Cold dark matter identification: Diurnal modulation reexamined

(2) Tandar; (3) PPE Division; A.O. Gattone (2); CERN); CNEA; D. Abriola (2); D.E. Di Gregorio (2); Depto de Fisica; D. Tomasi (2); F. Hasenbalg (1)

Cold dark matter identification: Diurnal modulation reexamined

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

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 astro-ph/9702165 v2 pith:UMBPFKUW submitted 1997-02-19 astro-ph hep-ph

Cold dark matter identification: Diurnal modulation reexamined

F. Hasenbalg (1) , D. Abriola (2) , J.I. Collar (3) , D.E. Di Gregorio (2) , A.O. Gattone (2) , H. Huck (2) , D. Tomasi (2) , I. Urteaga (2) ((1) University of South Carolina

show 5 more authors

(2) Tandar Depto de Fisica CNEA (3) PPE Division CERN)

This is my paper

classification astro-ph hep-ph

keywords modulationdarkmatterachievecalculationscolddetectorsdifferences

verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved

0 comments

read the original abstract

We report on new estimates of the modulation expected in semiconductor detectors due to eclipsing of dark matter particles in the Earth. We reevaluate the theoretical modulation significances and discuss the differences found with previous calculations. We find that a significantly larger statistics than previously estimated is needed to achieve the same level of sensitivity in the modulated signal.

discussion (0)

Forward citations

Cited by 1 Pith paper

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

Dark Matter Weather: Probing Sub-GeV Interactions with Earth-Shielding Modulation
hep-ph 2026-07 conditional novelty 6.0

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.