  Many physical theories beyond the Standard Model predict time variations of
basic physics parameters. Direct measurement of the time variations of these
parameters is very difficult or impossible to achieve. By contrast,
measurements of fundamental constants are relatively easy to achieve, both in
the laboratory and by astronomical spectra of atoms and molecules in the early
universe. In this work measurements of the proton to electron mass ratio $\mu$
and the fine structure constant $\alpha$ are combined to place mildly model
dependent limits on the fractional variation of the Quantum Chromodynamic Scale
and the sum of the fractional variations of the Higgs Vacuum Expectation Value
and the Yukawa couplings on time scales of more than half the age of the
universe. The addition of another model parameter allows the fractional
variation of the Higgs VEV and the Yukawa couplings to be computed separately.
Limits on their variation are found at the level of less than $5 \times
10^{-5}$ over the past seven gigayears. A model dependent relation between the
expected fractional variation of $\alpha$ relative to $\mu$ tightens the limits
to $10^{-7}$ over the same time span. Limits on the present day rate of change
of the constants and parameters are then calculated using slow roll
quintessence. A primary result of this work is that studies of the
dimensionless fundamental constants such as $\alpha$ and $\mu$, whose values
depend on the values of the physics parameters, are excellent monitors of the
limits on the time variation of these parameters.
