i-ncidental N-naturalness

A bstract N -naturalness is a novel solution to the electroweak hierarchy problem which posits N copies of the Standard Model with varying Higgs mass-squared parameters. Reheating proceeds through a “reheaton” particle that deposits most of its energy density into the Standard Model and small but potentially measurable fractions into the other copies. Typically the sector with the lightest negative Higgs mass-squared is identified as the Standard Model. We demonstrate that N -naturalness admits a broader class of realizations in which the Standard Model is identified with a heavier sector, rather than being restricted to the lightest. This is made possible by resonant mixing between the reheaton and the Higgs, which generically causes one sector to be preferentially reheated and to acquire the largest share of the energy density, singling it out as the Standard Model. We demonstrate that this scenario is consistent with current cosmological bounds on new relativistic degrees of freedom and overclosure constraints from heavy stable relics, while future cosmic microwave background and high redshift surveys will probe significant portions of the remaining parameter space. Furthermore, we highlight the possibility of a novel stochastic gravitational wave spectrum from the many cosmological first order QCD phase transitions occurring across the other sectors.

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Publication Details

Journal
Journal of High Energy Physics
Published
2026-05-12
DOI
https://doi.org/10.1007/jhep05(2026)127
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
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article

i-ncidental N-naturalness

Brian Batell, Akshay Ghalsasi, Matthew Low, Wenjie Huang
Journal of High Energy Physics
Cosmology and Gravitation Theories
article

i-ncidental N-naturalness

Brian Batell, Akshay Ghalsasi, Matthew Low, Wenjie Huang
article en

Abstract

A bstract N -naturalness is a novel solution to the electroweak hierarchy problem which posits N copies of the Standard Model with varying Higgs mass-squared parameters. Reheating proceeds through a “reheaton” particle that deposits most of its energy density into the Standard Model and small but potentially measurable fractions into the other copies. Typically the sector with the lightest negative Higgs mass-squared is identified as the Standard Model. We demonstrate that N -naturalness admits a broader class of realizations in which the Standard Model is identified with a heavier sector, rather than being restricted to the lightest. This is made possible by resonant mixing between the reheaton and the Higgs, which generically causes one sector to be preferentially reheated and to acquire the largest share of the energy density, singling it out as the Standard Model. We demonstrate that this scenario is consistent with current cosmological bounds on new relativistic degrees of freedom and overclosure constraints from heavy stable relics, while future cosmic microwave background and high redshift surveys will probe significant portions of the remaining parameter space. Furthermore, we highlight the possibility of a novel stochastic gravitational wave spectrum from the many cosmological first order QCD phase transitions occurring across the other sectors.

Journal of High Energy PhysicsVol. 2026(5)
University of Pittsburgh (US), Harvard University Press (US)
Affordable and clean energy
Openalex Percentile: Top 4%
Cosmology and Gravitation Theories
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