Polarized vector oscillons

TL;DR: In this article , it was shown that oscillons also exist in the low-energy effective theory of an interacting massive (real) vector field, and two types of vector oscillons with vanishing orbital angular momentum, and approximately spherically symmetric energy density, but not field configurations.

Abstract: Oscillons are spatially localized, time-periodic, and long-lived configurations that were primarily proposed in scalar field theories with attractive self-interactions. In this paper, we demonstrate that oscillons also exist in the low-energy effective theory of an interacting massive (real) vector field. We provide two types of vector oscillons with vanishing orbital angular momentum, and approximately spherically symmetric energy density, but not field configurations. These are: (1) ``directional'' oscillons (linearly polarized), with vanishing total intrinsic spin, and (2) ``spinning'' oscillons (circularly polarized) with a macroscopic intrinsic spin equal to $\ensuremath{\hbar}\ifmmode\times\else\texttimes\fi{}$ number of particles in the oscillon. In contrast to the case with only gravitational interactions, the two oscillons have different energy at a fixed particle number even in the nonrelativistic limit. By carrying out relativistic $3+1\mathrm{d}$ simulations, we show that these oscillons can be long-lived (compared to the oscillation time for the fields), and can arise from a range of Gaussian initial spatial profiles. These considerations make vector oscillons potentially relevant during the early universe and in dark photon dark matter, with novel phenomenology related to their polarization.