Figure 17 from MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA): BINARIES, PULSATIONS, AND EXPLOSIONS

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MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA): BINARIES, PULSATIONS, AND EXPLOSIONS

Authors: Bill Paxton, Pablo Marchant, Josiah Schwab, Evan B. Bauer, Lars Bildsten, Matteo Cantiello, Luc Dessart, R. Farmer, H. Hu, N. Langer, R. H. D. Townsend, Dean M. Townsley, and F. X. Timmes

2015 The Astrophysical Journal Supplement Series 220 15.

Provider: AAS Journals

Caption: Figure 17.

Top: evolution of internal energy ﹩{E}_{\mathrm{int}}﹩, gravitational energy ﹩{E}_{\mathrm{grav}}﹩, kinetic energy ﹩{E}_{\mathrm{kin}}﹩, and their sum ﹩{E}_{\mathrm{tot}}﹩ for the envelope shock test simulated with MESA and V1D. Bottom: log of cumulative relative error CRE (Equation (58)) of the total energy ﹩{E}_{\mathrm{tot}}﹩. We neglect sources (nuclear burning) and sinks (radiation losses), which are negligible.

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