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For a long time, protons were thought to be stable—that the laws of physics would not allow for a proton (which is baryonic matter) to spontaneously decay into a positron and photons (non-baryonic matter) because of conservation of the baryon number. However, it has recently been suggested that the predominance of matter over antimatter in the universe is the result of a very slight imbalance in the ratio that occurred very early in its formation. This imbalance would have been exceptionally small, on the order of 1 in every 10,000 particles, but after most of the matter and antimatter annihilated, what was left over was all the baryonic matter in our current universe. This means that in essence, rather than breaking the law of conservation of the baryon number, proton decay is actually the inevitable mechanism for bringing the baryon number back to equilibrium—in a sense correcting the original imbalance that made all current matter in our universe possible.1 Technical Details
Given a vast period of time (protons are theorized to have a half-life of 1036 years), a proton will decay into a positron and a pion that itself immediately decays into photons in the range of gamma radiation
- p → e+π0
This process has yet to be observed experimentally, but is predicted by many Grand Unification Theories (see theory of everything).
Early GUT theories (which were in fact the first sound theory to suggest proton decay) postulated that the proton's half-life would be at least 1031 years. As further experiments and calculations were performed in the 1990s, it became clear that the proton half-life could not lie below that of 1032 years. Many books from that period refer to this figure for the possible decay time for baryonic matter.
Recent experiments at the Super-Kamiokande water Cherenkov radiation detector in JapanJapan (, Nippon/Nihon literally "the origin of the sun") is a country in East Asia situated on a chain of islands east of the Asian continent on the western edge of the Pacific Ocean. The largest of these islands are, from north to south, Hokkaido , Honsh indicate a lower boundary for proton half-life of > 1035 years. The observation of neutrino oscillations also point towards proton decay being a real effect.
Although the phenomenon is referred to as "proton decay", the effect would also be seen in neutronNeutron Classification Subatomic particle Fermion Hadron Baryon Nucleon Neutron Properties Mass: 940 MeV/ c 2 Electric Charge: 0 C Spin: 1/2 In physics, the neutron is a subatomic particle with no net electric charge and a mass of 940 MeV/ c 2 ( kg; verys bound inside atomic nuclei.
2 Further Reading
- Particle Data Group current best estimates of proton lifetime;
- Adams, Fred and Laughlin, Greg The Five Ages of the Universe : Inside the Physics of Eternity BooksEnthsiast.com
Nuclear physics
