{"record":{"author":{"account_ref":null,"orcid":null},"builds_on":[],"content_schema":"pubphys.content.topic/1","content_sha256":"b607f91067088f47d855e16f77bc159dad93912bfe1a7d1bd605eceaf0130e35","created":"2026-10-03T07:17:50Z","files":[],"origin":{"assisted_by":[],"kind":"seed"},"parents":[],"salt":"c2483c0d9d1a2366e0b7617bd770ef44915dd25dc98a3c322cc0511cc6eebb1b","schema":"pubphys.record/2","site":"pubphys.com","target":null,"type":"topic"},"content":{"external_id":"astro.pulsars-magnetars","field":"astro","n":"1","review_cite":"A. Philippov, A. Timokhin, A. Spitkovsky, Origin of pulsar radio emission, Physical Review Letters, 2020","review_link":"https://arxiv.org/abs/2001.02236","review_verified":"true","summary":"Pulsars are spinning neutron stars that sweep radio beams across Earth like a lighthouse, and magnetars are neutron stars with fields a hundred to a thousand times stronger still. How the radio beam is made, and how magnetars get their fields, are both open.","title":"Pulsar radio emission and magnetar origin","topic_ref":null,"why":"Pulsars are precise clocks used to detect gravitational waves, and their emission tests plasma physics in fields of $1e12\\,\\mathrm{G}$ and above."},"attested":{"attestation":{"batch":null,"client_id":null,"id_token_sha256":null,"kind":"platform"},"record_hash":"cf74b0d6cbf0f14a95f95d071c68e45a587fcae015fdd13da4686d4a258fa561","schema":"pubphys.attested/1"},"envelope":{"attested_hash":"2512298d20d62fb7d008711f77de0d7a9aa2c3bd3d5d472a1b57fa8bd188bb8f","platform_signature":{"key_id":"c6afc19b31429869751f06879c75cd64ea92654423d15b44be775bf1310a60da","sig":"TiTRtnMI7dfNnt6nVqaSR7_Pq9rjyPhB-H7z7CGosFW_r1xQ5GFFvfd1U5B-wke9TSnNPELdkGKf5zcalJ36Cw"},"schema":"pubphys.envelope/1"},"record_hash":"cf74b0d6cbf0f14a95f95d071c68e45a587fcae015fdd13da4686d4a258fa561","leaf_index":48}