Calculate (in MeV) the total binding energy and the binding energy per nucleon for H3and for He3.

Short Answer

Expert verified

For H3atom, Binding energy = 8.48MeV

Binding energy per nucleon = 2.83MeV

For He3atom, Binding energy = 7.78MeV

Binding energy per nucleon = 2.594MeV

Step by step solution

01

 Step1: Given information.

We have been given that,

H3,He3

We need to find the binding energy and binding energy per nucleon for both atoms.

02

 Step2: Calculation for binding energy and binding energy per nucleon of H3

Binding energy is given by,

BE=ZmE+NmN-mA

Where,

Z= atomic number ,N= number of neutrons ,mA=mass of atom,

mN=mass of neutron , mE=mass of element.

For H3atom, BE=1×1.00783u+2×1.00866u-3.01605u×931.49MeV/u=(3.02515-3.01605)×931.49MeV/u=8.48MeV

Binding energy per nucleon = BEAMeV

Therefore,

For H3, BE=8.48MeV,A=3

Binding energy per nucleon = 8.483MeV

= 2.83MeV

03

Calculation for binding energy and binding energy per nucleon of He3.

Binding energy is given by,

BE=ZmE+NmN-mAMeV

For He3,

Z=1,N=2,A=3

BE=1×1.00783u+2×1.783u-3.01605u931.49MeV/u=3.02515-3.0164931.49MeV=7.78MeV

Now,

Binding energy per nucleon is = BEAMeV

= 7.783MeV A=3

= 2.594MeV

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 Vaia!

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

The technique known as potassium-argon dating is used to date old lava flows. The potassium isotope 40 K has a 1.28-billionyear half-life and is naturally present at very low levels. 40 K decays by two routes: 89% undergo beta-minus decay into 40 Ca while 11% undergo electron capture to become 40 Ar. Argon is a gas, and there is no argon in flowing lava because the gas escapes. Once the lava solidifies, any argon produced in the decay of 40 K is trapped inside and cannot escape. A geologist brings you a piece of solidified lava in which you find the 40 Ar/ 40 K ratio to be 0.013. What is the age of the rock?

137 Cs is a common product of nuclear fission. Suppose an accident spills 550 mCi of 137 Cs in a lab room.

a. What mass of 137 Cs is spilled?

b. If the spill is not cleaned up, how long will it take until the radiation level drops to an acceptable level, for a room this size, of 25 mCi?

Stars are powered by nuclear reactions that fuse hydrogen into helium. The fate of many stars, once most of the hydrogen is used up, is to collapse, under gravitational pull, into a neutron star. The force of gravity becomes so large that protons and electrons are fused into neutrons in the reaction p++en+ν. The entire star is then a tightly packed ball of neutrons with the density of nuclear matter.

a. Suppose the sun collapses into a neutron star. What will its radius be? Give your answer in km.

b. The sun's rotation period is now 27 days. What will its rotation period be after it collapses?

Rapidly rotating neutron stars emit pulses of radio waves at the rotation frequency and are known as pulsars.

Calculate the mass, radius, and density of the nucleus of (a)Li7and(b)207Pb.

Give all answers in SI units.

a. Draw energy-level diagrams, similar to Figure 42.11, for all A=14nuclei listed in Appendix C. Show all the occupied neutron and proton levels.

b. Which of these nuclei is stable? What is the decay mode of any that are radioactive?

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.

Sign-up for free