SearcharxivSearch

arXiv · 2509.25276

Charge quantisation without compactness: the Higgs and Yukawa mechanisms from matter geometry

Abstract

In the \emph{geometry-first} formulation of gauge theory \citep{Gomes_internal}, Hermitian vector bundles and their covariant derivatives are the primitive objects. Here gauge groups arise only as the automorphism groups of a small set of structured fundamental fibres, and every matter field is a section of a tensor product of the fundamental bundles. This is a constraint on gauge theories. In the abelian sector it enforces charge quantisation, even without compactness: charges count tensor powers of a fundamental line bundle, so they lie on an integral lattice even when the automorphism group is the non-compact $\mathbb{C}^\times$, whereas a symmetry-first theory built on $\mathbb{R}$ admits irrationally related charges. The Standard Model satisfies the constraint, and its two mass-generating mechanisms follow from the fibre geometry. The Higgs mechanism arises from the second fundamental form of the sub-bundle singled out by the Higgs vacuum. This works with no appeal to symmetry breaking or Goldstone's theorem, and the full electroweak spectrum, $m_W=m_Z\cos\theta_W$ included, is computed from the same operator. Each Yukawa coupling is the canonical fibrewise contraction fixed by the inner products and volume forms of the fundamental bundles. Exceptional gauge groups remain formally presentable, but on progressively less elementary fibre structure; at $E_8$ the fundamental fibre is the Lie algebra $\mathfrak{e}_8$ itself, and the claim of conceptual priority collapses. A companion paper shows the two formulations are not equivalent, in a categorical sense \citep{Gomes_nonequiv}.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Henrique Gomes. 2025-09-28. Charge quantisation without compactness: the Higgs and Yukawa mechanisms from matter geometry. https://arxiv.org/abs/2509.25276

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

Scientific Promise

Scientists constantly face decisions about what lines of research to pursue. This Element introduces the philosophical debate about scientific pursuitworthiness. It explains how it can be rational to pursue a theory even if the theory is less well supported than its rivals, and it discusses existing philosophical frameworks for guiding pursuit decisions. The Element also develops a new perspective. Existing accounts focus predominantly on theories, while experiments are largely neglected. This is an important shortcoming. Theoretical promise depends on experimental promise, and experimental promise raises questions of its own. Drawing on the epistemology of experimentation, the Element advances an account of experimental pursuitworthiness. It is argued that such pursuitworthiness depends on experimental virtues like a clear signal and simplicity of design. Moreover, the kinds of uncertainty that constrain the assessment of scientific pursuits are examined. Finally, the Element highlights open questions in the philosophy of scientific pursuitworthiness.

physics.hist-ph

Is Black Hole Evaporation Prediction Friendly?

Manchak and Weatherall (2018) formulate the black hole information paradox as a failure of predictability in black hole evaporation spacetimes, diagnosed by non-global hyperbolicity. I offer a strategy for resolving this paradox. I argue that failures of predictability in black hole evaporation are not well diagnosed by non-global hyperbolicity. I then consider two weakenings of global hyperbolicity: prediction and retrodiction friendliness, the failure of which could ground a new paradox. However, deidealized black hole evaporation models can be prediction and retrodiction friendly. Therefore, the information paradox cannot be based upon failures of global hyperbolicity, nor either retrodiction or prediction unfriendliness.

physics.hist-ph

The Crab Nebula progenitor: recovering the 1054 AD supernova event as galactic Gamma-ray burst

In 1054 AD a daytime star appeared in the constellation of Taurus, for three weeks, and it was reported in various sources from Europe to China/Japan: it was one of the few documented galactic supernovae of the last two millenia. This paradigm has been established about sixty years ago, as the comprehension of the physics of supernovae progressed with enough observational data. The Gamma-ray bursts were discovered in the same period, but only in the past few years have their observations become daily and their distances have been fully understood as cosmological. After the explosion, the exponential decay of the luminosity in gamma-rays and X-rays has been followed with telescopes onboard dedicated satellites. Also the exponential decay of the afterglow's optical and radio frequencies have been observed with the largest optical and radio telescopes. Within the binary-driven hypernova framework, successful in explaining all the observed phases of the Gamma-ray bursts, the universal exponential decay can be extended to 1000 years after the burst, to account for the present values of Gamma and X-rays as well as optical and radio frequencies of the Crab Nebula. Both the daytime visibility of the burst, and the simultaneous radiation plagues appeared in Constantinople and Cairo is a strong evidence of the presence of Gamma-rays in the lower atmosphere, coming from the same source originating the Crab nebula. The association to the daytime visibility of that star and the following plague meets exactly the etymology of the word dis-aster, bad star.

physics.hist-ph