concept

neutrino mass

Neutrino mass is a fundamental property of neutrinos, sought through experiments like Antarctic detectors.
10 related articles · 2 formulas

Description

Neutrino mass is the intrinsic mass of neutrinos, the ghostly particles that barely interact with matter. For decades, neutrinos were thought to be massless, but the discovery of neutrino oscillations — where neutrinos change flavor as they travel — proved they must have tiny but nonzero masses. The absolute scale of these masses remains unknown, and determining it is one of the key open problems in particle physics and cosmology. Neutrino masses are so small that they are often described as 'weighing a ghost', and their exact values could reveal physics beyond the Standard Model.

History

The possibility of neutrino mass was first suggested by Bruno Pontecorvo in the 1950s, and the first evidence for oscillations came from the Super-Kamiokande experiment in 1998. The absolute mass scale has been pursued since the 1980s, with the KATRIN experiment providing the most stringent direct limits since 2019.

How it works

Neutrino mass is measured indirectly through the kinematics of beta decay, where a nucleus emits an electron and a neutrino. By precisely measuring the maximum energy of the emitted electron, one can infer the neutrino's mass, since the total energy must be shared between the particles. Experiments like KATRIN use a huge spectrometer to analyze the electron energy spectrum near its endpoint. Alternatively, cosmological observations of the cosmic microwave background and galaxy clustering can constrain the sum of neutrino masses, because massive neutrinos suppress the growth of structure on small scales.

In practice

Knowing neutrino masses helps calibrate cosmological models and could guide the search for new particles, but there are no direct technological applications yet; the main impact is in fundamental physics and astrophysics.

Fun fact

The sum of all three neutrino masses is at least a million times smaller than the mass of an electron, yet neutrinos are so abundant that they collectively outweigh all the stars in the universe.

Concept graph →

Formulas

$$\Omega_\nu h^2 = \frac{\sum m_\nu}{93.14\,\text{eV}}$$
Relates neutrino mass sum to cosmological density parameter.
What is in the formula
Ω_νvariableNeutrino density parameter — density parameter
hvariableDimensionless Hubble constant — hubble constant dimensionless
Σ m_νvariableSum of neutrino masses — neutrino mass sum electronvolt
93.14constantNumerical factor converting eV to density parameter — neutrino density conversion = 93.14 electronvolt
ω_νh^2=\frac{\summ_ν}{93.12эв} · 2607.01226v1
$$m^* = m - g_\sigma \sigma$$
Nucleon mass is reduced by scalar meson field coupling.
What is in the formula
m^*variableEffective nucleon mass in the medium — effective mass kilogram
mvariableBare nucleon mass (in vacuum) — mass kilogram
\sigmavariableScalar meson field expectation value — scalar field
g_\sigmaconstantCoupling constant between nucleons and the scalar sigma meson — coupling constant = varies (model-dependent)
m^*_n=m_n-g_σφ · 2607.13930

Related articles · 10

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