From: OsherD on
From Osher Doctorow

I should remind readers that the recent papers in this thread have
concerned HSP ("Human Scale/Scenario Physics") as a Unification theory
or alternative of Quantum Gravity.

As I have described in this thread, various Quantum approximations to
HSP exist, including the Nonlinear Schrodinger Equation and the Gross-
Pitaevski Equation (GPE) which apply to solitons, Bose-Einstein
Condensates (BECs), etc. When the spatial unmixed partial
derivatives such as Dxx, Dyy, Dzz are small, the Laplacian or DELTA^2
operator can be approximately ignored in these equations, and they
simplify into first partial derivative (including time) and related
equations (like characteristic equations or equations of
characteristics in PDEs) which are properly in HSP.

It is arguably not surprising that large "spatial accelerations" like
Dxx, Dyy, Dzz and large speeds/velocities relative to HSP and many
microscopic phenomena (which are extremely small compared to HSP)
introduce distortions which deviate from HSP. Recall from my recent
postings here that, arguably, whatever the scale of the Observer (in
this case the Human Observer), the physics will look like HSP at that
scale and the other scales asymptotically or "near-asymptotically"
will be distorted. So if a galaxy-scale Observer or a Quantum scale
observer exists, that observer would obtain HSP or an analog or almost-
analog of it for his local or near-local region, with the other scales
being distorted.

Osher Doctorow
From: OsherD on
From Osher Doctorow

For time-acceleration, however, that is for the operator Dtt (2nd
derivative or partial derivative with respect to time), HSP still
applies, because Probable Causation/Influence (PI), the key to HSP,
involves Causation as basically a time quantity. So the acceleration
eras of the Universe are well handled by PI and HSP.

Osher Doctorow