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Blandford-Znajek process as Alfvénic superradiance

Sousuke NodaCenter for Gravitation and Cosmology, College of Physical Science and Technology, Yangzhou University, Yangzhou 225009, ChinaYasusada NambuDepartment of Physics, Graduate School of Science, Nagoya University, Chikusa, Nagoya 464-8602, JapanTakuma TsukamotoDepartment of Physics, Graduate School of Science, Nagoya University, Chikusa, Nagoya 464-8602, JapanMasaaki TakahashiDepartment of Physics and Astronomy, Aichi University of Education, Kariya, Aichi 448-8542, Japan
2020en
ABI

Аннотация

The superradiant scattering of Alfv\'en waves (Alfv\'enic superradiance) in a forcefree magnetosphere is discussed to reveal the relationship between the Blandford-Znajek (BZ) process and superradiance. For simplicity, we consider a four-dimensional rotating black string spacetime of which each $z=\text{const}$ slice is a Ba\~nados-Teitelboim-Zanelli solution as an analogy of the equatorial plane of the Kerr spacetime. Then, it is confirmed that the condition for Alfv\'enic superradiance coincides with that for the BZ process, and the wave amplification can be very large due to a resonant scattering for some parameter sets of the wave frequency and the angular velocity of the magnetic field line. Moreover, by analysis of the Poynting flux, we first show that the BZ process can be interpreted as the long wavelength limit of Alfv\'enic superradiance.

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