Fermions alter the spacetime around cosmic strings in dynamical Chern–Simons gravity
This paper studies how certain kinds of fermions change the gravitational field of cosmic strings when gravity is extended to include a parity-violating term called dynamical Chern–Simons (dCS) gravity. In plain terms, the authors show that when a particle physics model that produces a dCS coupling is combined with the special currents that can live on a cosmic string, the usual string spacetime predicted by general relativity is modified.
The starting model contains a complex scalar field that interacts chirally with fermions through a Yukawa coupling. When the scalar field picks a vacuum value, a symmetry is broken and the low-energy remnant is a pseudoscalar Goldstone boson. Integrating out the heavy fermions and the massive radial mode generates the dCS coupling: a term that ties that pseudoscalar to a curvature combination called the Pontryagin density. In the ultraviolet completion discussed by the authors, the heavy fermions could be examples such as right-handed sterile neutrinos.
Cosmic strings are one-dimensional topological defects that can form in such symmetry-breaking phase transitions. In ordinary general relativity a straight global string sources a known exterior metric (the Cohen–Kaplan solution) and has an energy density that grows slowly with distance. The authors note that an unexcited, axisymmetric straight string does not excite the dCS modification because the extra tensor from the Pontryagin coupling vanishes for that symmetry.
The new effect comes when fermionic zero modes live on the string worldsheet. These are low-energy fermion states bound to the string that can carry a null current along the string. The paper generalizes the Callan–Harvey zero-mode solution to this setup and shows that the null current sources the C-tensor of dCS gravity. That sourcing breaks parity and produces a non–general-relativity correction to the string metric. The authors derive the leading-order modification to the exterior metric in the regime of weak gravity and weak coupling to the dCS scalar, and they outline an effective action description for more general string configurations.