4.2 HW 2

  4.2.1 Problems listing
  4.2.2 Problem 2.2.3
  4.2.3 Problem 2.2.10 (or part a of problem 2)
  4.2.4 Problem 2.2.11 (or part b of problem 2)
  4.2.5 Problem 3
  4.2.6 Problem 4
  4.2.7 key solution for HW 2

4.2.1 Problems listing

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4.2.2 Problem 2.2.3

Evaluate 01exdx. Show that 0ex4dx=Γ(54)

Solution

Let y=x. Thereforedydx=121x=121y

Anddx=2ydy When x=0, y=0 and when x=1,y=1. Substituting this back into 01exdx gives 01ey(2ydy)=201yeydy. This integral is evaluated using integration by parts. udv=uv|0101vdu Let u=y and dv=ey, then du=dy and v=ey. The above becomes2(01yeydy)=2(uv|0101vdu)=2(yey|0101eydy)=2((e10)ey|01)=2(e(e1))=2(ee+1)=2

Hence 01exdx=2 For the second part of the question asking to evaluate 0ex4dx, letx=y14 Then dxdy=14y(141) When x=0,y=0 and when x=,y=. Hence the above integral becomes0ex4dx=0ey(14y(141)dy)(1)=140y(141)eydy

Comparing the above to integral (2.1.39) in the book which says(2)F(n)=0yneydy(3)Γ(n)=F(n1)

Then putting n=14 in (3) givesΓ(14)=F(141)=0y(141)eydy

Which is (1). This means that0y(141)eydy=Γ(14) Hence (4)140y(141)eydy=14Γ(14) To obtain the final form, the following property of Gamma functions is usedΓ(n+1)=nΓ(n) Which means that when n=14, the above becomesΓ(14+1)=14Γ(14)Γ(54)=14Γ(14)

Using this in (4) shows that140y(141)eydy=Γ(54) Which implies0ex4dx=Γ(54) Which is what we are asked to show.

4.2.3 Problem 2.2.10 (or part a of problem 2)

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Figure 4.3:Problem statment

Solution

Let I(a)=01ta1lntdt Where a=1 for the specific integral in this problem. The above is the parametrized general form. Taking derivative w.r.t a gives dI(a)da=dda(01ta1lntdt)=01dda(ta1lnt)dt(1)=011lntdda(ta1)dt

But dda(ta1)=dda(ealnt1)(2)=ln(t)(ealnt)

Substituting (2) into (1) givesdI(a)da=011lnt(ln(t)(ealnt))dt=01ealntdt=01tadt=ta+1a+1|01(3)=11+aa1

Integrating the above is used to I(a) givesI(a)=0a11+τdτ=ln(1+τ)|0a=ln(1+a)ln(1)=ln(1+a)a1

When a=1 the above becomesI(1)=01t1lntdt=ln(1+1)=ln(2)

Hence01t1lntdt=ln(2)

4.2.4 Problem 2.2.11 (or part b of problem 2)

   4.2.4.1 part (1)
   4.2.4.2 part (2)

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Figure 4.4:Problem statment

Solution

4.2.4.1 part (1)

I=0eaxsinkxdx Taking derivative w.r.t a givesdIda=dda(0eaxsinkxdx)=0dda(eaxsinkx)dx=0xeaxsinkxdx=0xeaxsinkxdx

Which is the integral the problem is asking to find. Therefore, since I is also given as ka2+k2 then0xeaxsinkxdx=dda(ka2+k2)=kdda(1a2+k2)=k(1)(a2+k2)2(2a)=2ak(a2+k2)2

Therefore0xeaxsinkxdx=2ak(a2+k2)2

4.2.4.2 part (2)

I=0eaxsinkxdx Taking derivative w.r.t. k givesdIdk=ddk(0eaxsinkxdx)=0ddk(eaxsinkx)dx=0eaxddk(sinkx)dx=0xeaxcoskxdx

Which is the integral the problem is asking to find. Therefore, since I is also given as ka2+k2 then0xeaxcoskxdx=ddk(ka2+k2)=(a2+k2)k(2k)(a2+k2)2=a2+k22k2(a2+k2)2=a2k2(a2+k2)2

Hence0xeaxcoskxdx=a2k2(a2+k2)2

4.2.5 Problem 3

   4.2.5.1 Part (a)
   4.2.5.2 Part b

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Figure 4.5:Problem statment

Solution

4.2.5.1 Part (a)

P(x,β)=Aeαx2+βx3 Expanding around β=0 by fixing x, gives(1)P(x,β)=P(x,0)+βPβ|β=0+β22!2Pβ2|β=0+ But (2)P(x,0)=Aeαx2 And(3)Pβ=Ax3eαx2+βx3 No need to take more derivatives since the problem is asking for first order of β. Substituting (2,3) into (1) givesP(x,β)=Aeαx2+βAx3eαx2+βx3|β=0+(4)=Aeαx2+βAx3eαx2+

Using the above in the definition P(x)dx=1 gives(Aeαx2+βAx3eαx2)dx=1(5)A(eαx2dx+βx3eαx2dx)=1

