An Introduction to Modern Astrophysics · Problem 10.14
The Sun — Carroll & Ostlie
Physics — Astrophysics · nuclear-reaction-sequences
Problem
Complete the following reaction sequences. Be sure to include any necessary leptons. (a) (b) (c)Intuitive explanation
Nuclear reactions must conserve both mass number (total nucleons) and atomic number (total protons). When a nucleus transforms or collides, track what's missing by comparing the totals on each side—that missing piece is your answer. Pay special attention to beta-plus decay, which emits a positron and always requires a ghostly partner to balance the books.
Intuitive explanation
Nuclear reactions must conserve both mass number (total nucleons) and atomic number (total protons). When a nucleus transforms or collides, track what's missing by comparing the totals on each side—that missing piece is your answer. Pay special attention to beta-plus decay, which emits a positron and always requires a ghostly partner to balance the books.