1. Introduction
Elegant mathematical analysis of the classical Cramér–Lundberg risk model has a prominent place in nonlife insurance theory. The theory yields precise or approximate computations of ruin probabilities, appropriate reserves, distribution of the total claim amount, and other properties of an idealized insurance portfolio; see, for instance, Asmussen and Albrecher (Reference Asmussen and Albrecher2010) or Mikosch (Reference Mikosch2009). In recent years, some special models have been proposed to account for the possibility of clustering of insurance events. For instance, in the context of Hawkes processes, some results on ruin probabilities can be found in Stabile and Torrisi (Reference Stabile and Torrisi2010) and Zhu (Reference Zhu2013). General cluster point processes and Poisson cluster processes in particular have proved useful in a variety of fields when modelling events that cluster in either space or time. This includes seismology, telecommunications, forensic science, molecular biology, and finance; we refer the reader to Section 6.4 of Daley and Vere Jones (Reference Daley and Vere-Jones2003) for some examples.
The main goal of this article is to study the asymptotic distribution of the total claim amount in the setting where the Cramér–Lundberg risk model is augmented with a Poisson cluster structure. To make this more precise, we model the arrival of claims in an insurance portfolio by a marked point process, say
where the
$$\tau_k$$ are nonnegative random variables representing arrival times with some degree of clustering and the
$$A^k$$ represent corresponding marks in a rather general metric space
$$\mathbb{S}$$. Observe that we do allow for the possibility that marks influence the arrival rate of future claims. In the language of point processes theory, we assume that the marks are merely unpredictable and not independent of the arrival times (Daley and Vere Jones (Reference Daley and Vere-Jones2003)). For each marked event, the claim size can be calculated using a measurable mapping of marks to nonnegative real numbers,
$$f(A^k)$$ say. So the total claim amount in the time interval [0, t] can be calculated as
In the sequel we aim to determine the effect of the clustering on the quantity S(t) as
$$t{\to\infty}$$
even in the case when the distribution of the individual claims does not satisfy assumptions of the classical central limit theorem. The paper is organized as follows. In Section 2 we rigorously introduce the marked Poisson cluster model and present some specific cluster modes which have attracted attention in the related literature; see Faÿ et al. Reference Faÿ, González-Arévalo, Mikosch and Samorodnitsky(2006), Stabile and Torrisi (Reference Stabile and Torrisi2010), and Karabash and Zhu (Reference Karabash and Zhu2015). As a proposition in Section 3 we present the central limit theorem for the total claim amount S(t) in our setting under appropriate second moment conditions. In Section 4 we prove a functional limit theorem concerning the sums of regularly varying nonnegative random variables when subordinated to an independent renewal process. Based on this, we prove the limit theorem for the total claim amount S(t) in cases when individual claims have infinite variance. Finally, in Section 5 we apply our results to the models we introduced in Section 2. In particular, we give a detailed analysis of the asymptotic behaviour of S(t) for marked Hawkes processes which have been extensively studied in recent years.
2. The general marked Poisson cluster model
Consider an independently marked homogeneous Poisson point process with mean measure (vLeb) on the state space
$$[0,\infty)$$
for some constant
$$\nu {\,>\,}0$$
, where Leb denotes the Lebesgue measure on
$$[0,\infty)$$
, with marks in a completely metrizable separable space
$$\mathbb{S}$$
,
The marks
$$A_i$$
are assumed to follow a common distribution Q on a measurable space
$$(\mathbb{S}, \mathscr{s})$$
, where
$$\mathscr{s}$$
denotes a corresponding Borel
$$\sigma$$
-algebra. In other words,
$$N^0$$
is a Poisson point process with intensity
$$\nu \times Q$$
on the space
$$[0,\infty) \times
\mathbb{S}$$
. For nonlife insurance modelling purposes, the marks can take values in
$${\mathbb{R}}^d$$
with coordinates representing the size of the claim, the claim type, the severity of the accident, etc.
Denote the space of locally finite point measures on this space by
$$M_p=
M_p ( [0,\infty) \times \mathbb{S})$$
, and assume that at each time
$${\Gamma_i}$$
with mark
$$A_i$$
another point process in
$$M_p $$
is generated independently, which we denote by
$$G^{A_i}$$
. Intuitively,
$$G^{A_i}$$
represents a cluster of points that is superimposed on
$$N^0$$
after time
$$
{\Gamma_i}$$
. Formally, there exists a probability kernel K, from
$$\mathbb{S}$$
to
$$M_p$$
, such that, conditionally on
$$N^0,$$
point processes
$$G^{A_i}$$
are independent and almost-surely (a.s.) finite, with distribution
$$K(A_i,\cdot)$$
; thus, dependence between the
$$G^{A_i}$$
and
$$A_i$$
is permitted. Based on
$$N^0$$
and clusters
$$G^{A_i}$$
we define a cluster Poisson process.
In order to keep the track of the cluster structure, we can alternatively consider the process
$$G^{A_i}$$
as a part of the mark attached to
$$N^0$$
at time
$$ {\Gamma_i}$$
. Indeed,
can be viewed as a marked Poisson process on
$$[0,\infty)$$
with marks in the space
$$ \mathbb{S} \times M_p$$
. We can write
\begin{equation*}
G^{A_i} = \sum_{j= 1}^{K_i} \delta_{T_{ij},\,A_{ij}},
\end{equation*}
where
$${(T_{ij})}_{j\geq 1}$$
is a sequence of nonnegative random variables and
$$K_i$$
is an
$$\mathbb{N}_0$$
-valued random variable. If we count the original point arriving at time
$${\Gamma_i}$$
, the actual cluster size is
$$K_i+1$$
. Furthermore, for any original arrival point
$${\Gamma_i}$$
and corresponding random cluster
$$G^{A_i}$$
, we introduce a point process
Note that
$$K_i$$
may possibly depend on
$$A_i$$
, but we do assume throughout that
Finally, to describe the size and other characteristics of the claims together with their arrival times, we use a marked point process N as a random element in
$$M_p$$
of the form
\begin{equation}
N= \sum_{i=1}^\infty \sum_{j = 0}^{K_i} \delta_{ {\Gamma_i}+T_{ij},A_{ij}},
\label{eqn1}
\end{equation}
where we set
$$T_{i0} = 0$$
and
$$A_{i0} = A_i$$
. In this representation, the claims arriving at time
$$ {\Gamma_i}$$
and corresponding to the index
$$j=0$$
are called ancestral or immigrant claims, while the claims arriving at times
$$ {\Gamma_i}+T_{ij},\, j \geq 1$$
, are referred to as progeny or offspring. Moreover, since N is locally finite, we could also write
with
$$\tau_k\leq \tau_{k+1}$$
for all
$$k \geq 1$$
. Note that in this representation we ignore the information regarding the clusters of the point process. Clearly, if the cluster processes
$$G^{A_i}$$
are independently marked with the same mark distribution Q independent of
$$A_i$$
, then all the marks
$$A^k$$
are independent and identically distributed (i.i.d.).
The size of the claims is produced by an application of a measurable function, say
$$f\colon\mathbb{S} \to \mathbb{R}_+$$
, on the marks. In particular, the sum of all the claims due to the arrival of an immigrant claim at time
$$ {\Gamma_i}$$
equals
while the total claim size in the period [0, t] can be calculated as
Remark 2.1
In all our considerations, we take into account (without any real loss of generality) the original immigrant claims arriving at times
$${\Gamma_i}$$
as well. In principle, we could ignore these claims and treat
$${\Gamma_i}$$
as times of incidents that trigger, with a possible delay, a cluster of subsequent payments. Such a choice seems particularly useful if one aims to model the so-called incurred but not reported (IBNR) claims, when estimating appropriate reserves in an insurance portfolio (Mikosch (Reference Mikosch2009)). In such a case, in the definition of the process N, we would omit the points of the original Poisson process
$$N^0$$
and instead consider
\begin{equation*}
N= \sum_{i=1}^\infty \sum_{j = 1}^{K_i} \delta_{
{\Gamma_i}+T_{ij},A_{ij}}.
\end{equation*}
2.1 Some special models
Several examples of Poisson cluster processes have been studied in the monograph of Daley and Vere Jones (Reference Daley and Vere-Jones2003); see Example 6.3 therein for instance. Here we study the marked adaptation of Example 6.3(a)–(c) of Daley and Vere Jones (Reference Daley and Vere-Jones2003).
2.1.1 Mixed binomial Poisson cluster process
Assume that the clusters have the form
\begin{equation*}
G^{A_i} = \sum_{j=1}^{K_i} \delta_{W_{ij}, A_{ij}},
\end{equation*}
with
$$(K_i,(W_{ij})_{j\ge 1},(A_{ij})_{j\ge 0})_{i\ge 0}$$
being an i.i.d. sequence. Assume moreover that the
$$(A_{ij})_{j\ge 0}$$
are i.i.d. for any fixed
$$i=1,2,\ldots $$
and that
$$(A_{ij})_{j\ge1}$$
is independent of
$$K_i,(W_{ij})_{j\ge 1}$$
for all
$$i\ge 0$$
. We allow for possible dependence between
$$K_i,(W_{ij})_{j\ge 1}$$
and the ancestral mark
$$A_{i0}$$
; however, we assume that
$$K_i$$
and
$$(W_{ij})_{j\ge 1}$$
are conditionally independent given
$$A_{i0}$$
. As before, we assume that
$${\mathbb{E}}[K]{\lt}\infty$$
. Observe that we use the notation
$$W_{ij}$$
instead of
$$T_{ij}$$
to emphasize the relatively simple structure of clusters in this model in contrast with the other two models considered in this section. Such a process N is a version of the so-called Neyman–Scott process; see, e.g. Example 6.3(a) of Daley and Vere Jones (Reference Daley and Vere-Jones2003).
2.1.2 Renewal Poisson cluster process
Assume next that the clusters
$$G^{A_i}$$
have the distribution
\begin{equation*}
G^{A_i} = \sum_{j=1}^{K_i} \delta_{T_{ij}, A_{ij}},
\end{equation*}
where
$$(T_{ij})_j$$
represents a renewal sequence
and we keep all other assumptions from the model in Subsection 2.1.1 (in particular,
$$(W_{ij})_{j\ge 1}$$
are conditionally i.i.d. and independent of
$$K_i$$
given
$$A_{i0}$$
). A general unmarked model of this type is called the Bartlett-Lewis model and analysed in Example 6.3(b) of Daley and Vere Jones (Reference Daley and Vere-Jones2003). See also Faÿ et al. (Reference Faÿ, González-Arévalo, Mikosch and Samorodnitsky2006) for an application of such a point process to the modelling of teletraffic data.
These two simple cluster models were considered by Mikosch (Reference Mikosch2009) in the context of insurance applications. In particular, Subsection 11.3.2 and Example 11.3.5 therein provide expressions for the first two moments of the number of claims in a given time interval [0, t]. Both models can be criticized as overly simple, but the assumption that claims (or delayed payouts) are separated by i.i.d. times (as in the renewal Poisson cluster process) often appears in the risk theory (cf. the Sparre Andersen model; see Asmussen and Albrecher (Reference Asmussen and Albrecher2010)).
2.1.3 Marked Hawkes process
A key motivating example in our analysis is the so-called (linear) marked Hawkes process. Hawkes processes of this type have a neat Poisson cluster representation due to Hawkes and Oakes (Reference Hawkes and Oakes1974). For this model, the clusters
$$G^{A}$$
are a recursive aggregation of Cox processes, i.e. Poisson processes with random mean measure
$$ \tilde{\mu}_A \times Q$$
, where
$$ \tilde{\mu}_A $$
has the form
for some fertility (or self-exciting) function h; cf. Example 6.4(c) of Daley and Vere Jones (Reference Daley and Vere-Jones2003).
