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A 8.59-MeV alpha particle (mass \(=3.7274 \mathrm{GeV} / \mathrm{c}^{2}\) ) inside a heavy nucleus encounters a barrier whose average height is \(15.9 \mathrm{MeV}\). The tunneling probability is measured to be \(1.042 \cdot 10^{-18} .\) What is the width of the barrier? (Hint: A potentially useful value is \(\hbar c=197.327 \mathrm{MeV} \mathrm{fm} .)\)

Short Answer

Expert verified
Answer: The width of the potential barrier is approximately 57.12 fm (femtometer).

Step by step solution

01

Known and unknown values

First, let's list down all the given values: - Energy of the alpha particle (E): 8.59 MeV - Mass of the alpha particle (m): 3.7274 GeV/c^2 - Height of the barrier (V_0): 15.9 MeV - Tunneling probability (T): 1.042 × 10^(-18) Additionally, we have the value of ħc (Planck's constant, h, divided by 2π, times the speed of light): 197.327 MeV·fm. We need to find the width of the barrier (d).
02

Determine k and K values

We will use the following equations to determine the values of k and K representing the wave numbers of regions inside and outside the potential barrier, respectively: k = sqrt(2mE/ħ^2) K = sqrt(2m(V_0 - E)/ħ^2)
03

Conversion of units

Before proceeding with calculations, let's convert the mass and energies into their respective units: E = 8.59 MeV × (1 GeV / 1000 MeV) = 8.59 × 10^(-3) GeV m = 3.7274 GeV/c^2 Now, let's compute k and K: k = sqrt(2 × 3.7274 × 8.59 × 10^(-3) / (197.327 fm)^2) k ≈ 0.053823 fm^(-1) K = sqrt(2 × 3.7274 × (15.9 - 8.59) × 10^(-3) / (197.327 fm)^2) K ≈ 0.079496 fm^(-1)
04

Calculate the width of the barrier

Now, we will use the tunneling probability (T) and the wave number values (k and K) to determine the width of the barrier (d): T = e^(-2Kd) From this, we can identify d: d = (1/(-2K)) × ln(T) d ≈ (1/(-2 × 0.079496)) × ln(1.042 × 10^(-18)) d ≈ 57.12 fm Therefore, the width of the barrier is approximately 57.12 fm (femtometer).

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Most popular questions from this chapter

Consider a square potential, \(U(x)=0\) for \(x<-\alpha, U(x)=-U_{0}\) for \(-\alpha \leq x \leq \alpha,\) where \(U_{0}\) is a positive constant, and \(U(x)=0\) for \(x>\alpha .\) For \(E>0,\) the solutions of the time-independent Schrödinger equation in the three regions will be the following: For \(x<-\alpha, \psi(x)=e^{i \kappa x}+R e^{-i \kappa x},\) where \(\kappa^{2}=2 m E / \hbar^{2}\) and \(R\) is the amplitude of a reflected wave. For \(-\alpha \leq x \leq \alpha, \psi(x)=A e^{i \kappa^{\prime} x}+B e^{-i \kappa^{\prime} x},\) and \(\left(\kappa^{\prime}\right)^{2}=2 m\left(E+U_{0}\right) / \hbar^{2}\) For \(x>\alpha, \psi(x)=T e^{i \kappa x}\) where \(T\) is the amplitude of the transmitted wave. Match \(\psi(x)\) and \(d \psi(x) / d x\) at \(-\alpha\) and \(\alpha\) and find an expression for \(R\). What is the condition for which \(R=0\) (that is, there is no reflected wave)?

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