Rough Volatility: Kernel Normalization and Conditional Variance
Summary
The document discusses a rough volatility representation in which changes in log variance are decomposed into a future Wiener integral and a term determined by the history up to the current time. The historical component is measurable using current information, while the future component is independent of it. This decomposition supports calculating conditional expected variance by integrating over the independent Gaussian contribution.
The response addresses why a rescaled Gaussian integral can omit the fractional Brownian motion normalization constant: the constant changes the process variance, but not its path roughness. Applying Kolmogorov continuity arguments to the power-law kernel gives a Hölder regularity determined by the kernel exponent, linked here to the Hurst parameter. The post also raises how conditioning on the full filtration differs from conditioning only on current variance in a non-Markovian model, but directs readers elsewhere for the detailed derivation. Thus, its explanation of normalization and roughness is concise rather than a complete treatment of conditional expectations.
Key ideas
- The log variance increment separates into a past-dependent term and an independent future Gaussian term.
- The past-dependent component is known conditional on the information available at the current time.
- A normalization factor changes variance scaling without changing the kernel's roughness exponent.
- The power-law kernel's exponent determines the stated Hölder regularity of the Gaussian integral.
- In a non-Markovian rough volatility model, current variance alone need not summarize all relevant history.
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# Realised variance under simple rough volatility model
# Realised variance under simple rough volatility model
Using the Mandelbrot-Vann Ness representation of fractional Brownian motion in terms of Wiener integrals, increments of the logarithm of realized variance $v = \sigma^{2}$, under the physical measure $\mathcal{P}$, are expressed as
\begin{equation} \begin{aligned} \log v_{u}-\log v_{t} &=2 \nu C_{H}\left(W_{u}^{H}-W_{t}^{H}\right) \\ &=2 \nu C_{H}\left(\int_{-\infty}^{u}|u-s|^{H-\frac{1}{2}} d W_{s}^{\mathbb{P}}-\int_{-\infty}^{t}|t-s|^{H-\frac{1}{2}} d W_{s}^{\mathbb{P}}\right) \\ &=2 \nu C_{H}\left(\int_{t}^{u}|u-s|^{H-\frac{1}{2}} d W_{s}^{\mathbb{P}}+\int_{-\infty}^{t}\left[|u-s|^{H-\frac{1}{2}}-|t-s|^{H-\frac{1}{2}}\right] d W_{s}^{\mathbb{P}}\right) \\ &=: 2 \nu C_{H}\left[M_{t}(u)+Z_{t}(u)\right] \end{aligned} \end{equation}
With $H$,our hurst parameter that determines the roughness of the fractional Brownian motion .In this expression, the left integral $M_{t}(u)$ is independent of $\mathcal{F}_{t}$ and the right integral $Z_{t}(u)$ is $\mathcal{F}_{t}$-measurable.Note that $\tilde{W}^{P}$ is defined as:
\begin{equation} \tilde{W}^{P}:=\sqrt{2 H} \int_{t}^{u} \frac{d W_{s}^{\mathbb{P}}}{(u-s)^{\gamma}} \end{equation} On this step I don't know why we separated $\tilde{W}^{P}$ from $C_{H}$,shouldn't the term $C_{H}$ be mandatory to have a proper fractional Brownian motion of parameter $H$ .Moreover I don't get why we added a $\sqrt{2H}$ in the expression.To continue it is said that $\tilde{W}^{P}$ has the same properties as $M_{t}(u)$, only with variance $(u − t)^{2H}$ . With $\eta:=\frac{2\nu C_{H}}{\sqrt{2H}}$ we have $2\nu M_{t}(u) C_{H}= \eta \tilde{W}^{P}$ and so : \begin{equation} \mathbb{E}^{\mathbb{P}}\left[v_{u} \mid \mathcal{F}_{t}\right]=v_{t} \exp \left\{2 \nu C_{H} Z_{t}(u)+\frac{1}{2} \eta^{2} \mathbb{E}\left|\tilde{W}_{t}^{\mathbb{P}}(u)\right|^{2}\right\} \end{equation} However,I do not clearly understand this passage.is it because $Z_{t}(u)$ depends only on historical values,which makes it non Markovian that we do not treat it as a random variable here ? After that ,the last step is straightforward to derive as : \begin{equation} \begin{aligned} v_{u} &=v_{t} \exp \left\{\eta \tilde{W}_{t}^{\mathbb{P}}(u)+2 \nu C_{H} Z_{t}(u)\right\} \\ &=\mathbb{E}^{\mathbb{P}}\left[v_{u} \mid \mathcal{F}_{t}\right] \mathcal{E}\left(\eta \tilde{W}_{t}^{\mathbb{P}}(u)\right) \end{aligned} \end{equation}
With $\mathcal{E}$ being the Wick stochastic integral such :
\begin{equation} \mathcal{E}(\Psi)=\exp \left(\Psi-\frac{1}{2} \mathbb{E}\left[|\Psi|^{2}\right]\right) \end{equation}
Lastly I also don't understand why in the rough volatility models we have $\mathbb{E}^{\mathbb{P}}\left[v_{u} \mid \mathcal{F}_{t}\right] \neq \mathbb{E}^{\mathbb{P}}\left[v_{u} \mid v_{t}\right]$.
Thank you for your help.
## Answer by Jose Avilez (score 5, accepted)
https://quant.stackexchange.com/a/66498
My answer on MSE has details on the computations of $\mathbb{E}(v_s \, | \, \mathcal{F}_t)$ and $\mathbb{E}(v_s \, | \, \mathcal{v}_t)$, which answers why the rough Bergomi model is not Markovian. See here.
However, on this post you have an extra question: why do we rip out $C_H$ in our definition of $\tilde{W}$?
The answer is simple: it's just a normalisation constant. This affects the variance of the process, but it does not affect the roughness of the process. In particular, the Hölder exponent of $$\tilde{W}_t(u) = \sqrt{2H}\int_t^u \frac{dW_s}{(u-s)^\gamma}$$ is solely dependent on the choice of $\gamma$ in the power law kernel $(u-s)^{-\gamma}$. To see this, you may apply Kolmogorov's continuity criterion to get that $\tilde{W}_t(u)$ admits a.s. $(\frac{1}{2} - \gamma - \epsilon)$-Hölder continuous paths. Since we set $H = \frac{1}{2} - \gamma$, this is equivalent to a.s. $(H-\epsilon)$-continuous paths, which is the expected roughness for fBM.Shown in full with attribution under the source's licence. Licence: CC BY-SA 4.0 (Stack Exchange)
This summary was written by Stratmill's research agent from the original; it is not a copy of the source.