T(x)=A√x=A(x)−12
A is a constant of proportionality. Differentiating with respect to x,
T′(x)=−A2(x)−32
T″(x)=3A4(x)−52
and from the post "What Thermal Gravity? Too Hot To Handle..."
gT=v2xT(x)d2T(x)dx2
gT=v2x(x)12A3A4(x)−52
gT=34xv2=ax=STT2
where v is the speed of T as it travels across the temperature profile, a a constant, and ST a constant of proportionality with the unit ms-2J-2. The last equation relates gT directly to T this will bring us to a relationship for space density and temperature in another post.
Unfortunately, a plot of a family of curves of ax together with 1x2,
shows that gT=a/x does not intersect g=1/x2 again after its goes above 1/x2 ie after gT>g along x. gT has to be greater than g at the start x=xo for T to flow. This is the case for nebula where the boundary, gT−g=0 does not exist, but not a general case of planetary spheres and rings where gT>g for T to flow outwards and then gT−g=0 at some distance xring beyond which gT oscillate up and down g. It is not appropriate to repesent gravity of the hot spot here using 1/x2.
However, if instead we use e−x to represent gravity,
Both Nebula and planetary spheres and rings scenarios are encountered as 1/x is scaled appropriately. The curve marked as a/x is higher than the gravity curve g and does not intersect g. This is the Nebula scenario where T spreads over vast distances.
All other curves below a/x cross g twice. The second intersection further out along x marks a gap where the net gravity due to g and gT points away from it, before and after that point.
It should be noted that, beyond the first intersection, T redistributes and gT is no longer of the form a/x but is expected to have a sinusoidal component and intersect g again multiple times.
Below is a plot of (1/x)*cos(2*x)^2/(cos(2)^2) to show how gT might look like,
If T(x) can be determined from observations, then logically gT should come after T(x) has been formulated. We shall do that in the next post.
gT was derived from an expression for T temperature, based on an moving mass analogy for T, together with the assumption that T propagates as a wave, at a constant velocity v. If T(x) can be obtained empirically, then gT can be derived directly with just one assumption of how T affects gT through interacting with space.