Mikael17
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- TL;DR
- time dilatation inside the sun
How can time dilation, lets say 500000 km inside the sun be calculated ?
The discussion focuses on calculating gravitational time dilation 500,000 km inside the Sun using the interior Schwarzschild metric. Participants emphasize the need for a density and pressure profile for more accurate results, suggesting that numerical methods are required for precise calculations. The weak field approximation is highlighted as a more accurate approach compared to the interior Schwarzschild metric, particularly when applying a standard solar model for the density profile.
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To do much better you'd need a density and pressure profile, and I would suspect you'd have to do it numerically. Especially if you stopped pretending it was a non-rotating sphere.Dale said:One of the assumptions is constant density, so that probably isn’t the best assumption, but it should be a reasonable approximation given the resulting simplification
Yes. I agree that anything more exact than this would probably have to be numerical.Ibix said:To do much better you'd need a density and pressure profile, and I would suspect you'd have to do it numerically. Especially if you stopped pretending it was a non-rotating sphere.
Here:Ibix said:Is ##n## (23.28c and d) defined somewhere? Number density of particles?
Ibix said:To do much better you'd need a density and pressure profile, and I would suspect you'd have to do it numerically. Especially if you stopped pretending it was a non-rotating sphere.
Dale said:This would be the interior Schwarzschild metric:
https://en.m.wikipedia.org/wiki/Interior_Schwarzschild_metric
One of the assumptions is constant density, so that probably isn’t the best assumption, but it should be a reasonable approximation given the resulting simplification
The weak field approximation is going to be way more accurate than the interior Schwarzschild metric in this case. Input a solar model for the density and voila.Dale said:Yes. I agree that anything more exact than this would probably have to be numerical.
I have to admit that it didn’t even occur to me!Orodruin said:The weak field approximation is going to be way more accurate than the interior Schwarzschild metric in this case. Input a solar model for the density and voila.