{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:PEDIO7XFM7LFLYYTDCVL6445KV","short_pith_number":"pith:PEDIO7XF","canonical_record":{"source":{"id":"1101.0042","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2010-12-30T07:17:53Z","cross_cats_sorted":["astro-ph.CO","hep-th"],"title_canon_sha256":"2f89302cc1d6fe3e223be86e11246cd5392273c6435913c8a594175fcb47a74f","abstract_canon_sha256":"dda34fc44e423ff7f4fe3cefda6d788232308a07cf15b191922b023df1b5dd35"},"schema_version":"1.0"},"canonical_sha256":"7906877ee567d655e31318aabf739d5545f62f37b9fd487fb73bd366fc393d4d","source":{"kind":"arxiv","id":"1101.0042","version":3},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1101.0042","created_at":"2026-05-18T02:23:06Z"},{"alias_kind":"arxiv_version","alias_value":"1101.0042v3","created_at":"2026-05-18T02:23:06Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1101.0042","created_at":"2026-05-18T02:23:06Z"},{"alias_kind":"pith_short_12","alias_value":"PEDIO7XFM7LF","created_at":"2026-05-18T12:26:12Z"},{"alias_kind":"pith_short_16","alias_value":"PEDIO7XFM7LFLYYT","created_at":"2026-05-18T12:26:12Z"},{"alias_kind":"pith_short_8","alias_value":"PEDIO7XF","created_at":"2026-05-18T12:26:12Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:PEDIO7XFM7LFLYYTDCVL6445KV","target":"record","payload":{"canonical_record":{"source":{"id":"1101.0042","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2010-12-30T07:17:53Z","cross_cats_sorted":["astro-ph.CO","hep-th"],"title_canon_sha256":"2f89302cc1d6fe3e223be86e11246cd5392273c6435913c8a594175fcb47a74f","abstract_canon_sha256":"dda34fc44e423ff7f4fe3cefda6d788232308a07cf15b191922b023df1b5dd35"},"schema_version":"1.0"},"canonical_sha256":"7906877ee567d655e31318aabf739d5545f62f37b9fd487fb73bd366fc393d4d","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:23:06.016589Z","signature_b64":"2li04VjiHAhyKhIHmWwme280F6TDi3wv5ySeC1RbzHMsVatB/N9IE75FrmHQbD/Tr7SfLE0BaSzpWxKJN0wTBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7906877ee567d655e31318aabf739d5545f62f37b9fd487fb73bd366fc393d4d","last_reissued_at":"2026-05-18T02:23:06.016053Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:23:06.016053Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1101.0042","source_version":3,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:23:06Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"h1gg2zImMUCVNIXKHNnVZxx5ECSiMkxkm1YbfNNTazKmmZfbxV2teXqxz3j/ZZ05rDJh1afBZ+FBXYqRzZDDAg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T13:21:12.466285Z"},"content_sha256":"2906eafae3f91327ca7fba384cba7f0a1ef4145d2cd2d8b51392ac6bf95170dd","schema_version":"1.0","event_id":"sha256:2906eafae3f91327ca7fba384cba7f0a1ef4145d2cd2d8b51392ac6bf95170dd"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:PEDIO7XFM7LFLYYTDCVL6445KV","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Quasinormal modes of a scalar perturbation coupling with Einstein's tensor in the warped $AdS_3$ black hole spacetime","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"Jiliang Jing, Songbai Chen, Weiping Yao","submitted_at":"2010-12-30T07:17:53Z","abstract_excerpt":"We have studied the quasinormal modes of a massive scalar field coupling to Einstein's tensor in the spacelike stretched $AdS_3$ black hole spacetime. We find that both the right-moving and left-moving quasinormal frequencies depend not only on the warped parameter $v$ of black hole, but also on the coupling between the scalar field and Einstein's tensor. Moreover, we also discuss the warped $AdS/CFT$ correspondence from the quasinormal modes and probe the effects of the coupling on the left and right conformal weights $h_L$ and $h_R$ of the operators dual to the scalar field in the boundary."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1101.0042","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:23:06Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"jexLVnWBoyUMf5X5UhYRw9wD3WKjhma+GP8VOYgBOyIB/BAQ+kHR6X8lGTcG/N8Qy/Ir5jmVy8WPUBLHmP2gDg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T13:21:12.466917Z"},"content_sha256":"e7e61d90f5e708a1b5f986487d0bb24a20b73632014bec34ccd49695abcea05b","schema_version":"1.0","event_id":"sha256:e7e61d90f5e708a1b5f986487d0bb24a20b73632014bec34ccd49695abcea05b"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/PEDIO7XFM7LFLYYTDCVL6445KV/bundle.json","state_url":"https://pith.science/pith/PEDIO7XFM7LFLYYTDCVL6445KV/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