{ "id": "2004.05514", "version": "v1", "published": "2020-04-12T00:54:00.000Z", "updated": "2020-04-12T00:54:00.000Z", "title": "GRB 111209A/SN 2011kl: Collapse of a supramassive magnetar with r-mode oscillation and fall-back accretion onto a newborn black hole", "authors": [ "Jie Lin", "Rui-Jing Lu", "Da-Bin Lin", "Xiang-Gao Wang" ], "comment": "15 pages, 3 figures. To be accepted for publication in ApJ", "categories": [ "astro-ph.HE" ], "abstract": "Ultra-long-duration gamma-ray burst GRB 111209A was found to be associated with a very luminous supernovae (SNe) SN 2011kl. The physics of GRB 111209A/SN 2011kl has been extensively studied in the literures, but does not settle down yet. By investigating in detail the characteristics of the X-ray light curve of GRB 111209A, coupled with the temporal and spectral features observed in SN 2011kl, we argue that a short-living supramassive magnetar can be responsible for the initial shallow X-ray emission. Then the electromagnetic extraction of spin energy from a black hole results in the steeply declining X-ray flux when the magnetar collapses into a black hole (BH). A fraction of the envelope materials falls back and activates the accretion onto the newborn BH, which produces the X-ray rebrightening bump at late times. During this process, a centrifugally driven baryon-rich quasi-isotropic Blandford \\& Payne outflow from the revived accretion disk deposits its kinetic energy on the SN ejecta, which powers luminous SN 2011kl. Finally, we place a limitation on the magnetar's physical parameters based on the observations.", "revisions": [ { "version": "v1", "updated": "2020-04-12T00:54:00.000Z" } ], "analyses": { "keywords": [ "grb 111209a/sn 2011kl", "newborn black hole", "supramassive magnetar", "r-mode oscillation", "driven baryon-rich quasi-isotropic blandford" ], "note": { "typesetting": "TeX", "pages": 15, "language": "en", "license": "arXiv", "status": "editable" } } }