A zero-one law of almost sure local extinction for (1 + β)-super-Brownian motion Xiaowen Zhou 1 Department of Mathematics and Statistics, Concordia University, 1455 de Maisonneuve Blvd. West, Montreal, Quebec, H3G 1M8, Canada E-mail address:[email protected] Abstract This paper considers the almost sure local extinction for d-dimensional (1 + β)-superBrownian motion X starting at Lebesgue measure on Rd . Given closed balls (Bg(t) )t>0 centered at 0 and with radiuses g(t) that are non-decreasing and right continuous in time t, let τ := sup{t : Xt (Bg(t) ) > 0}. For dβ < 2, it is shown that P{τ = ∞} is equal to either 0 or 1 depending on whether the R∞ value of integral 1 g(y)d y −1−1/β dy is finite or infinite. An asymptotic bound for P{τ > t} is given when P{τ < ∞} = 1. Keywords: (1+β)-super-Brownian motion, almost sure local extinction, zero-one law, historical super-Brownian motion, integral test AMS Subject Classification 2000: 60G57, 60J80 1. Introduction Given a positive integer d and a constant d < p < d + 2, write φp (x) := (1 + |x|2 )−p/2 , x ∈ Rd ; write Fp for the collection of all nonnegative continuous functions φ on Rd such that supx φ(x)/φp (x) < ∞; write Mp for the set of all measures µ on Rd such that µ(φp ) < ∞. For 0 < β ≤ 1 the d-dimensional (1 + β)-super-Brownian motion X with branching rate γ > 0 and initial measure m ∈ Mp is a measure-valued stochastic process with its probability law specified by the Laplace functional h i Pm e−Xt (φ) = e−m(Vt φ) , where for φ ∈ Fp , v(t, x) := Vt φ(x) solves the nonlinear p.d.e. ∂v(t, x) 1 γ = ∆v(t, x) − v(t, x)1+β , v(0, x) = φ(x). ∂t 2 1+β 1This work is supported by an NSERC grant. 1 2 Such a process arises from the scaling limit of empirical measures of critical branching motions in which the offspring distributions are in the domain of attraction for stable law. The persistence-extinction dichotomy is well known for super-Brownian motion. In low dimensions the super-Brownian motion X, started at Lebesgue measure λ, suffers local extinction; i.e. Xt (A) → 0 in probability as t → ∞ for any compact set A. On the other hand, in high dimensions X started at λ is persistent; i.e. the limiting random measure X∞ of (Xt ) satisfies P[X∞ ] = λ, and consequently the local extinction can not happen. It is known that X is persistent if and only if dβ > 2. For the case dβ = 2, Xt (A) converges to 0 in probability, but not almost surely. See [1] for the earliest work and Sections 5.2 and 5.3 of [7] for a more detailed discussion. It was first proved in [10] that almost surely Xt (A) = 0 for t large enough if X is the onedimensional 2-super-Brownian motion, and we say X suffers almost sure local extinction. A key fact which was first obtained in [9] was that the Laplace functional of weighted local time for super-Brownian motion can be expressed in terms of nonlinear p.d.e. The proof for the almost sure local extinction then relied on analyzing the weighted local time using the corresponding p.d.e.. A stronger version of the local extinction property can be found in Proposition 3.2 of [8]. For any η, it is shown