It is useful to introduce a time shift operator
$$\theta_t$$
as
for an arbitrary point measure
$$m = \sum_j \delta_{t_j,a_j} \in M_p$$
and
$$t\geq 0$$
. Now, for the ground process
$$N^0 \,{=}\, \sum_{i\geq 1}
\delta_{{\Gamma_i},A_i}$$
, which is a Poisson point process with intensity
$$\nu \times Q$$
on the space
$$[0,\infty) \times \mathbb{S}$$
, the cluster process corresponding to a point
$$( \Gamma,A)$$
satisfies the recursive relation
\begin{equation}
G^A = \sum_{l=1}^{{L_A}} ( {\delta_{\tau^1_l,A^1_l} } +\theta_{\tau^1_l}
G^{A^1_l} ),
\label{eqn4}
\end{equation}
where, given A,
$$N^A = \sum_{l=1}^{{L_A}} \delta_{\tau^1_l,A^1_l}$$
is a Poisson processes with random mean measure
$$ \tilde{\mu}_A \times Q,$$
and the sequence
$$(G^{A^1_l})_l$$
is i.i.d., distributed as
$$G^A$$
and independent of
$$N^A$$
. Thus, at any ancestral point
$$(\Gamma,A)$$
a cluster of points appears as a whole cascade of points to the right in time generated recursively according to (2.4). Note that, by definition,
$$L_A$$
has Poisson distribution conditionally on A, with mean
$$\kappa_A=\int_0^\infty h(s,A) \,\mathrm{d} s$$
. It corresponds to the number of first-generation progeny
$$(A^1_l)$$
in the cascade. Note also that the point processes forming the second generation are again Poisson conditionally on the corresponding first generation mark
$$A_l^1$$
. The cascade
$$G^A$$
corresponds to the process formed by the successive generations, drawn recursively as Poisson processes given the former generation.
The marked Hawkes process is obtained by attaching to the ancestors
$$({\Gamma_i},A_{i})$$
of the marked Poisson process
$$ N^0 = \sum_{i\geq 1}
\delta_{ {\Gamma_i},A_i} $$
a cluster of points, denoted by
$$C_i$$
, which contains the point
$$(0,A_{i})$$
and a whole cascade
$$G^{A_i}$$
of points to the right in time generated recursively according to (2.4) given
$$A_i$$
. Under the assumption that
the total number of points in a cluster is generated by a subcritical branching process. Therefore, the clusters are finite a.s., and we denote their size by
$$K_i {+1}= C_i[0,\infty)$$
. It is known and not difficult to show that, under (2.5), the clusters always satisfy
Observe that the clusters
$$C_i$$
are independent by construction and can be represented as
$${C_i} = \sum\limits_{j = 0}^{{K_i}} {{\delta _\Gamma }_i + {T_{ij}},Aij} $$
with the
$$A_{ij}$$
being i.i.d. and
$$T_{i0} = 0$$
. We note that in the case when marks do not influence the conditional density, i.e. when
$$h(s,a) =
h(s)$$
, the random variable
$$K_i{+1}$$
has a so-called Borel distribution with parameter
$$\kappa$$
; see Haight and Breuer (Reference Haight and Breuer1960). Observe also that, in general, marks and arrival times of the final Hawkes process N are not independent of each other, rather, in the terminology of Daley and Vere Jones (Reference Daley and Vere-Jones2003), the marks in the process N are only unpredictable.
Hawkes processes are typically introduced through their conditional intensity. More precisely, a point process
$$ N = \sum_{k}
\delta_{\tau_k,A^k}$$
represents a Hawkes process of this type if the random marks
$$(A^k)$$
are i.i.d. with distribution Q on the space
$$\mathbb{S}$$
, while the arrivals
$$(\tau_k)$$
have conditional intensity of the form
where
$$\nu {\gt} 0$$
is a constant and
$$h\colon[0,\infty)\times \mathbb{S}\to
\mathbb{R}_+$$
is assumed to be integrable in the sense that
$$\int_0^\infty
{\mathbb{E}} h(s,A) \,\mathrm{d} s {\lt} \infty$$
. Observe that
$$\nu$$
is exactly the constant which determines the intensity of the underlying Poisson process
$$N^0$$
due to the Poisson cluster representation of the linear Hawkes processes; cf. Hawkes and Oakes (Reference Hawkes and Oakes1974). Observe that
$$\lambda$$
is
$$\mathscr{f}_t$$
-predictable, where
$$\mathscr{f}_t$$
stands for an internal history of N,
$$\mathscr{f}_t = \sigma\{N(I \times S)\colon I \in
\mathscr{b}(\mathbb{R}),\, I \subset ({-}\,\infty, t],\, S \in \mathscr{s}\}$$
. Moreover, the
$$A^n$$
are assumed to be independent of the past arrival times
$$\tau_i,\,i {\lt} n$$
; see also Bràaud (Reference Brémaud1981). Writing
$$N_t = N((0,t] \times
\mathbb{S})$$
we can observe that
$$(N_t)$$
is an integer-valued process with nondecreasing paths. The role of intensity can be described heuristically by the relation
2.1.4 Stationary version
In any of the three examples above, the point process N can be clearly made stationary if we start the construction in (2.1) on the state space
$${\mathbb{R}} \times \mathbb{S}$$
with a Poisson process
$$
\sum_i \delta_{{\Gamma_i}}$$
on the whole real line. The resulting stationary cluster process is denoted by
$$N^*$$
. However, from an applied perspective, it seems more interesting to study the nonstationary version where both the ground process
$$N^0$$
and the cluster process itself have arrivals only from some point onwards, e.g. in the interval
$$[0,\infty)$$
as, for instance, in Karabash and Zhu (Reference Karabash and Zhu2015).
The stability of various cluster models, i.e. the convergence towards a stationary distribution in an appropriate sense, has been extensively studied for various point processes. For instance, it is known that the unmarked Hawkes process on
$$[0,\infty)$$
converges to the stationary version on any compact set and on the positive line under the condition that
see Daley and Vere Jones (2003, p. 232). Using the method of Poisson embedding, originally due to Kerstan (Reference Kerstan1964), Brémaud and Massoulié (Reference Brémaud and Massoulié1996, Section 3) obtained general results on the stability of Hawkes processes, even in the nonlinear case.
3 Central limit theorem
As explained in Section 2, the total claim amount for claims arriving before time t can be written as
The long term behavior of S(t) for general marked Poisson cluster processes is the main goal of our study. As before, by Q we denote the probability distribution of marks on the space
$$\mathbb{S}$$
. Moreover, unless stated otherwise, we assume that the process starts from 0 at time
$$t=0$$
, that is,
$$N ({-}\,\infty, 0] = 0$$
.
In the case of the Hawkes process, the process
$$N_t = N([0,t] \times
\mathbb{S}) ,\, t \geq 0$$
, which counts only the arrival of claims until time t has been studied in the literature before. It was shown recently, under appropriate moment conditions, that in the unmarked case multitype Hawkes processes satisfy the (functional) central limit theorem; see Bacry et al. (Reference Bacry, Delattre, Hoffmann and Muzy2013). Karabash and Zhu (Reference Karabash and Zhu2015) showed that
$$N_t$$
satisfies the central limit theorem even in the more general case of the nonlinear Hawkes process and that linear but marked Hawkes have the same property. In the present section we describe the asymptotic behaviour of the total claim amount process (S(t)) for a wide class of marked Poisson cluster processes, even in the case when the total claim process has heavy tails, and potentially infinite variance or infinite mean.
It is useful in the sequel to introduce the random variable
Recall from (2.2) the definition of
$$D_i$$
as
\begin{equation*}
D_i = \int_{[0,\infty)\times \mathbb{S}} f(u) C_i (\mathrm{d} s,\!\,\mathrm{d} u) =
\sum_{j=0}^{K_i} \,f(A_{ij}) = \sum_{j=0}^{K_i} X_{ij} ,
\end{equation*}
where
$$K_i+1 = C_i[0,\infty)$$
denotes the size of the ith cluster and where we let
$$X_{ij} = \,f(A_{ij})$$
. As before,
$$D_i$$
has an interpretation as the total claim amount coming from the ith immigrant and its progeny. Note that the
$$D_i$$
form an i.i.d. sequence because the ancestral mark in every cluster comes from an independently marked homogeneous Poisson point process.
Observe that in the nonstationary case we can write
\begin{equation}
S(t) = \sum_{i=1}^{\tau(t)} D_i
- D_{\tau(t)} - {\varepsilon}_t,\qquad t \geq 0,
\label{eqn7}
\end{equation}
where the last error term represents the leftover or the residue at time t, i.e. the sum of all the claims arriving after t which belong to the progeny of immigrants arriving before time t, that is
Clearly, in order to characterize the limiting behaviour of S(t), it is useful to determine moments and the tail behaviour of the random variables
$$D_i$$
for each individual cluster model. To simplify the notation, for a generic member of an identically distributed sequence or an array, say
$$(D_n)$$
,
$$(A_{ij})$$
, we write
$$D,\, A\,$$
etc. Under the conditions of existence of second-order moments and the behavior of the residue term
$${\varepsilon}_t$$
, it is not difficult to derive the following proposition.
Proposition 3.1
Consider the marked Poisson cluster model defined in Section 2. Suppose that
$${\mathbb{E}} D^2 {\lt}\infty$$
and that
$${\varepsilon}_t = o_P(\sqrt{t})$$
. Then, for
$$t{\to\infty}$$
,
where
$$\mu_D = {\mathbb{E}} D$$
.
Proof. Denote the first term on the right-hand side of (3.1) by
\begin{equation*}
S^D(t) = \sum_{i=1}^{\tau(t)} D_i, \qquad t \geq 0.
\end{equation*}
An application of the central limit theorem for two-dimensional random walks (see Gut (2009, Section 4.2, Theorem 2.3)) yields
Since we assumed that
$${{\varepsilon}_{t}}/{\sqrt t} \xrightarrow{{\mathbb{P}\ }} 0$$
, it remains to show that
However, this follows at once from Gut (2009, Theorem 1.2.3) for instance, or from the fact that in this setting the sequences
$$({\Gamma_n})$$
and
$$(D_n)$$
are independent.
Note that (3.1) holds for f taking possibly negative values as well. However, when modelling insurance claims, the nonnegativity assumption seems completely natural, and in the heavy-tail case our proofs actually depend on it; cf. the proof of Theorem 4.1. In the special case
$$f\equiv 1$$
, we obtain the central limit theorem for the number of arrivals in the time interval [0, t]. Related results have previously appeared in the literature; see, for instance, Daley (Reference Daley1972) or Karabash and Zhu (Reference Karabash and Zhu2015). The short proof above stems from the classical Anscombe theorem, as presented in Gut (2009, Chapter IV) (cf. Daley (1972, Theorem 3(ii))), unlike the argument in Karabash and Zhu (Reference Karabash and Zhu2015) which relies on the martingale central limit theorem and does not seem to be easily extendible, especially for the heavy-tailed claims we consider next.
Remark 3.1
It is not too difficult to find examples where the residue term is not negligible. Consider the renewal cluster model of Subsection 2.1.2 with
$$K=1$$
and
$$X=1$$
. Let the
$$W_{i1}$$
be i.i.d. and regularly varying with index
$$\alpha {\lt} \tfrac12.$$
Then
$$\varepsilon_t$$
has Poisson distribution with parameter
$${\mathbb{E}} [W {{\bf 1}}_{\{W{\lt}t\}}]
{\to\infty} $$
and, thus, by Karamata’s theorem,
$${\varepsilon_t}/{\sqrt{t}}$$
tends to infinity in probability. Similarly, we can show that
$$\mathop{\rm var}\nolimits\,({\varepsilon_t}/{\sqrt{t}})={\mathbb{E}} [W {{\bf
1}}_ {\{W{\lt}t\}}]/t\to 0$$
so that
$$(\varepsilon_t-{\mathbb{E}} [W {{\bf 1}}_
{\{W{\lt}t\}}])/\sqrt t$$
tends to 0 in probability. Thus, 3.2 no longer holds, and instead we have
4 Infinite-variance stable limit
It is known that if the claims are sufficiently heavy tailed, properly scaled, and centred, sums S(t) may converge to an infinite variance stable random variable. In the case of random sums
$$S_n= X_1+\cdots +X_n$$
of i.i.d. random variables, the corresponding statement is true if and only if the claims are regularly varying with index
$$\alpha\in (0,2)$$
. For the Cramér–Lundberg model, i.e. when
$$N=N_0$$
, with i.i.d. regularly varying claims of index
$$\alpha \in (1,2)$$
, the corresponding limit theorem follows from Theorem 4.4.3 of Gut (Reference Gut2009). A crucial step in the investigation of the heavy-tailed case is to determine the tail behaviour of the random variables of (2.2).
