{ "id": "1805.05722", "version": "v1", "published": "2018-05-15T12:08:53.000Z", "updated": "2018-05-15T12:08:53.000Z", "title": "A lower occurrence rate of bright X-ray flares in SN-GRBs than $z<1$ GRBs: evidence of energy partitions?", "authors": [ "Hui-Jun Mu", "Wei-Min Gu", "Jirong Mao", "Tong Liu", "Shu-Jin Hou", "Da-Bin Lin", "Junfeng Wang", "Taotao Fang", "En-Wei Liang" ], "comment": "10 pages, 4 figures, accepted for publication in MNRAS", "categories": [ "astro-ph.HE" ], "abstract": "The occurrence rates of bright X-ray flares in z<1 gamma-ray bursts (GRBs) with or without observed supernovae (SNe) association were compared. Our Sample I: the z<1 long GRBs (LGRBs) with SNe association (SN-GRBs) and with early Swift/X-Ray Telescope (XRT) observations, consists of 18 GRBs, among which only two GRBs have bright X-ray flares. Our Sample II: for comparison, all the z<1 LGRBs without observed SNe association and with early Swift/XRT observations, consists of 45 GRBs, among which 16 GRBs present bright X-ray flares. Thus, the study indicates a lower occurrence rate of bright X-ray flares in Sample I (11.1%) than in Sample II (35.6%). In addition, if dim X-ray fluctuations are included as flares, then 16.7% of Sample I and 55.6% of Sample II are found to have flares, again showing the discrepancy between these two samples. We examined the physical origin of these bright X-ray flares and found that most of them are probably related to the central engine reactivity. To understand the discrepancy, we propose that such a lower occurrence rate of flares in the SN-GRB sample may hint at an energy partition among the GRB, SNe, and X-ray flares under a saturated energy budget of massive star explosion.", "revisions": [ { "version": "v1", "updated": "2018-05-15T12:08:53.000Z" } ], "analyses": { "keywords": [ "bright x-ray flares", "lower occurrence rate", "energy partition", "sne association", "central engine reactivity" ], "note": { "typesetting": "TeX", "pages": 10, "language": "en", "license": "arXiv", "status": "editable" } } }