Solution: Black-Scholes Call Price as a Risk-Neutral Expectation
Part 1: Q ( S T > K ) \mathbb{Q}(S_T > K) Q ( S T > K )
Under Q \mathbb{Q} Q , ln S T = ln S 0 + ( r − 1 2 σ 2 ) T + σ W T Q \ln S_T = \ln S_0 + (r - \tfrac{1}{2}\sigma^2)T + \sigma W_T^{\mathbb{Q}} ln S T = ln S 0 + ( r − 2 1 σ 2 ) T + σ W T Q with W T Q ∼ N ( 0 , T ) W_T^{\mathbb{Q}} \sim \mathcal{N}(0, T) W T Q ∼ N ( 0 , T ) . So ln S T \ln S_T ln S T is Gaussian with mean ln S 0 + ( r − 1 2 σ 2 ) T \ln S_0 + (r - \tfrac{1}{2}\sigma^2)T ln S 0 + ( r − 2 1 σ 2 ) T and variance σ 2 T \sigma^2 T σ 2 T .
Q ( S T > K ) = Q ( ln S T > ln K ) = Q ( ln S T − [ ln S 0 + ( r − 1 2 σ 2 ) T ] σ T > ln K − ln S 0 − ( r − 1 2 σ 2 ) T σ T ) \mathbb{Q}(S_T > K) = \mathbb{Q}(\ln S_T > \ln K) = \mathbb{Q}\!\left(\frac{\ln S_T - [\ln S_0 + (r - \tfrac{1}{2}\sigma^2)T]}{\sigma\sqrt{T}} > \frac{\ln K - \ln S_0 - (r - \tfrac{1}{2}\sigma^2)T}{\sigma\sqrt{T}}\right) Q ( S T > K ) = Q ( ln S T > ln K ) = Q ( σ T ln S T − [ ln S 0 + ( r − 2 1 σ 2 ) T ] > σ T ln K − ln S 0 − ( r − 2 1 σ 2 ) T )
The left side is standard normal Z Z Z , the right side is − d 2 -d_2 − d 2 . Hence
Q ( S T > K ) = Q ( Z > − d 2 ) = Φ ( d 2 ) \mathbb{Q}(S_T > K) = \mathbb{Q}(Z > -d_2) = \Phi(d_2) Q ( S T > K ) = Q ( Z > − d 2 ) = Φ ( d 2 )
using the symmetry Q ( Z > − d 2 ) = Q ( Z < d 2 ) = Φ ( d 2 ) \mathbb{Q}(Z > -d_2) = \mathbb{Q}(Z < d_2) = \Phi(d_2) Q ( Z > − d 2 ) = Q ( Z < d 2 ) = Φ ( d 2 ) .
Part 2: E Q [ S T 1 { S T > K } ] \mathbb{E}^{\mathbb{Q}}[S_T \mathbf{1}_{\{S_T > K\}}] E Q [ S T 1 { S T > K } ]
Write z = W T Q / T z = W_T^{\mathbb{Q}} / \sqrt{T} z = W T Q / T , so z ∼ N ( 0 , 1 ) z \sim \mathcal{N}(0, 1) z ∼ N ( 0 , 1 ) and W T Q = T z W_T^{\mathbb{Q}} = \sqrt{T}z W T Q = T z . Then
S T = S 0 e ( r − σ 2 / 2 ) T + σ T z S_T = S_0 e^{(r - \sigma^2/2)T + \sigma\sqrt{T}z} S T = S 0 e ( r − σ 2 /2 ) T + σ T z
and the event { S T > K } \{S_T > K\} { S T > K } is equivalent to { z > − d 2 } \{z > -d_2\} { z > − d 2 } (same manipulation as Part 1).
E Q [ S T 1 { S T > K } ] = ∫ − d 2 ∞ S 0 e ( r − σ 2 / 2 ) T + σ T z ⋅ 1 2 π e − z 2 / 2 d z \mathbb{E}^{\mathbb{Q}}[S_T \mathbf{1}_{\{S_T > K\}}] = \int_{-d_2}^{\infty} S_0 e^{(r - \sigma^2/2)T + \sigma\sqrt{T}z} \cdot \frac{1}{\sqrt{2\pi}} e^{-z^2/2}\,dz E Q [ S T 1 { S T > K } ] = ∫ − d 2 ∞ S 0 e ( r − σ 2 /2 ) T + σ T z ⋅ 2 π 1 e − z 2 /2 d z
Pull the S 0 e ( r − σ 2 / 2 ) T S_0 e^{(r - \sigma^2/2)T} S 0 e ( r − σ 2 /2 ) T out and combine exponents inside the integral:
= S 0 e ( r − σ 2 / 2 ) T ∫ − d 2 ∞ 1 2 π e σ T z − z 2 / 2 d z = S_0 e^{(r - \sigma^2/2)T} \int_{-d_2}^{\infty} \frac{1}{\sqrt{2\pi}} e^{\sigma\sqrt{T}z - z^2/2}\,dz = S 0 e ( r − σ 2 /2 ) T ∫ − d 2 ∞ 2 π 1 e σ T z − z 2 /2 d z
Complete the square in the exponent:
σ T z − z 2 2 = − 1 2 ( z − σ T ) 2 + σ 2 T 2 \sigma\sqrt{T}\,z - \frac{z^2}{2} = -\frac{1}{2}\bigl(z - \sigma\sqrt{T}\bigr)^2 + \frac{\sigma^2 T}{2} σ T z − 2 z 2 = − 2 1 ( z − σ T ) 2 + 2 σ 2 T
Substitute back:
= S 0 e ( r − σ 2 / 2 ) T e σ 2 T / 2 ∫ − d 2 ∞ 1 2 π e − ( z − σ T ) 2 / 2 d z = S_0 e^{(r - \sigma^2/2)T} e^{\sigma^2 T / 2} \int_{-d_2}^{\infty} \frac{1}{\sqrt{2\pi}} e^{-(z - \sigma\sqrt{T})^2/2}\,dz = S 0 e ( r − σ 2 /2 ) T e σ 2 T /2 ∫ − d 2 ∞ 2 π 1 e − ( z − σ T ) 2 /2 d z
