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Searches for light dark matter using condensed matter systems

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arxiv 2108.03239 v2 pith:3V4LU3WT submitted 2021-08-06 hep-ph astro-ph.COcond-mat.mtrl-scihep-ex

classification hep-phastro-ph.COcond-mat.mtrl-scihep-ex
keywords mattercondenseddarkdetectionreviewsearchessystemstarget
verification ladder T0 review T1 audit T2 compute T3 formal
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Identifying the nature of dark matter (DM) has long been a pressing question for particle physics. In the face of ever-more-powerful exclusions and null results from large-exposure searches for TeV-scale DM interacting with nuclei, a significant amount of attention has shifted to lighter (sub-GeV) DM candidates. Direct detection of the light dark matter in our galaxy by observing DM scattering off a target system requires new approaches compared to prior searches. Lighter DM particles have less available kinetic energy, and achieving a kinematic match between DM and the target mandates the proper treatment of collective excitations in condensed matter systems, such as charged quasiparticles or phonons. In this context, the condensed matter physics of the target material is crucial, necessitating an interdisciplinary approach. In this review, we provide a self-contained introduction to direct detection of keV--GeV DM with condensed matter systems. We give a brief survey of dark matter models and basics of condensed matter, while the bulk of the review deals with the theoretical treatment of DM-nucleon and DM-electron interactions. We also review recent experimental developments in detector technology, and conclude with an outlook for the field of sub-GeV DM detection over the next decade.

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Cited by 6 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Spin-Dependent Scattering of Sub-GeV Dark Matter: Models and Constraints

    hep-ph 2025-06 conditional novelty 8.0 of 10

    A new calculation of spin-dependent sub-GeV dark matter phonon scattering shows only the light scalar mediator model retains testable parameter space, conditional on the supernova trapping window.

  2. Coherence from interference: a solvable model of sub-GeV dark matter-nucleus scattering

    hep-ph 2026-07 conditional novelty 6.0 of 10

    In an exactly solvable 1D lattice, coherent and incoherent DM-nucleus structure factors differ only by a crystal-momentum delta function that becomes unimportant for n≥2 phonons, validating hybrid Inc+LW rate calculations.

  3. Migdal Ionization as a Probe of Light Dark Matter from Nuclear Transition

    hep-ph 2026-07 conditional novelty 6.0 of 10

    Migdal ionization of reactor-produced sub-MeV dark matter in TEXONO germanium yields new 95% C.L. limits on the reference DM–proton cross section for 0.01 MeV ≤ mχ ≲ 2.6 MeV.

  4. SPLENDOR: a novel detector platform to search for light dark matter with narrow-gap semiconductors

    physics.ins-det 2025-07 conditional novelty 6.0 of 10

    A dark matter detector platform combining a 60 meV-gap semiconductor (Eu5In2Sb6) with cryogenic HEMT readout and daily modulation analysis is presented, with projected sensitivity to sub-MeV dark matter.

  5. Sub-GeV Dark Matter Under Pressure from Direct Detection

    hep-ph 2025-07 conditional novelty 4.0 of 10

    PandaX-4T S2-only data yields world-leading sub-GeV dark matter-electron scattering limits for heavy mediators in the 20-200 MeV range, although the result largely overlaps with the collaboration's own just-released analysis.

  6. 2024 TASI Lectures: A Dark Matter Primer

    hep-ph 2025-06 conditional novelty 1.0 of 10

    A graduate-level primer covering the evidence for dark matter, the main cosmological production mechanisms (freeze-out, freeze-in, misalignment), and the direct detection formalism, with no new results.

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