1952
DOI: 10.1103/physrev.88.1369
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Gravitation and Electrodynamics

Abstract: DIFFUSIONCONSTANT AND MOBILITY 1369 obtained : 3 £>/M=0.0268±0.0013ev, r=303±l°K, ^r/^=0.0262±0.0001 ev. 3 The probable error in the values of T and kT/q were not obtained using the method of least squares which would give a value much less than this. Generous allowance is made for systematic uncertainty in recording ambient temperature.It would appear that these results verify the relation D/fx -kT/q. Although there have been other experimental verifications of this relationship using colloidal particles and… Show more

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Cited by 47 publications
(41 citation statements)
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“…The first case was assumed by Papapetrou [75,85,89,90,91] and later by Moffat [71,72]. The second case was assumed by Kurşunoglu and Hély after reading a physical meaning from the contracted Bianchi identities [92,93,94,95,96,97,98,99,100,101]. The fourth case was assumed by Lichnerowicz, who proved, by availing only of the field equations, that g (µν) enters the eikonal equation as the contravariant metric, both geometrically and physically [102].…”
Section: The Equations Of Motionmentioning
confidence: 99%
“…The first case was assumed by Papapetrou [75,85,89,90,91] and later by Moffat [71,72]. The second case was assumed by Kurşunoglu and Hély after reading a physical meaning from the contracted Bianchi identities [92,93,94,95,96,97,98,99,100,101]. The fourth case was assumed by Lichnerowicz, who proved, by availing only of the field equations, that g (µν) enters the eikonal equation as the contravariant metric, both geometrically and physically [102].…”
Section: The Equations Of Motionmentioning
confidence: 99%
“…We assume this special case because it gives us Einstein-Maxwell-Yang-Mills theory, and because it greatly simplifies the theory. With the assumption (44) we also havẽ R νµ = tr(R νµ )I/d, and the term ([A α ,Γ (18). It is important to emphasize that any solution of the restricted theory (44) will also be a solution of the more general theory.…”
Section: The Caseh νµ = 0 With Nonsymmetric Fieldsmentioning
confidence: 99%
“…The additional cosmological constant Λ z in our Lagrangian density (5,18) could have several contributions. If there was a contribution from zero-point fluctuations it would be approximately [14,15,16,17] …”
Section: The Caseh νµ = 0 With Nonsymmetric Fieldsmentioning
confidence: 99%
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