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Neutrino Decay Reconciles Two Worlds ⚡ экспресс

Original: "Neutrino decays as a natural explanation of the neutrino mass tension"
· Guillermo Franco Abellán
arXiv:2601.04312v2 · 2026-01-07 · CC BY 4.0 · ⏱ 1 min · Cosmology HEP Phenomenology HEP Theory
Neutrino decay into invisible particles explains the discrepancy between cosmological and laboratory data on mass.
Abstract

Cosmological observations say the total mass of all neutrino types is tiny, while oscillation experiments require it to be noticeably larger. This contradiction can be resolved if neutrinos decay over time into lighter, invisible particles — like vanishing guests at a party. This hypothesis lifts the mass constraints and reconciles the data. So, could neutrinos be heavier than we thought?

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In the thirties, Pauli realized: without tiny ghost-like particles, the energy of stars doesn't add up. Thus neutrinos were born—intangible wanderers that permeate everything. They must have mass, otherwise they can't transform into one another, but observations of the expansion of the Universe showed their total weight was nearly zero. Meanwhile, laboratory experiments insisted on a larger number.

A new study compares neutrinos to potatoes in a leaky sack. If half the tubers go missing along the way, weighing the remainder will leave you short. It's the same with cosmology: if neutrinos decay into completely invisible particles over a period of ten million to a billion years, today we measure only their surviving fraction. Fresh data from the DESI survey and the cosmic microwave background from the Big Bang allow a mass up to four times higher than previous estimates—enough to settle the dispute.

An unexpected twist: decay into familiar neutrino types yields almost no benefit. The sack still seems full. So nature is hiding something beyond the Standard Model inside it—particles we don't yet know about. That's where the search should go.

🎯 There are almost as many neutrinos in the Universe as photons of the cosmic microwave background—about 330 per cubic centimeter.

Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesAdam RiessBrian Schmidt
Tags
Standard Model expansion of the universe big bang
Laws
Friedmann equationsHubble's lawNoether's theoremEinstein field equationsPlanck's lawspin–statistics theorem
Original: arXiv:2601.04312v2 · CC BY 4.0 · bridge42worlds