that starting with Lebesgue measure λ on R, almost surely Xt ([−tη , tη ]) = 0 for t large enough. Also see Proposition 7 of [4] for another result along this line. We also refer to [8] and [4] for the applications of such results in the study of super-Brownian motion in random medium. In this paper we further improve the known results on almost sure local extinction for (1+β)super-Brownian motion with Lebesgue initial measure on Rd . For d < 2/β, given (Bg(t) ), a collection of closed balls in Rd with non-decreasing and right continuous radiuses g(t), we show that almost surely Xt (Bg(t) ) = 0 for t large enough provided Z ∞ g(y)d y −1−1/β dy < ∞. 1 Our approach is similar to those in [8] and [10]. It exploits the additivity (branching property), the extinction probability for super-Brownian motion and the asymptotic speed of propagation for super-Brownian motion support. To illustrate the idea we only consider the case such that d = 1, β = 1 and At = [−ta , ta ], 0 < a < 1, the proof can be sketched as follows. For large t the super-Brownian motion started at the Lebesgue measure restricted on interval [−ta − tδ , ta + tδ ] with 1/2 < δ < 1 can only survive up to time t with probability of the order ta∨δ−1 . In addition, for large t the “front” of support for the super-Brownian motion started at the Lebesgue measure restricted on the complement of the interval [−tα − tδ , tα + tδ ] can not move toward 0 at a speed much faster than t1/2 . Consequently, the support for the later pro0 cess can only intersect interval [−tα , tα ] with probability of the order e−tδ for 0 < δ 0 < 2δ + 1. 3 Choosing a sequence (tn ) that increases geometrically, the desired result then follows readily form Borel-Cantelli lemma. On the other hand, with d < 2/β, for any constant c > 0 the time-space-mass scaling −1/β t Xt (Bct1/dβ ) converges in distribution to a Poisson sum of i.i.d. Gamma random variables as t → ∞; see Theorem 3.1 of [3]. It follows that lim sup P{Xt (Bct1/dβ ) > 0} > 0. t→∞ Consequently, the above-mentioned almost sure local extinction can not happen for (Bct1/dβ ). In this paper we also find a more general condition in terms of a similar integral test on g, under which the almost sure local extinction does not occur for X with respect to regions (Bg(t) ). More precisely, we show that P{sup{t : Xt (Bg(t) ) > 0} = ∞} = 1 if Z ∞ g(y)d y −1−1/β dy = ∞. 1 For d = 1, β = 1 and g(t) = 2t/ ln t for t large enough, the proof proceeds as follows. For tn := 2n , n = 1, 2, . . ., write X n for independent super-Brownian motion with initial measure the Lebesgue measure restricted to interval (tn−1 / ln tn−1 , tn / ln tn ), respectively. The extinction probability for super-Brownian motion gives P{Xtnn (1) > 0} ≥ c/n for some c > 0 and for all n large enough. It then follows from Borel-Cantelli lemma that with probability one Xtnn (1) > 0 for infinitely many n. Since the support for X n can not propagate much faster than t1/2 , by Borel-Cantelli again Xtnn (R − [−g(tn ), g(tn )]) > 0 for only finitely many n. The desired result follows. These integral tests on almost sure local extinction for super Brownian motion answer a question asked by Edwin Perkins. This paper is arranged as follows. Using the modulus of continuity for historical superBrownian motion, in Section 2 we first present several estimates on the hitting probability of Br by the super-Brownian motion. We then obtain the zero-one law on the almost sure local extinction in Section 3. An old result is also revisited in Section 3. 