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Contents lists available atScienceDirect

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

b

aMathematics 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 define

fα

(

r

) =

f

(

r

, α),

r

>

0

, α ∈ [

0

,

2

π [ .

Throughout this paper we fix

µ

a probability measure on

[

0

,

2

π [

, also we define f

(

r

) =

2π 0

f

(

r

, α) µ(

d

α),

r

>

0

.

Let

(

Pt+

)

t0be the semigroup of a reflecting Brownian motion on

[

0

, ∞[

and let

(

Pt0

)

t0be 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 and

α ∈ [

0

,

2

π [

. We recall the following

Theorem 1.1 (Barlow et al., 1989).

(

Pt

)

t0is a Feller semigroup onC0

(

E

)

, the associated process is by definition the Walsh’s Brownian motion

(

Zt

)

t0(with angles distributed as

µ

).

We can writeZt

= (

Rt

,

Θt

)

where the radial partRt

= |

Zt

|

is a reflected Brownian motion and

(

Θt

)

t0is 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

(2)

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-metric

ρ

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, sup

0<r<Ksupp(µ)

|

fα

(

r

) | + |

fα′′

(

r

) |

< ∞ .

Note that iff

D, then supαsupp(µ)

|

fα

(

0

+ ) | < ∞

and in particular

supp(µ)

|

fα

(

0

+ ) | µ(

d

α)

is finite. From now on, we will extend any functiong

:

supp

(µ) →

Rto

[

0

,

2

π [

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

) =

limϵ0 1 2ϵ

t

01{Rsϵ}ds. ThenBZis an

(

FtZ

)

t-Brownian motion (Lemma 2.2Barlow et al.(1989)). Our main result is the following

Theorem 1.2. Let

(

Zt

)

t0be 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(

d

α)

×

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, supst

|

Hs

| < ∞

. Thus the stochastic integral with respect toBZis well defined. Again by (iii), the integralt

01{Zs̸=0}f′′

(

Zs

)

dsis well defined.

First, we will consider the casez

=

0. Takef

D,t

>

0 and for

ε >

0, define

τ

0ε

=

0 and forn

0

σ

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}where

α =

arg

(

z

)

. Note thatg

Dandgα

(

0+

) =

0. We will prove our formula first for g. We have

g

(

Zt

) −

g

(

0

) =

lim ε0

n=0

g

(

Zσnε+1t

) −

g

(

Zσnεt

)

=

lim ε0

Aεt

+

Dεt where

Aεt

=

n=0

g

(

Zσnε+1t

) −

g

(

Zτnε+1t

)

 and

Dεt

=

n=0

g

(

Zτnε+1t

) −

g

(

Zσnεt

)

=

n=0

g

(

Zτnε+1t

) −

g

(

Zσnε

)

 1{σnεt}

.

We will first identify limε0Dεt. We need the following

Lemma 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

BZσε

n 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 place

(3)

of

(

Z

,

BZ

, σ

nε

, τ

nε+1

)

where

τ

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{σnεt}

tτnε+1 σnε

g

(

Zs

)

dBZs

+

1

2g′′

(

Zs

)

ds

=

n=0

tτnε+1 σnε

g

(

Zs

)

dBZs

+

1

2g′′

(

Zs

)

ds

=

n=0

t

0

1[σε n, τnε+1[

(

s

)

g

(

Zs

)

dBZs

+

1

2g′′

(

Zs

)

ds

=

t

0

n=0

1[σnε, τnε+1[

(

s

)

g

(

Zs

)

dBZs

+

1

2g′′

(

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 tot

01{Zs̸=0}

(

g

(

Zs

)

dBZs

+

1

2g′′

(

Zs

)

ds

)

. NowAεt

=

Htε

+

KtεwithHtε

=

n=0

g

(

Zσnε+1

) −

g

(

0

)

 1{σε

n+1t}and

|

Ktε

| ≤ |

g

(

Zt

) −

g

(

0

) |

1{|Zt|≤ε}

0 as

ε →

0. Note that

σ

nεisFR-measurable,

θ

n

=

arg

(

Zσnε

)

is independent ofFRand in particular

σ

nεand

θ

nare independent. Therefore we obtain

E

[|

Htε

|] ≤

n=0

E

[|

g

(ε, θ

n+1

) −

g

(

0

) |

1{σnε+1t}

]

n=0

E

[|

g

(ε, θ

n+1

) −

g

(

0

) |]

P

nε+1

t

)

2π 0

|

g

(ε, α) −

g

(

0

) |

ε µ(

d

α) ε

n=0

P

nε+1

t

).

But

ε

n=0P

nε+1

t

) →

E

[

Lt

(

R

) ]

as

ε →

0 and for

ε <

1, we have

|

g

(ε, α) −

g

(

0

) |

ε ≤

sup

0<r<1supp(µ)

|

gα

(

r

) | < ∞

so that by dominated convergence, as

ε →

0,

2π 0

|

g

(ε, α) −

g

(

0

) |

ε µ(

d

α) →

2π 0

|

gα

(

0+

) | µ(

d

α) =

0 and finallyHtε

0 inL1. Summarizing, we get

g

(

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

=

fΘt

(

0

+ )

1{Zt̸=0}. Set Ct

=

YtRt

t

0

YsdRs

.

