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This book presents original research results on the leading edge of physics. Each article has been carefully selected in an attempt to present substantial research results across a broad spectrum, including navigation control of automated interstellar probes by means of quasars’ reference frames; impacts on airless objects under microgravity and possible related structures; nature of energy; phenomenon of axions’ and neutrinos’ clouds around objects; shock wave front of sun axions and neutrinos in molecular matter; ensembles of clusters in chloroprene caoutchouc and dynamics of clusters in chloroprene rubber; effects of an aligned magnetic field on an hydromagnetic flow around a corner; laminar gas flows in spiral galaxies; electromagnetic interaction between environmental fields and living systems and its effect on health and well-being; coherent structures in magnetohydrodynamic turbulent flows; a comprehensive picture of the galactic open star clusters’ age distribution; different mechanisms and applications of particle accelerators; pressure effect on novel iron based superconductors; and propagation of electromagnetic wave in underdense and overdense plasma.
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This book presents original research results on the leading edge of physics. Each article has been carefully selected in an attempt to present substantial research results across a broad spectrum, including navigation control of automated interstellar probes by means of quasars’ reference frames; impacts on airless objects under microgravity and possible related structures; nature of energy; phenomenon of axions’ and neutrinos’ clouds around objects; shock wave front of sun axions and neutrinos in molecular matter; ensembles of clusters in chloroprene caoutchouc and dynamics of clusters in chloroprene rubber; effects of an aligned magnetic field on an hydromagnetic flow around a corner; laminar gas flows in spiral galaxies; electromagnetic interaction between environmental fields and living systems and its effect on health and well-being; coherent structures in magnetohydrodynamic turbulent flows; a comprehensive picture of the galactic open star clusters’ age distribution; different mechanisms and applications of particle accelerators; pressure effect on novel iron based superconductors; and propagation of electromagnetic wave in underdense and overdense plasma.