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相关论文: The R-axion and non-Gaussianity

200 篇论文

We present a comprehensive study of primordial fluctuations generated from G-inflation, in which the inflaton Lagrangian is of the form $K(\phi, X)-G(\phi, X)\Box\phi$ with $X=-(\partial\phi)^2/2$. The Lagrangian still gives rise to…

高能物理 - 理论 · 物理学 2011-06-07 Tsutomu Kobayashi , Masahide Yamaguchi , Jun'ichi Yokoyama

We argue that in an inflationary cosmology a consequence of the lack of time translational invariance is that spontaneous breaking of a continuous symmetry and Goldstone's theorem \emph{do not} imply the existence of \emph{massless}…

宇宙学与河外天体物理 · 物理学 2012-07-12 Daniel Boyanovsky

In the Einstein frame picture of Starobinky's $R^2$ inflation model, cosmic inflation is driven by a slowly rolling inflaton field, called scalaron, and followed by a coherently oscillating scalaron phase. Since the scalaron oscillates…

宇宙学与河外天体物理 · 物理学 2014-07-16 Naoyuki Takeda , Yuki Watanabe

We construct a self-interacting dark matter model that could simultaneously explain the observed muon anomalous magnetic moment. It is based on a gauged U$(1)_{L_{\mu} - L_{\tau}}$ extension of the standard model, where we introduce a…

高能物理 - 唯象学 · 物理学 2018-07-31 Ayuki Kamada , Kunio Kaneta , Keisuke Yanagi , Hai-Bo Yu

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…

高能物理 - 唯象学 · 物理学 2009-11-07 Ralf Hofmann , Mathias Th. Keil

We study the production of massive gauge bosons during inflation from the axion-type coupling to the inflaton and the corresponding oscillatory features in the primordial non-Gaussianity. In a window in which both the gauge boson mass and…

高能物理 - 唯象学 · 物理学 2020-12-02 Lian-Tao Wang , Zhong-Zhi Xianyu

A spectator axion-gauge sector, minimally coupled to the inflaton, with the axion experiencing a momentary stage of fast roll during cosmological inflation, can generate unique signatures in primordial density fluctuations and the…

宇宙学与河外天体物理 · 物理学 2025-01-28 Angelo Caravano , Marco Peloso

We study the inflation due to the D-flat direction of an extra $U(1)$. This scenario is a hybrid of a right-handed sneutrino inflaton scenario and a gauge non-singlet inflaton scenario. The inflaton is a gauge non-singlet field which…

高能物理 - 唯象学 · 物理学 2009-10-28 Daijiro Suematsu , Yoshio Yamagishi

A new estimate of the mass of the pseudo dilaton is offered by following the funda- mental nature that a massless Nambu-Goldstone boson, called a dilaton, in the Einstein frame acquires a nonzero mass through the loop effects which occur…

广义相对论与量子宇宙学 · 物理学 2015-12-07 Yasunori Fujii

The Standard Model (SM) of particle physics is a big success. However, it lacks explanations for cosmic inflation, the matter-anti-matter asymmetry of the Universe, dark matter, neutrino oscillations, and the feebleness of CP violation in…

高能物理 - 唯象学 · 物理学 2019-09-04 Guillermo Ballesteros , Javier Redondo , Andreas Ringwald , Carlos Tamarit

We revisit inflationary cosmology of axion models in the light of recent developments on the inflaton decay in supergravity. We find that all the cosmological difficulties, including gravitino, axino overproduction and axionic isocurvature…

高能物理 - 唯象学 · 物理学 2008-11-26 Masahiro Kawasaki , Kazunori Nakayama

It was recently shown that gravitons with a very small mass should have formed a Bose-Einstein condensate in the very early Universe, whose density and quantum potential can account for the dark matter and dark energy in the Universe…

广义相对论与量子宇宙学 · 物理学 2015-10-13 Saurya Das

We investigate the recently proposed natural double inflation model in supergravity. Chaotic inflation first takes place by virtue of the Nambu-Goldstone-like shift symmetry. During chaotic inflation, an initial value of second inflation…

高能物理 - 唯象学 · 物理学 2009-11-07 Masahide Yamaguchi

In a two-flavor color superconductor, the SU(3)_c gauge symmetry is spontaneously broken by diquark condensation. The Nambu-Goldstone excitations of the diquark condensate mix with the gluons associated with the broken generators of the…

核理论 · 物理学 2009-11-07 Dirk H. Rischke , Igor A. Shovkovy

The majoron is a well-motivated light (pseudo-Nambu-Goldstone) boson associated with the spontaneous breaking of a global lepton-number symmetry. In this {\it letter}, we relate the spontaneous breaking scale and its soft-breaking mass by…

高能物理 - 唯象学 · 物理学 2024-06-28 Qiuyue Liang , Xavier Ponce Díaz , Tsutomu T. Yanagida

We consider the expected level of primordial non-Gaussianities in models in which density perturbations are produced by spatial fluctuations in the decay rate of the inflaton. We consider both the non-Gaussianities resulting from the…

天体物理学 · 物理学 2008-11-26 Matias Zaldarriaga

A moderate extension of the minimal supersymmetric standard model which includes a U(1)_(B-L) gauge group (B and L being the baryon and lepton number) and a Peccei-Quinn symmetry, U(1)_PQ, is presented. The hybrid inflationary scenario is…

高能物理 - 唯象学 · 物理学 2008-11-26 G. Lazarides

There are a number of observational hints from astrophysics which point to the existence of stellar energy losses beyond the ones accounted for by neutrino emission. These excessive energy losses may be explained by the existence of a new…

高能物理 - 唯象学 · 物理学 2017-10-18 Maurizio Giannotti , Igor G. Irastorza , Javier Redondo , Andreas Ringwald , Ken'ichi Saikawa

We discuss inflation models within supersymmetry and supergravity frameworks with a landscape of chiral superfields and one $U(1)$ shift symmetry which is broken by non-perturbative symmetry breaking terms in the superpotential. We label…

高能物理 - 唯象学 · 物理学 2018-04-18 Pran Nath , Maksim Piskunov

We show that a baryon asymmetry can be generated by dissipative effects during warm inflation via a supersymmetric two-stage mechanism, where the inflaton is coupled to heavy mediator fields that then decay into light species through B- and…

高能物理 - 唯象学 · 物理学 2015-05-30 Mar Bastero-Gil , Arjun Berera , Rudnei O. Ramos , Joao G. Rosa