= S 0 e r T ∫ − d 2 ∞ 1 2 π e − ( z − σ T ) 2 / 2 d z = S_0 e^{rT} \int_{-d_2}^{\infty} \frac{1}{\sqrt{2\pi}} e^{-(z - \sigma\sqrt{T})^2/2}\,dz = S 0 e r T ∫ − d 2 ∞ 2 π 1 e − ( z − σ T ) 2 /2 d z
Substitute u = z − σ T u = z - \sigma\sqrt{T} u = z − σ T , d u = d z du = dz d u = d z . The lower limit becomes u = − d 2 − σ T u = -d_2 - \sigma\sqrt{T} u = − d 2 − σ T . Note that d 1 = d 2 + σ T d_1 = d_2 + \sigma\sqrt{T} d 1 = d 2 + σ T , so − d 2 − σ T = − d 1 -d_2 - \sigma\sqrt{T} = -d_1 − d 2 − σ T = − d 1 . Hence
= S 0 e r T ∫ − d 1 ∞ 1 2 π e − u 2 / 2 d u = S 0 e r T ⋅ P ( Z > − d 1 ) = S 0 e r T Φ ( d 1 ) = S_0 e^{rT} \int_{-d_1}^{\infty} \frac{1}{\sqrt{2\pi}} e^{-u^2/2}\,du = S_0 e^{rT} \cdot \mathbb{P}(Z > -d_1) = S_0 e^{rT} \Phi(d_1) = S 0 e r T ∫ − d 1 ∞ 2 π 1 e − u 2 /2 d u = S 0 e r T ⋅ P ( Z > − d 1 ) = S 0 e r T Φ ( d 1 )
So E Q [ S T 1 { S T > K } ] = S 0 e r T Φ ( d 1 ) \mathbb{E}^{\mathbb{Q}}[S_T \mathbf{1}_{\{S_T > K\}}] = S_0 e^{rT}\Phi(d_1) E Q [ S T 1 { S T > K } ] = S 0 e r T Φ ( d 1 ) .
Part 3: combine
C 0 = e − r T ( E Q [ S T 1 { S T > K } ] − K Q ( S T > K ) ) C_0 = e^{-rT}\bigl(\mathbb{E}^{\mathbb{Q}}[S_T \mathbf{1}_{\{S_T > K\}}] - K\,\mathbb{Q}(S_T > K)\bigr) C 0 = e − r T ( E Q [ S T 1 { S T > K } ] − K Q ( S T > K ) )
= e − r T ( S 0 e r T Φ ( d 1 ) − K Φ ( d 2 ) ) = e^{-rT}\bigl(S_0 e^{rT}\Phi(d_1) - K\Phi(d_2)\bigr) = e − r T ( S 0 e r T Φ ( d 1 ) − K Φ ( d 2 ) )
= S 0 Φ ( d 1 ) − K e − r T Φ ( d 2 ) = S_0\Phi(d_1) - K e^{-rT}\Phi(d_2) = S 0 Φ ( d 1 ) − K e − r T Φ ( d 2 )
This is the
Black-Scholes call price .
□ \square □
Part 4: absence of μ \mu μ
The entire calculation was performed under
Q \mathbb{Q} Q , where the stock drift is
r r r . The real-world drift
μ \mu μ never appeared. This is expected:
risk-neutral pricing replaces the real-world drift with r r r , so no formula derived as a
Q \mathbb{Q} Q -expectation can depend on
μ \mu μ . The market's view of the equity risk premium is irrelevant to the option's no-arbitrage price — only the replicability (here, through
σ \sigma σ ) matters.
Takeaways
The call price splits into two pieces. Φ ( d 1 ) \Phi(d_1) Φ ( d 1 ) is the risk-neutral expected in-the-money payoff per unit of stock, and Φ ( d 2 ) \Phi(d_2) Φ ( d 2 ) is the risk-neutral exercise probability. Both are outputs of the same log-normal integral, separated by the completing-the-square step.
d 1 d_1 d 1 and d 2 d_2 d 2 differ by σ T \sigma\sqrt{T} σ T . Not by accident: the shift comes from the Gaussian change of variable in the S T S_T S T -weighted integral, which is exactly the "change of numeraire" from the bank account to the stock — a measure change in its own right.
Risk-neutral calculations are drift-free. The computation went through without any assumption about μ \mu μ . This is the computational payoff of risk-neutral pricing: a single measure change makes the derivative price a deterministic function of S 0 , K , r , T , σ S_0, K, r, T, \sigma S 0 , K , r , T , σ .