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List of bounds

Check each individual file to find out precisely which constraint I'm using. Constraints which are not strictly valid for monochromatic mass functions are marked with an asterisk (*). Projected constraints are marked with a dagger (†). Constraints which are now generally discredited are marked with a 'slashed zero' (ø).

  • 3G-GW-1y, 3G-GW-10y†: Projected constraints from 3G Gravitational Wave detectors (based on 1 year and 10 years of operation) - arXiv:2111.06990
  • 511keV: Constraints on PBH evaporation from the 511 keV gamma ray line - arXiv:1906.09994 and arXiv:1906.07740
  • 511keV-DeLaTorreLuque2024: Updated PBH evaporation constraints from 511 keV line - arXiv:2406.11949
  • AMS: Constraints from AMS-02, due to positron + electron production by evaporation - arXiv:2403.04988
  • Comptel: Constraints from PBH evaporation using Comptel GC observations - arXiv:2010.04797
  • CMB: Constraints from modification of the CMB spectrum due to accreting PBHs, including particle DM accretion - arXiv:2002.10771
  • CMB-Agius2024: Updated CMB constraints from accreting PBHs, assuming Park-Ricotti accretion model - arXiv:2403.18895
  • CMBevap: Constraints from modification of the CMB spectrum due to evaporating PBHs - arXiv:1612.07738
  • EROS: Microlensing constraints from EROS - astro-ph/0607207
  • EDGES: Constraints from energy injection in the 21cm EDGES signal due to accreting PBHs - arXiv:1803.09697
  • EDGESevap-Clark2018: Constraints from energy injection in the 21cm EDGES signal due to evaporating PBHs - Clark et al., arXiv:1803.09390
  • EDGESevap-Mittal2021: Constraints from energy injection in the 21cm EDGES signal due to evaporating PBHs - Mittal et al., arXiv:2107.02190
  • EDGESevap-Saha2021: Constraints from energy injection due to evaporating PBHs (rotating and non-rotating), leading to an EDGES-like 21cm signal - Saha & Laha, arXiv:2112.10794
  • EGRB: Constraints on PBH evaporation from extragalactic gamma-rays - arXiv:0912.5297
  • FLø: Femto-lensing of gamma-ray bursts - arXiv:1204.2056
  • FL-small†: Femto-lensing of small gamma-ray bursts - arXiv:1807.11495
  • FRB: Non-observation of lensing of Fast Radio Bursts - arXiv:2003.13349
  • FRB-Leung2022: Updated constraints on FRB Lensing with CHIME/FRB - arXiv:2204.06001
  • GECCO†: Projections for evaporation constraints from MeV-gamma ray telescope GECCO - arXiv:2101.10370
  • GRB-parallax†: Lensing parallax of 1000 GRBs (using spatially separated telescopes) - arXiv:1908.00078
  • GW-lensing†: Microlensing of GWs by PBHs - arXiv:1712.01396
  • HSC: Microlensing constraints from the Hyper-Supreme Cam - arXiv:1701.02151, updated in arXiv:1910.01285 and then again in arXiv:2007.12697
  • Icarus: Icarus microlensing event ('caustic crossing') - arXiv:1710.00148
  • INTEGRAL: Constaints from MeV background from evaporating PBHs - arXiv:2004.00627
  • K: Microlensing constraints from Kepler - arXiv:1307.5798
  • Leo-I: Dynamics of Leo-I - arXiv:1906.10463
  • Leo-T: Heating due to dynamic friction and accretion in Leo T - arXiv:2007.02213
  • Leo-Tevap: Heating due to evaporation in dwarf galaxy Leo T - arXiv:2007.07739
  • LIGO: Direct constraints on PBH-PBH mergers with LIGO - arXiv:1805.09034 and arXiv:1904.08976
  • LIGO-perturbed: Conservative constraints on PBH-PBH mergers incorporating effects of binary perturbations - arXiv:1908.09752
  • LIGO-HMR*: Constraints on PBH-PBH mergers in which one PBH is ~37 solar mass and the other is sub-solar - arXiv:2202.11024
  • LIGO-subsolar: Constraints on PBH fraction from direct searches for gravitational waves from subsolar mass binary black hole mergers in LVK O1+O2+O3 data - arXiv:2202.11024
  • LIGO-SGWB-O2: Stochastic BG of PBH mergers with LIGO (Observing Run 2) - arXiv:1904.02396
