Saturday, February 13, 2016

general relativity - Transforming an equation to the co-vector version


Ok, this question is more a result of my lack of knowledge of how to manipulate equations involving index notation rather than about physics...


I have the geodesic equation with Uλ˙xλ:-


˙Uλ+ΓλμνUμUν


And I want to transform to the co-vector Uμ=gμλUλ.


Can I simply multiply each vector by gμν? Like so:-


gμλ˙Uλ+ΓλμνgμαUαgνβUβ


Or do I need to use gσνgνμ=δσμ to rewrite Uμ=gμλUλ and then sub it in?



Edit: Here's my attempt at the sub in method


So using gλμgμλ=δλλ to rewrite Uμ=gμλUλ as Uλ=gλμUμ. (Is this even correct?). Then differentiate:- ˙Uλ=˙gλμUμ+gλμ˙Uμ

Can I assume that the differential of the metric wrt time is going to be zero? Obivously this is not going to be true in general since massive bodies move! But generally in simple problems would this be taken as true?




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