{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,5,7]],"date-time":"2026-05-07T19:12:22Z","timestamp":1778181142421,"version":"3.51.4"},"reference-count":29,"publisher":"Springer Science and Business Media LLC","issue":"8","license":[{"start":{"date-parts":[[2012,8,1]],"date-time":"2012-08-01T00:00:00Z","timestamp":1343779200000},"content-version":"tdm","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/2.0"},{"start":{"date-parts":[[2012,8,23]],"date-time":"2012-08-23T00:00:00Z","timestamp":1345680000000},"content-version":"vor","delay-in-days":22,"URL":"https:\/\/creativecommons.org\/licenses\/by\/2.0"}],"content-domain":{"domain":["link.springer.com"],"crossmark-restriction":false},"short-container-title":["J. High Energ. Phys."],"published-print":{"date-parts":[[2012,8]]},"abstract":"<jats:title>A<jats:sc>bstract<\/jats:sc>\n          <\/jats:title>\n          <jats:p>We use a mix of analytic and numerical methods to exhaustively study a class of asymptotically global AdS solitons and hairy black hole solutions in negative cosmological constant Einstein Maxwell gravity coupled to a charged massless scalar field. Our results depend sensitively on the charge <jats:italic>e<\/jats:italic> of the scalar field. The solitonic branch of solutions we study hits the Chandrashekhar limit at finite mass at small <jats:italic>e<\/jats:italic>, but extends to arbitrarily large mass at larger <jats:italic>e<\/jats:italic>. At low values of <jats:italic>e<\/jats:italic> no hairy black holes exist. At intermediate values of <jats:italic>e<\/jats:italic> hairy black holes exist above a critical charge. At large <jats:italic>e<\/jats:italic> hairy black holes exist at all values of the charge. The lowest mass hairy black hole is a smooth zero entropy soliton at small charge, but a (probably) singular nonzero entropy hairy black hole at larger charge. In a phase diagram of solutions, the hairy black holes merge with the familiar Reissner-Nordstr\u00f6m\u2212AdS black holes along a curve that is determined by the onset of the superradiant instability in the latter family.<\/jats:p>","DOI":"10.1007\/jhep08(2012)117","type":"journal-article","created":{"date-parts":[[2012,8,23]],"date-time":"2012-08-23T19:47:05Z","timestamp":1345751225000},"update-policy":"https:\/\/doi.org\/10.1007\/springer_crossmark_policy","source":"Crossref","is-referenced-by-count":97,"title":["Hairy black holes and solitons in global AdS5"],"prefix":"10.1007","volume":"2012","author":[{"given":"\u00d3scar J. 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