{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:ZCJWNL7ZMDUNO7QRPJUDC5RAQU","short_pith_number":"pith:ZCJWNL7Z","schema_version":"1.0","canonical_sha256":"c89366aff960e8d77e117a683176208522041f45219884ad9891b57941b34fdc","source":{"kind":"arxiv","id":"1610.02033","version":3},"attestation_state":"computed","paper":{"title":"Causality Constraints on Massive Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-th","authors_text":"Gustavo Lucena G\\'omez, Rakibur Rahman, Xi\\'an O. Camanho","submitted_at":"2016-10-06T20:00:01Z","abstract_excerpt":"The de Rham-Gabadadze-Tolley massive gravity admits pp-wave backgrounds on which linear fluctuations are shown to undergo time advances for all values of the parameters. The perturbations may propagate in closed time-like curves unless the parameter space is constrained to a line. These classical phenomena take place well within the theory's validity regime."},"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":"1610.02033","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2016-10-06T20:00:01Z","cross_cats_sorted":["astro-ph.CO","gr-qc"],"title_canon_sha256":"0419c84dcd883475d348b1dc4f40dcd1d2a92d9e45f5decb592a171f40026e3e","abstract_canon_sha256":"469a6cf9e26cca071193821708850b22fc10c40dfcc280ee28a1183d4e443753"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:33:10.728780Z","signature_b64":"1dQxjH8YPAOVA0eHB+6cc6duBnR7KWl4pfMG7gVKAQKZzIPuEaMtHeQFaVJ9EGKnnNrnyn0cCJvPYzhiYuDcAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c89366aff960e8d77e117a683176208522041f45219884ad9891b57941b34fdc","last_reissued_at":"2026-05-18T00:33:10.728059Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:33:10.728059Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Causality Constraints on Massive Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-th","authors_text":"Gustavo Lucena G\\'omez, Rakibur Rahman, Xi\\'an O. Camanho","submitted_at":"2016-10-06T20:00:01Z","abstract_excerpt":"The de Rham-Gabadadze-Tolley massive gravity admits pp-wave backgrounds on which linear fluctuations are shown to undergo time advances for all values of the parameters. The perturbations may propagate in closed time-like curves unless the parameter space is constrained to a line. These classical phenomena take place well within the theory's validity regime."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.02033","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":""},"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":"1610.02033","created_at":"2026-05-18T00:33:10.728170+00:00"},{"alias_kind":"arxiv_version","alias_value":"1610.02033v3","created_at":"2026-05-18T00:33:10.728170+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.02033","created_at":"2026-05-18T00:33:10.728170+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZCJWNL7ZMDUN","created_at":"2026-05-18T12:30:53.716459+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZCJWNL7ZMDUNO7QR","created_at":"2026-05-18T12:30:53.716459+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZCJWNL7Z","created_at":"2026-05-18T12:30:53.716459+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.20319","citing_title":"The Equivalence Principle at High Energies Completes the Spectrum","ref_index":40,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ZCJWNL7ZMDUNO7QRPJUDC5RAQU","json":"https://pith.science/pith/ZCJWNL7ZMDUNO7QRPJUDC5RAQU.json","graph_json":"https://pith.science/api/pith-number/ZCJWNL7ZMDUNO7QRPJUDC5RAQU/graph.json","events_json":"https://pith.science/api/pith-number/ZCJWNL7ZMDUNO7QRPJUDC5RAQU/events.json","paper":"https://pith.science/paper/ZCJWNL7Z"},"agent_actions":{"view_html":"https://pith.science/pith/ZCJWNL7ZMDUNO7QRPJUDC5RAQU","download_json":"https://pith.science/pith/ZCJWNL7ZMDUNO7QRPJUDC5RAQU.json","view_paper":"https://pith.science/paper/ZCJWNL7Z","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1610.02033&json=true","fetch_graph":"https://pith.science/api/pith-number/ZCJWNL7ZMDUNO7QRPJUDC5RAQU/graph.json","fetch_events":"https://pith.science/api/pith-number/ZCJWNL7ZMDUNO7QRPJUDC5RAQU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZCJWNL7ZMDUNO7QRPJUDC5RAQU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZCJWNL7ZMDUNO7QRPJUDC5RAQU/action/storage_attestation","attest_author":"https://pith.science/pith/ZCJWNL7ZMDUNO7QRPJUDC5RAQU/action/author_attestation","sign_citation":"https://pith.science/pith/ZCJWNL7ZMDUNO7QRPJUDC5RAQU/action/citation_signature","submit_replication":"https://pith.science/pith/ZCJWNL7ZMDUNO7QRPJUDC5RAQU/action/replication_record"}},"created_at":"2026-05-18T00:33:10.728170+00:00","updated_at":"2026-05-18T00:33:10.728170+00:00"}