Table of Contents
First law of thermodynamics
The first law of thermodynamics states that:
The algebraic sum of net heat and work interactions between a system and its surrounding in a thermodynamic cycle is zero
Mathematically
For a cyclic process
ΣQ = ΣW
Where:
Q = Heat interaction
W = Work interaction
For a finite non-cyclic process
Q1-2 = W1-2 + ΔE
Where:
E = Internal energy
In general
E = U + KE + PE + any other kind of stored energy
Where:
U = Intermolecular energy
KE = Kinetic energy
PE = Potential energy
For a closed system in equilibrium KE, PE and other kinds of stored energy are zero.
Which means
E = U
Hence for a finite non-cyclic process first law of thermodynamics becomes
Q1-2 = W1-2 + ΔU
If we consider only P*ΔV work, above equation becomes
Q1-2 = P*ΔV + ΔU
Note: Conventionally work done by the system and the heat given to the system are always taken positive.
Internal energy
A property of a system whose change in a process executed by the system equal to the difference between the heat and work interactions by the system with its surrounding.
Enthalpy
Enthalpy is a thermodynamic quantity which is equal to total heat content in a system.
Mathematically
H = U + PV
According to the first law of the thermodynamics
Q1-2 = P*ΔV + ΔU
Q1-2 = P(V2-V1) + U2 – U1
Rearranging the above equation
Q1-2 = U2 + P2V2 – (U1 + P1V1)
From the equation of enthalpy, it implies
Q1-2 = H2 – H1
Specific heat
Specific heat is the quantity of heat which is required to raise the temperature of unit mass by one degree Celsius.
There are two types of specific heat
-
Specific heat at constant volume
Cv = ( ∂u/ ∂T)v=constant
-
Specific heat at constant pressure
Cp = ( ∂h/ ∂T)p=constant
First law applied to the open system (or control volume)
Unlike a closed system mass flows in and out of an open system. Here we have to take conservation of mass into account.
Conservation of mass
(dm1/dt) – (dm2/dt) = dmcv/dt
Where
dm1/dt = Rate of mass entering to the system
dm2/dt = Rate of mass leaving from the system
dmcv/dt = Rate of mass stored in the system
Conservation of energy
e = u + p*v + g*z + (V2/2)
Where
e = stored energy in the stream of fluid
u = internal energy stored in the stream of fluid
V2/2 = kinetic energy of the stream of fluid
g*z = potential energy stored in the stream of fluid
p*v = pressure work
Mathematical expression of first law for open system
(dm1/dt)*e1 + (∂Q/∂t) – (dm2/dt)*e2 – (∂W/∂t) = dEcv/dt
At steady state
m1 = m2 = m
dEcv/dt = 0
Hence the equation becomes
(dm/dt)*e1 + (∂Q/∂t) – (dm/dt)*e2 – (∂W/∂t) = 0
Above equation is also known as steady flow energy equation.
Also read:
What is a thermodynamic state?
Macroscopic approach to study thermodynamics