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相关论文: INFLATION VERSUS THE COSMOLOGICAL MODULI PROBLEM

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We study the process whereby quantum cosmological perturbations become classical within inflationary cosmology. By setting up a master-equation formulation we show how quantum coherence for super-Hubble modes can be destroyed by their…

天体物理学 · 物理学 2009-04-08 C. P. Burgess , R. Holman , D. Hoover

We consider the well motivated model of the (standard) supersymmetric F-term hybrid inflation (FHI) which can be realized close to the grand unification scale. The predicted scalar spectral index $n_s$ cannot be smaller than 0.98 and can…

高能物理 - 唯象学 · 物理学 2015-05-13 C. Pallis

We investigate inflation and its scalar perturbation driven by a massive scalar field in the unimodular theory of gravity. We introduce a parameter $\xi$ with which the theory is invariant under general unimodular coordinate…

广义相对论与量子宇宙学 · 物理学 2015-03-04 Inyong Cho , Naveen K. Singh

We develop a cosmological model where primordial inflation is driven by a 'solid', defined as a system of three derivatively coupled scalar fields obeying certain symmetries and spontaneously breaking a certain subgroup of these. The…

高能物理 - 理论 · 物理学 2015-06-11 Solomon Endlich , Alberto Nicolis , Junpu Wang

Inflation has been the leading early universe scenario for two decades, and has become an accepted element of the successful `cosmic concordance' model. However, there are many puzzling features of the resulting theory. It requires both…

高能物理 - 理论 · 物理学 2009-11-10 Neil Turok , Paul J. Seinhardt

Problem of cosmological singularity of general relativity theory is discussed. The possible resolution of this problem in the framework of inflationary cosmology is proposed. Physical conditions leading to bouncing inflationary solutions in…

广义相对论与量子宇宙学 · 物理学 2007-05-23 A. V. Minkevich

A new supergravity D-term, not associated to gauged R-symmetry, was recently discovered and used to construct new supergravity models. In this paper we use a generalization of the new D-term that we used in previous works, to construct a…

高能物理 - 理论 · 物理学 2022-08-29 Hun Jang , Massimo Porrati

We consider the abundance of gravitinos created from the vacuum fluctuation, in a class of `new' inflation models for which global supersymmetry is a good approximation. Immediately after inflation, gravitinos are produced, with number…

高能物理 - 唯象学 · 物理学 2009-10-31 David H Lyth

Supersymmetric hybrid inflation is an exquisite framework to connect inflationary cosmology to particle physics at the scale of grand unification. Ending in a phase transition associated with spontaneous symmetry breaking, it can naturally…

高能物理 - 唯象学 · 物理学 2014-07-31 Wilfried Buchmuller , Valerie Domcke , Kohei Kamada , Kai Schmitz

The standard model of cosmology is based on the hot Big Bang theory and the inflationary paradigm. Recent precise observations of the temperature and polarization anisotropies in the cosmic microwave background and the matter distribution…

高能物理 - 唯象学 · 物理学 2016-10-05 Juan Garcia-Bellido

In this paper, we study the inflection point inflation generated by a polynomial superpotential and a canonical K\"ahler potential under the supergravity framework, where only one chiral superfield is needed. We find that the special form…

高能物理 - 唯象学 · 物理学 2025-10-09 Manuel Drees , Wenbin Zhao

We consider a cosmological model with bulk viscosity ($\eta$) and variable cosmological $(\Lambda\propto \rho^{-\alpha}, \alpha=\rm const.$) and gravitational ($G$) constants. The model exhibits many interesting cosmological features.…

高能物理 - 理论 · 物理学 2008-11-26 Arbab I. Arbab

We study the initial value problem of new inflation models in the scheme of supergravity. We find that an inflaton generally acquires a mass of the order of the Hubble parameter via gravitationally suppressed interactions with particles in…

高能物理 - 唯象学 · 物理学 2009-10-31 T. Asaka , M. Kawasaki , Masahide Yamaguchi

We investigate the cosmological inflation in a class of supergravity models that are generalizations of non-supersymmetric $R^2$ models. Although such models have been extensively studied recently, especially after the launch of the PLANCK…

高能物理 - 理论 · 物理学 2015-06-23 G. A. Diamandis , B. C. Georgalas , K. Kaskavelis , P. Kouroumalou , A. B. Lahanas , G. Pavlopoulos

The potential during inflation must be very flat in, at least, the direction of the inflaton. In renormalizable global supersymmetry, flat directions are ubiquitous, but they are not preserved in a generic supergravity theory. It is known…

高能物理 - 理论 · 物理学 2009-09-29 Mary K. Gaillard , David H. Lyth , Hitoshi Murayama

We investigate the inflationary realization in the context of unimodular $F(T)$ gravity, which is based on the $F(T)$ modification of teleparallel gravity, in which one imposes the unimodular condition through the use of Lagrange…

广义相对论与量子宇宙学 · 物理学 2017-06-29 Kazuharu Bamba , Sergei D. Odintsov , Emmanuel N. Saridakis

In hybrid inflation, the inflaton generically has a tadpole due to gravitational effects in supergravity, which significantly changes the inflaton dynamics in high-scale supersymmetry. We point out that the tadpole can be cancelled if there…

高能物理 - 唯象学 · 物理学 2015-06-12 Tetsutaro Higaki , Kwang Sik Jeong , Fuminobu Takahashi

We investigate a class of models of topological inflation in which a super-Hubble-sized global monopole seeds inflation. These models are attractive since inflation starts from rather generic initial conditions, but their not so attractive…

广义相对论与量子宇宙学 · 物理学 2016-05-04 Anja Marunović , Tomislav Prokopec

Measurements of the Higgs boson and top quark masses indicate that the Standard Model Higgs potential becomes unstable around $\Lambda_I \sim 10^{11}$ GeV. This instability is cosmologically relevant since quantum fluctuations during…

高能物理 - 唯象学 · 物理学 2015-06-19 Anson Hook , John Kearney , Bibhushan Shakya , Kathryn M. Zurek

In the framework of chaotic inflation we study the case of a massive scalar field using a semiclassical approach. We derive the energy density fluctuations in the infrared sector generated by matter field and gauge-invariant metric…

广义相对论与量子宇宙学 · 物理学 2010-11-11 F. Lara , F. Astorga , M. Bellini