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Non-equilibrium anti-Stokes Raman spectroscopy for investigating Higgs modes in superconductors

  • Tomke E. Glier
  • , Sida Tian
  • , Mika Rerrer
  • , Lea Westphal
  • , Garret Lüllau
  • , Liwen Feng
  • , Jakob Dolgner
  • , Rafael Haenel
  • , Marta Zonno
  • , Hiroshi Eisaki
  • , Martin Greven
  • , Andrea Damascelli
  • , Stefan Kaiser
  • , Dirk Manske
  • , Michael Rübhausen

Research output: Contribution to journalArticlepeer-review

Abstract

Even before its role in electroweak symmetry breaking, the Anderson-Higgs mechanism was introduced to explain the Meissner effect in superconductors. Spontaneous symmetry-breaking yields massless phase modes representing the low-energy excitations of the Mexican-Hat potential. Only in superconductors the phase mode is shifted towards higher energies owing to the gauge field of the charged condensate. This results in a low-energy excitation spectrum governed by the Higgs mode. Consequently, the Bardeen-Cooper-Schrieffer-like Meissner effect signifies a macroscopic quantum condensate in which a photon acquires mass, representing a one-to-one analogy to high-energy physics. We report on an innovative spectroscopic technique to study symmetries and energies of the Higgs modes in the high-temperature superconductor Bi2Sr2CaCu2O8 after a soft quench of the Mexican-Hat potential. Population inversion induced by an initial laser pulse leads to an additional anti-Stokes Raman-scattering signal, which is consistent with polarization-dependent Higgs modes. Within Ginzburg-Landau theory, the Higgs-mode energy is connected to the Cooper-pair coherence length. Within a Bardeen-Cooper-Schrieffer weak-coupling model we develop a quantitative and coherent description of single-particle and two-particle channels. This opens the avenue for Higgs Spectroscopy in quantum condensates and provides a unique pathway to control and explore Higgs physics.

Original languageEnglish (US)
Article number7027
JournalNature communications
Volume16
Issue number1
DOIs
StatePublished - Dec 2025

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© The Author(s) 2025.

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