So the Nernst equation reveals the quantitative connection between the concentrations of compounds and cell potential. The Nernst equation is utilized when the concentrations of our compounds differ from 1 molar. We're gonna say that the Nernst equation equals our cell potential here. And this cell potential represents cell potential under non-standard conditions, meaning that our concentration isn't equal to 1 molar, our temperature wouldn't be 25 degrees Celsius.
Our pH would not equal 7. Our pressure wouldn't be 1 atmosphere. All of those values represent standard conditions. So 1 atmosphere, pH of 7, a temperature of 25 degrees Celsius as well as a concentration of 1 molar. When we have all of these conditions met, that means we're dealing with cell potential under standard conditions.
So that's \( E^0_{\text{cell}} \). So this represents our cell potential under standard conditions. Minus \( \frac{RT}{nF} \times \ln \frac{a}{a} \). So here again we said that this represented our standard cell potential. \( R \) here is our gas constant.
It is equal to 8.314 J/(mol\cdot K). Also remember here that when we talk about joules we're talking about energy. A joule is equal to volts times coulombs. Remember a volt is equal to joules over coulombs. So you substitute joules over coulombs times coulombs and that's how it equals joules.
So we can say this or 8.314 V\(\cdot\)C/(mol\(\cdot\)K). \( n \) equals the number of electrons transferred within our redox reaction. \( F \) equals Faraday's constant which is 96485 C/mol of electrons. \( A \) represents our activities. So activity here would just be our activity coefficient times the concentration of the ion if necessary.
Many times we may not be given some type of coefficient so you can just say activity, you could substitute in the concentration for that value. Now, we're going to say that this expression here represents products over reactants in terms of our redox reaction and it's equal to \( Q \), our reaction quotient that's \( R \cdot T \) divided by \( F \), here at 25 degrees Celsius, remember we have our \( R \) constant, we have our temperature of 25 degrees Celsius. We add 273.15 to this. So that gives me 298.15 K. \( F \) is our Faraday's constant.
Here we would see that from this moles would cancel out, kelvins would cancel out. What we'd have left at the end is joules over coulombs which is equal to volts. So \( \frac{RT}{F} \) reduces all the way down to 0.0257 V. So that means that our Nernst equation now becomes cell potential under non-standard conditions equals cell potential under standard conditions minus 0.0257 V/n, the number of electrons transferred, times \( \ln Q \). Remember \( Q \) is just your equilibrium expression.
Now here, if we multiply \( ln \) by 2.303 we can attain the log function. Now when we multiply this portion here by 2.303, we get a new value of 0.05916 V/n, now \( \log Q \). This is true because we say that \( \log(x) = \ln(x) / \ln(10) \). \( \ln(10) \) equals 2.303. So when I multiply both sides by 2.303, we can see that multiplying by 2 point potential calculated from the Nernst equation is the maximum potential at the instant the circuit the cell circuit is connected.
So that's the moment that the current or the flow of electrons moves from the anode to the cathode. So we're talking about the transferring of electrons from one electrode to another electrode. And we're gonna say as the cell discharges and current flows, the electrolyte concentrations will change. What's going to happen here is that \( Q \) will begin to increase and as a result, our cell potential over time will decrease until it gets to a point where the cell potential of my electrochemical cell equals 0. That's when we have a dead battery because at that moment, the battery has reached equilibrium.
So over time, the reaction will reach equilibrium and then \( Q \) which is our reaction quotient will equal \( K \) which is our equilibrium constant. The cell potential like I said would equal 0. We'd have a dead battery at that moment. Now as a result of this, once we've reached equilibrium we can substitute in \( K \) instead of \( Q \). So now our new equation can become \( e_{\text{cell}} \) equals \( e_{\text{cell}} \) under standard conditions minus \( RTNF \times \ln(K) \).
So here, if we were to work this out we could have 0 equals \( e_{\text{cell}} \) minus remember this value here would be 0.0257 volts/n, now times \( \ln(K) \). So what we can do here is subtract cell potential from both sides. So that'd be negative standard cell potential equals negative 0.0257 volts/n times \( \ln(K) \). Multiply both sides by \( n \). Then divide both sides now by negative 0.0257 volts.
So we get at this point \( \ln(K) = n \) times your cell potential under standard conditions divided by 0.0257 volts. To get rid of this \( \ln \), we take the inverse of the natural log so that means that \( K = e^{(n \times \text{your cell potential under standard conditions} / 0.0257 \, \text{volts})} \). And that's when we're dealing with \( \ln \). If we're to substitute in \( \log \) instead, so if we're dealing with a log function then, it would be 0.05916 volts/n times \( \log(K) \). In this instance, if we did the same exact, mathematical conversions.
In this case, because we're dealing with \( \log \), we'd find that \( K \) at the end equals \( 10^{(n \times \text{your cell potential under standard conditions} / 0.05916 \, \text{volts})} \). So this is how we connect our equilibrium constant to our standard cell potential with these two formulas. 1 when we're dealing with \( \ln \) and 1 where we're dealing with \( \log \). Now we could also say that when you're at equilibrium, we can talk about the connection to Gibbs free energy and your equilibrium constant \( K \). So here we'd say that \( \Delta G \) under nonstandard conditions equals \( \Delta G \) under standard conditions minus \( RT\ln(K) \).
When we've reached equilibrium, this \( \Delta G \) equals 0. So that means 0 equals \( \Delta G0 \)-\( RT\ln(K) \). Subtract \( \Delta G0 \) from both sides. Subtract \( \Delta G0 \) from both sides. So negative \( \Delta G0 \) equals negative\( RT\ln(K) \).
Divide both sides now by negative\( RT \). So \( \ln(K) = \Delta G0 / RT \). And so \( K = e^{(\Delta G0 / RT)} \). So we get this value at the end in terms of our connection between Gibbs Free Energy and your equilibrium constant \( K \). So just keep in mind some of the connections that we've seen here in terms of how things are connected to one another.
These two equations are just a way of us connecting cell potential to \( K \), and then from \( K \) to \( \Delta G \). And we know that from earlier we could also connect to cell potential from \( \Delta G \) as well when we have \( \Delta G = -n \times \text{Faraday's constant} \times \text{cell potential} \). Later on, we'll talk about this connection between the three variables. But for now, just realize we deal with the Nernst equation when we have concentrations that are not equal to 1 molar. And remember, the Nernst Equation can be written in 2 different ways.
We can write it in this version when we're dealing with \( \ln \) or we can have the Nernst Equation in this version when we're dealing with \( \log \). To go from \( \ln \) to \( \log \), you just use 2.303 to go from your \( \ln \) function to your \( \log \) function. So keep in mind the intricate dynamics involved in the Nernst equation in how it connects your cell potential in standard conditions to non-standard conditions.