I Gravity of the Sun: Einstein's Calculation and Beyond

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Einstein's calculation of the Sun's gravity indicates a focus point around 542 AU. This value applies to rays grazing the Sun, including neutrinos and gravitational waves, but their behavior may differ due to various factors. Gravitational lenses are not precise, and the focal distance can vary based on the ray's distance from the Sun's center. Neutrinos are likely to penetrate deeper into the Sun than light, while gravitational waves can pass through without obstruction. Current limitations in neutrino and gravitational wave astronomy prevent practical testing of these theoretical concepts.
Nik_2213
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IIRC, the Sun's gravity was calculated by Einstein et-al to provide a 'focus' about 550 AU out. Current value is ~542 AU.
Aside from effects due solar oblateness, frame dragging etc, may I assume this value also applies to eg neutrinos, gravitational waves etc etc ??
 
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Yes and no.

The calculation is for rays grazing the Sun, and I would expect that neutrinos and gravitational waves grazing the same surface would focus at the same distance, give or take a small bit. But gravitational lenses are terrible lenses, and the focal distance depends very much on the distance of the ray from the Sun center at perihelion. And I suspect the Sun is transparent to neutrinos for some depth below where it becomes opaque to light. And it's transparent to gravitational waves right through. So you may well be able to find focuses for them closer to the Sun.

Note that we don't have good enough neutrino or gravitational wave astronomy instruments to test anything like gravitational lensing of these things, so this is purely theoretical at this stage. We've no reason to doubt it works, but it hasn't been tested.
 
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Moderator's note: Spin-off from another thread due to topic change. In the second link referenced, there is a claim about a physical interpretation of frame field. Consider a family of observers whose worldlines fill a region of spacetime. Each of them carries a clock and a set of mutually orthogonal rulers. Each observer points in the (timelike) direction defined by its worldline's tangent at any given event along it. What about the rulers each of them carries ? My interpretation: each...

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