EBK PHYSICS FOR SCIENTISTS & ENGINEERS
EBK PHYSICS FOR SCIENTISTS & ENGINEERS
5th Edition
ISBN: 9780134296074
Author: GIANCOLI
Publisher: VST
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Chapter 42, Problem 2P
To determine

Whether the reaction requires threshold energy or not.

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15. A star initially has 1040 deuterons. It produces energy via the 3 4 processes, H² +₁H² →→ ₁H³ + p and, H² + ₁H³ → ₂Heª + n. 1 the If the average power radiated by the star is 10¹6 W, deuteron supply of the star is exhausted in a time of the order of (a) 106 S (c) 10 ¹² s (b) 108 s (d) 10¹6 s The mass of the nuclei are as follows M(H²) = 2.014 amu; M(n) = 1.008 amu; M(p) = 1.007 amu; M(He* )= 4.001 amu. 4
Calculate the threshold energy for the following reactings: (i) n+Th²³2 → Th²³1 + 2n (ii)n+Th232 → Th²33 + y
6. Find the threshold kinetic energy for the following reactions: (a) p+p→→n+E+Kº+a* (b) p+n→p+E+K*
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