# Strong convergence rates for Euler approximations to a class of   stochastic path-dependent volatility models

**Authors:** Andrei Cozma, Christoph Reisinger

arXiv: 1706.07375 · 2018-10-09

## TL;DR

This paper proves strong convergence rates of order 1/2 (up to a log factor) for Euler schemes approximating a class of path-dependent stochastic volatility models, including Heston-type models, under mild conditions.

## Contribution

It establishes the first positive convergence rate for Euler schemes applied to these complex path-dependent stochastic volatility models.

## Key findings

- Convergence order of 1/2 (up to a log factor) is achieved.
- Euler schemes are proven to be effective for path-dependent models.
- The results include Heston-type and other stochastic-local volatility models.

## Abstract

We consider a class of stochastic path-dependent volatility models where the stochastic volatility, whose square follows the Cox-Ingersoll-Ross model, is multiplied by a (leverage) function of the spot price, its running maximum, and time. We propose a Monte Carlo simulation scheme which combines a log-Euler scheme for the spot process with the full truncation Euler scheme or the backward Euler-Maruyama scheme for the squared stochastic volatility component. Under some mild regularity assumptions and a condition on the Feller ratio, we establish the strong convergence with order 1/2 (up to a logarithmic factor) of the approximation process up to a critical time. The model studied in this paper contains as special cases Heston-type stochastic-local volatility models, the state-of-the-art in derivative pricing, and a relatively new class of path-dependent volatility models. The present paper is the first to prove the convergence of the popular Euler schemes with a positive rate, which is moreover consistent with that for Lipschitz coefficients and hence optimal.

## Full text

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## Figures

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## References

54 references — full list in the complete paper: https://tomesphere.com/paper/1706.07375/full.md

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Source: https://tomesphere.com/paper/1706.07375