{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:2BIYMMDCISIYUO2OHK6YF5KMCY","short_pith_number":"pith:2BIYMMDC","schema_version":"1.0","canonical_sha256":"d05186306244918a3b4e3abd82f54c1602327f63f5693672b7f31a3cd85bd631","source":{"kind":"arxiv","id":"2411.18030","version":1},"attestation_state":"computed","paper":{"title":"LISA test-mass charging. Particle flux modeling, Monte Carlo simulations and induced effects on the sensitivity of the observatory","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Catia Grimani, Francesco Dimiccoli, Martina Muratore, Mattia Villani, Michele Fabi, Paolo Sarra, Rita Dolesi, Valerio Ferroni, William Joseph Weber","submitted_at":"2024-11-27T03:54:27Z","abstract_excerpt":"Context. The LISA space observatory will explore the sub-Hz spectrum of gravitational wave emission from the Universe. The space environment, where will be immersed in, is responsible for charge accumulation on its free falling test masses (TMs) due to the galactic cosmic rays (GCRs) and solar energetic particles (SEP) impinging on the spacecraft. Primary and secondary particles produced in the spacecraft material eventually reach the TMs by depositing a net positive charge fluctuating in time. This work is relevant for any present and future space missions that, like LISA, host free-falling T"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2411.18030","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.IM","submitted_at":"2024-11-27T03:54:27Z","cross_cats_sorted":[],"title_canon_sha256":"52938e23f38c731633d6445e2b0eadd9cd2e19cacfd0915d2a5732fe42f73699","abstract_canon_sha256":"8e3e071f14247b83cfcd00acd4c6f70d78c8ea5778a0ec4b029a36c14d844357"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:52:46.670739Z","signature_b64":"Il9c2+77YjOoJeHGqt+gwNRlf4ntblDXp7DcA2hFjChmwC4SXSC5lOFdX+n588EHwndTRm8+/qVKkAHIA7drBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d05186306244918a3b4e3abd82f54c1602327f63f5693672b7f31a3cd85bd631","last_reissued_at":"2026-07-05T11:52:46.670329Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:52:46.670329Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"LISA test-mass charging. Particle flux modeling, Monte Carlo simulations and induced effects on the sensitivity of the observatory","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Catia Grimani, Francesco Dimiccoli, Martina Muratore, Mattia Villani, Michele Fabi, Paolo Sarra, Rita Dolesi, Valerio Ferroni, William Joseph Weber","submitted_at":"2024-11-27T03:54:27Z","abstract_excerpt":"Context. The LISA space observatory will explore the sub-Hz spectrum of gravitational wave emission from the Universe. The space environment, where will be immersed in, is responsible for charge accumulation on its free falling test masses (TMs) due to the galactic cosmic rays (GCRs) and solar energetic particles (SEP) impinging on the spacecraft. Primary and secondary particles produced in the spacecraft material eventually reach the TMs by depositing a net positive charge fluctuating in time. This work is relevant for any present and future space missions that, like LISA, host free-falling T"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.18030","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2411.18030/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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"},"aliases":[{"alias_kind":"arxiv","alias_value":"2411.18030","created_at":"2026-07-05T11:52:46.670382+00:00"},{"alias_kind":"arxiv_version","alias_value":"2411.18030v1","created_at":"2026-07-05T11:52:46.670382+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2411.18030","created_at":"2026-07-05T11:52:46.670382+00:00"},{"alias_kind":"pith_short_12","alias_value":"2BIYMMDCISIY","created_at":"2026-07-05T11:52:46.670382+00:00"},{"alias_kind":"pith_short_16","alias_value":"2BIYMMDCISIYUO2O","created_at":"2026-07-05T11:52:46.670382+00:00"},{"alias_kind":"pith_short_8","alias_value":"2BIYMMDC","created_at":"2026-07-05T11:52:46.670382+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2BIYMMDCISIYUO2OHK6YF5KMCY","json":"https://pith.science/pith/2BIYMMDCISIYUO2OHK6YF5KMCY.json","graph_json":"https://pith.science/api/pith-number/2BIYMMDCISIYUO2OHK6YF5KMCY/graph.json","events_json":"https://pith.science/api/pith-number/2BIYMMDCISIYUO2OHK6YF5KMCY/events.json","paper":"https://pith.science/paper/2BIYMMDC"},"agent_actions":{"view_html":"https://pith.science/pith/2BIYMMDCISIYUO2OHK6YF5KMCY","download_json":"https://pith.science/pith/2BIYMMDCISIYUO2OHK6YF5KMCY.json","view_paper":"https://pith.science/paper/2BIYMMDC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2411.18030&json=true","fetch_graph":"https://pith.science/api/pith-number/2BIYMMDCISIYUO2OHK6YF5KMCY/graph.json","fetch_events":"https://pith.science/api/pith-number/2BIYMMDCISIYUO2OHK6YF5KMCY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2BIYMMDCISIYUO2OHK6YF5KMCY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2BIYMMDCISIYUO2OHK6YF5KMCY/action/storage_attestation","attest_author":"https://pith.science/pith/2BIYMMDCISIYUO2OHK6YF5KMCY/action/author_attestation","sign_citation":"https://pith.science/pith/2BIYMMDCISIYUO2OHK6YF5KMCY/action/citation_signature","submit_replication":"https://pith.science/pith/2BIYMMDCISIYUO2OHK6YF5KMCY/action/replication_record"}},"created_at":"2026-07-05T11:52:46.670382+00:00","updated_at":"2026-07-05T11:52:46.670382+00:00"}