Evidence for Non-Baryonic Dark Matter in High Energy Regions above 10 GeV

Sekine, Matsuo (2023) Evidence for Non-Baryonic Dark Matter in High Energy Regions above 10 GeV. In: Fundamental Research and Application of Physical Science Vol. 6. B P International, pp. 35-47. ISBN 978-81-19217-84-7

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Abstract

At an infinite sublayer level, there exists an infinite number of quarks u( ) with the flavors f=u,d,s,c,b and anti-quarks u( ) having all one-half electric charge Q=±1/2. 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 Rp-parity is -1. It is emphasized that supersymmetric particle, neutralino has also the Rp-parity of -1 and well known good cold dark matter candidate. In modern particle physics, all ordinary particles have the Rp-parity of+1, while both the ultimate quarks and u( ) neutralino have the -parity of Rp-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.

Item Type: Book Section
Subjects: Oalibrary Press > Physics and Astronomy
Depositing User: Managing Editor
Date Deposited: 29 Sep 2023 12:51
Last Modified: 29 Sep 2023 12:51
URI: http://asian.go4publish.com/id/eprint/2681

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