{"schema":"pubphys.bundle/1","record":{"author":{"account_ref":null,"orcid":null},"builds_on":[],"content_schema":"pubphys.content.revision/1","content_sha256":"33fd58cef641b1000dbba92bf61dba48db51e85d60688eaf38a0a0eda65a1775","created":"2026-10-15T23:43:22Z","files":[],"origin":{"assisted_by":["ai:gpt-5.5"],"kind":"seed"},"parents":["03c9004886ff9250e10ade4a407fa1c24ffc5d131250344ef66c8da48c738132","ce59fb6cd812fc05906d0c60a71c75ea22bc686bcf38e7c3ef7010834d98ee7b"],"salt":"39a5ac8bcb24bed380878f60806482baf6e501e7e0ee0571555571ca0f01cb06","schema":"pubphys.record/2","site":"pubphys.com","target":null,"type":"revision"},"content":{"answer_type":"value","assisted_by":["ai:gpt-5.5"],"external_id":"astro.system-architectures.super-earth-cold-jupiter","kind":"well-posed","literature_status":"contested","n":"2","parents":[],"plain":"Whether stars with close-in super-Earths are more or less likely to also have a Jupiter-like planet far out tells whether giant planets help or block the formation of inner small planets. Different surveys disagree.","posed_since":"2018","precise":"Measure $P(\\mathrm{CJ}\\mid \\mathrm{SE})$, the occurrence of cold Jupiters ($M\\,\\mathrm{sin}\\,i \\sim 0.3-13\\ M_{\\mathrm{Jup}}, a \\sim 1-10\\ \\mathrm{AU}$) around hosts of inner super-Earths ($R = 1-4\\,R_{\\mathrm{earth}}, P < 100\\,\\mathrm{d}$), versus the field rate of about 10 percent. Zhu and Wu 2018 and Bryan et al. 2019 ($39 \\pm 7\\%$) report an excess of about three times, while Bonomo et al. 2023 (A&A 677, A33) find $9.3(+7.7,-2.9)\\%$ and no excess. The answer is $P(\\mathrm{CJ}\\mid \\mathrm{SE})$ with metallicity dependence and uncertainty sufficient to decide the excess.","problem_ref":"03c9004886ff9250e10ade4a407fa1c24ffc5d131250344ef66c8da48c738132","references":"","settled_by":"Long-baseline radial-velocity follow-up of a large, homogeneously selected sample of super-Earth hosts with metallicities matched to a control sample.","status_note":"Bonomo et al. 2023 found no excess, contradicting the 2018-2019 results; the difference may reflect sample metallicity or selection.","title":"Do inner super-Earths and outer cold Jupiters tend to occur 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