The Spinor-Tensor Gravity of the Classical Dirac Field
Piero Chiarelli

TL;DR
This paper derives a gravity theory from the Dirac field using quantum hydrodynamics, revealing a spontaneous emergence of a cosmological gravity tensor that influences classical and quantum gravitational behavior.
Contribution
It introduces a novel spinor-tensor gravity framework derived from the Dirac field, connecting quantum hydrodynamics with classical and cosmological gravity.
Findings
Emergence of a cosmological gravity tensor (CGT) from the Dirac field.
CGT contributes to the energy-impulse tensor density, leading to a cosmological constant in the classical limit.
Perturbative corrections to Newtonian gravity from the CGT align with observed cosmological constants.
Abstract
In this work, with the help of the quantum hydrodynamic formalism, the gravitational equation associated to the Dirac field is derived. The hydrodynamic representation of the Dirac equation have been generalizaed to the curved space-time in the covariant form. Thence, the metric of the spacetime has been defined by imposing the minimum action principle. The derived gravity shows the spontaneous emergence of the cosmological gravity tensor (CGT) as a part of the energy-impulse tensor density (EITD) that in the classical limit leads to the cosmological constant (CC). Even if the classical cosmological constant is set to zero, the CGT is non zero, allowing to have a stable quantum vacuum (out of the collapsed branched polymer phase). The theory shows that in the classical limit, the gravity equation leads to the general relativity equation. In the perturbative approach, the CGT leads to a…
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