“…) 00 for a test mass m T . Due to a change of the a w 0 sign for antimatter, free-fall LIV could still be large for antimatter while strongly constrained for normal matter, 5 as can be measured, e.g., in GBAR in the future (free fall of antihydrogen). 1 Deriving the equations of motion from the lagrangian by the Euler-Lagrange equations and expressing frame dependence with respect to a common inertial frame (the Sun-centered celestial equatorial frame) leads to the full LIV time variation model, which we can use to model the observables of gravimeters and WEP tests.…”