We will identifyCtfollowingProkaj(2009). Put Ytε

=

k=0

Yt1[σε kkε+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 and

YtεRt

Y0εR0

t

0

YsεdRs

=

t

0

RsdYsε

.

(4)

(4)

As

ε →

0, we haveYtε

Yta.s. Since

|

Yε

| ≤

Mfor someM

>

0, then the dominated convergence for stochastic integrals givest

0YsεdRs

t

0YsdRsin probability. The definition ofYεentails that

t

0

RsdYsε

=

k=0

Rσε kYσε

k 1{σε kt}

= ε

k=0

Yσε k1{σε

kt}

.

LetN

(

t

, ε)

be the number of upcrossings of the interval

[

0

,

t

]

byR. So

t

0

RsdYsε

= ε

N(t,ε)

j=0

fθj

(

0

+ ).

Since

(

fθj

(

0

+ ))

j0is a sequence of independent random variables having the same law

µ

, 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

[

fθ0

(

0

+ ) ] .

ButE

[

fθ

0

(

0

+ ) ] =

2π

0 fα

(

0

+ ) µ(

d

α)

and sot

0RsdYsε

→ [

2π

0 fα

(

0

+ ) µ(

d

α) ]

Lt

(

R

)

as

ε →

0. Letting

ε →

0 in(4), we obtain Ct

=

 2π 0

fα

(

0

+ ) µ(

d

α)

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}fΘs

(

0

+ )

dBZs

.

Now forz

=

0, our formula follows from(3). The casez

̸=

0 holds by discussingt

≤ τ

andt

> τ

where

τ

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 all

v ∈

V, denoteIv+

= {

i

I

;

gi

= v }

,Iv

= {

i

I

;

di

= v }

andIv

=

Iv+

Iv. We assume that CardIv

< ∞

for all

v

and that infiILi

>

0. To each

v ∈

V andi

Iv, we associate a parameterpvi

∈ [

0

,

1

]

such that

iIvpvi

=

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 all

v ∈

V

iI+ v

pvi lim

r0+

(

f

ei

)

(

r

) =

iI v

pvi lim

rLi

(

f

ei

)

(

r

)

1{Li<∞}

+

lim

r0

(

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 all

v ∈

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 from

v

,Z‘‘jumps’’ toEiwith probabilitypvi. We have the following

Proposition 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 vertex

v

. 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 to

(5)

simplify notations. LetG+

= ∪

iI+

v Ei

,

G

= ∪

iI 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

,

2

π [→

Ris an integrable function with respect to

µ

and satisfies2π

0 mh

(α)µ(

d

α) =

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(

d

α) ×

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(

d

α) ×

E

[

Lt

(

R

) |

FsZ

]

=

hN

(

Zs

) −

2π 0

(

mh

(α) ∧

N

)µ(

d

α) ×

Ls

(

R

) +

2π 0

(

mh

(α) ∧

N

)µ(

d

α) ×

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

min0utWuby 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: ifXsatisfies

Xt

=

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

s,t

(

z

))

0st,zEis a stochastic flow of mappings (SFM) onEas soon as

ϕ

s,tis measurable with respect to

(

z

, ω)

,

ϕ

s,tand

ϕ

0,tsare equal in law, for any sequence

{[

si

,

ti

] ,

1

i

n

}

of non-overlapping intervals the mappings

ϕ

si,ti

are 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 angle

µ

if for all 0

s

t,z

Eand allf

Dsuch that2π

0 fα

(

0

+ )µ(

d

α) =

0, a.s.

f

s,t

(

z

)) =

f

(

z

) +

t

s

1{ϕs,u(z)̸=0}f

s,u

(

z

))

dWu

+

1 2

t

s

1{ϕs,u(z)̸=0}f′′

s,u

(

z

))

du

.

(5) FollowingLe Jan and Raimond(2006), we will construct a SFM

ϕ

solving this equation: by Kolmogorov extension theorem, there exists a probability space

(

,

A

,

P

)

on which one can construct a process

(

Θs,t

,

Ws,t

)

0st< taking values in

[

0

,

2

π [×

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,tis

µ

.

(6)

(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

)

1inandWis given by

µ

on the event mins,t

̸∈ {

minsi,ti

;

1

i

n

}

and is given by

δ

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, define

τ

s

(

z

) =

inf

{

r

s

:

Ws,r

= −|

z

|}

and

ϕ

s,t

(

z

) =

|

z

| +

Ws,t

,

arg

(

z

)

1{tτs(z)}

+

Wt

mins,t

,

Θs,t

1{ts(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{tτs(z)}

+

2π 0

δ

Wtmins,t

µ(

d

α)

1{ts(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 angle

µ

if for all 0

s

t,z

Eand allf

Dsuch that2π

0 fα

(

0

+ )µ(

d

α) =

0, a.s.

Ks,tf

(

z

) =

f

(

z

) +

t

s

Ks,u

(

f1R2\{0}

)(

z

)

dWu

+

1 2

t

s

Ks,u

(

f′′1R2\{0}

)(

z

)

du

.

(6)

Note that, now we have two solutions to(6):

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 that

ϕ

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.

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