Skip to main content

Research Repository

Advanced Search

Towards Schwinger production of magnetic monopoles in heavy-ion collisions

Gould, Oliver; Ho, David L. -J.; Rajantie, Arttu

Authors

David L. -J. Ho

Arttu Rajantie



Abstract

Magnetic monopoles may be produced by the Schwinger effect in the strong magnetic fields of peripheral heavy-ion collisions. We review the form of the electromagnetic fields in such collisions and calculate from first principles the cross section for monopole pair production. Using the worldline instanton method, we work to all orders in the magnetic charge, and hence are not hampered by the breakdown of perturbation theory. Our result depends on the spacetime inhomogeneity through a single dimensionless parameter, the Keldysh parameter, which is independent of collision energy for a given monopole mass. For realistic heavy-ion collisions, the computational cost of the calculation becomes prohibitive and the finite size of the monopoles needs to be taken into account, and therefore our current results are not applicable to them—we indicate methods of overcoming these limitations, to be addressed in further work. Nonetheless, our results show that the spacetime dependence enhances the production cross section and would therefore lead to stronger monopole mass bounds than in the constant-field case.

Citation

Gould, O., Ho, D. L. .-J., & Rajantie, A. (2019). Towards Schwinger production of magnetic monopoles in heavy-ion collisions. Physical Review D, 100, Article 015041. https://doi.org/10.1103/PhysRevD.100.015041

Journal Article Type Article
Acceptance Date Feb 26, 2019
Online Publication Date Jul 29, 2019
Publication Date Jul 29, 2019
Deposit Date Jan 6, 2023
Journal Physical Review D
Print ISSN 2470-0010
Electronic ISSN 2470-0029
Publisher American Physical Society
Peer Reviewed Peer Reviewed
Volume 100
Article Number 015041
DOI https://doi.org/10.1103/PhysRevD.100.015041
Public URL https://nottingham-repository.worktribe.com/output/6187505
Publisher URL https://journals.aps.org/prd/abstract/10.1103/PhysRevD.100.015041