{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:VUK6H3LRCQNLRSBX226UKAWRB5","short_pith_number":"pith:VUK6H3LR","schema_version":"1.0","canonical_sha256":"ad15e3ed71141ab8c837d6bd4502d10f59f1abef605096bb0a276363d421b231","source":{"kind":"arxiv","id":"1004.3962","version":2},"attestation_state":"computed","paper":{"title":"Brane-World Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-th","authors_text":"Kazuya Koyama (ICG, Portsmouth), Roy Maartens (ICG","submitted_at":"2010-04-22T17:08:31Z","abstract_excerpt":"The observable universe could be a 1+3-surface (the \"brane\") embedded in a 1+3+\\textit{d}-dimensional spacetime (the \"bulk\"), with Standard Model particles and fields trapped on the brane while gravity is free to access the bulk. At least one of the \\textit{d} extra spatial dimensions could be very large relative to the Planck scale, which lowers the fundamental gravity scale, possibly even down to the electroweak ($\\sim$ TeV) level. This revolutionary picture arises in the framework of recent developments in M theory. The 1+10-dimensional M theory encompasses the known 1+9-dimensional superst"},"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":"1004.3962","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2010-04-22T17:08:31Z","cross_cats_sorted":["astro-ph.CO","gr-qc"],"title_canon_sha256":"a2506427fdc3d5498c0cb2896ad35d3846f8d37c0781c5ebbec9a21f922f1970","abstract_canon_sha256":"85562215792457e6aba2b7617055682cbe581b7a29e6909763a07b1db9c0a441"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:07:54.974608Z","signature_b64":"QtczPTGoSjRebgdMJILaoh16Ls2gWjClUJEESp2YXc+VuYrXOGLy7WluFYIRvSKEIF2zYtmfI5KCpKAYCVQfAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ad15e3ed71141ab8c837d6bd4502d10f59f1abef605096bb0a276363d421b231","last_reissued_at":"2026-05-18T02:07:54.973910Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:07:54.973910Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Brane-World Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-th","authors_text":"Kazuya Koyama (ICG, Portsmouth), Roy Maartens (ICG","submitted_at":"2010-04-22T17:08:31Z","abstract_excerpt":"The observable universe could be a 1+3-surface (the \"brane\") embedded in a 1+3+\\textit{d}-dimensional spacetime (the \"bulk\"), with Standard Model particles and fields trapped on the brane while gravity is free to access the bulk. At least one of the \\textit{d} extra spatial dimensions could be very large relative to the Planck scale, which lowers the fundamental gravity scale, possibly even down to the electroweak ($\\sim$ TeV) level. This revolutionary picture arises in the framework of recent developments in M theory. The 1+10-dimensional M theory encompasses the known 1+9-dimensional superst"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1004.3962","kind":"arxiv","version":2},"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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1004.3962","created_at":"2026-05-18T02:07:54.974017+00:00"},{"alias_kind":"arxiv_version","alias_value":"1004.3962v2","created_at":"2026-05-18T02:07:54.974017+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1004.3962","created_at":"2026-05-18T02:07:54.974017+00:00"},{"alias_kind":"pith_short_12","alias_value":"VUK6H3LRCQNL","created_at":"2026-05-18T12:26:15.391820+00:00"},{"alias_kind":"pith_short_16","alias_value":"VUK6H3LRCQNLRSBX","created_at":"2026-05-18T12:26:15.391820+00:00"},{"alias_kind":"pith_short_8","alias_value":"VUK6H3LR","created_at":"2026-05-18T12:26:15.391820+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.08907","citing_title":"The Status of Gravitational Vector Perturbations with Recent CMB Data","ref_index":62,"is_internal_anchor":false},{"citing_arxiv_id":"2604.07858","citing_title":"Quasinormal modes of the thick braneworld in $f(T)$ gravity","ref_index":41,"is_internal_anchor":false},{"citing_arxiv_id":"2604.04601","citing_title":"Cosmic Inflation From Regular Black Holes","ref_index":62,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VUK6H3LRCQNLRSBX226UKAWRB5","json":"https://pith.science/pith/VUK6H3LRCQNLRSBX226UKAWRB5.json","graph_json":"https://pith.science/api/pith-number/VUK6H3LRCQNLRSBX226UKAWRB5/graph.json","events_json":"https://pith.science/api/pith-number/VUK6H3LRCQNLRSBX226UKAWRB5/events.json","paper":"https://pith.science/paper/VUK6H3LR"},"agent_actions":{"view_html":"https://pith.science/pith/VUK6H3LRCQNLRSBX226UKAWRB5","download_json":"https://pith.science/pith/VUK6H3LRCQNLRSBX226UKAWRB5.json","view_paper":"https://pith.science/paper/VUK6H3LR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1004.3962&json=true","fetch_graph":"https://pith.science/api/pith-number/VUK6H3LRCQNLRSBX226UKAWRB5/graph.json","fetch_events":"https://pith.science/api/pith-number/VUK6H3LRCQNLRSBX226UKAWRB5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VUK6H3LRCQNLRSBX226UKAWRB5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VUK6H3LRCQNLRSBX226UKAWRB5/action/storage_attestation","attest_author":"https://pith.science/pith/VUK6H3LRCQNLRSBX226UKAWRB5/action/author_attestation","sign_citation":"https://pith.science/pith/VUK6H3LRCQNLRSBX226UKAWRB5/action/citation_signature","submit_replication":"https://pith.science/pith/VUK6H3LRCQNLRSBX226UKAWRB5/action/replication_record"}},"created_at":"2026-05-18T02:07:54.974017+00:00","updated_at":"2026-05-18T02:07:54.974017+00:00"}