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Hybrid inflation within supersymmetric grand unified theories, as well as inflation through brane collisions within braneworld cosmological models, lead to the formation of one-dimensional defects. Observational data, mainly from the cosmic…

高能物理 - 理论 · 物理学 2015-06-26 Mairi Sakellariadou

In models of inflation driven by an axion-like pseudoscalar field, the inflaton, a, may couple to the standard model hypercharge via a Chern-Simons-type interaction, $L \subset a/(4\Lambda) F\tilde{F}$. This coupling results in explosive…

高能物理 - 唯象学 · 物理学 2017-12-20 Daniel Jimenez , Kohei Kamada , Kai Schmitz , Xun-Jie Xu

We reconsider the old problem of the dynamics of spontaneous symmetry breaking using 3d lattice simulations, and develop a theory of tachyonic preheating, which occurs due to the spinodal instability of the scalar field. Tachyonic…

高能物理 - 唯象学 · 物理学 2016-09-06 Gary Felder , Juan Garcia-Bellido , Patrick B. Greene , Lev Kofman , Andrei Linde , Igor Tkachev

We study the possibility that particle production during inflation could source observable gravity waves on scales relevant for Cosmic Microwave Background experiments. A crucial constraint on such scenarios arises because particle…

宇宙学与河外天体物理 · 物理学 2015-06-05 Neil Barnaby , Jordan Moxon , Ryo Namba , Marco Peloso , Gary Shiu , Peng Zhou

It is sometimes argued that observation of tensor modes from inflation would provide the first evidence for quantum gravity. However, in the usual inflationary formalism, also the scalar modes involve quantised metric perturbations. We…

宇宙学与河外天体物理 · 物理学 2015-05-05 Tommi Markkanen , Syksy Rasanen , Pyry Wahlman

It is conjectured that inflation, taking account of quantum gravity, leads to a discrete spectrum of cosmological perturbations, instead of the continuous Gaussian spectrum predicted by standard field theory in an unquantized background.…

天体物理学 · 物理学 2009-11-10 Craig J. Hogan

We consider models of inflation with U(1) gauge fields and charged scalar fields including symmetry breaking potential, chaotic inflation and hybrid inflation. We show that there exist attractor solutions where the anisotropies produced…

宇宙学与河外天体物理 · 物理学 2011-02-18 Razieh Emami , Hassan Firouzjahi , S. M. Sadegh Movahed , Moslem Zarei

It was recently found that the decay of inflaton and the SUSY breaking field produces many gravitinos in the gravity mediation scenario. These discoveries led to an exclusion of many inflation models such as chaotic, (smooth) hybrid,…

高能物理 - 唯象学 · 物理学 2008-11-26 H. Nakajima , Y. Shinbara

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 discuss the gravitational waves (GW) in the context of vector inflation. We derive the action for tensor perturbations and find that tachyonic instabilities are present in most (but not all) of the inflationary models with large fields.…

天体物理学 · 物理学 2009-03-20 Alexey Golovnev , Viatcheslav Mukhanov , Vitaly Vanchurin

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

Most models of inflation have small parameters, either to guarantee sufficient inflation or the correct magnitude of the density perturbations. In this paper we show that, in supersymmetric theories with weak scale supersymmetry breaking,…

高能物理 - 唯象学 · 物理学 2007-05-23 Lisa Randall , Marin Soljacic , Alan Guth

Preheating after inflation involves large, time-dependent field inhomogeneities, which act as a classical source of gravitational radiation. The resulting spectrum might be probed by direct detection experiments if inflation occurs at a low…

天体物理学 · 物理学 2008-11-26 Jean Francois Dufaux , Amanda Bergman , Gary N. Felder , Lev Kofman , Jean-Philippe Uzan

The gravitational waves (GW) background generated in a double inflationary model, with two scalar fields mutually interacting through gravity only, and its relative contribution $T/S$ to large-angle temperature fluctuations of the relic…

天体物理学 · 物理学 2009-10-28 David Polarski , Alexei A. Starobinsky

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 present a scenario where an axion-like field drives inflation until a potential barrier, which keeps a waterfall field at the origin, disappears and a waterfall transition occurs. Such a barrier separates the scale of inflation from that…

高能物理 - 唯象学 · 物理学 2021-08-18 Jinn-Ouk Gong , Kwang Sik Jeong

We construct a hybrid inflationary model associated with the superheavy scale of the minimal supersymmetric standard model which is based on the simplest superpotential for symmetry breaking and in which the inflaton potential along the…

高能物理 - 唯象学 · 物理学 2009-06-19 C. Panagiotakopoulos

We study the formation of primordial black holes and the generation of gravitational waves in a class of cosmological models that are direct supersymmetric analogs of the observationally favored nonminimally coupled Higgs inflation model.…

宇宙学与河外天体物理 · 物理学 2023-03-01 Shinsuke Kawai , Jinsu Kim

We consider gravitational wave production due to parametric resonance at the end of inflation, or ``preheating''. This leads to large inhomogeneities which source a stochastic background of gravitational waves at scales inside the comoving…

天体物理学 · 物理学 2008-11-26 Richard Easther , John T. Giblin , Eugene A. Lim

Non-abelian discrete gauge symmetries can provide the inflaton with a flat potential even when one takes into account gravitational strength effects. The discreteness of the symmetries also provide special field values where inflation can…

高能物理 - 唯象学 · 物理学 2009-10-31 E. D. Stewart , J. D. Cohn