In physics, geometrothermodynamics (GTD) is a formalism developed in 2007 by Hernando Quevedo to describe the properties of thermodynamic systems in terms of concepts of differential geometry.[1]
Consider a thermodynamic system in the framework of classical equilibrium thermodynamics. The states of thermodynamic equilibrium are considered as points of an abstract equilibrium space in which a Riemannian metric can be introduced in several ways. In particular, one can introduce Hessian metrics like the Fisher information metric, the Weinhold metric, the Ruppeiner metric and others, whose components are calculated as the Hessian of a particular thermodynamic potential.
Another possibility is to introduce metrics which are independent of the thermodynamic potential, a property which is shared by all thermodynamic systems in classical thermodynamics.[2] Since a change of thermodynamic potential is equivalent to a Legendre transformation, and Legendre transformations do not act in the equilibrium space, it is necessary to introduce an auxiliary space to correctly handle the Legendre transformations. This is the so-called thermodynamic phase space. If the phase space is equipped with a Legendre invariant Riemannian metric, a smooth map can be introduced that induces a thermodynamic metric in the equilibrium manifold. The thermodynamic metric can then be used with different thermodynamic potentials without changing the geometric properties of the equilibrium manifold. One expects the geometric properties of the equilibrium manifold to be related to the macroscopic physical properties.
The details of this relation can be summarized in three main points:
The main ingredient of GTD is a (2n + 1)-dimensional manifold
l{T}
ZA=\{\Phi,Ea,Ia\}
\Phi
Ea
a=1,2,\ldots,n
Ia
\Theta=d\Phi-\deltaabIadEb
\deltaab={\rm diag}(+1,\ldots,+1)
\Theta\wedge (d\Theta)n ≠ 0
n
\{ZA\}\longrightarrow\{\widetilde{Z}A\}=\{\tilde\Phi,\tildeEa,\tildeIa\} , \Phi=\tilde\Phi-\deltakl\tildeEk\tildeIl, Ei=-\tildeIi, Ej=\tildeEj, Ii=\tildeEi, Ij=\tildeIj ,
where
i\cupj
\{1,\ldots,n\}
k,l=1,\ldots,i
i=\{1,\ldots,n\}
i=\emptyset
l{T}
G
(l{T},\Theta,G)
l{E}\subsetl{T}
\varphi:l{E} → l{T}
\varphi:\{Ea\}\mapsto\{\Phi,Ea,Ia\}
\Phi=\Phi(Ea)
Ia=Ia(Ea)
\varphi*(\Theta)=\varphi*(d\Phi -\deltaabIadEb)=0
\varphi*
\varphi
l{E}
g=\varphi*(G)
l{E}
\Phi=\Phi(Ea)
GI=(d\Phi-\deltaabIadEb)2+Λ(\xiabEaIb)\left(\deltacddEcd
d\right) , \delta | |
I | |
ab |
={\rmdiag}(1,\ldots,1)
GII=(d\Phi-\deltaabIadEb)2+Λ(\xiabEaIb)\left(ηcddEcd
d\right) , η | |
I | |
ab |
={\rmdiag}(-1,1,\ldots,1)
where
\xiab
\deltaab
ηab
Λ
ZA
GI
GII
GIII=(d\Phi-\deltaabIadEb)2+Λ(Ea
2k+1 | |
I | |
a) |
\left(dEadIa\right) , Ea=\deltaabEb , Ia=\deltaabIb .
The components of the corresponding metric for the equilibrium manifold
{lE}
gab=
\partialZA | |
\partialEa |
\partialZB | |
\partialEb |
GAB .
GTD has been applied to describe laboratory systems like the ideal gas, van der Waals gas, the Ising model, etc., more exotic systems like black holes in different gravity theories,[4] in the context of relativistic cosmology,[5] and to describe chemical reactions.[6]