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Some Properties for the American Option-Pricing Model

Hong-Ming Yin

Department of Mathematics, Washington State University, Pullman, USA Email: [email protected]

Received March 24,2012; revised April 26, 2012; accepted May 6, 2012

ABSTRACT

In this paper we study global properties of the optimal excising boundary for the American option-pricing model. It is shown that a global comparison principle with respect to time-dependent volatility holds. Moreover, we proved a global regularity for the free boundary.

Keywords: American Option Model; Regularity of Free Boundary; Comparison Principle

1. Introduction

It is well-known that, for the American option-pricing model, there is an optimal holding region for contracts holders (see [1-5]). The part of the boundary for the re-gion is unknown (free boundary), which is often referred as the optimal excising boundary for option traders. This free boundary has to be calculated along with the option price of the security. The mathematical model for the problem is highly nonlinear and there is no explicit solu-tion representasolu-tion even when volatility and interest rate are assumed to be constants (see [4]). On the other hand, for the financial world as well as for the intrinsic interest itself, it is extremely important to find the location of the free boundary along with the option price of the security. Particularly, people would like to know how the price of a security changes near the option expiry time since it may change dramatically [6,7].

During the past few decades, there are many research papers concerning for various option-pricing models. There are several Monographs devoted to this topic (see, for examples, [1,3,4,8]). For the American option model as well as its generalization, the existence and uniqueness are studied by many researchers ( here just a few exam-ples, [2,5,9-12]). A basic fact is that the American op-tion-pricing model can be reformulated as a variational inequality of parabolic type. Hence, many known results about existence and uniqueness can be applied to the model. However, the disadvantage of the method is that there is no information about the free boundary. To overcome the shortcoming, several authors employed other methods to establish the existence and uniqueness for the problem (see [7,13-17]). Because of the practical importance, many researchers paid a special attention to the asymptotic behavior for the free boundary near the expiration time(see [6,18-25]). Moreover, various

nu-merical computations for the location of free boundary are also carried out by many people (see, for examples, [14,25-28] and the references therein). More recently, some global property of the free boundary attracts some interest. The authors of [29,30] proved that the free boundary is convex if the volatility in the model is as-sumed to be a constant. However, this global property is not valid in the real financial market since the volatility depends on time and other economical factors. When the volatility depends on time and the security, the problem becomes much more challenging. In this paper we would like to study some global property of the free boundary. We want to find how the optimal exercising boundary changes when the volatility changes during the life-time of the option contract. This question is very important for structured products in the financial world.

We first recall the classical model for the American option-pricing model with one security or one type of asset. Let V s t

 

, be the option price for a security such as a stock with price s at time . Then it is well- known that

t

 

,t

V s satisfies the Black-Scholes equation with no dividend [31,32]:

 

2

2 1

0 := = 0, , ,

2

t ss s

L V V  s VrsVrV s tQT (1.1)

where r is the interest rate and  represents the market volatility of the stock, is the region defined below.

1

T

Q

For the American put-option model (call-option is similar), in order to avoid loss for option holders, it is desirable to hold the option only when s lies in the re- gion (called optimal holding region):

   

1

:= , : < < , 0 < < ,

T

Q s t S t st T

(2)

 

,

V s t 0, called the optimal exercising boundary. On the free boundary s=S t

 

, we know from the continuity of the option price that V s t

,

satisfies:

 

,

=

 

, 0 < <

V S t t KS t t T (1.2)

 

,

= 1, 0 < < ,

s

V S t tt T (1.3) where K is the striking price.

We also know the payoff value at the terminal time once the striking price is given:

T

  

, =

,

 

< ,

V s T KsS Ts

.

,

.

