LE13715
- Approximately 25% of the energy density of the universe consists of dark matter. One possible candidate for this dark matter is primordial black holes produced in the first second after the Big Bang. A primordial black hole in the Galaxy's dark-matter halo could pass through our Sun without accreting appreciably, but its
gravitational tidal field would cause the Sun to oscillate like a ringing bell. In this paper, we calculate for the first time the amplitude and frequencies of these solar oscillations. NASA's Solar Dynamics Observatory could detect these oscillations if the mass of the primordial black hole exceeds 10^21 g, the mass of a large
asteroid. Given the inferred local density of dark matter, the event rate for such primordial black holes passing through the Sun is about 10^-7 per year. These oscillations may also be detectable in other stars by reanalyzing the same observations used to search for extrasolar planets.