A Dark Dimension in the Tritium Spectrum: How KATRIN Searches for a Fifth Dimension ✛ ✎

Original: "Searching for a Dark Dimension Right-handed Neutrino in KATRIN"
arXiv:2509.05233 · 2025-09-05 · arXiv non-exclusive · independent analysis · 3 min
A neutrino living in a fifth dimension would leave a distinctive kink in the tritium beta spectrum, and KATRIN is poised to see it.

Context

The dark dimension scenario posits that an extra dimension of micron size is tied to the dark energy scale. In this context, the right-handed neutrino can propagate in the bulk rather than being localized on the brane, which naturally explains the smallness of neutrino masses. This work sits alongside studies of sterile neutrinos and neutrino oscillations, but differs in that it considers not a single sterile state but a whole tower of Kaluza-Klein excitations arising from the compactification of the extra dimension. This links the search for new neutrinos to fundamental questions in quantum gravity and dark energy.

Methods

The authors construct a five-dimensional model where three right-handed neutrinos live in the bulk, while the Standard Model is localized on a brane. They solve the mass equations for the Kaluza-Klein states, obtaining the spectrum and mixing matrices. They then compute the differential tritium beta decay spectrum including contributions from all excitations and compare it with predictions from the Standard Model and the 3+1 model with a sterile neutrino. For analytical analysis, they identify two limiting cases: small and large bulk neutrino mass relative to the compactification scale.

Results

For a small bulk mass (compared to the inverse radius), the beta decay spectrum contains a series of kinks corresponding to Kaluza-Klein excitations. For a radius smaller than about 0.4 microns, several kinks could fall within KATRIN's sensitivity. For a large bulk mass, a single effective kink appears at an energy equal to the bulk mass, with an effective mixing angle that can be computed analytically. This allows direct use of existing KATRIN limits on sterile neutrinos to constrain the dark dimension parameters. For example, for a radius of 10 microns and a bulk mass around 1 eV, a significant portion of the parameter space remains allowed but could be probed in future measurements.

Implications

The work shows that KATRIN can not only search for sterile neutrinos but also test the dark dimension hypothesis. Unlike previous studies that mainly focused on small Yukawa couplings, this work considers the large coupling regime, opening a new window in parameter space. This makes the connection between neutrino physics and quantum gravity more concrete and testable.

Future development

The model can be extended to multiple extra dimensions or more complex geometries. It will also require accounting for finite spectral line widths and systematic uncertainties in KATRIN. Future TRISTAN data with improved resolution will allow probing the kiloelectronvolt mass region, potentially providing additional constraints.

Impact

The results will affect the interpretation of KATRIN data and future searches for sterile neutrinos, as well as theoretical models with extra dimensions.

Next steps

Perform detailed numerical simulations of the full beta decay spectrum including all Kaluza-Klein states and compare with actual KATRIN data.

Key open problems

This work directly addresses the unresolved problem of neutrino mass origin and the possible role of extra dimensions. It also touches on whether neutrinos are Dirac or Majorana, which has implications for neutrinoless double beta decay.

The knowledge machine's view

This section is addressed to the author of the paper and their colleagues. Neighbouring works were found by meaning-based search across our archive, not by word overlap. We do not review: we show the field around the work.

What the work does

The authors build a five-dimensional model with right-handed neutrinos in the bulk and compute signatures in the tritium beta-decay spectrum for KATRIN. Two limiting cases of bulk mass are considered: a small mass gives a series of kinks, while a large mass yields a single effective kink, resembling a sterile neutrino signal. The resulting constraints on the dark dimension parameters show that a significant portion of the parameter space is accessible to KATRIN.

Where its strength is

This work connects the search for new neutrinos with the fundamental dark dimension hypothesis, proposing a concrete experimental signal: kinks in the KATRIN spectrum. Especially valuable is the considered regime of large Yukawa couplings, which had not been analyzed before and opens a new window in the parameter space.

Where it could go next

  • It might be interesting to compare the obtained constraints with global analyses of sterile neutrinos, which include data from many experiments. In our archive, there is a nearby paper on the hunt for sterile neutrinos in various channels, which could help place the dark dimension predictions in a broader context.based on: Hunting for Sterile Neutrinos arXiv:2603.23256
  • For a more accurate forecast of KATRIN's sensitivity to Kaluza-Klein kinks, one could refer to the analysis of systematic effects and search techniques for sterile neutrinos in this experiment. The archive contains a review related to KATRIN that discusses such issues.
  • It is interesting to consider how the dark dimension might manifest in other astrophysical neutrino sources, for example, solar neutrinos. A nearby paper on the search for sterile neutrinos in the solar spectrum could provide additional constraints or signals for the model.based on: Catchers of Solar Ghosts arXiv:2606.17042

Worth trying

  • Apply the method of translating KATRIN constraints on sterile neutrinos into constraints on dark dimension parameters for various values of the radius and bulk mass.
  • Check how the spectrum prediction changes when accounting for the finite width of resonances and the experimental resolution of KATRIN, possibly using simulations.
  • Assess whether future experiments, such as Project 8, could resolve individual Kaluza-Klein kinks at small bulk mass.

Why this may matter

A test of the dark dimension at KATRIN would be the first experimental hint of extra dimensions related to dark energy, linking neutrino physics with quantum gravity.

If the extra dimension has a radius of 10 microns, the Kaluza-Klein excitations of the neutrino are separated in mass by only 0.02 eV, which is smaller than the mass differences between ordinary neutrinos.

The idea of extra dimensions where particles can live evokes the concept of hyperspace from science fiction, for instance in Greg Egan's novel 'Diaspora', where characters travel through extra dimensions.

Key numbers

  • radius of the extra dimension: on the order of a micron
  • mass of Kaluza-Klein excitations: from 0.4 to 40 eV
  • tritium spectrum endpoint energy: 18.57 keV
  • KATRIN sensitivity to neutrino mass: 0.45 eV (90% C.L.)
  • upper bound on radius from gravitational tests: 30 μm
Scientists
Paul DiracMarie CurieEnrico FermiChien-Shiung Wu
Concepts
katrin right handed neutrino sterile neutrino extra dimension super kamiokande antineutrino neutron mass kagra juno hyper kamiokande neutrinoless double beta decay compactness dilaton sterile neutrino dark matter neutron star dark matter negative pressure