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2017

The Maxwell-Chern-Simons gravity and its cosmological implications

Haghani, Zahra, Harko, Tiberiu, Shahidi, Shahab

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We consider the cosmological implications of a gravitational theory containing two vector fields coupled minimally to gravity as well as a generalized Chern-Simons term that couples the two vector fields.

One of the vector fields is the usual Maxwell field, while the other is a constrained vector field with constant norm included in the action via a Lagrange multiplier.
The theory admits a de Sitter type solution, with healthy cosmological perturbations.
We will show that there is 6 degrees of freedom propagate on top of de Sitter space-time, two tensor polarizations and four degrees of freedom related to two massless vector fields interacting with each other via Chern-Simons interaction term.

The Maxwell-Chern-Simons gravity and its cosmological implications · Around

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