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Related papers: Gauged Nambu-Jona-Lasinio inflation

200 papers

The Higgs-Yukawa model in curved spacetime (renormalizable in the usual sense) is considered near the critical point, employing the $1/N$--expansion and renormalization group techniques. By making use of the equivalence of this model with…

High Energy Physics - Theory · Physics 2016-09-06 E. Elizalde , S. D. Odintsov

The minimal $U(1)_{L_\mu-L_\tau}$ gauge symmetry extended Standard Model (SM) is a well motivated framework that resolves the discrepancy between the theoretical prediction and experimental observation of muon anomalous magnetic moment. We…

High Energy Physics - Phenomenology · Physics 2024-10-08 Arnab Paul , Sourov Roy , Abhijit Kumar Saha

We review the construction of a concrete supersymmetric grand unified model, which naturally leads to a moderate violation of "asymptotic" Yukawa unification and, thus, can allow an acceptable b-quark mass within the constrained minimal…

High Energy Physics - Phenomenology · Physics 2017-08-23 G. Lazarides , C. Pallis

The Nambu-Jona-Lasinio model is the special case of the renormalized Yukawa model with the compositeness condition. We use it to calculate the effective coupling constants in terms of the compositeness sale (momentum cut off) at the…

High Energy Physics - Phenomenology · Physics 2007-05-23 Keiichi Akama

We consider a model of D-term inflation in which the inflaton coincides with the standard Higgs doublet. Non-renormalizable terms are controlled by a discrete R-symmetry of the superpotential. We consider radiative corrections to the scalar…

High Energy Physics - Phenomenology · Physics 2010-05-25 K. Tamvakis

Higgs G-inflation is an inflation model that takes advantage of a Galileon-like derivative coupling. It is a non-renormalizable operator and is strongly coupled at high energy scales. Perturbative analysis does not have a predictive power…

High Energy Physics - Phenomenology · Physics 2015-05-20 Kohei Kamada

Non-perturbative renormalizability, or non-triviality, of the gauged Nambu-Jona-Lasinio (NJL) model in four dimensions is examined by using non-perturbative (exact) renormalization group in large $N_c$ limit. When running of the gauge…

High Energy Physics - Theory · Physics 2009-10-31 Ken-Ichi Kubota , Haruhiko Terao

$R^2$-Higgs inflation stands out as one of the best-fit models of Planck data. Using a covariant formalism for the inflationary dynamics and the production of helical gauge fields, we show that the observed baryon asymmetry of the Universe…

Cosmology and Nongalactic Astrophysics · Physics 2024-02-20 Yann Cado , Christoph Englert , Tanmoy Modak , Mariano Quirós

We propose a model for cosmic inflation which is based on an effective description of strongly interacting, nonsupersymmetric matter within the framework of dynamical Abelian projection and centerization. The underlying gauge symmetry is…

High Energy Physics - Phenomenology · Physics 2009-11-07 Ralf Hofmann , Mathias Th. Keil

In this paper we will analyze generic predictions of an inflection-point model of inflation with Hubble-induced corrections and study them in light of the Planck data. Typically inflection-point models of inflation can be embedded within…

High Energy Physics - Phenomenology · Physics 2013-07-29 Sayantan Choudhury , Anupam Mazumdar , Supratik Pal

We study a Higgs inflation model with a running kinetic term, taking account of the renormalization group evolution of relevant coupling constants. Specifically we study two types of the running kinetic Higgs inflation, where the inflaton…

High Energy Physics - Phenomenology · Physics 2016-07-21 Fuminobu Takahashi , Ryo Takahashi

We propose a model for cosmic inflation which is based on an effective description of strongly interacting, nonsupersymmetric matter within the framework of dynamical abelian projection and centerization. The underlying gauge symmetry is…

High Energy Physics - Phenomenology · Physics 2007-05-23 Ralf Hofmann , Mathias Th. Keil

We investigate inflation driven by the Higgs boson in the Palatini formulation of General Relativity. Our analysis primarily focuses on a small non-minimal coupling of the Higgs field to gravity in the range $0<\xi\lesssim 1$. We…

High Energy Physics - Phenomenology · Physics 2023-06-07 Arthur Poisson , Inar Timiryasov , Sebastian Zell

The possibility to construct an inflationary scenario for renormalization-group improved potentials corresponding to the Higgs sector of quantum field models is investigated. Taking into account quantum corrections to the…

General Relativity and Quantum Cosmology · Physics 2017-03-22 E. O. Pozdeeva , S. Yu. Vernov

We derive one- and two-loop renormalization group equations (RGEs) of Higgs-$R^2$ inflation. This model has a non-minimal coupling between the Higgs and the Ricci scalar and a Ricci scalar squared term on top of the standard model. The RGEs…

High Energy Physics - Phenomenology · Physics 2021-03-17 Yohei Ema , Kyohei Mukaida , Jorinde van de Vis

The existence of the inflationary era in the early Universe seems to be strongly supported by recent CMB observations. However, only a few realistic inflation scenarios which have close relation to particle physics seem to have been known…

High Energy Physics - Phenomenology · Physics 2015-01-05 Romy H. S. Budhi , Shoichi Kashiwase , Daijiro Suematsu

A new modified string-inspired modular invariant supergravity model is proposed and is applied to realize the slow roll inflation in Einstein frame, so that the model explains WMAP observations very well. Gravitino mass and their production…

High Energy Physics - Phenomenology · Physics 2010-11-23 Yuta Koshimizu , Toyokazu Fukuoka , Kenji Takagi , Hikoya Kasari , Mitsuo J. Hayashi

We study how direct detection of the inflationary gravitational wave background constrains inflationary parameters and complements CMB polarization measurements. The error ellipsoids calculated using the Fisher information matrix approach…

Cosmology and Nongalactic Astrophysics · Physics 2010-08-03 Sachiko Kuroyanagi , Christopher Gordon , Joseph Silk , Naoshi Sugiyama

Natural inflation is a well-motivated model for the early universe in which an inflaton potential of the pseudo-Nambu-Goldstone form, $V(\phi) = \Lambda^4[1 + \cos{(\phi/f)}]$, can naturally drive a cosmic accelerated epoch. This paper…

Cosmology and Nongalactic Astrophysics · Physics 2024-04-23 F. B. M. dos Santos , G. Rodrigues , J. G. Rodrigues , R. de Souza , J. S. Alcaniz

A variant of hybrid inflation which is applicable in a wide class of supersymmetric grand unified models and reproduces the observed temperature perturbations of cosmic background radiation with natural values of the parameters is…

High Energy Physics - Phenomenology · Physics 2009-10-30 G. Lazarides