Abstract
In this work, we first propose a cosmological scenario inherently based on the effective Nambu–Jona-Lasio (NJL) model near the infrared (IR) limit of the Hořava-Lifshitz (HL) theory. Having used the one-loop correction, we employ the NJL framework in the ultraviolet (UV) limit of the HL theory, with critical exponent z=3, to demonstrate in the IR limit that the symmetry of the potential at the critical coupling value is broken at z=1. We also derive the effective Higgs-like potential in the low energy regimes. Here the symmetry of the effective potential will be broken near z=1 at a certain value of the critical coupling. In our scenario, the scalar channel of the NJL model plays the role of a composite inflaton. We find that the Lorentz invariance (LI) appears at the IR regime of the HL theory and employ the standard inflationary (slow-roll) paradigm as a probe of physics at very high energy. We compute inflationary parameters and compare them with recent Planck 2015 data. Interestingly, we discover that the predictions of the model are in perfect agreement with the Planck analysis. Our salient feature is that we used inflation to quantify the IR and UV fixed points of underlying theory. We discover that the IR fixed point of HL gravity is compatible with the grand unified energy scale; whilst the UV fixed point is the Planck energy scale.
Highlights
Quantum theory of gravity is one of the unsolved problems in theoretical physics and there is enormous uncertainty about its nature
The symmetry of the effective potential will be broken near z = 1 at a certain value of the critical coupling
We propose a cosmological scenario inherently based on the effective NJL model near the IR limit of the HL theory
Summary
Quantum theory of gravity is one of the unsolved problems in theoretical physics and there is enormous uncertainty about its nature. The simplest models of inflation make use of elementary scalar fields It was pointed out in Ref.[9] that the inflationary mechanism in the early Universe can be connected to the standard model (SM). The constituent fermion mass of the condensation can be generated for arbitrary coupling constant of the theory This phenomenon has the same profile as that of the NJL model in holographic Sakai-Sugimoto (AdS/QCD) scenario [22]. In the latter, we will show how the symmetry breaking of the model at some certain value of the coupling constant in the IR limit of the Lifshitz-like theory can happen like a standard relativistic NJL model. We first demonstrate the interval of UV and IR regimes of the HL theory via the inflationary constraints
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