Abstract
The familiar consequences of charge-independence of a nuclear Hamiltonian are derived without introducing the concept of charge space and the extended Pauli principle. Ordinary wave-functions, separately antisymmetric in their protons and neutrons, are used throughout. This has the pedagogical advantage of emphasizing that the physical regularities associated with isobaric spin are consequences of charge-independence alone, and do not depend upon the charge-space formalism.
Original language | English (US) |
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Pages (from-to) | 216-222 |
Number of pages | 7 |
Journal | American Journal of Physics |
Volume | 34 |
Issue number | 3 |
DOIs | |
State | Published - Mar 1966 |
Externally published | Yes |