Search Results - "Scott, Laura J. A."

3D Simulations and MLT. I. Renzini's Critique by Arnett, W. David, Meakin, Casey, Hirschi, Raphael, Cristini, Andrea, Georgy, Cyril, Campbell, Simon, Scott, Laura J. A., Kaiser, Etienne A., Viallet, Maxime, Mocák, Miroslav

“…Renzini wrote an influential critique of "overshooting" in mixing-length theory (MLT), as used in stellar evolution codes, and concluded that three-dimensional…”
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Relative importance of convective uncertainties in massive stars by Kaiser, Etienne A, Hirschi, Raphael, Arnett, W David, Georgy, Cyril, Scott, Laura J A, Cristini, Andrea

“…ABSTRACT In this work, we investigate the impact of uncertainties due to convective boundary mixing (CBM), commonly called ‘overshoot’, namely the boundary…”
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aims – a new tool for stellar parameter determinations using asteroseismic constraints by Rendle, Ben M, Buldgen, Gaël, Miglio, Andrea, Reese, Daniel, Noels, Arlette, Davies, Guy R, Campante, Tiago L, Chaplin, William J, Lund, Mikkel N, Kuszlewicz, James S, Scott, Laura J A, Scuflaire, Richard, Ball, Warrick H, Smetana, Jiri, Nsamba, Benard

“…A key aspect in the determination of stellar properties is the comparison of observational constraints with predictions from stellar models. Asteroseismic…”
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Relative Importance of Convective Uncertainties by Kaiser, Etienne A, Hirschi, Raphael, Arnett, W. David, Cristini, Andrea, Georgy, Cyril, Scott, Laura J. A

“…Convection plays a key role in the evolution of stars due to energy transport and mixing of composition. Despite its importance, this process is still not well…”
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Relative Importance of Convective Uncertainties in Massive Stars by Kaiser, Etienne A, Hirschi, Raphael, Arnett, W. David, Georgy, Cyril, Scott, Laura J. A, Cristini, Andrea

“…In this work, we investigate the impact of uncertainties due to convective boundary mixing (CBM), commonly called `overshoot', namely the boundary location and…”
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3D Simulations and MLT: II. Onsager's Ideal Turbulence by Arnett, W. David, Hirschi, Raphael, Campbell, Simon W, Mocák, Miroslav, Georgy, Cyril, Meakin, Casey, Cristini, Andrea, Scott, Laura J. A, Kaiser, Etienne A, Viallet, Maxime

“…We simulate stellar convection at high Reynolds number (Re$\lesssim$7000) with causal time stepping but no explicit viscosity. We use the 3D Euler equations…”
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