2. Framework

Notation

Let X be a random variable (rv) with cumulative distribution function (cdf) $F_X$ , and, given they exist, probability density function (pdf) $f_X$ , mean $\mu$ , variance $\sigma^2$ , as well as, for any integer $r\geq 1$ , the r-th absolute centred moment, $\mu(X,r) \,{:\!=}\, \mathbb{E}[\lvert X - \mu \rvert^r ]$ and quantile of order p defined as $q_X(p)\,{:\!=}\, \inf \{ x \in \mathbb{R}: F_X(x) \geq p \}$ . For a n-sample $(X_1,\cdots,X_n)$ , we denote the associated order statistics by $X_{(1)}\leq ...\leq X_{(n)}$ .

Recall the sample estimator of the quantile for any order $p \in (0,1]$ , defined as $ q_n (p) = X_{( \lceil np \rceil )}$ , where $\lceil x \rceil = \min{ \{ m \in \mathbb{Z} : m \geq x \} }$ , $\lfloor x \rfloor = \max{ \{ m \in \mathbb{Z} : m \leq x \} }$ and [x], are the rounded-up, rounded-off integer parts and the nearest integer of a real number $x \in \mathbb{R}$ , respectively.

The r-th absolute centred sample moment is defined, for $r \in \mathbb{N}$ , by

(1) \begin{equation}\hat{m}(X,n,r) \,{:\!=}\, \frac{1}{n} \sum_{i=1}^n \lvert X_i - \bar{X}_n \rvert^r,\end{equation}

$\bar{X}_n$ denoting the empirical mean. Special cases of this latter estimator include the sample variance ( $r=2$ ) and the sample Mean Absolute Deviation (denoted as MAD) around the sample mean ( $r=1$ ).

Some standard notations: $u^T$ for the transpose of a vector u and, for the signum function, $\displaystyle \textrm{sgn}(x) \,{:\!=}\, -\unicode{x1D7D9}_{(x<0)}+\unicode{x1D7D9}_{(x>0)}$ . Moreover the notations $\overset{d}\rightarrow$ , $\overset{a.s.}\rightarrow$ , $\overset{P}\rightarrow$ , and $\overset{D_d[0,1]}\rightarrow$ correspond to the convergence in distribution, almost surely, in probability and in distribution of a random vector in the d-dimensional Skorohod space $D_d[0,1]$ . Further, for real-valued functions f, g, we write $f(x) = O(g(x))$ (as $x \rightarrow \infty)$ if and only if there exists a positive constant M and a real number $x_0$ s.t. $\lvert f(x) \rvert \leq M g(x)$ for all $x \geq x_0$ , and $f(x)=o(g(x))$ (as $x \rightarrow \infty$ ) if for all $\epsilon>0$ there exists a real number $x_0$ s.t. $\lvert f(x) \rvert \leq \epsilon g(x)$ for all $x \geq x_0$ . Analogously, for a sequence of rv’s $X_n$ and constants $a_n$ , we denote by $X_n = o_P(a_n)$ the convergence in probability to 0 of $X_n/a_n$ .

Risk Measures

Let us recall the definitions of the risk measures we consider in this paper. One of the most used risk measures is Value-at-Risk (VaR), popularised by JP Morgan in 1996 (see Morgan & Reuters, Reference Morgan and Reuters1996), and defined as follows: If we assume a loss random variable L having a continuous, strictly increasing distribution function $F_L$ , the VaR at level p of L is simply the quantile $q_L(p)$ of order p of L:

(2) \begin{equation}\textrm{VaR}_{p} = \inf \Big\{ x \,{:}\, P [L \leq x] \geq p \Big\} = q_L(p).\end{equation}

Despite the availability of other approaches, in practice the VaR is usually estimated on historical data (see e.g. Pérignon & Smith, Reference Pérignon and Smith2010 or European Banking Authority, 2019) for quantitative surveys on this matter), using the empirical quantile $\widehat{\textrm{VaR}}_{n} (p) =q_{n}(p)$ associated to a n-loss sample $(L_{1}, \dotsc, L_{n})$ with $p \in (0,1)$ .

VaR has been shown not to be a coherent risk measure, Artzner et al. (Reference Artzner, Delbaen, Eber and Heath1999), contrary to Expected Shortfall (ES), introduced in slightly different formulations in Artzner et al. (Reference Artzner, Delbaen, Eber and Heath1997, Reference Artzner, Delbaen, Eber and Heath1999), Acerbi & Tasche (Reference Acerbi and Tasche2002), Rockafellar & Uryasev (Reference Rockafellar and Uryasev2002). ES is defined as follows (e.g. Acerbi & Tasche, Reference Acerbi and Tasche2002) for a loss random variable L and a level $p \in (0,1)$ :

(3) \begin{equation} \textrm{ES}_{p} = \frac{1}{1-p} \int_{p}^1 q_L (u) du =\mathbb{E}[L \vert L \geq q_L(p)].\end{equation}

While the first equality in (3) is the definition of ES, the second one holds only if L is continuous. There are different ways of estimating ES, we focus on the two most direct ones when using historical estimation.

First, simply approximating the conditional expectation in (3) by averaging over k sample quantiles, i.e.

(4) \begin{equation} \widetilde{\textrm{ES}}_{n,k} (p)\,{:\!=}\, \frac{1}{k} \sum_{i=1}^k q_n(p_i),\end{equation}

for a specific choice of $p=p_1 < p_2 <...<p:k <1$ . This was e.g. proposed in Emmer et al. (Reference Emmer, Kratz and Tasche2015) in the context of backtesting expected shortfall (using $p_i = 0.25\ p (5-i)+ 0.25(i-1),\ i=1,...,4$ ).

Another way was proposed in Chen (Reference Chen2008) and can be seen as a special case of $\widetilde{\textrm{ES}}_{n,k} (p)$ choosing $k=n-[np]+1$ and the $p_i$ accordingly, estimating it as a conditional mean of the sample:

(5) \begin{equation} \widehat{\textrm{ES}}_{n} (p)\,{:\!=}\, \frac{1}{n-[np]+1} \sum_{i=1}^n L_i \ \unicode{x1D7D9}_{(L_i \geq q_n (p))}.\end{equation}

The discussions about which risk measure would be most appropriate to use for evaluating the risk of financial institutions have often included a third risk measure, the expectile. It was introduced, in the context of least-squares estimation in Newey & Powell (1987) and later used as a risk measure in finance and actuarial science (see e.g. Kuan et al., Reference Kuan, Yeh and Hsu2009; Bellini et al., Reference Bellini, Cesarone, Colombo and Tardella2021 and references therein, to refer to the pioneering paper and a very recent one, respectively). This risk measure satisfies many favourable properties (in particular for backtesting), making it appealing from a theoretical point of view (see e.g. Bellini & Bignozzi, Reference Bellini and Bignozzi2015; Ziegel, Reference Ziegel2016 and references therein). It is defined, for a square-integrable loss random variable L and level $p \in (0,1)$ , by the following minimiser

