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Baumgardt, De Marchi & Kroupa (2008)

San Diego State University

Abstract (paraphrased)

Demonstrates that primordial mass segregation can explain both the IMF-slope-vs-concentration trend and the depletion of low-mass stars in globular clusters. progenax uses this paper as the physical motivation for primordial segregation; the implemented energy-ordered IC machinery is exposed through the progenax.cluster layer.

Use in progenax

Notes

The canonical primordial segregation IC algorithm: most massive stars onto the most bound orbits of an equilibrium pool, with bin widths proportional to cumulative mass.

Deliberate, documented departure from the published recipe. Baumgardt+2008 draw orbits randomly within cumulative-mass bins; progenax’s energy_sorted_segregation instead uses a deterministic isotonic rounding of the bin-centre targets to a strictly increasing orbit-index sequence. The random per-bin draw fails for steep IMFs — cumulative-mass bins collapse below one orbit, forcing many low-mass ranks onto the same orbit (coincident stars, V=V = -\infty). The deterministic assignment guarantees a distinct orbit per star for any mass spectrum; realisation variety comes from re-drawing the random orbit pool. See the module docstring of src/progenax/cluster/mass_segregation.py.

The historical λ_seg catalog blend that once smoothed this construction was retired in the 2026-06 unified redesign (its intermediate states drift from per-mass-group virial balance); differentiable segregation control now comes from the equilibrium MultiComponentCluster.from_mass_segregation route.

References
  1. Baumgardt, H., De Marchi, G., & Kroupa, P. (2008). Evidence for primordial mass segregation in globular clusters. The Astrophysical Journal, 685, 247–253. 10.1086/590488