The Origin of Black Hole Spin in Galactic Low-Mass X-ray Binaries

Abstract

Galactic field black hole (BH) low-mass X-ray binaries (LMXBs) are believed to form in situ via the evolution of isolated binaries. In the standard formation channel, these systems survived a common envelope phase, after which the remaining helium core of the primary star and the subsequently formed BH are not expected to be highly spinning. However, the measured spins of BHs in LMXBs cover the whole range of spin parameters. We propose here that the BH spin in LMXBs is acquired through accretion onto the BH after its formation. In order to test this hypothesis, we calculated extensive grids of detailed binary mass-transfer sequences. For each sequence, we examined whether, at any point in time, the calculated binary properties are in agreement with their observationally inferred counterparts of 16 Galactic LMXBs. The "successful" sequences give estimates of the mass that the BH has accreted since the onset of Roche-Lobe overflow. We find that in all Galactic LMXBs with measured BH spin, the origin of the spin can be accounted for by the accreted matter, and we make predictions about the maximum BH spin in LMXBs where no measurement is yet available. Furthermore, we derive limits on the maximum spin that any BH can have depending on current properties of the binary it resides in. Finally we discuss the implication that our findings have on the BH birth-mass distribution, which is shifted by ~1.5 Msolar towards lower masses, compared to the currently observed one.

arXiv comment17 pages, 8 Figures, 5 Tables. Revisions to address referee's comments. Accepted for publication to ApJ

References in corpus (98)

• Modules for Experiments in Stellar Astrophysics (MESA)
• Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars
• X-ray Properties of Black-Hole Binaries
• The Supernova -- Gamma-Ray Burst Connection
• Common Envelope Evolution: Where we stand and how we can move forward
• Compact Remnant Mass Function: Dependence on the Explosion Mechanism and Metallicity
• Pre-Supernova Evolution of Massive Single and Binary Stars
• Presupernova Evolution of Differentially Rotating Massive Stars Including Magnetic Fields
• The Black Hole Mass Distribution in the Galaxy
• On The Maximum Mass of Stellar Black Holes
• The Spin of the Near-Extreme Kerr Black Hole GRS 1915+105
• Hot Jupiters from Secular Planet--Planet Interactions
• Black Hole Spin in X-Ray Binaries: Observational Consequences
• The Mass Distribution of Stellar-Mass Black Holes
• 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
• Secular Dynamics in Hierarchical Three-Body Systems
• Estimating the Spin of Stellar-Mass Black Holes via Spectral Fitting of the X-ray Continuum
• The Mass of the Black Hole in Cygnus X-1
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• Black Hole Spin via Continuum Fitting and the Role of Spin in Powering Transient Jets
• An unusually massive stellar black hole in the Galaxy
• Simulations of Magnetized Disks Around Black Holes: Effects of Black Hole Spin, Disk Thickness, and Magnetic Field Geometry
• X-ray irradiation in low mass binary systems
• Precise mass and spin measurements for a stellar-mass black hole through X-ray timing: the case of GRO J1655-40
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• The Extreme Spin of the Black Hole in Cygnus X-1
• A Parallax Distance to the Microquasar GRS 1915+105 and a Revised Estimate of its Black Hole Mass
• Mass Measurements of Black Holes in X-Ray Transients: Is There a Mass Gap?
• The Rates of Hypernovae and Gamma-Ray Bursts: Implications for their Progenitors
• Dynamical Evidence for a Black Hole in GX 339-4
• A Black Hole in the Superluminal source SAX J1819.3-2525 (V4641 Sgr)
• Mergers and Obliquities in Stellar Triples
• Optical and Infrared Photometry of the Micro-Quasar GRO J1655-40 in Quiescence
• Investigating stellar-mass black hole kicks
• Observational Evidence for a Correlation Between Jet Power and Black Hole Spin
• The Spin of the Black Hole Microquasar XTE J1550-564 via the Continuum-Fitting and Fe-Line Methods
• An Improved Dynamical Model for the Microquasar XTE J1550-564
• High-Frequency Quasi-Periodic Oscillations in black-hole binaries
• Three-Dimensional Simulations of Magnetized Thin Accretion Disks around Black Holes: Stress in the Plunging Region
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• Confirmation Via the Continuum-Fitting Method that the Spin of the Black Hole in Cygnus X-1 is Extreme
• The Inclination of the Soft X-ray Transient A0620--00 and the Mass of its Black Hole
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• Measuring Black Hole Spin by the Continuum-Fitting Method: Effect of Deviations from the Novikov-Thorne Disc Model
• Orbital Parameters for the Soft X-ray Transient 4U 1543-47: Evidence for a Black Hole
• Understanding Compact Object Formation and Natal Kicks I. Calculation Methods and the case of GRO J1655-40
• Confronting the models of 3:2 quasiperiodic oscillations with the rapid spin of the microquasar GRS 1915+105
• Jet Power and Black Hole Spin: Testing an Empirical Relationship and Using it to Predict the Spins of Six Black Holes
• Identification of the donor in the X-ray binary GRS 1915+105
• Failed Supernovae Explain the Compact Remnant Mass Function
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• Understanding Compact Object Formation and Natal Kicks: II. The case of XTE J1118+480
• Black hole spin measurements through the relativistic precession model: XTE J1550-564
• Precise Measurement of the Spin Parameter of the Stellar-Mass Black Hole M33 X-7
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• The Eye of the Storm: Light from the Inner Plunging Region of Black Hole Accretion Discs
• The not-so-massive black hole in the microquasar GRS1915+105
• The rotational broadening and the mass of the donor star of GRS 1915+105
• Observational constraints on the powering mechanism of transient relativistic jets
• Understanding Compact Object Formation and Natal Kicks. III. The case of Cygnus X-1
• The Spin of the Black Hole in the Soft X-ray Transient A0620--00
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• Formation of the black-hole binary M33 X-7 via mass-exchange in a tight massive system
• The X-ray transient XTE J1859+226 in Outburst & Quiescence
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• The Mass of the Black Hole in LMC X-3
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• Infrared Observations of Nova Muscae 1991: Black Hole Mass Determination from Ellipsoidal Variations
• Long Gamma-Ray Burst Progenitors: Boundary Conditions and Binary Models
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• Hydrodynamical Simulations of the Stream-Core Interaction in the Slow Merger of Massive Stars
• Understanding Compact Object Formation and Natal Kicks. IV. The case of IC 10 X-1
• The Eccentric Accretion Disc of the Black Hole A0620-00
• The fast spiral-in of the companion star to the black hole XTE J1118+480
• Constraints on the Size of Extra Dimensions from the Orbital Evolution of Black-Hole X-Ray Binaries
• Hydrogen-Poor Disks in Compact X-Ray Binaries
• Spin Tilts in the Double Pulsar Reveal Supernova Spin Angular-Momentum Production
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• The Spin of the Black Hole GS 1124-683: Observation of a Retrograde Accretion Disk?
• The need for hypercritical accretion in massive black-hole binaries with large Kerr parameters
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• On the origin of black hole spin in high-mass black hole binaries: Cygnus X-1
• Chemical Abundances in the Secondary Star of the Black Hole Binary V4641 Sagittarii (SAX J1819.3-2525)

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