(6) \begin{equation} e_{p} = \textrm{argmin}_{x \in \mathbb{R}} \left( p\mathbb{E}[\max(L-x,0)^2] + (1-p) \mathbb{E}[\max(x-L,0)^2] \right).\end{equation}

There are various ways to estimate the expectile, the most natural one being the argmin of the empirical version of (6). Here, for simplicity, we choose to estimate it through a sample quantile using the following relation given in Yao & Tong (Reference Yao and Tong1996): Let $q_L(p)$ be the quantile at level $p \in (0,1)$ , then there exists a bijection $\kappa: (0,1) \mapsto (0,1)$ such that $e_{\kappa(p)} (L) = q_L(p)$ with

(7) \begin{equation} \kappa ( p ) = \frac{p\, q_L(p) - \int_{-\infty}^{q_L(p)} x\, dF_L(x)}{\mathbb{E}[L] - 2 \int_{-\infty}^{q_L(p)} x\, dF_L(x) - (1-2p) q_L(p)}.\end{equation}

Thus, we consider the sample estimator for the expectile at level p denoted as

(8) \begin{equation} \hat{e}_n(p) \,{:\!=}\, q_n (\kappa^{-1} (p)).\end{equation}

As unified notation representing these risk measures and their estimators defined above, we introduce, for $j=1,...,4$ :

(9) \begin{equation} \zeta^{(j)} (p) = \begin{cases} \textrm{VaR}_{p} & \text{for}\,\, j=1, \\ \\[-8pt] \textrm{ES}_{p} & \text{for}\,\, j=2, \\ \\[-8pt] \textrm{ES}_{p} & \text{for}\,\, j=3,\\ \\[-8pt] e_{p} & \text{for}\,\, j=4, \end{cases} \quad \text{with estimators} \, \zeta_n^{(j)} (p) = \begin{cases} \widehat{\textrm{VaR}}_{n}(p) & \text{for}\,\, j=1, \\ \\[-8pt] \widehat{\textrm{ES}}_{n}(p) & \text{for}\,\, j=2, \\ \\[-8pt] \widetilde{\textrm{ES}}_{n,k}(p) & \text{for}\,\, j=3,\\ \\[-8pt] \hat{e}_n(p) & \text{for}\,\, j=4. \end{cases}\end{equation}

Since we will work in a dynamic setting, time needs to be introduced. Therefore, we introduce a time-series notation of our estimated quantities. By

(10) \begin{equation} \widehat{\textrm{VaR}}_{n,t}(p), \;\widehat{\textrm{ES}}_{n,t}(p), \;\widetilde{\textrm{ES}}_{n,k,t}(p), \;\hat{e}_{n,t}(p),\; \zeta_{n,t}^{(j)} (p),\end{equation}

we denote the corresponding estimators estimated at time t over the last n observations before time t.

Framework setup

The samples considered in this study will be either realisations from iid rv’s (white noise process) or from augmented GARCH(p, q) processes (with the latter naturally including the former as a special case), since they include two families that allow one to isolate the pro-cyclicality effects, as shown in Bräutigam (Reference Bräutigam2020) (see also Bräutigam et al., Reference Bräutigam, Dacorogna and Kratz2022): One is the iid model that exemplifies the inherent part of pro-cyclicality (due to the use of historical estimation), and the other is the GARCH(1,1) model that shows that pro-cyclicality is caused by GARCH effects, i.e. return-to-the-mean and clustering of volatility (thus further amplifying the effect of pro-cyclicality).

Recall that an augmented GARCH(p, q) process $X=(X_t)_{t \in \mathbb{Z}}$ , due to Duan (Reference Duan1997), satisfies, for integers $p \geq 1$ and $q\geq 0$ ,

(11) \begin{align}X_t &= \sigma_t \ \epsilon_t \end{align}

(12) \begin{align}\text{with} \quad \Lambda(\sigma_t^2) &= \sum_{i=1}^p g_i (\epsilon_{t-i}) + \sum_{j=1}^q c_j (\epsilon_{t-j}) \Lambda(\sigma_{t-j}^2), \end{align}

where $(\epsilon_t)$ is a series of iid rv’s with mean 0 and variance 1, $\sigma_t^2 = \textrm{Var}(X_t)$ and $\Lambda, g_i, c_j, i=1,...,p, j=1,...,q$ , are real-valued measurable functions. Also, as in Lee (Reference Lee2014), we restrict the choice of $\Lambda$ to the so-called group of either polynomial GARCH(p, q) or exponential GARCH(p, q) processes:

\begin{equation*} {\textrm{(Lee)}}\qquad\qquad\qquad\qquad\qquad \Lambda(x) = x^{\delta}, \text{for some} \, \delta >0, \quad \text{or} \quad \Lambda(x) = \log(x)\qquad\qquad\qquad\qquad\qquad\qquad\end{equation*}

Using this family of processes, let us now explain how we proceed to assess the pro-cyclicality of the proposed risk measure estimators (defined in (9) and (10)), based on the methodology developed in Bräutigam (Reference Bräutigam2020) and Bräutigam et al. (Reference Bräutigam, Dacorogna and Kratz2022). Namely, we use an indicator, the look-forward ratio, that quantifies the difference between the historically predicted risk and the estimated realised future risk (measured ex post) by considering the ratio of those two quantities: $\displaystyle {\zeta}_{n, \, t+n}^{(j)}(p)/{\zeta}_{n, \, t}^{(j)}(p)$ (with the time-series notation, i.e. estimation at any time $t, t+n$ over the last n observations before time $t, t+n$ ). We study this ratio as a function of the realised volatility (a proxy for market states). Then, we investigate theoretically the dependence between the look-forward ratio and the realised volatility estimated with the r-th absolute central sample moment (1), denoted $\hat{m}(X,n,r,t)$ (or $\hat{m}(n,r,t)$ when no confusion possible). A negative dependence will characterise the degree of pro-cyclicality of the considered risk measures estimators. As their dependence is nonlinear, we study the joint asymptotic distribution between the logarithm of the look-forward ratio and the r-th absolute central sample moment.

Note that the two quantities defining the look-forward ratio are estimators defined on disjoint, finite samples. Thus, some care has to be taken to translate the setting from a finite sample of overall size n, into an asymptotic one, where $n \rightarrow \infty$ . In order to simplify computations, we use a little trick to obtain the disjointness of the estimators. Namely, we consider $\zeta_{n/2,\, t+n/2}^{(j)}(p), \zeta_{n/2,\, t}^{(j)}(p)$ and $\hat{m} (n/2,r,t)$ , where we assume w.l.o.g. that $n/2$ is an integer. It means that the estimators are evaluated on a sample of size $n/2$ each.

