Image Details

Choose export citation format:

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 2.

MR diagram for WDs in the ﹩f({ \mathcal R },{{ \mathcal L }}_{m})﹩ gravity model with a square-root exponential coupling. The dimensional parameter β has units of inverse pressure, [β] = cm2 dyne−1, and is fixed to the dimensionless value ﹩\tilde{\beta }=2﹩ throughout this work. The coupling parameter γ varies from −2.0ζ to 5.5ζ, with ζ = 10−1. The solid black curve represents the GR prediction, while the dashed curves correspond to different values of γ

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse