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Lecture 18More on option pricing
Lecture 18 1 / 21
Introduction
In this lecture we will see more applications of option pricing theory.
Lecture 18 2 / 21
Greeks (1)
The price f of a derivative depends on several parameters.
The sensitivity of the price with respect to parameter is called a greek.
Some of the most important greeks are
∆ =∂f
∂S
Γ =∂2f
∂S2
Θ =∂f
∂t
V =∂f
∂σ(‘Vega’)
Lecture 18 3 / 21
Greeks (1)
The price f of a derivative depends on several parameters.
The sensitivity of the price with respect to parameter is called a greek.
Some of the most important greeks are
∆ =∂f
∂S
Γ =∂2f
∂S2
Θ =∂f
∂t
V =∂f
∂σ(‘Vega’)
Lecture 18 3 / 21
Greeks (1)
The price f of a derivative depends on several parameters.
The sensitivity of the price with respect to parameter is called a greek.
Some of the most important greeks are
∆ =∂f
∂S
Γ =∂2f
∂S2
Θ =∂f
∂t
V =∂f
∂σ(‘Vega’)
Lecture 18 3 / 21
Greeks (1)
The price f of a derivative depends on several parameters.
The sensitivity of the price with respect to parameter is called a greek.
Some of the most important greeks are
∆ =∂f
∂S
Γ =∂2f
∂S2
Θ =∂f
∂t
V =∂f
∂σ(‘Vega’)
Lecture 18 3 / 21
Greeks (1)
The price f of a derivative depends on several parameters.
The sensitivity of the price with respect to parameter is called a greek.
Some of the most important greeks are
∆ =∂f
∂S
Γ =∂2f
∂S2
Θ =∂f
∂t
V =∂f
∂σ(‘Vega’)
Lecture 18 3 / 21
Greeks (1)
The price f of a derivative depends on several parameters.
The sensitivity of the price with respect to parameter is called a greek.
Some of the most important greeks are
∆ =∂f
∂S
Γ =∂2f
∂S2
Θ =∂f
∂t
V =∂f
∂σ(‘Vega’)
Lecture 18 3 / 21
Greeks (2)
The greeks are used in risk management.
Note that
∆ =∂f
∂S,
which means that xt = ∆ in the hedging portfolio of the derivative.
In the Black-Scholes model we have
∆call = Φ(d1),
where again
d1 =ln(S/K ) + (rf + σ2/2)(T − t)
σ√T − t
.
Lecture 18 4 / 21
Greeks (2)
The greeks are used in risk management.
Note that
∆ =∂f
∂S,
which means that xt = ∆ in the hedging portfolio of the derivative.
In the Black-Scholes model we have
∆call = Φ(d1),
where again
d1 =ln(S/K ) + (rf + σ2/2)(T − t)
σ√T − t
.
Lecture 18 4 / 21
Greeks (2)
The greeks are used in risk management.
Note that
∆ =∂f
∂S,
which means that xt = ∆ in the hedging portfolio of the derivative.
In the Black-Scholes model we have
∆call = Φ(d1),
where again
d1 =ln(S/K ) + (rf + σ2/2)(T − t)
σ√T − t
.
Lecture 18 4 / 21
Greeks (3)
What is the Delta of a put?
Use the put-call parity:
Price of put + S = Price of call + Ke−rf (T−t).
Taking ∂/∂S on the LHS and the RHS yields
∆put + 1 = ∆call ⇔ ∆put = ∆call − 1.
In the Black-Scholes model we get
∆put = N(d1)− 1 = −N(−d1).
Lecture 18 5 / 21
Greeks (3)
What is the Delta of a put?
Use the put-call parity:
Price of put + S = Price of call + Ke−rf (T−t).
Taking ∂/∂S on the LHS and the RHS yields
∆put + 1 = ∆call ⇔ ∆put = ∆call − 1.
In the Black-Scholes model we get
∆put = N(d1)− 1 = −N(−d1).
Lecture 18 5 / 21
Greeks (3)
What is the Delta of a put?
Use the put-call parity:
Price of put + S = Price of call + Ke−rf (T−t).
Taking ∂/∂S on the LHS and the RHS yields
∆put + 1 = ∆call
⇔ ∆put = ∆call − 1.
In the Black-Scholes model we get
∆put = N(d1)− 1 = −N(−d1).