Denoting the correlation of the asymptotic distribution for the two quantities of interest, to ease and by abuse of notation, as

(13) \begin{equation} \lim_{n \rightarrow \infty} \textrm{Cor}\left(\log\left \lvert \frac{{\zeta}_{n/2, \, t+n/2}^{(j)}(p)}{{\zeta}_{n/2, \, t}^{(j)}(p)} \right\rvert, \hat{m}(X,n/2, \, r, \,t)\right),\quad j=1,...,4, \, r>0,\end{equation}

the measure of the pro-cyclicality of risk measure estimators amounts then to the degree of negative correlation of (13).

3. An Asymptotic Theorem for Assessing Pro-Cyclicality

Let us now present the main result on pro-cyclicality. For the ease of presentation, the main theorem is presented in Section 3.1 while the discussion and explanation of the specific conditions under which this result holds are deferred to Section 3.2.

3.1 Main result

Extending the study Bräutigam et al. (Reference Bräutigam, Dacorogna and Kratz2022) (see also Bräutigam, Reference Bräutigam2020) performed for the VaR, we provide here a general asymptotic theorem to assess theoretically the negative dependence for the historical estimators of any of the considered risk measures and any of the dispersion measures. With such a generality, it highlights even more the impact of historical risk measurements on pro-cyclicality. Moreover, we state this main theorem for the large family of augmented GARCH processes (defined in (11) and (12)), including of course the two models, iid and GARCH(1,1), which we used to isolate and prove the effect of pro-cyclicality. This generalisation is made for modelers using more sophisticated GARCH models as e.g. HAR, EGARCH, to model the volatility dynamics. To allow for such an extension, we need a set of conditions for the asymptotic theorem to hold. The simpler the model, the weaker the conditions. Those conditions will be made specific after the statement of the theorem (in Section 3.2) to discuss them, from the simplest iid case, which is also more intuitive, to the general augmented GARCH case that requires more work.

Let us present the result in its full generality. We refer to Appendix A for its proof.

Theorem 1 Let $X= (X_t)_{t \in \mathbb{Z}}$ be either a white noise process or from the family of augmented GARCH(p,q) processes and have stationary distribution with its cdf, pdf, and quantile denoted as $F_X, f_X, q_X$ , respectively. Consider a risk measure estimator $\zeta_n^{(j)} (p)$ , $j \in \{ 1,...,4\}$ , and the r-th absolute central sample moment $\hat{m}(n,r)$ , for a chosen integer $r>0$ . Given the choice of process, risk and dispersion measures, assume its corresponding set of conditions (given explicitly in Section 3.2), i.e. either one of (S ₁), (S ₂), (S ₃), (S ₄) in the iid case, or one of ( ${S^{\ast}_{1}}$ ), ( ${S^{\ast}_{2}}$ ), ( ${S^{\ast}_{3}}$ ), ( ${S^{\ast}_{4}}$ ) when X belongs to the the family of augmented GARCH(p,q) processes.

Then, the asymptotic distribution of the logarithm of the look-forward ratio of the risk measure estimator with the r-th absolute central sample moment, at any given fixed time t, is bivariate normal, i.e.

\[ \sqrt{n} \begin{pmatrix} \log \left\lvert \frac{\zeta_{n/2,\, t+n/2}^{(j)}(p)}{\zeta_{n/2,\, t}^{(j)}(p)} \right \rvert \\ \\[-8pt] \hat{m}(n/2, \, r, \,t) - \mu(X,r) \end{pmatrix} \overset{d}{\rightarrow} \mathcal{N}(0, \tilde{\Gamma}), \]

with $\tilde{\Gamma}=(\tilde{\Gamma}_{ik})_{1\le i,\,k\le 2}$ and $\tilde{\Gamma}_{ik} = \begin{cases} 4\Gamma_{ik}/\left( \zeta^{(j)} (p) \right)^2 & \textit{for} \, i=k=1,\\ \\[-8pt] 2\Gamma_{ik} & \textit{for} \, i=k=2 ,\\ \\[-8pt] -2\Gamma_{ik}/\zeta^{(j)} (p) & \textit{otherwise,} \end{cases} $

$\Gamma$ being the covariance matrix of the asymptotic bivariate distribution between $\zeta_n^{(j)} (p)$ and $\hat{m}(n,r)$ (see Appendix A.1 for the explicit expressions in the different cases). In particular, the correlation of this asymptotic bivariate distribution equals

(14) \begin{equation} \frac{\tilde{\Gamma}_{12}}{\sqrt{\tilde{\Gamma}_{11}} \sqrt{\tilde{\Gamma}_{22}}} = \frac{-1}{\sqrt{2}} \textrm{sgn}(\zeta^{(j)} (p)) \frac{\Gamma_{12}}{\sqrt{\Gamma_{11}} \sqrt{\Gamma_{22}}} = \frac{-1}{\sqrt{2}} \frac{\lvert \Gamma_{12} \rvert}{\sqrt{\Gamma_{11}} \sqrt{\Gamma_{22}}},\end{equation}

thus, it is always nonpositive.

3.2 Discussion of the conditions sets

Let us introduce and explain the different types of conditions we need to consider.

First, we impose four conditions on the distribution function $F_X$ . They are needed for the asymptotic representation of the different risk measure (and measure of dispersion) estimators: The continuity of $F_X$ (or its l-th derivative), the l-fold differentiability of $F_X$ for any integer $l> 0$ , and the positivity of its density $f_X$ . These conditions hold at a given point or neighbourhood and are named as

$(C_{0})\quad F_X \, \text{is continuous},$

$(C_{l})\quad \text{the} \, l \, \text{-th derivative of} \, F_X \, \text{is continuous,}$

$(C_{l}^{\prime})\quad F_X \, \text{is} \, l\text{-times differentiable,}$

$(P)\quad f_X \, \text{is positive.}$

Equally, to establish any Cental Limit Theorem (CLT), we need a condition on the finiteness of the moments of the innovation process of the augmented GARCH process, (M _k ), for $k \in \mathbb{N}$ ,

\begin{align*} \textrm{(}{{M}_{{k}}}\textrm{)}\qquad\qquad\qquad\qquad \mathbb{E}[\lvert \epsilon_0 \rvert^{2k}] < \infty.\qquad\qquad\qquad\qquad\qquad\qquad\qquad\qquad\qquad\qquad\qquad\qquad\qquad\qquad \end{align*}

To motivate which of these conditions are exactly needed for asymptotic theorem, let us informally explain how to establish (13) considering the iid case. In a later step, we then point out the additional conditions needed for the class of augmented GARCH(p, q) processes.

