Are Ultra-Long Gamma-Ray Bursts Caused by Blue Supergiant Collapsars, Newborn Magnetars, or White Dwarf Tidal Disruption Events?
Kunihito Ioka, Kenta Hotokezaka, Tsvi Piran

TL;DR
Ultra-long gamma-ray bursts (ulGRBs) with durations around 10,000 seconds may originate from blue supergiant collapsars, magnetars, or white dwarf tidal disruption events, with recent observations challenging some models and suggesting TDEs as a plausible energy source.
Contribution
This paper proposes that white dwarf tidal disruption events can explain observed supernova-like bumps in ulGRBs, expanding the possible origins of these phenomena.
Findings
WD-TDEs can produce SN-like bumps with observed energies and velocities.
X-ray ionization can suppress hydrogen lines in ejecta.
SN 2011kl's light curve is consistent with multiple models, but magnetar explanation is less natural.
Abstract
Ultra-long gamma-ray bursts (ulGRBs) are a new population of GRBs with extreme durations of s. Leading candidates for their origin are blue supergiant collapsars, magnetars, and white dwarf tidal disruption events (WD-TDEs) caused by massive black holes (BHs). Recent observations of supernova-like (SN-like) bumps associated with ulGRBs challenged both the WD-TDE and the blue supergiant models because of the detection of SNe and the absence of hydrogen lines, respectively. We propose that WD-TDEs can accommodate the observed SN-like bumps if the fallback WD matter releases energy into the unbound WD ejecta. The observed ejecta energy, luminosity, and velocity are explained by the gravitational energy, Eddington luminosity, and escape velocity of the formed accretion disk, respectively. We also show that the observed X-rays can ionize the ejecta, eliminating lines. The…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