Lecture 18 5 / 21
Greeks (3)
What is the Delta of a put?
Use the put-call parity:
Price of put + S = Price of call + Ke−rf (T−t).
Taking ∂/∂S on the LHS and the RHS yields
∆put + 1 = ∆call ⇔ ∆put = ∆call − 1.
In the Black-Scholes model we get
∆put = N(d1)− 1 = −N(−d1).
Lecture 18 5 / 21
Greeks (3)
What is the Delta of a put?
Use the put-call parity:
Price of put + S = Price of call + Ke−rf (T−t).
Taking ∂/∂S on the LHS and the RHS yields
∆put + 1 = ∆call ⇔ ∆put = ∆call − 1.
In the Black-Scholes model we get
∆put = N(d1)− 1
= −N(−d1).
Lecture 18 5 / 21
Greeks (3)
What is the Delta of a put?
Use the put-call parity:
Price of put + S = Price of call + Ke−rf (T−t).
Taking ∂/∂S on the LHS and the RHS yields
∆put + 1 = ∆call ⇔ ∆put = ∆call − 1.
In the Black-Scholes model we get
∆put = N(d1)− 1 = −N(−d1).
Lecture 18 5 / 21
Perpetual American options (1)
When the derivative is of American type, then we are allowed to choosethe time at which we want to get the derivatives payoff.
In general it is a very hard problem to determine the price and the optimaltime at which an American option should be exercised.
There is however one case when the problem is simplified, and that iswhen the option is of perpetual type.
A perpetual derivative has T =∞.
Lecture 18 6 / 21
Perpetual American options (1)
When the derivative is of American type, then we are allowed to choosethe time at which we want to get the derivatives payoff.
In general it is a very hard problem to determine the price and the optimaltime at which an American option should be exercised.
There is however one case when the problem is simplified, and that iswhen the option is of perpetual type.
A perpetual derivative has T =∞.
Lecture 18 6 / 21
Perpetual American options (1)
When the derivative is of American type, then we are allowed to choosethe time at which we want to get the derivatives payoff.
In general it is a very hard problem to determine the price and the optimaltime at which an American option should be exercised.
There is however one case when the problem is simplified, and that iswhen the option is of perpetual type.
A perpetual derivative has T =∞.
Lecture 18 6 / 21
Perpetual American options (1)
When the derivative is of American type, then we are allowed to choosethe time at which we want to get the derivatives payoff.
In general it is a very hard problem to determine the price and the optimaltime at which an American option should be exercised.
There is however one case when the problem is simplified, and that iswhen the option is of perpetual type.
A perpetual derivative has T =∞.
Lecture 18 6 / 21
Perpetual American options (2)
Let us consider the Black-Scholes model.
Recall Black-Scholes equation:
∂f
∂t+ rf S
∂f
∂S+
1
2σ2S2 ∂
2f
∂S2− rf f = 0.
When T =∞ in the Black-Scholes mode, the term ∂f /∂t disappears fromthe equation due to time-homogeneity, and we get an ODE instead of aPDE:
rf Sf′ +
1
2σ2S2f ′′ − rf f = 0.
To solve this equation, we look for solutions on the form
f (S) = Sa
with a ∈ R.
Lecture 18 7 / 21
Perpetual American options (2)
Let us consider the Black-Scholes model.
Recall Black-Scholes equation:
∂f
∂t+ rf S
∂f
∂S+
1
2σ2S2 ∂
2f
∂S2− rf f = 0.
When T =∞ in the Black-Scholes mode, the term ∂f /∂t disappears fromthe equation due to time-homogeneity, and we get an ODE instead of aPDE:
rf Sf′ +
1
2σ2S2f ′′ − rf f = 0.
To solve this equation, we look for solutions on the form
f (S) = Sa
with a ∈ R.
Lecture 18 7 / 21
Perpetual American options (2)
Let us consider the Black-Scholes model.
Recall Black-Scholes equation:
∂f
∂t+ rf S
∂f
∂S+
1
2σ2S2 ∂
2f
∂S2− rf f = 0.
When T =∞ in the Black-Scholes mode, the term ∂f /∂t disappears fromthe equation due to time-homogeneity
, and we get an ODE instead of aPDE:
rf Sf′ +
1
2σ2S2f ′′ − rf f = 0.
To solve this equation, we look for solutions on the form
f (S) = Sa
with a ∈ R.
