EpiStack

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EpiStack v1 — FLF competition

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analysis tests

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black holes1

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hypotheses

Folder: v1/analysis-tests/black-holes1/hypotheses

10 items under this folder.

  • Jul 20, 2026

    H-1 - Stable LHC black holes trapped in Earth would accrete it catastrophically within the solar lifetime

    • Jul 20, 2026

      H-10 - The exogenous terminal-catastrophe rate is not bounded below 1 per Gyr

      • Jul 20, 2026

        H-2 - Stable LHC black holes pose no macroscopic risk to Earth within the solar lifetime

        • Jul 20, 2026

          H-3 - Two or more large compact extra dimensions lower the fundamental gravity scale to about a TeV

          • Jul 20, 2026

            H-4 - Black holes radiate thermally and evaporate, so a TeV-mass black hole would decay near-instantly

            • Jul 20, 2026

              H-5 - The exogenous terminal-catastrophe rate is below about 1 per Gyr at 99.9 percent confidence

              • Jul 20, 2026

                H-6 - Stable LHC black holes have some fate or impact not listed here

                • Jul 20, 2026

                  H-7 - Hawking evaporation fails and TeV-mass black holes are long-lived

                  • Jul 20, 2026

                    H-8 - The fundamental gravity scale is far above LHC energies so no black holes form

                    • Jul 20, 2026

                      H-9 - TeV-scale gravity arises via some mechanism not listed here


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