Helmholtz Equation: Derivation, Thermodynamics, Applications

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Helmholtz Equation is the linear partial differential equation that is named after Hermann von Helmholtz. In this equation, we deal with three functions mainly- Laplacian, Wavenumber, and Amplitude. The Helmholtz equation is the eigenvalue equation that is solved by separating variables only in coordinate systems.

Key Terms- Helmholtz Equation, differential equation, Laplacian, Amplitude, Wave equation, Thermodynamics


What is Helmholtz Equation

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Helmholtz equation is a Physics and Mathematics equation named after Hermann von Helmholtz.

  • It is a partial differential equation with the given mathematical formula. 
  • We need to consider three important functions mainly- Laplacian (which can be denoted as ∇2), the Wave Number (which is denoted by k), and the Amplitude (which is denoted as A). 
  • This is an Eigenvalue Equation, and can be solved by separating variables in 11 coordinated systems.
  • Helmholtz equation is used to solve problems in physics such as seismology, electromagnetic radiation, and acoustics.

∇2A + k2A = 0

Where,

  • ∇2 = Laplacian
  • k = Wave Number
  • A = Amplitude

Also Read: Oscillations and Waves Important Notes


Derivation of Helmholtz Equation

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The equation of wave is given by,

(∇2 – 1/c2 ∂2/∂x2) u(r, t) = 0 (Wave Equation) (Eq.1)

After separating the variables, we get,

u(r, t) = A(r) T(t) (Eq.2)

Now substituting (2) in (1):

∇2 A/A = 1/c2 T*d2 T/dt2

In this equation, the expression on LHS depends on r and RHS depends on t. But the equations are valid only if both the sides are equal to some constant value.

After solving linear partial differential equations by separating the variables we will get 2 equations – one for A (r) and other for T (t).

∇2 A/A = - k2 (Eq.3)

And, 1/c2 T. d2T/dt2 = - k2  s (Eq.4)

After rearranging we get the Helmholtz equation which is:

∇2A+k2A = (Δ2 + k2)A = 0

Where,

-k2 = Separation constant

Also Read:


Derivation of Helmholtz Free Energy Equation

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The Helmholtz function is given by,

F = U - TS

Where,

U = Internal energy

T = Temperature

S = Entropy

Now, Fi = Initial Helmholtz function

And, Fr = Final function

During the isothermal reversible process, when the temperature is constant the work done will be:

W ≤ Fi - Fr

As per the above statement, the Helmholtz function is converted into work. Therefore, this function is also known as free energy in thermodynamics.

Suppose an isolated system acquires “δQ” heat from surroundings, while the temperature is constant.

So,

Entropy gained by the system will be “dS”

& Entropy lost by surroundings will be “δQ/T”

As per the 2nd law of thermodynamics, net entropy = positive

From Classius inequality:

dS - δQ/T ≥ 0

dS ≥ δQ/T

Now, multiply both the sides by T,

TdS ≥ δQ

Now, putting δQ = dU + δW (1st law of thermodynamics)

TdS ≥ (dU + δW)

Now,

TdS ≥ dU + δW

Or,

δW ≤ TdS - dU

Integrating both the sides, we get:

W ≤ T (Sr - Si) - (Ur - Ui)

W ≤ (Ui - TSi) - (Ur - TSr)

Now, if we will see the equation, the term (Ui - TSi) is the initial Helmholtz function and the term (Ur - TSr) is the final Helmholtz function.

Therefore, we can say that:

W ≤ Fi - Fr

Also Read:

Helmholtz Equation Thermodynamics

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Gibbs free energy is a function of temperature & pressure and it is given by,

G = G (T, P)

And, G(T) = H(T) - T S(T)

Where,

H = Enthalpy

S = Entropy

Now, divide LHS and RHS by T:

G(T)/T = H(T)/T - T S(T)/T

Now, doing the partial differentiation on both the sides:

At constant pressure, P

(∂G(T)/T)p = - H(T)/2 + 1/T (∂H(T)P /∂T - (∂S(T)/∂T)P

Since 1/T (∂H(T))p /∂T and (∂S(t)/∂t)P are equal you can cancel them out. After cancellation you will get the equation as:

(∂S/∂T)P = CP (T)/T = 1/T (∂H/∂T)P

CP(T) = (∂S/∂T)P

(∂S/∂T)P = - H/T2

(∂ΔG/∂T)P = - ΔH/T2

This known as the Gibbs-Helmholtz equation in thermodynamics.

