arXiv subjects

Christopher Lindsay

Publications and source records attributed to Christopher Lindsay.

4 recordsLinked to original sources

arXiv2026

Self-Consistent Nonlinear Classical Cepheid Pulsations During Stellar Evolution with MESA

We extend the time-dependent convection treatment in \code{MESA} by introducing eddy-viscous damping. This software change brings \code{MESA-TDC} into closer alignment with the radial stellar pulsation framework of \code{MESA-RSP}. We demonstrate that the inclusion of the eddy viscosity in hydrodynamic stellar models remains stable on evolutionary timescales. We then present the first self-consistent integration of large-amplitude, nonlinear Classical Cepheid pulsations directly within a \code{MESA-star} evolutionary run, demonstrating that the time-dependent convection formalism implemented in \code{MESA-star} and the \code{MESA} radial stellar pulsation (RSP) module are physically identical. Starting from a 6~\Msun\ blue-loop stellar evolution model, we demonstrate evolving the entire stellar model through pulsations as well as pausing the evolution, excising the core, and remeshing the envelope to match the grid used by \code{MESA-RSP}. We compare the pulsation properties (e.g., period, light and radius curves, and growth rate) with a matched \code{MESA-RSP} run, and find reasonable agreement between the two modules. This unified approach eliminates the reliance on separate post-processing workflows and enables fully coupled evolution-pulsation simulations. This approach enables future studies of stellar pulsations with the inclusion of composition gradients, mass loss, or rotation. It also enables future studies of the $\epsilon$ mechanism as well as providing a physical source of viscosity for other science cases explored using \code{MESA}'s hydrodynamics solver. We have integrated these modifications into the \code{MESA-star} module, enabling open-source use by the community.

astro-ph.SR↗

arXiv2026

Towards Automated Lexicography: Generating and Evaluating Definitions for Learner's Dictionaries

We study dictionary definition generation (DDG), i.e., the generation of non-contextualized definitions for given headwords. Dictionary definitions are an essential resource for learning word senses, but manually creating them is costly, which motivates us to automate the process. Specifically, we address learner's dictionary definition generation (LDDG), where definitions should consist of simple words. First, we introduce a reliable evaluation approach for DDG, based on our new evaluation criteria and powered by an LLM-as-a-judge. To provide reference definitions for the evaluation, we also construct a Japanese dataset in collaboration with a professional lexicographer. Validation results demonstrate that our evaluation approach agrees reasonably well with human annotators. Second, we propose an LDDG approach via iterative simplification with an LLM. Experimental results indicate that definitions generated by our approach achieve high scores on our criteria while maintaining lexical simplicity.

cs.CL↗

arXiv2025

Acoustic modes in M67 cluster stars trace deepening convective envelopes

Acoustic oscillations in stars are sensitive to stellar interiors. Frequency differences between overtone modes -- large separations -- probe stellar density, while differences between low-degree modes -- small separations -- probe the sound speed gradient in the energy-generating core of main sequence Sun-like stars, and hence their ages. At later phases of stellar evolution, characterised by inert cores, small separations are believed to lose much of their power to probe deep interiors and simply become proportional to large separations. Here, we present clear evidence of a rapidly evolving convective zone as stars evolve from the subgiant phase into red giants. By measuring acoustic oscillations in 27 stars from the open cluster M67, we observe deviations of proportionality between small and large separations, which are caused by the influence of the bottom of the convective envelope. These deviations become apparent as the convective envelope penetrates deep into the star during subgiant and red giant evolution, eventually entering an ultra-deep regime that leads to the red giant branch luminosity bump. The tight sequence of cluster stars, free of large spreads in ages and fundamental properties, is essential for revealing the connection between the observed small separations and the chemical discontinuities occurring at the bottom of the convective envelope. We use this sequence to show that combining large and small separations can improve estimations of the masses and ages of field stars well after the main sequence.

astro-ph.SR↗

arXiv2022

A Standardized Framework for Collecting Graduate Student Input in Faculty Searches

We present a procedure designed to standardize input received during faculty searches with the goal of amplifying student voices. The framework was originally used to collect feedback from graduate students, but it can be adapted easily to collect feedback from undergraduate students, faculty, staff or other stakeholders. Implementing this framework requires agreement across participating parties and minimal organization prior to the start of faculty candidate visits.

astro-ph.IM↗