Non-polynomial quasi-topological gravity models reproduce the standard thermal history, generate dynamical dark energy of geometric origin, and fit supernova, cosmic chronometer, and BAO data competitively with ΛCDM.
Surface Terms of Quintic Quasitopological Gravity and Thermodynamics of Quasi-Topological Magnetic Brane Coupled to Nonlinear Electrodynamics,
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Numerical solutions for quintic quasi-topological Lifshitz black holes in 5D with massive vector field are built via near-horizon expansion and shooting, yielding positive heat capacity for representative parameters across z=1,2 and k=-1,0,1.
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Cosmologically viable non-polynomial quasi-topological gravity: explicit models, $\Lambda$CDM limit and observational constraints
Non-polynomial quasi-topological gravity models reproduce the standard thermal history, generate dynamical dark energy of geometric origin, and fit supernova, cosmic chronometer, and BAO data competitively with ΛCDM.
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Quintic Modification to Lifshitz Quasi-topological Black Holes
Numerical solutions for quintic quasi-topological Lifshitz black holes in 5D with massive vector field are built via near-horizon expansion and shooting, yielding positive heat capacity for representative parameters across z=1,2 and k=-1,0,1.