For regularly varying
$$D_i$$
with index
$$\alpha \in (1,2)$$
, the limit theory for two-dimensional random walks in Section 4.2 of Gut (Reference Gut2009) still applies. Note that if we can show that the
$$D_i$$
have regularly varying distribution then there exists a sequence
$$(a_n),\, a_n {\to\infty}$$
, such that
and an
$$\alpha$$
-stable random variable
$$G_\alpha$$
such that
$${S^D_n} =
D_1+\cdots +D_n$$
as
$$n\to\infty$$
satisfies
where
$$\mu_D = {\mathbb{E}} D_i$$
. It is also known that the sequence
$$(a_n)$$
is regularly varying itself with index
$$1/\alpha$$
; see Resnick (Reference Resnick1987). In the sequel, we also set
$$a_t = a_{\lfloor t \rfloor }$$
for any
$$t \geq 1$$
.
4.1 Case
$$\alpha \in (1,2)$$
In this case the arguments of the previous section can be adopted to show the following result.
Proposition 4.1
Consider the marked Poisson cluster model introduced in Section 2. Suppose that the
$$D_i$$
are regularly varying with index
$$\alpha \in (1,2)$$
and that
$${\varepsilon}_t = o_P(a_{t}) $$
. Then there exists an
$$\alpha$$
-stable random variable
$$G_\alpha$$
such that, for
$$\mu_D = {\mathbb{E}} D_i$$
,
Proof. The proof again follows from (3.1) by an application of Theorem 4.2.6 of Gut (Reference Gut2009) on the random walks
$$(\Gamma_n)$$
and
$$(S^D_n)$$
together with (4.1). By assumption, we have
$${\varepsilon}_t/a_{\nu
t}\sim \nu^{-1/\alpha} {\varepsilon}_t /a_t {\xrightarrow{{\mathbb{P}\ }}} 0$$
. To complete the proof, we observe that the sequences
$$({\Gamma_n})$$
and
$$(D_n)$$
are independent; hence,
4.2 Case
$$\alpha \in (0,1)$$
In this case we were not able to find any result of Anscombe’s theorem type for two-dimensional random walks of the type used above. Therefore, as our initial step, we prove a theorem which we believe is new and of independent interest. It concerns partial sums of i.i.d. nonnegative regularly varying random variables, say
$$(Y_n)$$
, subordinated to an independent renewal process. More precisely, set
$$V_n= Y_1+\cdots + Y_n,\,
n\geq 1$$
. Suppose that the sequence
$$(Y_n)$$
is independent of another i.i.d. sequence of nonnegative and nontrivial random variables
$$(W_n)$$
. Denote by
the corresponding renewal process, where we set
$$\sup \varnothing = 0$$
. Recall that, for regularly varying random variables
$$Y_i$$
, there exists a sequence
$$(a_n)$$
such that
$$n {\mathbb{P}} (Y_i{\gt}a_n) \to 1$$
as
$$n
{\to\infty}$$
. The limiting behaviour of the process
$$V_{\sigma(t)}$$
was considered by Anderson (Reference Anderson1988) in the case where the
$$W_i$$
are themselves regularly varying with index
$$\leq 1.$$
Since
$${\sigma(t)}/{t} {\xrightarrow{\text{a.s.}}} \nu,$$
if
$$0{\lt}{\mathbb{E}} W_i = {1}/{\nu} {\lt} \infty,$$
we may expect that
$$V_{\sigma(t)}$$
has similar asymptotic behaviour as
$$V_{\nu t}$$
for
$$t
\rightarrow \infty$$
. It is not too difficult to make this argument rigorous if, for instance,
$${\mathbb{E}} W_i^2 {\lt} \infty,$$
because then
$$ ( \sigma(t) -
t \nu )^2/t,\, t{\gt}0$$
, is uniformly integrable by Gut (2009, Section 2.5). The following functional limit theorem gives a precise description of the asymptotic behaviour of
$$V_{\sigma(t)}$$
whenever
$$W_i$$
has a finite mean.
Theorem 4.1
Suppose that
$$(Y_n)$$
and
$$(W_n)$$
are independent nonnegative i.i.d. sequences of random variables such that the
$$Y_i$$
are regularly varying with index
$$\alpha \in (0,1)$$
, and such that
$$ 0{\lt} 1/\nu = {\mathbb{E}} W_i {\lt}
\infty $$
. Then in the space
$$D[0,\infty)$$
endowed with the Skorokhod’s
$$J_1$$
topology
where
$$(G_\alpha(s))_{s\geq 0}$$
is an
$$\alpha$$
-stable subordinator.
Proof. Since the
$$Y_i$$
are regularly varying, it is known (Resnick (Reference Resnick1987), (Reference Resnick2007)) that the point process convergence
holds as
$$n {\to\infty}$$
with respect to the vague topology on the space of Radon point measures on
$$[0,\infty)\times (0,\infty]$$
. The abbreviation PRM stands for the Poisson random measure, indicating that the limit is a Poisson process. Starting from (4.4), it was shown in Resnick (Reference Resnick2007, Chapter 7) for instance that, for an
$$\alpha$$
-stable subordinator
$$G_\alpha(\cdot)$$
as in the statement of the theorem,
in the Skorokhod’s
$$J_1$$
topology on the space
$$ D[0,\infty)$$
. Observe that, since
$$\alpha \in (0,1)$$
, no centering is needed, and we can substitute the integer index n by a continuous index
$$t {\to\infty}$$
. Note further that we have the joint convergence
in the product topology on the space of point measures and càdlàg functions. Moreover, it is known that the jump times and sizes of the
$$\alpha$$
-stable subordinator
$$G_\alpha$$
correspond to the points of the limiting point process
$$M_{\alpha}$$
.
The space of point measures and the space of càdlàg functions
$$D[0,\infty)$$
are both Polish, in respective topologies; therefore, Skorokhod’s representation theorem applies. Thus, we can assume that the convergence in (4.5) holds a.s. on a certain probability space
$$(\Omega,\mathscr{f},P)$$
, and in particular there exists
$$\Omega' \subseteq
\Omega$$
such that
$$P(\Omega') = 1$$
and, for all
$$\omega \in \Omega'$$
,
$$V'_t
\to G_\alpha $$
in
$$J_1$$
and
$$M'_t \to M_\alpha$$
in vague topology. By Theorem 2.15 of Jacod and Shiryaev (2003, Chapter VI), for any such
$$\omega$$
, there exists a dense set
$$B=B(\omega)$$
of points in
$$[0,\infty)$$
such that
for every
$$s \in B $$
, where actually B is simply the set of all nonjump times in the path of the process
$$G_\alpha $$
. On the other hand, it is known that in the
$$J_1$$
topology, on some set
$$\Omega''$$
such that
$$P(\Omega'') = 1$$
,
where id stands for the identity map. This follows directly by an application of Theorem 2.15 of Jacod and Shiryaev (2003, Chapter VI). Moreover, by Proposition VI.1.17 of Jacod and Shiryaev (Reference Jacod and Shiryaev2003), the convergence in (4.6) holds locally uniformly on
$$D[0,\infty)$$
.
Now consider, for fixed
$$t{\gt}0$$
and
$$\omega \in \Omega' \cap \Omega''$$
,
From (4.6) we may expect that
$$V_t (s) \approx V'_{t\nu } (s).$$
Indeed, for any fixed
$$0{\lt}\delta{\lt}1$$
and all large t, we know that
$$
\lfloor tc\nu (1-\delta) \rfloor\leq\sigma(tc) \leq \lfloor tc\nu
(1+\delta) \rfloor$$
, which by monotonicity of the sums implies that
Now, for
$$c(1-\delta) $$
and
$$c(1+\delta)$$
in B, the left-hand side and the right-hand side above converge to
$$G_\alpha(c(1-\delta))$$
and
$$G_\alpha(c(1+\delta))$$
. Thus, if we consider
$$c\in B$$
and let
$$\delta \to
0$$
then
for all
$$\omega \in \Omega' \cap \Omega''$$
and thus with probability 1.
By Theorem 2.15 of Jacod and Shiryaev (2003, Chapter VI), to prove (4.3), it remains to show that, for all
$$\omega \in \Omega' \cap
\Omega''$$
and
$$c\in B$$
, as
$$t {\to\infty}$$
,
\begin{equation}
\sum_{0{\lt}s\leq c} | \Delta V_t(s)|^2 = \sum_{i{\lt}\sigma(tc) }
\bigg(\frac{Y_i}{a_{t\nu}}\bigg)^2 \to \sum_{0{\lt}s\leq c} | \Delta
G_\alpha(s)|^2 ,
\label{eqn16}
\end{equation}
where, for an arbitrary càdlàg process X(t) at time
$$t \geq 0$$
, we define
$$\Delta X(t) = X_{t} - X_{t-} $$
. Observe that
defines an
$$\alpha/2$$
-stable subordinator and that the squared random variables
$$Y_i^2$$
are again regularly varying with index
$$\alpha/2$$
with the property that
$$n\ {\mathbb{P}}(Y_i^2 {\gt}a^2_n) \to 1$$
. A similar approximation argument as for (4.7) shows that (4.8) indeed holds, which concludes the proof.
Assume now that
$$P(D{\gt}x)= x^{-\alpha} \ell(x)$$
for some slowly varying function
$$\ell$$
and
$$\alpha \in(0,1)$$
. Select a sequence
$$a_n {\to\infty}$$
such that
$$n\, P(D{\gt}a_n) \to 1$$
as
$$n{\to\infty}$$
. Under suitable conditions on the residue term
$${\varepsilon}_t$$
, we obtain the following result.
Proposition 4.2
Assume that the
$$D_i$$
are regularly varying with index
$$\alpha \in (0,1)$$
and that
$${\varepsilon}_t \,{=}\, o_P(a_{t}) $$
. Then there exists an
$$\alpha$$
-stable random variable
$$G_\alpha$$
such that
Proof. The proof follows roughly the same lines as the proof of Proposition 4.1, but here we rely on an application of the previous theorem to the random walks
$$(\Gamma_n)$$
and
$$(S^D_n)$$
. However, instead of the
$$Y_i$$
and
$$W_i$$
we have the
$$D_i$$
and an independent sequence of i.i.d. exponential random variables with parameter
$$\nu$$
.
Remark 4.1
One can consider the total claim amount in the period [0, t] for the stationary model of Subsection 2.1.4, i.e.
Here, again,
$$S^*(t)$$
has a similar representation as in (3.1) but with an additional term on the right-hand side, i.e.
\begin{equation*}
S^*(t) = \sum_{i=1}^{\tau(t)} D_i - D_{\tau(t)} - {{\varepsilon}}_t +
{{\varepsilon}}^*_{0,t},\qquad t \geq 0,
\end{equation*}
where
Clearly, by stationarity,
Hence,
$${\varepsilon}_t = o_P(a_{t}) $$
yields
$${\varepsilon}^-_t =
o_P(a_{t}) $$
for any sequence
$$(a_t)$$
and, therefore,
In particular, the conclusions of Propositions 3.1, 4.1, and 4.2 hold for random variables
$$S^*(t)$$
also under the additional assumption that
5 Total claim amount for special models
As we have seen in the previous two sections, it is relatively easy to describe the asymptotic behaviour of the total claim amount S(t) as long as we are able to determine the moments and tail properties of the random variables
$$D_i$$
, and the residue random variable
$${\varepsilon}_t$$
in (3.1) (and also
$$\tilde {\varepsilon}_t$$
in (4.11) for the stationary version). However, this is typically a rather technical task, highly dependent on an individual Poisson cluster model. In this section we revisit three models introduced in Subsection 2.1, characterizing for each the limiting distribution of the total claim amount under appropriate conditions. Note that the cluster sum D for all three models admits the representation
\[
D\stackrel{\text{D}}{=} \sum_{j=0}^K X_j
\]
for
$$(X_j)_{j\ge 0}$$
i.i.d. copies of f(A) and some integer valued K such that
$${\mathbb{E}}[K_1]{\lt}\infty$$
. Throughout, we assume that the random variables K and
$$(X_j)_{j\ge 1}$$
are independent. The sum
$$\sum_{j=1}^KX_j$$
has a so-called compound distribution. Its first two moments exist under the following conditions.
