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