Dark Matter search

(2) Univ.; (3) IHEP Beijing); A. Incicchitti (2); C. J. Dai (3); D. Prosperi (2); F. Cappella (1); F. Montecchia (1); F. Nozzoli (1); H. H. Kuang (3); INFN Roma

Dark Matter search

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arxiv astro-ph/0307403 v1 pith:676I6NBL submitted 2003-07-23 astro-ph hep-ex

Dark Matter search

R. Bernabei (1) , P. Belli (1) , F. Cappella (1) , R. Cerulli (1) , F. Montecchia (1) , F. Nozzoli (1) , A. Incicchitti (2) , D. Prosperi (2)

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C. J. Dai (3) H. H. Kuang (3) J. M. Ma (3) Z. P. Ye (3) ((1) Univ. INFN Roma2 (2) Univ. INFN Roma (3) IHEP Beijing)

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keywords addressedannualdamadarkmattermodelparticleresults

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Main arguments on the Dark Matter particle direct detection approach are addressed on the basis of the work and of the results of the about 100 kg highly radiopure NaI(Tl) DAMA experiment (DAMA/NaI), which has been operative at the Gran Sasso National Laboratory of the I.N.F.N. for more than one decade, including the preparation. The effectiveness of the WIMP model independent annual modulation signature is pointed out by discussing the results obtained over 7 annual cycles (107731 kg day total exposure); the WIMP presence in the galactic halo is strongly supported at 6.3 standard deviation C.L. The complexity of the corollary model dependent quests for a candidate particle is also addressed and several of the many possible scenarios are examined.

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DAMA/LIBRA and dark matter: decisive tension or contrived cancellation
hep-ph 2025-10 conditional novelty 6.0

DAMA's annual modulation signal is incompatible at >5σ with ANAIS-112 and COSINE-100 under physical dark-matter recoil models; reconciliation requires contrived opposite-sign sodium/iodine tuning.