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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 9.

Adiabatic index, Γ, as a function of radial coordinate within nonlinear model of ﹩f({ \mathcal R },{{ \mathcal L }}_{m},{ \mathcal T })﹩ gravity. The solid black line denotes the GR, while the colored lines represent the different values of α. Here, the purple dashed line represents Γ = 4/3 below which a stellar object will be unstable.

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