{"paper":{"title":"Effect of cosmic rays on the resonant gravitational wave detector NAUTILUS at temperature T=1.5 K","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"A. Marini, A.Moleti, A. Rocchi, D. Babusci, E. Coccia, F. Ronga, G. Giordano, G. Mazzitelli, G. Modestino, G. Pizzella, G.V. Pallottino, I.Modena, L. Quintieri, M. Bassan, M. Visco, P. Astone, P. Bonifazi, P. Carelli, R. Terenzi, S. D'Antonio, V. Fafone, Y. Minenkov","submitted_at":"2002-06-26T15:34:59Z","abstract_excerpt":"The interaction between cosmic rays and the gravitational wave bar detector NAUTILUS is experimentally studied with the aluminum bar at temperature of T=1.5 K. The results are compared with those obtained in the previous runs when the bar was at T=0.14 K. The results of the run at T = 1.5 K are in agreement with the thermo-acoustic model; no large signals at unexpected rate are noticed, unlike the data taken in the run at T = 0.14 K. The observations suggest a larger efficiency in the mechanism of conversion of the particle energy into vibrational mode energy when the aluminum bar is in the su"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/0206079","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}