitational radiation for its role in the damping of the motion of bound systems.en
dc.format.extent211395 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherEuropean Southern Observatoryen
dc.relation.urihttp://adsabs.harvard.edu/abs/1993A%26A...275...37Sen
dc.subjectGalactic dynamicsen
dc.subjectNon-Newtonian gravitationen
dc.titleOn the Maxwellian alternative to the galactic dark matter problemen
dc.typeArticleen
Appears in Collections:IIAP Publications

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