2. Preliminaries Recall that for m ∈ Mp the Laplace functional for the total mass has the expression ( µ ) ¶1 β 1+β (2.1) Pm [exp{−αXt (1)}] = exp − αm(1) , 1 + β + γβtαβ which implies the extinction probability (2.2) ) ( µ ¶1 1+β β m(1) . Pm {Xt (1) = 0} = exp − γβt 4 Write MFt (D) for the set of finite measures on D(Rd ) supported by paths which are constant after time t. Let H, under Q0,m , be the historical (1+β)-super-Brownian motion corresponding to X. Then Ht is MFt (D)-valued with Xt as its projection at t. It keeps track of the history of all the “individuals” in a super-Brownian motion that are still “alive” at time t . We refer to [6] and [11] for explicit definition and more discussions on historical processes. To prove Lemma 2.2 we need a result on the historical modulus of continuity for H. Such a result is well known for 2-super-Brownian motion. For (1 + β)-super-Brownian motion it was proved in [5]. Lemma 2.2 can be obtained by following the line of proof for Theorem III.1.3. of [11]. Write S(Ht ) for the support for Ht . Lemma 2.1. Given a d-dimensional historical (1 + β)-super-Brownian motion H and m ∈ MF0 (D), for c > 2 large enough there exists a random variable ∆ > 0 such that Q0,m a.s. for all t ≥ 0, S(Ht ) ⊂ {y ∈ C(R) : |y(r) − y(s)| ≤ c|(r − s) log(|r − s|)|1/2 , ∀r, s > 0, |r − s| ≤ ∆}. Moreover, there are constants ρ = ρ(β) > 0 and c = c(d, β, c) > 0 such that Q0,m {∆ ≤ r} ≤ cm(1)rρ . (2.3) For any A ∈ B(Rr ) write λ1(A) for the Lebesgue measure restricted on A, i.e. λ1(A)(B) = λ(A ∩ B). Write Br := {x ∈ Rd : |x| ≤ r} for r > 0. Write Xr = Xr,· for a d-dimensional (1 + β)-super-Brownian motion with initial measure Xr,0 = λ1(Bcr ), Bcr = Rd − Br . Write Sr,· for the support process for Xr,· . The following result gives an estimate on the speed of propagation for a super-Brownain motion over time. Roughly, its support can not move much faster that t1/2 . Lemma 2.2. Given a > 0 and δ > 1/2, for any δ 0 with 0 < δ 0 < 2δ − 1 we have (2.4) © ª 0 lim exp{tδ } sup P ∃s ≤ t, Xr+tδ ,s (Br ) > 0 = 0. t→∞ r≤ta Proof. Given t > 0 and 0 < r < ta , write X·j for independent historical super-Brownian motion with initial measures mj := λ1(Br+tδ +tδ(j+1) − Br+tδ +tδj ), j = 0, 1, 2, . . . . Write H·j for the corresponding historical super-Brownian motion. Note that we have suppressed the dependence of X·j and H·j on both t and r. Put A(t0 , r0 ) := {y ∈ C(Rd ) : inf0 |y(s)| ≤ r0 }. s≤t 5 l m l m 00 00 Given δ 0 < δ 00 < 2δ − 1, let l0 := t exp{tδ } and lj := t exp{tδ j } for j > 0. Then for t large enough we have ∞ © ª X © ª P ∃s ≤ t, Xr+tδ ,s (Br ) > 0 ≤ P ∃s ≤ t, Xsj (Br ) > 0 j=0 (2.5) ≤ ∞ X © ª Q0,mj ∃s ≤ t, Hsj (A(s, r)) > 0 . j=0 