Polarization maps of direct images from scalar-hairy Kerr black holes exhibit dephasing in the polarization-vector twist (larger for weakly scalarized cases) and a reversal for vertical magnetic fields at high inclinations.
Agol, Sagittarius a* polarization: No advection-dominated accretion flow, low accretion rate, and nonthermal synchrotron emission, The Astrophysical Journal538, L121 (2000)
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
gr-qc 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Polarized Equatorial Emission around Kerr Black Holes with Synchronized Scalar Hair. I. Direct images
Polarization maps of direct images from scalar-hairy Kerr black holes exhibit dephasing in the polarization-vector twist (larger for weakly scalarized cases) and a reversal for vertical magnetic fields at high inclinations.