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Constraints on Primordial Black Holes: the Importance of Accretion

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arxiv 2003.12589 v2 pith:7EWSVFMA submitted 2020-03-27 astro-ph.CO gr-qchep-ph

classification astro-ph.COgr-qchep-ph
keywords accretionblackconstraintsholesprimordialmassmassesaccount
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We consider the constraints on the fraction of dark matter in the universe in the form of primordial black holes taking into account the crucial role of accretion which may change both their mass and mass function. We show that accretion may drastically weaken the constraints at the present epoch for primordial black holes with masses larger than a few solar masses.

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Forward citations

Cited by 8 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. The cosmic history of Primordial Black Hole accretion and its uncertainties

    astro-ph.CO 2024-12 conditional novelty 7.0 of 10

    Accounting for radiative feedback and formation-time effects, accretion grows primordial black holes by at most a few percent in the radiation era and negligibly in the baryonic Park-Ricotti model, while the Bondi mod...

  2. Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope

    astro-ph.IM 2026-07 accept novelty 6.0 of 10

    Degrading the Einstein Telescope's sensitivity in specific frequency bands hurts different science goals in predictable ways, but the mission remains scientifically strong even in the worst modelled cases.

  3. Reconstruction of Primordial Power Spectrum from Gravitational Waves of High-Redshift Black Hole Binaries

    astro-ph.CO 2026-07 conditional novelty 6.0 of 10

    Gradient-descent inversion of redshifted BBH mass distributions recovers the PBH mass function and, via regularized Press-Schechter, a candidate O(10^{-2}) bump in the small-scale primordial power spectrum.

  4. Primordial Black Hole mass growth from neutrinos during the radiation era

    astro-ph.CO 2026-07 conditional novelty 6.0 of 10

    PBHs of ~1e3–1e7 solar masses can significantly grow by absorbing neutrinos before matter-radiation equality.

  5. Effect of post-recombination accretion on primordial binary black hole mergers within virialized dark matter halos

    astro-ph.CO 2026-07 conditional novelty 6.0 of 10

    BHL-type post-recombination accretion can raise late three-body PBH merger rates enough for TianQin detections at f~10^{-6} and for LVK limits to bound delayed virialization.

  6. Closing the Mass Window for Stupendously Large Black Holes

    astro-ph.CO 2025-08 conditional novelty 5.0 of 10

    Primordial black holes heavier than about 10^11 solar masses generate isocurvature perturbations that violate Planck CMB and BAO bounds, ruling them out as a significant dark matter component.

  7. January Food Benchmark (JFB): A Public Benchmark Dataset and Evaluation Suite for Multimodal Food Analysis

    cs.CV 2025-08 reject novelty 4.0 of 10

    The abstract promises a food-image benchmark and a winning model, but the manuscript pages contain only a different paper on primordial black holes, leaving every benchmark claim unsubstantiated.

  8. Relativistic accretion and burdened primordial black holes

    astro-ph.CO 2025-07 conditional novelty 4.0 of 10

    Combining relativistic accretion with memory-burdened evaporation widens the parameter space for primordial black holes as dark matter and changes dark matter and dark radiation emission predictions.

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