But x3eαx2dx=0 This is because eαx2 is an even function over (,+) and x3 is odd. Eq (5) now simplifies toAeαx2dx=1 But eαx2dx=πα (α>0) because it is standard Gaussian integral. The above now becomesAπα=1A=απα>0

4.2.5.2 Part b

x¯=xP(x)dx Using Eq. (4) from part (a), the above becomesx¯=x(Aeαx2+βAx3eαx2)dx=Axeαx2dx+Aβx4eαx2dx

But xeαx2dx=0 since eαx2 is an even function over (,+) and x is an odd function. The above simplifies to(6)x¯=Aβx4eαx2dx To evaluate the above, starting from the standard Gaussian integral given by I(α)=eαx2dx=πα Taking derivative w.r.t α of both sides of the above results inI(α)=ddαeαx2dx=ddαπα=x2eαx2dx=π(12)α32=x2eαx2dx=π2α32

Taking one more derivative w.r.t α givesI(α)=ddαx2eαx2dx=ddα(π2α32)=x4eαx2dx=π2(32α52)=x4eαx2dx=π2(32α52)

Now the integrand is the one we want. This shows thatx4eαx2dx=3π4α52 Using the above result in (6) givesx¯=Aβ(3π4α52) But A=απ from part(a). Hence the above becomesx¯=απβ(3π4α52)=α12β34α52=β34α5212=34βα2α>0

4.2.6 Problem 4

   4.2.6.1 Part a
   4.2.6.2 Part b

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Figure 4.6:Problem statment

Solution

4.2.6.1 Part a

dN=(4πVh3c3)E21+eEkTdE The total energy is thereforeEtotal= EdN Hence the energy density ρ isρ=1VEdN=1V0(4πVh3c3)EE21+eEkTdE=(1V)(4πVh3c3)0E31+eEkTdE(1)=4πh3c30E31+eEkTdE

k (Boltzmann constant) has units of [J][K] where J is joule and K is temperature in Kelvin. Hence units of EkT is [J][J][K][K] which is dimensionless. Let x=EkT Therefore dxdE=1kT When E=0,x=0 and when E=,x=. Substituting this into the integral in (1) gives0E31+eEkTdE=0(xkT)31+ex(kTdx)(2)=(kT)40x31+exdx

Substituting (2) into (1) gives(3)ρ=(4πh3c3)(kT)40x31+exdx Units of c (speed of light) is [L][T] where [L] is length in meters and [T] is time in seconds. Units for Planck constant h is [J][T] (Joule-second). Therefore the factor (4πh3c3)(kT)4 above in (3) in front of the integral has units(4πh3c3)(kT)4=1([J][T])3([L][T])3([J][K][K])4=1[J]3[L]3([J])4=[J][L]3

Which has the correct units of energy density. Let this factor be called Φ=(4πh3c3)(kT)4. Then (3) can be written asρ=Φ0x31+exdx

4.2.6.2 Part b

The dimensionless integral found in part (a) is(1)I=0x3ex+1dx But 1ex+1=1ex121e2x1 We did the above, to make the denominator has the form ex1, which is easier to work with following the lecture notes than working with ex+1. Eq (1) now becomes(2)I=0x3ex1dx20x3e2x1dx The first integral has the standard form 0xnex1dx. Hence0x3ex1=(3!)ξ(4) (Derivations of the above is given at the end of this problem). Now we evaluate on the second integral in (2). Let y=2x, then dydx=2. The limits do not change. The integral becomes0y38ey1dy2=1160y3ey1dy We see that 0y3ey1dy now has the same form as the first integral. Hence 0y3ey1dy=(3!)ξ(4). Putting these two results back into (2) gives the final resultI=(3!)ξ(4)2(116(3!)ξ(4))=(3!)ξ(4)(12(116))=(6)ξ(4)(118)=(6)ξ(4)78=214ξ(4)

But from class handout, ξ(4)=π490. Hence0x3ex+1dx=214(π490)=74(π430)=7120π45.6822

Using this in the result obtained in part (a) gives the energy density asρ=Φ0x31+exdx=(7π4120)(4πh3c3)(kT)4

Derivation of the integral

In the above, we used the result that 0xnex1dx=(n!)ξ(n+1). For n=3 this becomes (3!)ξ(4).

To show how this came above, we start by multiplying the numerator and denominator of the integrand by ex. This gives(3)0xnex1exdx Let y=ex thenex1ex=y1y=y(1+y+y2+y3+)=y+y2+y3+=k=1yk=k=1ekx

Using the above sum in Eq (3) gives0xnex1exdx=0xnk=1ekxdx=k=10xnekxdx

Let z=kx. Then dzdx=k. When x=0,z=0 and when x=,z=. The above becomes0xnex1exdx=k=10(zk)nez(dzk)=k=11kn+10znezdz=k=11kn+1(0xnexdx)

But 0xnexdx=n!, which can be shown by integration by parts repeatedly n times. The above integral now becomes0xnex1exdx=(n!)k=11kn+1 The sum k=11kn+1 is called the Zeta function ζ(n+1). When n=3 the above result becomes0x3ex1dx=(3!)k=11k4=(3!)ζ(4)

Which is the result used earlier.

4.2.7 key solution for HW 2

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