Calculate the lifetimes of U238andPo212, using Equations8.25and 8.28 . Hint: The density of nuclear matter is relatively constant (i.e., the same for all nuclei), sor13is proportional to (the number of neutrons plus protons). Empirically,

r1=(1.07fm)A1/3

Short Answer

Expert verified

τυ2382.4×1014yrs.τρο2123.2×10-4s.

Step by step solution

01

To write the relatively constant.

The density of nuclear matter relatively constant is,

γ=K1ZE-K2Zr1.

Where,

role="math" localid="1658403215569" K1=1.980MeV1/2K2=1.485fm-1/2

Zis the atomic number.

Eis the energy.

r1is the radius and r11.07fmA1/3.

Accordingly, we can write

γ1.980MeV1/2ZE-1.54ZA1/3

02

To calculate the lifetimes of U238 .

Consider first the uranium-238 nucleus. It has A=238 and Z=92 .

Accordingly, the daughter nucleus has Z=90 (which is the thorium-234).

Hence,

γ1.980MeV1/290E-1.54902381/3γ178.2MeV1/21E-36.37

To calculate E , we need to look up for the masses mp,md,andmin any standard nuclear physics textbook.

We see thatmU238=238.05078826u,mτh234=234.04360123u,andm=4.00262u.

It is convenient to write the masses in u (unified atomic mass unit ) and then multiply the result by 931 to convert the answer into the MeV energy unit .

It follows that,

E=238.05078826-234.04360123-4.002602×931E4.27MeV

Substituting the result into the formula for γyields,

γ=178.2MeV1/214.27MeV-36.37γ49.87

It is left to estimate the speed of the alpha particle (using the relation E=1/2mV2)

v2Emv=2×4.27×1061.6×10-19J6.65×10-27kgv1.43×107m/s

Finally, we calculate the lifetime of U238using Equation,

τ=2×1.07fmA1/3ve2γτ=2×1.07×10-15m×2381/31.43×107m/se2249.88τ=2×6.38×10-151.43×107e249.88sτ=7.46×1021sτ==7.46×10213.15×107yrτ=2.4×1014yrs.

03

To calculate the lifetimes of Po212.

Now consider the polonium-212 nucleus. It has A=212 and Z=84 .

Accordingly, the daughter nucleus has Z=82 (which is the lead Pb-208).

Hence,

γ1.980MeV1/282E-1.54822121/3γ162.36MeV1/21E-34.05

Again, to calculate E, we need to look up for the massess mp,md,andm

We see that

mpo212=211.9988867969u,mτh234=234.04360123u,andm=4.00262u.mU238=238.05078826u,mpb208=207.976666552071u,andm=4.00262u.

It follows that,

E=211.988867969-207.9766552071-4.002602×931E8.95MeV

Substituting the result into the formula for yields,

γ=162.36MeV1/218.95MeV-34.05γ20.22

We calculate the lifetime of po212using Equation

τ=2×1.07fmA1/3ve2γτ=2×1.07×10-15m×2121/32.08×107m/se220.22τ=2×6.38×10-152.08×107e40.44sτ=3.2×10--4s.

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Most popular questions from this chapter

Consider the case of a symmetrical double well, such as the one pictured in Figure. We are interested in Figure 8.13bound states with E<V(0) .
(a) Write down the WKB wave functions in regions (i) x>x2 , (ii) x1<x<x2 , and (iii) 0<x<x1. Impose the appropriate connection formulas at and (this has already been done, in Equation 8.46, for x2 ; you will have to work out x1 for yourself), to show that


ψ(x)={DPxexp-1hx2xpx'dx'2DPxsin1hx2xpx'dx'+π4DPx2cosθ1hvx1pxdx+sinθe1hvx1pxdx

FIGURE 8.13: Symmetrical double well; Problem 8.15.
Where

θ1hx1x2p(x)dx .

(b) Because v(x) is symmetric, we need only consider even (+)and odd (-)wave functions. In the former case ψ(0)=0 , and in the latter case ψ=(0)=0 . Show that this leads to the following quantization condition:

tanθ=±2ef.

Where

f1h-x1x1p(x)dx

Equation 8.59determines the (approximate) allowed energies (note that Ecomes into 1 and x2, so θ and ϕ are both functions of E ).

(c) We are particularly interested in a high and/or broad central barrier, in which case ϕ is large, and eϕis huge. Equation 8.59 then tells us thatA θmust be very close to a half-integer multiple of π . With this in mind, write localid="1658823154085" (θ=n+1/2)π+o . where localid="1658823172105" ||<<1, and show that the quantization condition becomes

localid="1658823190448" θ=(n+12)πm12e-f.

(d) Suppose each well is a parabola: 16

localid="1658823244259" v(x)={12mω2x+a2,ifx<012mω2x-a2,ifx<0 .

Sketch this potential, find (Equation 8.58 ), and show that

localid="1658823297094" En±=(n+12)hωmhω2πe-f

Comment: If the central barrier were impenetrable localid="1658823318311" (f) , we would simply have two detached harmonic oscillators, and the energies, localid="1658823339386" En=(n+1/2)hω , would be doubly degenerate, since the particle could be in the left well or in the right one. When the barrier becomes finite (putting the two wells into "communication"), the degeneracy is lifted. The even (localid="1658823360600" ψn+) states have slightly lower energy, and the odd ones ψn. have slightly higher energy.
(e) Suppose the particle starts out in the right well-or, more precisely, in a state of the form

localid="1658823391675" ψ(x,0)=12(ψn++ψn)

which, assuming the phases are picked in the "natural" way, will be concentrated in the right well. Show that it oscillates back and forth between the wells, with a period

localid="1658823416179" τ=2π2ωe.

(f) Calculate , for the specific potential in part (d), and show that for , localid="1658823448873" V(0).>>E,ϕ~mωa2/h.

Derive the connection formulas at a downward-sloping turning point, and confirm equation8.50.

ψ(x)={D'|p(x)|exp-1hxx1|p(x')|dx'.ifx<x12D'p(x)sin-1hx1xp(x')dx'+π4.ifx<x1

Use the WKB approximation to find the allowed energies of the harmonic oscillator.

Consider a particle of massm in the n th stationary state of the harmonic oscillator (angular frequency ω ).

(a) Find the turning point, x2 .
(b) How far (d) could you go above the turning point before the error in the linearized potential reaches 1%? That is, if V(x2+d)-VIin(x2+d)V(x2)=0.01 what is ?
(c) The asymptotic form of Ai(z) is accurate to 1% as long as localid="1656047781997" z5. For the din part (b), determine the smallest nsuch thatαd5 . (For any n larger than this there exists an overlap region in which the liberalized potential is good to 1% and the large-z form of the Airy function is good to 1% .)

Consider the quantum mechanical analog to the classical problem of a ball (mass m) bouncing elastically on the floor.
(a) What is the potential energy, as a function of height x above the floor? (For negative x, the potential is infinite x - the ball can't get there at all.)
(b) Solve the Schrödinger equation for this potential, expressing your answer in terms of the appropriate Airy function (note that Bi(z) blows up for large z, and must therefore be rejected). Don’t bother to normalize ψ(x).
(c) Using g=9.80m/s2and m=0.100kg , find the first four allowed energies, in joules, correct to three significant digits. Hint: See Milton Abramowitz and Irene A. Stegun, Handbook of Mathematical Functions, Dover, New York (1970), page 478; the notation is defined on page 450.
(d) What is the ground state energy, in ,eV of an electron in this gravitational field? How high off the ground is this electron, on the average? Hint: Use the virial theorem to determine <x> .

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