Simple recipes for compact remnant masses and natal kicks
arXiv:2006.08360 · doi:10.1093/mnras/staa3043
Abstract
Based on recent results from three-dimensional supernova simulations and semi-analytical parametrised models, we develop analytical prescriptions for the dependence of the mass of neutron stars and black holes and the natal kicks, if any, on the pre-supernova carbon-oxygen core and helium shell masses. Our recipes are probabilistic rather than deterministic in order to account for the intrinsic stochasticity of stellar evolution and supernovae. We anticipate that these recipes will be particularly useful for rapid population synthesis, and we illustrate their application to distributions of remnant masses and kicks for a population of single stars.
Version accepted to MNRAS
References in corpus (13)
- Binary interaction dominates the evolution of massive stars
- GW190814: Gravitational Waves from the Coalescence of a 23 M Black Hole with a 2.6 M Compact Object
- Observational constraints on the progenitors of core-collapse supernovae : the case for missing high mass stars
- The Landscape of the Neutrino Mechanism of Core-Collapse Supernovae: Neutron Star and Black Hole Mass Functions, Explosion Energies and Nickel Yields
- The observed velocity distribution of young pulsars
- Hydrodynamics of core-collapse supernovae and their progenitors
- The Explosion of Helium Stars Evolved With Mass Loss
- Neutron star kicks by the gravitational tug-boat mechanism in asymmetric supernova explosions: progenitor and explosion dependence
- Three-dimensional Models of Core-collapse Supernovae From Low-mass Progenitors With Implications for Crab
- Black hole formation and fallback during the supernova explosion of a star
- Towards a Realistic Explosion Landscape for Binary Population Synthesis
- The Galactic distribution of X-ray binaries and its implications for compact object formation and natal kicks
- The Black Hole Formation Probability
Cited by in corpus (53)
- Observation of Gravitational Waves from the Coalescence of a Compact Object and a Neutron Star
- Multiple Stellar Evolution: a population synthesis algorithm to model the stellar, binary, and dynamical evolution of multiple-star systems
- The final core collapse of pulsational pair instability supernovae
- Binary black hole mergers from Population III stars: uncertainties from star formation and binary star properties
- Core-Collapse Supernovae in Binaries as the Origin of Galactic Hyper-Runaway Stars
- Interplay Between Neutrino Kicks and Hydrodynamic Kicks of Neutron Stars and Black Holes
- Heavy double neutron stars: birth, mid-life and death
- Stripped-envelope stars in different metallicity environments. II. Type I supernovae and compact remnants
- GW241011 and GW241110: Exploring Binary Formation and Fundamental Physics with Asymmetric, High-Spin Black Hole Coalescence
- A potential mass-gap black hole in a wide binary with a circular orbit
- X-ray emission from BH+O star binaries expected to descend from the observed galactic WR+O binaries
- An Observationally-Derived Kick Distribution for Neutron Stars in Binary Systems
- A Channel to Form Fast-spinning Black Hole--Neutron Star Binary Mergers as Multi-messenger Sources
- Calibration of neutron star natal kick velocities to isolated pulsar observations
- Explodability criteria for the neutrino-driven supernova mechanism
- Mass-transferring binary stars as progenitors of interacting hydrogen-free supernovae
- On the Neutron Star/Black Hole Mass Gap and Black Hole Searches
- Remnant masses from 1D+ core-collapse supernovae simulations: bimodal neutron star mass distribution and black holes in the low-mass gap
- Biases in estimates of black hole kicks from the spin distribution of binary black holes
- Exploring binary black hole mergers and host galaxies with Shark and COMPAS
- The Galactic Underworld: The spatial distribution of compact remnants
- Rapid population synthesis of black-hole high-mass X-ray binaries: implications for binary stellar evolution
- Lower-mass-gap Black Holes in Dense Star Clusters
- Populations of evolved massive binary stars in the Small Magellanic Cloud I: Predictions from detailed evolution models
- Black Hole Ultra-compact X-ray Binaries: Galactic Low-Frequency Gravitational Wave Sources
- Observational implications of cosmologically coupled black holes
- Kinematic constraints on the ages and kick velocities of Galactic neutron star binaries
- Formation of GW230529 from Isolated Binary Evolution
- New constraints on the Bray conservation-of-momentum natal kick model from multiple distinct observations
- Thermal luminosity degeneracy of magnetized neutron stars with and without hyperon cores
- Light Curves of Type IIP Supernovae from Neutrino-driven Explosions of Red Supergiants Obtained by a Semi-analytic Approach
- High mass function ellipsoidal variables in the Gaia Focused Product Release: searching for black hole candidates in the binary zoo
- The initial mass-remnant mass relation for core collapse supernovae
- VFTS 243 as predicted by the BPASS fiducial models
- On the large apparent black hole spin-orbit misalignment angle in GW200115
- A kinematically constrained kick distribution for isolated neutron stars
- Astrophysics with the Laser Interferometer Space Antenna
- Population Synthesis of Black Hole Binaries with Compact Star Companions
- Natal kicks of compact objects
- Formation and Stability of Area Quantized Black Holes
- A possible formation scenario of the Gaia ID 3425577610762832384: inner binary merger inside a triple common envelope
- On the Formation of GW190521-like Binary Black Hole Merger Systems
- Stellar-Mass Black Holes
- Probing Spin-Orbit Resonances with the Binary Black Hole Population
- Cosmology with Binary Neutron Stars: Does Mass-Redshift Correlation Matter?
- Challenges in Forming Millisecond Pulsar-Black Holes from Isolated Binaries
- SNR G292.0+1.8: A Remnant of a Low-Mass Progenitor Stripped-Envelope Supernova
- Astrometric microlensing probes of the isolated neutron star population with Roman
- Where are Gaia's small black holes?
- Forming Double Neutron Stars using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems
- Dynamical double black holes and their host cluster properties
- Proper Motion and Natal Kick in the Galactic Black Hole X-ray Binary AT2019wey
- A multi-wavelength study of GRS 1716-249 in outburst : constraints on its system parameters