From the post "Stress When The Heat Is On, Thermal Stress",
∂(ds)∂x=∂(ds)∂T.dT(x)dx+∂∂T{∂(ds)∂x}.T
{1−T.∂∂T}∂(ds)∂x=∂(ds)∂T.dT(x)dx
∂(ds)∂x={1−T.∂∂T}−1{∂(ds)∂T.dT(x)dx}
where
{1−T.∂∂T}−1 is the inverse of the operator {1−T.∂∂T}
This turns out to be very difficult.
But consider this,
∂∂ln(T)≡∂T∂ln(T)∂∂T≡T∂∂T
So,
{1−∂∂ln(T)}∂(ds)∂x=∂(ds)∂T.dT(x)dx
{1−∂∂ln(T)}∂(ds)∂x=∂(ds)∂x∂x∂T.dT(x)dTdTdx
that is to say,
{1−∂∂ln(T)}∂(ds)∂x=∂(ds)∂x.dT(x)dT
{1−∂∂ln(T)}∂(ds)∂x=∂(ds)∂x
which suggests (just mathematical trickery),
∂∂ln(T){∂(ds)∂x}=0
that ∂(ds)∂x is independent of ln(T) or
∂∂x{∂(ds)∂ln(T)}=0
that ∂(ds)∂ln(T) is independent of x
One way this could happen is that ds is a linear combination of functions in x and ln(T). This is to say,
ds=A.f(x)+B.h(ln(T))
where A and B are constants and f(x) is a function only of x and h(ln(T)) is a function only of ln(T).
That space density ds is the superposition of space distribution itself, expressed as A.f(x), and the effect of thermal energy in the form of B.h(ln(T)).
In the case of uniformly distributed space,
f(x)=C where C is a constant
ds=dn+B.h(ln(T))
where A.C=dn is the normal space density and,
h(ln(T))|limT→0=0
such that when T=0, ds=dn
The points here are the ln(T) dependence of ds and superposition ds=A.f(x)+B.h(ln(T)).