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Statistics and Probability Letters
journal homepage:www.elsevier.com/locate/stapro
Itô’s formula for Walsh’s Brownian motion and applications
Hatem Hajri
a,∗, Wajdi Touhami
baMathematics Research Unit, University of Luxembourg, Campus Kirchberg, 6 rue Richard Coudenhove-Kalergi, L-1359 Luxembourg, Grand-Duchy of Luxembourg, Luxembourg
bFaculté des Sciences de Tunis, Campus Universitaire 2092 - El Manar Tunis, Tunisie
a r t i c l e i n f o
Article history:
Received 15 July 2013
Received in revised form 28 December 2013 Accepted 29 December 2013
Available online 10 January 2014 Keywords:
Walsh’s Brownian motion Itô’s formula
Harmonic functions Stochastic flows
a b s t r a c t
We prove an Itô’s formula for Walsh’s Brownian motion in the plane with angles according to a probability measureµon[0,2π[. This extends Freidlin–Sheu formula which corre- sponds to the case whereµhas finite support. We also give some applications.
©2014 Elsevier B.V. All rights reserved.
1. Itô’s formula for Walsh’s Brownian motion
LetE
=
R2; we will use polar co-ordinates (r, α
) to denote points inE. We denote byC(
E)
the space of all continuous functions onE. Forf∈
C(
E)
, we definefα
(
r) =
f(
r, α),
r>
0, α ∈ [
0,
2π [ .
Throughout this paper we fix
µ
a probability measure on[
0,
2π [
, also we define f(
r) =
2π 0
f
(
r, α) µ(
dα),
r>
0.
Let
(
Pt+)
t≥0be the semigroup of a reflecting Brownian motion on[
0, ∞[
and let(
Pt0)
t≥0be the semigroup of a Brownian motion on[
0, ∞[
killed at 0. Then fort≥
0, definePtto act onf∈
C0(
E)
as follows:Ptf
(
0, α) =
Pt+f(
0),
Ptf
(
r, α) =
Pt+f(
r) +
Pt0(
fα−
f)(
r)
forr>
0 andα ∈ [
0,
2π [
. We recall the followingTheorem 1.1 (Barlow et al., 1989).
(
Pt)
t≥0is a Feller semigroup onC0(
E)
, the associated process is by definition the Walsh’s Brownian motion(
Zt)
t≥0(with angles distributed asµ
).We can writeZt
= (
Rt,
Θt)
where the radial partRt= |
Zt|
is a reflected Brownian motion and(
Θt)
t≥0is called the angular process ofZ. To well defineΘt, whenZt=
0, we set by conventionΘt=
0.∗Corresponding author.
E-mail addresses:[email protected](H. Hajri),[email protected](W. Touhami).
0167-7152/$ – see front matter©2014 Elsevier B.V. All rights reserved.
http://dx.doi.org/10.1016/j.spl.2013.12.021
Notations:
We denote byEµ, the state space of Walsh’s Brownian motion, i.e.Eµ
= { (
r, α) :
r≥
0, α ∈
supp(µ) }
. We define the tree-metricρ
onR2as follows: forz1= (
r1, α
1),
z2= (
r2, α
2) ∈
R2,ρ(
z1,
z2) = (
r1+
r2)
1{α1̸=α2}+ |
r1−
r2|
1{α1=α2}.
Note that the sample paths of Walsh’s Brownian motion are continuous with respect to the tree-topology, since the process cannot jump from one ray to another one without passing through the origin. These paths are also continuous with respect to the relative topology induced by the Euclidean metric onR2.
Now denote byDthe set of all functionsf
:
Eµ→
Rsuch that (i) fis continuous for the tree-topology.(ii) For all
α ∈
supp(µ)
,fαisC2on]
0, ∞]
andfα′(
0+ ),
fα′′(
0+ )
exist and are finite.(iii) For allK
>
0, sup0<r<K,α∈supp(µ)
|
fα′(
r) | + |
fα′′(
r) |
< ∞ .
