Atomic nucleus excited with laser: A breakthrough after decades

Terminology and Physics Background

  • Discussion over the phrase “classical quantum physics”: some interpret it as non‑relativistic QM vs relativistic quantum field theory.
  • Clarification that relativistic quantum mechanics does exist (Dirac equation, QFT), but a full unification with general relativity is still missing.
  • Nuclear physics is described as still heavily phenomenological; connecting detailed nuclear structure to underlying QCD remains hard.

Why Th‑229 Is Special

  • Thorium‑229 has an unusually low‑energy nuclear isomer (~8.4 eV), far below typical nuclear transitions (MeV range).
  • This transition lies in deep UV (~148.38 nm), unique in being reachable with lasers rather than only high‑energy gamma sources.
  • No good theoretical explanation yet for why its energy is so low; current theory can’t predict such levels with that precision.

Laser, Wavelength, and Linewidth

  • Transition energy must be hit extremely precisely; nuclear states have huge Q factors and narrow linewidths (linked to long lifetimes).
  • Generating 148 nm light with narrow linewidth is technically difficult; current work uses four‑wave mixing in noble gases and frequency comb techniques.
  • The reported result has been independently confirmed using different Th‑doped crystals, boosting confidence in the signal.

Nuclear Excitation Mechanism

  • “Exciting a nucleus” means promoting it from ground to an isomeric state; it later decays probabilistically.
  • For Th‑229 in neutral atoms/solids, decay predominantly occurs via internal conversion: the nucleus transfers energy to an electron, which is ejected.
  • In more highly ionized states, this channel can be blocked, forcing gamma‑like photon emission instead.

Potential Applications

  • Main focus: nuclear clocks. Nuclear levels are less sensitive to external fields than electronic ones and can be hosted in solids, potentially enabling:
    • Higher stability and higher Q than current optical/cesium clocks.
    • Simpler, more compact devices with many nuclei in a crystal instead of trapped single ions.
  • Better clocks improve many areas of metrology, spectroscopy, and interferometry.
  • High‑precision clocks can act as “relativity sensors” to map tiny gravitational potential differences, possibly refining:
    • Gravimetric mineral exploration and geoid mapping.
    • Earth science and maybe earthquake precursors.
  • Possible implications for chip‑scale atomic magnetometers, quantum navigation, and speculative quantum‑computing qubits based on nuclear states are mentioned but not detailed.

Limits, Challenges, and Skepticism

  • Several commenters ask what truly new capabilities better clocks would unlock; others reply that “use cases follow capability,” citing gravitational waves and precision metrology.
  • Gravimetric resource detection already exists; better clocks would improve resolution but can’t fully solve inverse‑problem ambiguities.
  • Gravitational submarine detection is deemed practically impossible by thread participants, even with extreme sensitivity.
  • Nuclear lasers (gamma/UV based on this transition) are considered “maybe feasible but unclear why useful,” except as a tool for precision physics.
  • Little or no direct relevance to power‑reactor thorium fuel cycles; connection is mainly that Th‑229 arises in reactors.

Other Side Topics

  • Clarifications about gamma vs X‑ray vs UV labeling: often distinguished by source (nuclear vs electronic), with overlapping energies.
  • Some joking about naming, band analogies (“octave above blue”), and the broader state of our understanding of nuclear/QCD structure.