{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:4LKLWVXMZGUJFO2XRZ4YDPKOJS","short_pith_number":"pith:4LKLWVXM","schema_version":"1.0","canonical_sha256":"e2d4bb56ecc9a892bb578e7981bd4e4c8b93f909fa45652211743efb586d5b9d","source":{"kind":"arxiv","id":"2404.17334","version":3},"attestation_state":"computed","paper":{"title":"From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Dieter Lust, Ignatios Antoniadis, Jorge F. Soriano, Luis A. Anchordoqui, Neena T. Noble","submitted_at":"2024-04-26T11:32:27Z","abstract_excerpt":"Promptly after high-resolution experiments harbinger the field of precision cosmology low- and high-redshift observations abruptly gave rise to a tension in the measurement of the present-day expansion rate of the Universe ($H_0$) and the clustering of matter ($S_8$). The statistically significant discrepancies between the locally measured values of $H_0$ and $S_8$ and the ones inferred from observations of the cosmic microwave background assuming the canonical $\\Lambda$ cold dark matter (CDM) cosmological model have become a new cornerstone of theoretical physics. $\\Lambda_s$CDM is one of the"},"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":"2404.17334","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2024-04-26T11:32:27Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"ffc6f356679357f46b3ab8a07f10f35aff89ba1089cec17bad0c4f091f8c80ba","abstract_canon_sha256":"ec6d5e3c84d9c0f88de8cc8f32585eb2c4d9f547dc6dda84efc5f8e4c81b92cc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:32:07.315669Z","signature_b64":"0/ECw18Zk6BUuZI0YdkjMwHrLEiw0TQA2e8W4Y7BqjOU8wxPJpYjpq6vrv2s7FIlWA5xiEtJOkNUINg6fKvlCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e2d4bb56ecc9a892bb578e7981bd4e4c8b93f909fa45652211743efb586d5b9d","last_reissued_at":"2026-07-05T09:32:07.315063Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:32:07.315063Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"From infinite to infinitesimal: Using the Universe as a dataset to probe Casimir corrections to the vacuum energy from fields inhabiting the dark dimension","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Dieter Lust, Ignatios Antoniadis, Jorge F. Soriano, Luis A. Anchordoqui, Neena T. Noble","submitted_at":"2024-04-26T11:32:27Z","abstract_excerpt":"Promptly after high-resolution experiments harbinger the field of precision cosmology low- and high-redshift observations abruptly gave rise to a tension in the measurement of the present-day expansion rate of the Universe ($H_0$) and the clustering of matter ($S_8$). The statistically significant discrepancies between the locally measured values of $H_0$ and $S_8$ and the ones inferred from observations of the cosmic microwave background assuming the canonical $\\Lambda$ cold dark matter (CDM) cosmological model have become a new cornerstone of theoretical physics. $\\Lambda_s$CDM is one of the"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2404.17334","kind":"arxiv","version":3},"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/2404.17334/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":"2404.17334","created_at":"2026-07-05T09:32:07.315130+00:00"},{"alias_kind":"arxiv_version","alias_value":"2404.17334v3","created_at":"2026-07-05T09:32:07.315130+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2404.17334","created_at":"2026-07-05T09:32:07.315130+00:00"},{"alias_kind":"pith_short_12","alias_value":"4LKLWVXMZGUJ","created_at":"2026-07-05T09:32:07.315130+00:00"},{"alias_kind":"pith_short_16","alias_value":"4LKLWVXMZGUJFO2X","created_at":"2026-07-05T09:32:07.315130+00:00"},{"alias_kind":"pith_short_8","alias_value":"4LKLWVXM","created_at":"2026-07-05T09:32:07.315130+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":9,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.11062","citing_title":"A Friendly Phantom: Late-time AdS-to-dS transition and cosmological tensions","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2606.06495","citing_title":"What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2","ref_index":99,"is_internal_anchor":false},{"citing_arxiv_id":"2606.31324","citing_title":"Cosmological Viability of Exponential Infrared $f(T)$ Gravity","ref_index":187,"is_internal_anchor":false},{"citing_arxiv_id":"2402.07716","citing_title":"$\\Lambda_{\\rm s}$CDM cosmology from a type-II minimally modified gravity","ref_index":86,"is_internal_anchor":false},{"citing_arxiv_id":"2602.11936","citing_title":"Probing Dynamical Dark Energy with Late-Time Data: Evidence, Tensions, and the Limits of the $w_0w_a$CDM Framework","ref_index":90,"is_internal_anchor":false},{"citing_arxiv_id":"2605.21456","citing_title":"Negative neutrino mass or negative dark energy?","ref_index":85,"is_internal_anchor":false},{"citing_arxiv_id":"2510.18741","citing_title":"Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\\Lambda_{\\rm s}$CDM versus $\\Lambda$CDM","ref_index":191,"is_internal_anchor":false},{"citing_arxiv_id":"2602.12347","citing_title":"Sign-Switching Dark Energy: Smooth Transitions with Recent DESI DR2 Observations","ref_index":101,"is_internal_anchor":false},{"citing_arxiv_id":"2604.12987","citing_title":"Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe?","ref_index":51,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4LKLWVXMZGUJFO2XRZ4YDPKOJS","json":"https://pith.science/pith/4LKLWVXMZGUJFO2XRZ4YDPKOJS.json","graph_json":"https://pith.science/api/pith-number/4LKLWVXMZGUJFO2XRZ4YDPKOJS/graph.json","events_json":"https://pith.science/api/pith-number/4LKLWVXMZGUJFO2XRZ4YDPKOJS/events.json","paper":"https://pith.science/paper/4LKLWVXM"},"agent_actions":{"view_html":"https://pith.science/pith/4LKLWVXMZGUJFO2XRZ4YDPKOJS","download_json":"https://pith.science/pith/4LKLWVXMZGUJFO2XRZ4YDPKOJS.json","view_paper":"https://pith.science/paper/4LKLWVXM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2404.17334&json=true","fetch_graph":"https://pith.science/api/pith-number/4LKLWVXMZGUJFO2XRZ4YDPKOJS/graph.json","fetch_events":"https://pith.science/api/pith-number/4LKLWVXMZGUJFO2XRZ4YDPKOJS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4LKLWVXMZGUJFO2XRZ4YDPKOJS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4LKLWVXMZGUJFO2XRZ4YDPKOJS/action/storage_attestation","attest_author":"https://pith.science/pith/4LKLWVXMZGUJFO2XRZ4YDPKOJS/action/author_attestation","sign_citation":"https://pith.science/pith/4LKLWVXMZGUJFO2XRZ4YDPKOJS/action/citation_signature","submit_replication":"https://pith.science/pith/4LKLWVXMZGUJFO2XRZ4YDPKOJS/action/replication_record"}},"created_at":"2026-07-05T09:32:07.315130+00:00","updated_at":"2026-07-05T09:32:07.315130+00:00"}