Lecture 18 7 / 21
Perpetual American options (2)
Let us consider the Black-Scholes model.
Recall Black-Scholes equation:
∂f
∂t+ rf S
∂f
∂S+
1
2σ2S2 ∂
2f
∂S2− rf f = 0.
When T =∞ in the Black-Scholes mode, the term ∂f /∂t disappears fromthe equation due to time-homogeneity, and we get an ODE instead of aPDE:
rf Sf′ +
1
2σ2S2f ′′ − rf f = 0.
To solve this equation, we look for solutions on the form
f (S) = Sa
with a ∈ R.
Lecture 18 7 / 21
Perpetual American options (2)
Let us consider the Black-Scholes model.
Recall Black-Scholes equation:
∂f
∂t+ rf S
∂f
∂S+
1
2σ2S2 ∂
2f
∂S2− rf f = 0.
When T =∞ in the Black-Scholes mode, the term ∂f /∂t disappears fromthe equation due to time-homogeneity, and we get an ODE instead of aPDE:
rf Sf′ +
1
2σ2S2f ′′ − rf f = 0.
To solve this equation, we look for solutions on the form
f (S) = Sa
with a ∈ R.
Lecture 18 7 / 21
Perpetual American options (2)
Let us consider the Black-Scholes model.
Recall Black-Scholes equation:
∂f
∂t+ rf S
∂f
∂S+
1
2σ2S2 ∂
2f
∂S2− rf f = 0.
When T =∞ in the Black-Scholes mode, the term ∂f /∂t disappears fromthe equation due to time-homogeneity, and we get an ODE instead of aPDE:
rf Sf′ +
1
2σ2S2f ′′ − rf f = 0.
To solve this equation, we look for solutions on the form
f (S) = Sa
with a ∈ R.
Lecture 18 7 / 21
Perpetual American options (3)
Inserting this into the ODE yields
rf SaSa−1 +
1
2σ2S2a(a− 1)Sa−2 − rf S
a = 0
⇔
Sa
[rf a +
1
2σ2a(a− 1)− rf
]= 0.
⇔
a2 +
(2rfσ2− 1
)a− 2rf
σ2= 0.
The solution to this equation is
a1 = 1 and a2 = −2rfσ2
Lecture 18 8 / 21
Perpetual American options (3)
Inserting this into the ODE yields
rf SaSa−1 +
1
2σ2S2a(a− 1)Sa−2 − rf S
a = 0
⇔
Sa
[rf a +
1
2σ2a(a− 1)− rf
]= 0.
⇔
a2 +
(2rfσ2− 1
)a− 2rf
σ2= 0.
The solution to this equation is
a1 = 1 and a2 = −2rfσ2
Lecture 18 8 / 21
Perpetual American options (3)
Inserting this into the ODE yields
rf SaSa−1 +
1
2σ2S2a(a− 1)Sa−2 − rf S
a = 0
⇔
Sa
[rf a +
1
2σ2a(a− 1)− rf
]= 0.
⇔
a2 +
(2rfσ2− 1
)a− 2rf
σ2= 0.
The solution to this equation is
a1 = 1 and a2 = −2rfσ2
Lecture 18 8 / 21
Perpetual American options (3)
Inserting this into the ODE yields
rf SaSa−1 +
1
2σ2S2a(a− 1)Sa−2 − rf S
a = 0
⇔
Sa
[rf a +
1
2σ2a(a− 1)− rf
]= 0.
⇔
a2 +
(2rfσ2− 1
)a− 2rf
σ2= 0.
The solution to this equation is
a1 = 1 and a2 = −2rfσ2
Lecture 18 8 / 21
Perpetual American options (4)
Hence, the solution to the time-homogenuous Black-Scholes equation isgiven by
f (S) = A1S + A2S−2rf /σ2
.
for A1,A2 ∈ R.
How do we determine the constants A1 and A2?
They will depend on the derivative’s payoff.
Lecture 18 9 / 21
Perpetual American options (4)
Hence, the solution to the time-homogenuous Black-Scholes equation isgiven by
f (S) = A1S + A2S−2rf /σ2
.
for A1,A2 ∈ R.
How do we determine the constants A1 and A2?
They will depend on the derivative’s payoff.
