The deficit at the time of ruin

28 X.S. Lin, G.E. Willmot Insurance: Mathematics and Economics 27 2000 19–44 Now, for any i = 0, 1, . . . , and j = 0, 1, . . . , Z ∞ u x − u j µx i i e −µx dx = µ i i e −µu Z ∞ x j x + u i e −µx dx = µ i i e −µu i X k=0 i k u k Z ∞ x j +i−k e −µx dx = µ −j −1 e −µu i X k=0 j + i − k i − k µu k k . Thus, α n u, ρ = e −µu ∞ X k=0 ¯ C ∗ k,n µu k k , 3.17 where ¯ C ∗ k,n = ∞ X i=0 ¯ C k+i   βµ −n−1 µ n ρ n + i i − n−1 X j =0 n j µ n−j ρµ −j −1 µ n ρ j + i i   . In the rest of this paper, we turn to evaluation of φu for a particular weight function wx, y.

4. The deficit at the time of ruin

In this section we consider in more detail the possibly discounted deficit at the time of ruin beginning with the moments. We are focusing on their analytic solutions. For numerical algorithms, see Dickson et al. 1995 and the references therein. Consider the special case wx 1 , x 2 = x k 2 , where k is a positive integer. A relatively simple representation exists for φu in 1.1. Theorem 4.1. For k = 1, 2, 3, . . . , E{e −δT |U T | k T ∞} = 1 βψu [kµ k−1 ρα k−1 u, ρ − µ k ρ ¯ Ku], 4.1 where µ n ρ = R ∞ x n dGx is given in 2.7 and α n u, ρ is given in Theorem 3.1. Proof. Using 2.4 and 2.8, Eq. 1.8 becomes, with wx 1 , x 2 = x k 2 , H u = e ρu R ∞ u e −ρx R ∞ x y − x k dP y dx R ∞ e −ρy ¯ P y dy = p k e ρu R ∞ u e −ρx ¯ P k x dx p 1 R ∞ e −ρy dP 1 y = p k R ∞ e −ρy ¯ P k y dy p 1 R ∞ e −ρy dP 1 y ¯ G k u. Furthermore, using 2.3, H u = p k+1 R ∞ e −ρy dP k+1 y k + 1p 1 R ∞ e −ρy dP 1 y ¯ G k u, and from 2.6 and 2.7, we obtain the simple result H u = µ k ρ ¯ G k u. 4.2 X.S. Lin, G.E. Willmot Insurance: Mathematics and Economics 27 2000 19–44 29 Then, using 3.1, since ¯ G k u = R ∞ u ¯ G k−1 x dxg k−1 ρ, we obtain H ′ u = − µ k ρ g k−1 ρ ¯ G k−1 u = −kµ k−1 ρ ¯ G k−1 u, and from 1.17, φ u = kµ k−1 ρ β Z u ¯ Ku − x ¯ G k−1 x dx + µ k ρ β Z ∞ u ¯ G k−1 x g k−1 ρ dx − µ k ρ β ¯ Ku = kµ k−1 ρ β Z u ¯ Ku − x ¯ G k−1 x dx + Z ∞ u ¯ G k−1 x dx − µ k ρ β ¯ Ku = kµ k−1 ρ β α k−1 u, ρ − µ k ρ β ¯ Ku, using 3.3. That is, E{e −δT |U T | k I T ∞} = kµ k−1 ρ β α k−1 u, ρ − µ k ρ β ¯ Ku, 4.3 and division by ψu gives 4.1. When k = 1, with the help of 3.5, 4.3 reduces to E{e −δT U T |I T ∞} = Z ∞ u ¯ Kx dx − µ 1 ρ β ¯ Ku. 4.4 When δ = 0 we have the following important corollary. Corollary 4.1. For k = 1, 2, 3, . . . , E{|U T | k T ∞} = p k p 1 θ τ k u ψu − p k+1 k + 1p 1 θ , 4.5 where τ k u is given in Corollary 3.1. Proof. When δ = 0, ¯ Ku = ψu, α k−1 u, 0 = τ k u, µ n 0 is given by 2.6, and β = θ . Then 4.1 reduces to 4.5. When k = 1, 4.5 reduces to using 3.10 E{|U T | T ∞} = Z ∞ u ψx ψu dx − p 2 2p 1 θ . 4.6 The second moment of the deficit, hence the variance of the deficit, can also easily be evaluated from 4.5. As demonstrated in Examples 3.1 and 3.2, ψu and τ k u can be computed explicitly when P x is a combination of exponentials, a mixture of Erlangs, or approximated using a Tijms approximation. Thus, with the help of 4.5 the moments of the deficit |U T | are also obtainable as shown in the following examples. Example 4.1 Combinations of exponentials. We again begin with an exponential. In this case, E{|U T | k T ∞} = p k p 1 θ τ k u ψu − p k+1 k + 1p 1 θ = kµ −k µ −1 θ µ −1 e −Ru 1 + θ −1 e −Ru − k + 1µ −k−1 k + 1µ −1 θ = kµ −k , which agrees with the fact that in the exponential case the deficit is also exponentially distributed and it is independent of the time of ruin. 30 X.S. Lin, G.E. Willmot Insurance: Mathematics and Economics 27 2000 19–44 Next, we examine a combination of two exponentials. This is also the case when a Tijms approximation is used. It follows from 3.16 that E{|U T | k T ∞} = p k p 1 θ τ k u ψu − p k+1 k + 1p 1 θ = ˆ C 1,k e −R 1 u + ˆ C 2,k e −R 2 u C 1 e −R 1 u + C 2 e −R 2 u , 4.7 where ˆ C 1,k = kC 1 R −k 1 p 1 θ   p 1 θ − k X j =1 p j +1 R j 1 j + 1   , ˆ C 2,k = kC 2 R −k 2 p 1 θ   p 1 θ − k X j =1 p j +1 R j 2 j + 1   . Example 4.2 Mixtures of Erlangs. For a mixture of Erlangs claim size