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It is shown that $BR(\\phi\\rightarrow\\gamma f_0(a_0)\\rightarrow\\gamma\\pi\\pi(\\pi\\eta))\\approx (1\\div 2)\\times 10^{-5}\\ ,\\BR(\\phi\\rightarrow\\gamma (f_0+a_0)\\rightarrow\\gamma K^+K^-)\\alt 10^{-6}$ and $BR(\\phi\\rightarrow\\gamma (f_0+a_0) \\to \\gamma K^0\\bar K^0)\\alt 10^{-8}$. The mass spectra in the $\\pi\\pi\\ ,\\ \\pi\\eta\\ ,\\ K^+K^-\\ ,\\ K^0\\bar K^0$ channels are calculated. The imaginary part of the amplitude $\\phi\\rightarrow\\gamma f_0(a_0)"},"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":"hep-ph/9605245","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"1996-05-07T18:18:33Z","cross_cats_sorted":[],"title_canon_sha256":"8902ff32c2e00088d4b3880cf355de8cdaf31e39acbd81c4dc0c985e6f7be802","abstract_canon_sha256":"eead2f4a8ca21c34ab742b8c4e8736bdd64027443b851dfd4bec207c97bdafbb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:35:58.371143Z","signature_b64":"laWyHTTp/eM8S9XcXu7Wf8UAVhRhGXwes50s7weQFAucv9nFiP45KyPAlBLBuULtwgOz5Wfx3nzVbd/AVtJBAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9f9311ac3d5b83dff6e37b5e33392aa48cee848520ac86f14e0a31d45415fa7d","last_reissued_at":"2026-05-18T04:35:58.370287Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:35:58.370287Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Production of scalar $K\\bar K$ molecules in $\\phi$ radiative decays","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"(2) Institute for Theoretical, Experimental Physics, Moscow), N.N.Achasov (1), Novosibirsk, V.I.Shevchenko (2) ((1) S.L.Sobolev Institute for Mathematics, V.V.Gubin (1)","submitted_at":"1996-05-07T18:18:33Z","abstract_excerpt":"The potentialities of the production of the scalar $K\\bar K$ molecules in the $\\phi$ radiative decays are considered beyond the narrow resonance width approximation. It is shown that $BR(\\phi\\rightarrow\\gamma f_0(a_0)\\rightarrow\\gamma\\pi\\pi(\\pi\\eta))\\approx (1\\div 2)\\times 10^{-5}\\ ,\\BR(\\phi\\rightarrow\\gamma (f_0+a_0)\\rightarrow\\gamma K^+K^-)\\alt 10^{-6}$ and $BR(\\phi\\rightarrow\\gamma (f_0+a_0) \\to \\gamma K^0\\bar K^0)\\alt 10^{-8}$. The mass spectra in the $\\pi\\pi\\ ,\\ \\pi\\eta\\ ,\\ K^+K^-\\ ,\\ K^0\\bar K^0$ channels are calculated. The imaginary part of the amplitude $\\phi\\rightarrow\\gamma f_0(a_0)"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/9605245","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":"hep-ph/9605245","created_at":"2026-05-18T04:35:58.370427+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/9605245v1","created_at":"2026-05-18T04:35:58.370427+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/9605245","created_at":"2026-05-18T04:35:58.370427+00:00"},{"alias_kind":"pith_short_12","alias_value":"T6JRDLB5LOB5","created_at":"2026-05-18T12:25:48.327863+00:00"},{"alias_kind":"pith_short_16","alias_value":"T6JRDLB5LOB575XD","created_at":"2026-05-18T12:25:48.327863+00:00"},{"alias_kind":"pith_short_8","alias_value":"T6JRDLB5","created_at":"2026-05-18T12:25:48.327863+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2603.02671","citing_title":"Radiative decays of hadronic molecules: From confusion to inspiration","ref_index":14,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/T6JRDLB5LOB575XDPNPDGOJKUS","json":"https://pith.science/pith/T6JRDLB5LOB575XDPNPDGOJKUS.json","graph_json":"https://pith.science/api/pith-number/T6JRDLB5LOB575XDPNPDGOJKUS/graph.json","events_json":"https://pith.science/api/pith-number/T6JRDLB5LOB575XDPNPDGOJKUS/events.json","paper":"https://pith.science/paper/T6JRDLB5"},"agent_actions":{"view_html":"https://pith.science/pith/T6JRDLB5LOB575XDPNPDGOJKUS","download_json":"https://pith.science/pith/T6JRDLB5LOB575XDPNPDGOJKUS.json","view_paper":"https://pith.science/paper/T6JRDLB5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/9605245&json=true","fetch_graph":"https://pith.science/api/pith-number/T6JRDLB5LOB575XDPNPDGOJKUS/graph.json","fetch_events":"https://pith.science/api/pith-number/T6JRDLB5LOB575XDPNPDGOJKUS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/T6JRDLB5LOB575XDPNPDGOJKUS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/T6JRDLB5LOB575XDPNPDGOJKUS/action/storage_attestation","attest_author":"https://pith.science/pith/T6JRDLB5LOB575XDPNPDGOJKUS/action/author_attestation","sign_citation":"https://pith.science/pith/T6JRDLB5LOB575XDPNPDGOJKUS/action/citation_signature","submit_replication":"https://pith.science/pith/T6JRDLB5LOB575XDPNPDGOJKUS/action/replication_record"}},"created_at":"2026-05-18T04:35:58.370427+00:00","updated_at":"2026-05-18T04:35:58.370427+00:00"}