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Photodissociation cross sections of ArH+ are computed in an ab initio approach including explicit account of spin-orbit coupling. Results. We report the photodissociation cross section of ArH+ as a function of wavelength. Photodissociation probabilities are derived for different impinging radiation fields.The photodissociation probability of for a very small unshielded cloud surrounded "},"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":"1404.2051","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-04-08T09:14:12Z","cross_cats_sorted":[],"title_canon_sha256":"931f7c48241087edc1132d3dcc866ceb4813779b0fcafbf840f54da24bb13690","abstract_canon_sha256":"f4ca2722e8afe4e3b89a528c54873ba4c646b89c454d0346bcdf8f8fb4cea644"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:00:46.487242Z","signature_b64":"flBs2dtzy6v0IAEV8qR1rlGeMCPRdSRrvMqJKFW7VVKhYMTNMiZiITpuoa8kUwlyU8BqyWmK8P/1GtYT49LJDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5aaa424ced352e2f9340bd99fb129311c03003f9ec87f95bf6881bfd9e45e2be","last_reissued_at":"2026-05-18T01:00:46.486821Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:00:46.486821Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Photodissociation of interstellar ArH+","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A.B. 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