Homework 10 Solutions - Introduction to Probability | MATH 180A, Assignments of Mathematics

Material Type: Assignment; Class: Introduction to Probability; Subject: Mathematics; University: University of California - San Diego; Term: Fall 2009;

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Math 180A, Fall 2009
Homework 10 Solutions
4.5.4. If a > 0, then
FaX+b(x) = P(aX +bx) = P(X(xb)/a) = F((xb)/a).
If a < 0, then
FaX+b(x) = P(aX +bx) = P(X(xb)/a)
= 1 P(X < (xb)/a) = 1 F(xb)
a.
4.5.5. By the symmetry of fX, we have FX(x) = 1 FX(x), so it is enough to calculate FX(x)
for x0. We have
FX(x) = Zx
−∞
1
2e−|t|dt
=1
2+1
2Zx
0
etdt
=1
2+1
2(1 ex)
= 1 1
2ex.
Therefore,
FX(x) = 1
2ex, x 0,
11
2ex, x 0.
4.5.6. (a) P(X1/2) = 1 P(X < 1/2) = 1 (1/2)3= 7/8.
(b) f(x) = F(x) = 3x2for 0 < x < 1.
(c) E(X) = R1
0x·3x3dx =R1
03x3dx = 3/4.
(d) Xis the largest of Y1,Y2, and Y3. Therefore, for 0 x1,
P(Xx) = P(Y1x, Y2x, Y3x)
=P(Y1x)·P(Y2x)·P(Y3x)
=x·x·x=x3,
as desired.
4.5.7. (a) Observe that Yis a one-to-one function of T. For y=twe have t=y2and
dt/dy = 2y, so
fY(y) = fT(y2)·2y=λeλy22y= 2λyeλy 2,
for y0.
(b) When λ= 3,
E(Y) = Z
0
6y2e3y2dy = 31/2Z
0
z1/2ezdz,
1
pf2

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Math 180A, Fall 2009

Homework 10 Solutions

4.5.4. If a > 0, then

FaX+b(x) = P (aX + b ≤ x) = P (X ≤ (x − b)/a) = F ((x − b)/a).

If a < 0, then

FaX+b(x) = P (aX + b ≤ x) = P (X ≥ (x − b)/a)

= 1 − P (X < (x − b)/a) = 1 − F

(x − b)

a

4.5.5. By the symmetry of fX , we have FX (−x) = 1 − FX (x), so it is enough to calculate FX (x)

for x ≥ 0. We have

FX (x) =

∫ (^) x

−∞

e−|t|^ dt

∫ (^) x

0

e

−t dt

(1 − e

−x )

e−x.

Therefore,

FX (x) =

2 e

x, x ≤ 0,

1 − 12 e−x, x ≥ 0.

4.5.6. (a) P (X ≥ 1 /2) = 1 − P (X < 1 /2) = 1 − (1/2)^3 = 7/8.

(b) f (x) = F ′(x) = 3x^2 for 0 < x < 1.

(c) E(X) =

0 x^ ·^3 x

(^3) dx = ∫^1 0 3 x

(^3) dx = 3/4.

(d) X is the largest of Y 1 , Y 2 , and Y 3. Therefore, for 0 ≤ x ≤ 1,

P (X ≤ x) = P (Y 1 ≤ x, Y 2 ≤ x, Y 3 ≤ x)

= P (Y 1 ≤ x) · P (Y 2 ≤ x) · P (Y 3 ≤ x)

= x · x · x = x^3 ,

as desired.

4.5.7. (a) Observe that Y is a one-to-one function of T. For y =

t we have t = y^2 and

dt/dy = 2y, so

fY (y) = fT (y

2 ) · 2 y = λe

−λy^2 2 y = 2λye

−λy^2 ,

for y ≥ 0.

(b) When λ = 3,

E(Y ) =

0

6 y^2 e−^3 y

2 dy = 3−^1 /^2

0

z^1 /^2 e−z^ dz,

where we have made the change of variables z = 3 y^2. This integral is equal to Γ(3/2) =

(1/2)Γ(1/2) =

π/2. Therefore, E(Y ) = (^12)

π/3 = 0.512.

Alternatively, we can evaluate E(Y ) by integrating by parts:

E(Y ) =

0

6 y

2 e

− 3 y^2 dy =

0

y · 6 ye

− 3 y^2 dy

= −ye

− 3 y^2

0

0

e

− 3 y^2 dy

0

e

− 3 y^2 dy

Making the change of variables x =

6 y (so x^2 /2 = 3y^2 and dx =

6 dy), this last integral can be

rewritten as 1 √ 6

0

e

−x^2 / 2 dx.

But the symmetry of the standard normal density implies that

∫ (^) ∞

0

2 π

e

−x^2 / 2 dx = 1/ 2 ,

so that (^) ∫ (^) ∞

0

e−x

(^2) / 2 dx =

π/ 2.

It follows that

E(Y ) =

π/ 2 √ 6

π/ 3 ,

as before.

4.5.8. Let the lifetimes of the individual components be Ti and let L be the lifetime of the system.

Let us write λi = μ− i 1 for the rate of the exponential random variable Ti.

(c) The random variable min(T 1 , T 2 ) has the exponential distribution with parameter λ 1 + λ 2 ;

the random variable min(T 3 , T 4 ) has the exponential distribution with parameter λ 3 +λ 3. Therefore

P (L > t) = 1 − P (L ≤ t) = 1 − P (min(T 1 , T 2 ) ≤ t, min(T 3 , T 4 ) ≤ t)

= 1 − (1 − e

−t(λ 1 +λ 2 ) )(1 − e

−t(λ 3 +λ 4 ) ).

When μi = i this becomes

P (L > t) = 1 − (1 − e

− 2 t/ 3 )(1 − e

− 7 t/ 12 ) = e

− 2 t/ 3

  • e

− 7 t/ 12 − e

− 7 t/ 18 .

(d) We now have

P (L > t) = P (max(T 1 , T 2 ) > t, T 3 > t) = P (max(T 1 , T 2 ) > t) · P (T 3 > t)

[

1 − (1 − e

−λ 1 t )(1 − e

−λ 2 t )

]

e

−λ 3 t .

When μi = i this becomes

P (L > t) =

[

1 − (1 − e

−t )(1 − e

−t/ 2 )

]

e

−t/ 3 = e

− 4 t/ 3

  • e

− 5 t/ 6 − e

− 11 t/ 6 .