Overshooting: Mixing Length Yields Divergent Results
Open Access
- 1 August 1997
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 484 (2) , L161-163
- https://doi.org/10.1086/310792
Abstract
Overshooting (OV) is the signature of the nonlocal nature of convection. To describe the latter, one needs five nonlocal, coupled differential equations to describe turbulent kinetic energies (total K and in the z-direction Kz), potential energy, convective flux, and rate of dissipation ε. We show analytically that if ε is assumed to be given by the local expression, ε = K3/2l-1 (mixing length l = αHp or l = z/a, since the region is small in extent), the remaining differential equations exhibit singularities (divergences) for specific values of a within the range of values usually employed. No solution can be found. Thus, OV results from such an approach are quite accidental, as they stem from an arbitrary fine tuning of a.Keywords
This publication has 12 references indexed in Scilit:
- The Age of NGC 3680 and a Test of Convective OvershootThe Astronomical Journal, 1997
- Turbulent Convection in a Spectral ModelPhysical Review Letters, 1997
- A dynamical model for turbulence. I. General formalismPhysics of Fluids, 1996
- The gravitational lens system B1422 + 231: dark matter, superluminal expansion and the Hubble constantMonthly Notices of the Royal Astronomical Society, 1994
- Helioseismic measurement of the extent of overshoot below the solar convection zoneMonthly Notices of the Royal Astronomical Society, 1994
- Turbulent convection with overshooting - Reynolds stress approachThe Astrophysical Journal, 1992
- Solar pulsational stability - I. Pulsation-mode thermodynamicsMonthly Notices of the Royal Astronomical Society, 1992
- New strong evidence for the importance of convective overshooting in intermediate-mass starsThe Astrophysical Journal, 1990
- Mixing-length theory for pulsating starsThe Astrophysical Journal, 1977
- Convective Overshoot Mixing in Old Open Clusters .The Astrophysical Journal, 1974