jeremyfiennes said:
For a photon passing close to the Sun, Newtonian physics predicts a deflection of 0.85o. GR gives the correct 1.7o. Can the true value alternatively be obtained via 1) a Newtonian model, and 2) gravitational time dilation: the photon's slower speed near the Sun leads to it spending more time in its gravitational field, and hence a higher deflection?
The correct deflection value can be obtained by the PPN approximation, which is a weak-field approximation to General relativity. In this PPN formulation, there is exactly one parameter that controls the amount of the 'extra' deflection of the photon, this parameter is usually caled ##\gamma##.
See for instance the wiki article on PPN,
<<here>>.
The description of the PPN parameter ##\gamma## has nothing direclty due to gravitational time dilation, but is described in the wiki article (and in textbooks) as
##\gamma## : How much space curvature ##g_{ij}## is produced by unit rest mass ?
The GR prediction has ##\gamma=1##. Setting ##\gamma=0## cuts the deflection in half. Unfortunately, it's not quite correct to say that the Newtonaion prediction corresonds to setting ##\gamma=0##.
It's clear, historically, that the "extra" deflection of light was considered to be a good test of General Relativity. WIki
<<link>> has the following to say about it, but I haven't read the citied references.
Henry Cavendish in 1784 (in an unpublished manuscript) and
Johann Georg von Soldner in 1801 (published in 1804) had pointed out that Newtonian gravity predicts that starlight will bend around a massive object.
[15][16] The same value as Soldner's was calculated by Einstein in 1911 based on the equivalence principle alone. However, Einstein noted in 1915 in the process of completing general relativity, that his (and thus Soldner's) 1911 result is only half of the correct value. Einstein became the first to calculate the correct value for light bending.
[17]
There are some other methods for getting the correct prediction of light for the deflection of light, such as using an action principle. But I don't think there's anything that's exactly what you describe in 2).