Bulletin of the American Physical Society
APS April Meeting 2019
Volume 64, Number 3
Saturday–Tuesday, April 13–16, 2019; Denver, Colorado
Session Z10: Dark Matter Theory
3:30 PM–5:18 PM,
Tuesday, April 16, 2019
Sheraton
Room: Governor's Square 12
Sponsoring
Unit:
DAP
Chair: Rakshya Khatiwada, Fermilab
Abstract: Z10.00008 : Charged dark matters, missing neutrinos, cosmic rays and extended standard model
4:54 PM–5:06 PM
View Presentation
Abstract
Presenter:
Jae-Kwang Hwang
(JJJ Physics Laboratory)
Author:
Jae-Kwang Hwang
(JJJ Physics Laboratory)
In the present work, the charged B1, B2 and B3 bastons with the condition of k(mm) = k >> k(dd) > k(dm) = k(lq) = 0 are explained as the good candidates of the dark matters. The proposed rest mass (26.12 eV/c2) of the B1 dark matter is indirectly confirmed from the supernova 1987A data. The missing neutrinos are newly explained by using the dark matters and lepton charge force. The neutrino excess anomaly of the MinibooNE data is explained by the B1 dark matter scattering within the Cherenkov detectors. And the rest masses of 1.4 TeV/c2 and 42.7 GeV/c2 are assigned to the Le particle and the B2 dark matter, respectively, from the cosmic ray observations. In the present work, the Q1 baryon decays are used to explain the anti-Helium cosmic ray events. Because of the graviton evaporation and photon confinement, the very small Coulomb’s constant (k(dd)) of 10x-54k and gravitation constant (GN(dd)) of 10xGN for the charged dark matters at the present time are proposed. The x value can have the positive, zero or negative value around zero. Therefore, Fc(mm) > Fg(dd) (?) Fg(mm) > Fg(dm) > Fc(dd) > Fc(dm) = Fc(lq) = 0 for the proton-like particle.
[1] Jae-Kwang Hwang, Mod. Phys. Lett. A32, 1730023 (2017).
[2] Jae-Kwang Hwang, Preprints, 2018120251 (2018).
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