{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2005:V576ABRRV2XNCEIECJJHTGHFOO","short_pith_number":"pith:V576ABRR","schema_version":"1.0","canonical_sha256":"af7fe00631aeaed1110412527998e573a849cc11479e379f92233779bc8c69e0","source":{"kind":"arxiv","id":"gr-qc/0502084","version":1},"attestation_state":"computed","paper":{"title":"Wormholes supported by a phantom energy","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"S. V. Sushkov","submitted_at":"2005-02-21T13:11:39Z","abstract_excerpt":"We extend the notion of phantom energy--which is generally accepted for homogeneously distributed matter with $w<-1$ in the universe--on inhomogeneous spherically symmetric spacetime configurations. A spherically symmetric distribution of phantom energy is shown to be able to support the existence of static wormholes. We find an exact solution describing a static spherically symmetric wormhole with phantom energy and show that a spatial distribution of the phantom energy is mainly restricted by the vicinity of the wormhole's throat. The maximal size of the spherical region, surrounding the thr"},"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":"gr-qc/0502084","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"2005-02-21T13:11:39Z","cross_cats_sorted":[],"title_canon_sha256":"c126c6411e9b623df01d89fac034942ac3517c764ade4cd5b5175ff42aa79b8f","abstract_canon_sha256":"5fad30bd695f2e51044cc53b39b6d13a0711a5a3aa4d5d9b26a71d971ccf3de2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:55:10.424704Z","signature_b64":"ZtQHQOKzUBjGzzIhOeHx9oZDSKu8Mwd0Yy9weXS2KVjQtwCwFMvp/DP/IL0LIuqXj3gQDRLSz0dxAlFlkPDLCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"af7fe00631aeaed1110412527998e573a849cc11479e379f92233779bc8c69e0","last_reissued_at":"2026-07-04T16:55:10.424374Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:55:10.424374Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Wormholes supported by a phantom energy","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"S. V. Sushkov","submitted_at":"2005-02-21T13:11:39Z","abstract_excerpt":"We extend the notion of phantom energy--which is generally accepted for homogeneously distributed matter with $w<-1$ in the universe--on inhomogeneous spherically symmetric spacetime configurations. A spherically symmetric distribution of phantom energy is shown to be able to support the existence of static wormholes. We find an exact solution describing a static spherically symmetric wormhole with phantom energy and show that a spatial distribution of the phantom energy is mainly restricted by the vicinity of the wormhole's throat. The maximal size of the spherical region, surrounding the thr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/0502084","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/gr-qc/0502084/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":"gr-qc/0502084","created_at":"2026-07-04T16:55:10.424428+00:00"},{"alias_kind":"arxiv_version","alias_value":"gr-qc/0502084v1","created_at":"2026-07-04T16:55:10.424428+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.gr-qc/0502084","created_at":"2026-07-04T16:55:10.424428+00:00"},{"alias_kind":"pith_short_12","alias_value":"V576ABRRV2XN","created_at":"2026-07-04T16:55:10.424428+00:00"},{"alias_kind":"pith_short_16","alias_value":"V576ABRRV2XNCEIE","created_at":"2026-07-04T16:55:10.424428+00:00"},{"alias_kind":"pith_short_8","alias_value":"V576ABRR","created_at":"2026-07-04T16:55:10.424428+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2606.00178","citing_title":"Traversable Wormholes Supported by Entropy-Inspired Effective Matter Sectors","ref_index":29,"is_internal_anchor":true},{"citing_arxiv_id":"2505.22066","citing_title":"Cosmic Strings as Dynamical Dark Energy: Novel Constraints","ref_index":42,"is_internal_anchor":true},{"citing_arxiv_id":"2602.14182","citing_title":"On the Cuspy Structure of Rotating Wormhole Shadows","ref_index":34,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/V576ABRRV2XNCEIECJJHTGHFOO","json":"https://pith.science/pith/V576ABRRV2XNCEIECJJHTGHFOO.json","graph_json":"https://pith.science/api/pith-number/V576ABRRV2XNCEIECJJHTGHFOO/graph.json","events_json":"https://pith.science/api/pith-number/V576ABRRV2XNCEIECJJHTGHFOO/events.json","paper":"https://pith.science/paper/V576ABRR"},"agent_actions":{"view_html":"https://pith.science/pith/V576ABRRV2XNCEIECJJHTGHFOO","download_json":"https://pith.science/pith/V576ABRRV2XNCEIECJJHTGHFOO.json","view_paper":"https://pith.science/paper/V576ABRR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=gr-qc/0502084&json=true","fetch_graph":"https://pith.science/api/pith-number/V576ABRRV2XNCEIECJJHTGHFOO/graph.json","fetch_events":"https://pith.science/api/pith-number/V576ABRRV2XNCEIECJJHTGHFOO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/V576ABRRV2XNCEIECJJHTGHFOO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/V576ABRRV2XNCEIECJJHTGHFOO/action/storage_attestation","attest_author":"https://pith.science/pith/V576ABRRV2XNCEIECJJHTGHFOO/action/author_attestation","sign_citation":"https://pith.science/pith/V576ABRRV2XNCEIECJJHTGHFOO/action/citation_signature","submit_replication":"https://pith.science/pith/V576ABRRV2XNCEIECJJHTGHFOO/action/replication_record"}},"created_at":"2026-07-04T16:55:10.424428+00:00","updated_at":"2026-07-04T16:55:10.424428+00:00"}