The big idea¶
Two clouds with the same dense-gas mass can form stars at different rates if their density gradients differ: a centrally-concentrated clump has more of its mass at high density, where the local free-fall time is short, so it forms stars faster than a uniform (“top-hat”) clump of the same mass. PP20 capture this geometric boost with a single magnification factor , so that
is the top-hat lower limit; for any centrally-concentrated profile.
Physical & observational context (Sections 1–3)¶
The dense-gas star-formation law — , equivalently — is observationally near-linear (Lada et al. 2010 find ) but carries real scatter. PP20’s thesis is that the scatter is not purely random: it partly tracks the cloud’s internal density gradient. Steeper gradients (larger ) push more mass into the short-free-fall-time inner region, raising . The two key inputs PP20 separate (their Eq. 2) are the intrinsic efficiency per free-fall time (a true SF-physics number) and the purely geometric boost — so that measuring a cloud’s gradient unlocks its and lets one read cleanly from the data.
The radial slope is inferred observationally from the cloud -pdf or projected -pdf: for a power-law tail of index in the -pdf, (Kritsuk et al. 2011); in the Kainulainen et al. (2014) notation. The Kainulainen sample has a mean (range ), which is the canonical observational anchor: . PP20 also apply the framework to the Central Molecular Zone (CMZ), whose clouds sit ~10× below the nearby-cloud locus in .
Core equations¶
Why has this form. The dense-gas SFR is the mass-weighted free-fall rate, , while the “naive” rate uses the mean density, . Hence
Closed form for a power-law sphere (Eq. 6, in Eq. 9). Performing the integrals over the sphere gives
PP20 print the constant as the rounded 2.6; the exact value is , fixed by the physical top-hat limit . The factor in the denominator means diverges only as — there is no pole at (a previously caught transcription fabrication). Spot values:
| 0 | 1 | 1.5 | 1.67 | |
|---|---|---|---|---|
| 1 (exact) | 1.089 | (exact) | 1.79 |
Forbidden regions (their Fig. 1). Equation (6) is the upper limit on (pure power law), and is the lower limit (top-hat); real cored profiles lie between. For a pure power law would drive the central density — and the SFR — to infinity, so PP20 add a flat inner core: a cored profile has a finite even for , obtained by numerically integrating the ratio above over . The core damps the boost: a relative core size already reduces significantly (their Fig. 1), because it shrinks the centre-to-edge density contrast.
Link to BM19. The PDF slope (Burkhart & Mocz) and the radial slope are the same quantity: . So .
Use in progenax¶
The magnification factor ζ — three ways to compute it — full derivation, equivalence proof, spot values, and the generalisation to cored and direct-3D profiles.
experimental/gravoturb/theory/dense_gas_sfr.py—magnification_factor(analytic),magnification_factor_with_core(trapezoid),zeta_from_field(field estimator).
Validation: anchors to (AC3); the direct field estimator matches the analytic to on a sampled power law (AC4).
Notes¶
is a Part-III / SFR-interpretation quantity: it is not needed to generate the gravoturbulent ICs, only to interpret the dense-gas SFR afterwards.
The 2026-04-28 transcription fix at PP20 ζ(p) transcription fix removed the spurious pole; the clean-room
pp20.pyre-derives the exact constant from first principles.
- Parmentier, G., & Pasquali, A. (2020). A new parameterization of the star formation rate–dense gas mass relation: Embracing gas density gradients. The Astrophysical Journal, 903, 56. 10.3847/1538-4357/abb8d3