{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:EW63V6RZK4XYAUZ63CBENOMDVR","short_pith_number":"pith:EW63V6RZ","schema_version":"1.0","canonical_sha256":"25bdbafa39572f80533ed88246b983ac6a5dae421a54ed7b23a0dd9386b6d611","source":{"kind":"arxiv","id":"2209.07167","version":2},"attestation_state":"computed","paper":{"title":"Forecast Analysis on Interacting Dark Energy Models from Future Generation PICO and DESI Missions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Albin Joseph, Rajib Saha","submitted_at":"2022-09-15T09:37:15Z","abstract_excerpt":"The next-generation CMB satellite missions are expected to provide robust constraints on a wide range of cosmological parameters with unprecedented precision. But these constraints on the parameters could weaken if we do not attribute dark energy to a cosmological constant. The cosmological models involving interaction between dark energy and dark matter can give rise to comparable energy densities at the present epoch, thereby alleviating the so-called cosmic coincidence problem. In the present paper, we perform a forecast analysis to test the ability of the future generation high-sensitive C"},"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":"2209.07167","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2022-09-15T09:37:15Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"00052e9e2056d9d786d75fbb3e90d98e480c91194be2e67523baf85d25e23c36","abstract_canon_sha256":"eeb9b265cadbf95586c759588214e14158976fb6b7c543112343d93b8a1d5407"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:24:14.000977Z","signature_b64":"Eug9AqY2gACPBHFxkbUg7dRERyGOQ6ZKTE4bQmlU44nCyGqPd+0wl+zow6KG2RXiwGKOgvybDMFicNpexpSHDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"25bdbafa39572f80533ed88246b983ac6a5dae421a54ed7b23a0dd9386b6d611","last_reissued_at":"2026-07-05T05:24:14.000571Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:24:14.000571Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Forecast Analysis on Interacting Dark Energy Models from Future Generation PICO and DESI Missions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Albin Joseph, Rajib Saha","submitted_at":"2022-09-15T09:37:15Z","abstract_excerpt":"The next-generation CMB satellite missions are expected to provide robust constraints on a wide range of cosmological parameters with unprecedented precision. But these constraints on the parameters could weaken if we do not attribute dark energy to a cosmological constant. The cosmological models involving interaction between dark energy and dark matter can give rise to comparable energy densities at the present epoch, thereby alleviating the so-called cosmic coincidence problem. In the present paper, we perform a forecast analysis to test the ability of the future generation high-sensitive C"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2209.07167","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2209.07167/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":"2209.07167","created_at":"2026-07-05T05:24:14.000626+00:00"},{"alias_kind":"arxiv_version","alias_value":"2209.07167v2","created_at":"2026-07-05T05:24:14.000626+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2209.07167","created_at":"2026-07-05T05:24:14.000626+00:00"},{"alias_kind":"pith_short_12","alias_value":"EW63V6RZK4XY","created_at":"2026-07-05T05:24:14.000626+00:00"},{"alias_kind":"pith_short_16","alias_value":"EW63V6RZK4XYAUZ6","created_at":"2026-07-05T05:24:14.000626+00:00"},{"alias_kind":"pith_short_8","alias_value":"EW63V6RZ","created_at":"2026-07-05T05:24:14.000626+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.11368","citing_title":"Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies","ref_index":56,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EW63V6RZK4XYAUZ63CBENOMDVR","json":"https://pith.science/pith/EW63V6RZK4XYAUZ63CBENOMDVR.json","graph_json":"https://pith.science/api/pith-number/EW63V6RZK4XYAUZ63CBENOMDVR/graph.json","events_json":"https://pith.science/api/pith-number/EW63V6RZK4XYAUZ63CBENOMDVR/events.json","paper":"https://pith.science/paper/EW63V6RZ"},"agent_actions":{"view_html":"https://pith.science/pith/EW63V6RZK4XYAUZ63CBENOMDVR","download_json":"https://pith.science/pith/EW63V6RZK4XYAUZ63CBENOMDVR.json","view_paper":"https://pith.science/paper/EW63V6RZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2209.07167&json=true","fetch_graph":"https://pith.science/api/pith-number/EW63V6RZK4XYAUZ63CBENOMDVR/graph.json","fetch_events":"https://pith.science/api/pith-number/EW63V6RZK4XYAUZ63CBENOMDVR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EW63V6RZK4XYAUZ63CBENOMDVR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EW63V6RZK4XYAUZ63CBENOMDVR/action/storage_attestation","attest_author":"https://pith.science/pith/EW63V6RZK4XYAUZ63CBENOMDVR/action/author_attestation","sign_citation":"https://pith.science/pith/EW63V6RZK4XYAUZ63CBENOMDVR/action/citation_signature","submit_replication":"https://pith.science/pith/EW63V6RZK4XYAUZ63CBENOMDVR/action/replication_record"}},"created_at":"2026-07-05T05:24:14.000626+00:00","updated_at":"2026-07-05T05:24:14.000626+00:00"}