Note that iff
∈
D, then supα∈supp(µ)|
fα′(
0+ ) | < ∞
and in particularsupp(µ)
|
fα′(
0+ ) | µ(
dα)
is finite. From now on, we will extend any functiong:
supp(µ) →
Rto[
0,
2π [
by settingg=
0 outside supp(µ)
. Forf∈
Dandz= (
r, α) ̸=
0, we set f′(
z) =
fα′(
r)
andf′′(
z) =
fα′′(
r)
.Now define
BZt
=
Rt−
R0−
Lt(
R)
(1)whereLt
(
R)
stands for the symmetric local time at zero ofR, i.e.Lt(
R) =
limϵ→0 1 2ϵt
01{Rs≤ϵ}ds. ThenBZis an
(
FtZ)
t-Brownian motion (Lemma 2.2Barlow et al.(1989)). Our main result is the followingTheorem 1.2. Let
(
Zt)
t≥0be a Walsh’s Brownian motion started from z, then for all f∈
D, we have f(
Zt) =
f(
z) +
t
0
1{Zs̸=0}f′
(
Zs)
dBZs+
1 2 t
0
1{Zs̸=0}f′′
(
Zs)
ds+
2π 0
fα′
(
0+) µ(
dα)
×
Lt(
R).
When supp
(µ)
is finite this formula is due toFreidlin and Sheu(2000) (see alsoHajri(2011) for another proof based on the skew Brownian motion). Our proof is based on standard approximations and Riemann–Stieltjes integration.Proof. Note thatHs
(ω) =
1{Zs(ω)̸=0}f′(
Zs(ω))
is progressively measurable with respect to the filtration(
FtZ)
and is locally bounded by the assumption (iii) onf, i.e. a.s.∀
t≥
0, sups≤t|
Hs| < ∞
. Thus the stochastic integral with respect toBZis well defined. Again by (iii), the integralt01{Zs̸=0}f′′
(
Zs)
dsis well defined.First, we will consider the casez
=
0. Takef∈
D,t>
0 and forε >
0, defineτ
0ε=
0 and forn≥
0σ
nε=
inf{
r≥ τ
nε: |
Zr| = ε } , τ
nε+1=
inf{
r≥ σ
nε:
Zr=
0} .
Setg
(
z) =
f(
z) −
fα′(
0+ ) |
z|
1{z̸=0}whereα =
arg(
z)
. Note thatg∈
Dandgα′(
0+) =
0. We will prove our formula first for g. We haveg
(
Zt) −
g(
0) =
lim ε→0∞
n=0
g
(
Zσnε+1∧t) −
g(
Zσnε∧t)
=
lim ε→0Aεt
+
Dεt whereAεt
=
∞
n=0
g
(
Zσnε+1∧t) −
g(
Zτnε+1∧t)
andDεt
=
∞
n=0
g
(
Zτnε+1∧t) −
g(
Zσnε∧t)
=
∞
n=0
g
(
Zτnε+1∧t) −
g(
Zσnε)
1{σnε≤t}.
We will first identify limε→0Dεt. We need the followingLemma 1.3. Let h
∈
D, then for all t∈ [ σ
nε, τ
nε+1]
we have h(
Zt) =
h(
Zσnε) +
t
σnε
1{Zs̸=0}h′
(
Zs)
dBZs+
1 2 t
σnε
h′′
(
Zs)
1{Zs̸=0}ds.
(2)Proof. Note thatBZ·+σε
n
−
BZσεn is a Brownian motion independent ofFσZnε. Thus by conditioning with respect toFσZnε, it will be sufficient to prove that a Walsh’s Brownian motionYstarted from a fixedy
̸=
0 satisfies(2)with(
Y,
BY,
0, τ
′)
in placeof
(
Z,
BZ, σ
nε, τ
nε+1)
whereτ
′is the first hitting time of 0 byY. SinceLt( |
Y| ) =
0 for allt≤ τ
′, our claim holds by a simple application of Itô’s formula for|
Y|
using the functionfarg(y).Applying the previous lemma, we get Dεt
=
∞
n=0
1{σnε≤t}
t∧τnε+1 σnε
g′
(
Zs)
dBZs+
12g′′
(
Zs)
ds
=
∞
n=0
t∧τnε+1 σnε
g′
(
Zs)
dBZs+
12g′′
(
Zs)
ds
=
∞
n=0
t
0
1[σε n, τnε+1[
(
s)
g′
(
Zs)
dBZs+
12g′′
(
Zs)
ds
=
t
0
∞
n=0
1[σnε, τnε+1[
(
s)
g′
(
Zs)
dBZs+
12g′′
(
Zs)
ds
where we have used dominated convergence for stochastic integrals (seeRevuz and Yor(1999) page 142) in the last line.
