I am wondering whether discussions of inflationary cosmology in these forums generally includes or explicitly excludes prior Plank era and GUT era dynamics. I never gave it any thought until reading the following.

The Wikipedia article provides a perspective I just don't remember from other sources. If inflationary cosmology excludes Planck and GUT eras, are there some alternative pre inflationary dynamics we are supposed to associate with inflation?

In fact the ultimate theory of the Cosmology must consist Planck scale, but in inflationary models we "assume" that the energy scale of inflaton field is far lower than Planck energy scale since in Planck scale the Quantum gravity phenomenons become important which we do not know them well.About the GUT scale the point is that if inflation has occurred before GUT symmetry breaking, we encounter the problem of creation of monopoles , which inflationary scenario is invented to solve ! Symmetry breaking of GUT scale (10^-5 M_{planck}) produces so many monopoles , inflation destroys them by means of expanding the universe.

After doing some reading on the subject since I posted, I've become more certain of what I suspected...the above Wikipedia view is one author's view and I strongly suspect not widely shared.

For the record there is a lot of unknown or uncertain quantum activity within inflation itself, not just at Planck scale. That variety is reflected in at least 70 or more inflation models.

Here is one interesting comment from Alan Guth in Scientific American : [The interview may also be of interest to string theory enthusiasts.]

For polarization data release of Planck we have to wait about 6 months! I thinks the Alan Guth point of view is that if inflation paradigm is correct , its forecast about tensor perturbation should be consistent with the data as well as scalar perturbation. This can confirm the true energy scale choice of inflaton field( about GUT scale.) Almost all of the models predict small tensor perturbation power with respect to scalar power.

Indeed, we don't know what the energy scale of inflation was: in the absence of a primordial B-mode in the CMB, Planck is only able to place an upper bound on the energy scale, something like 10^16 GeV which is on or about GUT scale. So phenomenologically, inflation can occur at the GUT scale. However, it doesn't need to: it is possible to build inflation models that occur closer to the electroweak scale! This would imply either that, yes, there is some pre-inflationary standard cosmology that passes through the GUT scale, or that the universe simply never passed through a GUT era.

bapowell , I am not sure but doesn't too low energy scale of inflation contradicts with solving horizon problem or amplitude of the power spectrum on the CMB?

It has no direct bearing on the horizon problem, which depends on the amount of inflation which is determined by both how long it takes the inflaton to decay or roll to the true vacuum and the energy density. True, the rate of expansion is higher with greater energy density, so low-scale inflation just takes longer to solve the horizon problem.

As far as the amplitude of the scalar perturbations, this depends on the energy scale of inflation but also on the first derivative of the potential; so one can accommodate low-scale inflation by suitably adjusting the slope of the potential.

.In inflationary cosmology, times before the end of inflation (roughly 10−32 second after the Big Bang) follow not the traditional big bang timeline. The universe before the end of inflation is a very cold near-vacuum and persists for much longer than 10−32 second.

this line in the above post in the wiki article referenced above is also inaccurate prior to inflation the average temperatures is hotter prior to inflation not a very cold near vacuum