IID case – In this case, recall that the sample used for any risk measure estimator at time $t+n/2$ , $\zeta_{n/2,\, t+n/2}^{(j)}(p)$ , is, by construction, disjoint from the sample used at time t. Thus, the estimator $\zeta_{n/2,\, t+n/2}^{(j)}(p)$ will be uncorrelated with the r-th absolute centred sample moment $\hat{m}(n/2,r,t)$ , at time t, as well as with the risk measure estimator $\zeta_{n/2,\, t}^{(j)}(p)$ at time t.

Translating this for the correlation of the asymptotic distribution (again abusing the notation), i.e. (13), it should hold, for $j=1,...,4$ ,

(15) \begin{align} \lim_{n \rightarrow \infty} &\textrm{Cor}\left( \log{\left\lvert \frac{\zeta_{n/2,\, t+n/2}^{(j)}(p)}{\zeta_{n/2,\, t}^{(j)}(p)}\right\rvert}, \,\hat{m}(n/2, \, r, \,t) \right) = \lim_{n \rightarrow \infty} \frac{\textrm{Cov}( - \log{\lvert \zeta_{n/2,\, t}^{(j)}(p) \rvert}, \hat{m}(n/2, \, r, \,t))} {\sqrt{2 \textrm{Var}(\log{\lvert \zeta_{n/2,\, t}^{(j)}(p) \rvert})} \sqrt{\textrm{Var}(\hat{m}(n/2, \, r, \,t))}} \nonumber\\ & = \frac{-1}{\sqrt{2}} \lim_{n \rightarrow \infty} \textrm{Cor}( \log \lvert \zeta_{n,\, t}^{(j)}(p) \rvert, \hat{m}(n,r,t))= \frac{-1}{\sqrt{2}} \left\lvert \lim_{n \rightarrow \infty} \textrm{Cor}( \zeta_{n,\, t}^{(j)}(p), \hat{m}(n,r,t)) \right\rvert, \end{align}

where the first equality follows by the uncorrelatedness (which also holds for finite n), the second by the scale invariance of the correlation, and the third as a consequence of the Delta-method with the logarithm.

Thus, in the iid case, establishing (13) reduces to proving a joint asymptotic normality between $\zeta_{n,\, t}^{(j)}(p)$ and $\hat{m}(n,r,t)$ . To do so, we need conditions to obtain an appropriate representation of the risk measure estimator $\zeta_{n,\, t}^{(j)}(p)$ and moment conditions depending on the chosen dispersion measure $\hat{m}(n,r,t)$ . We group the set of conditions $(S_j)$ by the choice of risk measure $\zeta_{n,\, t}^{(j)}(p), j=1,...4$ , for a given measure of dispersion $\hat{m}(n,r,t)$ , $r\in \mathbb{N}$ , where

\begin{equation*}(S_{1})=S(p) \qquad \text{and}\qquad (S_{4})=S\left(\kappa^{-}(p)\right) \qquad\text{with}\quad S(\cdot): \left\{\begin{array}{l} (C_1^{\prime}) (\text{see}\ ({\text{$C_{l}^{\prime}$}})) \, \text{at} \, q_X(\cdot)\\[4pt] ({P}) \, \text{at} \, \mu \, \text{for} \, r=1, \; \text{and} \, \text{at} \, q_X(\cdot) \\[4pt] (M_r) (\text{see}\ ({\text{$M_{k}$}}))\end{array} \right.\end{equation*}

\begin{equation*} (S_{2}) : \left\{\begin{array}{l}(C_3) (\text{see}\ ({\text{$C_{l}$}})) \, \text{in a neighbourhood of} \, q_X(p) \\[4pt] F_X \, \text{absolutely continuous} \\[4pt] (M_r) \;\text{and} \; (M_{1+\gamma}) (\text{see}\ ({\text{$M_{k}$}})) \, \text{for some} \, \gamma>0 \\[4pt] ({P}) \, \text{at} \, \mu \, \text{for} \, r=1\end{array} \right. \quad \text{and}\qquad (S_{3}): \left\{\begin{array}{l}\text{For} \, l=2,...,k:\\[4pt] S(p_l) \\[4pt] (C_1^{\prime}) (\text{see}\ ({\text{$C_{l}^{\prime}$}})) \, \text{at} \, q_X(p_l) \\[4pt] ({\text{$P$}}) \, \text{at} \, q_X(p_l)\end{array} \right.\end{equation*}

Augmented GARCH( p , q ) – Clearly, in the case of the augmented GARCH(p, q) processes family, we will need additional conditions for the asymptotic normality to hold. There are two reasons for this. First, the conditions to establish such a limit theorem are stronger. Second, any two estimators, even if computed over disjoint samples, might be correlated (in contrast to the iid case), so the argumentation in (13) does not hold without further requirements.

Let us first discuss conditions for establishing a bivariate asymptotic theorem between $\zeta_{n,\, t}^{(j)}(p)$ and $\hat{m}(n,r,t)$ for the family of augmented GARCH(p, q) processes.

Note that already for a strictly stationary solution to (11) and (12) to exist, the functions $\Lambda, g_i, c_j$ as well as the innovation process $(\epsilon_t)_{t \in \mathbb{Z}}$ have to fulfil some regularity conditions (see e.g. Lee, Reference Lee2014, Lemma 1), namely the positivity of the functions used, (A), and the boundedness in $L_r$ -norm for either the polynomial GARCH, (P_v ), or exponential/logarithmic GARCH, (L_v ), respectively, for a given integer $v>0$ :

\begin{align*} (A)\quad\quad\quad\qquad\qquad\qquad\qquad\qquad g_i \geq 0, c_j \geq 0, i=1,...,p,\ j=1,...,q,\qquad\qquad\qquad\qquad\qquad\end{align*}

\begin{align*} (P_{v})\quad\qquad\qquad\qquad\qquad\qquad\sum_{i=1}^p \| g_i(\epsilon_0) \|_v < \infty, \quad \sum_{j=1}^q \| c_j(\epsilon_0) \|_v < 1,\qquad\qquad\qquad\qquad\qquad\end{align*}

\begin{align*} (L_{v}) \quad\qquad\qquad\qquad\qquad\qquad \mathbb{E}\left[ \exp\left(4v\sum_{i=1}^p \lvert g_i(\epsilon_0) \rvert^2\right)\right] < \infty, \quad \sum_{j=1}^q \lvert c_j(\epsilon_0) \rvert < 1.\qquad\qquad\qquad\end{align*}

Note that Condition (L_v ) requires the $c_j$ to be bounded functions.

It was shown by Lee that these conditions are sufficient conditions for establishing a CLT for the volatility process (see Lee, Reference Lee2014, Corollary 1) and, together with the finiteness of the innovations process, i.e. $(M_r)$ (see (M _k )), also for the CLT of the augmented GARCH(p, q) process itself.