Using dominated convergence again we see that as
ε →
0,Dεt converges in probability tot01{Zs̸=0}
(
g′(
Zs)
dBZs+
12g′′
(
Zs)
ds)
. NowAεt=
Htε+
KtεwithHtε=
∞n=0
g
(
Zσnε+1) −
g(
0)
1{σεn+1≤t}and
|
Ktε| ≤ |
g(
Zt) −
g(
0) |
1{|Zt|≤ε}→
0 asε →
0. Note thatσ
nεisFR-measurable,θ
n=
arg(
Zσnε)
is independent ofFRand in particularσ
nεandθ
nare independent. Therefore we obtainE
[|
Htε|] ≤
∞
n=0
E
[|
g(ε, θ
n+1) −
g(
0) |
1{σnε+1≤t}]
≤
∞
n=0
E
[|
g(ε, θ
n+1) −
g(
0) |]
P(σ
nε+1≤
t)
≤
2π 0
|
g(ε, α) −
g(
0) |
ε µ(
dα) ε
∞
n=0
P
(σ
nε+1≤
t).
But
ε
∞n=0P
(σ
nε+1≤
t) →
E[
Lt(
R) ]
asε →
0 and forε <
1, we have|
g(ε, α) −
g(
0) |
ε ≤
sup0<r<1,α∈supp(µ)
|
gα′(
r) | < ∞
so that by dominated convergence, asε →
0, 2π 0
|
g(ε, α) −
g(
0) |
ε µ(
dα) →
2π 0
|
gα′(
0+) | µ(
dα) =
0 and finallyHtε→
0 inL1. Summarizing, we getg
(
Zt) =
g(
0) +
t
0
1{Zs̸=0}g′
(
Zs)
dBZs+
1 2 t
0
1{Zs̸=0}g′′
(
Zs)
ds.
(3)Note that a.s.g
(
Zt) =
f(
Zt) −
RtYtwithYt=
fΘ′t(
0+ )
1{Zt̸=0}. Set Ct=
YtRt−
t
0
YsdRs
.
We will identifyCtfollowingProkaj(2009). Put Ytε
=
∞
k=0
Yt1[σε k,τkε+1[
(
t).
ThenYεis right-continuous and is constant on every interval
[ σ
kε, τ
kε+1[
. SinceRis continuous, thenRis Riemann–Stieltjes integrable with respect toYεalmost surely andYtεRt
−
Y0εR0−
t
0
YsεdRs
=
t
0
RsdYsε
.
(4)As
ε →
0, we haveYtε→
Yta.s. Since|
Yε| ≤
Mfor someM>
0, then the dominated convergence for stochastic integrals givest0YsεdRs
→
t0YsdRsin probability. The definition ofYεentails that
t
0
RsdYsε
=
∞
k=0
Rσε kYσε
k 1{σε k≤t}
= ε
∞
k=0
Yσε k1{σε
k≤t}
.
LetN
(
t, ε)
be the number of upcrossings of the interval[
0,
t]
byR. So t
0
RsdYsε
= ε
N(t,ε)
j=0
fθ′j
(
0+ ).
Since
(
fθ′j(
0+ ))
j≥0is a sequence of independent random variables having the same lawµ
, the Bernoulli law of large numbers yields t
0
RsdYsε
= ε
N(
t, ε)
N(t,ε)
j=0
fθ′
j
(
0+ )
N
(
t, ε) →
Lt(
R)
E[
fθ′0(
0+ ) ] .
ButE[
fθ′0
(
0+ ) ] =
2π0 fα′
(
0+ ) µ(
dα)
and sot0RsdYsε
→ [
2π0 fα′
(
0+ ) µ(
dα) ]
Lt(
R)
asε →
0. Lettingε →
0 in(4), we obtain Ct=
2π 0
fα′
(
0+ ) µ(
dα)
Lt
(
R).
Using the fact that 1{Rs>0}dRs
=
1{Rs>0}dBZs, it follows that t
0
YsdRs
=
t
0
YsdBZs
=
t
0
1{Zs̸=0}fΘ′s
(
0+ )
dBZs.
