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Considering a spherical surface at some radius around such a star, the magnetic field is radial in the polar cap as opposed to most of 4 pi (the full solid angle), where the magnetic field is nearly tangential. This difference yields a flatter spectrum, and also an enhanced positron injection for the cosmic rays accelerated in the polar cap. This reasoning naturally exp"},"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":"0903.4048","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2009-03-24T09:39:07Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"60aa0ddbf897cfd534440f458add3425d4781dad7d1f7bfad0dee9080aedec64","abstract_canon_sha256":"d450148f006553322d772a14d636a8890c99ff090cb131a2e09e32f01b33e91b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:48:45.775645Z","signature_b64":"0adx556oWpK3IjuiysxlC0HbRQfUea3JDAdcWPP2b1zVQA51nPoGfMnxDfWjVZDA1zBdtFLKIAmoWMOYmCwZDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"301f3df81bdb522d13445520cc44f4c02bfc2088ea26d670a0267927d25248e6","last_reissued_at":"2026-07-04T15:48:45.775270Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:48:45.775270Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmic ray electrons and positrons from supernova explosions of massive stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"A. Meli, E.-S. Seo, J.K. Becker, P.L. Biermann, T. Stanev, W. Rhode","submitted_at":"2009-03-24T09:39:07Z","abstract_excerpt":"We attribute the recently discovered cosmic ray electron and cosmic ray positron excess components and their cutoffs to the acceleration in the supernova shock in the polar cap of exploding Wolf Rayet and Red Super Giant stars. Considering a spherical surface at some radius around such a star, the magnetic field is radial in the polar cap as opposed to most of 4 pi (the full solid angle), where the magnetic field is nearly tangential. This difference yields a flatter spectrum, and also an enhanced positron injection for the cosmic rays accelerated in the polar cap. 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