Black holes capable of Eddington-limited accretion and radiation are also subject to astrophysical retention bounds.
Assessment
The evidence favors the claim, but the examination is incomplete or the evidence is indirect.
This claim is the linchpin of the Giddings and Mangano safety argument for hypothetical TeV-scale black holes: any black hole that could accrete and radiate near the Eddington limit, as in Plaga's proposed hazard scenario, would by the same physics be produced by cosmic rays striking white dwarfs and neutron stars, be stopped inside them, and accrete there faster than it could on Earth, so the observed survival of those stars bounds its behavior. Each step of that chain now rests on peer-reviewed calculation and stands supported: cosmic-ray production inside compact stars, stopping of both charged and neutral black holes, the density-scaling comparison between terrestrial and compact-star accretion, and the constraint that stellar survival places on accretion rates.
The only published objection is Plaga's, who argued that Eddington-limited micro black holes could evade the astrophysical bounds. Giddings and Mangano's rebuttal, corroborated independently by Casadio, Fabi and Harms, found that scenario internally inconsistent: the Eddington argument does not apply at the relevant microscopic radii, and the radiated power was overstated by many orders of magnitude. Plaga's position was maintained only in unrefereed revisions and gained no independent support. The claim falls short of verified only because it concerns hypothetical objects whose existence may never be tested directly; a refereed technical rebuttal of the stopping calculation or the density-scaling step would be needed to reopen the question.
Full reasoning: the evidence and decisions behind this verdict
Trigger: the density-scaling bridge, "a black hole accreting hazardously fast on Earth would accrete faster inside white dwarfs or neutron stars," received its first assessment: SUPPORTED (confidence 0.8, credence 0.88). The prior verdict here (SUPPORTED, 0.86) had named this bridge as the sole remaining unassessed dependency, so the change is material in the confirming direction and closes the last named gap.
State of the subclaims. All four legs of the same-physics coverage argument now stand supported: production by cosmic rays on compact stars (0.8), stopping inside those stars whether charged or neutral (0.8), the density-scaling bridge (0.8, credence 0.88, with Plaga's Eddington-limit objection to this step evaluated as failing, found inconsistent by Giddings-Mangano and by Casadio-Fabi-Harms), and the constraint from white dwarf and neutron star survival (0.88). The against-argument's sole premise, that Eddington-limited accretion would evade astrophysical observations, stands contradicted (0.75, credence 0.12).
Instances. The single instance affirms the claim (Giddings and Mangano, arXiv:0808.4087). The only denial in the discourse is Plaga's unrefereed reply, whose key premises are now assessed contradicted or failing; this is not credible two-sided contestation.
Verdict. SUPPORTED, confidence raised from 0.86 to 0.90: every dependency is now assessed, the supporting chain is complete and favorable, and the counter-argument has been examined at each step and found wanting. This follows an adversarial examination of the strongest published objection rather than a one-sided reading. VERIFIED remains unavailable in principle: the derivation concerns hypothetical TeV-scale black holes whose premises may never be instantiated, so the chain cannot terminate in direct observation of the objects themselves. Credence 0.88, tracking the now-assessed weakest links of the chain, which share a common peer-reviewed basis with independent corroboration.
What would change the conclusion: a refereed technical rebuttal of the stopping calculation or the density-scaling step, a downgrade of any supporting leg to contested or contradicted, or independent corroboration of Plaga's evasion mechanism that survives peer review.
Decomposition
How this claim breaks down: each argument is stated as it runs, with its subclaims linked inline. ↗︎ opens a subclaim; the map shows how they fit together.
Because If TeV-scale black hole production is possible in particle collisions, cosmic rays striking white dwarfs or neutron stars would produce such black holes. and Stable microscopic black holes produced by cosmic rays striking white dwarfs or neutron stars would be stopped inside those stars, whether charged or neutral., any black hole capable of Eddington-limited accretion and radiation would also arise and be retained inside compact stars. Given that A black hole accreting hazardously fast on Earth would accrete faster inside white dwarfs or neutron stars., and because Survival of white dwarfs and neutron stars constrains TeV-scale black hole accretion rates., such black holes fall squarely within the regime the compact-star survival bounds constrain, so the claim follows.
Because Eddington-limited accretion by metastable micro black holes would evade existing astrophysical observations., the compact-star survival record would carry no information about such objects, and the retention bounds would fail to reach the Eddington-limited scenario, contrary to the claim.
Provenance
Where this claim has been said, linked to its canonical form.
the same physics that would allow a black hole to accrete and radiate as Plaga describes also forces it into the regime where their astrophysical bounds apply, so the proposed "gap" does not exist
Giddings and Mangano's rebuttal (arXiv:0808.4087) to Plaga's central claim.
Assessment history
0 status changes over 5 assessments. full history →
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Created by extractor · Jul 17, 2026. Every judgment on this page is accompanied by a reasoning trace.