For over five decades, astrophysical observations have revealed a persistent mass discrepancy in the universe: the dynamics of galaxies, galaxy clusters, and the large-scale structure of the universe cannot be explained by visible baryonic matter alone. To reconcile the standard theory of gravity with these observations, the scientific community has pursued two primary pathways. The dominant paradigm, the Lambda Cold Matter (ΛCDM) model, postulates the existence of undetected, non-baryonic dark matter particles. Conversely, Modified Newtonian Dynamics (MOND) and its relativistic formulations propose that the laws of gravity themselves undergo a structural transition in the ultra-weak-field regime of low accelerations.
While the standard model enjoys immense success at cosmological scales, the laboratory detection of dark matter remains elusive. At the same time, modified gravity frameworks struggle to explain cosmological observations without introducing their own auxiliary fields. Rather than a straightforward empirical dispute, this controversy centers on fundamental questions of scientific methodology, theory evaluation, and the epistemic standards by which competing physical explanations are judged.
The ANDROMEDA project integrates the History and Philosophy of Science (HPS) directly with modern cosmology to address these foundational issues. Utilizing historical epistemology and philosophical analysis, the project evaluates the conceptual underpinnings of both research programs. The overall objectives are: (1) to construct a philosophically informed historical narrative of the parallel development of dark matter and modified gravity since the 1970s; (2) to critically assess the epistemic standards—such as predictive power, falsifiability, and theoretical reduction—used to adjudicate between them; and (3) to investigate their compatibility across different physical scales.
This interdisciplinary approach provides a rigorous framework for theory evaluation and clarifies the rational, multi-scale foundations of modern cosmological research.