Dark energy and spontaneous mirror symmetry breaking

Abstract

Dark energy is interpreted as the leftover of mostly canceled vacuum energy due to the spontaneous mirror symmetry breaking (SMSB) at the electroweak phase transition. Based on the newly proposed mirror-matter model (M${}^3$), the extended standard model with mirror matter (SM${}^3$) is elaborated to provide a consistent foundation for understanding dark energy, dark matter, baryogenesis, and many other puzzles. New insights of Higgs, top quark, and lepton masses are presented under SM${}^3$ using staged quark condensation and four-fermion interactions for SMSB. In particular, the nature and mass scales of neutrinos are naturally explained under the new theory. The new cosmology model based on SM${}^3$ could potentially resolve more cosmic enigmas. The possible underlying principles for SMSB and SM${}^3$ of a maximally interacting, supersymmetric, and mirrored world are also discussed.

See arXiv:1902.01837 for dark matter & n-lifetime; arXiv:1904.03835 for baryon asymmetry; arXiv:1906.10262 for CKM unitarity & lab tests; arXiv:1902.03685 for stellar evolution; arXiv:1903.07474 for UHE cosmic rays; arXiv:2006.10746 for invisible decays; https://osf.io/8qawc & arXiv:2003.04687 for SUSY mirror models; https://osf.io/2jywx for black holes; http://sites.nd.edu/wtan/smm/ for updates

References in corpus (8)

• Dynamics of dark energy
• Dark Energy and the Accelerating Universe
• Constraints on symmetry from holography
• Neutron -- Mirror Neutron Oscillation: How Fast Might It Be?
• Neutron oscillations for solving neutron lifetime and dark matter puzzles
• Laboratory tests of the ordinary-mirror particle oscillations and the extended CKM matrix
• Kaon oscillations and baryon asymmetry of the universe
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Cited by in corpus (1)

• Laboratory tests of the ordinary-mirror particle oscillations and the extended CKM matrix