Updated constraints on self-interacting dark matter from Supernova 1987A

Cameron Mahoney; Adam K. Leibovich; Andrew R. Zentner

doi:10.1103/physrevd.96.043018

Updated constraints on self-interacting dark matter from Supernova 1987A

Physical Review D ◽

10.1103/physrevd.96.043018 ◽

2017 ◽

Vol 96 (4) ◽

Cited By ~ 7

Author(s):

Cameron Mahoney ◽

Adam K. Leibovich ◽

Andrew R. Zentner

Keyword(s):

Dark Matter ◽

Supernova 1987A

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Charged Dark Matters, Missing Neutrinos, Cosmic Rays and Extended Standard Model

10.20944/preprints201812.0251.v1 ◽

2018 ◽

Author(s):

Jae-Kwang Hwang

Keyword(s):

Dark Matter ◽

Rest Mass ◽

Cosmic Ray ◽

Positive Zero ◽

Cherenkov Detectors ◽

Supernova 1987A ◽

Lepton Charge ◽

Dark Matters ◽

Photon Confinement ◽

Dark Matter Scattering

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.

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