(1.4)

 

, 0,

V s ts  (1.5) For later use, we introduce :

 

 

2

1 2

= , : 0 < < , 0 < <

= ,

T

T T T T

Q s t s S t t T

Q QQ 

where

 

= = : 0 <

T s S t t T

 

In financial markets, the volatility  plays a major role for the option pricing model. Option price often changes dramatically when the stock market is in a cha-otic movement. This was the case when the flash-crash happened on May 6, 2010 as well as the case on Oct. 19, 1987. On the other hand, for a relatively stable market, the volatility mainly depends on time. This is particularly true for an index fund such as S&P500 index in the U.S. market. Hence, we assume that throughout this paper. Our question is how the free boundary

 

t

=  

 

S t

changes when the volatility 

 

t changes during the life-span of the option contract. We show that there is a global comparison principle for the free boundary with respect to the change of volatility . Moreover, a global existence result is also established as a by-product. Our proof is based on the line method (see [15]), which is different from existing literature (see [21,13] and the references therein). Although the existence of a solution for the problem is already known, our method does have several advantages. One of them is that the free boundary is determined along with the option price at each discrete time simultaneously. Moreover, a global regularity for the free boundary is also obtained. To author’s knowl-edge, this regularity result is new and optimal (see [19, 21,12]).

t

The paper is organized as follows. In Section 2, we construct a sequence of approximation solutions by using the line method. After deriving some uniform estimates, a global existence is established. Moreover, an optimal global regularity for the free boundary is also obtained. In Section 3, we first derive some comparison properties for the approximation solution and then show that the

limit solution preserves the same property. Some con-cluding remarks are given in Section 4.

Remark 1.1: After this paper is completed, the author le

2. Existence and Uniqueness

ased on the discrete

owing conditions are always assumed through- ou

arned that E. Ekströn proved a result in [33] (2004) about the monotonicity of option price with respect to volatility. However, there is no result about the compari-son result for the free boundary. Moreover, the method in [33] is totally different from ours here. In addition, we also present a regularity result for the free boundary.

Since our argument in Section 3 is b

problem, we give the complete details about the con-struction of the approximation solution sequence. We also show that the approximation sequence is convergent to the solution of the original problem (1.1)-(1.5). As a byproduct, an optimal regularity of the free boundary is obtained.

The foll t this paper.

H(1): Let 

   

t ,r tC

 

0,T for some 

 

0,1 . ch that There exist positive constants a b, and R su

 

 

0 <a tb,0r tR.

Now we construct an approximate solution sequence by

teger. Divide using the line method.

Let N be a positive in

 

0,T into su rva

N

binte ls with equal length h= T :

N

Define

0 1

0 =t <t <<tN = , =T ti ih i, = 0,1,,N

 

1

1

= tk d

k tk

h ,.

   

 

1

1

= tk d , = 1, 2, . k

tk

r r k

h

   N

If we use difference quotient to approximate Vt and replace 

 

t and r t

 

by n and rn, we have

1 2

, , 1

, 2

, , = 0.

n n

n n ss

n n s n n

V s t V s t

s V s t h

r sV s t r V s t

 

 

This leads us to define the approximate solution

 

n

V s and Sn as follows:

m the terminal conditio

Fro n, we know

  

, =

V s T Ks

 

=

S T K .

and So we define

.

Suppose we have obtained and

  

=

, 0 < , =

N N

V s Ks  sS K

 

1

n

(3)

define Vn

 

s and Sn as follows:

 

2

< <

n n = 1 ,

2

,

n n n n

n

1 1 1

n

s V r r V V s

h h

  (2.1)

1, (2.2)

where w exte d

sV   K as nde S s   n n V S

 

n V s e have  

 

= S Vn, n

 

Sn = 0, s ,

   (2.3)

 

s into the whole interval

1

n

0,

by

 

1 = ,

V

1.

n

It see th e above free boun ary problem (2

erpolation to define the free bo

0 < < n

V s Ks s S

is easy to at th

)

d

.1)-(2.3) has a unique solution

V

 

s S,

for each

n. Actually, since the problem is ional one n find the solution Vn

 

s and Sn explicitly (see [4]

for detailed calculation Now we use the int

n n

one-dimens ca

. undary SN

 

t

as follows:

 

1

1

1

=

, = 1, 2, , .

N n n

n n,

t t

S t S S

h h

t t t n N

      define

n   n

, use the notation

tt

Also, we

We also

 

, =

N

V s t Vn s tnt<tn1, = 0,1,nN1.