Now forz
=
0, our formula follows from(3). The casez̸=
0 holds by discussingt≤ τ
andt> τ
whereτ
is the first hitting time of 0 byZand using the Itô’s formula satisfied byZ·+τ which is a Walsh’s Brownian motion started from 0.2. Some applications
2.1. Walsh’s Brownian motion on graphs
The result of this section can be deduced fromHajri and Raimond(inpress) but it has not been announced in that paper.
Our purpose is to give an Itô’s formula for Walsh’s Brownian motion with the more general state space of a graph. This diffusion is defined by means of its infinitesimal generator inFreidlin and Sheu(2000) (see also Chapter 4 inJehring(2009)).
Along an edge it is like a Brownian motion and around a vertex it behaves like a Walsh’s Brownian motion.
LetGbe a metric graph equipped with the shortest path distance, denote byV, the set of its vertices, and by
{
Ei;
i∈
I}
the set of its edges whereIis a finite or countable set. To each edgeEi, we associate an isometryei:
Ji→ ¯
Ei, withJi= [
0,
Li]
when Li< ∞
andJi= [
0, ∞ )
orJi= ( −∞ ,
0]
whenLi= ∞
. WhenLi< ∞
, denote{
gi,
di} = {
ei(
0),
ei(
Li) }
. WhenLi= ∞
, de- note{
gi,
di} = {
ei(
0), ∞}
whenJi= [
0, ∞ )
and{
gi,
di} = {∞ ,
ei(
0) }
whenJi= ( −∞ ,
0]
. For allv ∈
V, denoteIv+= {
i∈
I;
gi= v }
,Iv−= {
i∈
I;
di= v }
andIv=
Iv+∪
Iv−. We assume that CardIv< ∞
for allv
and that infi∈ILi>
0. To eachv ∈
V andi∈
Iv, we associate a parameterpvi∈ [
0,
1]
such thati∈Ivpvi
=
1. Letp= (
piv, v ∈
V,
i∈
Iv)
and denote byDpGthe set of all continuous functionsf:
G→
Rsuch that for alli∈
I,f◦
eiisC2on the interior ofJiwith bounded first and second derivatives both extendable by continuity toJiand such that for allv ∈
V
i∈I+ v
pvi lim
r→0+
(
f◦
ei)
′(
r) =
i∈I− v
pvi lim
r→Li−
(
f◦
ei)
′(
r)
1{Li<∞}+
limr→0−
(
f◦
ei)
′(
r)
1{Li=∞}
.
Forf
∈
DpGandx=
ei(
r) ∈
G\
V, setf′(
x) = (
f◦
ei)
′(
r)
,f′′(
x) = (
f◦
ei)
′′(
r)
and take the following conventions for allv ∈
V,f′(v) =
f′′(v) =
0.LetZbe a Walsh’s Brownian motion onGassociated to the familypand started fromz, i.e. ifEiis an adjacent edge to
v
, then fromv
,Z‘‘jumps’’ toEiwith probabilitypvi. We have the followingProposition 2.1. There exists a Brownian motion W such that for all f
∈
DpG, we have f(
Zt) =
f(
z) +
t
0
f′
(
Zu)
dWu+
1 2 t
0
f′′
(
Zu)
du.
Proof. We takez
= v
a vertex point. We will defineWuntilZhits another vertexv
′. The definition ofWshould be clear then using the strong Markov property and the successive hitting times ofVbyZ. Thus we can also assume thatGis a star graph (has only one vertex and eventually an infinite number of edges) which we embed in the complex plane just tosimplify notations. LetG+
= ∪
i∈I+v Ei
,
G−= ∪
i∈I− v Eiand Wt=
t
0
(
1G+(
Zs) −
1G−(
Zs))
dBZs.
Now our result holds by applyingTheorem 1.2and taking care of the definition of the derivative offin the proposition.
2.2. Harmonic functions on Walsh’s Brownian motion
InJehring(2009), Harmonic functions on Walsh’s Brownian motion are studied. The following lemma (Lemma 3.2 in Jehring(2009)) is the most technical point in proving Theorem 3.2 inJehring(2009). Its proof uses the Excursion theory and non trivial calculations (see Appendix A inJehring(2009)). We will derive it in few lines fromTheorem 1.2.
