/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Q13P Question: Assume that immediatel... [FREE SOLUTION] | 91Ó°ÊÓ

91Ó°ÊÓ

Question: Assume that immediately after the fission of U236according to Eq. 43-1, the resulting Xe140andSr94nuclei are just touching at their surfaces. (a) Assuming the nuclei to be spherical, calculate the electric potential energy associated with the repulsion between the two fragments. (Hint: Use Eq. 42-3 to calculate the radii of the fragments.) (b) Compare this energy with the energy released in a typical fission event.

Short Answer

Expert verified

(a) The potential electrical energy is 251 MeV.

(b) The electrical potential energy is greater than typical fission energy.

Step by step solution

01

Given data

The mass number of Xenon,AXe=140

The mass number of Strontium, ASr=94

The mass number of Uranium,AU=236

02

Determine the formulas to calculate the electric potential energy

The expression to calculate the radii of the fragment is given as follows.

r=r0A1/3 ...(i)

Here, A is the mass number.

The expression to calculate the electrical potential energy is given as follows.

W=14πε0q1q2r ...(ii)

Here, q1.q2are the charges and r is the distance between the charges.

03

(a) Calculate the electrical potential energy.

The atomic number of Strontium,ZSr=38

The atomic number of Xenon,ZXe=54

Calculate the radii of the Xenon,

Substitute 1.2 fm for r0and 140 for A into equation (i).

rXe=1.2fm×1401/3rXe=1.2fm×5.1924rXe=6.2fm

Calculate the radii of the strontium,

Substitute 1.2 fm forr0and 94 for A into equation (i).

rSr=1.2fm×941/3rSr=1.2fm×4.546rSr=5.48fm

Calculate the electrical potential energy.

SubstituteZXefor q1,ZSrfor q2,rSr+rXefor r into above equation (i).

W=14π×ε0×ZXeZSrrXe+rSr

Substitute 6.24 for rXe, 5.48 for rSr, 54e forZXeand 38e forZXeinto above equation.

localid="1661927633337" W=14π×8.85×10−12C2/Nm2×54e×38e(6.24+5.48)×10−15mW=8.99×109Nm2C2×2052e211.72×10−15m

Substitute1.6×10−19Cfor e into above equation.

W=8.99×109Nm2C2×20521.6×10−19C211.72×10−15mW=18447.48×2.56×1024×10−38J11.72W=47225.54×10−14J11.72W=4029×10−11J

Convert the energy into MeV,

W=4.033×10−111.602×10−19eVW=2.515×108eVW=251.5MeV

By rounding down the value of the energy is 251 MeV.

Hence the potential electrical energy is 251 MeV.

04

(b) Compare the electrical potential energy with typical fission energy.

The energy released in the typical fission energy is 200 MeV and the electrical potential energy from the part (a) is 251 MeV . By comparing the two energies, it is clear that the electrical potential energy is greater than the typical fission energy. This energy appears in the form of kinetic, beat and sound energy.

Hence the electrical potential energy is greater than typical fission energy.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with 91Ó°ÊÓ!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

Verify the Q values reported in Eqs. 43-13, 43-14, and 43-15. The needed masses are

H11.007825uHe44.002603uH22.014102un1.008665uH33.016049u

Assume that the core of the Sun has one-eighth of the Sun’s mass and is compressed within a sphere whose radius is one-fourth of the solar radius. Assume further that the composition of the core is 35% hydrogen by mass and that essentially all the Sun’s energy is generated there. If the Sun continues to burn hydrogen at the current rate of 6.2×1011kg/s, how long will it be before the hydrogen is entirely consumed? The Sun’s mass is 2.0×1030kg.

We have seen that Qfor the overall proton–proton fusion cycle is 26.7 MeV. How can you relate this number to the Qvalues for the reactions that make up this cycle, as displayed in Fig. 43-11?

(a) Calculate the disintegration energy Q for the fission of the molybdenum isotope M98ointo two equal parts. The masses you will need are 97.90541u forM98o and 48.95002u for S49c. (b) If Q turns out to be positive, discuss why this process does not occur spontaneously.

The neutron generation time (see Problem 19) of a particular reactor is 1.3 ms .The reactor is generating energy at the rate of 1200.0 MW.To perform certain maintenance checks, the power level must temporarily be reduced to 350.00 MW. It is desired that the transition to the reduced power level take 2.6000 s. To what (constant) value should the multiplication factor be set to effect the transition in the desired time?

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.