A flat distribution of defaults

Take a basket of nn credits. Each one defaults with the same probability pp, and every pair of them has the same asset correlation ρ\rho. How many defaults should you expect, and how are they distributed?

Two cases are easy. If the names are independent, the count is binomial. If they are perfectly correlated they share one fate: either none default or all of them do. Everything between those two needs numerical work.

Except at one point, where the answer is as simple as an answer can be.

The model

This is the Gaussian copula, the standard model for a credit basket. Each name has a latent asset return, and the name defaults when that return falls below a threshold. Matching the threshold to the default probability pp puts it at Ξ¦βˆ’1(p)\Phi^{-1}(p) standard deviations.

Correlation enters through a single market factor MM:

Rk=ρ M+1βˆ’Οβ€‰ZkR_k = \sqrt{\rho}\, M + \sqrt{1-\rho}\, Z_k

where ZkZ_k is noise particular to name kk. Conditional on the market β€” once MM is known β€” the names are independent, so the number of defaults is binomial with a shifted probability. Integrating that binomial over the market factor gives the distribution:

p(m)=Φ ⁣(Ξ¦βˆ’1(p)βˆ’mρ1βˆ’Ο)p(m) = \Phi\!\left( \frac{\Phi^{-1}(p) - m\sqrt{\rho}}{\sqrt{1-\rho}} \right) Pr⁑[N=j]=(nj)βˆ«βˆ’βˆžβˆžp(m)j (1βˆ’p(m))nβˆ’jΟ†(m) dm\Pr[N = j] = \binom{n}{j} \int_{-\infty}^{\infty} p(m)^{j}\,\bigl(1 - p(m)\bigr)^{n-j} \varphi(m)\, dm

That integral normally wants a quadrature rule. Which is the point: closed-form answers are scarce here, and scarce enough that a single one is worth having, if only to check the numerical methods against.

The special case

Look at p(m)p(m). It would be much friendlier if Ξ¦βˆ’1(p)\Phi^{-1}(p) were zero β€” that is, if p=12p = \tfrac{1}{2}. And friendlier still if the ρ\sqrt{\rho} and 1βˆ’Ο\sqrt{1-\rho} matched, which happens when ρ=12\rho = \tfrac{1}{2}. Put both together and the conditional probability collapses to

p(m)=Ξ¦(βˆ’m)=1βˆ’Ξ¦(m)p(m) = \Phi(-m) = 1 - \Phi(m)

Substituting u=Ξ¦(m)u = \Phi(m) turns the integral into a beta integral, and out comes B(nβˆ’j+1, j+1)B(n-j+1,\, j+1). But there is a better route that needs no calculus at all.

With p=12p = \tfrac{1}{2} and ρ=12\rho = \tfrac{1}{2} the factor model is just

Rk=12 (M+Zk)R_k = \sqrt{\tfrac{1}{2}}\,(M + Z_k)

and name kk defaults when Rk<0R_k < 0 β€” equivalently when M<βˆ’ZkM < -Z_k. Write Mβˆ—=βˆ’MM^{*} = -M, and name kk defaults exactly when Mβˆ—>ZkM^{*} > Z_k.

So the number of defaults is the number of the ZZβ€˜s that Mβˆ—M^{*} exceeds. Sort Mβˆ—M^{*} and the nn noise terms into one list. They are identically distributed continuous random variables, so Mβˆ—M^{*} is equally likely to land in any of the n+1n+1 positions. Therefore

Pr⁑[N=j]=1n+1\Pr[N = j] = \frac{1}{n+1}

Every outcome β€” no defaults, one default, all of them β€” is equally likely. The distribution is flat, and it stays flat for any nn.

Try it

Move the correlation and watch the binomial spread out, flatten, and then collapse toward the two-point distribution at ρ=1\rho = 1. The dashed line marks 1/(n+1)1/(n+1). It is only the answer at one setting, but you can see the shape pass through it.

1/(n+1) = 9.1%0 defaults: 9.1%1 default: 9.1%2 defaults: 9.1%3 defaults: 9.1%4 defaults: 9.1%5 defaults: 9.1%6 defaults: 9.1%7 defaults: 9.1%8 defaults: 9.1%9 defaults: 9.1%10 defaults: 9.1%Number of defaults
E[defaults] 5.00Οƒ 3.16Flat: every outcome from 0 to n is equally likely.

What to look for

The mean never moves. Slide the correlation from zero to one and the expected number of defaults stays at npn p throughout. Correlation does not change how likely any individual name is to default; it changes only how much they default together. Everything correlation does, it does to the shape.

The tails are what correlation buys. At low correlation the distribution concentrates near the mean and the extremes are negligible. Raise it and probability drains out of the middle into both ends β€” many defaults at once becomes far more likely, and so does none at all. This is the whole reason correlation matters for a tranche: a senior tranche only takes losses in the right tail, which barely exists at low correlation and is substantial at high.

Flat is not the same as random. A uniform distribution over 0…n0 \ldots n defaults looks like the least informative outcome possible, but it comes from a very specific pair of parameters. Move either one and the flatness goes.

Notes

The distribution is computed by numerical integration over the market factor, using a composite Gauss-Legendre rule with panels placed on the transition region β€” as ρ\rho approaches 1 the conditional default probability becomes nearly a step function in mm, and a fixed grid misses it. At p=ρ=12p = \rho = \tfrac{1}{2} the computed values agree with 1/(n+1)1/(n+1) to machine precision, which is the tightest check available: the code has to reproduce an exact identity, not merely come close.

This page follows Pete Benson, β€œDistribution of Defaults in a Credit Basket: An Interesting Special Case”, RiskMetrics Journal, Vol. 6, No. 1, Winter 2005, pp. 3–8. Per the editor’s note in that issue, the result became a standard interview question at RiskMetrics.