• if
$${\mathbb{E}}[X]{\lt}\infty$$
and
$${\mathbb{E}}[K]{\lt}\infty$$
, then
$$\mu_D =
{\mathbb{E}} D=(1+{\mathbb{E}}[K]){\mathbb{E}}[X] {\lt} \infty$$
,
• if
$${\mathbb{E}}[X^2]{\lt}\!\infty$$
and
$${\mathbb{E}}[K^2]{\lt}\infty$$
, then
$${\mathbb{E}} D^2=({\mathbb{E}}[K]+1){\mathbb{E}}[X^2]+({\mathbb{E}}[K^2]
+{\mathbb{E}}[K]){\mathbb{E}}[X]^2 {\lt} \infty$$
.
The tail behaviour of compound sums was often studied under various conditions (see Robert and Segers (Reference Robert and Segers2008), Faÿ et al. (Reference Faÿ, González-Arévalo, Mikosch and Samorodnitsky2006)), Hult and Samorodnitsky (Reference Hult and Samorodnitsky2008), and Denisov et al. (Reference Denisov, Foss and Korshunov2010)). We list below some of these conditions, which are applicable to our setting.
(RV1) If X is regularly varying with index
$$\alpha {\gt}0$$
and
$${\mathbb{P}}(K{\gt}x)\,{=}\,o({\mathbb{P}}(X{\gt}x))$$
, then
$${\mathbb{P}}(D\,{{\gt}}\,x) \sim
({\mathbb{E}}[K]+1){\mathbb{P}}(X{\gt}x)$$
as
$$x\to \infty$$
, see Faÿ et al. (2006, Proposition 4.1).
(RV2) If K is regularly varying with index
$$\alpha \in (1,2)$$
and
$${\mathbb{P}}(X{\gt}x)=o({\mathbb{P}}(K{\gt}x))$$
, then
$${\mathbb{P}}(D\,{{\gt}}\,x) \sim
{\mathbb{P}}(K{\gt}x/{\mathbb{E}}[X])$$
as
$$x\to \infty$$
; see Robert and Segers (2008, Theorem 3.2) or Faÿ et al. (2006, Proposition 4.3).
(RV3) If X and K are both regularly varying with index
$$\alpha \in (1,2)$$
and tail equivalent (see Embrechts et al. (Reference Embrechts, Klüppelberg and Mikosch1997, Definition 3.3.3)), then
$${\mathbb{P}}(D{\gt}x) \sim ({\mathbb{E}}[K]+1){\mathbb{P}}(X{\gt}x) +
{\mathbb{P}}(K{\gt}x/{\mathbb{E}}[X])$$
as
$$x\to \infty$$
(see Denisov et al. (2010, Theorem 7)).
We will refer to these three conditions as the sufficient conditions (RV).
5.1 Mixed binomial cluster model
Recall from Subsection 2.1.1 that the clusters in this model have the form
\begin{equation*}
G^{A_i} = \sum_{j=1}^{K_i} \delta_{W_{ij}, A_{ij}}.
\end{equation*}
Assume that
•
$${({K_i},\,{({W_{ij}})_{j \ge 1}},\,{({A_{ij}})_{j \ge 0}})_{i \ge 0}}$$
constitutes an i.i.d. sequence,•
$$(A_{ij})_{j\ge0}$$
are i.i.d. for any fixed i,•
$$(A_{ij})_{j\ge1}$$
is independent of
$$K_i,(W_{ij})_{j\ge 1}$$
for all
$$i\ge
0$$
,•
$$(W_{ij})_{j\ge 1}$$
are conditionally i.i.d. and independent of
$$K_i$$
given
$$A_{i0}$$
.
Thus, we do not exclude the possibility of dependence between
$$K_i,(W_{ij})_{j\ge 1}$$
and the ancestral mark
$$A_{i0}$$
. For any
$$\gamma{\,\gt\,}0$$
, we denote by
generic random variables with the same distribution as
$$A_{ij}$$
,
$$X_{ij}=\,f(A_{ij})$$
,
$$K_i$$
,
$$W_{ij}$$
,
$${\mathbb{E}}[K_i\ \,\,|\, \ \, A_{i0}]$$
, and
$${\mathbb{E}}[K_i^\gamma\ \,\,|\, \ \, A_{i0}]$$
, respectively. Using the cluster representation, we can derive the asymptotic properties of S(t). Let us first consider the Gaussian central limit theorem under appropriate second moment assumptions. Denote by
$${\mathbb{P}}(W \in \cdot \ \,\,|\, \ \, A)$$
the distribution of the
$$W_{ij}$$
given
$$A_{i0}$$
.
Corollary 5.1. Assume that
$${\mathbb{E}}[X^2]{\lt}\infty$$
and
$${\mathbb{E}}[K^2]{\lt}\infty$$
. If
then relation (3.2) holds.
Observe that (5.1) is slightly weaker than the existence of the moment
$${\mathbb{E}}[K \sqrt W]{\lt}\infty$$
.
Proof of Corollary 5.1. It follows from the compound sum representation of D that
$${\mathbb{E}}
D^2\,{{\lt}}\,\infty$$
as soon as
$${\mathbb{E}}[X^2]{\lt}\infty$$
and
$${\mathbb{E}}[K^2]{\lt}\infty$$
. By Proposition 3.1, it remains to show that
$${\varepsilon}_t \,{=}\, o_P(\sqrt t)$$
. To this end, we use the Markov inequality
We use Lemma 7.2.12 of Mikosch (Reference Mikosch2009) with
$$f(s) =
\sum_{j=1}^{K_i}{{\bf 1}}_{\{W_{ij}{>} t-s\}} \,f(A_{ij})$$
in order to compute the right-hand side term as
\begin{align*}
\frac{\int_0^t{\mathbb{E}}[\!\sum_{j=1}^{K_i}{{\bf 1}}_{\{W_{ij}{>} t-s\}}
\,f(A_{ij})]\nu \,\mathrm{d} s}{\sqrt t}
&=\frac{\nu{\mathbb{E}}[X]\int_0^t{\mathbb{E}}[{\mathbb{E}}[\!
\sum_{j=1}^{K_i}{{\bf 1}}_{\{W_{ij}{>} t-s\}} \ \,\,|\, \ \, A_{i0}]]\,\mathrm{d} s}{\sqrt
t}
\\
&=\frac{\nu{\mathbb{E}}[X]\int_0^t{\mathbb{E}}[m_A{\mathbb{P}}(W{>} x\ \,\,|\, \ \,
A)]\,\mathrm{d} x}{\sqrt t}.
\end{align*}
Note that the last identity follows due to the independence of
$$K_i$$
and
$$(W_{ij})_{j\ge 0}$$
conditionally on
$$A_{i0}$$
. We conclude by l’Hôpital’s rule that this converges to 0 under (5.1).
For regularly varying D of order
$$1{\lt}\alpha{\lt}2$$
, we obtain the corresponding limit theorem under weaker assumptions on the tail of the waiting time W.
Corollary 5.2. Assume that one of the (RV) conditions holds for
$$1{\lt}\alpha{\lt}2$$
, so that D is regularly varying. When
for some
$$\delta{>}0$$
, relation (4.2) holds.
Condition 5.2 is slightly weaker than assuming that
$${\mathbb{E}}[m_A W^{1+\delta-1/\alpha}]{\lt}\infty$$
. Note that, when
$$\alpha\to 1^+$$
and K is independent of W, this condition boils down to the existence of a
$$\delta$$
th moment of W for any strictly positive
$$\delta$$
.
Proof of Corollary 5.2. By definition,
$$(a_t)$$
satisfies
$$t{\mathbb{P}}(D{>}a_t)\to 1$$
as
$$t\to
\infty$$
and
$$(a_t)$$
is regularly varying with index
$$1/\alpha$$
. Applying the Markov inequality as in the proof of Corollary 5.1, we obtain
The claim follows by l’Hôpital’s rule and the relation
$$t^{1/\alpha-\delta} = o(a_t)$$
for any
$$\delta{>}0$$
.
Remark 5.1
In the context of the mixed binomial model, consider the total claim amount of the stationary process denoted by
$$S^*(t)$$
which also takes into account the arrivals in the interval
$$({-}\,\infty,0)$$
; see Remark 4.1. Assume for simplicity that the
$$K_i$$
and
$$(W_{ij})$$
are unconditionally independent. Then
$$\tilde {\varepsilon}_t$$
from (4.11) is
$$o_P(a_{t})$$
under the same conditions as in Corollaries 5.1 and 5.2, where we set
$$a_t = \sqrt t$$
in the former case. Indeed, we will show that
so that
$${\mathbb{E}} \tilde {\varepsilon}_t= o_P(a_{t})$$
as well since the right-hand side is dominated by
$${\mathbb{E}} {\varepsilon}^-_t = o(a_t)$$
; cf. 4.10.
Note first that, under the assumptions of the last two corollaries, individual claims have finite expectation, i.e.
$${\mathbb{E}} X {\lt}\infty$$
. So it suffices to show that
\begin{equation*}
I_1 \,{:\!=}\, \frac{{\mathbb{E}} \tilde {\varepsilon}_t}{ {\mathbb{E}} X} =
{\mathbb{E}} \sum_{\Gamma_i {\lt} -t } \sum_{j=1}^{K_i} {{\bf 1}}_{\{ 0 {\lt}
\Gamma_i+W_{ij}{\lt}t\}} = {\mathbb{E}} \sum_{-t{\lt}\Gamma_i {\lt} 0 }
\sum_{j=1}^{K_i} {{\bf 1}}_{\{\Gamma_i+W_{ij}{>}t\}} \,{=\!:}\, I_2 .
\end{equation*}
From
$$I_1$$
and
$$I_2$$
we respectively subtract the left-hand and right-hand sides of the equality
\[
{\mathbb{E}} \sum_{-2t{\lt}\Gamma_i {\lt} -t } \sum_{j=1}^{K_i}
{{\bf 1}}_{\{\Gamma_i+W_{ij} \in (0,t) \}} {{\bf 1}}_{\{W_{ij}\in (t,2t]\}} =
{\mathbb{E}} \sum_{-t{\lt}\Gamma_i {\lt} 0 } \sum_{j=1}^{K_i}
{{\bf 1}}_{\{\Gamma_i+W_{ij} \in (t,2t)\} } {{\bf 1}}_{\{W_{ij}\in
(t,2t]\}},
\]
where the equality follows by the stationarity of the underlying Poisson process, to obtain
\begin{equation*}
J_1 = {\mathbb{E}} \sum_{-\infty{\lt}\Gamma_i {\lt} -t } \sum_{j=1}^{K_i}
{{\bf 1}}_{\{0{\lt}\Gamma_i+W_{ij} {\lt} t\} } {{\bf 1}}_{\{W_{ij} {>} 2t \}} =
{\mathbb{E}} K \int_{-\infty}^{-t} \nu \,\mathrm{d} s \int_{-s \vee 2t }^{t-s}
\,\mathrm{d} F_W(u)
\end{equation*}
and
\begin{equation*}
J_2 = {\mathbb{E}} \sum_{-t {\lt}\Gamma_i {\lt} 0 } \sum_{j=1}^{K_i}
{{\bf 1}}_{\{\Gamma_i+W_{ij} {>} t \}} {{\bf 1}}_{\{W_{ij} {>} 2t \}} =
{\mathbb{E}} K \int_{-t}^{0} \nu \,\mathrm{d} s \int_{2t}^\infty \,\mathrm{d} F_W(u),
\end{equation*}
where
$$F_W$$
denotes the distribution function of delays
$$(W_{ij})$$
. Finally, note that
Since we assumed that
$${\mathbb{E}}[K]{\lt}\infty$$
, the regular variation property of D with index
$$\alpha\in(0,1)$$
can arise only through the claim size distribution; see Proposition 4.8 of Faÿ et al. (Reference Faÿ, González-Arévalo, Mikosch and Samorodnitsky2006). It turns out that in such a heavy-tailed case, no additional assumption on the waiting time W is needed.
