In f(T,T_G) braneworlds, non-minimal torsional coupling localizes one chiral fermion zero mode, yields continuous massive spectra with resonances, and strengthens localization as measured by Shannon entropy.
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In quadratic curvature-matter coupled gravity, strange stars described by the MIT bag equation of state can attain a maximum mass of 3.11 solar masses, exceeding the general-relativistic limit and potentially accounting for the lighter companion in GW190814.
Kerr-Newman black holes in f(R) gravity retain the same hidden symmetries and universal gyromagnetic ratio g=2 as in general relativity.
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New mechanism for fermion localization in $f(T,T_G)$-brane
In f(T,T_G) braneworlds, non-minimal torsional coupling localizes one chiral fermion zero mode, yields continuous massive spectra with resonances, and strengthens localization as measured by Shannon entropy.
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Maximum mass limit of strange stars in quadratic curvature-matter coupled gravity
In quadratic curvature-matter coupled gravity, strange stars described by the MIT bag equation of state can attain a maximum mass of 3.11 solar masses, exceeding the general-relativistic limit and potentially accounting for the lighter companion in GW190814.
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Hidden Symmetries and Gyromagnetic Ratio of Kerr-Newman Black Holes in $f(R)$ Gravity
Kerr-Newman black holes in f(R) gravity retain the same hidden symmetries and universal gyromagnetic ratio g=2 as in general relativity.