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Mikael17
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- time dilatation inside the sun
How can time dilation, lets say 500000 km inside the sun be calculated ?
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.
Gravitational time dilation is a phenomenon predicted by Einstein's theory of General Relativity, where time passes more slowly in stronger gravitational fields. This means that closer to a massive object, such as the Sun, time would pass more slowly compared to a region with weaker gravitational fields.
Gravitational time dilation inside the Sun is relatively small but measurable. Due to the Sun's mass, the time dilation effect at its core is more pronounced than at its surface. However, the difference is not extremely large because the Sun's gravitational field, while strong, is not as intense as that of more massive objects like black holes.
Gravitational time dilation can be calculated using the formula derived from General Relativity: \( t_0 = t_f \sqrt{1 - \frac{2GM}{rc^2}} \), where \( t_0 \) is the time experienced at a distance \( r \) from the center of the Sun, \( t_f \) is the time experienced far away from the Sun, \( G \) is the gravitational constant, \( M \) is the mass of the Sun, and \( c \) is the speed of light. The closer you are to the Sun's core, the more pronounced the effect.
Gravitational time dilation does affect the rate at which time passes for nuclear reactions in the Sun's core, but the effect is extremely small. The nuclear reactions proceed at nearly the same rate as they would if there were no time dilation, because the difference in time passage is minimal compared to the overall timescale of these reactions.
The effects of gravitational time dilation inside the Sun are too small to be directly observed from Earth with current technology. However, time dilation effects can be observed in other astrophysical contexts, such as near black holes or neutron stars, where the gravitational fields are much stronger and the effects are more pronounced.