sweet springs said:
In other words in y-moving FR against Rindler FR , direction of gravity acceleration does not coincide with x' axis and horizontal direction if it means orthogonal to gravity acceleration does not coincide with y' axis.
I just did a quick calculation to confirm my recollection this is not true. The acceleration 4-vector is given by
$$a^b = u^a \nabla_a u^b$$
It turns out that this vector points in the same direction for both a point at rest on the elevator floor, and a point sliding along the floor.
The most notable physical effect in what passes for the frame of reference for the sliding block is not a change in the direction of gravity, but rather Thomas precession. This is not a change in "gravity", it's more subtle. It means that a gyroscope that initially points "up", towards some distant fixed star, will not continue to point "up" if it is mounted on a sliding block. This is in contrast to the gyroscope mounted on the floor of the elevator, which will not precess and will continue to point towards the distant fixed star.
For a paper which describes the effect above, see
https://arxiv.org/abs/0708.2490v1, which takes a non-tensor approach, though it's still not terribly easy to follow. I believe I've mentioned that paper previously.
The Thomas precession may not seem like something that one is necessarily interested in, but it's not really possible to fully understand the sliding block frame without understanding this property it has. See more below.
The approach I suggest to understanding what we might mean by "the frame of a sliding block" in the spirit of General Relativity is to write a metric. This spawned a very long thread, which I think you're aware of, where we explored just what metric would be associated with a sliding block. In the end, we came up with several different candidates for what one might mean by "a frame of a sliding block". The particular chocie I espoused was "the proper reference frame" of the sliding block, but there are other candidates that also have their merits. I won't rehash that here without some guidance, the thread was about 11 pages long.
It is only necessary to define a metric if one wants to understand what I call an "extended" frame of reference. In a purely local sense, one can define a frame of reference as a set of four vectors. However, this defintion of a "frame of reference" is only at a point, it does not encompass any experiment that has a non-zero volume. The problem of dropping a ball is an example of a problem that requires a frame of reference that encompasses a non-zero volume and not just a poit. So if we wanted to drop a ball in the sliding block frame, we'd need a metric.
The gyroscope precession is relevant to the path a ball dropped on the sliding block would take, because there will be generalized forces on the sliding block, "fictitious forces", if you will, that are essentially coriolis forces. These fictitious forces cause the gyroscope to precess, and they'd deflect the path of any falling body in the sliding block frame.
Defining a metric allows pretty much anything that GR can calculate to be calculated. Also, any complete description of a set of coordinates must allow one to compute the metric (otherwise it's not a complete description). So defining a metric is both necessary and sufficient in the context of GR to define a set of coordinates. There's a paper by Misner that mentions this, that I can quote. Outside the context of GR, mathematicans may demand more than this, but for instance the IAU defines the set of coordinates used to describe the ICRF, the International Celstial Reference Frame, by writing down it's metric.
From the GR point of view, the space-time itself is flat in the Minkowskii frame, the Rindler frame, and whatever frame one decides to use to represent the sliding block. To be more specific, the Riemann curvature tensor vanishes, and a tensor is a coordinate independent entity, so that if it vanishes in one coordinate system it vanishes in all coordinate systems.
Basically, the different "frames" are just different coordinate choices. It's perfectly possible and possibly much easier to use the Minkowskii frame to do all the calculations, then convert it to the frame of choice.
"The frame of choice" must be sufficiently well defined to allow one to translate the results from the Minkowskii frame to the new frame, however. One way of doing this is to define a map (called a diffeomorphism) that associates points between the Minkowskii frame and whatever frame one chooses to use. But this is not necessary, the "frame" can be defined by it's metric without any reference at all to Minkoskii space.
The machinery of GR is sufficiently powerful for one to do the computations in any frame one desires. It may be easier to do all the calculations in the Minkowskii frame and convert back to the new frame, but one can also do the calculations in an arbitrary frame of reference. The procedure for doing so starts write down the metric associated with the new frame. The metric defines the coordinates that one has chosen, and also allows one to use tensor methods (such as the geodesic equations) to compute quantites of physical interest in a manner that's native to that frame.