An Interesting answer at Quora....
https://www.quora.com/Is-a-curve-in...~ 186 GeV/cm^,constant speed of light locally.
Jim Whitescarver, learned relativity on my dad's knee 60+ years ago.
Answered March 5, 2016
The energy density of spacetime, ~ 186 GeV/cm^3, is always measured to be the same locally. It is as Wheeler remarked, only marginally less that matter. This constant density results in the constant speed of light locally.
However this density is relatively different depending on the local curvature of spacetime due to gravity. This diagram supplied by Prakyat Prasad shows it well.
Spacetime is curved into a timelike dimension near a large mass. No mater where you are light always takes one nanosecond to pass your ruler. However, if you are near a large mass a distant observer with measure the time to be longer than a nanosecond and say your time is relatively slower. We can equivalently say your light is relatively slower. Propagation speed is related to mass density of the medium so we can say that effective energy density is greater.
Given relatively "slower light", it would exhibit a slower than light rest frame relatively, this increased relative density of spacetime can account for dark matter near galactic centers, and relatively faster light in relatively less dense deep space can account for dark energy.
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https://www.quora.com/Is-a-curve-in...~ 186 GeV/cm^,constant speed of light locally.
Jim Whitescarver, learned relativity on my dad's knee 60+ years ago.
Answered March 5, 2016
The energy density of spacetime, ~ 186 GeV/cm^3, is always measured to be the same locally. It is as Wheeler remarked, only marginally less that matter. This constant density results in the constant speed of light locally.
However this density is relatively different depending on the local curvature of spacetime due to gravity. This diagram supplied by Prakyat Prasad shows it well.
Spacetime is curved into a timelike dimension near a large mass. No mater where you are light always takes one nanosecond to pass your ruler. However, if you are near a large mass a distant observer with measure the time to be longer than a nanosecond and say your time is relatively slower. We can equivalently say your light is relatively slower. Propagation speed is related to mass density of the medium so we can say that effective energy density is greater.
Given relatively "slower light", it would exhibit a slower than light rest frame relatively, this increased relative density of spacetime can account for dark matter near galactic centers, and relatively faster light in relatively less dense deep space can account for dark energy.
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