Abstract

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 eV≲ma≲10−22 eV10^{-28} \, \mathrm{eV} \lesssim m_a \lesssim 10^{-22} \, \mathrm{eV}, the resulting inhomogeneities collapse to form halos with masses spanning Mhalo∼105 M⊙M_{\rm halo} \sim 10^5 \, M_{\odot} to 1011 M⊙10^{11} \, M_{\odot}, with halo sizes ranging from O(1)O(1) to O(106) pcO(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.

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