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Supermassive Black Holes and the Evolution of Galaxies
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Black holes, an extreme consequence of the mathematics of General Relativity, have long been suspected of being the prime movers of quasars, which emit more energy than any other objects in the Universe. Recent evidence indicates that supermassive black holes, which are probably quasar remnants, reside at the centers of most galaxies. As our knowledge of the demographics of these relics of a violent earlier Universe improve, we see tantalizing clues that they participated intimately in the formation of galaxies and have strongly influenced their present-day structure.
Forward citations
Cited by 18 Pith papers
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Clustering of high-redshift quasars with DESI DR2
DESI DR2 quasar sample yields bias b_Q(z=2.48)=3.61 that evolves as b(z)=0.230[(1+z)^2-6.565]+2.394, consistent with constant ~10^12 M_sun halo mass and weak luminosity dependence at fixed redshift.
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Recycled Gas Dominates the Metal-rich Fuel of Supermassive Black Holes
In simulated massive galaxies, recycled stellar ejecta from inside the host galaxy dominate the metal-rich gas accreted by supermassive black holes, naturally explaining high and weakly evolving quasar metallicities.
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Pulsar Timing Array Sensitivity to Anisotropy: Empirical Sensitivity Curves, Scaling Relations, and the Multi-Resolution Pixel Basis
PTA anisotropy sensitivity scales as Npsr^0.8, delta-t^-0.08, and angular-scale exponents 1.6 to 2.1, and a new multi-resolution pixel basis is demonstrated.
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Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$
In z≈6 quasar simulations, super-Eddington black-hole growth clears escape channels, ejects cold clumps that raise neutral-hydrogen covering, and powers extended Hα nebulae that shrink when the quasar is obscured.
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Memoirs of the curvaton: non-perturbative non-Gaussianity and supermassive primordial black holes
Curvaton self-interactions in non-quadratic potentials produce a local non-Gaussian map that enables supermassive primordial black hole formation at peak amplitudes of order 10^{-5} while remaining consistent with μ-d...
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Uncertainties in the supermassive black hole abundance and implications for the GW background
Cross-catalog offsets in black hole mass proxies shift the predicted nHz gravitational wave background by factors comparable to PTA uncertainties; matching the observed amplitude requires a selection effect of about o...
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Characterizing the roles of transitory obscured phases and inner torus in shaping the fractions of obscured AGN at cosmic noon
Pure evolutionary AGN light curves can only reproduce cosmic-noon obscured fractions if the visible phase is tuned by luminosity or if a long-lived torus is added; starbursts and mergers alone cannot.
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Premature supermassive black hole mergers in cosmological simulations of structure formation
Most supermassive black hole mergers in the FABLE simulation occur prematurely, and correcting for this adds median 1.3 Gyr delays that suppress high-mass merger rates and alter LISA and pulsar timing array predictions.
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Evolution of SMBHs in light of PTA measurements: implications for growth by mergers and accretion
A simplified two-stage model shows that the pulsar timing array gravitational wave background implies a direct, possibly uncomfortable, link between black hole merger rates and quasar Eddington ratios.
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A Supermassive Black Hole Mass Measurement in NGC 5102 with Schwarzschild Orbit-superposition Modeling
The central black hole in NGC 5102 has a mass of (1.30+0.19−0.18)×10^6 solar masses, measured with Schwarzschild orbit-superposition models of STIS and MUSE stellar kinematics.
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Lattice study of primordial black hole formation in bumpy axion inflation
Lattice simulations of bumpy axion U(1) inflation in the strong backreaction regime generate curvature perturbations large enough for primordial black holes to comprise all dark matter.
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Insights from Analytical Theory of Eccentric Circumbinary Disks II. Forced Modes and Resonance for Precessing Binaries
Semi-analytical theory derives radial scalings for forced disk eccentricity (E ~ r^{-1} or r^{-2}) and resonance criteria for precessing binaries, plus a conjecture that cavity size tunes the ground eccentric mode to ...
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Thermodynamics of Kerr-Bertotti-Robinson black hole
A consistent thermodynamics of the Kerr-Bertotti-Robinson black hole is constructed by adopting the Christodoulou-Ruffini mass relation, yielding a first law and Smarr formula without an explicit magnetic-field work term.
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Constraints on the extreme mass-ratio inspiral population from LISA data
A neural-network-accelerated hierarchical Bayesian pipeline is developed and validated on a phenomenological model to constrain EMRI population parameters from LISA data.
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New estimates of the spin and accretion rate of the black hole M87*
Using Doppler beaming of the EHT image of M87*, the authors derive a spin parameter a ~ 0.8 and an accretion rate between 4e-5 and 4e-1 solar masses per year.
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A Survey of General Relativistic Magnetohydrodynamic Models for Black Hole Accretion Systems
A new public GRMHD simulation library of MAD and SANE accretion flows across five black hole spins confirms SANE spin equilibrium near a*~0.94 and MAD jet-powered spin-down.
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Accretion Disk Luminosity and Topological Characteristics for a Schwarzschild Black Hole Surrounded by a Hernquist Dark Matter Halo
For a model black hole embedded in a Hernquist dark matter halo, the paper computes accretion disk flux, luminosity, efficiency, quasi-normal modes and topological charges, all shifting systematically with halo densit...
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Constraining the Mass of a Hypothetical Secondary Black Hole in M87 with the NANOGrav 15-Year Data Set
Combining the NANOGrav 15-yr background, the merger limit, and a reflex-motion threshold gives q = 6.9e-3 to 4.2e-2 for an 11-year orbit and q = 3.7e-2 to 1 for a 0.9-year orbit in M87.
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