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¶
Mass segregation — energy-ranked algorithm, two released routes
progenax.energy_sorted_segregation— the PRIMORDIAL energy-ordered generator (public API)MultiComponentCluster.from_mass_segregation(delta)— the separate differentiable equilibrium route (not from this paper; equipartition law after Gieles & Zocchi 2015)
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, ). 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.
- 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