 

 

1

 

= s .

V s

h

Our show that the approxim e solution se

,

n h

goal is to orig

n n

V sV

= = , = 0,1, , . k QTt tk kN

at

quence

VN

 

s t, ,SN

 

t

is convergent to the solu-tion of the dary problem (1.1)-(1.5). To this end, we need to derive some uniform estimates.

inal free boun

Lemma 2.1: For all

 

s t, QT,

N N

V s t S

 

0 , K, 0 tK.

Proof the definition, we see

if T. Suppose we have shown that : From

N

t  t

0

s  , we

 

, =

 

N

0

N

V s t V s

1 tN =

 

1

 cla

n

V im that Vn

 

s 0. Indeed, if Vn

 

s gative minimum oint

attains a ne at some p

n,

*

sS  , then at this minimum point, we see

2

* =

1 1

> 0, 2ns Vn r sVn n rn h Vn s s

  

 

 

which contradicts the right-hand side of the Equation (2.1). It follows that Vn

 

s 0 on

Sn,

. By the definition of Vn

 

s on

0,Sn

, we see Vn

 

s 0 for s

0,

. Con ly, V 0 on QT.

other hand, we VN

s h

sequent

On the claim that as an

up

 

,

N

s t

,t

true for

per bound K. Indeed, it is obviously VN

 

s , which implies that VN

 

s t, K when t

tN1,tN

. We assume that

tn1,tn

is the first interval in which

 

0 <

max s Vn s >K. Then, suppose that V

 

s attains at an interior poin

n t

a positive maximum

Sn,

*

s   , then at s=s*, Vn

 

s* 0,Vn

 

s* = 0. Thus,

 

2 * * = 1 1 .

2 n n n n n n s s n n

1

s V r sV r V r V s

h h               

It follows from Equation (2.1) that

 

* 1 1 , 1 n n n

V s V K

r h

 

which is a contradiction. On the boundary s=Sn,

,

= .

n n n

V S t KSK

 

n

V sK when 0 s Sn

Obviously, . Consequen-

tly, 0VN

 

s,tK in dition (

T

Q . F e, from the boun 2.2), see 0SnK for all

= 0,1, ,

nN.

urthermor

dary con we

Q.E.D.

2.2: There exists a constant such that

Lemma C1

 

 

 

2( ) 2

=1 2 1 2 =1 , m N N

L m k s L k

m N h L

k k

V h V

h V C

     

where depends only on known data, but not on fo

1

C

f: T

N. ma

Proo his estimate is similar to the energy esti te r a parabolic equation. Indeed, we introduce new vari-ables:

= ln , = .

x sTt

Define

 

, =

   

, , =

 

U xV s t XS t .

Then the original free boundary problem .1)-(1.5) is eq

(1 uivalent to the following one:

 

 

 

 

 

2 1 2 1 1

ˆ ˆ ˆ

:=

2 2

ˆ

ˆ = 0, , ,

xx x

T

L U U U r U

r U x Q

               (2.4) 

 

( )

, = X , 0 < ,

U X   Ke  T (2.5)

 

 

, = X , 0 < , x

U X   e  T (2.6)

 

, 0 =

S T 

,

 

0 < < ,

U x KeX x  (2.7) where

   

ˆ =T , : < < , 0 <

Q xXx  T ,

 

     

ˆ = t ,rˆ =r t

(4)

Lemma 2.4: There exists a constant su that On the other hand, by the definition we know

It follows that

Thus,

.

Now we can extend

 

, = , 0 < <

 

, 0 < < .

