Modules for Experiments in Stellar Astrophysics (MESA)

Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation

Bill Paxton, R. Smolec, Josiah Schwab, A. Gautschy, Lars Bildsten, Matteo Cantiello, Aaron Dotter, R. Farmer, Jared A. Goldberg, Adam S. Jermyn, S. M. Kanbur, Pablo Marchant, Anne Thoul, Richard H.D. Townsend, William M. Wolf, Michael Zhang, Francis Timmes

Research output: Contribution to journalArticle

1 Citation (Scopus)

Abstract

We update the capabilities of the open-knowledge software instrument Modules for Experiments in Stellar Astrophysics (MESA). RSP is a new functionality in MESAstar that models the nonlinear radial stellar pulsations that characterize RR Lyrae, Cepheids, and other classes of variable stars. We significantly enhance numerical energy conservation capabilities, including during mass changes. For example, this enables calculations through the He flash that conserve energy to better than 0.001%. To improve the modeling of rotating stars in MESA, we introduce a new approach to modifying the pressure and temperature equations of stellar structure, as well as a formulation of the projection effects of gravity darkening. A new scheme for tracking convective boundaries yields reliable values of the convective core mass and allows the natural emergence of adiabatic semiconvection regions during both core hydrogen- and helium-burning phases. We quantify the parallel performance of MESA on current-generation multicore architectures and demonstrate improvements in the computational efficiency of radiative levitation. We report updates to the equation of state and nuclear reaction physics modules. We briefly discuss the current treatment of fallback in core-collapse supernova models and the thermodynamic evolution of supernova explosions. We close by discussing the new MESA Testhub software infrastructure to enhance source code development.

Original languageEnglish (US)
Article number10
JournalAstrophysical Journal, Supplement Series
Volume243
Issue number1
DOIs
StatePublished - Jan 1 2019

Fingerprint

variable stars
astrophysics
energy conservation
modules
experiment
supernovae
software
computer programs
stellar structure
darkening
equation of state
helium
levitation
explosion
physics
nuclear reactions
thermodynamics
infrastructure
hydrogen
flash

Keywords

  • stars: evolution
  • stars: general
  • stars: interiors
  • stars: oscillations (including pulsations)
  • stars: rotation
  • stars: variables: general

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Modules for Experiments in Stellar Astrophysics (MESA) : Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation. / Paxton, Bill; Smolec, R.; Schwab, Josiah; Gautschy, A.; Bildsten, Lars; Cantiello, Matteo; Dotter, Aaron; Farmer, R.; Goldberg, Jared A.; Jermyn, Adam S.; Kanbur, S. M.; Marchant, Pablo; Thoul, Anne; Townsend, Richard H.D.; Wolf, William M.; Zhang, Michael; Timmes, Francis.

In: Astrophysical Journal, Supplement Series, Vol. 243, No. 1, 10, 01.01.2019.

Research output: Contribution to journalArticle

Paxton, B, Smolec, R, Schwab, J, Gautschy, A, Bildsten, L, Cantiello, M, Dotter, A, Farmer, R, Goldberg, JA, Jermyn, AS, Kanbur, SM, Marchant, P, Thoul, A, Townsend, RHD, Wolf, WM, Zhang, M & Timmes, F 2019, 'Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation', Astrophysical Journal, Supplement Series, vol. 243, no. 1, 10. https://doi.org/10.3847/1538-4365/ab2241
Paxton, Bill ; Smolec, R. ; Schwab, Josiah ; Gautschy, A. ; Bildsten, Lars ; Cantiello, Matteo ; Dotter, Aaron ; Farmer, R. ; Goldberg, Jared A. ; Jermyn, Adam S. ; Kanbur, S. M. ; Marchant, Pablo ; Thoul, Anne ; Townsend, Richard H.D. ; Wolf, William M. ; Zhang, Michael ; Timmes, Francis. / Modules for Experiments in Stellar Astrophysics (MESA) : Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation. In: Astrophysical Journal, Supplement Series. 2019 ; Vol. 243, No. 1.
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