Lecture 18 9 / 21
Perpetual American options (4)
Hence, the solution to the time-homogenuous Black-Scholes equation isgiven by
f (S) = A1S + A2S−2rf /σ2
.
for A1,A2 ∈ R.
How do we determine the constants A1 and A2?
They will depend on the derivative’s payoff.
Lecture 18 9 / 21
The perpetual American put option (1)
Let us consider a put option with strike price K :
F (S(t)) = max(K − S(t), 0).
Note that there is no given exercise time – we have to choose that time aswell.
Now consider the general solution
f (S) = A1S + A2S−2rf /σ2
.
Sincelim
S→∞F (S) = 0,
we must havelim
S→∞f (S) = 0 ⇒ A1 = 0.
Lecture 18 10 / 21
The perpetual American put option (1)
Let us consider a put option with strike price K :
F (S(t)) = max(K − S(t), 0).
Note that there is no given exercise time – we have to choose that time aswell.
Now consider the general solution
f (S) = A1S + A2S−2rf /σ2
.
Sincelim
S→∞F (S) = 0,
we must havelim
S→∞f (S) = 0 ⇒ A1 = 0.
Lecture 18 10 / 21
The perpetual American put option (1)
Let us consider a put option with strike price K :
F (S(t)) = max(K − S(t), 0).
Note that there is no given exercise time – we have to choose that time aswell.
Now consider the general solution
f (S) = A1S + A2S−2rf /σ2
.
Sincelim
S→∞F (S) = 0,
we must havelim
S→∞f (S) = 0 ⇒ A1 = 0.
Lecture 18 10 / 21
The perpetual American put option (1)
Let us consider a put option with strike price K :
F (S(t)) = max(K − S(t), 0).
Note that there is no given exercise time – we have to choose that time aswell.
Now consider the general solution
f (S) = A1S + A2S−2rf /σ2
.
Sincelim
S→∞F (S) = 0
,
we must havelim
S→∞f (S) = 0 ⇒ A1 = 0.
Lecture 18 10 / 21
The perpetual American put option (1)
Let us consider a put option with strike price K :
F (S(t)) = max(K − S(t), 0).
Note that there is no given exercise time – we have to choose that time aswell.
Now consider the general solution
f (S) = A1S + A2S−2rf /σ2
.
Sincelim
S→∞F (S) = 0,
we must havelim
S→∞f (S) = 0
⇒ A1 = 0.
Lecture 18 10 / 21
The perpetual American put option (1)
Let us consider a put option with strike price K :
F (S(t)) = max(K − S(t), 0).
Note that there is no given exercise time – we have to choose that time aswell.
Now consider the general solution
f (S) = A1S + A2S−2rf /σ2
.
Sincelim
S→∞F (S) = 0,
we must havelim
S→∞f (S) = 0 ⇒ A1 = 0.
Lecture 18 10 / 21
The perpetual American put option (2)
We want to exercise the put option at the first time t such that
max(K − S(t), 0)︸ ︷︷ ︸value of exercising at t
≥ f (t, S(t))︸ ︷︷ ︸value of not exercising at t
.
But it is never optimal to exercise the option when
max(K − S(t), 0) = 0.
Lecture 18 11 / 21
The perpetual American put option (2)
We want to exercise the put option at the first time t such that
max(K − S(t), 0)︸ ︷︷ ︸value of exercising at t
≥ f (t, S(t))︸ ︷︷ ︸value of not exercising at t
.
But it is never optimal to exercise the option when
max(K − S(t), 0) = 0.
Lecture 18 11 / 21
The perpetual American put option (3)
Let Sc solve the equation
K − Sc = f (Sc) = A2S−2rf /σ2
c .
Here ‘c ’ stands for critical
and Sc is the critical level at which we chooseto use the option when the stock price equals (or is less than) Sc .
Note that we need to find Sc ; this is a part of the solution.
One can show that we also have smooth fit. This means that the valuefunction f (S) meets the payoff function max(K − S , 0) tangentially.
Lecture 18 12 / 21
The perpetual American put option (3)
Let Sc solve the equation
K − Sc = f (Sc) = A2S−2rf /σ2
c .
Here ‘c ’ stands for critical and Sc is the critical level at which we chooseto use the option when the stock price equals (or is less than) Sc .
Note that we need to find Sc ; this is a part of the solution.
One can show that we also have smooth fit. This means that the valuefunction f (S) meets the payoff function max(K − S , 0) tangentially.
