An effective LQG polymer metric applied to white dwarf TOV equations shows a free amplitude A_lambda can raise the maximum mass above the Chandrasekhar limit, while the mass asymmetry ratio eta has subpercent effects.
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White Dwarf Stellar Structure from Effective Polymer Geometry in Loop Quantum Gravity
An effective LQG polymer metric applied to white dwarf TOV equations shows a free amplitude A_lambda can raise the maximum mass above the Chandrasekhar limit, while the mass asymmetry ratio eta has subpercent effects.