{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:NUB4NT45PLDNJU5SJKZSGB4H6J","short_pith_number":"pith:NUB4NT45","schema_version":"1.0","canonical_sha256":"6d03c6cf9d7ac6d4d3b24ab3230787f26128b70776f93744273c7b9699637447","source":{"kind":"arxiv","id":"1810.09934","version":3},"attestation_state":"computed","paper":{"title":"Inflationary Cosmology: From Theory to Observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"astro-ph.CO","authors_text":"J. Alberto Vazquez, Luis E. Padilla, Tonatiuh Matos","submitted_at":"2018-10-10T06:38:16Z","abstract_excerpt":"The main aim of this paper is to provide a qualitative introduction to the cosmic inflation and its relationship with current cosmological observations. The inflationary model solves many of the fundamental problems that challenge the Standard Big Bang cosmology i.e. Flatness, Horizon and Monopole problem, and additionally provides an explanation for the initial conditions observed throughout the Large-Scale Structure of the Universe, such as galaxies. In this review we describe the general solutions carry out by a single scalar field. Then with the use of current surveys, we show the constrai"},"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":"1810.09934","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2018-10-10T06:38:16Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"28556d1fbeb0bbeb0f9e4f73bf4a9b4b2d8adbdc3afc706bebb1a174d1b60953","abstract_canon_sha256":"1a6154285f1ff8a2a61e6a4b7cf184d9f3e61228eed3d1a961017fd37a5098d1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:43:15.521179Z","signature_b64":"kc3Jyf/+uAkAOplnXNNBPFkBChandAcfIPRShybo+wjO8XdgUCrdGavnOO9cJ4BE00PFG/9BiZTgT9Txv5CfBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6d03c6cf9d7ac6d4d3b24ab3230787f26128b70776f93744273c7b9699637447","last_reissued_at":"2026-07-05T03:43:15.520788Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:43:15.520788Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Inflationary Cosmology: From Theory to Observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"astro-ph.CO","authors_text":"J. Alberto Vazquez, Luis E. Padilla, Tonatiuh Matos","submitted_at":"2018-10-10T06:38:16Z","abstract_excerpt":"The main aim of this paper is to provide a qualitative introduction to the cosmic inflation and its relationship with current cosmological observations. The inflationary model solves many of the fundamental problems that challenge the Standard Big Bang cosmology i.e. Flatness, Horizon and Monopole problem, and additionally provides an explanation for the initial conditions observed throughout the Large-Scale Structure of the Universe, such as galaxies. In this review we describe the general solutions carry out by a single scalar field. Then with the use of current surveys, we show the constrai"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1810.09934","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1810.09934/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":"1810.09934","created_at":"2026-07-05T03:43:15.520840+00:00"},{"alias_kind":"arxiv_version","alias_value":"1810.09934v3","created_at":"2026-07-05T03:43:15.520840+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1810.09934","created_at":"2026-07-05T03:43:15.520840+00:00"},{"alias_kind":"pith_short_12","alias_value":"NUB4NT45PLDN","created_at":"2026-07-05T03:43:15.520840+00:00"},{"alias_kind":"pith_short_16","alias_value":"NUB4NT45PLDNJU5S","created_at":"2026-07-05T03:43:15.520840+00:00"},{"alias_kind":"pith_short_8","alias_value":"NUB4NT45","created_at":"2026-07-05T03:43:15.520840+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.23990","citing_title":"Hamilton-Jacobi Approach to Inflationary Scenarios through Extended Entropies: An Observational Perspective","ref_index":84,"is_internal_anchor":false},{"citing_arxiv_id":"2604.26191","citing_title":"Gravitational Properties of the Monopole Bag","ref_index":2,"is_internal_anchor":false},{"citing_arxiv_id":"2604.26191","citing_title":"Gravitational Properties of the Monopole Bag","ref_index":2,"is_internal_anchor":false},{"citing_arxiv_id":"2604.10148","citing_title":"An Analytic Formalism of Inflation for Derivative Coupled Scalar Field and Validating its predictions for Some Inflationary Potentials","ref_index":5,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NUB4NT45PLDNJU5SJKZSGB4H6J","json":"https://pith.science/pith/NUB4NT45PLDNJU5SJKZSGB4H6J.json","graph_json":"https://pith.science/api/pith-number/NUB4NT45PLDNJU5SJKZSGB4H6J/graph.json","events_json":"https://pith.science/api/pith-number/NUB4NT45PLDNJU5SJKZSGB4H6J/events.json","paper":"https://pith.science/paper/NUB4NT45"},"agent_actions":{"view_html":"https://pith.science/pith/NUB4NT45PLDNJU5SJKZSGB4H6J","download_json":"https://pith.science/pith/NUB4NT45PLDNJU5SJKZSGB4H6J.json","view_paper":"https://pith.science/paper/NUB4NT45","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1810.09934&json=true","fetch_graph":"https://pith.science/api/pith-number/NUB4NT45PLDNJU5SJKZSGB4H6J/graph.json","fetch_events":"https://pith.science/api/pith-number/NUB4NT45PLDNJU5SJKZSGB4H6J/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NUB4NT45PLDNJU5SJKZSGB4H6J/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NUB4NT45PLDNJU5SJKZSGB4H6J/action/storage_attestation","attest_author":"https://pith.science/pith/NUB4NT45PLDNJU5SJKZSGB4H6J/action/author_attestation","sign_citation":"https://pith.science/pith/NUB4NT45PLDNJU5SJKZSGB4H6J/action/citation_signature","submit_replication":"https://pith.science/pith/NUB4NT45PLDNJU5SJKZSGB4H6J/action/replication_record"}},"created_at":"2026-07-05T03:43:15.520840+00:00","updated_at":"2026-07-05T03:43:15.520840+00:00"}