Corollary 5.3. Assume that X is regularly varying of order
$$0{\lt}\alpha{\lt}1$$
. Then relation 4.9 holds.
Proof. Observe that we cannot apply the Markov inequality anymore because
$${\mathbb{E}} D=\infty$$
. Instead, we use the fact that
$$\sum\nolimits_{j = 1}^t {{X_j}/{a_t}} $$
converges because X and D have equivalent regularly varying tails. Recall from (4.10) that
We denote the (increasing) number of summands in the right-hand side term by
$$M_t=\# \{i,j\colon 0\le {\Gamma_i} \leq t ,\, t {\lt} {\Gamma_i} +
W_{ij}\}$$
. We can apply Proposition 4.2 after observing that
$$\sum\nolimits_{j=1}^{M_t}X_j/a_{M_t}$$
is a tight family of random variables, because
$$M_t$$
is independent of the array
$$(X_{ij})$$
. Writing
and observing that
$$a_t$$
is regularly varying with index
$$1/\alpha$$
, we obtain the desired result provided that
$$M_t=o_P(t)$$
. It is sufficient to show the convergence to 0 of the ratio
Using similar calculations as in the proof of Corollary 5.1 (setting
$$X=1$$
), we obtain an explicit formula for the right-hand side term as
the convergence to 0 following from a Cesarò argument.
5.2 Renewal cluster model
Recall from Subsection 2.1.2 that the clusters of this model have the form
\begin{equation*}
G^{A_i} = \sum_{j=1}^{K_i} \delta_{T_{ij}, A_{ij}},
\end{equation*}
where
•
$$T_{ij}=W_{i1}+\cdots +W_{ij}$$
,• while
$$(K_i,(W_{ij})_{j\ge 1},(A_{ij})_{j\ge 0})_{i\ge 0}$$
constitutes an i.i.d. sequence satisfying the assumptions listed in Section 5.1.
The total claim amount coming from the ith immigrant and its progeny is again
\[
D \stackrel{\text{D}}{=} \sum_{j=0}^K X_j
\]
for
$$(X_j)$$
i.i.d. copies of f(A). Dealing with the waiting times
$$T_{ij}=W_{i1}+\cdots +W_{ij}$$
requires additional care than in the previous model. We first obtain the following result.
Corollary 5.4. Suppose that
$${\mathbb{E}} X^2 {\lt}\infty,$$
$${\mathbb{E}} K^2 {\lt}\infty$$
, and
$$
{\mathbb{E}} [K^{2}W^\delta] {\lt} \infty$$
for some
$$\delta{>}\tfrac12$$
. Then relation (3.2) holds.
Proof. The proof follows from Proposition 3.1. The second moment of the
$$D_i$$
is finite by the moment assumptions on X and K. It remains to show that the residue term satisfies
$${\varepsilon}_t = o_P(\sqrt{t}) $$
. Using Lemma 7.2.12 of Mikosch (Reference Mikosch2009) with
$$f(x) = \sum\nolimits_{j=1}^{K_i}{{\bf
1}}_{\{W_{i1}+\cdots+W_{ij}{\gt} x\}} \,f(A_{ij})$$
similarly as in the proof of Corollary 5.1, we obtain
\begin{align*}
{\mathbb{E}}[{\varepsilon}_t]&=
\int_0^t{\mathbb{E}}\bigg[\sum_{j=1}^{K_i}{{\bf
1}}_{\{W_{i1}+\cdots+W_{ij}{>}
x\}} \,f(A_{ij})\bigg]\nu \,\mathrm{d} x
\\
& = \nu \int_0^t{\mathbb{E}}\bigg[{\mathbb{E}}\bigg[\sum_{j=1}^{K_i} {{\bf
1}}_{\{W_{i1}+\cdots+W_{ij}{>} x\}} \,f(A_{ij})\biggm| K_i, (W_{ij})_{j\ge
1}\bigg]\bigg] \,\mathrm{d} x
\\
& = \nu {\mathbb{E}}[X]\int_0^t{\mathbb{E}}\bigg[ \sum_{j=1}^{K_i}{{\bf
1}}_{\{W_{i1}+\cdots+W_{ij}{>} x\}} \bigg] \,\mathrm{d} x
\end{align*}
by the independence between
$$K_i, (W_{ij})_{j\ge 1}$$
and
$$(\,f(A_{ij}))_{j\ge
1}$$
. The key argument in dealing with the renewal cluster model is the upper bound
\begin{equation}
\sum_{j=1}^{K_i}{{\bf 1}}_{\{W_{i1}+\cdots+W_{ij}{>}x\}}\le {{\bf 1}}_{\{
W_{i1}+\cdots+W_{iK_i}{>}x\}} K_i.
\label{eqn23}
\end{equation}
Assume without loss of generality that
$$\delta \le 1$$
. By the Markov inequality and the conditional independence of
$$K_i$$
and
$$(W_{ij})_{j\ge
0}$$
conditionally on
$$A_{i0}$$
, we obtain
\begin{align}
{\mathbb{E}}[ {{\bf 1}}_{W_{i1}+\cdots+W_{iK_i}{>} x}K_i\ \,\,|\, \ \, A_{i0} ]&\le
\frac{{\mathbb{E}}[K_i (W_{i1}+\cdots+W_{iK_i})^\delta\ \,\,|\, \ \,
A_{i0}]}{x^\delta}\nonumber
\\
&\le m_{A_{i0}}^{(2)} \frac{{\mathbb{E}}[W^\delta\ \,\,|\, \ \, A_{i0}]}{x^\delta},
\label{eqn24}\end{align}
using the notation
$$m_{A_{i0}}^{(\gamma)}={\mathbb{E}}[K_i^\gamma \ \,\,|\, \ \,
A_{i0}]$$
for any
$$\gamma{>}0$$
. The last inequality follows from the sublinearity of the mapping
$$x\mapsto x^\delta$$
for
$$\delta\le 1$$
. Thus, we obtain, for some constant
$$C{>}0$$
,
as
$$\delta{>}\tfrac12$$
by assumption.
Regularly varying claims can be handled with additional care as K may not be square integrable.
Corollary 5.5. Assume that one of the (RV) conditions holds so that D is regularly varying of order
$$1{\lt}\alpha{\lt}2.$$
Suppose further that
$${\mathbb{E}}[K^{1+\gamma}]{\lt}\infty$$
and
$${\mathbb{E}}[K^{1+\gamma}W^\delta]{\lt}\infty,$$
$$\delta{>}0,$$
$$\gamma {>}0$$
, and
$$
\delta{\gt}(\alpha-\gamma)/\alpha$$
. Then relation (4.2) holds.
Observe that we obtain somewhat stronger conditions than in the mixed binomial case; see Corollary 5.2 and the remark following it.
Proof of Corollary 5.5. Without loss of generality we assume that
$$\gamma\le1$$
. We use the Markov inequality of order
$$\gamma$$
Thanks to the subadditivity of the function
$$x\mapsto x^\gamma$$
we have
\begin{align*}
{\mathbb{E}}[{\varepsilon}_t^\gamma]&= {\mathbb{E}}\bigg[\bigg(\sum_{0\le
\Gamma_i\le t}\sum_{j=1}^{K_i}{{\bf 1}}_{\{\Gamma_i+W_{i1}
+\cdots+W_{ij}{>}t\}}\,f(A_{ij})\bigg)^\gamma\bigg]
\\
&\le {\mathbb{E}}\bigg[\sum_{0\le \Gamma_i\le t}\bigg(\sum_{j=1}^{K_i}{{\bf
1}}_{\{\Gamma_i+ W_{i1}+\cdots+W_{ij}{>}t\}}\,f(A_{ij})\bigg)^\gamma\bigg].
\end{align*}
Using Lemma 7.2.12 of Mikosch (Reference Mikosch2009) with
$$f(x) =
\sum\nolimits_{j=1}^{K_i}{{\bf 1}}_{\{W_{i1}+\cdots+W_{ij}{\gt}x\}}\,f(A_{ij})$$
similarly as in the proof of Corollary 5.1, we obtain
\begin{equation}
{\mathbb{E}}[{\varepsilon}_t^\gamma]\le\nu \int_0^t{\mathbb{E}}\bigg[
\bigg(\sum_{j=1}^{K_i}{{\bf
1}}_{\{W_{i1}+\cdots+W_{ij}{>}x\}}\,f(A_{ij})\bigg)^\gamma\bigg] \,\mathrm{d} x.
\label{eqn25}
\end{equation}
Using Jensen’s inequality,
\begin{align*}
&{\mathbb{E}}\bigg[{\mathbb{E}}\bigg[ \bigg(\sum_{j=1}^{K_i}{{\bf
1}}_{\{W_{i1}+\cdots+W_{ij}{>}x\}} \,f(A_{ij})\bigg)^\gamma\biggm| K_i, (W_{ij})_{j\ge
1}\bigg]\bigg]
\\
&\qquad\le {\mathbb{E}}\bigg[ \bigg({\mathbb{E}}\bigg[\sum_{j=1}^{K_i}{{\bf
1}}_{\{W_{i1}+\cdots+W_{ij}{>}x\}}\,f(A_{ij})\biggm| K_i, (W_{ij})_{j\ge
1}\bigg]\bigg)^\gamma\bigg],
\end{align*}
so that, using the independence between
$$K_i, (W_{ij})_{j\ge 1}$$
and
$$(\kern1.9pt f(A_{ij}))_{j\ge 1}$$
, we obtain
\[
{\mathbb{E}}[{\varepsilon}_t^\gamma]\le \nu
{\mathbb{E}}[X]^\gamma\int_0^t{\mathbb{E}}\bigg[\bigg(\sum_{j=1}^{K_i}{{\bf
1}}_{\{W_{i1}+\cdots+W_{ij}{>}x\}}\bigg)^\gamma\bigg]\,\mathrm{d} x.
\]
Using the stochastic domination (5.4), we obtain
Without loss of generality we assume that
$$0{\lt}\delta{\lt}1$$
. Applying the Markov inequality of order
$$\delta$$
conditionally on
$$A_{i0}$$
as in (5.5), we have
Substituting the previous inequality into this bound we obtain, for some
$$C{>}0$$
,
as
$$1-\delta{\lt}\gamma/\alpha$$
by assumption.
Corollary 5.6. If X is regularly varying of order
$$\alpha \in (0,1)$$
then relation 4.9 holds.
Proof. We use the same arguments as in the proof of Corollary 5.1 in order to obtain 5.3. The desired result follows if we can show that
$$M_t=\# \{i,j\colon 0\le {\Gamma_i} \leq t ,\, t {\lt} {\Gamma_i} +
W_{i1} + \cdots + W_{ij}\} = o_P(t)$$
. Using Markov’s inequality, it is enough to check that
$${\mathbb{E}}[M_t]/t=o(1)$$
. Following the same reasoning as in the proof of Corollary 5.5, we estimate the moment of
$$M_t$$
similarly as that of
$${\varepsilon}_t$$
in (5.6):
\[
{\mathbb{E}}[M_t]\le \int_0^t{\mathbb{E}}\bigg[ \sum_{j=1}^{K_i}{{\bf
1}}_{\{W_{i1}+\cdots+W_{ij}{>}x\}} \bigg]\nu \,\mathrm{d} x\le \int_0^t{\mathbb{E}}[ K_i
{{\bf 1}}_{\{W_{i1}+\cdots+W_{iK_i}{>}x\}} ]\nu \,\mathrm{d} x.
