VARIATION OF VACUUM ENERGY IF SCALE FACTOR BECOMES INFINITELY SMALL, WITH FIXED ENTROPY DUE TO A NON PATHOLOGICAL BIG BANG SINGULARITY ACCESSIBLE TO MODIFIED EINSTEIN EQUATIONS

When initial radius 0initialR → if Stoica actually derived Einstein equations in a formalism which remove the big bang singularity pathology, then the reason for Planck length no longer holds. The implications of 0initialR → are the first part of this manuscript. Then the resolution is alluded to by work from Muller and Lousto, as to implications of entanglement entropy. We present entanglement entropy in the early universe with a steadily shrinking scale factor, due to work from Muller and Lousto, and show that there are consequences due to initial entanged 2 2.3Entropy HS r a = for a time dependent horizon radius Hr in cosmology, with for flat space conditions Hr η = for conformal time In the case of a curved, but not flat space version of entropy, we look at vacuum energy as proportional to the inverse of scale factor squared times the inverse of initial entropy, effectively when there is no initial time in line with 2 1 ~ /H G H aρ − ⇔ ≈. The consequences for this initial entropy being entangled are elaborated in this manuscript. No matter how small the length gets, entropyS if it is entanglement entropy, will not go to zero. The requirement is that the smallest length of time, t, re scaled does not go to zero. Even if the length goes to zero. This preserves a minimum non zero Λ vacuum energy, and in doing so keep the bits, for computational bits cosmological evolution even if 0initialR