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A quest for weak objects and for invisible stars
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A quest for weak objects and for invisible stars
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High quality spectra to be produced by SUBARU 8 meter telescope will be extremely valuable for numerous astronomical projects. Here I concentrate on two classical types of weak broad line objects -- distant supernovae and white dwarfs -- with emphasis of their importance for fundamental physics, not only for astronomy. With regard to recent results of MACHO experiment and HST weak star counts I discuss one exotic possibility: invisible stars made of the so called ``mirror'' matter.
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Cited by 1 Pith paper
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Overdamping of Neutron-Mirror-Neutron Transitions in Neutron Stars
Collisional decoherence overdamps n–n′ transitions in neutron stars, yielding Γ ≈ 4ε²/M ≪ oscillation rates and a mirror admixture suppressed by ~4ε²/M² at all times.
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