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millisecond-pulsars

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Temporal Equivalence Principle: Suppressed Density Scaling in Globular Cluster Pulsars — 199 cluster vs 351 field millisecond pulsars show a +0.61 dex controlled spin-down residual (5.8σ) and suppressed density scaling (Γ=0.39±0.08 vs Newtonian 0.72), while 20-cluster CMC N-body realizations overpredict the excess by 3.2× (8.6σ).

  • Updated Oct 17, 2026
  • Python

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