The first nuclear clock will test if fundamental constants change

Physicists are developing ultra-precise “nuclear clocks,” such as one based on a thorium-229 nuclear transition, to test whether fundamental constants like the fine-structure constant or gravitational constant truly remain fixed over time and space. Commenters explore how current observations of atomic spectra, natural nuclear reactors like Oklo, and cosmological data already place tight limits on any variation, and how changing constants could affect everything from black holes to dark matter explanations. The conversation also delves into measurement limits, the role of unit choices, and what it would mean for physics if even tiny drifts in these constants were confirmed.

Variation of Fundamental Constants

  • Several comments focus on how much spatial or temporal variation in constants (fine-structure constant, G, proton–electron mass ratio) is compatible with existing observations. Current limits quoted are extremely small per year.
  • Spectral lines from distant galaxies (e.g., hydrogen Lyman series) are emphasized as sensitive probes: redshifted spectra still have the same relative line spacings once redshift is corrected, strongly constraining variation.
  • Oklo’s natural nuclear reactor is cited as evidence that the fine-structure constant has remained effectively unchanged over ~2 billion years.

Observational and Experimental Probes

  • Spectroscopy of distant galaxies and quasars: compare line positions and spacings to local lab values; look for anisotropies or “stacked” features like the Lyman-alpha forest.
  • Natural reactors and fossil processes (Oklo) provide long-baseline checks on nuclear physics parameters.
  • Ultra-precise atomic and optical lattice clocks already detect gravitational time dilation over centimeter height differences; a thorium-229 nuclear clock would further tighten constraints and search for tiny drifts.
  • Environmental noise (height changes, lunar/planetary tides, Earth’s orbit, mass redistribution) must be modeled out for such clocks.

Units, Dimensionless Ratios, and “What’s Really Fundamental”

  • Strong debate over which quantities are truly fundamental. Many constants can be removed by choosing natural units; what remain are dimensionless coupling strengths and a small number of dimensionful scales.
  • Some argue only interaction strengths (gravity, EM, strong, weak) are fundamental; particle masses and mixing parameters are then derived properties or ratios. Others point out that in the Standard Model a couple dozen parameters (including mass ratios and mixing angles) are empirically fundamental.
  • It’s stressed that variation of dimensionless constants (e.g., fine-structure constant) is physically meaningful, whereas variation of a dimensionful constant alone can be partly a matter of convention.

Cosmology, Dark Matter/Energy, and the Big Bang

  • Dark matter and dark energy are discussed as “placeholders” for discrepancies vs. as real but unknown substances. MOND and other modified-gravity ideas are mentioned but considered less successful overall than standard ΛCDM.
  • Some speculate varying constants might mimic dark components or alter inferred expansion rates, but this is presented as highly constrained and speculative.
  • There are side discussions about whether time existed “before” the Big Bang, cyclic/Big Crunch models, and whether changes in constants could trigger a bang; consensus is that such ideas are interesting but very hard to test.

Relativity, Time, and Clocks

  • Gravitational time dilation is central: clocks at different heights tick at measurably different rates; modern optical clocks can see ~1 cm differences.
  • The equivalence principle is noted to be only locally exact; for sufficiently large “elevators” tidal and redshift effects across the height become detectable.
  • There is extended debate about photons, proper time, affine parameters, and the popular simplification that photons “experience no time.” Some call this a pedagogical oversimplification rather than literally correct.

Energy Conservation and Thermodynamics

  • One commenter claims varying constants would break energy conservation and the second law. Replies counter that:
    • Energy conservation is subtle or ill-defined in general relativity; global conservation doesn’t strictly hold in expanding spacetime.
    • The second law is statistical and about entropy, not strictly tied to exact energy conservation; a varying total energy doesn’t automatically violate it.

Philosophical and Conceptual Debates

  • Some propose unfalsifiable ideas (e.g., constants or outcomes differ when unobserved); others criticize this as definitional or god-of-the-gaps reasoning.
  • There is discussion about whether existence and observability should be treated as equivalent, and the general impossibility of “proving a negative.”
  • A meta-point: if everything changed, including our rulers and clocks, some kinds of variation might be intrinsically undetectable; only relative and dimensionless changes are operationally meaningful.

Why a Nuclear Clock Matters

  • A thorium-229 nuclear clock would be sensitive to different combinations of constants than electronic/optical transitions, offering a new “ruler” to compare against existing clocks.
  • If any drift is seen, cross-checks with other clocks and astrophysical data could reveal whether fundamental couplings are changing, which would force a major revision of current physics.
  • If no drift is found at unprecedented precision, it further tightens bounds on any variation, reinforcing the assumption of constant laws across cosmological time and space.