Bernoulli’s Theorem is one of the most important theorems that provides the relation between velocity, pressure and viscosity. It was first derived by the Swiss Mathematician Daniel Bernoulli. Although the law was deduced by Bernoulli, the equation in its used form was derived by Leonhard Eurel in 1752.
According to Bernoulli’s principle, the total energy at any point in the subsurface per unit mass of a flowing fluid remains constant and is equal to the sum of the potential, kinetic and pressure head of the fluid. In simpler terms it is the energy conservation principle for ideal fluids in steady state or streamline motion and forms the basis of a lot of hydraulic applications. We will look at the different forms of energy associated with fluids:
P+1/2ρv2+ρgh=constant
P= The absolute pressure
V= Velocity of the fluid
h = Height above the reference point for the calculation of the potential energy
g = Acceleration due to gravity
If we follow a small volume of fluid along its path, the individual values of the energies change but the overall sum remains constant.
P1+1/2ρv12+ρgh1=P2+1/2ρv22+ρgh2
Bernoulli’s equation is a form of the energy conservation principle. If we carefully notice, the second and third terms are similar to the kinetic and potential energy formula where the mass ‘m’ is replaced by density ‘ρ’. Density is mass/volume and we can replace the kinetic energy term in the above equation, we get:
1/2ρv2=1/2mv2/V = KE/V
So 1/2ρv2 is the kinetic energy per unit volume. Making the same substitution into the third term in the equation, we find
ρgh=mgh/V=PEg/V
so ρgh is the gravitational potential energy per unit volume. Note that pressure P has units of energy per unit volume, too. Since P = F/A, its units are N/m2. If we multiply these by m/m, we obtain N ⋅ m/m3 = J/m3, or energy per unit volume. Bernoulli’s equation is, in fact, just a convenient statement of conservation of energy for an incompressible fluid in the absence of friction.
According to the principle of continuity, the overall mass remains constant when an incompressible fluid that is in streamline motion passes through different cross-sections.
By the energy conservation principle of incompressible fluids:
The rate of Mass entering the cross-section = the rate of mass leaving the cross-section
The rate of mass entering = ρA1V1Δt—– (1)
The rate of mass leaving = ρA2V2Δt—– (2)
Using the above equations,
ρA1V1=ρA2V2
This equation is known as the principle of continuity.