Lemma 2.2. Let h
:
E→
Rbe of the form h(
r, α) =
mh(α).
r+
h(
0)
for
(
r, α) ∈
E, where the function mh: [
0,
2π [→
Ris an integrable function with respect toµ
and satisfies2π0 mh
(α)µ(
dα) =
0. Then{
h(
Zt),
t≥
0}
is a martingale with respect to(
FZ)
tfor every starting point z∈
E.Note that whenmhis bounded our formula gives an explicit expression of this martingale:
h
(
Zt) =
h(
z) +
t
0
mh
(
Θs)
1{Zs̸=0}dBZs.
Proof. ByTheorem 1.2, using the functionhN
(
r, α) = (
mh(α) ∧
N).
r+
h(
0),
N≥
0, we see that hN(
Zt) =
hN(
z) +
t
0
(
mh(
Θu) ∧
N)
1{Zu̸=0}dBZu+
2π 0
(
mh(α) ∧
N)µ(
dα) ×
Lt(
R).
Thus for alls
≤
t,E
[
hN(
Zt) |
FsZ] =
hN(
z) +
s
0
(
mh(
Θu) ∧
N)
1{Zu̸=0}dBZu+
2π 0
(
mh(α) ∧
N)µ(
dα) ×
E[
Lt(
R) |
FsZ]
=
hN(
Zs) −
2π 0
(
mh(α) ∧
N)µ(
dα) ×
Ls(
R) +
2π 0
(
mh(α) ∧
N)µ(
dα) ×
E[
Lt(
R) |
FsZ] .
LettingN
→ ∞
and using dominated convergence (note thatE[|
mh(
Θt) ||
Zt|] < ∞
sincemh(
Θt)
and|
Zt|
are independent), we getE[
h(
Zt) |
FsZ] =
h(
Zs)
.2.3. Stochastic flows in the plane
LetZbe a Walsh’s Brownian motion started from 0 and defineW
=
BZ. Then, we haveRt=
Wt−
min0≤u≤tWuby Skorokhod Lemma (seeRevuz and Yor(1999) page 239),σ (
R) = σ (
W)
andΘt is independent ofW for allt>
0. This situation is close to Tanaka’s equation: ifXsatisfiesXt
=
t
0
sgn
(
Xs)
dWs,
then
σ( |
X| ) = σ (
W)
and sgn(
Xt)
is independent ofWfor allt>
0. Theorem 2 allows thus to define the analogue of Tanaka’s equation in the plane. This problem has been considered from the stochastic flows view point inHajri(2011) for supp(µ)
finite.We say that
(ϕ
s,t(
z))
0≤s≤t,z∈Eis a stochastic flow of mappings (SFM) onEas soon asϕ
s,tis measurable with respect to(
z, ω)
,ϕ
s,tandϕ
0,t−sare equal in law, for any sequence{[
si,
ti] ,
1≤
i≤
n}
of non-overlapping intervals the mappingsϕ
si,tiare independent, and we have the flow property: for alls
≤
t≤
uandz∈
E, a.s.ϕ
s,u(
z) = ϕ
t,u◦ ϕ
s,t(
z)
.Definition 2.3. Let
ϕ
be a SFM andWbe a Brownian motion. We say that(ϕ,
W)
solves Tanaka’s equation with angleµ
if for all 0≤
s≤
t,z∈
Eand allf∈
Dsuch that2π0 fα′
(
0+ )µ(
dα) =
0, a.s.f
(ϕ
s,t(
z)) =
f(
z) +
t
s
1{ϕs,u(z)̸=0}f′
(ϕ
s,u(
z))
dWu+
1 2 t
s
1{ϕs,u(z)̸=0}f′′
(ϕ
s,u(
z))
du.
(5) FollowingLe Jan and Raimond(2006), we will construct a SFMϕ
solving this equation: by Kolmogorov extension theorem, there exists a probability space(
Ω,
A,
P)
on which one can construct a process(
Θs,t,
Ws,t)
0≤s≤t<∞ taking values in[
0,
2π [×
Rsuch that (i)–(iv) below are satisfied(i) Ws,t
:=
Wt−
Wsfor alls≤
tandWis a Brownian motion.(ii) For fixeds
<
t,Θs,tandWare independent and the law ofΘs,tisµ
.(iii) Define mins,t
=
inf{
Wu;
u∈ [
s,
t]}
. Then for alls<
tandu< v
P(
Θs,t=
Θu,v|
mins,t=
minu,v) =
1.
