Solved Assignment for Stellar Structure and Evolution | PHYS 132, Assignments of Physics

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

Typology: Assignments

Pre 2010

Uploaded on 08/31/2009

koofers-user-kch
koofers-user-kch 🇺🇸

10 documents

1 / 1

Toggle sidebar

This page cannot be seen from the preview

Don't miss anything!

bg1
Phys 132 Homework 18 Solutions
Professor Crystal Martin
TA: Ellie Hadjiyska
Problem 18: (Phillips Problem 4.6)
The power per unit volume produced by the triple-αreaction is
"3α=(3m4m12)c2dn12
dt ,
where
dn12
dt =33/2n3
4
τ(1212) !h
2πm4kT "3
e(m
123m4)/kT
is the number density of carbon atoms produced per unit time. The individual symbols are as
defined in the textbook. The power per unit volume at T=2×108Kand10
8kg m3is 2.2×
1018 Wm3. Changing the temperature only changes T3in the denominator and the exponent in
the rate equation. Decreasing the temperature to 108K decreases T3by a factor of 8 (and the rate
by a factor of 8) and the exponential factor changes from e22 to e44. The resulting power per
unit volume is
"3α(T=10
8K)=8
e44
e22 "3α(T=2×108K)4.9×109Wm
3.
Decreasing the temperature by a factor of two sharply decreases the energy generation rate of the
reaction.
Altering the energy of the excited carbon is equivalent to changing the mass of the excited
state m
12, which only affects the exponential factor in the rate equation. At 108K, kT 10 KeV
and changing the excited state mass from 7.65 MeV to 7.66 MeV lowers the exponent by a factor
of 2.7. Therefore the overall power generated is lowered by a factor of 2.7 as well. A tiny change
in the excited state mass has a drastic effect on the production of carbon.

Partial preview of the text

Download Solved Assignment for Stellar Structure and Evolution | PHYS 132 and more Assignments Physics in PDF only on Docsity!

Phys 132 Homework 18 Solutions

Professor Crystal Martin TA: Ellie Hadjiyska

Problem 18: (Phillips Problem 4.6) The power per unit volume produced by the triple-α reaction is

" 3 α = (3m 4 − m 12 )c 2

dn (^12) dt ,

where dn (^12) dt

3 / (^2) n (^34) τ (12∗^ → 12)

h 2 πm 4 kT

e−(m∗^12 −^3 m^4 )/kT

is the number density of carbon atoms produced per unit time. The individual symbols are as defined in the textbook. The power per unit volume at T = 2 × 108 K and 10^8 kg m −^3 is 2. 2 × 1018 W m−^3. Changing the temperature only changes T 3 in the denominator and the exponent in the rate equation. Decreasing the temperature to 10 8 K decreases T 3 by a factor of 8 (and the rate by a factor of 8) and the exponential factor changes from e−^22 to e−^44. The resulting power per unit volume is

" 3 α (T = 10^8 K) = 8

e−^44 e−^22 "^3 α^ (T^ = 2^ ×^10

(^8) K) ≈ 4. 9 × 109 W m − (^3).

Decreasing the temperature by a factor of two sharply decreases the energy generation rate of the reaction.

Altering the energy of the excited carbon is equivalent to changing the mass of the excited state m∗ 12 , which only affects the exponential factor in the rate equation. At 10^8 K, kT ≈ 10 KeV and changing the excited state mass from 7.65 MeV to 7.66 MeV lowers the exponent by a factor of ∼ 2 .7. Therefore the overall power generated is lowered by a factor of 2.7 as well. A tiny change in the excited state mass has a drastic effect on the production of carbon.