Homework 19 Solutions - Stellar Structure | PHYS 132, Assignments of Physics

Material Type: Assignment; Professor: Martin; Class: STELLAR STRCTR/EVOL; Subject: Physics; University: University of California - Santa Barbara; Term: Spring 2008;

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Phys 132 Homework 19 Solutions
Professor Crystal Martin
TA: Ellie Hadjiyska
Problem 19 : (Phillips Problem 2.4) We are given a stellar atmosphere that is almost pure
hydrogen with 50% of the hydrogen molecules dissociated into hydrogen atoms and the pressure
P= 100 Pa. We want to find the temperature.
We will treat the hydrogen as being in one of two states: undissociated with energy ²10 and
dissociated with energy ²24.48 eV.
Since 50% dissociated, the number of undissociated H2molecules equals the number of H2molecules
that did dissociate. We get 2 H atoms for every H2molecule that dissociates, so n(H) = 2n(H2)
(Note: This is not the same as what was quoted in the hint). Thermodynamic equilibrium is
established if the sums of the chemical potentials on both sides are equal. Since photons have zero
chemical potential and
γ+H2H+H
then
µ(H2) = µ(H) + µ(H) = 2µ(H) (1)
where
µ(H2) = m(H2)c2kT ln µg(H2)nQ(H2)
n(H2)(2)
and
µ(H) = m(H)c2kT ln µg(H)nQ(H)
n(H)(3)
The mass of the hydrogen molecule is equal to the mass of the atoms making it up plus the binding
energy ²2=4.48 eV. i.e.
m(H2)c2= 2m(H)c2+²2
Using this with Eqs. (??), (??), and (??) gives
²2=m(H2)c22m(H)c2=kT ln "g(H2)nQ(H2)
n(H2)µn(H)
g(H)nQ(H)2#(4)
or setting the statistical weights g(H2) = g(H) = 1, we get
exp (²2/kT ) = n(H)
nQ(H)µnQ(H2)
nQ(H)µn(H)
n(H2)
pf2

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Phys 132 Homework 19 Solutions

Professor Crystal Martin TA: Ellie Hadjiyska

Problem 19 : (Phillips Problem 2.4) We are given a stellar atmosphere that is almost pure hydrogen with 50% of the hydrogen molecules dissociated into hydrogen atoms and the pressure P = 100 Pa. We want to find the temperature.

We will treat the hydrogen as being in one of two states: undissociated with energy ≤ 1 ∼ 0 and dissociated with energy ≤ 2 ≈ 4 .48 eV.

Since 50% dissociated, the number of undissociated H 2 molecules equals the number of H 2 molecules that did dissociate. We get 2 H atoms for every H 2 molecule that dissociates, so n(H) = 2n(H 2 ) (Note: This is not the same as what was quoted in the hint). Thermodynamic equilibrium is established if the sums of the chemical potentials on both sides are equal. Since photons have zero chemical potential and γ + H 2 ≠ H + H

then

μ(H 2 ) = μ(H) + μ(H) = 2μ(H) (1)

where

μ(H 2 ) = m(H 2 )c^2 − kT ln

( (^) g(H 2 )nQ(H 2 ) n(H 2 )

and

μ(H) = m(H)c^2 − kT ln

( (^) g(H)n Q(H) n(H)

The mass of the hydrogen molecule is equal to the mass of the atoms making it up plus the binding energy ≤ 2 = − 4 .48 eV. i.e. m(H 2 )c^2 = 2m(H)c^2 + ≤ 2

Using this with Eqs. (??), (??), and (??) gives

≤ 2 = m(H 2 )c^2 − 2 m(H)c^2 = kT ln

[

g(H 2 )nQ(H 2 ) n(H 2 )

n(H) g(H)nQ(H)

) 2 ]

or setting the statistical weights g(H 2 ) = g(H) = 1, we get

exp (≤ 2 /kT ) = n(H) nQ(H)

( (^) n Q(H 2 ) nQ(H)

n(H) n(H 2 )

We have already shown that the last factor n(H)/n(H 2 ) = 2 on the right hand side. The middle factor is the ratio of the quantum concentrations. Since the quantum concentration is given by (Phillips Eq. (2.22)

nQ =

[

2 πmkT h^2

] 3 / 2

or nQ ∝ m^3 /^2 , the middle factor is just the ratio of the corresponding masses to the 3/2 power:

exp (≤ 2 /kT ) = 2

n(H) nQ(H)

m(H 2 ) m(H)

= 2^5 /^2

n(H) nQ(H)^ (5)

Using n(H) = 2n(H 2 ), the total number of particles in the gas n is given by

n = n(H) + n(H 2 ) = 3n(H 2 ) =

2 n(H)

Putting this into the ideal gas law gives

P =^3 2

n(H)kT

or n(H) =

2 P

3 kT Plugging this into Eq. (??) along with the quantum concentration gives

exp (≤ 2 /kT ) = 2^5 /^2 32 kTP

h^2 2 πmH kT

If we let x ≡ 4 .48 eV kT , then we get the transcendental equation

x−^5 /^2 e−x^ = 2. 35 × 10 −^13

which can be solved numerically using Mathematica or other similar program. We get

x =

4 .48 eV kT = 21.^4

or kT = 0.21 eV which corresponds to a temperature of T ≈ 2400 K.