Solution of the strong CP problem in baby-universe theory

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General Properties Of Qcd, Charge Conjugation, Parity, Time Reversal, And Other Discrete Symmetries

Scientific paper

The strong CP problem is solved by use of quantum gravity. It is argued that the coherent-state parameters αi describing the effect of wormholes (baby universes) adjust themselves so as to make the strong interactions CP invariant. There remains though a small CP breaking so that θ¯ is not exactly zero. The main prediction is that we do not need the axion proposed by Peccei and Quinn.

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