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相关论文: Inflation and The Minimal Supersymmetric Standard …

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It is shown that in the phenomenologically realistic supersymmetric $B-L$ MSSM theory, a linear combination of the neutral, up Higgs field with the third family left-and right-handed sneutrinos can play the role of the cosmological…

高能物理 - 唯象学 · 物理学 2017-02-15 Rehan Deen , Burt A. Ovrut , Austin Purves

We propose a cosmological inflationary scenario based on the supergravity-embedded Standard Model supplemented by the right-handed neutrinos. We show that with an appropriate Kahler potential the L-H_u direction gives rise to successful…

高能物理 - 唯象学 · 物理学 2013-05-30 Masato Arai , Shinsuke Kawai , Nobuchika Okada

We review the main aspects of the warm inflation scenario, focusing on the inflationary dynamics and the predictions related to the primordial spectrum of perturbations, to be compared with the recent cosmological observations. We study in…

高能物理 - 唯象学 · 物理学 2010-04-21 Mar Bastero-Gil , Arjun Berera

Scalar fields in the minimal supersymmetric standard model may have large field values during inflation. Because of approximate global symmetry, it is plausible that the phase directions of them are nearly massless during inflation and…

高能物理 - 唯象学 · 物理学 2020-12-30 Keisuke Harigaya , Masaki Yamada

The early stages of the universe evolution are discussed according to the hot big bang model and the grand unified theories. The shortcomings of big bang are summarized and their resolution by inflationary cosmology is sketched.…

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

We review an inflationary scenario with the anisotropic expansion rate. An anisotropic inflationary universe can be realized by a vector field coupled with an inflaton, which can be regarded as a counter example to the cosmic no-hair…

高能物理 - 理论 · 物理学 2015-06-04 Jiro Soda

The minimal supersymmetric (or F-term) hybrid inflation is defined by a unique renormalizable superpotential, fixed by a $U(1)$ R-symmetry, and it employs a canonical K\"{a}hler potential. The inflationary potential takes into account both…

高能物理 - 唯象学 · 物理学 2013-12-17 Constantinos Pallis , Qaisar Shafi

An epoch of accelerated expansion, or inflation, in the early universe solves several cosmological problems. While there are many models of inflation only recently has it become possible to discriminate between some of the models using…

高能物理 - 唯象学 · 物理学 2007-06-29 Raghavan Rangarajan

Observations of the temperature anisotropies in the Cosmic Microwave Background (CMB) radiation show that the models of inflation with the monomial potentials are inconsistent with the allowed $n_s-r$ bounds. However certain monomial…

宇宙学与河外天体物理 · 物理学 2022-03-17 Richa Arya , Raghavan Rangarajan

We study the scenario of inflection point inflation where a flat direction of the minimal supersymmetric standard model (MSSM) is identified with the inflaton. Specifically, we consider in full generality the cases where a MSSM flat…

高能物理 - 唯象学 · 物理学 2024-08-27 Naoyuki Haba , Yasuhiro Shimizu , Yoshihiro Tanabe , Toshifumi Yamada

We explore a broad class of three-parameter inflationary models, called the $\Lambda$-inflation, and its observational predictions: high abundance of cosmic gravitational waves consistent with the Harrison-Zel'dovich spectrum of primordial…

天体物理学 · 物理学 2016-12-28 V. N. Lukash , E. V. Mikheeva

The early Universe inflation is well known as a promising theory to explain the origin of large scale structure of the Universe, a causal theory for the origin of primordial density fluctuations which may explain the observed density…

天体物理学 · 物理学 2007-05-23 Xin-he Meng

Recent fits of cosmological parameters by the Wilkinson Microwave Anisotropy Probe (WMAP) measurement favor a primordial scalar spectrum with varying index. This result, if stands, could severely constrain inflation model buildings. Most…

天体物理学 · 物理学 2008-11-26 Bo Feng , Mingzhe Li , Ren-Jie Zhang , Xinmin Zhang

The big bang model and the history of the early universe according to the grand unified theories are introduced. The shortcomings of big bang are discussed together with their resolution by inflationary cosmology. Inflation, the subsequent…

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

We consider inflation in a universe with a positive cosmological constant and a nonminimally coupled scalar field, in which the field couples both quadratically and quartically to the Ricci scalar. When considered in the Einstein frame and…

广义相对论与量子宇宙学 · 物理学 2015-08-21 Dražen Glavan , Anja Marunović , Tomislav Prokopec

A {\it gauge invariant} combination of LLe {\it sleptons} within the Minimal Supersymmetric Standard Model is one of the few inflaton candidates that can naturally explain population of the observable sector and creation of matter after…

高能物理 - 唯象学 · 物理学 2015-03-19 Rouzbeh Allahverdi , Andrea Ferrantelli , Juan Garcia-Bellido , Anupam Mazumdar

Supersymmetry-based hybrid inflation models (referred to as `spontaneously broken supersymmetry' by the Planck collaboration) are attractive for several reasons, including the appealing feature that inflation is associated with local gauge…

宇宙学与河外天体物理 · 物理学 2025-04-22 Mansoor Ur Rehman , Qaisar Shafi

A minimal extension of the Standard Model (SM) with a single new mass scale and providing a complete and consistent picture of particle physics and cosmology up to the Planck scale is presented. We add to the SM three right-handed…

高能物理 - 唯象学 · 物理学 2017-02-22 Guillermo Ballesteros , Javier Redondo , Andreas Ringwald , Carlos Tamarit

This article presents a possible inflation scenario as a consequence of non-minimal gravitational couplings in the Conformal Standard Model. The model consists, in comparison to the SM, of additional right-chiral neutrinos and complex…

广义相对论与量子宇宙学 · 物理学 2018-02-27 Jan Kwapisz , Krzysztof A. Meissner

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…

高能物理 - 唯象学 · 物理学 2024-10-08 Arnab Paul , Sourov Roy , Abhijit Kumar Saha