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arxiv 1701.07223 v2 pith:P7RMD2NS submitted 2017-01-25 astro-ph.CO gr-qc

Constraints on Primordial Black Holes with Extended Mass Functions

classification astro-ph.CO gr-qc
keywords massconstraintsodotrangeblackholesprimordialeven
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Constraints on primordial black holes in the range $10^{-18} M_{\odot}$ to $10^{3} M_{\odot}$ are reevaluated for a general class of extended mass functions. Whereas previous work has assumed that PBHs are produced with one single mass, instead there is expected to be a range of masses even in the case of production from a single mechanism; constraints therefore change from previous literature. Although tightly constrained in the majority of cases, it is shown that, even under conservative assumptions, primordial black holes in the mass range $10^{-10} M_{\odot}$ to $10^{-8} M_{\odot}$ could still constitute the entirety of the dark matter. This stresses both the importance for a comprehensive reevaluation of all respective constraints that have previously been evaluated only for a monochromatic mass function, and the need to obtain more constraints in the allowed mass range.

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Cited by 3 Pith papers

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

  1. Dark ages bounds on non-accreting massive compact halo objects

    astro-ph.CO 2026-04 unverdicted novelty 5.0

    Upper bounds on the dark matter fraction in MACHOs of 10^3 to 10^7 solar masses are derived from limits on distortions to the global 21-cm signal at z~17, z~89, and z>300.

  2. CMB constraints on ultra-light primordial black holes with extended mass distributions

    astro-ph.CO 2019-07 unverdicted novelty 5.0

    For ultra-light PBHs with extended mass distributions, new CMB-derived 95% exclusion bounds on f_PBH are obtained by jointly varying ΛCDM parameters, yielding f_PBH < 1.6 × 10^{-5} for a uniform distribution between 1...

  3. Primordial Black Holes as Dark Matter: Recent Developments

    astro-ph.CO 2020-06 unverdicted novelty 3.0

    Primordial black holes in specific mass ranges could account for some or all dark matter while resolving structure-formation and seed problems in standard cosmology.