## Friday, May 08, 2015

### Decoding Hagan's arbitrage free SABR PDE derivation

Here are the main steps of Hagan derivation. Let's recall his notation for the SABR model where typically, $$C(F) = F^\beta$$

First, he defines the moments of stochastic volatility:
Then he integrates the Fokker-Planck equation over all A, to obtain
On the backward Komolgorov equation, he applies a Lamperti transform like change of variable:
And then makes another change of variable so that the PDE has the same initial conditions for all moments:
It turns out that there is a magical symmetry for k=0 and k=2.
Note that in the second equation, the second derivative applies to the whole.
Because of this, he can express $$Q^{(2)}$$ in terms of $$Q^{(0)}$$:
And he plugs that back to the integrated Fokker-Planck equation to obtain the arbitrage free SABR PDE:

There is a simple more common explanation in the world of local stochastic volatility for what's going on. For example, in the particle method paper from Guyon-LabordÃ¨re, we have the following expression for the true local volatility.

In the first equation, the numerator is simply $$Q^{(2)}$$ and the denominator $$Q^{(0)}$$. Of course, the integrated Fokker-Planck equation can be rewritten as:

$$Q^{(0)}_T = \frac{1}{2}\epsilon^2 \left[C^2(F) \frac{Q^{(2)}}{Q^{(0)}} Q^{(0)}\right]_{FF}$$

Karlsmark uses that approach directly in his thesis, using the expansions of Doust for $$Q^{(k)}$$. Looking a Doust expansions, the fraction reduces straightforwardly to the same expression as Hagan, and the symmetry in the equations appears a bit less coincidental.

### Decoding Hagan's arbitrage free SABR PDE derivation

Here are the main steps of Hagan derivation. Let's recall his notation for the SABR model where typically, $$C(F) = F^\beta$$

First, he defines the moments of stochastic volatility:
Then he integrates the Fokker-Planck equation over all A, to obtain
On the backward Komolgorov equation, he applies a Lamperti transform like change of variable:
And then makes another change of variable so that the PDE has the same initial conditions for all moments:
Because of this, he can express $$Q^{(2)}$$ in terms of $$Q^{(0)}$$:
In the first equation, the numerator is simply $$Q^{(2)}$$ and the denominator $$Q^{(0)}$$. Of course, the integrated Fokker-Planck equation can be rewritten as:
$$Q^{(0)}_T = \frac{1}{2}\epsilon^2 \left[C^2(F) \frac{Q^{(2)}}{Q^{(0)}} Q^{(0)}\right]_{FF}$$
Karlsmark uses that approach directly in his thesis, using the expansions of Doust for $$Q^{(k)}$$. Looking a Doust expansions, the fraction reduces straightforwardly to the same expression as Hagan, and the symmetry in the equations appears a bit less coincidental.