Aug 19, 2011
The Planet-Saving Implications of Einstein’s “Happiest Thought”
Posted by Otto E. Rössler in categories: existential risks, particle physics
He always called it so. That in free fall after jumping out of the window (he was feeling sick at the moment) you do not feel the weight of a heavy stomach. The laws of nature then are the same as those valid in free outer space — those of special relativity.
The long overlooked consequence: gravity reduces rest mass energy and charge and increases size along with the clock period T focused on by Einstein. His T-change in gravity is accompanied by an L-, M- and Ch-change (Telemach theorem). Very simple but planet-saving. For it totally alters the properties of black holes. They arise more easily, do not Hawking evaporate, cannot be detected if produced at CERN, and grow exponentially inside earth.
The risk of the planet being shrunk to a 2-cm black hole in a few years’ time is currently being raised at CERN every day by 1/30 of the calculated final risk of 3 percent reached by the end of October. No scientist contradicts this accusation openly.
It is so easy: Interrupt and wait until the vitally needed counterproof has been found. No one will be happier than me and the mothers of the planet. Please, allow them to know about the situation.