How can i derive this Gibbs energy equation?

In summary, the conversation discusses the relationship between standard state cell potential and equilibrium constant for a reaction in an electrochemical cell. This is derived by combining the equations ΔG=-nFE and ΔG=ΔGθ + RT lnQ, where Q represents the equilibrium constant and ΔGθ is related to Eθ, the standard cell potential. At equilibrium, Q is equal to K and the net free energy change for the whole process is zero. This results in the equation ΔGθ=nFEθ=RT lnK, showing the relationship between Eθ and K.
  • #1
lioric
306
20

Homework Statement



For an electrochemical cell Gibbs free energy is is given by G=-nFE
Gibbs free energy for a reaction at any moment in time and standard state free energy is given by G=Go + RT lnQ

Derive an expression relating standard state cell potential and equilibrium constant for a reaction


Homework Equations



ΔG=-nFE and ΔG=ΔGθ + RT lnQ

The Attempt at a Solution



I actually don t have an idea
But i m guessing that i have to mix both equations up since ΔG is common and then I'm totally clueless
 
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  • #2
What will be the value of ΔG and Q at equilibrium? And if Eθ were the standard cell potential, how would it be related to ΔGθ?
 
  • #3
Q would be K G would be-nFE
 
  • #4
lioric said:
Q would be K G would be-nFE

Q would be K. You are right there. However, ΔGθ=nFEθ (you have already written so). Now to the part which is key to solving this,

When you have the reactants and products at equilibrium, what do you think the net free energy change for the whole process ( forward +backward reactions) is?

Say A [itex]\Leftrightarrow[/itex] B. For the forward reaction, let ΔG be the free energy change. What will be the free energy change for the reverse reaction? So what will be net free energy change (free energy change for forward reaction + free energy change for the reverse reaction)?

If you figure this out, the answer to the original question just pops out.:wink:
 
  • #5


To derive the Gibbs energy equation for an electrochemical cell, we can start with the definition of Gibbs free energy:

ΔG = ΔH - TΔS

Where ΔH is the enthalpy and ΔS is the entropy of the system. For an electrochemical cell, the enthalpy change is related to the electrical work done by the cell, which is given by:

ΔH = -nFE

Where n is the number of moles of electrons transferred and F is the Faraday constant (96,485 C/mol). Substituting this into the Gibbs free energy equation, we get:

ΔG = -nFE - TΔS

Next, we can use the relation between entropy change and standard state free energy:

ΔS = ΔSθ + R lnQ

Where ΔSθ is the standard state entropy and Q is the reaction quotient. Substituting this into the Gibbs free energy equation, we get:

ΔG = -nFE - T(ΔSθ + R lnQ)

Simplifying, we get:

ΔG = -nFE - RT lnQ + RTΔSθ

Finally, we can use the relation between standard state free energy and standard state cell potential:

ΔGθ = -nFEθ

Where Eθ is the standard state cell potential. Substituting this into the equation, we get:

ΔG = ΔGθ + RT lnQ + RTΔSθ

Rearranging, we get the desired expression:

ΔGθ = -RT lnK

Where K is the equilibrium constant for the reaction. This shows that the standard state cell potential is related to the equilibrium constant through the Gibbs free energy equation.
 

1. What is the Gibbs energy equation?

The Gibbs energy equation, also known as the Gibbs free energy equation, is a fundamental equation in thermodynamics that relates the energy of a system to its temperature, pressure, and entropy. It is used to determine the spontaneity of a chemical or physical process and is often written as ΔG = ΔH - TΔS, where ΔG is the change in Gibbs energy, ΔH is the change in enthalpy, T is the temperature in Kelvin, and ΔS is the change in entropy.

2. How is the Gibbs energy equation derived?

The Gibbs energy equation is derived from the laws of thermodynamics, particularly the first and second laws. The first law states that energy cannot be created or destroyed, only transferred and transformed. The second law states that the total entropy of a closed system always increases over time. By combining these laws with other thermodynamic equations, such as the equation for entropy, the Gibbs energy equation can be derived.

3. What is the significance of the Gibbs energy equation?

The Gibbs energy equation is significant because it allows us to predict the spontaneity of a process and the direction in which it will occur. If ΔG is negative, the process is spontaneous and will occur in the forward direction. If ΔG is positive, the process is non-spontaneous and will not occur without an external driving force. If ΔG is zero, the process is at equilibrium and is reversible. Thus, the Gibbs energy equation helps us understand and control chemical and physical processes.

4. Can the Gibbs energy equation be applied to all systems?

Yes, the Gibbs energy equation can be applied to all systems, including open, closed, and isolated systems. However, it is most commonly used for closed systems, where energy can be exchanged with the surroundings but matter cannot. In open systems, where both energy and matter can be exchanged, the Helmholtz energy equation is used instead. In isolated systems, where neither energy nor matter can be exchanged, the internal energy equation is used.

5. How can I use the Gibbs energy equation in practical applications?

The Gibbs energy equation is used in many practical applications, including chemical reactions, phase transitions, and material stability. For example, in chemical reactions, the Gibbs energy equation can be used to determine the conditions under which a reaction will be spontaneous and produce a desired product. In material stability, the equation can be used to predict the stability of different phases of a material at different temperatures and pressures. Overall, the Gibbs energy equation is a powerful tool in understanding and predicting the behavior of various systems.

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