Near-extremal black holes as initial conditions of long GRB-supernovae and probes of their gravitational wave emission
arXiv:1509.00407 · doi:10.1088/0004-637X/810/1/7
Abstract
Long gamma-ray bursts (GRBs) associated with supernovae and short GRBs with Extended Emission (SGRBEE) from mergers are probably powered by black holes as a common inner engine, as their prompt GRB emission satisfies the same Amati correlation in the plane. We introduce modified Bardeen equations to identify hyper-accretion driving newly formed black holes in core-collapse supernovae to near-extremal spin as a precursor to prompt GRB emission. Subsequent spin-down is observed in the BATSE catalog of long GRBs. Spin-down provides a natural unification of long durations associated with the lifetime of black hole spin for normal long GRBs and SGRBEEs, given the absence of major fallback matter in mergers. The results point to major emissions unseen in high frequency gravitational waves. A novel matched filtering method is described for LIGO-Virgo and KAGRA broadband probes of nearby core-collapse supernovae at essentially maximal sensitivity.
References in corpus (15)
- An optical supernova associated with the X-ray flash XRF 060218
- Accurate evolutions of inspiralling neutron-star binaries: prompt and delayed collapse to black hole
- Early-Time Photometry and Spectroscopy of the Fast Evolving SN 2006AJ Associated with GRB 060218
- Mass Fall-back and Accretion in the Central Engine of Gamma-Ray Bursts
- GRB 060218/SN 2006aj: A Gamma-Ray Burst and Prompt Supernova at z=0.0335
- Supernova 2006aj and the associated X-Ray Flash 060218
- Fragmentation of Collapsar Disks and the Production of Gravitational Waves
- Jet formation in GRBs: A semi-analytic model of MHD flow in Kerr geometry with realistic plasma injection
- On the origin of short GRBs with Extended Emission and long GRBs without associated SN
- On the Composition of GRBs' Collapsar Jets
- Broad band turbulent spectra in gamma-ray burst light curves
- Gravitational radiation from magnetically funnelled supernova fallback onto a magnetar
- Non-thermal transient sources from rotating black holes
- Extreme luminosities in ejecta produced by intermittent outflows around rotating black holes
- Proposed searches for candidate sources of gravitational waves in a nearby core-collapse supernova survey
Cited by in corpus (16)
- Observations of Protoplanetary Disk Structures
- Tracing the formation of the Milky Way through ultra metal-poor stars
- A comprehensive statistical study on gamma-ray bursts
- Transition from Inspiral to Plunge: A Complete Near-Extremal Trajectory and Associated Waveform
- Constraining the spin parameter of near-extremal black holes using LISA
- Gravitational perturbations from NHEK to Kerr
- General relativistic rotational energy extraction from black holes-accretion disk systems
- On extreme transient events from rotating black holes and their gravitational wave emission
- Directed searches for broadband extended gravitational-wave emission in nearby energetic core-collapse supernovae
- Prospects for multi-messenger extended emission from core-collapse supernovae in the Local Universe
- Multi-messenger Extended Emission from the compact remnant in GW170817
- Relating Kerr SMBHs in Active Galactic Nuclei to RAD configurations
- Central engine of GRB170817A: Neutron star versus Kerr black hole based on multimessenger calorimetry and event timing
- Insights into planet formation from debris disks: I. The solar system as an archetype for planetesimal evolution
- The gas disk: Evolution and chemistry
- Broadband extended emission in gravitational waves from core-collapse supernovae