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globular-clusters

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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 27, 2026
  • Python

This aim of this project is to analyze globular star clusters in the Milky Way, in order to understand their dynamics. The conducted study examined the properties that affect the central velocity dispersion, their impact and the correlations between them.

  • Updated Feb 24, 2024
  • HTML

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