English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

We extend the concept of matter parity $P_M=(-1)^{3(B-L)}$ tonon-supersymmetric theories and argue that $P_M$ is the natural explanation tothe existence of Dark Matter of the Universe. We show that thenon-supersymmetric Dark Matter must be contained in scalar 16 representation(s)of $SO(10),$ thus the unique low energy Dark Matter candidates are $P_M$-oddcomplex scalar singlet(s) $S$ and inert scalar doublet(s) $H_2.$ We havecalculated the thermal relic Dark Matter abundance of the model and shown thatits minimal form may be testable at LHC via the SM Higgs boson decays $H_1\toDM DM.$ The PAMELA anomaly can be explained with the decays $DM\to \nu l W$induced via seesaw-like operator which is additionally suppressed by Planckscale. Because the SM fermions are odd under matter parity too, the DM sectoris just our scalar relative.

Matter parity as the origin of scalar Dark Matter