V s t Ks s S t t T

 

0 = ˆ

L VrK, 0 <s<S t

 

, 0 < < .t T

 

 

= , < < , 0 < <

L U1r t K   x X   T

 

,

U x into the region

1

ˆ =T 0,

Q RT , we use the continuity of U x

 

, and

 

, x x

U  in QˆT to see that U

 

x, is a weak ollowing problem:

 

solution of the f

 

1 = , , ,

L U f xx QˆT, (2.8)

where if

 

, 0 =

x

, <

U x Ke   

 

 

< .

x  (2.9) , = 0

f x <x< X  , 0  T and

 

, = ˆ

 

f x rK if X

 

 <x< , 0 <T . method method to d

Now efine

,

we can use the line

 

Un x and UN

 

x which are exactly the same as for

on page

a classical parabolic equation (see [34], estimate (5.15) 137) a n the desired energy estimate. By the definition, we see clearly that

 

nd obtai

 

, = ,

N N

V s t U x

for

 

s t, QT1. Q.E.D.

Lemma 2.3: There exists a constant C2 such that

 

  2,

N s L QT

V C

where depends only on known da , but not on .

Proof: Note that is uniformly Lipschitz con- o

2

C ta N

 

, 0

U x

tinuous n X

 

0 ,

. We may assume that U

 

x, 0 is differentiable bounded derivative on

 

0 ,

X

 .

Define

with a

 

, = x(

 

,

W xU x .

It follows that W satisfies the following equations:

 

 

 

1 1

ˆ ˆ ˆ

2 2

 

 

2 2

ˆ

ˆ = 0, , ,

xx x

W    W r     W

T

rW xQ

 

 

(2.10)

(2.11)

The maximum principle yields that

 

,

= X , 0 < ,

W X   e   T

 

, 0 = x

 

, 0 ,

 

0 < <

W x U x X x , (2.12)

,

W x

is uni-formly bounded and the bound depend known da

s only on n easily

ta. By using the same argument, we ca deduce the uniform bound for N

 

,

s

V s t .

Q.E.D.

Let  > 0 be a small number and define

 

=

 

, : 0 . .

T QT s t t T

Q     

3

C ch

 

 

 

 

where depends only on the known data an

  3,

N N

h

ss L QT x L QT

V V C

   

3

C d  , but

not on .

f: ns

um at

N

Proo From the theory of parabolic equatio , we may ass e th U x

 

, is differentiable up to X

 

 . Set

 

, =Uxx

   

, , , T.

P x xx Q

From the boundary condition (2.5), we see

 

,

 

 

,

= X 

 

.

x

U X   X U X   e X 

It follows by (2.6) that

 

,

=

UX   0, X

 

 <x<.

From the Equation (2.4) and the boundary conditions (2.5) and (2.6), we see

 

 

 

 

 

 

ˆ ˆ

,

X

r e

K e

 

2

1 1

ˆ , =

2 2

X

P X

   

 

 

 

which is uniformly bounded.

By differentiating Equation (2.4) with respect to x

    

twice, we see P x

 

, satisfies

 

2

 

 

2

 

1 1

ˆ ˆ ˆ ˆ

2 2

 

1

= 0, , .

xx x

T

P P P r P

xQ

  

For any

r

          

> 0

 , the Schauder’s theory implies that

,

=

P xUxx x, is uniformly bounded and the bound depends on known data and  . Now we can

m principle again on

apply the maximu QT

 

 to conclude that P x

 

, is uniformly b nded. One can also use the same argument for W to conclude the es- timate for

ou

 

x, xt

U  in QT

 

 . Similar estimates hold for the discretized solution N

 

V s,t s and

h

 

, N

x

V s t .

Q.E.D.

Lemma 2.5: There exists a constant C4 such that

 

2

dt

where depends only on known data and

4 0

d

d ,

T N

S t t C

 

2

C  , but not

on

f:

N.

Proo First of all, SN

 

t is continuous and is also diffe ntire able on

 

0,T except =t t nn, = 0,1,N

ws that

. It fol- lo SN

 

tH1

0,T

.

From the def of VN undary condition

inition

 

s t, and the bo (2.2), we know that, for tn1t<tn,

 

n1

d

= .

d

N Sn S

S t

t h

(5)

Note that Sn1<Sn, then

 

 

1 1

1

1

=

, , 1

= =

n n n n

, d

N N

S

n n n N

y Sn

V S V S

V S t V S t

V y t y

h h

It follows that n n

S S

h

 

 

 

 

2 2

1 =1

5

d d

d = d

d

,

N

T N tn N

tn n

N h L

QT

t t S t t

t

C V C

 

 



where depends only on known data and

0 dtS

5

C  .

