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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 3.

M–R plot for WDs within the nonlinear ﹩f({ \mathcal R },{{ \mathcal L }}_{m},{ \mathcal T })﹩ gravity model. The solid black curve represents the GR prediction, whereas the colored curves correspond to the dimensionless coupling parameter values α ranging from −3χ to +5χ with χ = 106.

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