The paper derives a dark energy density of roughly (10^-3 eV)^4 from a mirror-symmetric model with a 10^-14 breaking scale, matching observation, but the derivation rests on a nonstandard vacuum-energy superposition assumption.
Invisible decays of neutral hadrons
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abstract
Invisible decays of neutral hadrons are evaluated as ordinary-mirror particle oscillations using the newly developed mirror matter model. Assuming equivalence of the $CP$ violation and mirror symmetry breaking scales for neutral kaon oscillations, rather precise values of the mirror matter model parameters are predicted for such ordinary-mirror particle oscillations. Not only do these parameter values satisfy the cosmological constraints, but they can also be used to precisely determine the oscillation or invisible decay rates of neutral hadrons. In particular, invisible decay branching fractions for relatively long-lived hadrons such as $K^0_L$, $K^0_S$, $\Lambda^0$, and $\Xi^0$ due to such oscillations are calculated to be $9.9\times 10^{-6}$, $1.8\times 10^{-6}$, $4.4\times 10^{-7}$, and $3.6\times 10^{-8}$, respectively. These significant invisible decays are readily detectable at existing accelerator facilities.
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physics.gen-ph 1years
2019 1verdicts
REJECT 1roles
background 1polarities
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Dark energy and spontaneous mirror symmetry breaking
The paper derives a dark energy density of roughly (10^-3 eV)^4 from a mirror-symmetric model with a 10^-14 breaking scale, matching observation, but the derivation rests on a nonstandard vacuum-energy superposition assumption.