Skip to content
CosmosExplorer

The Higgs measurements put empty space on a knife edge between stable and able to decay.

Higgs Vacuum Decay

2013Dario Buttazzo, Giuseppe Degrassi, Gian Giudice, Alessandro StrumiaFrontierReviewed June 3, 2026

The central values of the measured Higgs and top-quark masses place the Standard Model vacuum near or within the metastable region, meaning empty space could in principle tunnel to a lower-energy state and end the universe as we know it.

Skip 3D content

§1 · The claim, in one sentence

Higgs Vacuum Decay is the cosmic fate written into the Standard Model itself. The shape of the Higgs potential at very high energies depends on the masses of the Higgs boson and the top quark, and for the central measured values the electroweak vacuum sits near or within the metastable region: a local minimum, not the global one. Buttazzo and collaborators 2013 made this precise, finding that our vacuum could in principle decay by quantum tunnelling to a lower-energy true , though with a lifetime far longer than the present age of the universe.

§2 · Why it might be true

The Higgs field has a potential energy that depends on its value, and the vacuum we live in sits at the bottom of that potential. But the potential's shape at energies far above what colliders probe is fixed by the same physics that sets the particle masses. Extrapolating the Standard Model upward, the measured Higgs mass near 125 GeV and top-quark mass near 173 GeV put the potential in a regime where a second, deeper minimum exists at very high field values.

That makes our vacuum metastable. It is stable against small disturbances, but a rare quantum could tunnel a small region into the deeper minimum, creating a bubble of true vacuum. Inside that bubble the Higgs field sits at its high-value minimum, so particle masses and the structure of matter are completely different, and the bubble wall sweeps outward at nearly the speed of light, converting the universe as it goes.

Buttazzo, Degrassi, Giudice, and collaborators 2013 turned this into a precision result. Plotting the measured masses on the stability diagram, the Standard Model sits in the metastable band, close to the stability boundary. The predicted decay time is enormous, vastly exceeding the age of the universe, so this is not an imminent threat. But it is striking: the universe appears to be balanced near criticality, and whether it is truly metastable hinges on parameters we measure and on physics beyond the Standard Model we do not yet know.

The family stance

The universe could end by a change of vacuum. If empty space is only metastable, a bubble of true vacuum nucleates somewhere, expands at nearly light speed, and converts everything it sweeps over to a different physics, almost certainly hostile to existing structure. The trigger is quantum tunnelling, and the odds depend on precisely measured particle masses.

§2.5 · Evidence

  • The calculation uses only measured Standard Model parameters and established quantum field theory, so the metastability result is mainstream, not speculative
  • Independent analyses generally find the Standard Model lies close to the stability-metastability boundary, in the metastable region for central parameter values
  • This is the rare cosmic-fate scenario directly tied to collider measurements, making it falsifiable through precision particle physics

§3 · What you'd need to test it

  • The Higgs potential develops a second, deeper minimum at very high field values, given the measured Higgs and top-quark masses
  • The electroweak vacuum is metastable, able in principle to decay by quantum tunnelling to the true vacuum
  • The decay creates a bubble of true vacuum expanding at nearly light speed, with different particle physics inside
  • The predicted vacuum lifetime far exceeds the age of the universe, so the scenario is a long-term possibility, not an imminent event; more precise top-mass measurements sharpen the stability verdict

§4 · Where it breaks

  • The verdict is sensitive to the top-quark mass, whose value and interpretation still carry uncertainty; a slightly lower top mass would make the vacuum absolutely stable
  • Unknown physics between the electroweak and Planck scales could change the high-energy potential and remove the instability entirely
  • Metastability is a statement about a calculation; the claim that the universe will actually decay remains unconfirmed and the lifetime is enormous
Go deeper

Buttazzo, Degrassi, Giardino, Giudice, Sala, Salvio, and Strumia 2013 (JHEP 12, 089) computed the Standard Model effective potential to high precision and the tunnelling action for vacuum decay. The key output is the stability diagram in the Higgs-mass and top-mass plane, divided into stable, metastable, and unstable regions. The measured point lands in the metastable region, a few standard deviations from absolute stability, with the top-quark mass the dominant uncertainty.

The decay itself is a Coleman-De Luccia process: a bubble of true vacuum nucleates and, if larger than a critical size, expands. The near-criticality is itself intriguing. Some authors read the Standard Model's perch near the stability boundary as a hint of deeper structure, perhaps tied to inflation or Planck-scale physics, rather than a coincidence. This is why vacuum stability is an active research frontier and not a closed question.

Cross-references: the foundational tunnelling theory this calculation applies, Coleman-De Luccia false-vacuum decay with gravity, lives in the Chapter 1 vacuum family (the Coleman-De Luccia Bubble Nucleation variant) and is surfaced here as a bridge. The Eternal Inflation family in Chapter 1 uses the same false-vacuum machinery in the opposite direction, as a driver of cosmic birth rather than cosmic death.

Variants in this family

0votes
Currently #1 in Ch.7
§5 · Who built it, and when(1 source, 1 established)

Up next

Spotted an error? Have a source to add?

Prefer email?

You can also send a prefilled email with the variant URL already filled in.

Related theories