de Sitter group and Einstein-Hilbert Lagrangian
Prasanta Mahato

TL;DR
This paper explores the role of axial vector torsion in Einstein-Cartan space, linking Einstein-Hilbert parameters to topological densities through a modified Pontryagin term.
Contribution
It introduces a novel Lagrangian density derived from a modified SO(4,1) Pontryagin density, connecting Einstein-Hilbert constants with topological invariants.
Findings
$$ and $$ appear as integration constants
$$ linked with Nieh-Yan density
Modified Pontryagin density yields new insights into torsion and gravity
Abstract
Axial vector torsion in the Einstein-Cartan space is considered here. By picking a particular term from the SO(4,1) Pontryagin density and then modifying it in a SO(3,1) invariant way, we get a Lagrangian density with Lagrange multipliers. Then considering torsion and torsion-less connection as independent fields, it has been found that and of Einstein-Hilbert Lagrangian, appear as integration constants in such a way that has been found to be linked with the topological Nieh-Yan density of space.
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