Question

Certain cold stars (called white dwarfs) are stabilized against gravitational collapse by the degeneracy pressure of their electrons. Assuming constant density, the radius R of such an object can be calculated as follows: (a) Write the total electron energy in terms of the radius, the number of nucleons (protons and newtons) N, the number of electrons per nucleon q, and the mass of the electron m. (b) Look up, or calculate, the gravitational energy of a uniformly dense sphere. Express your answer in terms of G (the constant of universal gravitation), R, N, and M (the mass of a nucleon). Note that the gravitational energy is negative. (c) Find the radius for which the total energy, (a) plus (b), is a minimum. (d) Determine the radius, in kilometers, of a white dwarf with the mass of the sun. (e) Determine the Fermi energy, in electron volts, for the white dwarf in (d), and compare it With the rest energy of an electron.(Note that this system is getting dangerously relativistic.

Solution

Verified
Step 1
1 of 4

a) From equation 5.45 we have (with V=4πR33V=\dfrac{4\pi R^3}{3}):

E=2(3π2Nq)5/310π2m(34πR3)2/3=AR2.\begin{align*} E &= \frac{\hbar^2 (3\pi^2Nq)^{5/3}}{10\pi^2m}\left( \frac{3}{4\pi R^3} \right)^{2/3}\\ &=\frac{A}{R^2}. \end{align*}

b) Gravitational energy needed to build layer of material mass dmdm:

Egrav=Gmrdmm=ρV,V=4πr33m=4πρ3r3dm=4πρr2drEgrav=Gr4πρ3r34πρr2dr=16π2Gρ230Rr4dr=16π2Gρ2R515ρ=NMV=3NM4πR3Egrav=3G5N2M2R=BR.\begin{align*} E_{\text{grav}} &= - \int \frac{Gm}{r}dm\\ m=\rho \cdot V,& \quad V = \frac{4\pi r^3}{3} \\ m&= \frac{4 \pi \rho}{3} r^3 \\ dm &= 4\pi \rho r^2 dr\\ \Rightarrow E_{\text{grav}}&= - \int \frac{G}{r} \frac{4 \pi \rho}{3}r^3 \cdot 4 \pi \rho r^2 dr\\ &= -\frac{16\pi^2G\rho^2}{3} \int_0^R r^4 dr\\ &=-\frac{16\pi^2G\rho^2R^5}{15}\\ \rho &= \frac{NM}{V} = \frac{3NM}{4\pi R^3}\\ \Rightarrow E_{\text{grav}}&= - \frac{3G}{5}\frac{N^2M^2}{R}=-\frac{B}{R}. \end{align*}

Create an account to view solutions

By signing up, you accept Quizlet's Terms of Service and Privacy Policy
Continue with GoogleContinue with Facebook

Create an account to view solutions

By signing up, you accept Quizlet's Terms of Service and Privacy Policy
Continue with GoogleContinue with Facebook

Recommended textbook solutions

Physics for Scientists and Engineers: A Strategic Approach with Modern Physics 4th Edition by Randall D. Knight

Physics for Scientists and Engineers: A Strategic Approach with Modern Physics

4th EditionISBN: 9780133942651 (5 more)Randall D. Knight
3,508 solutions
Introduction to Quantum Mechanics 3rd Edition by Darrell F. Schroeter, David J. Griffiths

Introduction to Quantum Mechanics

3rd EditionISBN: 9781107189638 (3 more)Darrell F. Schroeter, David J. Griffiths
485 solutions
Physics for Scientists and Engineers 9th Edition by John W. Jewett, Raymond A. Serway

Physics for Scientists and Engineers

9th EditionISBN: 9781133947271 (2 more)John W. Jewett, Raymond A. Serway
6,057 solutions
Classical Mechanics 1st Edition by John R. Taylor

Classical Mechanics

1st EditionISBN: 9781891389221 (5 more)John R. Taylor
741 solutions

More related questions

1/4

1/7