Limits on Primordial Black Hole Evaporation from LUX-ZEPLIN

arXiv:2609.29462 · astro-ph.CO, gr-qc, hep-ph · Submitted 2026-09-24 · Read on arXiv

astro-ph.CO, gr-qc, hep-ph

Submitted: 2026-09-24

Updated: 2026-10-01

Terminology

• Abundance — 10× in this paper · explained in 1 episode
• Momentum transfer — 9× in this paper · explained in 2 episodes
• Cold Dark Matter — 5× in this paper
• No-Go Theorem — 3× in this paper · explained in 2 episodes
• Weakly Interacting Massive Particle — 2× in this paper
• Primordial Black Holes (PBHs) — 1× in this paper · explained in 7 episodes

Sources

• Planck 2018 results. VI. Cosmological parameters
• A direct empirical proof of the existence of dark matter
• Particle Dark Matter: Evidence, Candidates and Constraints
• Planck 2018 results. I. Overview and the cosmological legacy of Planck
• Supersymmetric Dark Matter
• WIMP dark matter candidates and searches - current status and future prospects
• Direct Detection of WIMP Dark Matter: Concepts and Status
• Direct Detection of Dark Matter -- APPEC Committee Report
• First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment
• First Dark Matter Search with Nuclear Recoils from the XENONnT Experiment
• Dark Matter Search Results from the PandaX-4T Commissioning Run
• Dark Matter Search Results from a One Tonne$\times$Year Exposure of XENON1T
• Projected WIMP sensitivity of the LUX-ZEPLIN (LZ) dark matter experiment
• Inelastic Dark Matter
• Candidates for Inelastic Dark Matter
• A Theory of Dark Matter
• Inelastic Dark Matter in Light of DAMA/LIBRA
• The Inelastic Frontier: Discovering Dark Matter at High Recoil Energy
• A Model Independent Approach to Inelastic Dark Matter Scattering

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