which, breaking H into its energy eigenstates gives
|ψ(t)⟩=∑pneiEnt|ψEn⟩.
In Minkowski space, the time t is literally imaginary. What if we rotated it 90∘ in the complex plane so that it’s just like the other dimensions? This is called the Wick rotation, it=−β, and we recover the Boltzmann (Gibbs) distribution
|ψ(t)⟩=∑ane−βEn|ψEn⟩
or equivalently
Pr[ψ(t)=ψEn]∝e−βEn.
β takes on the role of inverse-temperature. Now, what is the entropy-maximizing distribution? Let
pn=Pr[ψ(t)=ψEn].
We want
maxentropy=−∑pnlnpn,s.t.∑pnEn=constant.
Lagrange multipliers give
lnpn=βEn+constant
or the same Boltzmann (Gibbs) distribution we saw earlier. So basically, if we switch to a coordinate axis where time is identical to the other distributions, we find that evolution through time is equivalent to a maximum-entopy distribution in this other coordinate axis.
Now, this is almost circular reasoning, because why is Schroedinger’s equation the way it is? Basically, if you have some observer t (careful here! we’re reusing variable names with different meanings!), and you have some object ψ, and you say that ψ looks the same to the observer as the observer changes, that’s written mathematically as
∂ψ∂t=Aψ
where A is some matrix/linear transformation. So
ψ(t)=eAtψ(0)=escalingZt+rotationiHtψ(0).
After a long enough time, we’re really only looking at rotation. So, why is our “observer” the same as the time dimension? Well, it’s not. But imagine it’s moves mostly in that dimension, maybe around 299,792,458 times faster, with a little mixing in of the other three. Then the mixing in of the other three will make it so the entropy-maximizing distribution we see in 4 space dimensions should also be entropy-maximizing if we Wick rotate any one of those dimensions.
I think it’s because Schroedinger’s equation is
ψ(t)⟩=eiHtψ(0)⟩
which, breaking H into its energy eigenstates gives
|ψ(t)⟩=∑pneiEnt|ψEn⟩.
In Minkowski space, the time t is literally imaginary. What if we rotated it 90∘ in the complex plane so that it’s just like the other dimensions? This is called the Wick rotation, it=−β, and we recover the Boltzmann (Gibbs) distribution
|ψ(t)⟩=∑ane−βEn|ψEn⟩
or equivalently
Pr[ψ(t)=ψEn]∝e−βEn.
β takes on the role of inverse-temperature. Now, what is the entropy-maximizing distribution? Let
pn=Pr[ψ(t)=ψEn].
We want
maxentropy=−∑pnlnpn,s.t.∑pnEn=constant.
Lagrange multipliers give
lnpn=βEn+constant
or the same Boltzmann (Gibbs) distribution we saw earlier. So basically, if we switch to a coordinate axis where time is identical to the other distributions, we find that evolution through time is equivalent to a maximum-entopy distribution in this other coordinate axis.
Now, this is almost circular reasoning, because why is Schroedinger’s equation the way it is? Basically, if you have some observer t (careful here! we’re reusing variable names with different meanings!), and you have some object ψ, and you say that ψ looks the same to the observer as the observer changes, that’s written mathematically as
∂ψ∂t=Aψ
where A is some matrix/linear transformation. So
ψ(t)=eAtψ(0)=escalingZt+rotationiHtψ(0).
After a long enough time, we’re really only looking at rotation. So, why is our “observer” the same as the time dimension? Well, it’s not. But imagine it’s moves mostly in that dimension, maybe around 299,792,458 times faster, with a little mixing in of the other three. Then the mixing in of the other three will make it so the entropy-maximizing distribution we see in 4 space dimensions should also be entropy-maximizing if we Wick rotate any one of those dimensions.