Gravitational Time Dilation in L1 Point: Summed, Canceled or Else?

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SUMMARY

Gravitational time dilation at the Lagrangian (L1) point between two massive objects is primarily additive, as confirmed by Perok. While the L1 point serves as an approximation in General Relativity (GR), it is exact in Newtonian physics. The discussion highlights that gravitational radiation effects, such as inspiral, can be negligible in certain scenarios like the solar system but may not be in cases like the Hulse-Taylor binary. Thus, the gravitational time dilation effects at L1 can be considered to sum under specific conditions.

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Chris Miller
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TL;DR
Gravitational time dilation at Lagrangian points
In the Lagrangian (L1) point between two hypothetically massive (and close) objects , is gravitational time dilation effect summed or canceled, or something else?
 
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Chris Miller said:
Summary:: Gravitational time dilation at Lagrangian points

In the Lagrangian (L1) point between two hypothetically massive (and close) objects , is gravitational time dilation effect summed or canceled, or something else?

It's an approximation, but it more or less adds, as Perok says.

The L1 point itself is an approximation in GR (though it's exact in Newtonian theory). The Newtonian analysis doesn't take into account, for example, the gravitational radiation that would make an orbiting body inspiral. Usually this is quite negligible, for instance it's negligible in the solar system. But it's not necessarily negligible for the Hulse-Taylor binary, for another example. If there is no inspiral, one can argue that the solution is stationary, and in that case Perok's source's arguments apply for the weak field case.
 
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