\]
We again used stochastic domination (5.4) to obtain the last upper bound. From a Cesaró argument, the result will follow if
We can check this negligibility property because the random sequence
$$K_i
{{\bf 1}}_{\{W_{i1}+\cdots+W_{iK_i}{>}x\}} \to 0$$
a.s. by the finiteness of
$$W_{i1}+\cdots+W_{iK_i}$$
and because the sequence is dominated by
$$K_i$$
that is integrable.
5.3 Marked Hawkes process
Recall from Section 2.1.3 that the clusters of the Hawkes model satisfy recursive relation (2.4). In other words, the clusters
$$G^{A_i}$$ represent a recursive aggregation of Poisson processes with random mean measure
$$ \tilde{\mu}_A \times Q$$ which satisfies
$$\kappa =
{\mathbb{E}} \int h(s,A) \,\mathrm{d} s {\lt} 1$$
.
In general, it is not entirely straightforward to see when the moments of D are finite. However, note that the
$$D_i$$
are i.i.d. and satisfy the distributional equation
\begin{equation}
D \stackrel{\text{D}}{=} f(A) + \sum_{j=1}^{L_A} D_j ,
\label{eqn26}
\end{equation}
where
$$L_A$$
has the Poisson distribution conditionally on A, with mean
$$\kappa_A=\int_0^\infty h(s,A) \,\mathrm{d} s.$$
Recall from (2.5) that
$$\kappa = {\mathbb{E}} \kappa_A {\lt} 1.$$
The
$$D_j$$
on the right-hand side are independent of
$$\kappa_A$$
and i.i.d. with the same distribution as D. Conditionally on A, the waiting times are i.i.d. with common density
$$h(t,A)/\kappa_A ,\,t\ge0$$
. Thus, we can relate the clusters of the Hawkes process with those of a mixed binomial process from Section 5.1 with
$$K=L_A$$
. In order to obtain the asymptotic properties of S(t), we still need to characterize the moment and tail properties of D.
Consider the Laplace transform of D, i.e.
$$\varphi(s) = {\mathbb{E}}
\mathrm{e}^{-sD}$$
for
$$s \geq 0$$
. Also, recall that the Laplace transform of a Poisson compound sum is of the form
where M is Poiss
$$(m_A)$$
distributed, independent of the i.i.d. sequence
$$(Z_i)$$
of nonnegative random variables with common distribution (see, for instance, Section 7.2.2 of Mikosch (Reference Mikosch2009)). Note that
$$\varphi$$
is an infinitely differentiable function for
$$s{\gt}0$$
. To simplify the notation, let
a generic claim size and observe that, by (5.7),
$$\varphi$$
satisfies
\begin{align}
\varphi(s) & = {\mathbb{E}} [ {\mathbb{E}}[ \mathrm{e}^{-s(X +
\sum_{j=1}^{L_A}D_j)} \ \,\,|\, \ \, A ]]\nonumber
\\
&= {\mathbb{E}} [ \mathrm{e}^{-sX}
{\mathbb{E}}[\mathrm{e}^{ -s \sum_{j=1}^{L_A}D_j} \ \,\,|\, \ \, A ]] \nonumber
\\
& = {\mathbb{E}} [ \mathrm{e}^{-sX} \mathrm{e}^{\kappa_A ({\mathbb{E}} \mathrm{e}^{-sD} -1) } ]
\nonumber
\\
&= {\mathbb{E}}[ \mathrm{e}^{-sX} \mathrm{e}^{\kappa_A (\varphi(s) -1) }].
\label{eqn27}\end{align}
When
$${\mathbb{E}} [\kappa_A ]=\kappa{\lt}1$$
, it is known that this functional equation has a unique solution
$$\varphi$$
which further uniquely determines the distribution of D. By studying the behaviour of the derivatives of
$$\varphi(s)$$
for
$$s\to 0+$$
, we obtain the following result.
Lemma 5.1
If
$${\mathbb{E}} X^2 {\lt}\infty$$
and
$${\mathbb{E}} \kappa_A^2{\lt}\infty$$
then
Note that this expression coincides with the expression in [Karabash and Zhu (Reference Karabash and Zhu2015), when
$$X=f(A)\equiv 1$$
, i.e. in the case when one simply counts the number of claims.
Proof of Lemma 5.1. Differentiating (5.8) with respect to
$$s{\gt}0$$
produces
As
$${\mathbb{E}}(\kappa_A)=\kappa{\lt}1$$
, we obtain
As
$$\varphi(s)\le 1,\,s\ge 0$$
, the integrand in the numerator is dominated by X and that in the denominator by
$$\kappa_A $$
. By the dominated convergence argument,
$$\lim _{s \to 0+}\varphi'(s)$$
exists and is equal to
In particular,
$${\mathbb{E}} D = {\mathbb{E}} X/(1-\kappa)$$
. Differentiating (5.8) again produces the second moment of D. Indeed, we have
so that
Here, again, applying the dominated convergence theorem twice, we can let
$$s\to 0+$$
and obtain
This completes the proof since
$$X\,{=}\ f(A)$$
.
The following theorem describes the behavior of the total claim amount (S(t)) for the marked Hawkes process under appropriate second moment assumptions. Recall from (2.3) that
$$\tilde{\mu}_{A} (B) = \int_B
h(s, A) \,\mathrm{d} s.$$
Theorem 5.1. If
$$\kappa{\lt}1$$
,
$${\mathbb{E}} X^2 {\lt}\infty$$
, and
$${\mathbb{E}}[ \kappa_A
^2]{\lt}\infty$$
then, in either the stationary or nonstationary case, if
relation (3.2) holds.
Proof. In order to apply Proposition 3.1, we have to check that
$${\varepsilon}_t = o_P(\sqrt t)$$
. The proof is based on the following domination argument on
$${\varepsilon}_t$$
. Recall that we can write
\begin{equation*}
N = \sum_i \sum_j \delta_{{\Gamma_i} + T_{ij},A_{ij}} =
\sum_{k=1}^\infty \delta_{\tau_k,A^{k}} ,
\end{equation*}
without loss of generality assuming that
$$0\leq \tau_1\leq \tau_2\leq
\cdots$$
. At each time
$$\tau_j$$
, a claim arrives generated by one of the previous claims or an entirely new (immigrant) claim appears. In the former case, if
$$\tau_j$$
is a direct offspring of a claim at time
$$\tau_i$$
, we write
$$\tau_i\to \tau_j$$
. Progeny
$$\tau_j$$
then creates potentially further claims. We denote by
$$D_{\tau_j}$$
the total amount of claims generated by the arrival at
$$\tau_j$$
(counting the claim at
$$\tau_j$$
itself as well). Clearly, the
$$D_{\tau_j}$$
are identically distributed as D and even independent if we consider claims which are not offspring of one another. They are also independent of everything happening in the past.
The process N is naturally dominated by the stationary marked Hawkes process
$$N^*$$
which is well defined on the whole real line as we assumed that
$$\kappa = {\mathbb{E}} \kappa_A {\lt}1$$
; see the discussion at the end of Subsection 2.1. For the original and stationary Hawkes processes, N and
$$N^*$$
, by
$$\lambda$$
and
$$ \lambda^*$$
we denote the corresponding predictable intensities. By the construction of these two point processes,
$$\lambda \leq \lambda^*$$
. Recall that
$$\tau_i\to \tau_j$$
is equivalent to
$$\tau_j=\tau_i+W_{ik},\,k\le L^i = L_{A^i}$$
, where, by assumption, the
$$W_{ik}$$
are i.i.d. with common density
$$h(t,A^i)/ \kappa_{A^i},\,t\ge0$$
, and independent of
$$L^{i}$$
conditionally on the mark
$$A^i$$
of the claim at
$$\tau_i$$
. Moreover, conditionally on
$$A^i$$
, the number of direct progeny of the claim at
$$\tau_i$$
, denoted by
$$L^{i}$$
, has Poisson distribution with parameter
$$\tilde{\mu}_{A^i}$$
. Therefore, using conditional independence and equal distribution of the
$$D^{'}$$
we obtain
\begin{align*}
{\mathbb{E}}[{\varepsilon}_t] &= {\mathbb{E}}\bigg[ \sum_{{\Gamma_i} \leq
t}\sum_j {{\bf 1}}_{\{\Gamma_i + T_{ij} {\gt}t\}} X_{ij}\bigg]
\\
&= {\mathbb{E}}\bigg[\sum_{\tau_i \leq t} \sum_{\tau_j {\gt} t} D_{\tau_j}
{{\bf 1}}_{\{\tau_i\to \tau_j\}}\bigg]
\\
&={\mathbb{E}}\bigg[\sum_{\tau_i \leq t}
{\mathbb{E}}\bigg[\sum_{k=1}^{L^{i}} D_{\tau_i+W_{ik}}
{{\bf 1}}_{\{\tau_i+W_{ik} {\gt} t\}} \biggm| (\tau_i,A^i)_{i\ge 0}; \,\tau_i \le
t\bigg]\bigg]
\\
&= \mu_D {\mathbb{E}} \bigg[ \int_{0}^t \int_{\mathbb{S}}
\tilde{\mu}_a((t-s,\infty)) N(\mathrm{d} s,\,\mathrm{d} a) \bigg],
\end{align*}
where
$$ \tilde{\mu}_{a} ((u,\infty)) = \int_u^\infty h(s, a) \,\mathrm{d} s$$
. Observe that, from the projection theorem (see Brémaud (Reference Brémaud1981, Chapter 8, Theorem 3)), the last expression equals
We can further bound this estimate by
\begin{align*}
{\mathbb{E}}\bigg[\int_0^t \int_{\mathbb{S}}
\tilde{\mu}_a((t-s,\infty)) Q(\mathrm{d} a) \lambda^*(s)\,\mathrm{d} s\bigg]&=\int_0^t
\int_{\mathbb{S}} \tilde{\mu}_a((t-s,\infty)) Q(\mathrm{d} a)
{\mathbb{E}}[\lambda^*(s)]\,\mathrm{d} s
\\
&=\frac{\nu}{1-\kappa}\int_0^t \int_{\mathbb{S}}
\tilde{\mu}_a((t-s,\infty)) Q(\mathrm{d} a) \,\mathrm{d} s.
\end{align*}
Here we used Fubini’s theorem, and the expression
$${\mathbb{E}} [
\lambda^*(s) ] \equiv \nu /(1-\kappa)$$
. Observe that this expectation is constant since
$$N^*$$
is a stationary point process; to show that it equals
$$ \nu/(1-\kappa)$$
, note that
\begin{align*}\\[-24pt]
{\mu}^* &= {\mathbb{E}} { \lambda^*(s)}
\\
&= {\mathbb{E}} \bigg[ \nu
+ \int_{-\infty}^s \int_{\mathbb{S}} h(s-u,a) N^*(\mathrm{d} u,\,\mathrm{d} a) \bigg]
\\
& = \nu + \int_{-\infty}^s \int_{\mathbb{S}} h(s-u,a)
{\mathbb{E}}({\lambda}^*(u))\,\mathrm{d} uQ(\mathrm{d} a)[0]
\\
& = \nu + {\mu}^* \int_{-\infty}^s {\mathbb{E}} h(s-u,A)\,\mathrm{d} u
\\
& = \nu + {\mu}^*\int_0^{\infty}{\mathbb{E}} h(v,A)\,\mathrm{d} v;
\end{align*}
see also Daley and Vere Jones (Reference Daley and Vere-Jones2003, Example 6.3(c)). Hence,
$${\mu}^* = \nu
+ {\mu}^* \kappa$$
and
$$ {\mu}^* = {\nu}/({1-\kappa})$$
, as claimed above. Now, we have
Hence, the residual term is bounded in expectation by the expression we obtained in the mixed binomial case in Section 5.1. Thus, the result will follow from the proof of Corollary 5.1 under condition (5.1), which is further equivalent to (5.11) thanks to the expression of the density of the waiting times.
