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Dollar Gamma, Homogeneity, and Martingale Expectations

Article Quant Q&A · Author: chris

Summary

The document examines whether the expected value of an option’s dollar gamma, defined as spot price squared times gamma, remains equal to its initial value under a lognormal Black–Scholes process. One response uses the homogeneity of the Black–Scholes price to relate dollar gamma to strike squared times the strike curvature. That curvature is connected to a discounted terminal-price density, motivating a martingale argument through the pricing equation and Feynman–Kac.

A second response relates vega to dollar gamma and derives an expectation that includes an interest-rate factor. It concludes that the proposed equality holds when the interest rate is zero, while for nonzero rates the expectation grows by that factor. The answers offer distinct arguments and assumptions; one also claims a broader PDE-based extension beyond Black–Scholes. The discussion is theoretical and does not fully work through every proof step, so the conditions for any generalization require care.

Key ideas

  • Black–Scholes price homogeneity links dollar gamma to strike squared times strike curvature.
  • Strike curvature can be represented using the discounted density of the terminal underlying price.
  • A martingale argument can connect the current dollar gamma to its future expectation under suitable assumptions.
  • The second derivation relates vega to dollar gamma and finds an interest-rate adjustment to the expectation.
  • The zero-rate case recovers the stated equality, while nonzero rates alter it.

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Full text
# Expectation of Gamma times S$^2$ in Black-Scholes model


# Expectation of Gamma times S$^2$ in Black-Scholes model












Can somebody prove that:

$$E[S_t^2 \times \Gamma(t,S_t)] = S_0^2 \times \Gamma(0,S_0)$$

where $S_t$ follows a lognormal process as in the Black-Scholes model, and Gamma is the second derivative $\partial^2 C/\partial S^2$ of the option price with respect to S.

I can see it is true using simulation, but I can't prove it. It seems to be true for the Vega as well.

## Answer by user34971 (score 14)

https://quant.stackexchange.com/a/45474

What you have to do is to show that the dollar gamma satisfies the Black-Scholes PDE. Using Feynman-Kac it then follows that the dollar gamma is an expectation of a "payoff", just like the Black-Scholes claim price is an expectation of a payoff. And if something is the expectation of a payoff then it's a martingale.

Actually, you don't need the Black-Scholes assumption. This will work for any model (LV, SV, LSV...).

I'll leave the above for you to carry out. What I'd like to show is a nice little trick using the homogeneity property of the Black-Scholes price formula: Denoting partial derivatives by subscripts, the homogeneity of the BS call price function means that $$ C = SC_S + KC_K $$ Take again the derivative to $S$ of the above equation, and also take the derivative to $K$ of the above equation. That will give you two equations, and after some cancelling will lead you the the following equality: $$ S^2C_{SS} = K^2C_{KK} $$ The left hand side is the dollar gamma. The right hand side is $K^2$ times the discounted probability density. But the discounted probability density is just $$ C_{KK} = e^{-r(T-t)} E_t [ \delta(S_T-K)] $$ where $\delta$ is the Dirac delta-function. Hence the dollar gamma is a martingale.

Note that the homogeneity trick also immediately shows that the dollar delta is a martingale as well since $C_K = - e^{-r(T-t)} E_t [\theta (S_T - K)] $, where $\theta$ is the Heaviside function.

## Answer by Gordon (score 9)

https://quant.stackexchange.com/a/45487

The conjecture is true when the interest rate is zero. Note that, from this question, under the Black-Scholes model, \begin{align*} \Gamma(t,S_t) &= \frac{N'(d_1(t))}{S_t \sigma \sqrt{T-t}}\\ Vega(t,S_t) &= S_tN'(d_1(t)) \sqrt{T-t}, \end{align*} where \begin{align*} d_1(t) = \frac{\ln \frac{S_t}{K} + \big(r+\frac{1}{2}\sigma^2\big)(T-t)}{\sigma \sqrt{T-t}}. \end{align*} Then, it is easy to see that \begin{align*} Vega(t,S_t) = \sigma\, (T-t)\, S_t^2\, \Gamma(t,S_t). \end{align*} Consequently, \begin{align*} E\big( \sigma (T-t)\,S_t^2\, \Gamma(t,S_t)\big) &= E\big(Vega(t,S_t)\big) \tag{1}\\ &= E\left(\frac{\partial}{\partial \sigma}E\left(e^{-r(T-t)} (S_T-K)^+\big|\mathscr{F}_t\right) \right). \end{align*} However, we are not able to take the partial differential out as this differential only involves the volatility from $t$ to $T$, and, if we take it out, then the volatility from $0$ to $T$ is involved.

We denote by $\sigma_1=\sigma$ the volatility from $0$ to $t$, and $\sigma_2=\sigma$ the volatility from $t$ to $T$. Moreover, let \begin{align*} \hat{\sigma} = \sqrt{\frac{1}{T}\left(\sigma_1^2 t + \sigma_2^2 (T-t)\right)} = \sigma. \end{align*} Then \begin{align*} E\big(Vega(t,S_t)\big) &= E\left(\frac{\partial}{\partial \sigma_2}E\left(e^{-r(T-t)} (S_T-K)^+\big|\mathscr{F}_t\right) \right)\\ &=\frac{\partial}{\partial \sigma_2}E\left(e^{-r(T-t)} (S_T-K)^+\right)\\ &= e^{rt} \frac{\partial}{\partial \sigma_2}E\left(e^{-rT} (S_T-K)^+\right)\\ &= e^{rt} \frac{\partial}{\partial \hat{\sigma}}E\left(e^{-rT} (S_T-K)^+\right) \frac{\partial \hat{\sigma}}{\partial \sigma_2}\\ &=e^{rt} Vega(0,S_0) \frac{T-t}{T}\\ &= e^{rt} \sigma\, T\,S_0^2\, \Gamma(0,S_0) \frac{T-t}{T}\\ &= e^{rt} \sigma\, (T-t)\,S_0^2\, \Gamma(0,S_0). \end{align*} Therefore, from $(1)$, \begin{align*} E\big(S_t^2\, \Gamma(t,S_t)\big) = e^{rt} S_0^2\,\Gamma(0,S_0). \end{align*}

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This summary was written by Stratmill's research agent from the original; it is not a copy of the source.