Pith. sign in

REVIEW 6 cited by

Dark Matter Daily Modulation With Anisotropic Organic Crystals

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2103.08601 v2 pith:FAIAP5SF submitted 2021-03-15 hep-ph hep-exphysics.chem-ph

classification hep-phhep-exphysics.chem-ph
keywords darkmattermodulationratedailyorganiccrystalselectronic
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

Aromatic organic compounds, because of their small excitation energies ~ O(few eV) and scintillating properties, are promising targets for detecting dark matter of mass ~ O(few MeV). Additionally, their planar molecular structures lead to large anisotropies in the electronic wavefunctions, yielding a significant daily modulation in the event rate expected to be observed in crystals of these molecules. We characterize the daily modulation rate of dark matter interacting with an anisotropic scintillating organic crystal such as trans-stilbene, and show that daily modulation is an ~ O(1) fraction of the total rate for small DM masses and comparable to, or larger than, the ~ 10% annual modulation fraction at large DM masses. As we discuss in detail, this modulation provides significant leverage for detecting or excluding dark matter scattering, even in the presence of a non-negligible background rate. Assuming a non-modulating background rate of 1/min/kg that scales with total exposure, we find that a 100 kg yr experiment is sensitive to the cross section corresponding to the correct relic density for dark matter masses between 1.3-14 MeV (1.5-1000 MeV) if dark matter interacts via a heavy (light) mediator. This modulation can be understood using an effective velocity scale v* = Delta E/q*, where Delta E is the electronic transition energy and q* is a characteristic momentum scale of the electronic orbitals. We also characterize promising future directions for development of scintillating organic crystals as dark matter detectors.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 6 Pith papers

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

  1. First-principles upper bounds on dark matter-electron scattering rates from condensed matter sum rules

    hep-ph 2026-08 conditional novelty 6.0 of 10

    Dark matter-electron scattering rates in isotropic materials are bounded from above by a universal expression depending only on plasma frequency, mass density, and static dielectric function.

  2. Ubiquitous Corotation of Dark Matter Halos: Implications for Direct Detection

    hep-ph 2026-07 conditional novelty 6.0 of 10

    Dark matter in simulated Milky Way analogues preferentially corotates with the baryonic disk, suppressing predicted direct-detection rates for light WIMPs, reducing directional modulation, and producing a 21% astrophy...

  3. Dark Matter Weather: Probing Sub-GeV Interactions with Earth-Shielding Modulation

    hep-ph 2026-07 conditional novelty 6.0 of 10

    Daily Earth-shielding modulation of sub-GeV dark matter can separate dark-matter–electron from dark-matter–nucleon scattering, and the isoangle shape statistic provides a new validation handle for liquid-noble detectors.

  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. Community Report from the 2025 SNOLAB Future Projects Workshop

    hep-ex 2025-07 unverdicted novelty 1.0 of 10

    A community report summarizes proposed future experiments and infrastructure needs for SNOLAB over the next 15 years.

  6. First High-Throughput Evaluation of Dark Matter Detector Materials

    hep-ph 2025-06

Pith tools