Non-homogeneous exoplanets in metric-affine gravity

Abstract

The improved description of the planets' interior is provided. We examine the modified gravity effects on the Earth-like planets composed of the iron core and silicate mantle. We confirm that the mass-radius relations, as well as density profiles, differ with respect to the commonly adopted Newtonian models.

corrected version accepted by the journal, 15 pages, 4 figures

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• Refining Bounds for Snyder and GUP Models through Seismic Wave Analysis