Figure 1. Plot in function of r (arbitrary units) of the characteristic gravitational billow wave shape solution (numerical) hxx with respect to a discontinuity source located about r=0 (e.g. Kxx (t=0) =) at fixed times t1<t2<t3 with its attenuating moving peak at r = ct


Outstanding Outcomes from a Recent Theory of Gravity

Sandro Antonelli

International Journal of Physics. 2014, 2(6), 267-276 doi:10.12691/ijp-2-6-10