Einstein's "special" or "restricted" theory of relativity was published in 1905, and can be considered a distillate of the equations are relationships of Lorentz Aether Theory ("LET", 1904). Lorentz aether theory was developed through the late 1800s, and was likely the most popular aether model in Germany when Einstein was a student ... his lecturer Minkowski would probably have impressed on Einstein the notion that these relationships had to be correct.
In 1909, Minkowski published his rendition of the Lorentz-Einstein equations as a pure spacetime geometry.
relativity + flat spacetime = special relativity
relativity + bodies with no gravitational fields = special relativity
relativity + time-symmetry = special relativity
However, if the existence of matter is associated with curvature, or if physics looks different in forward and reversed time, special relativity is ruled out.
All solutions to the relativity of inertial motion are related by Lorentzlike factors, and of these solutions, only special relativity looks the same in forward and reversed time. [] All other solutions are asymmetrical with respect to time: Newtonian theory gives E'/E = (c-v)/c for recession in forward time, and E'/E = c/(c+v) in reversed time. If, like Einstein, we find time-asymmetry abhorrent, we can average out these two predictions to give their geoemetric mean, sqrt[ (c-v) / (c+v) ], and this is then special relativity.
Special relativity therefore has the special status of being the time-average of Newtonian thery, and in fact, of all possible relativistic theories. It is the averaged, homogenised version of the real equations of motion.