n o To estimate Q0,mj ∃s ≤ t, Hsj (A(s, r)) > 0 , by Lemma III.1.2. (for (1+β)-branching superBrownian motion) in [11], for j > 0 we first have n o j Q0,mj H(i+1)t/l (A(it/l , r + 1)) > 0 j j " ( µ )# ¶1 1+β β j = 1 − Q0,mj exp − Hit/lj (A(it/lj , r + 1)) γβt/lj µ ¶1 i h 1 1+β β j β (A(it/l , r + 1)) . ≤ lj Q0,mj Hit/l j j γβt Since the mean measure of Hj (r) under Q0,mj is the Wiener measure stopped at time r, then for 1 ≤ i ≤ lj − 1 we then have i h j (A(it/l , r + 1)) ≤ mj (1)P Q0,mj Hit/l j j ≤ ( 2dmj (1) √ 2π ) sup |Ws | > tδ + tδj − 1 s≤it/lj Z ∞ tδ +tδj −1 idt/lj √ e−x 2 /2 dx ½ 2δj ¾ t ≤ mj (1) exp − , 2dt where W is a d-dimensional Brownian motion starting at 0 and t is large enough. Let Tj := inf{t : X j (Br ) > 0} with the convention inf ∅ = ∞. For Tj < ∞ choose a nonnegative integer i such that it/lj ≤ Tj < (i + 1)t/lj . Then for i ≥ 1, by time (i − 1)t/lj either the super-Brownian motion X j has already charged the set Br+1 or it has not charged Br+1 yet. In the later case we must have ∆ ≤ 2t/lj because the support process for X j has to travel a distance of at least 1 between time (i − 1)t/lj and time T . For i = 0 the support process also has to travel a long distance between time 0 and time T , which implies ∆ < t/lj . Putting these together, by Lemma 2.1 we 6 have © ª Q0,mj ∃s ≤ t, Hsj (A(s, r)) > 0 lj −1 ≤ X i=1 o n j (A(it/l , r + 1)) > 0 + Q0,mj {∆ ≤ 2t/lj } Q0,mj H(i+1)t/l j j ¶1 ½ 2δj ¾ 1 + β β β1 t 00 ≤ lj mj (1) exp − + cmj (1)2ρ exp{−ρtδ j } γβt 2dt i=1 ¶1 µ ½ 2δj−1 ¾ 1 + β β 1+ β1 t 00 lj mj (1) exp − + cmj (1)2ρ exp{−ρtδ j }. ≤ γβt 2d P∞ Since X has the same distribution as j=0 Xj , limit (2.4) follows from (2.5) and (2.6). (2.6) lj −1 µ X ¤ We can make δ depend on t in Lemma 2.2 by modifying the proof for Lemma 2.2. Lemma 2.3. Given a > 0 and k > 0, for the processes considered in Lemma 2.2 there exists k 0 > 0 such that n o lim tk sup P ∃s ≤ t, Xr+k0 (t ln t)1/2 ,s (Br ) > 0 = 0. t→∞ r≤ta Proof. We can choose 1/2 < δ < 1. Choose q satisfying qρ − d(a ∨ δ) > k and put lj = dt1+qj e, j ≥ 0. Put mj = λ1(Br+k0 (t ln t)1/2 +tδ(j+1) − Br+k0 (t ln t)1/2 +tδj ), j ≥ 0, where k 02 > 2d [d(a ∨ δ) + (1 + q)(1 + 1/β) + k] . Then just follow the line of proof for Lemma 2.2. ¤ Remark 2.4. In dimension one both Lemma 2.2 and Lemma 2.4 can be improved in the sense that the supreme is taken for all t > 0 instead of for 0 < t ≤ ta . Remark 2.5. If the Xr in Lemma 2.2 is replaced by a d-dimensional (1 + β)-super-Brownian motion with initial measure Xr,0 = λ1(Bg(r) ), where g is any nonnegative increasing function such that ∃δ > 0, lim inf g(t)/t1/2+δ > 0, t→∞ then by a similar argument we can show that for any δ 0 , δ 00 > 0, n ³ ´ o 0 lim g(t)δ P Xt,t Bc(1+δ00 )g(t) > 0 = 0. t→∞ The proof for the next result also follows that for Lemma 2.2. 