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Related papers: Pattern Formation in the Early Universe

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Particle production caused by the oscillation after inflation is important since it explains reheating after inflation. On the particle theory side, we know that effective action may have additional higher dimensional terms (usually called…

High Energy Physics - Phenomenology · Physics 2015-05-13 Seishi Enomoto , Nobuhiro Maekawa , Tomohiro Matsuda

It is well known that, in potentials that are quadratic near the minimum but shallower away, such as small $\alpha$ ($\ll M_P^2$) attractors, the inflaton condensate fragments into localized compact objects known as oscillons during…

Cosmology and Nongalactic Astrophysics · Physics 2026-04-15 Bao-Min Gu , Yu-Peng Zhang , Fu-Wen Shu , Yu-Xiao Liu

One of the most interesting phenomena in the soft-matter realm consists in the spontaneous formation of super-molecular structures (microphases) in condition of thermodynamic equilibrium. A simple mechanism responsible for this…

Soft Condensed Matter · Physics 2017-08-23 A. Imperio , D. Pini , L. Reatto

We study pattern formation in planar fluid systems driven by intermolecular cohesion (which manifests as a line tension) and dipole-dipole repulsion which are observed in physical systems including ferrofluids in Hele-Shaw cells and…

Soft Condensed Matter · Physics 2015-04-01 Jaron Kent-Dobias , Andrew J. Bernoff

Cosmic inflation provides a compelling framework for explaining several observed features of our Universe, but its viability depends on an efficient reheating phase that converts the inflaton's energy into Standard Model particles. This…

Cosmology and Nongalactic Astrophysics · Physics 2025-07-14 Leia Barrowes , Fred C. Adams , Anthony M. Bloch , Scott Watson

The formation of structure in the Universe offers some of the most powerful evidence in favour of the existence of dark matter in the Universe. We summarize recent work by ourselves and our collaborators, using linear and quasi-linear…

Astrophysics · Physics 2007-05-23 Andrew R Liddle , Pedro T P Viana

Many models of supersymmetry breaking, in the context of either supergravity or superstring theories, predict the presence of particles with Planck-suppressed couplings and masses around the weak scale. These particles are generically…

High Energy Physics - Phenomenology · Physics 2010-02-03 G. F. Giudice , A. Riotto , I. Tkachev

Experimentally distinguishing different primordial universe paradigms that lead to the Big Bang model is an outstanding challenge in modern cosmology and astrophysics. We show that a generic type of signals that exist in primordial universe…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 Xingang Chen

Exciton-polaritons generated by light-induced potentials can spontaneously condense into macroscopic quantum states that display nontrivial spatial and temporal density modulation. While these patterns and their dynamics can be reproduced…

Mesoscale and Nanoscale Physics · Physics 2013-11-20 Li Ge , Ani Nersisyan , Baris Oztop , Hakan E. Tureci

We present fully non-linear simulations of a self-interacting scalar field in the early universe undergoing tachyonic preheating. We find that density perturbations on sub-horizon scales which are amplified by tachyonic instability maintain…

High Energy Physics - Phenomenology · Physics 2009-11-11 Teruaki Suyama , Takahiro Tanaka , Bruce Bassett , Hideaki Kudoh

At the end of inflation, the coherent oscillations of the inflaton field may resonantly amplify the long wavelength modes of both bosons and fermions coupled to it. We study the resonant production of both kinds of particles during…

High Energy Physics - Phenomenology · Physics 2009-10-31 Juan Garcia-Bellido , Silvia Mollerach , Esteban Roulet

Preheating describes the stage of rapidly depositing the energy of cosmological scalar field into excitations of other light fields. This stage is characterized by exponential particle production due to the parametric resonance. We study…

High Energy Physics - Theory · Physics 2015-03-19 Yi-Fu Cai , Robert Brandenberger , Xinmin Zhang

Gravitational waves are propagating undulations in the spacetime fabric, which interact very weakly with their environment. In cosmology, gravitational-wave distortions are produced by most of the inflationary scenarios and their…

General Relativity and Quantum Cosmology · Physics 2016-03-30 Despoina Pazouli , Christos G. Tsagas

The standard theory of cosmic structure formation posits that the present-day rich structure of the Universe developed through gravitational amplification of tiny matter density fluctuations generated in its very early history. Recent…

Cosmology and Nongalactic Astrophysics · Physics 2009-06-25 Naoki Yoshida

We generalize dark matter production to a two-metric framework whereby the physical metric, which couples to the Standard Model (SM), is conformally and/or disformally related to the metric governing the gravitational dynamics. We show that…

High Energy Physics - Phenomenology · Physics 2021-02-03 Philippe Brax , Kunio Kaneta , Yann Mambrini , Mathias Pierre

The evolution of the universe started from a hot and dense Big Bang point. Temperature fluctuation map of cosmic microwave background (CMB) radiation and initial seeds of large scale structures (LSS) are explained by an inflationary period…

General Relativity and Quantum Cosmology · Physics 2020-02-19 Vahid Kamali

A short introduction to structure formation is given, followed by a discussion of the possible characteristics of the initial perturbations assuming a generic inflationary origin. Observational data related to large-scale structure and the…

Astrophysics · Physics 2014-10-13 Pedro Viana

The processes in nonequilibrium dissipative media caused by coherent structure formation and lead to the complicated dynamics are of interest for nonlinear physics. Here we consider a model of the flow of interacting electronics patterns.…

chao-dyn · Physics 2008-02-03 E. S. Mchedlova , D. I. Trubetskov

The reheating of the universe after hybrid inflation proceeds through the nucleation and subsequent collision of large concentrations of energy density in the form of bubble-like structures moving at relativistic speeds. This generates a…

General Relativity and Quantum Cosmology · Physics 2008-01-29 Juan Garcia-Bellido , Daniel G. Figueroa

In order for an inflationary universe to evolve into a hot universe, a process known as reheating is required. However, the precise mechanism of reheating remains unknown. We show that if the reheating is triggered by thermal dissipation…

Cosmology and Nongalactic Astrophysics · Physics 2026-03-11 Kazuma Minami , Kyohei Mukaida , Kazunori Nakayama
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