For this, Lee exploited the known fact that the $L_2$ -near-epoch dependence ( $L_2$ -NED) paired with corresponding finite moments is a sufficient condition for establishing the CLT.

Let us recall the concept of $L_p$ -near-epoch dependence ( $L_p$ -NED), using a definition due to Andrews (Reference Andrews1988) but restricted to stationary processes. Let $(Z_n)_{n \in \mathbb{Z}}$ , be a sequence of rv’s and $\mathcal{F}_s^t = \sigma(Z_s,...,Z_t)$ , for $s \leq t$ , the corresponding sigma-algebra. By $\lvert \cdot \rvert$ , we denote the Euclidean norm and the usual $L_p$ -norm is denoted by $\| \cdot \|_p \,{:\!=}\, \mathbb{E}^{1/p}[ \lvert \cdot \rvert^p]$ .

Definition 2 ( $L_p$ -NED, Andrews, Reference Andrews1988) For $p>0$ , a stationary sequence $(X_n)_{n \in \mathbb{Z}}$ is called $L_p$ -NED on $\left( Z_n\right)_{ n\in \mathbb{Z} }$ if, for $k \geq 0$ ,

\[ \| X_1 - \mathbb{E}[X_1 \vert \mathcal{F}_{n-k}^{n+k}] \|_p \leq \nu(k), \]

for non-negative constants $\nu(k)$ such that $\nu(k) \rightarrow 0$ as $k \rightarrow \infty$ .

If $\nu(k)= O(k^{-\tau -\epsilon})$ for some $\epsilon >0$ , we say that $X_n$ is $L_p$ -NED of size $\left(\!-\tau\right)$ .

If $\nu(k)=O(e^{-\delta k})$ for some $\delta>0$ , we say that $X_n$ is geometrically $L_p$ -NED.

Now that we have discussed the conditions for establishing a CLT, let us go back to (13) and the fact that two estimators, even if computed over disjoint samples, might be correlated as those processes exhibit dependence. In this case, we show that the condition of strong mixing with geometric rate makes the estimators on disjoint samples asymptotically uncorrelated, thus, recovering structurally the pro-cyclicality behaviour as in the iid case. It means that, besides $L_2$ -NED dependence, also strong mixing with geometric rate is an additional condition needed for the class of augmented GARCH(p, q) processes.

Let us recall for completeness the notion of strong mixing, denoting for a sequence of random variables $(Z_n)_{n \in \mathbb{Z}}$ the corresponding $\sigma$ -algebra as $\mathcal{F}_s^t = \sigma(Z_s,...,Z_t)$ for $s\leq t$ :

Definition 3 (Strong mixing) Define, as measure of dependence, for any integer $n\geq 1$ ,

(16) \begin{equation} \alpha(n) \,{:\!=}\, \sup_{j \in \mathbb{Z}} \sup_{C \in \mathcal{F}_{-\infty}^j, D \in \mathcal{F}_{j+n}^{\infty}} \lvert P(C \cap D) - P(C)P(D) \rvert.\end{equation}

The sequence of rv’s $(Z_n)_{n \in \mathbb{Z}}$ is called strongly mixing if $\alpha(n) \rightarrow 0$ as $n \rightarrow \infty$ . It is called strongly mixing with geometric rate if there exist constants $\lambda \in (0,1)$ and c such that $\alpha(n) \leq c \lambda^n$ for every n.

If we denote the set of conditions for the family of augmented GARCH(p, q) processes X by $(S_j^{*})$ (as extension to the set of conditions $(S_j)$ in the iid case), again grouped by the choice of risk measure $\zeta_{n,\, t}^{(j)}(p), j=1,...4$ , for a given measure of dispersion $\hat{m}(n,r,t)$ , $r\in \mathbb{N}$ , we get:

\begin{equation*} (S^{*}_{1}) =S^{*}(p) \,\, \text{and}\,\, (S^{*}_{4}) =S^{*}(\kappa^{-}(p))\,\,\,\text{with}\;S^{*}(\cdot): \left\{\begin{array}{l} (C_2^{\prime}) (\text{see}\ ({\text{$C_{l}^{\prime}$}})) \, \text{at} \, q_X(\cdot) \\[4pt] ({\text{$P$}}) \, \text{at} \, \mu \, \text{for} \, r=1, \;\text{and at} \, q_X(\cdot) \\[4pt] (M_{r+ \tau}) (\text{see}\ ({\text{$M_{k}$}})) \, \text{for some} \, \tau>0\\[4pt] X \, \text{strongly mixing with geometric rate}\\[4pt] ({Lee}) \quad \text{and}\quad ({A}) \\[4pt] (P_{\max{(1, \frac{r}{\delta})}}) (\text{see}\ ({\text{$P_{v}$}})) \, \text{if} \, X \text{ is polynomial GARCH} \\[4pt] (L_r) (\text{see} \, ({\text{$L_{v}$}})) \, \text{if} \, X \text{ is exponential GARCH}\end{array} \right.\end{equation*}

\begin{equation*} (S^{*}_{2}) : \left\{\begin{array}{l} (S_{1}^{*}) \\[4pt] F_X \, \text{absolutely continuous}\\[4pt] (C_3) (\text{see}\ ({\text{$C_{l}$}})) \, \text{in a neighbourhood of} \, q_X(p) \\[4pt] (M_{1+\gamma}) (\text{see}\ ({\text{$M_{k}$}})) \, \text{for some} \, \gamma>0 \, \text{for} \, r=1\\[4pt]\text{All the 2nd partial derivatives of the bivariate} \\[3pt]\text{distribution of} \, (X_1, X_{k+1}) \, \text{for} \, k \geq 1, \, \text{are}\\[3pt]\text{bounded in a neighbourhood of} \, q_X(p)\end{array} \right. \quad \text{and}\qquad (S^{*}_{3}) : \left\{\begin{array}{l} \text{For} \, l=2,...,k:\\[4pt] S^{*}(p_l) \\[4pt] (C_1^{\prime}) (\text{see}\ ({\text{$C_{l}^{\prime}$}})) \, \text{at} \, q_X(p_l) \\[4pt] ({\text{$P$}}) \, \text{at} \, q_X(p_l)\end{array} \right.\end{equation*}

4. Comparing the Pro-Cyclicality of Risk Measures

We consider two different applications in this section. Both aim at further understanding the theoretically proven pro-cyclicality behaviour of the different risk measures in conjunction with the corresponding volatility estimators.

First, in Section 4.1, we evaluate empirically in a simulation study for light (Gaussian) and heavy-tailed distributions (Student-t distribution with 5 and 3 degrees of freedom) how well the finite sample results, as one encounters in practice, approximate the theoretical asymptotics.

Subsequently, in Section 4.2, we compare, for the same distributions and estimators as in Section 4.1, the strength of the theoretical correlation of the asymptotic distribution – thus comparing the existing degree of pro-cyclicality between the different risk measures.

