Perturbation Methods in Credit Derivatives. Colin Turfus. Читать онлайн. Newlib. NEWLIB.NET

Автор: Colin Turfus
Издательство: John Wiley & Sons Limited
Серия:
Жанр произведения: Ценные бумаги, инвестиции
Год издания: 0
isbn: 9781119609599
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from all possible default times in the exposure period, which requires in turn calculation of the value of the swap underlying at each such time for each Monte Carlo path. It is noted that analytic formulae for calculation of such protection are provided in §9.3.5 for single‐currency interest rate swaps and in §10.4 and §12.4 for cross‐currency swaps. The formulae are implemented and it is found that substantial speed‐up is achieve in pricing, and particularly in risk‐managing these trades.

      The CVA desk hear about this and note that the CVA calculations they perform on interest rate portfolios are closely related to the contingent CDS protection pricing problem. They start looking into whether they could incorporate a similar analytic pricing approach into their workflow.

      Another desk meanwhile trading hybrid products into emerging markets notices that the bank's pricing library now provides production‐quality analytic methods for option pricing under the Black–Karasinski model. They frequently use this model in preference to Hull–White as an interest rate model, as they find it performs better in market conditions with high and volatile interest rates. They are interested in what analytic functions are available and see that in Chapter 5 there are explicit formulae for caplets, swaptions and zero coupon bonds (stochastic discount factors) which they consider could be useful, particularly in the process of model calibration, where pricing of calibration instruments must otherwise be done by repeated Monte Carlo simulation.

      They note in addition that results in Chapter 14 allow calibration of the Black–Karasinski model in a multi‐curve framework where the LIBOR spread(s) over the risk‐free rate can be stochastic and potentially correlated with the risk‐free rate. Furthermore, they note that results in Chapter 13 facilitate the extension of Black–Karasinski option pricing formulae enabling the model to be conveniently calibrated to caps referencing backward‐looking risk‐free rates, as and when a market in these inevitably appears in the post‐IBOR world to which the finance industry is currently headed.

      An option being considered is to try and evolve the curves in their entirety rather than just principal components. Standard models such as HJM‐based or Black–Karasinski present themselves as candidates. But to be useful, there has to be a convenient mechanism for constructing the entire forward curve at each exposure time of interest, for use as input to the pricing model. The Black–Karasinski lognormal model is preferred to the simpler normal Hull–White alternative on the basis that, as the curve evolves upward or downward, lognormal volatilities rise or fall in proportion, which is intuitively sensible: if a Hull–White model is used instead, consideration would have to be given also to how the volatilities evolved as the associated curve moved up or down. Further, for the curve evolution to work in a credit curve context it must ensure positive values of all forward rates, which Black–Karasinski does, HJM‐based models can, but Hull–White does not.

      Encouragement is taken from the availability of the highly accurate analytic conditional bond formulae for the Black–Karasinski model set out in Chapter 5. But it is felt that the simple one‐factor model does not do justice to the range of possible evolutions of the shape, not just the level, of interest rate and credit curves. Specifically, there should be fluctuations which impact mainly at the short end of the curve which decay relatively quickly (rapid mean reversion), whereas fluctuations affecting the long end are likely to be longer‐lived (slow mean reversion). So the multi‐factor Black–Karasinski model framework derived in §6.4 and expounded in greater detail in §15.5 is of interest. Work is initiated to implement the forward rate formula (15.49) to allow forward interest rate and credit curves to be generated from simple evolved Brownian variables, mutually correlated as necessary.

      It is noted that the calculations set out in Chapter 8 illustrate how to price credit‐contingent (default or survival) cash flows accurately under circumstances of relatively weak credit risk, with credit intensity represented by a Black–Karasinski short‐rate model; further, that the relevant formulae are not limited in terms of the size of the credit volatility. The formula (8.54) for the value of protection payments is coded up and compared with the results from the Monte Carlo engine as the volatility level is increased. While the analytic results are seen to increase linearly with the credit volatility, the Monte Carlo results are found to deviate from this behaviour. It is concluded that there is likely model error resulting in this circumstance. A proposal is made that, in the event that volatility levels exceed a given threshold, a reserve should be set aside based on the difference between the Monte Carlo results and analytic results derived using the formulae presented in Chapter 8. A suggestion is also made that the front office quantitative analysts consider integrating a pricer based on the analytic formulae into the pricing library and migrating trades over from the Monte Carlo model.

      Buoyed by this success, the model validation team within the model risk management department consider implementing more of the analytic formulae in their benchmark library for use as “challenger models” in the model validation process. In addition they note from the suggestions in Chapter 16 that in addition to providing alternative benchmarks, these analytic formulae upon differentiation are able to provide explicit formulae for the sensitivity of prices to model and market parameters. In this way model uncertainty calculations can be conveniently carried out, potentially at a large number of points in the product‐model phase space. Thus the circumstances can be identified where the greatest model uncertainty is to be expected. In particular, model testing can be focussed on such “hot spots”.