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相关论文: D-term inflation and neutrino mass

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We propose that inflation and dark matter have a common origin, connected to the neutrino mass generation scheme. As a model we consider spontaneous breaking of global lepton number within the seesaw mechanism. We show that it provides an…

高能物理 - 唯象学 · 物理学 2014-10-01 Sofiane M. Boucenna , Stefano Morisi , Qaisar Shafi , Jose W. F. Valle

We analyse the consequences of a new gauge invariant Fayet-Iliopoulos (FI) term proposed recently to a class of inflation models driven by supersymmetry breaking with the inflaton being the superpartner of the goldstino. We first show that…

高能物理 - 理论 · 物理学 2018-06-19 Ignatios Antoniadis , Auttakit Chatrabhuti , Hiroshi Isono , Rob Knoops

We evaluate the constraints that the COBE observations put on baryogenesis in inflationary cosmologies.We consider the supersymmetric version of the proposal of Fukugita and Yanagida, that the baryon asymmetry of the universe is created by…

高能物理 - 唯象学 · 物理学 2009-09-15 B. A. Campbell , S. Davidson , K. A. Olive

We consider an extended version of superconformal subcritical hybrid inflation model by introducing three right-handed neutrinos that have the Majorana mass terms. In the model one of the right-handed sneutrinos plays a role of the inflaton…

高能物理 - 唯象学 · 物理学 2019-10-02 Yoshihiro Gunji , Koji Ishiwata

Using renormalization-group flow and cosmological constraints on inflation models, we exploit a unique connection between cosmological inflation and the dynamical mass of dark-matter particles in the luminogenesis model, a unification model…

高能物理 - 唯象学 · 物理学 2015-12-02 Pham Q. Hung , Kevin J. Ludwick

In this work, we interpret the 3-3-1-1 model when the B-L and 3-3-1 breaking scales behave simultaneously as the inflation scale. This setup not only realizes the previously-achieved consequences of inflation and leptogenesis, but also…

高能物理 - 唯象学 · 物理学 2017-04-04 D. T. Huong , P. V. Dong

The primordial inflation dilutes all matter except the quantum fluctuations which we see in the cosmic microwave background (CMB) radiation. Therefore the last phases of inflation must be embedded within a beyond the Standard Model (SM)…

高能物理 - 唯象学 · 物理学 2013-02-06 Celine Boehm , Jonathan Da Silva , Anupam Mazumdar , Ernestas Pukartas

Quintessential inflation provides a unified description of the early and late accelerated phases of the Universe, linking the inflationary epoch to the present-day dark energy-dominated era through a single scalar degree of freedom. In this…

宇宙学与河外天体物理 · 物理学 2026-02-25 Jamerson Rodrigues , Gabriel Rodrigues , Felipe B. M. dos Santos , Simony Santos da Costa , Jailson Alcaniz

No-scale supergravity provides a successful framework for Starobinsky-like inflation models. Two classes of models can be distinguished depending on the identification of the inflaton with the volume modulus, $T$ (C-models), or a…

高能物理 - 唯象学 · 物理学 2020-01-15 Kunio Kaneta , Yann Mambrini , Keith A. Olive , Sarunas Verner

We study a leptogenesis scenario in which the heavy Majorana neutrinos are produced non-thermally in inflaton decays in the supersymmetric economical SU(3)_C X SU(3)_L X U(1)_X model with inflationary scenario, and for this purpose neutrino…

高能物理 - 唯象学 · 物理学 2010-12-17 D. T. Huong , H. N. Long

We show that a short period of late D-term inflation can solve the cosmological moduli (radion) problem of (asymmetric) inflation at the TeV scale. Late inflation happens after the large compact dimensions are stabilized which is crucial…

高能物理 - 唯象学 · 物理学 2010-02-03 Edi Halyo

In a supersymmetric left-right symmetric model, inflation, baryogenesis (via leptogenesis) and neutrino oscillations can become closely linked. A familiar ansatz for the neutrino Dirac masses and mixing of the two heaviest families,…

高能物理 - 唯象学 · 物理学 2008-11-26 G. Lazarides , Q. Shafi , N. D. Vlachos

Comparisons of cosmological models to current data show that the presence of a non-trivial feature in the primordial power spectrum of fluctuations, around the scale k=0.05 h/Mpc, is an open and exciting possibility, testable in a near…

高能物理 - 唯象学 · 物理学 2009-10-31 Julien Lesgourgues

We propose a minimal extension of the standard model of particle physics to accommodate cosmic inflation, dark matter and light neutrino masses. While the inflationary phase is obtained from a modified chaotic inflation scenario, consistent…

高能物理 - 唯象学 · 物理学 2020-04-15 Debasish Borah , Dibyendu Nanda , Abhijit Kumar Saha

We study effects of the cosmic string in the D-term inflation model on the cosmic microwave background (CMB) anisotropy. In the D-term inflation model, gauged cosmic string is usually formed, which may significantly affect the CMB…

高能物理 - 唯象学 · 物理学 2009-11-10 Motoi Endo , Masahiro Kawasaki , Takeo Moroi

Dilaton stabilisation is usually considered to pose a serious obstacle to successful $D$-term inflation in superstring theories. We argue that the physics of gaugino condensation is likely to be modified during the inflationary phase in…

高能物理 - 唯象学 · 物理学 2009-10-31 S. F. King , A. Riotto

We consider a new physics model, where the Standard Model (SM) is extended by hyperchargeless $Y=0$ triplet fermions and Higgs triplet with hypercharge $Y=2$. The first two generation fermion triplets are even under the $Z_2$…

高能物理 - 唯象学 · 物理学 2023-04-21 Pritam Das , Najimuddin Khan

The scale at which supersymmetry is broken and the mechanism by which supersymmetry breaking is fed down to the observable sector has rich implications on the way Nature may have chosen to accomplish inflation. We discuss a simple model for…

高能物理 - 唯象学 · 物理学 2014-11-17 Antonio Riotto

We present a successful realization of sneutrino tribrid inflation model based on a gauged $U(1)_{B-L}$ extension of Minimal Supersymmetric Standard Model (MSSM). A single interaction term involving the $B-L$ Higgs field and the…

高能物理 - 唯象学 · 物理学 2021-11-18 Muhammad Atif Masoud , Mansoor Ur Rehman , Qaisar Shafi

We propose a minimal setup that realises dynamical inflection point inflation, and, using the same field content, generates neutrino masses, a baryon asymmetry of the universe, and dark matter. A dark $SU(2)_D$ gauge sector with a dark…

高能物理 - 唯象学 · 物理学 2024-02-15 Debasish Borah , Arnab Dasgupta , Daniel Stolarski