Turbulence and turbulent mixing in natural fluids

Turbulence and turbulent mixing in natural fluids begins with big bang turbulence powered by spinning combustible combinations of Planck particles and Planck antiparticles. Particle prograde accretions on a spinning pair releases 42% of the particle rest mass energy to produce more fuel for turbulent combustion. Negative viscous stresses and negative turbulence stresses work against gravity, extracting mass-energy and space-time from the vacuum. Turbulence mixes cooling temperatures until strong-force viscous stresses freeze out turbulent mixing patterns as the first fossil turbulence. Cosmic microwave background temperature anisotropies show big bang turbulence fossils along with fossils of weak plasma turbulence triggered as plasma photon-viscous forces permit gravitational fragmentation on supercluster to galaxy mass scales. Turbulent morphologies and viscous-turbulent lengths appear as linear gas-proto-galaxy-clusters in the Hubble ultra-deep-field at z~7. Proto-galaxies fragment into Jeans-mass-clumps of primordial-gas-planets at decoupling: the dark matter of galaxies. Shortly after the plasma to gas transition, planet-mergers produce stars that explode on overfeeding to fertilize and distribute the first life.Comment: 23 pages 12 figures, Turbulent Mixing and Beyond 2009 International Center for Theoretical Physics conference, Trieste, Italy. Revision according to Referee comments. Accepted for Physica Scripta Topical Issue to be published in 201

Removing black-hole singularities with nonlinear electrodynamics

We propose a way to remove black hole singularities by using a particular nonlinear electrodynamics Lagrangian that has been recently used in various astrophysics and cosmological frameworks. In particular, we adapt the cosmological analysis discussed in a previous work to the black hole physics. Such analysis will be improved by applying the Oppenheimer-Volkoff equation to the black hole case. At the end, fixed the radius of the star, the final density depends only on the introduced quintessential density term $\rho_{\gamma}$ and on the mass.Comment: In this last updated version we correct two typos which were present in Eqs. (21) and (22) in the version of this letter which has been published in Mod. Phys. Lett. A 25, 2423-2429 (2010). In the present version, both of Eqs. (21) and (22) are dimensionally and analytically correc

ANTIBODY RESPONSES TO ANTIGENIC DETERMINANTS OF INFLUENZA VIRUS HEMAGGLUTININ : II. Original Antigenic Sin: A Bone Marrow-Derived Lymphocyte Memory Phenomenon Modulated by Thymus-Derived Lymphocytes

Mice immunized sequentially with two related influenza virus hemagglutinins (HA) produced a secondary antibody response with two different specificities. Some antibodies were specific for determinants common to both HA's. Paradoxically, some antibodies were directed to determinants existing only in the HA first encountered. Primed spleen cells treated with anti-θ serum and complement were transferred from animals immunized with the first HA to either normal, irradiated, or thymus-deprived recipients. These memory cells were boosted in the recipients with either the homologous or the heterologous cross-reacting HA. B-memory lymphocytes were shown to be directly triggered by both HA's and to be able to secrete, independently of T lymphocytes, antibodies to both kinds of determinants. However, T cells were shown to modulate this secondary response by either enhancing or suppressing antibody secretion by B-memory cells, depending on experimental conditions. These results are discussed in terms of antigen recognition by B cells and of kinetics of development of immunological memory