YREC: the Yale rotating stellar evolution code

@article{Demarque2007YRECTY,
  title={YREC: the Yale rotating stellar evolution code},
  author={Pierre. Demarque and David B. Guenther and L. H. Li and A. Mazumdar and Christian W. Straka},
  journal={Astrophysics and Space Science},
  year={2007},
  volume={316},
  pages={31-41}
}
Abstract The stellar evolution code YREC is outlined with emphasis on its applications to helio- and asteroseismology. The procedure for calculating calibrated solar and stellar models is described. Other features of the code such as a non-local treatment of convective core overshoot, and the implementation of a parametrized description of turbulence in stellar models, are considered in some detail. The code has been extensively used for other astrophysical applications, some of which are… 
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References

SHOWING 1-10 OF 49 REFERENCES
Rotation in solar-type stars. I. Evolutionary models for the spin-down of the sun
We have calculated models of rotating 1 M/sub sun/ stars through the pre-main-sequence and main-sequence stages. The calculations start on the Hayashi track with rapid, rigid-body rotation. As the…
Two-dimensional Stellar Evolution Code Including Arbitrary Magnetic Fields. I. Mathematical Techniques and Test Cases
A high-precision two-dimensional stellar evolution code has been developed for studying solar variability due to structural changes produced by varying internal magnetic fields of arbitrary…
Asteroseismic diagnostics of stellar convective cores
We present a detailed study of the small frequency separations as diagnostics of the mass of the convective core and evolutionary stage of solar-type stars. We demonstrate how the small separations…
Evolution of Stellar Collision Products in Globular Clusters -- I. Head-on Collisions
We explore the evolution of collisionally merged stars in the blue straggler region of the HR diagram. The starting models for our stellar evolution calculations are the results of the smoothed…
Stellar Structure and Evolution
This book introduces the theory of the internal structure of stars and their evolution in time. It presents the basic physics of stellar interiors, methods for solving the underlying equations, and…
On the Rotational Evolution of Solar- and Late-Type Stars, Its Magnetic Origins, and the Possibility of Stellar Gyrochronology*
We propose a simple interpretation of the rotation period data for solar- and late-type stars. The open cluster and Mount Wilson star observations suggest that rotating stars lie primarily on two…
Convective penetration in stellar interiors
The evidence for convective penetration exhibited by geophysical fluids, laboratory experiments and computer simulations is recalled. A simple model is deduced from these observations, which serves…
Further improvements of a new model for turbulent convection in stars
The effects of including a variable molecular weight and of using the newest opacities of Rogers and Iglesias (1991) as inputs to a recent model by Canuto and Mazzitelli (1991) for stellar turbulent…
A simple convection model for selfgravitating fluid dynamics. Time-dependent convective energy transfer in protostars and nonlinear stellar pulsations
We describe a relatively simple time-dependent con- vection model that can be coupled to the equations of radiation hydrodynamics. We show that it behaves in a physically plau- sible way in…
An Application of Henyey's Approach to the Integration of the Equations of Stellar Structure.
ABSTRACT A method is described for the numerical solution of the equations of stellar structure by a technique especially designed for the solution of boundary-value problems. The numerical solution…
...
...