Most Black Holes are Born Very Slowly Rotating

Abstract

The age of gravitational wave (GW) astronomy has begun, and black hole (BH) mergers detected by LIGO are providing novel constraints on massive star evolution. A major uncertainty in stellar theory is the angular momentum (AM) transport within the star that determines its core rotation rate and the resulting BH's spin. Internal rotation rates of low-mass stars measured from asteroseismology prove that AM transport is efficient, suggesting that massive stellar cores may rotate slower than prior expectations. We investigate AM transport via the magnetic Tayler instability, which can largely explain the rotation rates of low-mass stars and white dwarfs. Implementing an updated AM transport prescription into models of high-mass stars, we compute the spins of their BH remnants. We predict that BHs born from single stars rotate very slowly, with $a\sim 10^{-2}$, regardless of initial rotation rate, possibly explaining the low ${\chi }_{\mathrm{eff}}$ of most BH binaries detected by LIGO thus far. A limited set of binary models suggests slow rotation for many binary scenarios as well, although homogeneous evolution and tidal spin-up of post-common envelope helium stars can create moderate or high BH spins. We make predictions for the values of ${\chi }_{\mathrm{eff}}$ in future LIGO events, and we discuss implications for engine-powered transients.

arXiv commentAccepted to ApJ Letters

References in corpus (49)

• Modules for Experiments in Stellar Astrophysics (MESA)
• Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars
• Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions
• Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions
• Binary Black Hole Mergers in the first Advanced LIGO Observing Run
• Presupernova Evolution of Rotating Massive Stars I: Numerical Method and Evolution of the Internal Stellar Structure
• Dynamo action by differential rotation in a stably stratified stellar interior
• The Progenitor Stars of Gamma-Ray Bursts
• Presupernova Evolution of Differentially Rotating Massive Stars Including Magnetic Fields
• Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries
• Stellar evolution with rotation XI: Wolf-Rayet star populations at different metallicities
• Fast core rotation in red-giant stars revealed by gravity-dominated mixed modes
• Single star progenitors of long gamma-ray bursts I: Model grids and redshift dependent GRB rate
• Spin down of the core rotation in red giants
• The chemically homogeneous evolutionary channel for binary black hole mergers: rates and properties of gravitational-wave events detectable by advanced LIGO
• Merging black hole binaries in galactic nuclei: implications for advanced-LIGO detections
• Slowing the Spins of Stellar Cores
• Illuminating Black Hole Binary Formation Channels with Spins in Advanced LIGO
• Are merging black holes born from stellar collapse or previous mergers?
• Angular momentum transport within evolved low-mass stars
• Are LIGO's Black Holes Made From Smaller Black Holes?
• Rotational mixing in massive binaries: detached short-period systems
• Very Low Energy Supernovae from Neutrino Mass Loss
• The spin of the second-born black hole in coalescing binary black holes
• Spin orientations of merging black holes formed from the evolution of stellar binaries
• Spin-Orbit Misalignment in Close Binaries with Two Compact Objects
• The Masses and Spins of Neutron Stars and Stellar-Mass Black Holes
• A Highly Spinning and Aligned Binary Black Hole Merger in the Advanced LIGO First Observing Run
• Hierarchical analysis of gravitational-wave measurements of binary black hole spin-orbit misalignments
• White Dwarf Rotation as a Function of Mass and a Dichotomy of Mode Linewidths: Kepler Observations of 27 Pulsating DA White Dwarfs Through K2 Campaign 8
• Determining the population properties of spinning black holes
• Seismic evidence for a weak radial differential rotation in intermediate-mass core helium burning stars
• Stellar evolution with rotation XIII: Predicted GRB rates at various Z
• Core rotation braking on the red giant branch for various mass ranges
• The Origin of Black Hole Spin in Galactic Low-Mass X-ray Binaries
• Using spin to understand the formation of LIGO's black holes
• On the Origin of Black Hole Spin in High-mass X-Ray Binaries
• Constraints on Binary Black Hole Populations from LIGO-Virgo Detections
• GW150914: Spin based constraints on the merger time of the progenitor system
• Research Note: The Expected Spins of Gravitational Wave Sources With Isolated Field Binary Progenitors
• The evolution of black-hole mass and angular momentum
• Mass Ejection in Failed Supernovae: Variation with Stellar Progenitor
• Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity
• The Role of the Magnetorotational Instability in Massive Stars
• Black Hole Formation in Fallback Supernova and the Spins of LIGO Sources
• Rotation of Giant Stars
• The Formation of Rapidly Rotating Black Holes in High Mass X-ray Binaries
• The Angular Momenta of Neutron Stars and Black Holes as a Window on Supernovae
• Rotation and Magnetism of Massive Stellar Cores

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