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書誌詳細
第一著者: SAXENA, TARUN KUMAR
フォーマット: Recurso digital
言語:英語
出版事項: Zenodo 2026
主題:
オンライン・アクセス:https://doi.org/10.5281/zenodo.19663555
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  • <p>Version 11.5 (April 2026)</p> <p>This version incorporates three referee-level clarifications:<br>- Explicit restriction to descriptive performance metrics (no likelihood-based model comparison)<br>- Expanded interpretation of the stellar mass-to-light ratio calibration<br>- Clarified domain limitation in the deep-acceleration regime with ranked theoretical interpretations</p> <p>MOSGM is evaluated on the SPARC dataset (171 galaxies) and compared to MOND under a consistent pipeline.</p> <p>Key results:<br>- Comparable rotation curve performance to MOND<br>- Reduced systematic velocity bias<br>- Clear falsifiable predictions</p> <p>This version supersedes v11.4.</p>