{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:OKAMPDVP3VL6XVUQMNBSZBZWIM","short_pith_number":"pith:OKAMPDVP","schema_version":"1.0","canonical_sha256":"7280c78eafdd57ebd69063432c87364336ace4b27bd927e7ac6dc2e137a40307","source":{"kind":"arxiv","id":"1712.03148","version":2},"attestation_state":"computed","paper":{"title":"Search for sterile neutrinos in a universe of vacuum energy interacting with cold dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Jing-Fei Zhang, Lu Feng, Xin Zhang","submitted_at":"2017-12-08T16:15:44Z","abstract_excerpt":"We investigate the cosmological constraints on sterile neutrinos in a universe in which vacuum energy interacts with cold dark matter by using latest observational data. We focus on two specific interaction models, $Q=\\beta H\\rho_{\\rm v}$ and $Q=\\beta H\\rho_{\\rm c}$. To overcome the problem of large-scale instability in the interacting dark energy scenario, we employ the parametrized post-Friedmann (PPF) approach for interacting dark energy to do the calculation of perturbation evolution. The observational data sets used in this work include the Planck 2015 temperature and polarization data, t"},"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":"1712.03148","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-12-08T16:15:44Z","cross_cats_sorted":["gr-qc","hep-ph"],"title_canon_sha256":"bc23599d3384daf049b8f897ef12807f49963f862badfb6309a08e7a6ef57443","abstract_canon_sha256":"4d57c7984c29f9d16ae2c12946924f3ffc426096abe92d2efd7efbde921eeaa4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:56:48.484915Z","signature_b64":"HARk5p03SiSfHSNjO8Jqy104DbVCU7IO6C9WE364fjDrKNhWdcLcT8/RC3sGZTrtgno9FxlIw0ycPheVCTLxAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7280c78eafdd57ebd69063432c87364336ace4b27bd927e7ac6dc2e137a40307","last_reissued_at":"2026-05-17T23:56:48.484548Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:56:48.484548Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Search for sterile neutrinos in a universe of vacuum energy interacting with cold dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Jing-Fei Zhang, Lu Feng, Xin Zhang","submitted_at":"2017-12-08T16:15:44Z","abstract_excerpt":"We investigate the cosmological constraints on sterile neutrinos in a universe in which vacuum energy interacts with cold dark matter by using latest observational data. We focus on two specific interaction models, $Q=\\beta H\\rho_{\\rm v}$ and $Q=\\beta H\\rho_{\\rm c}$. To overcome the problem of large-scale instability in the interacting dark energy scenario, we employ the parametrized post-Friedmann (PPF) approach for interacting dark energy to do the calculation of perturbation evolution. The observational data sets used in this work include the Planck 2015 temperature and polarization data, t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1712.03148","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":"1712.03148","created_at":"2026-05-17T23:56:48.484601+00:00"},{"alias_kind":"arxiv_version","alias_value":"1712.03148v2","created_at":"2026-05-17T23:56:48.484601+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1712.03148","created_at":"2026-05-17T23:56:48.484601+00:00"},{"alias_kind":"pith_short_12","alias_value":"OKAMPDVP3VL6","created_at":"2026-05-18T12:31:34.259226+00:00"},{"alias_kind":"pith_short_16","alias_value":"OKAMPDVP3VL6XVUQ","created_at":"2026-05-18T12:31:34.259226+00:00"},{"alias_kind":"pith_short_8","alias_value":"OKAMPDVP","created_at":"2026-05-18T12:31:34.259226+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2605.21310","citing_title":"Contrastive self-supervised convolutional autoencoder for core-collapse supernova gravitational-wave detection","ref_index":40,"is_internal_anchor":true},{"citing_arxiv_id":"2603.10787","citing_title":"Measuring neutrino mass in light of ACT DR6 and DESI DR2","ref_index":33,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OKAMPDVP3VL6XVUQMNBSZBZWIM","json":"https://pith.science/pith/OKAMPDVP3VL6XVUQMNBSZBZWIM.json","graph_json":"https://pith.science/api/pith-number/OKAMPDVP3VL6XVUQMNBSZBZWIM/graph.json","events_json":"https://pith.science/api/pith-number/OKAMPDVP3VL6XVUQMNBSZBZWIM/events.json","paper":"https://pith.science/paper/OKAMPDVP"},"agent_actions":{"view_html":"https://pith.science/pith/OKAMPDVP3VL6XVUQMNBSZBZWIM","download_json":"https://pith.science/pith/OKAMPDVP3VL6XVUQMNBSZBZWIM.json","view_paper":"https://pith.science/paper/OKAMPDVP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1712.03148&json=true","fetch_graph":"https://pith.science/api/pith-number/OKAMPDVP3VL6XVUQMNBSZBZWIM/graph.json","fetch_events":"https://pith.science/api/pith-number/OKAMPDVP3VL6XVUQMNBSZBZWIM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OKAMPDVP3VL6XVUQMNBSZBZWIM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OKAMPDVP3VL6XVUQMNBSZBZWIM/action/storage_attestation","attest_author":"https://pith.science/pith/OKAMPDVP3VL6XVUQMNBSZBZWIM/action/author_attestation","sign_citation":"https://pith.science/pith/OKAMPDVP3VL6XVUQMNBSZBZWIM/action/citation_signature","submit_replication":"https://pith.science/pith/OKAMPDVP3VL6XVUQMNBSZBZWIM/action/replication_record"}},"created_at":"2026-05-17T23:56:48.484601+00:00","updated_at":"2026-05-17T23:56:48.484601+00:00"}