Model-building implications from light magnetic monopoles: a case study of flavour deconstruction
5 affiliations
- 1PSI Center for Neutron and Muon Sciences, Paul Scherrer Institute PSI
- 2Universität Zürich
- 3Università degli Studi Roma Tre and, INFN Sezione di Roma Tre
- 4Institut für Theoretische Physik, ETH Zürich
- 5Universität Basel
Abstract
A bstract : We highlight a generic connection between extensions of the Standard Model featuring low-scale semi-simple embeddings of U(1) EM and the phenomenology of light magnetic monopoles in the early Universe. Combining cosmological, astrophysical, and direct-search constraints, we show that magnetic monopoles with masses far below the scale of Grand Unified Theories are generically excluded and require low-scale inflation to dilute their abundance, followed by reheating below the monopole-production scale. These constraints are particularly relevant for flavour non-universal models, which provide a well-motivated framework to address the hierarchical structure of Yukawa couplings while allowing new dynamics close to the TeV scale compatible with experimental bounds. In many of these constructions, the sequential breaking of semi-simple gauge groups through intermediate stages containing a U(1) factor generically leads to the production of light magnetic monopoles. We show that the parameter region naturally predicted by these models implies low-scale inflation, with reheating temperature as low as 10 ³ –10 ⁴ TeV. These results significantly reduce the otherwise large allowed inflationary window and establish a direct connection between flavour physics and the thermal history of the early Universe: future evidence for a low-scale semi-simple embedding of U(1) EM , in particular through flavour non-universal interactions, would point towards low-scale reheating, while probes of primordial gravitational waves could directly constrain the scale at which low-scale semi-simple groups can appear.
Related
- Probing flavour deconstruction via primordial gravitational waves.
- Reconstructing stochastic gravitational-wave signals from flavour deconstruction with LISA
- Magnetic monopoles: from Dirac to the Large Hadron Collider
- Magnetic monopoles produced by first-order phase transition
- Low-Mass Magnetic Monopoles in the Galaxy: Simulations and Comparison with Ultra-High-Energy Cosmic-Ray Data
BibTeX
@article{pesut2026modelbuilding,
title = {{Model-building implications from light magnetic monopoles: a case study of flavour deconstruction}},
author = {Marko Pesut and Davide Racco and Yunlong Zhao},
journal = {Journal of High Energy Physics},
year = {2026},
month = oct,
doi = {10.1007/jhep10(2026)083},
url = {https://link.springer.com/article/10.1007/JHEP10(2026)083},
note = {CC BY 4.0},
}
RIS
TY - JOUR
TI - Model-building implications from light magnetic monopoles: a case study of flavour deconstruction
AU - Marko Pesut
AU - Davide Racco
AU - Yunlong Zhao
PY - 2026
DA - 2026/10/08
JO - Journal of High Energy Physics
DO - 10.1007/jhep10(2026)083
UR - https://link.springer.com/article/10.1007/JHEP10(2026)083
AB - A bstract : We highlight a generic connection between extensions of the Standard Model featuring low-scale semi-simple embeddings of U(1) EM and the phenomenology of light magnetic monopoles in the early Universe. Combining cosmological, astrophysical, and direct-search constraints, we show that magnetic monopoles with masses far below the scale of Grand Unified Theories are generically excluded and require low-scale inflation to dilute their abundance, followed by reheating below the monopole-production scale. These constraints are particularly relevant for flavour non-universal models, which provide a well-motivated framework to address the hierarchical structure of Yukawa couplings while allowing new dynamics close to the TeV scale compatible with experimental bounds. In many of these constructions, the sequential breaking of semi-simple gauge groups through intermediate stages containing a U(1) factor generically leads to the production of light magnetic monopoles. We show that the parameter region naturally predicted by these models implies low-scale inflation, with reheating temperature as low as 10 ³ –10 ⁴ TeV. These results significantly reduce the otherwise large allowed inflationary window and establish a direct connection between flavour physics and the thermal history of the early Universe: future evidence for a low-scale semi-simple embedding of U(1) EM , in particular through flavour non-universal interactions, would point towards low-scale reheating, while probes of primordial gravitational waves could directly constrain the scale at which low-scale semi-simple groups can appear.
SN - 1029-8479
ER -