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Evidence for Non-Baryonic Dark Matter
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作者 Matsuo Sekine 《Journal of High Energy Physics, Gravitation and Cosmology》 CAS 2022年第3期800-809,共10页
There exists an infinite number of quarks u(∞) and anti-quarks  at an infinite sub-layer level. These particles are considered as the ultimate building blocks of the universe, since they are structure-less and a... There exists an infinite number of quarks u(∞) and anti-quarks  at an infinite sub-layer level. These particles are considered as the ultimate building blocks of the universe, since they are structure-less and absolutely stable. These particles are also regarded as the non-baryonic dark matter, since the baryon number is zero and the R<sub>p</sub>-parity is -1. It is emphasized that supersymmetric particle, neutralino has also the R<sub>p</sub>-parity of -1 and well known good cold dark matter candidate. In modern particle physics, all ordinary particles have the R<sub>p</sub>-parity of +1, while both the ultimate quark u(∞) and neutralino have the R<sub>p</sub>-parity of -1. This means that these particles can only be created or annihilated in pairs in reactions of ordinary particles. From electron-positron annihilation experiments at high energies, it is shown that the prediction value from the ultimate quark u(∞) is in good agreement with many ring-storage collider experiments. 展开更多
关键词 Non-Baryonic Dark Matter Negative Rp-Parity NEUTRALINO electon-positron Experiment
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