Q.E.

the re e ready to

exist

in follows the e same argum s fo

D.

With sults of Lemmas 2.1-2.5, we ar prove th following theorem. e

Theorem 2.6: The free boundary problem (1.1)-(1.5) has a unique solution

V s t

   

, ,S t

with

 

 

1,2

, 0, ;

V x tL T W  and

 

C

T

Proof: First of all, olution

1

0,

 

 .

ence of a weak s

S t

the

 

,

U s t

that in [

T

Q xactly ent a

1, page uenes

34] (Theorem 5. 138). The uniq s llows from the variational inequality. Moreover, regu-larity theory for parabolic equation implies that

 

,

 

2 ,1

 

1

2 2

, T T .

U s t C Q C Q

 

 

Moreover, since the coefficients of the Equation (2.4) depends only on

 

 

, we use the interior re ularity of para

g bolic equations to conclude that

 

2 ,1 1 2

s T

U C Q

 

 

 .

To see the regularity of the free boundary, we use Lemma 2.5 to see SN

 

tH1

0,T

and

  5

1 0, .

N

S C

  

It follows that

H T

 

 

1 2 0 ,

sup

t t  

1 2

1 2

.

N N

T

S t S t C t t

 

 

Hence, by Ascoli-Arzela’s lemma, we can extract a subsequence, still denoted by SN

 

t , such that SN

 

t

converges to a function, denoted by S t

 

. Moreover,

 

12

0,

S tC T . Since  > 0 is arbitrarily, we Furt

have S t

 

C12 0,

T

.

hermore, since f x

,

L

 

QˆT , we use Wp2,1

at for an ,

- estimate to obtain th y p> 1

 

 

2,1 ˆ ,

Wp QT

U C

where C depends only on kn ata

 

own d , p and  . Now we convert back to the origin variables to con-clude that

al

 

2,1

 

, .

V s tWp QT

By Sobolev’s embedding, we know that V s t

 

, and

 

, s

V s t

since

are continuous over QT. On the other hand,

 

, = , 0

 

, 0

V s t Ks  s S t  t T,

we obtain

 

,

=

 

,

 

,

= 1, < .

s

V S t t K S t V S t t

t T

0 <

 

To see more regularity for , we use the boundary condition (2.5)-(2.6). Ind the condition (2.5)- (2.6), we see

 

S t

eed, from

 

,

= .

U X   T

We differentiate (

0, <

2.6) to find

 

,

 

 

,

.

xx x

X

U X X U X

T

 

 

( )

= e X , <

     

  

 

From the Equation (2.4) we obtain

 

( ) 2

 

ˆ

 

, = X xx

Kr

U X   e   .

 

 

It follows that

 

ˆ

 

 

 

= , ,

ˆ

2 x < .

X U X T

Kr

 

  

    

Now we consider the free boundary problem for

 

, = x

 

,

W xU x in QT

 

 :

 

 

 

 

 

 

ˆ ˆ ˆ ˆ

2 2

,

xx x

W W r W r W

loc

          

 

2 2

1 1

ˆ

= 0, x, QTa

 

 

( )

, = X , < ,

W X   e   T locall

 

ˆ

 

 

 

= , ,

ˆ

2 < ,

X W X T

Kr

 

  

    

 

, 0 = x

 

, 0 ,

 

0 < < ,

W x U x X xlocal

   

W x, ,X

It is easy to see that a unique solution exists with X

 

 C1

 

,T . It follows that

 

1

0, .

S tC T

Q.E.D.

Remark 2.1: For the existence and uniqueness, we only need to assume that 

 

t and r

 

t are of class

0,

LT with a positive und .

un

As we m e interested in

lower bo for 

 

t

(6)

how the free boundary changes when 

 

t changes. It

.1)- and

turns out that a comparison principle holds.

