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Implications of Matter–Curvature Coupled Gravity on Chandrasekhar Mass Limit of White Dwarfs

  • Authors: N. Priyobarta, S. K. Maurya, Ksh. Newton Singh, B. Mishra

N. Priyobarta et al 2026 The Astrophysical Journal 1007 .

  • Provider: AAS Journals

Caption: Figure 1.

M–R plot for WDs within the power-law ﹩f({ \mathcal R },{{ \mathcal L }}_{m})﹩ gravity model. The solid black curve represents the predictions of GR, while the colored curves correspond to different values of the dimensionless coupling parameter σ, ranging from −1.50η to +3.0η, with η = 107.

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