Dark energy and spontaneous mirror symmetry breaking
arXiv:1908.11838
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), the extended standard model with mirror matter (SM) 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 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 could potentially resolve more cosmic enigmas. The possible underlying principles for SMSB and SM of a maximally interacting, supersymmetric, and mirrored world are also discussed.
arXiv commentSee 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 (16)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Dynamics of dark energy
- Dark Energy and the Accelerating Universe
- Planck 2018 results. I. Overview and the cosmological legacy of Planck
- Observational Probes of Cosmic Acceleration
- The Twin Higgs: Natural Electroweak Breaking from Mirror Symmetry
- From controversy to precision on the sigma meson: a review on the status of the non-ordinary resonance
- Constraints on symmetry from holography
- Neutron -- Mirror Neutron Oscillation: How Fast Might It Be?
- Neutron - Mirror Neutron Oscillations: How Fast Might They Be?
- Spontaneous Mirror Parity Violation, Common Origin of Matter and Dark Matter, and the LHC Signatures
- 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
- Neutron-mirror neutron oscillations in stars