7 Lemma 2.6. Let (Xr,· ) be a collection of d-dimensional (1 + β)-super-Brownian motion with initial measures Xr,0 = λ1(Br ), r > 0. Then for any a > 0, δ > 1/2 and 0 < δ 0 < 2δ − 1, we have ª © 0 lim exp{tδ } sup P ∃s ≤ t, Xr,s (Bcr+tδ ) > 0 = 0. t→∞ r≤ta 3. Main results Let g(t), t ≥ 0, be any nonnegative, nondecreasing and right continuous function. Define τ := sup{t ≥ 0 : Xt (Bg(t) ) > 0}. τ is then the first time when almost sure local extinction occurs with respect to (Bg(t) ). It is not a stopping time. Theorem 3.1. Let X be a d-dimensional (1 + β)-super-Brownian motion such that X0 = λ and dβ < 2. If Z ∞ −1− β1 dy < ∞, (3.1) g(y)d y 1 then (3.2) P{τ < ∞} = 1. Moreover, (3.3) µ Z d d − β1 2 (ln t) 2 ∨ lim sup P{τ > t} t t→∞ ∞ 1 d −1− β g(y) y ¶−1 dy < ∞. t Proof. For n = 1, 2, . . . put tn = en and rn = g(tn+1 ) + k 0 (tn+1 ln tn+1 )1/2 , where k 0 is obtained from Lemma 2.3 for a = (1 + β −1 )/d and k = 2. Throughout the proof for part (i) we write X·n and Y·n for independent (1+β)-super-Brownian motion with X0n = λ1(Brn ) and Y0n = λ1(Bcrn ), respectively. Then X· has the same distribution as X·n + Y·n . Condition (3.1) and the monotonicity of g give lim g(y)d y y→∞ −1− β1 = 0. Then it follows form Lemma 2.3 that for m large enough and n ≥ m, P{∃t < tn+1 , Ytn (Bg(tn+1 ) ) > 0} ≤ t−2 n+1 . 8 Applying (2.2) we have P{∃t ≥ tn , Xtn (Bg(tn+1 ) ) > 0} ≤ P{∃t ≥ tn , Xtn (Rd ) > 0} Ã µ ! ¶1 1+β β = 1 − exp − λ(Brn ) γβtn ¶1 µ 1 + β β d d − β1 ≤ 2 rn tn γβ µ ¶1 ´ −1 d 1+β β d ³ ≤ 2 d g(tn+1 )d + k 0d (tn+1 ln tn+1 ) 2 tn β γβ µ ¶1 µ ¶ 1 d 1 d 1 + β β d β1 d −β 0d 2 − β ≤ 2 de g(tn+1 ) tn+1 + k tn+1 (ln tn+1 ) 2 . γβ Plainly, P{∃tn ≤ t < tn+1 , Xt (Bg(tn+1 ) ) > 0} ≤ P{∃tn ≤ t < tn+1 , Xtn (Bg(tn+1 ) ) > 0} + P{∃tn ≤ t < tn+1 , Ytn (Bg(tn+1 ) ) > 0}. Moreover, for m large enough, ∞ X P{∃tn ≤ t < tn+1 , Xtn (Bg(tn+1 ) ) > 0} n=m (3.4) ¶1 µ ¶ ∞ µ 1 d 1 X d 1 + β β d β1 d −β 0d 2 − β 2 g(tn+1 ) tn+1 + k tn+1 (ln tn+1 ) ≤ 2 de γβ n=m µ ¶ 1 µZ ∞ ¶ Z ∞ 1 d 1 1 1+β β 0d x 2−β x d2 d β x d x−1 − β (e ) (ln e ) dx ≤ d2 e g(e ) (e ) dx + k γβ m+1 m+1 ! ¶1 Ã Z ∞ µ Z ∞ β 1 1 1 1 d d 1 + β − −1 −1− β eβ ≤ d2d e β dy + k 0d g(y)d y y 2 β (ln y) 2 dy γβ tm+1 tm+1 ! 1 ÃZ µ ¶ Z ∞ ³ 1 ´ 1+β β ∞ 1 1 d 1 d −1− − −1 0d d d β β dy ∨ g(y) y y 2 β (ln y) 2 dy . ≤ d2 e e β + k γβ tm+1 tm+1 Then Borel-Cantelli lemma together with the assumptions of Theorem 3.1 implies that almost surely, for n large enough, Xt (Bg(tn+1 ) ) = 0 for all t > tn . Finally, observe that {(x, t) : tn < t ≤ tn+1 , x ∈ Bg(t) } ⊂ {(x, t) : t > tn , x ∈ Bg(tn+1 ) }. The desired result (3.2) follows from {(x, t) : t > tm , x ∈ Bg(t) } ⊂ [ {(x, t) : tn < t ≤ tn+1 , x ∈ Bg(tn+1 ) }. n≥m 9 The estimate (3.3) follows form (3.4) and the inequality Z ∞ d d d d 4β − 1 −1 −1 y 2 β (ln y) 2 dx < t 2 β (ln t) 2 . 2 − dβ t . ¤ Remark 3.2. The estimate (3.3) reveals that E(τ ) < ∞ for g(t) = tα with α ≥ 0 if (1/2 ∨ α)d < 1/β − 1. To justify the sharpness of Theorem 3.1 we present the next result. The zero-one law follows readily. Theorem 3.3. For dβ < 2 let X be a d-dimensional (1 + β)-super-Brownian motion such that X0 = λ. If Z ∞ −1− β1 (3.5) g(y)d y dy = ∞, 1 then (3.6) P{τ = ∞} = 1. Proof. We can and will assume that g(1)/3 < 1. Choose ² > 0 satisfying (3.7) d/2 − 1/β + d² < 0. Because of (3.5) and (3.7) either g(t)/3 ≥ t1/2+² for all t large enough or there exists a finite, strictly increasing sequence (si ) such that s1 := 1, s2i := inf{s > s2i−1 : g(s)/3 ≥ 2s1/2+² } and s2i+1 := inf{s ≥ s2i : g(s)/3 < s1/2+² } for i = 1, 2, . . .. We only prove (3.6) for the second case, which is more involved. In this case observe that si → ∞, (3.8) g(s2i −)/3 ≤ 2s1/2+² ≤ g(s2i )/3 and g(s2i−1 −)/3 = g(s2i−1 )/3 = s1/2+² , where g(s−) denotes the left limit of g(·) at s. In addition, (3.9) g(s)/3 ≤ 2s1/2+² for s ∈ (s2i−1 , s2i ) and g(s)/3 ≥ s1/2+² for s ∈ (s2i , s2i+1 ). 