distribution, it follows immediately from Example 3.2 that the kth unconditional discounted moment is E{e −δT |U T | k I T ∞} = e −µu ∞ X j =0 ˆ C j,k µu j j , 4.8 where ˆ C j,k = 1 β [kµ k−1 ρ ¯ C ∗ j,k−1 − µ k ρ ¯ C j ]. The constants ¯ C ∗ j,k−1 and ¯ C j are given in Example 3.1. We remark that when the individual claim size is a combination of exponentials or a mixture of Erlangs, the density function of the deficit is of the same type but with new weights. These weights are expressed as functions of the initial surplus u. As a result, the moments of the deficit can be calculated accordingly for details, see Willmot 2000. The method we employed in this section provides a different approach in calculating the moments of the deficit. Under this method, the moments of the deficit are calculated directly. The coefficients in 4.7 and 4.8 are independent of the initial surplus u, which allows for the calculation of the moments of the deficit for different values of u without reevaluating the distribution of the deficit. Another advantage of this approach is that we are able to evaluate the expected discounted deficit using 4.1, which the approach in Willmot 2000 cannot. Next, we consider bounds for functions of the deficit. Theorem 4.2. If P x is IMRL DMRL, then for k = 1, 2, 3, . . . , E{e −δT |U T | k I T ∞} ≥ ≤µ k ρ ¯ Ku. 4.9 Proof. By Theorem 3.2b of Lin and Willmot 1999, Gx is IMRL DMRL. This implies Fagiuoli and Pellerey, 1994 that the j th equilibrium DF G j x is NWUE NBUE, i.e., ¯ G j +1 x ≥ ≤ ¯ G j x. Then by 4.2, H u = µ k ρ ¯ G k u ≥ ≤µ k ρ ¯ G k−1 u ≥ ≤ · · · ≥ ≤µ k ρ ¯ Gu. Thus, Theorem 4.1 of Lin and Willmot 1999 applies, which shows that if H u ≤ ≥c ¯ Gu, then φu ≤ ≥c ¯ Ku, and the result is proved. To derive a simple bound for more general functions of the deficit, we recall a result in Lin and Willmot 1999. X.S. Lin, G.E. Willmot Insurance: Mathematics and Economics 27 2000 19–44 31 Lemma 4.1. If ηx = 1 ¯ P x Z ∞ x wx, y − x dP y ≤ ≥c, 4.10 where 0 c ∞, then φu ≤ ≥c ¯ Ku. With the help of Lemma 4.1, we have the following simple bound. Theorem 4.3. Suppose that Ay = 1 − ¯ Ay is a DF on 0, ∞ satisfying ¯ P x + y ¯ P x ≥ ≤ ¯ Ay, x ≥ 0, y ≥ 0. 4.11 Then if wx is nondecreasing in x, E{e −δT w|U T |I T ∞} ≥ ≤ Z ∞ wy dAy ¯ Ku, u ≥ 0. 4.12 Proof. Let Z x for x ≥ 0 be a random variable such that PrZ x y = ¯ P x + y ¯ P x. Then with wx 1 , x 2 = wx 2 , 4.10 may be expressed as ηx = E{wZ x }. Then by 4.11 and Ross 1996, p. 405, if wx is nonde- creasing, then ηx ≥ ≤ R ∞ wy dAy. It is clear from the proof of Theorem 4.3 that if 4.11 holds and wx is nonincreasing in x, then inequality 4.12 is reversed. The key to the application of Theorem 4.3 is to identify the DF Ay for a given P x. If P x is NWU NBU, then 4.11 holds with Ay = P y. For more details on the choice of P x, see Willmot and Lin 1997. It is worth noting that Eq. 4.12 may be written when δ = 0 as E{w|U T | T ∞} ≥ ≤ Z ∞ wy dAy. 4.13 In the special case when wx 1 , x 2 = x k 2 and P x is DFR IFR, from Ross 1996, p. 405 and Theorem 3.5, µ k ρ ≥ ≤p k , and Theorem 4.2 gives a tighter bound than Theorem 4.3. If P x = 1 − exp−xp 1 and wx 1 , x 2 = wx 2 , then ηx = R ∞ wy dP y independent of x and H u = { R ∞ wy dP y} ¯ Gu, implying that φu = { R ∞ wy dP y} ¯ Ku. Thus, with wy = e −sy , E{exp[−δT − s|U T |]I T ∞} = 1 + p 1 s −1 E{e −δT I T ∞}. 4.14 Eq. 4.14 may be viewed as the joint Laplace transform of the defective distribution of T and |U T |, implying that T and |U T | are independent conditional on T ∞, and that |U T | is exponential with mean p 1 . This result is given by Gerber 1979, p. 138. The Laplace transform of the deficit for arbitrary claim size DF can also be evaluated in a similar manner. In that case, we simply let wx 1 , x 2 = e −sx 2 . However, the resulting formula will be complicated, except when the claim size is exponentially distributed as discussed above.

5. Surplus before the time of ruin

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