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We study thermally induced density perturbations during inflation. This scenario is characterized by two thermodynamical conditions: (1) The primordial perturbations originate in the epoch when the inflationary universe contains a…

天体物理学 · 物理学 2009-10-30 Wolung Lee , Li-Zhi Fang

A recent article by Galtier and Nazarenko [1] proposed that weakly nonlinear gravitational waves could result in a turbulent cascade, with energy flowing from high to low frequency modes or vice versa. This is an interesting proposition for…

广义相对论与量子宇宙学 · 物理学 2018-08-29 Katy Clough , Jens C. Niemeyer

We present a simple model for the turbulent kinetic energy behavior of subsonic plasma turbulence undergoing isotropic three-dimensional compression, such as may exist in various inertial confinement fusion experiments or astrophysical…

等离子体物理 · 物理学 2018-02-21 Seth Davidovits , Nathaniel J. Fisch

Since the idea of quantum turbulence was first proposed by Feynman, and later realized in experiments of superfluid helium and Bose-Einstein condensates, much emphasis has been put in finding signatures that distinguish quantum turbulence…

量子气体 · 物理学 2025-04-24 Julian Amette Estrada , Marc E. Brachet , Pablo D. Mininni

We investigate an efficient mechanism for generating magnetic fields in turbulent, collisionless plasmas. By using fully kinetic, particle-in-cell simulations of an initially non-magnetized plasma, we inspect the genesis of magnetization,…

等离子体物理 · 物理学 2021-12-01 F. Pucci , M. Viviani , F. Valentini , G. Lapenta , W. H. Matthaeus , S. Servidio

Cosmology is nowadays going through a true revolution in the quantity and quality of observations that are capable of providing crucial information about the origin and evolution of the universe. In the first years of the next millenium we…

天体物理学 · 物理学 2015-06-24 Juan Garcia-Bellido

There is a clear distinction between simple laminar and complex turbulent fluids. But in some cases, as for the nocturnal planetary boundary layer, a stable and well-ordered flow can develop intense and sporadic bursts of turbulent activity…

流体动力学 · 物理学 2015-06-17 C. Rorai , P. D. Mininni , A. Pouquet

Atomic cooling haloes with virial temperatures $\rm T_{vir} \geq 10^{4}$ K are the most plausible sites for the formation of the first galaxies and the first intermediate mass black holes. It is therefore important to assess whether one can…

宇宙学与河外天体物理 · 物理学 2015-06-11 M. A. Latif , D. R. G. Schleicher , W. Schmidt , J. Niemeyer

We propose a cosmological scenario in which the hot big bang universe is produced by the collision of a brane in the bulk space with a bounding orbifold plane, beginning from an otherwise cold, vacuous, static universe. The model addresses…

高能物理 - 理论 · 物理学 2008-11-26 Justin Khoury , Burt A. Ovrut , Paul J. Steinhardt , Neil Turok

Self-gravitational structure formation theory for astrophysics and cosmology is revised using nonlinear fluid mechanics. Gibson's 1996-2000 theory balances fluid mechanical forces with gravitational forces and density diffusion with…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson

It is known that unconfined dust explosions typically starts off with a relatively weak primary flame followed by a severe secondary explosion. We show that clustering of dust particles in a temperature stratified turbulent flow ahead of…

流体动力学 · 物理学 2017-05-18 M. Liberman , N. Kleeorin , I. Rogachevskii , N. E. L. Haugen

Primordial chemistry began, at the recombination epoch, when the adiabatic expansion caused the temperature of the radiation to fall below 4000K. The chemistry of the early Universe involves the elements hydrogen, its isotope deuterium,…

天体物理学 · 物理学 2009-10-31 Denis Puy

Magnetic reconnection is a fundamental process of magnetic field topology change. We analyze the connection of this process with turbulence which is ubiquitous in astrophysical environments. We show how Lazarian & Vishniac (1999) model of…

太阳与恒星天体物理 · 物理学 2014-08-15 A. Lazarian , G. Eyink , E. Vishniac , G. Kowal

Buoyancy-driven turbulent convection leads to a fully compressible flow with a strong top-down asymmetry of first- and second-order statistics when the adiabatic equilibrium profiles of temperature, density and pressure decay very strongly…

流体动力学 · 物理学 2024-07-30 John Panickacheril John , Jörg Schumacher

This review article aims at presenting the theory of inflation. We first describe the background spacetime behavior during the slow-roll phase and analyze how inflation ends and the Universe reheats. Then, we present the theory of…

高能物理 - 理论 · 物理学 2009-11-10 Jerome Martin

Several scenarios have been proposed in which primordial perturbations could originate from quantum vacuum fluctuations in a phase corresponding to a collapse phase (in an Einstein frame) preceding the Big Bang. I briefly review three…

天体物理学 · 物理学 2008-09-29 David Wands

The standard model of gravitational structure formation is based on the Jeans 1902 acoustic theory, neglecting crucial effects of viscosity, turbulence and diffusion. A Jeans length scale L_J emerges that exceeds the scale of causal…

宇宙学与河外天体物理 · 物理学 2011-05-19 Rudolph E. Schild , Carl H. Gibson

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…

高能物理 - 唯象学 · 物理学 2008-11-26 Juan Garcia-Bellido , Daniel G. Figueroa , Alfonso Sastre

The most efficient energy sources known in the Universe are accretion disks. Those around black holes convert 5 -- 40 per cent of rest-mass energy to radiation. Like water circling a drain, inflowing mass must lose angular momentum,…

天体物理学 · 物理学 2009-11-11 Hantao Ji , Michael J. Burin , Ethan Schartman , Jeremy Goodman

The inflationary scenario, which states that the early universe underwent a brief but dramatic period of accelerated spatial expansion, has become the current paradigm of early universe cosmology. Although inflationary cosmology has its…

广义相对论与量子宇宙学 · 物理学 2024-06-04 Eric Ling , Annachiara Piubello