{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:Z3U2D6465XZ6UUPGBXBPMPFQWL","short_pith_number":"pith:Z3U2D646","schema_version":"1.0","canonical_sha256":"cee9a1fb9eedf3ea51e60dc2f63cb0b2fd9c99287b466d7a7f8c4aba9da3cefc","source":{"kind":"arxiv","id":"2405.11790","version":1},"attestation_state":"computed","paper":{"title":"Graviton physics: Quantum field theory of gravitons, graviton noise and gravitational decoherence -- a concise tutorial","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","quant-ph"],"primary_cat":"hep-th","authors_text":"Bei-Lok Hu, Hing-Tong Cho, Jen-Tsung Hsiang","submitted_at":"2024-05-20T05:16:12Z","abstract_excerpt":"The detection of gravitational waves in 2015 ushered in a new era of gravitational wave astronomy capable of probing into the strong field dynamics of black holes and neutron stars. It has opened up an exciting new window for laboratory and space tests of Einstein's theory of classical general relativity. In recent years there are two interesting proposals aimed at revealing the quantum natures of perturbative gravity: 1) theoretical predictions in how graviton noise from the early universe after the vacuum of the gravitational field was strongly squeezed by inflationary expansion; 2) experime"},"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":"2405.11790","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2024-05-20T05:16:12Z","cross_cats_sorted":["gr-qc","quant-ph"],"title_canon_sha256":"62c7df88ee79ee252d7e82e67094863ef210e19f3c2a7ed462af176564422a10","abstract_canon_sha256":"751adf23c181e12573f5741d9890785fe105dc82efbbc512fb9bd20b68bb8e54"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:19:09.694278Z","signature_b64":"SffuzXBMdRoyhVJYwetKwkku8bth98vBhTFiKv6CwosTFrOon/9z2FRv14wWG8WdZyqRphZFhqnEv1Ipk07hDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cee9a1fb9eedf3ea51e60dc2f63cb0b2fd9c99287b466d7a7f8c4aba9da3cefc","last_reissued_at":"2026-07-05T09:19:09.693833Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:19:09.693833Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Graviton physics: Quantum field theory of gravitons, graviton noise and gravitational decoherence -- a concise tutorial","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","quant-ph"],"primary_cat":"hep-th","authors_text":"Bei-Lok Hu, Hing-Tong Cho, Jen-Tsung Hsiang","submitted_at":"2024-05-20T05:16:12Z","abstract_excerpt":"The detection of gravitational waves in 2015 ushered in a new era of gravitational wave astronomy capable of probing into the strong field dynamics of black holes and neutron stars. It has opened up an exciting new window for laboratory and space tests of Einstein's theory of classical general relativity. In recent years there are two interesting proposals aimed at revealing the quantum natures of perturbative gravity: 1) theoretical predictions in how graviton noise from the early universe after the vacuum of the gravitational field was strongly squeezed by inflationary expansion; 2) experime"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2405.11790","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/2405.11790/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":"2405.11790","created_at":"2026-07-05T09:19:09.693889+00:00"},{"alias_kind":"arxiv_version","alias_value":"2405.11790v1","created_at":"2026-07-05T09:19:09.693889+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2405.11790","created_at":"2026-07-05T09:19:09.693889+00:00"},{"alias_kind":"pith_short_12","alias_value":"Z3U2D6465XZ6","created_at":"2026-07-05T09:19:09.693889+00:00"},{"alias_kind":"pith_short_16","alias_value":"Z3U2D6465XZ6UUPG","created_at":"2026-07-05T09:19:09.693889+00:00"},{"alias_kind":"pith_short_8","alias_value":"Z3U2D646","created_at":"2026-07-05T09:19:09.693889+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.05916","citing_title":"Squeezed Gravitons and One-Loop Self-Energy under Light-Cone Smearing","ref_index":14,"is_internal_anchor":false},{"citing_arxiv_id":"2601.17849","citing_title":"Geometric noise spectrum in interferometers","ref_index":69,"is_internal_anchor":false},{"citing_arxiv_id":"2601.03214","citing_title":"When does entanglement through gravity imply gravitons?","ref_index":20,"is_internal_anchor":false},{"citing_arxiv_id":"2605.05916","citing_title":"Squeezed Gravitons and One-Loop Self-Energy under Light-Cone Smearing","ref_index":14,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/Z3U2D6465XZ6UUPGBXBPMPFQWL","json":"https://pith.science/pith/Z3U2D6465XZ6UUPGBXBPMPFQWL.json","graph_json":"https://pith.science/api/pith-number/Z3U2D6465XZ6UUPGBXBPMPFQWL/graph.json","events_json":"https://pith.science/api/pith-number/Z3U2D6465XZ6UUPGBXBPMPFQWL/events.json","paper":"https://pith.science/paper/Z3U2D646"},"agent_actions":{"view_html":"https://pith.science/pith/Z3U2D6465XZ6UUPGBXBPMPFQWL","download_json":"https://pith.science/pith/Z3U2D6465XZ6UUPGBXBPMPFQWL.json","view_paper":"https://pith.science/paper/Z3U2D646","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2405.11790&json=true","fetch_graph":"https://pith.science/api/pith-number/Z3U2D6465XZ6UUPGBXBPMPFQWL/graph.json","fetch_events":"https://pith.science/api/pith-number/Z3U2D6465XZ6UUPGBXBPMPFQWL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Z3U2D6465XZ6UUPGBXBPMPFQWL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Z3U2D6465XZ6UUPGBXBPMPFQWL/action/storage_attestation","attest_author":"https://pith.science/pith/Z3U2D6465XZ6UUPGBXBPMPFQWL/action/author_attestation","sign_citation":"https://pith.science/pith/Z3U2D6465XZ6UUPGBXBPMPFQWL/action/citation_signature","submit_replication":"https://pith.science/pith/Z3U2D6465XZ6UUPGBXBPMPFQWL/action/replication_record"}},"created_at":"2026-07-05T09:19:09.693889+00:00","updated_at":"2026-07-05T09:19:09.693889+00:00"}