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相关论文: Stochastic Isocurvature Baryon Fluctuations, Baryo…

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We study big bang nucleosynthesis in the presence of large mass-scale, non-linear entropy fluctuations. Overdense regions, with masses above the local baryon-Jeans mass, are expected to collapse and form condensed objects. Surviving…

天体物理学 · 物理学 2009-10-22 K. Jedamzik , G. M. Fuller

We investigate the effects of baryon/anti-baryon inhomogeneity on primordial nucleosynthesis. Recent work claims that electroweak baryogenesis could give rise to distinct regions of net baryon and anti-baryon number, which could survive…

天体物理学 · 物理学 2007-05-23 Kevork Abazajian , George M. Fuller

We show that the presence of primordial stochastic (hypercharge) magnetic fields before the electroweak (EW) phase transition induces isocurvature fluctuations (baryon number inhomogeneities). Depending on the details of the magnetic field…

高能物理 - 唯象学 · 物理学 2009-12-15 M. Giovannini , M. E. Shaposhnikov

We discuss effects of fluctuation geometry on primordial nucleosynthesis. For the first time we consider condensed cylinder and cylindrical-shell fluctuation geometries in addition to condensed spheres and spherical shells. We find that a…

天体物理学 · 物理学 2016-08-30 M. Orito , T. Kajino , R N. Boyd , G J. Mathews

Big bang nucleosynthesis constraints on baryon isocurvature perturbations are determined. A simple model ignoring the effects of the scale of the perturbations is first reviewed. This model is then extended to test the claim that large…

天体物理学 · 物理学 2009-09-25 Craig J. Copi , Keith A. Olive , David N. Schramm

We present a detailed study of inhomogeneous Big Bang nucleosynthesis where, for the first time, nuclear reactions are coupled to all significant fluctuation dissipation processes. Theses processes include neutrino heat transport, baryon…

天体物理学 · 物理学 2009-10-22 K. Jedamzik , G. M. Fuller , G. J. Mathews

A number of possible mechanisms have been suggested to generate density inhomogeneities in the early Universe which could survive until the onset of primordial nucleosynthesis and generate neutron-rich regions. In this work we are not…

高能天体物理现象 · 物理学 2015-04-20 T. Rauscher , F. -K. Thielemann

We reexamine big bang nucleosynthesis with large-scale baryon density inhomogeneities when the length scale of the density fluctuations exceeds the neutron diffusion length ($\sim 10^7-10^8$ cm at BBN), and the amplitude of the fluctuations…

宇宙学与河外天体物理 · 物理学 2018-09-12 John D. Barrow , Robert J. Scherrer

Baryon density inhomogeneities in the early universe can give rise to a floor of heavy elements (up to $A\approx 270$) produced in a primordial r-process with fission cycling. A parameter study with variation of the global baryon to photon…

高能天体物理现象 · 物理学 2015-04-20 T. Rauscher , J. H. Applegate , J. J. Cowan , F. -K. Thielemann , M. Wiescher

Across a large range of scales, accreting sources show remarkably similar patterns of variability, most notably the log-normality of the luminosity distribution and the linear root-mean square (rms)-flux relationship. These results are…

高能天体物理现象 · 物理学 2024-01-30 Samuel G. D. Turner , Christopher S. Reynolds

A stochastic model for intermittent fluctuations in the scrape-off layer of magnetically confined plasmas has been constructed based on a super-position of uncorrelated pulses arriving according to a Poisson process. In the most common…

等离子体物理 · 物理学 2018-05-04 Audun Theodorsen , Odd Erik Garcia

I give an estimate for the skewness and the kurtosis of the baryon number distribution in two representative models; i.e., models of a hadron resonance gas and relativistic mean-field nuclear matter. I emphasize formal similarity between…

高能物理 - 唯象学 · 物理学 2015-09-01 Kenji Fukushima

Primordial nucleosynthesis calculations are shown to be able to provide constraints on electroweak baryogenesis which produce a highly inhomogeneous distribution of the baryon-to-photon ratio. Such baryogenesis scenarios overproduce 4He…

天体物理学 · 物理学 2009-10-22 G. M. Fuller , K. Jedamzik , G. J. Mathews , A. Olinto

We study the spectrum of primordial fluctuations in theories where the inflaton field is coupled to massless fields and/or to itself. Conformally invariant theories generically predict a scale invariant spectrum. Scales entering the theory…

广义相对论与量子宇宙学 · 物理学 2014-11-17 Esteban A. Calzetta , Sonia Gonorazky

The fraction of matter that is in the form of baryons or dark matter could have spatial fluctuations in the form of baryon-dark matter isocurvature fluctuations. We use big bang nucleosynthesis calculations compared with observed light…

宇宙学与河外天体物理 · 物理学 2015-05-13 Gilbert P. Holder , Kenneth M. Nollett , Alexander van Engelen

The description of dynamical fluctuations near the QCD critical point in heavy-ion collisions is crucial for understanding the existing and upcoming experimental data from the beam energy scan programs. In this talk we discuss the evolution…

核理论 · 物理学 2018-04-10 Marlene Nahrgang , Marcus Bluhm , Thomas Schaefer , Steffen A. Bass

Event-by-event fluctuations of the baryon number, which is mostly carried by protons and neutrons, in relativistic heavy-ion collisions provide a sensitive probe for locating the conjectured critical point in the quantum chromodynamics…

核理论 · 物理学 2025-12-24 Yi-Heng Feng , Che Ming Ko , Xiaofeng Luo , Yu-Gang Ma , Kai-Jia Sun , Song Zhang

Single-point measurements of fluctuations in the scrape-off layer of magnetized plasmas are generally found to be dominated by large-amplitude bursts which are associated with radial motion of blob-like structures. A stochastic model for…

等离子体物理 · 物理学 2013-05-30 O. E. Garcia

Baryon number cumulants are invaluable tools to diagnose the primordial stage of heavy ion collisions if they can be measured. In experiments, however, proton number cumulants have been measured as substitutes. In fact, proton number…

核理论 · 物理学 2015-05-28 Masakiyo Kitazawa , Masayuki Asakawa

We show that primordial nucleosynthesis in baryon inhomogeneous big-bang models can lead to significant heavy-element production while still satisfying all the light-element abundance constraints including the low lithium abundance observed…

天体物理学 · 物理学 2009-10-22 K. Jedamzik , G. M. Fuller , G. J. Mathews , T. Kajino
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