4.1 Simulation study: finite sample performance

As in practice the estimation of risk measures occurs on a finite sample (usually a sample of 1 year of data which corresponds to 252 data points), we want to assess the finite sample performance, in view of the asymptotic results obtained in Theorem 1. When working with data, we estimate the risk measure and volatility estimators on finite samples of size n. To subsequently evaluate the corresponding covariance and correlation empirically we need, say l, independent realisations of these risk measure and realised volatility estimators.

To assess the finite sample performance, we conduct a simulation study following a similar but more general setup than in Section 4.1 of Bräutigam et al. (Reference Bräutigam, Dacorogna and Kratz2022). We simulate an iid sample with, e.g. mean $\mu=0$ and variance $\sigma^2 =1$ , from three different distributions each: Either a Gaussian distribution or Student t distributions with 3 and 5 degrees of freedom, respectively. The sample is of varying size $n \times l$ . It is determined by the fact that we use different sample sizes n for the estimation of either the risk measure or volatility, with $n=126,252,504, 1,008$ (being multiples or fractions of 1 year of data, i.e. 252 working days/data points), and different lengths l corresponding to the independent realisations of the risk measure or realised volatility estimator to estimate the sample correlation of interest.

Taking the example of risk levels relevant in practice (this means $p=0.99$ for the VaR and $p=0.975$ for the ES in the standard Basel regulation; for the expectile, it has been suggested in Bellini & Di Bernardino (Reference Bellini and Di Bernardino2017) to consider $p=0.99855$ ), we consider $p=0.95, 0.975,0.99, 0.99855$ . For each risk level, we compute l independent realisations of each risk measure estimator $(\zeta_{n,k}^{(j)}(p))_{k=1,...,l}, j=1,2,3,4$ on disjoint samples and, accordingly, l realisations of the realised volatility estimator $(\hat{m}(X,n,r))_{k})_{k=1,...,l}, r=1,2$ , i.e. focussing on the standard deviation and MAD for the latter.

We then estimate $\textrm{Cor}\left(\log \left\lvert \frac{\zeta_{n/2,\, t+n/2}^{(j)}(p)}{\zeta_{n/2,\, t}^{(j)}(p)} \right \rvert , \hat{m}(X,n/2, \, r, \,t) \right), j=1,2,3,4, r=1,2$ by its sample correlation (denoted by $\widehat{\textrm{Cor}}$ ), using these l pairs of independent realisations of the estimators. This procedure is repeated 1,000-fold in each case. We report the averages of the 1,000-fold repetition with, into brackets, the corresponding empirical 95% confidence interval. Further, we provide as benchmark the theoretical value of the correlation in its asymptotic distribution, denoted as “( $n \rightarrow \infty$ )” in the last column. The explicit expressions in the case of a Gaussian or Student distribution of the correlation of the asymptotic distribution used to calculate the theoretical values in the tables can be derived from Theorem 1 (and can be found in Appendix B.1).

In this section, we study exemplarily the finite sample performance of the historical Expected Shortfall estimator as risk measure estimator and the MAD as realised volatility estimator. We focus on the approximation of the correlation of the asymptotic distribution by its sample correlation as a function of the sample size n and the three different distributions considered. As risk levels, we consider $p=0.95$ and $p=0.99$ . Thus, we fix the length of the sample correlation time series to $l=50$ (from simulations performed with different sample sizes, we saw that this is long enough for a good estimation of the correlation; see Appendix D).

The other cases, VaR, expectile as risk measures, standard deviation as realised volatility estimator and other risk levels, show a similar behaviour and can be found in the extensive appendix for the simulation studies (see Appendix D).

Thus, let us look at the results displayed in Table 1. First, we consider the risk level $p=0.95$ . For the three distributions, we see that a sample size of $n=126$ suffices to estimate on average the correlation of the asymptotic distribution well enough (with slightly less precision for heavier tailed distributions). For the higher risk level $p=0.99$ , one can observe that the convergence to the theoretical value is slower and a sample size of $n=126$ does not yield as accurate results as for $p=0.95$ . Nevertheless, considering a sample size frequently used in practice, $n=252$ , i.e. 1 year of data, gives a sufficiently accurate picture. Note also that the size of the empirical confidence intervals depend on the size of the sample correlation, here chosen to be $l=50$ (recall that the results for other values of l can be found in Appendix D). They are in line with what is to be expected for $l=50$ : To show this, we can build confidence intervals for the sample Pearson correlation coefficient around the theoretical value (using the classical variance-stabilising Fisher transform of the correlation coefficient for a bivariate normal distribution to compute the confidence intervals – see the original paper Fisher, Reference Fisher1921 or e.g. a standard encyclopedia entry Rodriguez, Reference Rodriguez, Kotz, Balakrishnan, Read, Vidakovic and Johnson1982).

Table 1.

Average values from a 1,000-fold repetition. Comparing the sample Pearson correlations of the log-ratio of the historical Expected Shortfall with the sample MAD, as a function of the sample size n on which the quantile is estimated (fixed length $l=50$ of the bivariate sample used to estimate the correlation). We consider the thresholds $p = 0.95, 0.99$ . Underlying samples are simulated from a Gaussian, Student(5) and Student(3) distributions. Average empirical values are written first (with empirical 95% confidence interval in brackets). The theoretical correlation value in the asymptotic distribution “( $n \rightarrow \infty$ )” are provided as benchmark in the last column.

4.2 Theoretical comparison

Having confirmed in the previous section the validity of the theoretical results in a sample size setting used in practice, we are interested in the following in comparing the degree of (theoretical) pro-cyclicality depending on the choice of volatility estimator, the risk measure (estimator), and the heavy-tailedness of the distribution. As for the simulation study, we consider underlying iid models and evaluate the degree of negative correlation in the asymptotic distribution of the log-ratio of risk measure estimators with measure of dispersion estimators, given in (13).

As risk measure estimators, we consider the VaR estimator $\widehat{\textrm{VaR}}_n (p)$ , the expectile estimator $\hat{e}_n(p)$ , and three ES estimators, $\widetilde{\textrm{ES}}_{n,4}, \widetilde{\textrm{ES}}_{n,50}$ and $\widetilde{\textrm{ES}}_{n, \infty}$ (= $\widehat{\textrm{ES}}_n$ ). As in the simulation study, we focus on the sample MAD $\hat{m}(X,n,1)$ and the sample variance $\hat{m}(X,n,2)$ as they are the two most common realised volatility estimators.

As, from a risk management perspective, only large values for the risk level $p \in(0,1)$ are relevant, we focus on those cases. When considering the tail of the distribution, we choose the Gaussian distribution, ${\mathcal{N}} (0,1)$ , for its light tail, and, for heavy tailed distributions, the Student-t ones with varying degrees of freedom $\nu$ ( $\nu=3,4,5,10,50$ ) but always normalised to have mean 0 and variance 1.