  • LIGO-SGWB-O3: Stochastic BG of PBH mergers with LIGO (Observing Run 3) - arXiv:2202.11024
  • LIGO-SGWB-O1-O2-O3: Stochastic BG of PBH mergers with the first three LIGO observing runs. Bayesian constraints using a narrow log-normal mass function ("MN prior") - arXiv:2412.18318
  • LVK-SGWB-subsolar: Stochastic GW background constraints for LVK O3 run - arXiv:2202.11024
  • LyaEvap-Khan2025: Constraints on evaporating PBHs from Lyman-alpha forest temperature measurements - Khan et al., arXiv:2503.15595
  • Lyalphaforest: Ly-alpha forest constraint from the shot noise power spectrum arXiv:1903.10509
  • M: Microlensing constraints from MACHO - astro-ph/0011506
  • Microlensing: envelope of EROS, HSC, K and M
  • Microlensing-LongDuration: Constraints from long-duration microlensing, combining EROS and MACHO results - arXiv:2202.13819
  • NANOGrav: Scalar-induced GWs with NANOGrav - arXiv:1910.12239
  • NSø: Neutron star capture and destruction - arXiv:1301.4984
  • OGLE-highcadence: Constraints on planetrary mass PBHs from high-cadence OGLE observations - arXiv:2410.06251
  • OGLE-strict: Most recent OGLE bounds from 20 year observations (OGLE-III + OGLE-IV), assuming no PBH-induced microlensing events. Other options are OGLE-MW1 and OGLE-MW2, which correspond to the Cautun+ (2020) and Han & Gould (2003) Milky Way models respectively - arXiv:2403.02398, arXiv:2403.02386
  • OGLE-hint: Hint for Earth mass PBHs with OGLE - arXiv:1901.07120
  • OGLE-2019: Microlensing constraints from OGLE 5-year observations - arXiv:1901.07120
  • PBH-EMRIs†: Extreme mass-ratio inspirals of PBHs around supermassive black holes - arXiv:1910.07397
  • PTA-Doppler†: PBH-induced motions in Pulsar Timing Arrays - arXiv:1901.04490
  • PTA-Shapiro†: PBH-induced time delays in Pulsar Timing Arrays - arXiv:1901.04490
  • Quasars: Constraints from microlensing of quasars - arXiv:2203.04777
  • Quasars-Xray: Constraints from visible and X-ray microlensing of quasars (including and extending results of Quasars, arXiv:2203.04777, to lower masses) - arXiv:2307.07473
  • Radio: Radio constraints on accreting PBHs in the Milky Way - arXiv:1812.07967
  • SKA†: Forecast for the 21 cm power spectrum from SKA - arXiv:1906.07735
  • SNe-Lensing: Lensing of supernovae by PBHs - arXiv:1712.02240
  • SuperK: Bounds from evaporation into neutrinos from SuperKamiokande - arXiv:1912.01014
  • UFdwarfs: Constraints from the disruption of ultra-faint dwarfs - arXiv:1605.03665
  • WhiteDwarfmicro†: Projected microlensing constraints assuming observation of 1000 White Dwarfs in the LMC - arXiv:1905.06066
  • Voyager: Constraints on PBH evaporation from electron/positron measurements by Voyager 1 probe - arXiv:1807.03075
  • Voyager-DeLaTorreLuque2024: Updated constraints on PBH evaporation from electron/positron measurements by Voyager 1 probe - arXiv:2406.11949
  • WideBinaries: Constraints from disruption of Wide Binaries - arXiv:1406.5169
  • WDø: Constraints from the destruction of White Dwarfs by PBHs - arXiv:1505.04444
  • X-ray: X-ray constraints on accreting PBHs in the Milky Way - arXiv:1812.07967
  • Xrayevap: X-ray background constraint from evaporating PBHs - arXiv:2404.17119
  • Xrayevap-DeLaTorreLuque2024: X-ray background constraint from evaporating PBHs (with XMM-Newton) - arXiv:2406.11949
  • Xraylensing-NICER: Constraints from X-ray microlensing with NICER (1.74d) - arXiv:2405.20365
  • Xraylensing-eXTP-proj†: Projected constraints from microlensing of X-ray pulsars - arXiv:1812.01427
  • Xraylensing-NICER-proj†: Projected constraints from X-ray microlensing with NICER (60d) - arXiv:2405.20365
  • Xraylensing-STROBEX-proj†: Projected constraints from X-ray microlensing with STROBE-X (30d) - arXiv:2405.20365
  • Xraylensing-Xmu-proj†: Projected constraints from X-ray microlensing with Xmu (30d) - arXiv:2405.20365