10 We further define strictly increasing sequences (ti ) and (ni ) such that tni = si ; tk ≤ 2tk−1 for k = n2i−1 + 1, . . . , n2i ; and tk := inf{tk−1 < t ≤ s2i+1 : g(t) ≥ 2g(tk−1 )} for k = n2i + 1, . . . , n2i+1 , where we use the convention that inf ∅ := s2i+1 . Notice that 2g(tn2i ) < g(tn2i+2 ) and (3.10) g(tk+1 ) ≥ 2g(tk ) ≥ g(tk+1 −) for n2i ≤ k ≤ n2i+1 − 1. Put rn := g(tn+1 −)/3. Write (X·n )n≥1 for independent (1 + β)-super Brownian motions ¢ ¡ starting at λ1(Brn − Brn−1 ) n≥1 . To reach (3.6) it suffices to show that with probability one, Xtjj (Bg(tj ) ) > 0 for infinitely many j. Observe that Z tn Z tn −1− β1 −1− β1 dy ≤ g(tn −)d dy g(y)d y y t t n−1 n−1 (3.11) −1 −1 β ≤ βg(tn −)d (tn−1 − tn β ). In addition, (3.12) ( µ ) ¶1 β 1 + β P{Xtnn (1) > 0} = 1 − exp − λ(Brn − Brn−1 ) γβtn ( µ ) ¶1 1 1+β β −1 ≥ min λ(Brn − Brn−1 ), 1 − e 3 γβtn ) ( µ ¶1 ³ ´ 1 1+β β c(d) g(tn+1 −)d − g(tn −)d , 1 − e−1 ≥ min 3 γβtn where c(d) is a positive constant and we have used inequality 1 − e−x ≥ x/3 for 0 ≤ x ≤ 1. Since ∞ ∞ ³ ´ X X −1 −1 − β1 −1 tn β g(tn+1 −)d − g(tn −)d ≥ −t1 β g(t1 −)d + g(tn −)d (tn−1 − tn β ), n=1 n=2 combining (3.5), (3.11) and (3.12) we have ∞ X (3.13) P{Xtnn (1) > 0} = ∞. n=1 Further, we define a sequence (aj ) such that g(t −) for n j 2i−1 ≤ j ≤ n2i , i = 1, 2, . . . ; aj := g(tn −) for n2i < j < n2i+1 , i = 1, 2, . . . . 2i 11 Then ∞ nX 2i −1 X P{Xtjj (1) > 0} ≤ ³ ´ −1 tj β c(d, β, γ) g(tj+1 −)d − g(tj −)d ∞ nX 2i −1 X i=1 j=n2i−1 i=1 j=n2i−1 ≤ c(d, β, γ) ∞ X − β1 tj ³ ´ adj+1 − adj j=1 ≤ c(d, β, γ) (3.14) ∞ X − β1 adj+1 (tj −1 β − tj+1 ) j=1 ≤ c(d, β, γ) ∞ 1 X − β1 1/2+² d − β ) (12tj ) (tj − tj+1 j=1 Z ≤ c∗ (d, β, γ) ∞ td/2−1/β+d²−1 dt t1 < ∞, where c(d, β, γ) and c∗ (d, β, γ) are the obvious constants. To obtain the third inequality of (3.14) we use the fact that by (3.7) and (3.9), −1/β tj g(tj+1 −)d → 0 for n2i−1 ≤ j ≤ n2i − 1 and i → ∞. We also need (3.8) to obtain the fourth inequality. Inequalities (3.13) and (3.14)together leads to ∞ n2i+1 X X−1 P{Xtjj (1) > 0} = ∞. i=1 j=n2i It then follows readily from Borel-Cantelli lemma that with probability one, Xtjj (1) > 0 for infinitely many j with n2i ≤ j < n2i+1 and i = 1, 2, . . .. Therefore, to finish the proof we only need to show that with probability one, Xtjj (Bcg(tj ) ) = 0 for any n2i ≤ j < n2i+1 and i large enough. To this end, we might use Remark 2.5 together with (3.10) and the fact that for n2i ≤ j < n2i+1 , 1 g(tj ) − rj = g(tj ) − g(tj+1 −) 3 2 ≥ g(tj ) − g(tj ) 3 1 1/2+² , ≥ tj 3 and again, the Borel-Cantelli lemma. ¤ Remark 3.4. In the case dβ < 2, given ² > 0 we have P{τ < ∞} = 1 when g(t) = t1/dβ (ln t)−1/d (ln ln t)−(1+²)/d 12 for large