(iv) For alls
<
tand{ (
si,
ti) ;
1≤
i≤
n}
withsi<
ti, the law ofΘs,tknowing(
Θsi,ti)
1≤i≤nandWis given byµ
on the event mins,t̸∈ {
minsi,ti;
1≤
i≤
n}
and is given byδ
Θsi,tion the event{
mins,t=
minsi,ti}
with 1≤
i≤
n.Note that (i)–(iv) uniquely define the law of
(
Θs1,t1, . . . ,
Θsn,tn,
W)
for allsi<
ti, 1≤
i≤
n. This family of laws is consistent by construction.For 0
≤
s≤
t,z∈
E, defineτ
s(
z) =
inf{
r≥
s:
Ws,r= −|
z|}
and
ϕ
s,t(
z) =
|
z| +
Ws,t,
arg(
z)
1{t≤τs(z)}
+
Wt
−
mins,t,
Θs,t1{t>τs(z)}
.
FollowingLe Jan and Raimond(2006), one can prove that
ϕ
is a SFM such that(ϕ,
W)
satisfies(5). It is also possible to extend (5)to stochastic flows of kernels as inLe Jan and Raimond(2006). A stochastic flow of kernels (SFK)K= (
Ks,t;
s≤
t)
is the same as a SFM, but the mappings are replaced by kernels, and the flow property being now that for allz∈
E,s≤
t≤
u, a.s.Ks,u
(
x) =
Ks,tKt,u(
x)
. For example KsW,t(
z) =
E[ δ
ϕs,t(z)|
W] = δ
|z|+Ws,t,arg(z)1{t≤τs(z)}
+
2π 0
δ
Wt−mins,t,α
µ(
dα)
1{t>τs(z)}is a SFK. By conditioning with respect toWin(5), we see that
(
KW,
W)
is solution of the following equation.Definition 2.4. LetKbe a SFK andWbe a Brownian motion. We say that
(
K,
W)
solves Tanaka’s equation with angleµ
if for all 0≤
s≤
t,z∈
Eand allf∈
Dsuch that2π0 fα′
(
0+ )µ(
dα) =
0, a.s.Ks,tf
(
z) =
f(
z) +
t
s
Ks,u
(
f′1R2\{0})(
z)
dWu+
1 2 t
s
Ks,u
(
f′′1R2\{0})(
z)
du.
(6)Note that, now we have two solutions to(6):
(δ
ϕ,
W)
and(
KW,
W)
. InHajri(2011), when supp(µ)
is finite a complete de- scription of the laws of all SFK’sKsolutions of(6)is given under some further assumptions on stochastic flows (see the definitions inLe Jan and Raimond(2004)). Under these assumptions, it should be possible to prove in our setting thatϕ
is the law-unique SFM solution of(5),KWis the unique Wiener (i.e.σ(
W)
-measurable) flow solution of(6)and to give a complete classification of solutions to(6).Acknowledgements
The research of the first author is supported by the National Research Fund, Luxembourg, and cofunded under the Marie Curie Actions of the European Commission (FP7-COFUND).
References
Barlow, M., Pitman, J., Yor, M.,1989. On Walsh’s Brownian motions. Lecture Notes in Math. 1372, 275–293.
Freidlin, M., Sheu, S.,2000. Diffusion processes on graphs: stochastic differential equations, large derivation principle. Probab. Theory Related Fields 116 (2), 181–220.
Hajri, H.,2011. Stochastic flows related to Walsh Brownian motion. Electron. J. Probab. 16 (58), 1563–1599.
Hajri, H., Raimond, O., 2014. Stochastic flows on metric graphs. Electron. J. Probab.http://arxiv.org/abs/1305.0839(in press).
Jehring, K.E., 2009. Harmonic functions on Walsh’s Brownian motion, Ph.D. dissertation, Univ. of California Saint Diego.
Le Jan, Y., Raimond, O.,2004. Flows, coalescence and noise. Ann. Probab. 32 (2), 1247–1315.
Le Jan, Y., Raimond, O.,2006. Flows associated to Tanak’s SDE. ALEA Lat. Am. J. Probab. Math. Stat. 1, 21–34.
Prokaj, V.,2009. Unfolding the Skorohod reflection of a semimartingale. Statist. Probab. Lett. 79, 534–536.
Revuz, D., Yor, M.,1999. Continuous Martingales and Brownian Motion. Springer Verlag, Berlin.