Lecture 18 12 / 21
The perpetual American put option (3)
Let Sc solve the equation
K − Sc = f (Sc) = A2S−2rf /σ2
c .
Here ‘c ’ stands for critical and Sc is the critical level at which we chooseto use the option when the stock price equals (or is less than) Sc .
Note that we need to find Sc ; this is a part of the solution.
One can show that we also have smooth fit. This means that the valuefunction f (S) meets the payoff function max(K − S , 0) tangentially.
Lecture 18 12 / 21
The perpetual American put option (3)
Let Sc solve the equation
K − Sc = f (Sc) = A2S−2rf /σ2
c .
Here ‘c ’ stands for critical and Sc is the critical level at which we chooseto use the option when the stock price equals (or is less than) Sc .
Note that we need to find Sc ; this is a part of the solution.
One can show that we also have smooth fit. This means that the valuefunction f (S) meets the payoff function max(K − S , 0) tangentially.
Lecture 18 12 / 21
The perpetual American put option (4)
In formulas the smooth fit condition means that
f ′(Sc) =d
dS(K − S)
∣∣∣∣S=Sc
⇔
−2rfσ2
A2S−2rf /σ2−1c = −1.
We now have a system of equations with two equations and two unknowns:
K − Sc = A2S−2rf /σ2
c
1 =2rfσ2
A2S−2rf /σ2−1c
Lecture 18 13 / 21
The perpetual American put option (4)
In formulas the smooth fit condition means that
f ′(Sc) =d
dS(K − S)
∣∣∣∣S=Sc
⇔
−2rfσ2
A2S−2rf /σ2−1c = −1.
We now have a system of equations with two equations and two unknowns:
K − Sc = A2S−2rf /σ2
c
1 =2rfσ2
A2S−2rf /σ2−1c
Lecture 18 13 / 21
The perpetual American put option (4)
In formulas the smooth fit condition means that
f ′(Sc) =d
dS(K − S)
∣∣∣∣S=Sc
⇔
−2rfσ2
A2S−2rf /σ2−1c = −1.
We now have a system of equations with two equations and two unknowns
:
K − Sc = A2S−2rf /σ2
c
1 =2rfσ2
A2S−2rf /σ2−1c
Lecture 18 13 / 21
The perpetual American put option (4)
In formulas the smooth fit condition means that
f ′(Sc) =d
dS(K − S)
∣∣∣∣S=Sc
⇔
−2rfσ2
A2S−2rf /σ2−1c = −1.
We now have a system of equations with two equations and two unknowns:
K − Sc = A2S−2rf /σ2
c
1 =2rfσ2
A2S−2rf /σ2−1c
Lecture 18 13 / 21
The perpetual American put option (5)
It is not hard to solve the system of equations, and doing this we get
f (S) = (K − Sc)
(S
Sc
)−2rf /σ2
,
where
Sc = K · 2rf2rf + σ2
.
Lecture 18 14 / 21
The perpetual American call option
Why didn’t we study the perpetual American call option?
The reason is that one can show that it is never optimal to exercise thisoption.
In fact, using the general solution
f (S) = A1S + A2S−2rf /σ2
we must have A2 = 0 in this case – otherwise f (0) = ±∞.
The smooth fit condition will then imply
f (S) = S
andSc =∞.
Lecture 18 15 / 21
The perpetual American call option
Why didn’t we study the perpetual American call option?
The reason is that one can show that it is never optimal to exercise thisoption.
In fact, using the general solution
f (S) = A1S + A2S−2rf /σ2
we must have A2 = 0 in this case – otherwise f (0) = ±∞.
The smooth fit condition will then imply
f (S) = S
andSc =∞.
Lecture 18 15 / 21
The perpetual American call option
Why didn’t we study the perpetual American call option?
The reason is that one can show that it is never optimal to exercise thisoption.
In fact, using the general solution
f (S) = A1S + A2S−2rf /σ2
we must have A2 = 0 in this case – otherwise f (0) = ±∞.
The smooth fit condition will then imply
f (S) = S
andSc =∞.
Lecture 18 15 / 21
The perpetual American call option
Why didn’t we study the perpetual American call option?
The reason is that one can show that it is never optimal to exercise thisoption.
In fact, using the general solution
f (S) = A1S + A2S−2rf /σ2
we must have A2 = 0 in this case – otherwise f (0) = ±∞.