The closed form solutions for the degree of pro-cyclicality in the aforementioned cases follow from Theorem 1 and its corresponding bivariate CLT’s, and can be found in Appendix B.1. Here, we focus on visualising the solutions and comparing them.

Gaussian Distribution. In Figure 1, we plot the correlations in the asymptotic distribution of the different risk measure estimators with the sample standard deviation (left) and the sample MAD (right), respectively.

Figure 1

Gaussian case. Pro-cyclicality as defined in (13), considering on each plot three different risk measures (VaR, ES, evaluated in three possible ways, and expectile) for a risk level higher than 80%. On the left with the standard deviation, on the right with the sample MAD.

Observing the different plots, we can make the following claims on the pro-cyclicality behaviour for the Gaussian distribution (as an example of a light-tailed distribution).

We observe a switch of behaviour in the tail. The degree of pro-cyclicality for tail values for different risk measures has a turning point in the tail in which the ordering is reversed. For quantile values below the turning point, the ES exhibits the highest pro-cyclicality, then the VaR and then the expectile. After the turning point, this exact ordering is reversed. The choice of dispersion measure has no real impact in this case, as the behaviour looks similar with MAD and variance. The ordering of the different risk measures with respect to pro-cyclicality is the same for MAD and variance – also roughly their magnitude of pro-cyclicality. What differs is the location of the turning point: It is further in the tail with the variance (around $0.97$ ) than with MAD (around $0.92$ ). Considering VaR and ES, the values of the correlation are very similar after the turning point, while before, the pro-cyclicality for ES can be markedly (depending on the estimation method) higher than for VaR. From the plots it is also clear that the expectile, with the estimation method used, has the highest degree of pro-cyclicality in the far tail. It could be tested if this observation remains true when taking another method to estimate the expectile. We do not do it here, since the expectile is not yet a risk measure used in practice.

Student t Distribution. By considering the Student t distribution, we are interested in understanding how the observed behaviour may change with heavy-tailed distributions. Exemplary, we consider the case $\nu=5$ in Figure 2 since we need $\nu >4$ for $(M_2)$ (see (M _k )) to hold. However, in Appendix B (see Figure 1), we include an analysis when looking at different degrees of freedom ( $\nu=3,4,5,10,40$ ), investigating how the correlations change as a function of $\nu$ , also comparing them with the Gaussian limiting case.

In Figure 2, we observe that, for this heavy-tailed distribution, the correlation behaviour depends on the dispersion measure considered. Indeed, in contrast to the Gaussian case, the existence of the turning points depends on whether we use the sample variance or the MAD: It does not exist with the sample variance, but appears with the MAD (as for the Gaussian distribution) – with the location of the turning point having shifted further into the tail. Moreover, the degree of pro-cyclicality for the VaR and ES is very different when choosing the variance, whereas for the MAD (where the turning point still exists as in the Gaussian case), the tail behaviour is similar for both risk measures. For the expectile, the correlation behaviour is similar as in the Gaussian case, except in the extreme case when the quantile level p tends to 1: in such a case, the correlation does not tend to 0 but to a non-zero value, for both measures of dispersion. Moreover, the pro-cyclicality is the highest in the far tail for the sample MAD (right plots), as in the Gaussian case, but not anymore for the sample variance.

Figure 2

Case of a Student-t distribution with 5 degrees of freedom. Pro-cyclicality as defined in (13), (VaR, ES, evaluated in three possible ways, and expectile) quantified for a risk level higher than 80%. On the left with the standard deviation, on the right with the sample MAD.

Implications of the pro-cyclicality for the choice of risk measure. Let us end the comparison of the pro-cyclicality in Gaussian and Student iid models for the different risk measures by commenting on its implications for the choice of risk measure.

From the observations made on the figures, we have seen that the pro-cyclicality behaviour depends on the choice of the underlying risk measure, the dispersion measure, and also on the type of tail distribution. But, as already proven through Theorem 1, pro-cyclicality is inherent to and present (to a significant degree) with all risk measures due to the method of estimation, namely the historical estimation.

5. A Case Study on Real Data

In this part, we want to go one step beyond the illustration of the pro-cyclicality in the iid case and check about the effect of pro-cyclicality when considering real data. We want to use the results of Theorem 1 to statistically verify the empirical claims on the causes of pro-cyclicality. Namely, that the pro-cyclicality observed is partly from an intrinsic effect of using the method of historical estimation and partly due to the clustering and return-to-the-mean behaviour of volatility, as modeled with a GARCH(1, 1), for any risk and dispersion measures.

We could compute the theoretical pro-cyclicality value for a GARCH(1, 1) process given in Theorem 1 and compare it with the value obtained for the real data. But we do not have closed form solutions of the correlation of the asymptotic distribution for this family of models. Further, it is known that, for GARCH processes, the convergence to its asymptotic distribution is slow (as argued e.g. in Mikosch & Stărică (Reference Mikosch and Stărică2000) for the autocovariance/autocorrelation process). Hence, we consider the alternative and easier way suggested in Bräutigam et al. (Reference Bräutigam, Dacorogna and Kratz2022) for the VaR case: Instead of analysing the theoretical correlation for a GARCH model, we analyse the residuals of a GARCH(1, 1) fitted to the data, then the pro-cyclicality for this residual process.

Pro-cyclicality Analysis of Residuals. To start with, recall the GARCH(1,1) model:

$$ X_{t+1} = \epsilon_t\,\sigma_t,\quad \text{with} \, \sigma_t^2 = \omega + \alpha \, X_t^2 + \beta \sigma_{t-1}^2 \;\text{and}\, \omega>0, \alpha \geq 0, \beta \geq 0,$$

where $\left( \epsilon_t, t \in \mathbb{Z} \right)$ is an iid series with mean 0 and variance 1.

As in Bräutigam et al. (Reference Bräutigam, Dacorogna and Kratz2022) and Bräutigam (Reference Bräutigam2020), we consider 11 stock indices. The data used are the daily closing prices from Friday, January 2, 1987 to Friday, September 28, 2018 (detailed information about the countries and indices used can be found in Appendix C.1, Table 3). As measure of dispersion we choose the MAD. An important motivation for choosing the MAD over the variance as measure of dispersion is that it implies weaker conditions on the moments of the underlying distribution (recall Theorem 1).

For each of the 11 indices, we initialise $\hat{\sigma}_t$ by using 1 year of data (as “burn-in” sample) using the fitted GARCH parameters (see Table 4 in Appendix C.1 for details). This enables us to consider the time series of empirical residuals $\hat{\epsilon}_t \,{:\!=}\, X_{t+1} / \hat{\sigma}_t$ .