Also Read: Standard Enthalpy of Form


Applications of Helmholtz Equation

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Helmholtz equation is important for various applications. Some of them are as follows:

  1. It is used in seismology which is the scientific study of earthquakes and elastic waves.
  2. Exlplaining and analysing natural disaster like Tsunamis.
  3. This equation also plays an important role in Medical imaging.
  4. Through this equation Volcanic eruptions can be explained and predicted.
  5. This equation is also important for the calculation of Electromagnetism.
  6. CHELS: CHELS stands for combined Helmholtz equation-least squares. This method is used to recreate acoustic radiation from any arbitrary object.
  7. Gibbs-Helmholtz equation: It is used for calculating the change in enthalpy by using the change in the Gibbs energy when the temperature is different at constant pressure.

Also Read:


Things to Remember

  • Helmholtz Equation is named after Hermann von Helmholtz. It is a linear, partial, differential equation. 
  • It is used in Physics and Mathematics. Its mathematical formula is : ∇2A + k2A = 0
  • Helmholtz Free energy can be defined as the work done, extracted from the system, keeping the temperature and volume constant. 
  • Gibbs Helmholtz Equation has applications in the calculation of temperature change effect on the equilibrium constant and the calculation of enthalpy change for reactions when the temperature is not 298K. 

Some PYQs Related to this Chapter

  1. When 50cm350cm3 of 0.2N H2SO4 is mixed with…. (KCET 2004)
  2. 6 moles of an ideal gas expand isothermally and reversibly from….(VITEEE 2006)
  3. When ideal gas expands in vacuum, the work done by the gas is equal to… (ViTEEE 2006)
  4. 0.2 moles of an ideal gas is taken round the cycle ABC… (JIPMER 2009)
  5. In the equation PVγ = constant, the value of...(BITSAT 2010)
  6. A solid body of constant heat capacity… (BITSAT 2012)
  7. Initially two gas samples 1 and 2 are at the same condition… (BITSAT 2006)
  8. Which of the following is best close to an ideal black body… (NEET 2012)
  9. In the adiabatic compression, the decrease in volume is… (BITSAT 2008)
  10. One mole of a perfect gas expands isothermally to ten times… (JKSET 2004)

Sample Questions

Ques. Define Helmholtz function? (2 marks)

Ans: The thermodynamic function of a system which is equal to the difference between the internal energy and the product of temperature and entropy of the system is known as Helmholtz function.

Ques. How to calculate Helmholtz free energy? (4 marks)

Ans: We all know that:

U = Internal energy of the system

PV = Pressure-volume product

TS = Temperature-entropy product

T = Temperature above absolute zero

So, the Helmholtz equation will be:

F = U - TS & G = H - TS

And, H = U + PV

So, we can calculate the Helmholtz free energy by the equation:

G = U + PV - TS

Ques. What is the difference between Gibbs free energy and Helmholtz free energy? (2 marks)

Ans: The Helmholtz free energy is the work drawn out from the system while maintaining the constant temperature and volume.

Whereas Gibbs free energy is the maximum reversible work drawn out from the system while maintaining constant temperature and pressure.

Ques. Can Helmholtz free energy be negative? (2 marks)

Ans: As we all know that the work done, W = Fi – Fr. Therefore, the initial Helmholtz equation is always more than the final one. So, the difference (ΔF) between Fi and Fr will be negative.

Ques. Write the formula of Helmholtz free energy. (1 mark)

Ans: The formula of Helmholtz free energy is “F = U - TS”.

Ques. What did Helmholtz discover? (1 mark)

Ans: Helmholtz was a German physician and physicist who had an interest in the physiology of the senses. So, he discovered an ophthalmoscope which is an instrument used to examine the inside of a human eye.

Ques. What are the three Theorems of Helmholtz’s? (3 Marks)

Ans. Here are the three theorems associated with the Helmholtz-

Theorem-1: “The strength of a vortex filament is constant along its length.”

Theorem-2: “A vortex filament cannot end in a fluid; it must extend to the boundaries of the fluid or form a closed path.”

Theorem-3: “In the absence of rotational external forces, a fluid that is initially irrotational remains irrotational.”

Also Read:

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