The smooth fit condition will then imply
f (S) = S
andSc =∞.
Lecture 18 15 / 21
Risk-neutral valuation
One can show that the principle of risk-neutral valuation (or risk-neutralpricing) holds generally.
For a simple European derivative this means that the price is given by
f (t,S(t)) = e−rf (T−t)E [F (S(T ))|St ].
When calculating expected values E (· · · ), we use the dynamics
dS(t) = rf S(t)dt + σS(t)dz(t).
Lecture 18 16 / 21
Risk-neutral valuation
One can show that the principle of risk-neutral valuation (or risk-neutralpricing) holds generally.
For a simple European derivative this means that the price is given by
f (t,S(t)) = e−rf (T−t)E [F (S(T ))|St ].
When calculating expected values E (· · · ), we use the dynamics
dS(t) = rf S(t)dt + σS(t)dz(t).
Lecture 18 16 / 21
Risk-neutral valuation
One can show that the principle of risk-neutral valuation (or risk-neutralpricing) holds generally.
For a simple European derivative this means that the price is given by
f (t,S(t)) = e−rf (T−t)E [F (S(T ))|St ].
When calculating expected values E (· · · ), we use the dynamics
dS(t) = rf S(t)dt + σS(t)dz(t).
Lecture 18 16 / 21
Interest rate derivatives (1)
In general, money in the bank grows according to
dB(t) = r(t)B(t)dt with B(0) = 1.
We can solve this equation:
B(t) = e∫ t0 r(s)ds .
So far we have assumed that r(t) = rf , i.e. a constant, but we can as wellassume that r(t) is a stochastic process.
As when valuing options on stocks we can use either use a discrete timemodel or a continuous time model.
Lecture 18 17 / 21
Interest rate derivatives (1)
In general, money in the bank grows according to
dB(t) = r(t)B(t)dt with B(0) = 1.
We can solve this equation:
B(t) = e∫ t0 r(s)ds .
So far we have assumed that r(t) = rf , i.e. a constant, but we can as wellassume that r(t) is a stochastic process.
As when valuing options on stocks we can use either use a discrete timemodel or a continuous time model.
Lecture 18 17 / 21
Interest rate derivatives (1)
In general, money in the bank grows according to
dB(t) = r(t)B(t)dt with B(0) = 1.
We can solve this equation:
B(t) = e∫ t0 r(s)ds .
So far we have assumed that r(t) = rf , i.e. a constant, but we can as wellassume that r(t) is a stochastic process.
As when valuing options on stocks we can use either use a discrete timemodel or a continuous time model.
Lecture 18 17 / 21
Interest rate derivatives (1)
In general, money in the bank grows according to
dB(t) = r(t)B(t)dt with B(0) = 1.
We can solve this equation:
B(t) = e∫ t0 r(s)ds .
So far we have assumed that r(t) = rf , i.e. a constant, but we can as wellassume that r(t) is a stochastic process.
As when valuing options on stocks we can use either use a discrete timemodel or a continuous time model.
Lecture 18 17 / 21
Interest rate derivatives (2)
When using discrete time models, it is usual to use trinomial trees
:
u · rt↗
rt → rt↘
d · rt
t t + 1
Lecture 18 18 / 21
Interest rate derivatives (2)
When using discrete time models, it is usual to use trinomial trees:
u · rt↗
rt → rt↘
d · rt
t t + 1
Lecture 18 18 / 21
Interest rate derivatives (3)
In continuous time models, we use Ito diffusions to model the interest rater(t).
One can show that the value at time t ∈ [0,T ] of a zero-coupon bondwith maturity time T is given by
P(t,T ) = E(e−
∫ Tt r(s)ds
∣∣∣ rt) .Note that we use risk-neutral probabilities in this formula.
Let us now lok at some examples of models.
Lecture 18 19 / 21
Interest rate derivatives (3)
In continuous time models, we use Ito diffusions to model the interest rater(t).
One can show that the value at time t ∈ [0,T ] of a zero-coupon bondwith maturity time T is given by
P(t,T ) = E(e−
∫ Tt r(s)ds
∣∣∣ rt) .
Note that we use risk-neutral probabilities in this formula.
Let us now lok at some examples of models.
Lecture 18 19 / 21
Interest rate derivatives (3)
In continuous time models, we use Ito diffusions to model the interest rater(t).
