2,629 research outputs found
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
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
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