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相关论文: Multiple Point Principle of the Gauged B-L Model

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We present a complete particle physics model that explains three major problems of modern cosmology: inflation, dark matter and dark energy, and also gives a mechanism for leptogenesis. The model has a new gauge group $SU(2)_Z$ that grows…

天体物理学 · 物理学 2008-11-26 P. Q. Hung , Eduard Masso , Gabriel Zsembinszki

We discuss the dynamics of multiple scalar fields and the possibility of realistic inflation in the maximal gauged supergravity. In this paper, we address this problem in the framework of recently discovered 1-parameter deformation of ${\rm…

高能物理 - 理论 · 物理学 2015-05-27 Hideo Kodama , Masato Nozawa

We consider a minimal supersymmetric extension of the Standard Model, with right-handed neutrinos and local B-L, the difference between baryon and lepton number, a symmetry which is spontaneously broken at the scale of grand unification. To…

高能物理 - 唯象学 · 物理学 2015-04-09 Wilfried Buchmüller , Valerie Domcke , Kohei Kamada , Kai Schmitz

Curiously in the minimal left right symmetric model, chiral symmetry that protects the electron's mass ($m_e$), due to parity (P), implies in the symmetry limit the vanishing of its neutrino mixing angles. We break the chiral symmetry…

高能物理 - 唯象学 · 物理学 2024-12-16 Ravi Kuchimanchi

We investigate various classes of Gauge Mediated Supersymmetry Breaking models and show that the Next-to-Minimal Supersymmetric Standard Model can solve the mu-problem in a phenomenologically acceptable way. These models include scenarios…

高能物理 - 唯象学 · 物理学 2008-11-26 U. Ellwanger , C. -C. Jean-Louis , A. M. Teixeira

We discuss model building in tribrid inflation, which is a framework for realising inflation in the matter sector of supersymmetric particle physics models. The inflaton is a D-flat combination of matter fields, and inflation ends by a…

高能物理 - 唯象学 · 物理学 2013-10-16 Stefan Antusch , David Nolde

In numerical calculations of the primordial power spectrum of perturbations produced during inflation, for very little wavenumber $k$s, to implement the initial conditions required of the perturbation mode functions consistently, we must…

天体物理学 · 物理学 2007-05-23 Ding-fang Zeng , Yi-hong Gao

We present a consolidated gauge-sector account of the octonionic programme, starting from the trace-dynamics Lagrangian and ending with closed-form expressions for the strong and electromagnetic couplings, together with a brief review of…

高能物理 - 唯象学 · 物理学 2026-04-07 Tejinder P. Singh

Inflation can occur near a point of inflection in the potential of flat directions of the Minimal Supersymmetric Standard Model. In this paper we elaborate on the complementarity between the bounds from Cosmic Microwave Background…

高能物理 - 唯象学 · 物理学 2014-11-20 Rouzbeh Allahverdi , Bhaskar Dutta , Yudi Santoso

A model of multi-component hybrid inflation, dubbed multi-brid inflation, in which various observable quantities including the non-Gaussianity parameter f_{NL} can be analytically calculated was proposed recently. In particular, for a…

天体物理学 · 物理学 2009-10-09 Atsushi Naruko , Misao Sasaki

Motivated by the idea that inflation occurs at the GUT symmetry breaking scale, in this paper we construct a new class of large field inflaton potentials where the inflaton starts with a power law potential; after initial period of relative…

宇宙学与河外天体物理 · 物理学 2014-09-24 Dhiraj Kumar Hazra , Arman Shafieloo , George F. Smoot , Alexei A. Starobinsky

Following \cite{Lin:2009yt}, we explore the parameter space of the case when the supersymmetry (SUSY) breaking scale is lower, for example, in gauge mediated SUSY breaking model. During inflation, the form of the potential is $V_0$ plus…

高能物理 - 唯象学 · 物理学 2014-11-18 Chia-Min Lin , Kingman Cheung

We propose a new leptogenesis scenario in a gauged $B-L$ model with supersymmetry at the TeV energy scale. Instead of relying on the very small Yukawa couplings of the singlet neutrinos $N^c$ to generate the observed baryon asymmetry of the…

高能物理 - 唯象学 · 物理学 2010-03-02 Yuji Kajiyama , Shaaban Khalil , Hiroshi Okada , Ernest Ma

We explore the possibility that a multiple-stage inflationary scenario based on supersymmetric GUT models, can account for the break at $k_b \simeq 0.05 h/Mpc$ in the power spectrum of galaxy clustering, while it reproduces the angular…

高能物理 - 唯象学 · 物理学 2009-10-31 Mairi Sakellariadou

We calculate the $U(1)$ continuum gauge coupling using the values of action parameters at the multiple point in the phase diagram of a lattice gauge theory. The multiple point is where a maximum number of phases convene. We obtain for the…

高能物理 - 唯象学 · 物理学 2009-10-28 D. L. Bennett , H. B. Nielsen

In this paper we propose two simple minimal Higgs inflation scenarios through a simple modification of the Higgs potential, as opposed to the usual non-minimal Higgs-gravity coupling prescription. The modification is done in such a way that…

高能物理 - 唯象学 · 物理学 2017-04-26 Debaprasad Maity

We revisit arguments that simple models of inflation with a small red tilt in the scalar power spectrum generically yield an observable tensor spectrum. We show that criteria for fine-tuning based upon the algebraic simplicity of the…

天体物理学 · 物理学 2008-12-18 Simeon Bird , Hiranya V. Peiris , Richard Easther

If the Standard Model is valid up to very high energies it is known that the Higgs potential can develop a local minimum at field values around $10^{15}-10^{17}$ GeV, for a narrow band of values of the top quark and Higgs masses. We show…

高能物理 - 唯象学 · 物理学 2013-05-30 Isabella Masina , Alessio Notari

We systematically study the renormalizable three-term polynomial inflation in the supersymmetric and non-supersymmetric models. The supersymmetric inflaton potentials can be realized in supergravity theory, and only have two independent…

高能物理 - 唯象学 · 物理学 2015-10-26 Tianjun Li , Zheng Sun , Chi Tian , Lina Wu

Detailed analyses of the WMAP data indicate possible oscillatory features in the primordial curvature perturbation, which moreover appears to be suppressed beyond the present Hubble radius. Such deviations from the usual inflationary…

天体物理学 · 物理学 2014-11-18 Paul Hunt , Subir Sarkar
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