/PEDIO7XFM7LFLYYTDCVL6445KV/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-25T13:21:12Z","links":{"resolver":"https://pith.science/pith/PEDIO7XFM7LFLYYTDCVL6445KV","bundle":"https://pith.science/pith/PEDIO7XFM7LFLYYTDCVL6445KV/bundle.json","state":"https://pith.science/pith/PEDIO7XFM7LFLYYTDCVL6445KV/state.json","well_known_bundle":"https://pith.science/.well-known/pith/PEDIO7XFM7LFLYYTDCVL6445KV/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:PEDIO7XFM7LFLYYTDCVL6445KV","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"dda34fc44e423ff7f4fe3cefda6d788232308a07cf15b191922b023df1b5dd35","cross_cats_sorted":["astro-ph.CO","hep-th"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2010-12-30T07:17:53Z","title_canon_sha256":"2f89302cc1d6fe3e223be86e11246cd5392273c6435913c8a594175fcb47a74f"},"schema_version":"1.0","source":{"id":"1101.0042","kind":"arxiv","version":3}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1101.0042","created_at":"2026-05-18T02:23:06Z"},{"alias_kind":"arxiv_version","alias_value":"1101.0042v3","created_at":"2026-05-18T02:23:06Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1101.0042","created_at":"2026-05-18T02:23:06Z"},{"alias_kind":"pith_short_12","alias_value":"PEDIO7XFM7LF","created_at":"2026-05-18T12:26:12Z"},{"alias_kind":"pith_short_16","alias_value":"PEDIO7XFM7LFLYYT","created_at":"2026-05-18T12:26:12Z"},{"alias_kind":"pith_short_8","alias_value":"PEDIO7XF","created_at":"2026-05-18T12:26:12Z"}],"graph_snapshots":[{"event_id":"sha256:e7e61d90f5e708a1b5f986487d0bb24a20b73632014bec34ccd49695abcea05b","target":"graph","created_at":"2026-05-18T02:23:06Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"We have studied the quasinormal modes of a massive scalar field coupling to Einstein's tensor in the spacelike stretched $AdS_3$ black hole spacetime. We find that both the right-moving and left-moving quasinormal frequencies depend not only on the warped parameter $v$ of black hole, but also on the coupling between the scalar field and Einstein's tensor. Moreover, we also discuss the warped $AdS/CFT$ correspondence from the quasinormal modes and probe the effects of the coupling on the left and right conformal weights $h_L$ and $h_R$ of the operators dual to the scalar field in the boundary.","authors_text":"Jiliang Jing, Songbai Chen, Weiping Yao","cross_cats":["astro-ph.CO","hep-th"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2010-12-30T07:17:53Z","title":"Quasinormal modes of a scalar perturbation coupling with Einstein's tensor in the warped $AdS_3$ black hole spacetime"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1101.0042","kind":"arxiv","version":3},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:2906eafae3f91327ca7fba384cba7f0a1ef4145d2cd2d8b51392ac6bf95170dd","target":"record","created_at":"2026-05-18T02:23:06Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"dda34fc44e423ff7f4fe3cefda6d788232308a07cf15b191922b023df1b5dd35","cross_cats_sorted":["astro-ph.CO","hep-th"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2010-12-30T07:17:53Z","title_canon_sha256":"2f89302cc1d6fe3e223be86e11246cd5392273c6435913c8a594175fcb47a74f"},"schema_version":"1.0","source":{"id":"1101.0042","kind":"arxiv","version":3}},"canonical_sha256":"7906877ee567d655e31318aabf739d5545f62f37b9fd487fb73bd366fc393d4d","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"7906877ee567d655e31318aabf739d5545f62f37b9fd487fb73bd366fc393d4d","first_computed_at":"2026-05-18T02:23:06.016053Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:23:06.016053Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"2li04VjiHAhyKhIHmWwme280F6TDi3wv5ySeC1RbzHMsVatB/N9IE75FrmHQbD/Tr7SfLE0BaSzpWxKJN0wTBw==","signature_status":"signed_v1","signed_at":"2026-05-18T02:23:06.016589Z","signed_message":"canonical_sha256_bytes"},"source_id":"1101.0042","source_kind":"arxiv","source_version":3}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:2906eafae3f91327ca7fba384cba7f0a1ef4145d2cd2d8b51392ac6bf95170dd","sha256:e7e61d90f5e708a1b5f986487d0bb24a20b73632014bec34ccd49695abcea05b"],"state_sha256":"92c3979699dc7456493c8383d3c3ad27201b0aba41ba90865d864d8acdcc2780"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"oFF/D/yjlelFRMTFuojof69KeEtBurmaON/NK3qPy0MUOHaBBXWZVJYfGhkeeuobWCmVYuZorEhd00Zr7oguCg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-25T13:21:12.469671Z","bundle_sha256":"5f7b3a6dbee66787bcb810713549a82d0ff4dc5eec7efbd1df8f6453090f86aa"}}