Repeated partial disruptions in a WD-NS or WD-BH merger modulate the prompt emission of long-duration merger-type GRBs

Abstract

The progenitors of gamma-ray bursts (GRBs) have long been an unresolved issue. GRB 230307A stands out as an exceptionally bright event, belonging to the long-duration GRBs but also exhibiting a late emission component reminiscent of a kilonova. Together with the similar events GRBs 060614 and 211211A, they make up a new sub-group of GRBs with intriguing progenitors. If such long-duration merger-type GRBs originated from the coalescence of a white dwarf (WD) with a neutron star (NS) or a black hole (BH), as proposed in the recent literature, then the larger tidal disruption radius of the WD, together with a non-negligible residual orbital eccentricity, would make repeated partial tidal disruptions inevitable. This may modulate the mass accretion and jet launching process at the NS or BH, resulting in a quasi-periodic modulation (QPM) in the light curve of the GRB, on the orbital period. The detection of potential QPMs during the early episode of prompt emission of these three GRBs supports this scenario, and the relatively slow QPM ($>$ 1 s) suggests that the lighter object can not be a NS. We propose that the progenitor system of GRBs 230307A, 060614, and 211211A consist of a WD of mass 1.3 $M_{\odot }$, 0.9 $M_{\odot }$ and 1.4 $M_{\odot }$, respectively, and a NS (or BH). After several cycles of modulations, the WD is completely destructed, and the accretion of the remaining debris dominates the extended emission episode.

13 pages, 1 appendix, accepted for publication in ApJL

References in corpus (23)

• The Supernova -- Gamma-Ray Burst Connection
• The Physics of Gamma-Ray Bursts and Relativistic Jets
• A Kilonova Following a Long-Duration Gamma-Ray Burst at 350 Mpc
• A nearby long gamma-ray burst from a merger of compact objects
• A long-duration gamma-ray burst with a peculiar origin
• JWST detection of heavy neutron capture elements in a compact object merger
• A highly magnetised and rapidly rotating white dwarf as small as the Moon
• A Peculiarly Short-duration Gamma-Ray Burst from Massive Star Core Collapse
• A new type of long gamma--ray burst
• Quasi--Periodic Eruptions from Galaxy Nuclei
• Quasi-Periodic Erupters: A Stellar Mass-Transfer Model for the Radiation
• Long-duration Gamma-ray Burst and Associated Kilonova Emission from Fast-spinning Black Hole--Neutron Star Mergers
• GRB 211211A: a Neutron Star$-$White Dwarf Merger?
• On accretion disks formed in MHD simulations of black hole-neutron star mergers with accurate microphysics
• Discovery of a hot ultramassive rapidly rotating DBA White Dwarf
• A tidal disruption model for the gamma-ray burst of GRB 060614
• Tidal Stripping of a White Dwarf by an Intermediate-Mass Black Hole
• Tidal disruption events from eccentric orbits and lessons learned from the noteworthy ASASSN-14ko
• Pulsar timing noise and the minimum observation time to detect gravitational waves with pulsar timing arrays
• What Powered the Kilonova-Like Emission After GRB 230307A in the Framework of a Neutron Star-White Dwarf Merger?
• GRB 211211A-like Events and How Gravitational Waves May Tell Their Origins
• Self-consistent MHD simulation of jet launching in a neutron star - white dwarf merger
• Evidence for a compact stellar merger origin for GRB 230307A from Fermi-LAT and multi-wavelength afterglow observations

Cited by in corpus (4)

• Gamma-ray bursts and kilonovae from the accretion-induced collapse of white dwarfs
• Shared Properties of Merger-driven Long-duration Gamma-Ray Bursts
• A 4.5-s Quasiperiodic Spectral Oscillation in GRB 230307A: Evidence for Free Precession of a Post-Merger Magnetar?
• The metallicity dependence of long-duration gamma-ray bursts