Theorem 3.1: Let 1

 

t and 2

 

satisfy the

assumption H(1). Let

V s t1

   

, ,S t1

and

   

V s t, ,S t

be the solu ions of the

t

pr

2 2 oblem (1

(1.5) corresponding to  2

 

t .

t

 

1 t

If 1

 

t 2

 

t on

0,T

, then

 

 

1 , 2 , 1 ,

V s tV s t

, S tS2

t

0 < <t T.

To prove the theorem, we show that the c mparison property holds for the discrete solution und r certain co

o e ndition.

Lemma 3.1: If h< 21

bR , then

 

2

2

d

< ds Vn s 0, Sn S<.

Proof: If necessary, we may use an approximation to replace by a smooth c vex function on

  

=

N

V s Ks

0

N

V s en

at

on

SN,

. Without loss of generality, we may simply assume

 

  . Th from the regularity theory, we know th Vn

 

s is differentiable in

Sn,

. Let

 

=Vn s , Sn < <s .

Now for 1, we differentiate uation

 

n

u s

the Eq (2.1) twice with resp

=

n N

ect to s to see that satisfies the fo

 

n

u s

llowing equation:

 

2 2

1 1

(2 )

2 n n n n n n

1

= 0, < < .

n n

N n

s u r su u

      r h

V s S s

h

 

 



  

From the maximum principle, we see that un

 

s can not attain a negative minimum if 2 1

< 0 n rn

h

On the other hand, from the Equations (2.1) and (2.1) we

   .

see

 

2

2

= n .

n n

r u S

nSn

It follows that, if h< 21

bR,

Once we know , we can use the maxi-mum principl e same clusion for

Q.E.D.

 

<

n

u s 0, Sn s<.

 

1 0

N

us  

e to obtain th inite numbe

con

=N2. After a f r of steps, we obtain the desired result of Lemma 3.1.

Since we are interested in the relation between

V

and

n

 

,

n s Snn, for convenience we use

s,

:=V

s

and

n n

V Sn

 

 :=Sn instead of Vn

s,n

and Sn

 

n .

.2: Fo n= 0,1,,N1,

Lemma 3 r

,

 

n

V s

 d

> 0, < 0. dSn  

Proof: Let

,

, = Vn s

W s  .

 

 We differen

=

tiate Equation (2.1) for with re- spect to

=

n N

n to obtain:

 

2

2 2 2

2

d

1 1

:= = n.

n

V

LW s W rsW r W

2 h s ds

 

 

  

From Lemma 3.1, we see that

2 2

1 1

0, < < . 2 s W rsW rn h W Sn s

 

    

The maximum principle implies that

 

 

,

W s can not attain a negative minimum at an interior point in

Sn,

.

On Sn =Sn

 

 :

 

S  ,

=K S

 

 ,V

S

 

 ,

= 1.

n n n ns n

V  

We differentiate Vn

Sn

 

 ,

with respect to  to obtain

 

Sn  ,

=0.

W

It follow W s

,

0 for s

Sn,

,

 

a, the same argument to

= 1, , 0

n N  .

s that b

when

obtain e co

ndary condition have

=

n N

the sam

. Now we can use nclusion for

Moreover, from the second bou , we

 

dSn

 

 

, , = 0

V S  V S   .

om Equation (2.1) we know d

nss n nsn

Also, fr

2

2

= n .

nss n n

r V

S

It follows that

 

2

 

d

= ,

d 2

n n n

s n n

S S

W S r

 

.  

 

Since W s

,

attains its minimum 0 at the boundary

 

n

S  ,

Thus,

by Hopf’s lemma, we see W Ss

n

 

 ,

> 0.

 

d

< 0. d Sn  Q.E.D.

(7)

Proof of Theorem 3.1: Let 1

 

t and 2

 

t

satisfy the assumption H(1). Let

   

t and corres-

be the solutions

1 ,t ,S1

(1.5)

V s

of

(1.1)- 

2 s t, ,S

 

V 2 t

ponding 1

 

t and 2

 

t . If 1

 

t <2

 

t on

 

0,T .

