The first minutes of a binary-driven hypernova

Abstract

We simulate the first minutes of the evolution of a binary-driven hypernova (BdHN) event, with a special focus on the associated accretion processes of supernova (SN) ejecta onto the newborn neutron star ($\nu$NS) and the NS companion. We calculate the rotational evolution of the $\nu$NS and the NS under the torques exerted by the accreted matter and the magnetic field. We take into account general relativistic effects and use realistic hypercritical accretion rates obtained from three-dimensional smoothed-particle-hydrodynamics (SPH) numerical simulations of the BdHN for a variety of orbital periods. We show that the rotation power of the $\nu$NS has a unique double-peak structure while that of the NS has a single peak. These peaks are of comparable intensity and can occur very close in time or even simultaneously depending on the orbital period and the initial angular momentum of the stars. We outline the consequences of the above features in the early emission and their consequent observation in long gamma-ray bursts (GRBs).

arXiv commentAccepted for publication in Physical Review D

References in corpus (66)

• The Swift X-ray Telescope
• Collapsars - Gamma-Ray Bursts and Explosions in "Failed Supernovae"
• The Swift Ultra-Violet/Optical Telescope
• Discovery of the peculiar supernova 1998bw in the error box of GRB980425
• The Physics of Gamma-Ray Bursts
• The Supernova -- Gamma-Ray Burst Connection
• The Burst Alert Telescope (BAT) on the Swift MIDEX Mission
• Gamma-Ray Bursts as the Death Throes of Massive Binary Stars
• Progenitors of core-collapse supernovae
• Discovery of the X-Ray Afterglow of the Gamma-Ray Burst of February 28 1997
• Theories of Gamma-Ray Bursts
• Formation of Double Neutron Star Systems
• Observational constraints on the progenitors of core-collapse supernovae : the case for missing high mass stars
• Progenitor-Explosion Connection and Remnant Birth Masses for Neutrino-Driven Supernovae of Iron-Core Progenitors
• Formation Rates of Black Hole Accretion Disk Gamma-Ray Bursts
• Type Ib/c supernovae in binary systems I. Evolution and properties of the progenitor stars
• Maximum mass, moment of inertia and compactness of relativistic stars
• Teraelectronvolt emission from the $\gamma$-ray burst GRB 190114C
• Luminous Blue Variable eruptions and related transients: Diversity of progenitors and outburst properties
• Gasdynamics of Relativistically Expanding Gamma-Ray Burst Sources: Kinematics, Energetics, Magnetic Fields and Efficiency
• Hydrodynamics of Relativistic Fireballs
• Neutrino-Dominated Accretion and Supernovae
• Ultra-stripped Type Ic supernovae from close binary evolution
• The Dynamics and Outcomes of Rapid Infall onto Neutron Stars
• Constraints on Type Ib/c and GRB Progenitors
• Evolutionary Models for Type Ib/c Supernova Progenitors
• A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary
• Fast Rotating Neutron Stars with Realistic Nuclear Matter Equation of State
• Hypercritical Accretion, Induced Gravitational Collapse, and Binary-Driven Hypernovae
• On the Induced Gravitational Collapse of a Neutron Star to a Black Hole by a Type Ib/c Supernova
• The spin parameter of uniformly rotating compact stars
• Supernova Fallback: A Possible Site for the r-Process
• Multipolar electromagnetic fields around neutron stars: exact vacuum solutions and related properties
• Neutrinos from Fallback onto Newly Formed Neutron Stars
• Euclidean vs. non-Euclidean Gamma-Ray Bursts
• Neutron star universal relations with microscopic equations of state
• On the induced gravitational collapse scenario of gamma-ray bursts associated with supernovae
• Angular Momentum Role in the Hypercritical Accretion of Binary-Driven Hypernovae
• Binary-Stripped Stars as Core-Collapse Supernovae Progenitors
• Early X-ray Flares in GRBs
• Parameterizing the Supernova Engine and its Effects on Remnants and Basic Yields
• On the Neutron Star-Black Hole Binaries Produced by Binary-driven-Hypernovae
• GRB 090618: The First Example of a Neutron Star Gravitational Collapse to a Black Hole Induced by a Type Ib/c Supernova
• On the GeV emission of the type I BdHN GRB 130427A
• SPH simulations of the induced gravitational collapse scenario of long gamma-ray bursts associated with supernovae
• Gravitomagnetic interaction of a Kerr black hole with a magnetic field as the source of the jetted GeV radiation of gamma-ray bursts
• Two Predictions of supernova: GRB 130427A / SN 2013cq and GRB 180728A / SN 2018fip
• The blackholic quantum
• Observational Properties of Type Ib/c Supernova Progenitors in Binary Systems
• Magnetic Fields and Afterglows of BdHNe: Inferences from GRB 130427A, GRB 160509A, GRB 160625B, GRB 180728A and GRB 190114C
• The newborn black hole in GRB 191014C proves that it is alive
• Novel Model of an Ultra-stripped Supernova Progenitor of a Double Neutron Star
• Astrophysics: Extreme emission seen from $\gamma$-ray bursts
• Neutrino Oscillations Within the Induced Gravitational Collapse Paradigm of Long Gamma-Ray Bursts
• On a GRB afterglow model consistent with hypernovae observations
• On the last stable orbit around rapidly rotating neutron stars
• The morphology of the X-ray afterglows and of the jetted GeV emission in long GRBs
• Supernovae Powered by Collapsar Accretion in Gamma-Ray Burst Sources
• Nature of the ultrarelativistic prompt emission phase of GRB 190114C
• Type Ic Supernova of a 22 ${\text{M}}_{\odot }$ Progenitor
• Simulations of Accretion Powered Supernovae in the Progenitors of Gamma Ray Bursts
• Induced Gravitational Collapse, Binary-Driven Hypernovae, Long Gramma-ray Bursts and Their Connection with Short Gamma-ray Bursts
• Energy Release on the Surface of a Rapidly Rotating Neutron Star during Disk Accretion: A Thermodynamic Approach
• GRB 190829A -- A Showcase of Binary Late Evolution
• The structure of the ultrarelativistic prompt emission phase and the properties of the black hole in GRB 180720B
• A Brief Review of Binary Driven Hypernova

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