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相关论文: MSSM curvaton in the gauge-mediated SUSY breaking

200 篇论文

We consider inflaton couplings to MSSM flat directions and the thermalization of the inflaton decay products, taking into account gauge symmetry breaking due to flat direction condensates. We then search for a suitable curvaton candidate…

高能物理 - 唯象学 · 物理学 2009-11-11 Rouzbeh Allahverdi , Kari Enqvist , Asko Jokinen , Anupam Mazumdar

We study in detail the possibility that the flat directions of the Minimal Supersymmetric Standard Model (MSSM) could act as a curvaton and generate the observed adiabatic density perturbations. For that the flat direction energy density…

高能物理 - 唯象学 · 物理学 2009-11-10 Kari Enqvist , Asko Jokinen , Shinta Kasuya , Anupam Mazumdar

We consider the curvaton scenario in the context of supersymmetry (SUSY) with gravity-mediated SUSY breaking. In the case of a large initial curvaton amplitude during inflation and a negative order H^2 correction to the mass squared term…

高能物理 - 唯象学 · 物理学 2009-11-10 John McDonald

We discuss how the inflation induced supersymmetry breaking affects the flat directions of SUSY vacua. We show that under general assumptions all gauge nonsinglet fields, parameterizing flat directions (and in particular squarks and…

高能物理 - 唯象学 · 物理学 2016-09-01 Gia Dvali

Considering the mechanism of dissipative slow-roll that has been used in warm inflation scenario, we show that dissipation may alter usual cosmological scenarios associated with SUSY-flat directions. We mainly consider SUSY-flat directions…

高能物理 - 唯象学 · 物理学 2011-03-14 Tomohiro Matsuda

We analyse the curvaton scenario in the context of supersymmetry. Supersymmetric theories contain many scalars, and therefore many curvaton candidates. To obtain a scale invariant perturbation spectrum, the curvaton mass should be small…

天体物理学 · 物理学 2007-05-23 Marieke Postma

We consider the role of supersymmetric flat directions in reheating the Universe after inflation. One or more flat directions can develop large vevs during inflation, which can potentially affect reheating by slowing down scattering…

高能物理 - 唯象学 · 物理学 2009-09-15 Keith A. Olive , Marco Peloso

We provide string theory examples where a toy model of a SUSY GUT or the MSSM is embedded in a compactification along with a gauge sector which dynamically breaks supersymmetry. We argue that by changing microscopic details of the model…

高能物理 - 理论 · 物理学 2009-11-11 Duiliu-Emanuel Diaconescu , Bogdan Florea , Shamit Kachru , Peter Svrcek

We show that a contribution to the total curvature perturbation may be due to the presence of flat directions in supersymmetric models. It is generated at the first os- cillation of the flat direction condensate when the latter relaxes to…

高能物理 - 唯象学 · 物理学 2008-12-18 Antonio Riotto , Francesco Riva

Curvaton is an effectively massless field whose energy density during inflation is negligible but which later becomes dominant. This is a novel mechanism to generate the scale invariant perturbations. I discuss the possibility that the…

高能物理 - 唯象学 · 物理学 2009-11-10 Kari Enqvist

We review the cosmological implications of the flat directions of the Minimally Supersymmetric Standard Model (MSSM). We describe how field condensates are created along the flat directions because of inflationary fluctuations. The…

高能物理 - 唯象学 · 物理学 2011-07-19 Kari Enqvist , Anupam Mazumdar

We construct a gauge-mediation model with a D-term supersymmetry (SUSY) breaking. R-symmetry breaking necessary for generating the SUSY standard-model gaugino masses is given by gaugino condensation of a strongly coupled gauge theory in the…

高能物理 - 唯象学 · 物理学 2008-11-26 Y. Nakayama , Masato Taki , Taizan Watari , T. T. Yanagida

We study moduli-dominated SUSY breaking within the framework of string models. This type of SUSY breaking in general leads to non-universal soft masses, i.e. soft scalar masses and gaugino masses. Further gauginos are lighter than…

高能物理 - 唯象学 · 物理学 2011-07-19 Yoshiharu Kawamura , Shaaban Khalil , Tatsuo Kobayashi

We analyze the curvaton scenario in the context of supersymmety. Supersymmetric theories contain many scalars, and therefore many curvaton candidates. To obtain a scale invariant perturbation spectrum, the curvaton mass should be small…

高能物理 - 唯象学 · 物理学 2014-11-17 Marieke Postma

We consider instant preheating as the mechanism for generating the curvature perturbation at the end of chaotic inflation. Then we examine if inflation could be driven by a Minimal Supersymmetric Standard Model (MSSM) flat direction or a…

高能物理 - 唯象学 · 物理学 2010-10-27 Tomohiro Matsuda

Supersymmetric standard model with softly broken lepton symmetry provides a suitable framework to accommodate the solar and atmospheric neutrino anomalies. This model contains a natural explanation for large mixing and hierarchal masses…

高能物理 - 唯象学 · 物理学 2009-10-31 Anjan S. Joshipura , Sudhir K. Vempati

We study density perturbations, including their non-Gaussianity, in models in which the decay rate of the curvaton depends on another light scalar field, denoted the modulaton. Although this model shares some similarities with the standard…

宇宙学与河外天体物理 · 物理学 2015-06-12 David Langlois , Tomo Takahashi

Recent progress in realising dynamical supersymmetry breaking allows the construction of simple and calculable models of gauge mediation. We discuss the phenomenology of the particularly minimal case in which the mediation is direct, and…

高能物理 - 唯象学 · 物理学 2010-04-23 Steven Abel , Joerg Jaeckel , Valentin V. Khoze , Luis Matos

Thermal inflation is an attractive idea to dilute cosmic density of unwanted particles such as moduli fields which cause cosmological difficulties. However, it also dilutes preexisting baryon asymmetry and some viable baryogenesis is…

高能物理 - 唯象学 · 物理学 2016-04-06 Taku Hayakawa , Masahiro Kawasaki , Masaki Yamada

We propose that the inflaton is coupled to ordinary matter only gravitationally and that it decays into a completely hidden sector. In this scenario both baryonic and dark matter originate from the decay of a flat direction of the minimal…

高能物理 - 唯象学 · 物理学 2009-11-07 Kari Enqvist , Shinta Kasuya , Anupam Mazumdar
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