{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:LM6RJ5N2SSAKM2DKKWEAHIFHX3","short_pith_number":"pith:LM6RJ5N2","schema_version":"1.0","canonical_sha256":"5b3d14f5ba9480a6686a558803a0a7beca479f1b5f421bf88f94f99fb4eb0638","source":{"kind":"arxiv","id":"1710.05784","version":1},"attestation_state":"computed","paper":{"title":"Can an Axion be the Dark Energy particle ?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"Elias C. Vagenas","submitted_at":"2017-10-16T15:41:36Z","abstract_excerpt":"Following a phenomenological analysis done by the late Martin Perl for the detection of the dark energy, we show that an axion of energy $1.5\\times 10^{-3}~eV/c^2$ can be a viable candidate for the dark energy particle. In particular, we obtain the characteristic length and frequency of the axion as a quantum particle. Then, employing a relation that connects the energy density with the frequency of a particle, i.e., $\\rho\\sim f^{4}$, we show that the energy density of axions, with the aforesaid value of mass, as obtained from our theoretical analysis is proportional to the dark energy density"},"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":"1710.05784","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2017-10-16T15:41:36Z","cross_cats_sorted":["astro-ph.CO","hep-th"],"title_canon_sha256":"7c385b18a2298716af718387d4d04c83b7873409bae7b405aed3453cbe165e31","abstract_canon_sha256":"8cc3b8e734ef6e55371a76a009077afec525cad2c9e299b9e2e3f53547216107"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:06:51.067636Z","signature_b64":"gNPQM3IAJPcANyLbL3/dSQO2xccTs/W/EnB2pVCFiarIdYYlHswu8Z4E29Kpaakvycl1CHfl6jsrbyCgj4CoBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5b3d14f5ba9480a6686a558803a0a7beca479f1b5f421bf88f94f99fb4eb0638","last_reissued_at":"2026-05-18T00:06:51.067007Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:06:51.067007Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Can an Axion be the Dark Energy particle ?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"Elias C. Vagenas","submitted_at":"2017-10-16T15:41:36Z","abstract_excerpt":"Following a phenomenological analysis done by the late Martin Perl for the detection of the dark energy, we show that an axion of energy $1.5\\times 10^{-3}~eV/c^2$ can be a viable candidate for the dark energy particle. In particular, we obtain the characteristic length and frequency of the axion as a quantum particle. Then, employing a relation that connects the energy density with the frequency of a particle, i.e., $\\rho\\sim f^{4}$, we show that the energy density of axions, with the aforesaid value of mass, as obtained from our theoretical analysis is proportional to the dark energy density"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1710.05784","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":""},"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":"1710.05784","created_at":"2026-05-18T00:06:51.067090+00:00"},{"alias_kind":"arxiv_version","alias_value":"1710.05784v1","created_at":"2026-05-18T00:06:51.067090+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1710.05784","created_at":"2026-05-18T00:06:51.067090+00:00"},{"alias_kind":"pith_short_12","alias_value":"LM6RJ5N2SSAK","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_16","alias_value":"LM6RJ5N2SSAKM2DK","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_8","alias_value":"LM6RJ5N2","created_at":"2026-05-18T12:31:28.150371+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LM6RJ5N2SSAKM2DKKWEAHIFHX3","json":"https://pith.science/pith/LM6RJ5N2SSAKM2DKKWEAHIFHX3.json","graph_json":"https://pith.science/api/pith-number/LM6RJ5N2SSAKM2DKKWEAHIFHX3/graph.json","events_json":"https://pith.science/api/pith-number/LM6RJ5N2SSAKM2DKKWEAHIFHX3/events.json","paper":"https://pith.science/paper/LM6RJ5N2"},"agent_actions":{"view_html":"https://pith.science/pith/LM6RJ5N2SSAKM2DKKWEAHIFHX3","download_json":"https://pith.science/pith/LM6RJ5N2SSAKM2DKKWEAHIFHX3.json","view_paper":"https://pith.science/paper/LM6RJ5N2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1710.05784&json=true","fetch_graph":"https://pith.science/api/pith-number/LM6RJ5N2SSAKM2DKKWEAHIFHX3/graph.json","fetch_events":"https://pith.science/api/pith-number/LM6RJ5N2SSAKM2DKKWEAHIFHX3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LM6RJ5N2SSAKM2DKKWEAHIFHX3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LM6RJ5N2SSAKM2DKKWEAHIFHX3/action/storage_attestation","attest_author":"https://pith.science/pith/LM6RJ5N2SSAKM2DKKWEAHIFHX3/action/author_attestation","sign_citation":"https://pith.science/pith/LM6RJ5N2SSAKM2DKKWEAHIFHX3/action/citation_signature","submit_replication":"https://pith.science/pith/LM6RJ5N2SSAKM2DKKWEAHIFHX3/action/replication_record"}},"created_at":"2026-05-18T00:06:51.067090+00:00","updated_at":"2026-05-18T00:06:51.067090+00:00"}