We explore the rich phase space of singly spinning (both neutral and charged) black hole solutions in the large D limit. We find several ‘bumpy’ branches which are connected to multiple (concentric) black rings, and black Saturns. Additionally, we obtain stationary solutions without axisymmetry that are only stationary at D → ∞, but correspond to long-lived black hole solutions at finite D. These multipolar solutions can appear as intermediate configurations in the decay of ultra-spinning Myers-Perry black holes into stable black holes. Finally, we also construct stationary solutions corresponding to the instability of such a multipolar solution.
{ "_oai": { "updated": "2020-04-18T15:32:43Z", "id": "oai:repo.scoap3.org:53885", "sets": [ "JHEP" ] }, "authors": [ { "affiliations": [ { "country": "Spain", "value": "Departament de F\u00edsica Qu\u00e0ntica i Astrof\u00edsica, Institut de Ci\u00e8ncies del Cosmos, Universitat de Barcelona, Mart\u00ed i Franqu\u00e8s 1, Barcelona, E-08028, Spain", "organization": "Universitat de Barcelona" } ], "surname": "Licht", "email": "david.licht@icc.ub.edu", "full_name": "Licht, David", "given_names": "David" }, { "affiliations": [ { "country": "Spain", "value": "Departament de F\u00edsica Qu\u00e0ntica i Astrof\u00edsica, Institut de Ci\u00e8ncies del Cosmos, Universitat de Barcelona, Mart\u00ed i Franqu\u00e8s 1, Barcelona, E-08028, Spain", "organization": "Universitat de Barcelona" } ], "surname": "Luna", "email": "raimonluna@icc.ub.edu", "full_name": "Luna, Raimon", "given_names": "Raimon" }, { "affiliations": [ { "country": "Spain", "value": "Departament de F\u00edsica Qu\u00e0ntica i Astrof\u00edsica, Institut de Ci\u00e8ncies del Cosmos, Universitat de Barcelona, Mart\u00ed i Franqu\u00e8s 1, Barcelona, E-08028, Spain", "organization": "Universitat de Barcelona" }, { "country": "Japan", "value": "Department of Physics, Osaka City University, Sugimoto 3-3-138, Osaka, 558-8585, Japan", "organization": "Osaka City University" } ], "surname": "Suzuki", "email": "s.ryotaku@icc.ub.edu", "full_name": "Suzuki, Ryotaku", "given_names": "Ryotaku" } ], "titles": [ { "source": "Springer", "title": "Black ripples, flowers and dumbbells at large D" } ], "dois": [ { "value": "10.1007/JHEP04(2020)108" } ], "publication_info": [ { "page_end": "50", "journal_title": "Journal of High Energy Physics", "material": "article", "journal_volume": "2020", "artid": "JHEP04(2020)108", "year": 2020, "page_start": "1", "journal_issue": "4" } ], "$schema": "http://repo.scoap3.org/schemas/hep.json", "acquisition_source": { "date": "2020-04-18T17:30:29.420477", "source": "Springer", "method": "Springer", "submission_number": "7771c5d2818911eaad8602163e01809a" }, "page_nr": [ 50 ], "license": [ { "url": "https://creativecommons.org/licenses/by/3.0", "license": "CC-BY-3.0" } ], "copyright": [ { "holder": "The Author(s)", "year": "2020" } ], "control_number": "53885", "record_creation_date": "2020-04-18T17:30:29.420497", "_files": [ { "checksum": "md5:4c8e79f01f1d90577c73713a25fccfd1", "filetype": "xml", "bucket": "549ef08b-96dc-497f-8981-47539257bced", "version_id": "c59cbb60-9e1b-4247-b6ad-4fb6bf116e89", "key": "10.1007/JHEP04(2020)108.xml", "size": 10552 }, { "checksum": "md5:47898051a51a31a5ce794413ccde0059", "filetype": "pdf/a", "bucket": "549ef08b-96dc-497f-8981-47539257bced", "version_id": "4838edea-f081-4f9e-a5e5-38507d87361c", "key": "10.1007/JHEP04(2020)108_a.pdf", "size": 1730230 } ], "collections": [ { "primary": "Journal of High Energy Physics" } ], "arxiv_eprints": [ { "categories": [ "hep-th", "gr-qc" ], "value": "2002.07813" } ], "abstracts": [ { "source": "Springer", "value": "We explore the rich phase space of singly spinning (both neutral and charged) black hole solutions in the large D limit. We find several \u2018bumpy\u2019 branches which are connected to multiple (concentric) black rings, and black Saturns. Additionally, we obtain stationary solutions without axisymmetry that are only stationary at D \u2192 \u221e, but correspond to long-lived black hole solutions at finite D. These multipolar solutions can appear as intermediate configurations in the decay of ultra-spinning Myers-Perry black holes into stable black holes. Finally, we also construct stationary solutions corresponding to the instability of such a multipolar solution." } ], "imprints": [ { "date": "2020-04-17", "publisher": "Springer" } ] }