Dividing the last expression by
$$\sqrt t$$
and applying l’Hôpital’s rule proves the theorem for the nonstationary or pure Hawkes process; see [Karabash and Zhu (Reference Karabash and Zhu2015) where the same idea appears in the proof of Theorem 1.3.2.
To show that the central limit theorem holds in the stationary case, note that S(t) now has a similar representation as in (3.1) but with an additional term on the right-hand side, i.e.
\begin{equation}
S(t) = \sum_{i=1}^{\tau(t)} D_i - D_{\tau(t)} - {\varepsilon}_t
+{\varepsilon}_{0,t},\qquad t \geq 0,
\label{eqn32}
\end{equation}
where
A similar computation yields
\begin{align*}
{\mathbb{E}} {{\varepsilon}_{0,t}}&= {\mathbb{E}} \sum_{\Gamma_i
\leq 0} \sum_j {{\bf 1}}_{\{0{\lt}\Gamma_i + T_{ij} {\lt}t\}} X_{ij}
\\
&= {\mathbb{E}} \sum_{\tau_i \leq 0} \sum_{0{\lt} \tau_j{\lt}t} D_{\tau_j} {{\bf
1}}_{\{\tau_i\to \tau_j\}}
\\
&= {\mathbb{E}} \bigg[ \sum_{\tau_i \leq 0} \mu_D {\mathbb{E}} \bigg[
\sum_{0{\lt}\tau_j{\lt}t} {{\bf 1}}_{\{\tau_i\to \tau_j\}} \biggm| \mathscr{f}_0
\bigg] \bigg]
\\
& = \mu_D {\mathbb{E}} \bigg[ \sum_{\tau_i \leq 0}
\tilde{\mu}_{A^{i}}((0-\tau_i,t-\tau_i)) \bigg]
\\
& = \mu_D {\mathbb{E}} \bigg[ \int_{-\infty}^0 \int_{\mathbb{S}}
\tilde{\mu}_a(({-}\,s,t-s)) N^*(\mathrm{d} s,\,\mathrm{d} a) \bigg],
\end{align*}
where
$$\tilde{\mu}_{a} (B) = \int_B h(s, a) \,\mathrm{d} s$$
and
$$\mathscr{f}_0$$
stands for the internal history of the process up to time 0, i.e.
$$\mathscr{f}_0 = \sigma\{ N(I \times S)\colon I \in
\mathscr{b}(\mathbb{R}),\, I \subset ({-}\,\infty, 0],\, S \in \mathscr{s}\}.$$
Again, by the projection theorem (see Brémaud (Reference Brémaud1981, Chapter 8, Theorem 3)), the last expression equals
This is further equal to
\begin{align*}
&\mu_D \int_{-\infty}^0 \int_{\mathbb{S}}
\tilde{\mu}_a(({-}\,s,t-s)) {\mathbb{E}} [ \lambda^*(s) ] \,\mathrm{d} s\,Q(\mathrm{d} a)
\\
&\qquad = \mu_D \dfrac{\nu}{1-\kappa} \int_{-\infty}^0 \int_{\mathbb{S}}
\tilde{\mu}_a(({-}\,s,t-s)) \,\mathrm{d} s\,Q(\mathrm{d} a)
\\
&\qquad = \mu_D \dfrac{\nu}{1-\kappa} \int_{-\infty}^0 {\mathbb{E}}
\tilde{\mu}_A(({-}\,s,t-s)) \,\mathrm{d} s
\\
&\qquad = \mu_D \dfrac{\nu}{1-\kappa} \int_{0}^{\infty} {\mathbb{E}}
\tilde{\mu}_A((s,s+t)) \,\mathrm{d} s
\\
&\qquad = \mu_D \dfrac{\nu}{1-\kappa} \int_0^{\infty} {\mathbb{E}}
\int_s^{s+t} h(u,A)\,\mathrm{d} u \,\mathrm{d} s
\\
&\qquad = \mu_D\dfrac{\nu}{1-\kappa} \int_0^{\infty} {\mathbb{E}} (t\wedge u)
h(u,A) \,\mathrm{d} u
\\
&\qquad= \mu_D\dfrac{\nu}{1-\kappa} \bigg( \int_0^{t} {\mathbb{E}} [ u h(u,A)
] du+t\int_t^{\infty} {\mathbb{E}} [ h(u,A) ] \,\mathrm{d} u \bigg).
\end{align*}
Note that the second term in the last expression divided by
$$\sqrt t$$
tends to 0 by (5.11). Using integration by parts for the first term, we have
The first integral on the right-hand side divided by
$$\sqrt t$$
tends to 0 under (5.11). The last term divided by
$$\sqrt t$$
also tends to 0 by an application of l’Hôpital’s rule as in the nonstationary case.
Finally, we observe that
$${\varepsilon}_{0,t}/\sqrt t \xrightarrow{{\mathbb{P}\ }} 0$$
and the result in the stationary case is proved.
Observe that (5.11) is substantially weaker than (2.6) in the unmarked case. Namely, the former condition requires only that the total residue due to the claims on the compact interval [0,t] is of the order
$$o(\sqrt t)$$
in probability. In particular, in the unmarked case, the central limit theorem holds for the stationary and the nonstationary cases even if (2.6) is not satisfied, i.e. even when the nonstationary process is not convergent.
As mentioned above, there are related limit theorems in the literature concerning only the counting process
$$N_t$$
(see Karabash and Zhu (Reference Karabash and Zhu2015)), but in contrast to their result, our proof does not rely on the martingale central limit theorem, it stems from the rather simple relations (3.1) and (5.13).
In the following example, we consider some special cases of Hawkes processes for which a closed-form expression for the second moment
$${\mathbb{E}} D^2$$
can be found.
Example 5.1. (Marked Hawkes processes with claims independent of the cluster size.)
Assume that the random measure (2.3),
holds on
$$\mathbb{R}_+$$
and that the corresponding claim sizes
$$X=f(A)$$
are independent. In particular, this holds if
$$\tilde{\mu}_A (B) = \int_B h(s)
\,\mathrm{d} s$$
for some integrable function h, i.e. when
$$\tilde{\mu}_A$$
is a deterministic measure and we actually have a standard Hawkes process with independent marks. In this special case
$$K+1$$
is known to have the so-called Borel distribution; see Haight and Breuer (Reference Haight and Breuer1960).
Using the arguments from the proof of Lemma 5.1, we obtain
$$\mu_D =
{\mathbb{E}} D_i = {{\mathbb{E}} X}/({1-\kappa}).$$
Similarly, the variance of the
$$D_i$$
is finite as the variance of a compound sum, and equals
cf. Lemma 2.3.4 of Mikosch (Reference Mikosch2009). Hence,
$${\mathbb{E}} D^2 $$
in Theorem 5.1 has the form
In the special case when the claims are all constant, say
$$X=f(A)\equiv
c{\gt}0$$
, direct calculation yields
$${\mathbb{E}} D = c/({1-\kappa}),$$
with
$$\kappa={\mathbb{E}} [\kappa_A ]$$
, and
obtaining
in particular, for
$$c=1$$
, we recover expression in Karabash and Zhu (Reference Karabash and Zhu2015).
In the rest of this subsection, we study the marked Hawkes process in the case when the
$$D_i$$
are regularly varying with index
$$\alpha {\lt}2 $$
. Using the result of Hult and Samorodnitsky (Reference Hult and Samorodnitsky2008), we can show that, when the individual claims
$$X=f(A)$$
are regularly varying, this property is frequently passed on to the random variable D under appropriate moment assumptions on
$$\kappa_A
$$
. However, using the specific form of the Laplace transform for D given in (5.8), we can show regular variation of D under weaker conditions. This is the content of the following lemma.
Lemma 5.2
Assume that
$$\kappa{\lt}1$$
and that
$$X=f(A)$$
is regularly varying with index
$$\alpha \in (0,1)\cup (1,2)$$
. When
$$\alpha \in (1,2)$$
, assume additionally that
$$Y=X + \kappa_A \mu_D$$
is regularly varying of order
$$\alpha$$
. Then the random variable D is regularly varying with the same index
$$\alpha$$
.
Proof. We will use Karamata’s Tauberian theorem, as formulated and proved in Theorem 8.1.6 of Bingham et al. (Reference Bingham, Goldie and Teugels1987). In particular, the equivalence between Equations (8.1.12) and (8.1.11b) in Bingham et al. (Reference Bingham, Goldie and Teugels1987) yields the following result.
Theorem 5.2. The nonnegative random variable X is regularly varying with a noninteger tail index
$$\alpha{\gt}0$$
, i.e.
$$\skew4\bar F(x)\sim x^{-\alpha}\ell(x)$$
as
$$x\to\infty$$
if and only if
for some slowly varying function
$$\ell$$
and a constant depending only on
$$\alpha$$
:
$$c=-\Gamma(\alpha+1)\Gamma(1-\alpha)/\Gamma(\alpha-\lfloor \alpha
\rfloor)$$
.
Consider first the case
$$0{\lt}\alpha{\lt}1$$
. By differentiating once the expression for the Laplace transform, we obtain identity (5.9),
We are interested in the behavior of this derivative as
$$s\to 0+$$
. Using the inequality
$$|1-\mathrm{e}^{-x}|=1-\mathrm{e}^{-x}\le x$$
, we have
\begin{align*}
\bigg|\varphi'(s)-\frac{-{\mathbb{E}} [ \mathrm{e}^{-sX} X
]}{1-{\mathbb{E}}[\mathrm{e}^{-sX-\kappa_A (1-\varphi(s))}\kappa_A ]
}\bigg|&\le \frac{{\mathbb{E}} [ \kappa_A (1-\varphi(s)) \mathrm{e}^{-sX} X
]}{1-{\mathbb{E}}[\mathrm{e}^{-sX-\kappa_A (1-\varphi(s))}\kappa_A ] }
\\
&\le \frac{1-\varphi(s) }s\frac{{\mathbb{E}} [\kappa_A
\mathrm{e}^{-sX} sX ]}{1-{\mathbb{E}}[\mathrm{e}^{-sX-\kappa_A (1-\varphi(s))}\kappa_A
] }.
\end{align*}
As
$$\mathrm{e}^{-sX} sX\le \mathrm{e}^{-1},$$
we prove that
$${\mathbb{E}} [\kappa_A
\mathrm{e}^{-sX} sX ]=o(1)$$
as
$$s\to 0+$$
by dominated convergence. As in the proof of Lemma 5.1, the denominator
$$1-{\mathbb{E}}[\mathrm{e}^{-sX-\kappa_A
(1-\varphi(s))}\kappa_A ]$$
is controlled thanks to dominated convergence as well. Moreover, again using
$$1-\mathrm{e}^{-x}\le x$$
and denoting by
$$\varphi_X(s)={\mathbb{E}}[\mathrm{e}^{-sX}]$$
the Laplace transform of X, we have
so that
Collecting all these bounds and using the identity
$$\varphi'_X(s)=-{\mathbb{E}}[\mathrm{e}^{-sX}X]$$
, we obtain
The regular variation of the random variable D now follows from the regular variation of the random variable X by two consecutive applications of Theorem 5.2. First, as X is regularly varying of order
$$0{\lt}\alpha{\lt}1$$
, applying the direct part of the equivalence in Theorem 5.2 yields
Applying Karamata’s theorem, i.e. the equivalence between Equations (8.1.9) and (8.1.11b) of Bingham et al. (Reference Bingham, Goldie and Teugels1987, Theorem 8.1.6), we obtain
$$(1-\varphi_X(s))/s=O(\varphi'_X(s))$$
as
$$s\to 0+$$
. Using (5.14) and the limiting relation
we obtain
Finally, applying the reverse part of Theorem 5.2, we obtain
The case
$$1{\lt}\alpha{\lt}2$$
can be treated similarly, under the additional assumption that
$$Y=X + \kappa_A \mu_D$$
is regularly varying. We will again show that
$${P}(D{\gt}x)\sim (1-\kappa)^{-1}{P}(Y{\gt}x)$$
as
$$x\to \infty$$
. To prove this equivalence, recall identity (5.10),
As
$$\alpha{\gt}1$$
, we have that
$${\mathbb{E}}[Y]{\lt}\infty$$
and, thus,
$$
{\mathbb{E}}[X]{\lt}\infty$$
and
$$\mathbb{E}[D]=\mu_D=(1-\kappa)^{-1}{\mathbb{E}}[X]$$
. Observe that, for any
$$s{\gt}0$$
,
\begin{align*}
&\bigg|\varphi''(s)-\frac{{\mathbb{E}} [ \mathrm{e}^{-sY} Y^2
]}{1-{\mathbb{E}}[\mathrm{e}^{-sX-\kappa_A (1-\varphi(s))}\kappa_A ] }\bigg|
\\
&\qquad=\bigg|\frac{{\mathbb{E}}[\mathrm{e}^{-sX-\kappa_A (1-\varphi(s) )
} ( {-}\,X + \kappa_A \varphi' (s) )^2]-{\mathbb{E}} [
\mathrm{e}^{-sY} Y^2 ]}{1-{\mathbb{E}}[\mathrm{e}^{-sX-\kappa_A (1-\varphi(s))}\kappa_A
] }\bigg| .