One can show that the value at time t ∈ [0,T ] of a zero-coupon bondwith maturity time T is given by
P(t,T ) = E(e−
∫ Tt r(s)ds
∣∣∣ rt) .Note that we use risk-neutral probabilities in this formula.
Let us now lok at some examples of models.
Lecture 18 19 / 21
Interest rate derivatives (3)
In continuous time models, we use Ito diffusions to model the interest rater(t).
One can show that the value at time t ∈ [0,T ] of a zero-coupon bondwith maturity time T is given by
P(t,T ) = E(e−
∫ Tt r(s)ds
∣∣∣ rt) .Note that we use risk-neutral probabilities in this formula.
Let us now lok at some examples of models.
Lecture 18 19 / 21
Interest rate derivatives (4)
The Vasicek model:
dr(t) = a(b − r(t))dt + σdz(t)
The Cox-Ingersoll-Ross (CIR) model:
dr(t) = a(b − r(t))dt + σ√
r(t)dz(t).
The Ho-Lee model:
dr(t) = θ(t)dt + σdz(t)
The Hull-White model:
d(r) = [θ(t)− ar(t)]dt + σdz(t).
Lecture 18 20 / 21
Interest rate derivatives (4)
The Vasicek model:
dr(t) = a(b − r(t))dt + σdz(t)
The Cox-Ingersoll-Ross (CIR) model:
dr(t) = a(b − r(t))dt + σ√
r(t)dz(t).
The Ho-Lee model:
dr(t) = θ(t)dt + σdz(t)
The Hull-White model:
d(r) = [θ(t)− ar(t)]dt + σdz(t).
Lecture 18 20 / 21
Interest rate derivatives (4)
The Vasicek model:
dr(t) = a(b − r(t))dt + σdz(t)
The Cox-Ingersoll-Ross (CIR) model:
dr(t) = a(b − r(t))dt + σ√
r(t)dz(t).
The Ho-Lee model:
dr(t) = θ(t)dt + σdz(t)
The Hull-White model:
d(r) = [θ(t)− ar(t)]dt + σdz(t).
Lecture 18 20 / 21
Interest rate derivatives (4)
The Vasicek model:
dr(t) = a(b − r(t))dt + σdz(t)
The Cox-Ingersoll-Ross (CIR) model:
dr(t) = a(b − r(t))dt + σ√
r(t)dz(t).
The Ho-Lee model:
dr(t) = θ(t)dt + σdz(t)
The Hull-White model:
d(r) = [θ(t)− ar(t)]dt + σdz(t).
Lecture 18 20 / 21
Interest rate derivatives (4)
The Vasicek model:
dr(t) = a(b − r(t))dt + σdz(t)
The Cox-Ingersoll-Ross (CIR) model:
dr(t) = a(b − r(t))dt + σ√
r(t)dz(t).
The Ho-Lee model:
dr(t) = θ(t)dt + σdz(t)
The Hull-White model:
d(r) = [θ(t)− ar(t)]dt + σdz(t).
Lecture 18 20 / 21
Interest rate derivatives (5)
There is also an equation similar to the Black-Scholes equation in theinterest rate derivatives case.
Ifdr(t) = µ(r(t), t)dt + σ(r(t), t)dz(t)
then the price f (r(t), t) of a derivative satifies the PDE
∂f
∂t+ µ(r , t)
∂f
∂r+
1
2σ2(r , t)
∂2f
∂r2− rf = 0.
Lecture 18 21 / 21
Interest rate derivatives (5)
There is also an equation similar to the Black-Scholes equation in theinterest rate derivatives case.
Ifdr(t) = µ(r(t), t)dt + σ(r(t), t)dz(t)
then the price f (r(t), t) of a derivative satifies the PDE
∂f
∂t+ µ(r , t)
∂f
∂r+
1
2σ2(r , t)
∂2f
∂r2− rf = 0.
Lecture 18 21 / 21
Interest rate derivatives (5)
There is also an equation similar to the Black-Scholes equation in theinterest rate derivatives case.
Ifdr(t) = µ(r(t), t)dt + σ(r(t), t)dz(t)
then the price f (r(t), t) of a derivative satifies the PDE
∂f
∂t+ µ(r , t)
∂f
∂r+
1
2σ2(r , t)
∂2f
∂r2− rf = 0.
Lecture 18 21 / 21