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PRIMORDIAL BLACKHOLE AS A SEED FOR THE COSMIC MAGNETIC FIELD KCI 등재 SCOPUS

  • 언어ENG
  • URLhttps://db.koreascholar.com/Article/Detail/387459
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천문학회지 (Journal of The Korean Astronomical Society)
한국천문학회 (Korean Astronomical Society)
초록

We present a model that rotating primordial blackholes(PBHs) produced at the end of inflation generate the random, non-oriented primordial magnetic field. PBHs are copiously produced as the Universe completes the cosmic phase transition via bubble nucleation and tunneling processes in the extended inflation hypothesis. The PBHs produced acquire angular momentum through the mutual tidal gravitational interaction. For PBHs of mass less than 1013g, one can show that the evaporation (photon) luminosity of PBHs exceeds the Eddington limit. Thus throughout the lifetime of the rotating PBH, radiation flow from the central blackhole along the Kerr-geodesic exerts torque to ambient plasma. In the process similar to the Bierman's battery mechanism electron current reaching up to the horizon scale is induced. For PBHs of Grand Unified Theories extended inflation with the symmetry breaking temperature of TGUT ~1010 GeV, which evaporate near decoupling, we find that they generate random, non-oriented magnetic fields of ~10-11G on the last-scattering surface on (the present comoving) scales of ~O(10)Mpc.

저자
  • LA DAIL(Department of Earth Science, Sejong University)
  • PARK CHANGBOM(Department of Astronomy, Seoul National University)