t. On the other hand, P{τ = ∞} = 1 when g(t) = t1/dβ (ln t)−1/d (ln ln t)−1/d for large t. Remark 3.5. Notice that condition (3.5) can not guarantee the existence of a finite random time T such that Xt (Bg(t) ) > 0 for all t > T . For instance, given d = β = 1, using (2.2) and Lemma 2.2 one can show that lim inf P{Xt (Bt ) = 0} > 0. t→∞ Consequently such a T does not exist for g(t) = t. Remark 3.6. For t > 0 put It := inf{r ≥ 0 : Xt (Br ) > 0}. For any g satisfying (3.1) and any c > 0, by Theorem 3.1 we have almost surely, lim inf It /cg(t) ≥ 1. t→∞ Therefore, lim inf It /g(t) = ∞. t→∞ Similarly, for any g satisfying (3.5), we have almost surely, lim inf It /g(t) = 0. t→∞ Hence, we would not expect law of iterated logarithm type results for It as t → ∞. At the end of this paper we want to point out that the result on the time-space scaling limit of X mentioned in the introduction can also be recovered using Lemma 2.2. Proposition 3.7. (Dawson and Fleischmann) Given c > 0, for the process X in Theorem 3.1 we have ( µ ) ¶1 oi h n β 1 + β (3.15) lim P exp −αt−1/β Xt (Bct1/dβ ) = exp − αcd vd , t→∞ 1 + β + γβαβ where vd := 2π d/2 dΓ(d/2) denotes the volume of the d-dimensional sphere with radius 1. Therefore, the scaled process Zt := t−1/β Xt (Bct1/dβ ) has a limiting distribution with its Laplace transform determined by (3.15). Proof. Choose 1/2 < δ < 1/dβ. In this proof for each t > 0 we write Xt,· , Yt,· and Zt,· for independent (1 + β)-super-Brownian motions with Xt,0 = λ1(Bct1/dβ −tδ ), Yt,0 = λ1(Rd − Bct1/dβ +tδ ) and Zt,0 = λ1(Bct1/dβ +tδ − Bct1/dβ −tδ ), respectively. 13 Clearly, Xt,t (Rd − Bct1/dβ ) → 0 in probability by Lemma 2.6, and Yt,t (Bct1/dβ ) → 0 in probability by Lemma 2.2. In addition, t−1/β Zt,t (1) → 0 in probability. As a result, it follows from (2.1) that h n oi lim P exp −αt−1/β Xt (Bct1/dβ ) t→∞ h n oi = lim P exp −αt−1/β Xt,t (Bct1/dβ ) t→∞ h n oi = lim P exp −αt−1/β Xt,t (1) t→∞ ( µ ) ¶1 β 1+β = lim exp − αt−1/β λ(Bct1/dβ −tδ ) t→∞ 1 + β + γβαβ ( µ ) ¶1 β 1+β d = exp − αc vd . 1 + β + γβαβ ¤ Remark 3.8. If we choose a different scaling, similar to the proof for Proposition 3.7, using Lemma 2.2 we can show that oi n o h n lim P exp −λt−ξ Xt (Bctξ/d ) = exp −λcd vd t→∞ for the process X in Proposition 3.1 and for ξ > 1/β. i.e. t−ξ Xt (Bctξ/d ) converges weakly to the volume of Bc , which is well known. On the other hand, for ξ < 1/β oi h n lim P exp −λt−ξ Xt (Bctξ/d ) = 1. t→∞ Therefore, t−ξ Xt (Bctξ/d ) converges to 0 weakly as t → ∞. References [1] D. A. Dawson, The critical measure difusion, Z. Wahr. verw. Geb. 40, (1977) 125–145. [2] D. A. Dawson and K. Fleischmann, Critical dimension for a model of branching in a radom medium, Z. Wahr. verw. Geb. 70, (1985) 315–334. [3] D. A. Dawson and K. Fleischmann, Strong clumping of critical space-time branching models in subcritical dimensions, Stoch. Proc. Appl. 30 (1988) 193–208. [4] D. A. Dawson and K. Fleischmann, A continuous super-Brownian motion in a super-Brownian medium, J. Theor. Probab. 10 (1997) 213–276. [5] D. A. Dawson, K. J. 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