We define

 

1

1

= tk d , = 1, 2; = 1, 2

ik i

tk i

h

   

Let V s Sin

be t solutio of the em 1)-

(2.3) corres ding to volat

, , .

kN

he n probl (2. the ility

 

in ,

pon in. It is clear that

1n< 2n

  for n= 1, 2,,N if 1

 

t <2

 

t on

 

0,T . By Lemma 3.1 and Lemma 3.2, if h< 21

bR

we have

Fro

 

 

1n 1n > 2n 2n , = 0, , , .

SSn 1, 2 N

m the definition of SN

 

t , we know that ,

provided that

 

 

1 > 2 , 0

N N

S t S t  t T

2

1 <

h

bR.

Since 1

 

N

S t and 2

N

S

 

t re uniformly con

 

, re

a ve

to spectively, a . It

fo

.D.

: It is clear that the comparison result in Theorem 3.1 still holds if with positive lower and upper boun

4. Conclusion

igger when th

volatility is a function , it is not clear how the option price

boundary change when the vo rgent

 

1 S t

llows t and hat

2

S t s N 

 

1 2 , 0 .

S tS

tt T

It is also clear that V sV2

 

s t, on QT.

Q.E

Remark 3.1

 

1 ,t

 

t L 0,T

ds.

a

When the volatility is a constant, it has been known for a long time that the option price is b e volatil- ity is bigger. However, when the

of time,  =

 

t

nor the optimal excise latil- ity changes for the whole time period

 

0,T . In this pa- per we answered such a question. We show that a com- parison property for option price and the optimal excis- ing bound (Theorem 3.1) when the volatility

 

 

1 t 2 t

  . This result is important for option traders. Moreover, we proved a global regularity result for the free boundary by using a very different method from the existing literature.

ledgements

Some results in this paper were reported at the interna- tional conference “Problems and Challenges in Financial Engineering and Ri

ary hold

5. Acknow

sk Management” held in Tongji 1. The author would like to an, Professor Xinfu Chen,

all, New York, 2008. [2] P. Jaillet, D. Lamberton and B. Lapeyre, “Variational

Inequalities an can Options,” Acta Applied Mathe 990, pp. 263-289.

for Rational Mechanics

e near Expiration,” Mathematical

thematical

Fi-d Sons, Inc., New

. 139-158.

, pp. 241-286.

, No. 3,

a Jump-Diffusion Model,”

. Dai, “Convergence of the Explicit

tic Valuation of American Options,”

of Univisitatis

s and Surveys in Pure and Applied Mathematics,”

ournal of Applied Mathematics, Vol. 10, 2001, pp. 1-13.

Uni-Vol. 84, Addison-Wesley Longman, London, 1997. [17] D. Sevcovic, “Analysis of the Free Boundary for the

Pric-ing of an American Call Option,” European J versity from June 23-24, 201

thank Professor Baojun Bi

Professor Min Dai, Professor Weian Zheng and other participants for their comments, which improves the original version of the paper.

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s, Vol. 41,

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ndary for American Put

Keller, “Optimal Exercise

Bound-pplied

Mathe-es,”

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and Its Critical Stock Price,” Journal of Finance, Vol. 55, No. 5, 2000, pp. 2333-2356.

[19] E. Bayraktar and Hao Xing, “Analysis of the Optimal Exercise Boundary of American Options for Jump Diffu- sions,” SIAM Journal of Mathematical Analysi [28] No. 2, 2009, pp. 825-860.

[20] X. F. Chen and J. Chadam, “Analytic and Numerical

Approximations for the Early r the [29] X. F. Chen, J. Chadam, L. S. Jiang and W. A. Zheng, “Convexity of the Exercise Boundary of the American Put Option on a Zero Dividend Asset,” Mathem

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[22] S. D. Jacka, “Optimal Stopping and the American Put,” Mathematical Finance, Vol. 1, No. 1, 1991, pp. 1-14. [23] C. Knessl, “Asymptotic Analysis of the American Call

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References

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