\end{align*}
Let us decompose the numerator into two terms:
Using the identity
$$a^2-b^2=(a-b)(a+b)$$
,
$$I_1$$
is bounded by
\begin{align*}
I_1&\le (\mu_D + \varphi'(s)){\mathbb{E}}[\mathrm{e}^{-sX-\kappa_A
(1-\varphi(s))}\kappa_A (2X+\kappa_A (\mu_D-\varphi'(s)))]
\\
&\le \frac{\mu_D + \varphi'(s)}s({\mathbb{E}}[2\kappa_A
\mathrm{e}^{-sX}sX]+{\mathbb{E}}[\kappa_A \mathrm{e}^{-\kappa_A
(1-\varphi(s))}s(\mu_D-\varphi'(s))]).
\end{align*}
As
$$\mathrm{e}^{-sX}sX\le \mathrm{e}^{-1}$$
, then
$${\mathbb{E}}[2\kappa_A
\mathrm{e}^{-sX}sX]=o(1)$$
as
$$s\to 0^+$$
by dominated convergence. By the convexity of
$$\varphi(s)$$
we have
$$1-\varphi(s)\ge -\varphi'(s)s$$
for any
$$s{\gt}0$$
. Thus,
and the dominated convergence argument also applies to the second integrand as
$$-\varphi'(s)s\le 1-\varphi(s)=o(1)$$
. We obtain
$$I_1=o((\mu_D +
\varphi'(s))/s)$$
as
$$s\to 0^+$$
. In order to control the rate of
$$\left( {{\mu _D} + \varphi '(s)} \right)/s$$
, we note that
$$\varphi(s)$$
is
$$\mu_D$$
Lipschitz on
$$s\ge0$$
so that
$$|1-\varphi(s)|=1-\varphi(s)\le \mu_D s$$
. Then
and we bound
where
$$\varphi_Y(s)={\mathbb{E}}[\mathrm{e}^{-sY}]$$
denotes the Laplace transform of Y. It yields the estimates
$$\mu_D + \varphi'(s)=O(\mu_D +
\varphi_Y'(s))+ O(\kappa-{\mathbb{E}}[\mathrm{e}^{-sY }\kappa_A ])$$
. Again using the fact that
$$1-\mathrm{e}^{-x}\le x$$
on the second term, we obtain
$$I_1=o((\mu_D
+ \varphi_Y'(s))/s)+o(1)$$
as
$$s\to 0^+$$
.
We now turn to the term
$$I_2$$
that we identify as
As
$$1-\varphi(s)\le \mu_D s$$
, the term in the absolute value is negative for
$$s{\gt}0$$
and
Again using the basic inequality
$$1-\mathrm{e}^{-x}\le x$$
for
$$x\ge 0 $$
, we obtain the new estimate
\begin{align*}
I_2&\le {\mathbb{E}} [ \kappa_A (s\mu_D-(1-\varphi(s)) \mathrm{e}^{-sX-\kappa_A
(1-\varphi(s))}Y^2 ]
\\
&\le \frac{s\mu_D-(1-\varphi(s))}{s^2}{\mathbb{E}} [ \kappa_A
\mathrm{e}^{-sX-\kappa_A (1-\varphi(s))}(sY)^2 ].
\end{align*}
We have
As
$$\mathrm{e}^{-x} x^2\le 4\mathrm{e}^{-2}$$
for any
$$x{\gt}0$$
, we prove that
as
$$s\to 0^+$$
by dominated convergence. It remains to bound the term
uniformly for
$$s{\gt}0$$
sufficiently small. As
$$1-\varphi(s)\sim s\mu_D$$
as
$$s\to 0^+$$
, we have
$$0\le s\mu_D-(1-\varphi(s))\le 1-\varphi(s)$$
for sufficiently small s. Then we obtain
where the negligibility follows from dominated convergence and the basic inequality
$$\mathrm{e}^{-x} x^2\le 4\mathrm{e}^{-2}$$
for any
$$x{\gt}0$$
. We obtain
A similar computation to above yields
Thus, as
$$(s\mu_D-(1-\varphi(s))\le (s\mu_D-(1-\varphi_Y(s))/(1-\kappa)$$
and
$${\mathbb{E}}[Y]={\mathbb{E}}[X]+\kappa \mu_D=\mu_D$$
, we conclude that
as
$$s\to 0^+$$
. Let us first apply Theorem 5.2 on Y so that
$$\varphi''_Y(s)$$
is
$$\alpha-2$$
regularly varying around 0. Applying Karamata’s theorem again, i.e. the equivalence between (8.1.11b) and (8.1.9) (8.1.11b) and (8.1.10) of Bingham et al. (Reference Bingham, Goldie and Teugels1987, Theorem 8.1.6) respectively assert that
$$(s{\mathbb{E}}[Y]-(1-\varphi_Y(s)))/s^2=\smash{O(\varphi_Y''(s))}$$
and
$$\smash{({\mathbb{E}}[Y] + \varphi_Y'(s))/s=O(\varphi_Y''(s))}$$
as
$$s\to 0^+$$
. We then obtain
and, finally,
by applying the reverse part of Theorem 5.2.
We are now ready to characterize the asymptotic behavior of S(t) in the regularly varying case.
Theorem 5.3. Assume that the assumptions of Lemma 5.2 hold.
(i) If
$$\alpha \in (0,1)$$
and there exists
$$\delta{\gt}0$$
such that (5.15)then there exists a sequence
\begin{equation}
t ^{ \delta }{\mathbb{E}} [\tilde{\mu}_A(t,\infty)] \to 0\quad\text{as }t
{\to\infty},
\label{eqn34}
\end{equation}
$$(a_n),\, a_n{\to\infty},$$
and an
$$\alpha$$
-stable random variable
$$G_\alpha$$
such that
\begin{equation*}
\frac{S(t) }{ a_{\lfloor \nu t \rfloor} } \xrightarrow{\text{D}}
G_\alpha.
\end{equation*}
(ii) If
$$\alpha \in (1,2)$$
and (5.16)holds for some
\begin{equation}
t ^{1+\delta - 1/\alpha}
{\mathbb{E}} [\tilde{\mu}_A(t,\infty)] \to 0\quad\text{as }t {\to\infty}
\label{eqn35}
\end{equation}
$$\delta {\gt}0$$
, then there exists a sequence
$$(a_n),\,
a_n{\to\infty} ,$$
and an
$$\alpha$$
-stable random variable
$$G_\alpha$$
such that
\begin{equation*}
\frac{S(t) - t \nu \mu_D }{ a_{\lfloor \nu t \rfloor} } \xrightarrow{\text{D}} G_\alpha.
\end{equation*}
Proof. The proof is based on representation (3.1), and application of Propositions 4.1 and 4.2. In either case, it remains to show that
Consider first the case
$$\alpha \in (1,2)$$
. Since then
$$\mu_D =
{\mathbb{E}} D{\lt}\infty$$
, the argument in the proof of Theorem (5.1) still yields bound (5.12) on
$${\mathbb{E}} {\varepsilon}_t$$
. Using l’Hôpital’s rule again together with condition (5.16), we obtain
$${\mathbb{E}} {\varepsilon}_t
= o (t^{1/\alpha-\delta})$$
, where we assume without loss of generality that
$$\delta{\lt}1/\alpha$$
. Since
$$a_t = t^{1/\alpha} \ell(t)$$
for some slowly varying function
$$\ell$$
, it follows that
$${\varepsilon}_t
/a_t\xrightarrow{{\mathbb{P}\ }} 0$$
as
$$t{\to\infty}$$
.
For
$$\alpha \in (0,1)$$
, the random variable D has no finite mean. In order to prove that
$$ {\varepsilon}_t = o_P(a_t)$$
, we use the Markov inequality of order
$$0{\lt}\gamma{\lt}\alpha$$
as
$${\mathbb{E}} [D^\gamma]{\lt}\infty$$
. We will show that, under assumption (5.15),
By the sublinearity of
$$x\to x^\gamma,\,\gamma\le1$$
, we have
\begin{align*}
{\mathbb{E}}[{\varepsilon}_t^\gamma] &= {\mathbb{E}}\bigg[\bigg(
\sum_{{\Gamma_i} \leq t}\sum_j {{\bf 1}}_{\{\Gamma_i + T_{ij} {\gt}t\}}
X_{ij}\bigg)^\gamma\bigg]
\\
&= {\mathbb{E}}\bigg[\bigg(\sum_{\tau_i \leq t} \sum_{\tau_j {\gt} t}
D_{\tau_j} {{\bf 1}}_{\{\tau_i\to \tau_j\}}\bigg)^\gamma\bigg]
\\
&\leq {\mathbb{E}}\bigg[ \sum_{\tau_i \leq t} \sum_{\tau_j {\gt} t}
D_{\tau_j}^\gamma {{\bf 1}}_{\{\tau_i\to \tau_j\}} \bigg]
\\
&={\mathbb{E}}\bigg[\sum_{\tau_i \leq t}
{\mathbb{E}}\bigg[\sum_{k=1}^{L^{i}} D_{\tau_i+W_{ik}}^\gamma
{{\bf 1}}_{\{\tau_i+W_{ik} {\gt} t\}} \biggm| (\tau_i,A^i)_{i\ge 0}; \,\tau_i \le
t\bigg]\bigg]
\\
&= {\mathbb{E}}[D^\gamma] {\mathbb{E}} \bigg[ \int_{0}^t
\int_{\mathbb{S}} \tilde{\mu}_a((t-s,\infty)) N(\mathrm{d} s,\,\mathrm{d} a) \bigg].
\end{align*}
We can again compare the marked Hawkes process N with a stationary version of it,
$$N^*$$
say. By the same arguments as in the proof of Theorem 5.1, we obtain
By regular variation of order
$$1/\alpha$$
of
$$(a_t)$$
we have
$$t^{\gamma/\alpha-\delta'}=o(a_t^\gamma)$$
for any
$$\delta'{\gt}0$$
. Once again we use a Cesaró argument to prove that
$${\mathbb{E}}
[{\varepsilon}_t^\gamma]=o(a_t^\gamma)$$
under the condition that
As
$$\gamma$$
can be taken as close as possible to
$$\alpha$$
, the result holds under assumption (5.15).
Acknowledgements
The work of Bojan Basrak and Olivier Wintenberger was supported in part by the AMERISKA network, project ANR-14-CE20-0006. The work of Bojan Basrak was supported in part by the Croatian Science Foundation under project 3526, and by the European Regional Development Fund, under grant KK.01.1.1.01.0009 (DATACROSS). The authors thank Philippe Soulier for pointing out the work of Hult and Samorodnitsky (Reference Hult and Samorodnitsky2008).