We study magnetic field distribution of turbulent supernova
Remnant driven by the Richtmyer-Meshkov instability -- in other words, the
Effect of rippled shock -- by using three-dimensional magnetohydrodynamics
Simulations. We find that the induced turbulence has radially biased
We compute the scattering amplitude and the weak field potential energy
Between two separated point-like spinning, massive sources (such as two
Galaxies) in massive gravity. The spin-spin interaction potential energy in
This theory differs from that of the weak field limit of General Relativity
We discuss also how to make tunable
And broadband resonant mirrors by concatenating junctions. As an application,
We show how to construct cavities using these mirrors, thus connecting two
Research fields: JJ quantum metamaterials and coupled cavity arrays. We finish
By discussing the first non-line...
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