Gravity Induced Chiral Condensate Formation and the Cosmological Constant

Abstract

It is well known that the covariant coupling of fermionic matter to gravity induces a four-fermion interaction. The presence of this term in a homogenous and isotropic space-time results in a BCS-like Hamiltonian and the formation of a chiral condensate with a mass gap. We calculate the gap ($\Delta$) via a mean-field approximation for minimally coupled fermionic fields in a FRW background and find that it depends on the scale factor. The calculation also yields a correction to the bare cosmological constant (${\Lambda }_0$), and a non-zero vev for $<{\psi }^{†}\psi >$ which then behaves as a scalar field. Hence we conjecture that the presence of fermionic matter in gravity provides a natural mechanism for relaxation of the ${\Lambda }_0$ and explains the existence of a scalar field from (almost) first principles.

19 pages, 1 figure

Cited by in corpus (2)

• Fermions in Loop Quantum Cosmology and the Role of Parity
• CMB: A Look Inside the Inflaton