Hydrodynamics and a nonlinear dynamical formation model on binary stars

Abstract

Based on the hydrodynamics and hydromagnetics of nebula, we discuss the formation of binary stars using the qualitative analysis theory of a nonlinear equation. The nonlinear interaction and rotation play very crucial roles. Moreover, the Lorenz model may be derived from the equations of the hydrodynamics, whose two wings in the Lorenz model form just the binary stars, while the linear equations form only a single star.

Three Predictions of Gravitational Waves, and Black Holes

“…In a word, the big progresses in astronomy and universe are all related to important philosophy of science. Based on general relativity, we discussed some progresses: binary stars and their form [21][22][23], negative matter and inflation [24][25][26][27][28][29][30][31], etc. We proposed three predictions of gravitational waves: their observations must be nonlinear waves; velocity of gravitational wave should be slightly higher than the velocity of light; gravitational waves in black holes may emit and be observed.…”