Physics: Principles with Applications
Physics: Principles with Applications
6th Edition
ISBN: 9780130606204
Author: Douglas C. Giancoli
Publisher: Prentice Hall
bartleby

Concept explainers

Question
Book Icon
Chapter 31, Problem 35P

(a)

To determine

To show:In the cycle, no carbon is consumed

(a)

Expert Solution
Check Mark

Explanation of Solution

Carbon cycle of massive star

All the reactants and all the products are

  612C+11H713N+γ713N613C+e++v613C+11H714N+γ714N+11H815O+γ815O715N+e++v715N+11H612C+24He

Adding all the reactants and all the products

  612C+11H+713N+613C+11H+714N+11H+815O+715N+11H713N+γ+613C+e++v+714N+γ+815O+γ+715N+e++v+612C+24He

Cancelling those that appear on both sides of the reaction.

  411H24He+2e++2v+3γ

No carbon is consumed in this cycle because one 612C nucleus is required in the first step of the cycle, and one 612C nucleus is produced in the last step of the cycle.

(b)

To determine

To find:The total energy released

(b)

Expert Solution
Check Mark

Answer to Problem 35P

  26.73MeV

Explanation of Solution

Reaction in star

  411H24He+2e++2v+3γ

The number of electrons is balanced well as the number of protons and neutrons. The above "net" equation does not consider the electrons that neutral nuclei would have, because it does not conserve charge.

What the above reaction really represents (ignoring the gammas and neutrinos) is the following:

  411H24He+2e+411p211p+201n+2e+

Each positron-electron annihilation produces another 1.02MeV,

To use the values from Appendix B, we must add 4 electrons to each side of the reaction.

  (411p+4e)(211p+2e+201n)+2e++2e411H24He+2e++2e

The energy produced in the reaction is the Q -value.

  Q=4mH11c2mH24ec24me=[4(1.007825u)4.002603u4(0.000549u)](931.5MeV/c2u)c2=24.69MeV

The total energy released is 24.69MeV+2(1.02MeV)=26.73MeV

(c)

To determine

To find:Energy output for each reaction

(c)

Expert Solution
Check Mark

Explanation of Solution

The first equation: 612C+11H713N+γ

The first equation in the carbon cycle is electron-balanced,

The Q-value

  Q=m612Cc+mH11c2mN713c2=[12.000000u+1.007825u13.005739u](931.5MeV/c2u)c2=1.943MeV

The second equation: 713N613C+e++v

The second equation needs to have another electron, so that 713N613C+e+e++v

  Q=m713Nc2mc61322mec2=[13.005739u13.003355u2(0.000549u)](931.5MeV/c2u)c2=1.198MeV

We must include an electron-positron annihilation in this reaction. 1.198MeV+1.02MeV=2.218MeV

The third equation: 613C+11H714N+γ

The third equation of the carbon cycle is electron-balanced. Q=mc613c2+mH11c2mN114c2=[13.003355u+1.007825u14.003074u](931.5MeV/c2u)c2=7.551MeV

The fourth equation: 714N+11H815O+γ

The fourth equation of the carbon cycle is also electron-balanced.

  Q=mN714c2+mH11c2mO815c2=[14.003074u+1.007825u15.003066u](931.5MeV/c2u)c2=7.296MeV

The fifth equation: 815O715N+e++v

The fifth equation needs to have another electron, so 815O715N+e+e++v

  Q=m158O2m15N22mec2=[15.003066u15.000109u2(0.000549u)](931.5MeV/c2u)c2=1.732MeV

We must include an electron-positron annihilation in this reaction.

  1.732MeV+1.02MeV=2.752MeV .

The sixth equation: 715N+11H612C+24He

The sixth equation is electron-balanced.

  Q=mN715c2+mH11c2mC612c2mH24ec2=[15.000109u+1.007825u12.000000u4.002603u](931.5MeV/c2u)c2=4.966MeV

The total energy released is found by summing the energy released in each process.

  1.943MeV+2.218MeV+7.551MeV+7.296MeV+2.752MeV+4.966MeV=26.73MeV.

(d)

To determine

To find:The reason carbon cycle require higher temperature than proton-proton cycle

(d)

Expert Solution
Check Mark

Explanation of Solution

The carbon and nitrogen nuclei have higher Z values, leading to a greater Coulomb repulsion.To overcome the Coulomb repulsion between the nuclei, the carbon cycle need higher temperature so that the reactants have more initial kinetic energy.

Since, carbon has higher Coulomb repulsion than proton. So the temperature should be higher for carbon cycle reaction.

Chapter 31 Solutions

Physics: Principles with Applications

Knowledge Booster
Background pattern image
Physics
Learn more about
Need a deep-dive on the concept behind this application? Look no further. Learn more about this topic, physics and related others by exploring similar questions and additional content below.
Recommended textbooks for you
Text book image
College Physics
Physics
ISBN:9781305952300
Author:Raymond A. Serway, Chris Vuille
Publisher:Cengage Learning
Text book image
University Physics (14th Edition)
Physics
ISBN:9780133969290
Author:Hugh D. Young, Roger A. Freedman
Publisher:PEARSON
Text book image
Introduction To Quantum Mechanics
Physics
ISBN:9781107189638
Author:Griffiths, David J., Schroeter, Darrell F.
Publisher:Cambridge University Press
Text book image
Physics for Scientists and Engineers
Physics
ISBN:9781337553278
Author:Raymond A. Serway, John W. Jewett
Publisher:Cengage Learning
Text book image
Lecture- Tutorials for Introductory Astronomy
Physics
ISBN:9780321820464
Author:Edward E. Prather, Tim P. Slater, Jeff P. Adams, Gina Brissenden
Publisher:Addison-Wesley
Text book image
College Physics: A Strategic Approach (4th Editio...
Physics
ISBN:9780134609034
Author:Randall D. Knight (Professor Emeritus), Brian Jones, Stuart Field
Publisher:PEARSON