{"record":{"author":{"account_ref":null,"orcid":null},"builds_on":[],"content_schema":"pubphys.content.revision/1","content_sha256":"2df6a18cf1e8f744ff4f37f473e4a60a14fffefaad03756627a8a7f41a58fe26","created":"2026-10-15T23:43:22Z","files":[],"origin":{"assisted_by":[],"kind":"seed"},"parents":["ce59fb6cd812fc05906d0c60a71c75ea22bc686bcf38e7c3ef7010834d98ee7b","ec94cfc90cb6acfc4fa70a31cd2513e1f24fceb37eafca2fc8b0c231cf65a786"],"salt":"9afad27f673923c8ccee8220a01e4a719e9cec28bc0733458c97ab927796c91b","schema":"pubphys.record/2","site":"pubphys.com","target":null,"type":"revision"},"content":{"answer_type":"identification","assisted_by":[],"external_id":"astro.galactic-gamma-ray-anomalies.positron-origin","kind":"phenomenon","literature_status":"open","n":"2","parents":[],"plain":"About $5 \\times 10^{43}$ positrons per second annihilate in the Milky Way, mostly in the central bulge, and no known source class explains both the rate and the bulge-heavy pattern.","posed_since":"","precise":"Explain the $511\\,\\mathrm{keV}$ line (annihilation rate $\\sim 5 \\times 10^{43}\\,\\mathrm{positrons}/\\mathrm{s}$, bulge-to-disk luminosity ratio $\\sim 1$) with positrons injected below a few MeV (required by in-flight annihilation limits). Candidates: beta-plus decay of $\\mathrm{Al}-26$, $\\mathrm{Ti}-44$ and $\\mathrm{Co}-56$ from supernovae and novae, microquasars and low-mass X-ray binaries, past activity of Sgr A*, MeV-mass dark matter. Answer: a source mixture reproducing rate, morphology and spectrum, including positron transport.","problem_ref":"ec94cfc90cb6acfc4fa70a31cd2513e1f24fceb37eafca2fc8b0c231cf65a786","references":"","settled_by":"High-resolution imaging and spectroscopy of the line, resolving point sources or a profile that singles out one class.","status_note":"The COSI MeV mission, planned for launch in 2027, will map the line with better angular and energy resolution.","title":"What produces the Galaxy's 511 keV positron annihilation line?","topic_ref":null},"attested":{"attestation":{"batch":null,"client_id":null,"id_token_sha256":null,"kind":"platform"},"record_hash":"340a439d913c9e7abf10f55465a04105efd693220ef3c8f3b0e72be4303ef5f1","schema":"pubphys.attested/1"},"envelope":{"attested_hash":"1106046d3325e1d4cec75af6c627443315a0c606e53391b12617174b61fcad9f","platform_signature":{"key_id":"c6afc19b31429869751f06879c75cd64ea92654423d15b44be775bf1310a60da","sig":"is7coV7nWfykutyn_aAPEnD6ojEZxxq-lBqxYo2ZOQuQGJiKr_howbpv-0av7DikRZm8nR0B4bLfdzeM3MaBBg"},"schema":"pubphys.envelope/1"},"record_hash":"340a439d913c9e7abf10f55465a04105efd693220ef3c8f3b0e72be4303ef5f1","leaf_index":2358}