Then, to assess the pro-cyclicality for these residuals, we compute the sample correlation between the logarithm of the look-forward ratio and the sample MAD, recall (13) – but here, on the time series of residuals $\hat{\epsilon}_t$ (and not the real data itself!). In theory, this time series of residuals should be iid with mean 0 and variance 1. Hence, we can exactly assess the pro-cyclicality (i.e. the degree of negative correlation in the asymptotic distribution of the logarithm of the look-forward ratio and the MAD) for iid models, by applying Theorem 1 (for the iid case, i.e. under milder conditions than what would be needed for the GARCH).

To compare the sample correlation (based on a finite sample of about 300) with the theoretical asymptotic value of the correlation, we provide the corresponding confidence intervals for the sample Pearson linear correlation coefficient (for details, see Appendix C.2). Note that they are computed assuming a bivariate normal sample, although the bivariate normality of the logarithm of the look-forward ratio with the sample MAD holds only asymptotically. But, from preliminary simulation results, we observed that, for such a sample size, the empirical and theoretical confidence intervals for underlying Gaussian and Student samples are similar. Thus, we feel confident in providing those theoretical confidence intervals as approximate guidance. We then verify if the sample correlation based on the residuals falls in these iid confidence intervals and how the sample correlation based on the real data behaves in comparison (the corresponding raw values, i.e. the pro-cyclicality values for the 11 stock indices, can be found in Appendix C.1).

In the theoretical results, we have considered three different risk measures (VaR, ES, and expectile) and in the application for the iid case (Section 4) have looked at five different risk measure estimators. Here, dealing with an empirical setup, we restrict ourselves to the two risk measures that are effectively used in practice, VaR and ES, and their simplest form of estimation $\widehat{\textrm{VaR}}_n (p)$ and $\widetilde{\textrm{ES}}_{n, \infty}$ ( $=\widehat{\textrm{ES}}_n$ ). Note that, for completeness and to allow for comparison with ES, we include the case of the VaR already studied in Bräutigam et al. (Reference Bräutigam, Dacorogna and Kratz2022).

For each risk measure, we consider the results on each of the 11 indices, using one plot per index. In those plots, we compare for four thresholds $p = 0.95,0.975,0.99,0.995$ , the measured pro-cyclicality (i.e. the sample correlation between the log-ratio of the VaR or ES estimators, respectively, and the sample MAD) on the real data versus the one on the residuals. Further, 95%-confidence intervals for a sample correlation assuming an underlying white noise process are given – considering as alternatives a Gaussian or Student distribution, the latter with varying degrees of freedom, $\nu =4,...,7$ . In Figure 3, we consider, exemplarily, the S&P 500 and the FTSE index for the VaR and ES, respectively. The totality of the 22 plots are to be found in Appendix C.3 in Figures 2 and 3. Considering the VaR (in the first row of Figure 3), we observe that for the FTSE the pro-cyclicality value for the residuals is always in the confidence interval, whereas for the S&P 500 only two out of four times. For the ES in the second row, it is in all cases for both indices in the iid confidence interval.

Figure 3

Comparison of pro-cyclicality for the real data (blank circle) with the pro-cyclicality for the GARCH(1, 1)-residuals (filled circle), considering the S& P500 (on the left) and the FTSE (on the right). The first row considers the VaR as risk measure (estimator $\widehat{\textrm{VaR}}_{n}(p)$ ), the second row the ES (estimator $\widetilde{\textrm{ES}}_{n, \infty}$ ). Each plot contains the correlation for the four different quantile values p. For each of them, corresponding theoretical confidence intervals (for the sample correlation) assuming a specific underlying distribution (Gaussian or Student with different degrees of freedom) are plotted.

Considering all indices in the case of the ES (Figure 3 in Appendix C.3), in 37 out of 44 cases (84%), the sample correlation of the real data falls in the 95% confidence interval of the sample correlation of iid rv’s, while it is in 38 out of 44 cases (86%) for the VaR (see Figure 2 in Appendix C.3). Moreover, for exactly 1 out of 44 cases for ES and none for VaR, the sample correlation of the real data falls in these confidence intervals.

Thus, the same conclusion holds for ES as for VaR: We are left with a pro-cyclicality behaviour for the residuals like for iid data.

6. Conclusion

In this study, we investigated the pro-cyclicality of historical risk estimation considering popular quantile-based risk measures, using the methodology set in Bräutigam et al. (Reference Bräutigam, Dacorogna and Kratz2022), based on the joint behaviour of the look-forward ratio and the realised volatility. We extended the results obtained for the VaR in Bräutigam et al. (Reference Bräutigam, Dacorogna and Kratz2022) by considering ES and expectile and different realised volatility estimators for characterising the market states. The main theoretical result consists in establishing the joint asymptotic normality between the logarithm of the look-forward ratio (defined in terms of risk measures estimators) and dispersion measures estimators. By this, we are able to quantify the pro-cyclicality by the degree of negative dependence between the components of this distribution.

As the result reveals a negative correlation, it shows that pro-cyclicality exists, whatever the quantile-based risk measure, VaR, ES, or expectile, whether we consider a conditional or unconditional approach, and whatever the choice of dispersion measure to estimate the volatility.

To test the relevance of the theoretical results on finite samples, we undertake extensive simulation studies in the iid case. The results show in all cases a good approximation of the asymptotic negative dependence by the finite sample counterpart, highlighting the applicability of such asymptotic theorem. Using the corresponding closed-form solutions based on the theorem, we then compare the impact of choices of quantile-based risk measures and dispersion measures on the degree of pro-cyclicality, also taking into account the fatness of the tail of the underlying distribution.

Finally, in a case study on real data, we verify that historical risk measurements indeed lead to pro-cyclicality, irrespectively of the choice of quantile-based risk measures and dispersion measures, but also irrespectively of the choice of conditional versus unconditional approaches for historical risk estimation.

While we focused on the impact of historical estimation on pro-cyclicality, further research could be done when considering other risk estimation methods, with different (parametric or not) models, as e.g. (GARCH-)EVT one. Other popular stochastic processes for modelling financial returns (like e.g. ARMA-GARCH) could be included in the framework by extending the class of processes currently considered; related theoretical work on the topic developed for a broader class of augmented GARCH processes (Bräutigam & Kratz, Reference Bräutigam and Kratz2021) could be used as a starting point.

This work lays the ground for tackling pro-cyclicality at its root, namely the way risk is measured, rather than resorting to operational means as e.g. the transitional measures of Solvency 2 that temper with economic valuation. Our study opens the door for finding new direct ways to mitigate pro-cyclicality. Such a mitigation is sought after by risk managers and regulators, and our conclusions should help building a counter-cyclical risk measure, or at least a risk measure that limits the pro-cyclicality. This is what we are currently investigating.