دوامات غير مرئية تنحت ثقوبًا سوداء عملاقة سريع

الملخص الأصلي

كما كتبه المؤلفون، بالإنجليزية arXiv:2601.04145v1

We propose a mechanism for the generation of gravitationally bound dark photon halos during the matter-dominated era. Coupled to an ultralight axion field through a parity-violating Chern-Simons term, dark photons can be produced by the tachyonic instability of axion coherent oscillation. The dark photons with a net helicity lead to a metric vorticity and can generate chiral substructures. For axion masses in the range $$10^{-28} \, \mathrm{eV} \lesssim m_a \lesssim 10^{-22} \, \mathrm{eV}$$, the resulting inhomogeneities collapse to form halos with masses spanning $$M_{\rm halo} \sim 10^5 \, M_{\odot}$$ to $$10^{11} \, M_{\odot}$$, with halo sizes ranging from $$O(1)$$ to $$O(10^{6}) \, \mathrm{pc}$$. During halo collapse, the induced vorticity could mediate efficient angular-momentum transport, which enables monolithic collapse and provides primordial seeds for the early formation of supermassive black holes.