The heat equations or dQ equations (not to be confused with the heat partial differential equation) are a set of equations for the infinitesimal variation of heat dQ in a physical system. They are equations of two thermodynamic variable chosen among pressure P, volume V and temperature T, with the third constrained by the system's equation of state.
The equations are
dQ(P,V)dQ(P,T)dQ(V,T)=(∂P∂U)VdP+[(∂V∂U)P+P]dV=[(∂P∂U)T+P(∂P∂V)T]dP+(∂T∂H)PdT=[(∂V∂U)T+P]dV+(∂T∂U)VdT
where U is the internal energy of the system and H is enthalpy. The subscripts mean taking a derivative while holding that variable constant. These derivatives are coefficients that are measured experimentally. Specifically, we have
CV=(∂T∂U)VCP=(∂T∂H)P
as the heat capacity for constant-volume and isobaric transformations.
Derivation#
The heat equations are directly derived from the first law of thermodynamics. The internal energy must be
dU=dQ−dW=dQ−PdV
with dQ heat and dW=PdV work. The equation of state allows us to lock one the three variables P, V or T down, giving us three ways to express dU
dU(P,V)dU(P,T)dU(V,T)=(∂P∂U)VdP+(∂V∂U)PdV=(∂P∂U)TdP+(∂T∂U)PdT=(∂V∂U)TdV+(∂T∂U)VdT
for all permutations of the variables. Combining these with the first law dQ=dU+PdV gives us
dQ(P,V)dQ(P,T)dQ(V,T)=(∂P∂U)VdP+[(∂V∂U)P+P]dV=(∂P∂U)TdP+(∂T∂U)PdT+PdV=[(∂V∂U)T+P]dV+(∂T∂U)VdT
The first and third equations are done, but the second equation can't be used as is, because dV is still leftover from the work. We can get rid of it by expressing V in function of the other two:
dV=(∂P∂V)TdP+(∂T∂V)PdT
and so
dQ(P,T)=[(∂P∂U)T+P(∂P∂V)T]dP+(∂T∂(U+PV))PdT
For convenience, we can use the enthalpy H=U+PV to simplify things:
dQ(P,T)=[(∂P∂U)T+P(∂P∂V)T]dP+(∂T∂H)PdT