Black Hole suspected inside the Solar System

In this issue of 'Extreme Science', the newsletter of the Einstein-Hubble scientific association, we present the premises of an astounding discovery, made this morning by our fellow Antoine Einstein while he was reading the results collected during the night by the Perry-Mason interferometer at the LHC laboratory. Einstein was sitting at the CERN cafeteria, drinking black coffee with a cloud of milk from the Swiss Alps, in his favorite breakfeast bowl in Provence pottery on a nice and colourful Provence Tablecloth, one of the Provence Gifts our association got from our sponsor Mediterranean Interiors.

First a few words about what is officially known about Black Holes. Most Scientists believe a black hole is a region of space in which the gravitational field is so powerful that nothing can escape after having fallen past the event horizon. The name comes from the fact that even electromagnetic radiation (e.g. light) is unable to escape, rendering the interior invisible. However, black holes can be detected if they interact with matter outside the event horizon, for example by drawing in gas from an orbiting star. The gas spirals inward, heating up to very high temperatures and emitting large amounts of radiation in the process.[2][3][4]
While the idea of an object with gravity strong enough to prevent light from escaping was proposed in the 18th century, black holes as presently understood are described by Einstein's theory of general relativity, developed in 1916. This theory predicts that when a large enough amount of mass is present within a sufficiently small region of space, all paths through space are warped inwards towards the center of the volume, forcing all matter and radiation to fall inward.
While general relativity describes a black hole as a region of empty space with a pointlike singularity at the center and an event horizon at the outer edge, the description changes when the effects of quantum mechanics are taken into account. Research on this subject indicates that, rather than holding captured matter forever, black holes may slowly leak a form of thermal energy called Hawking radiation.[5][6][7] However, the final, correct description of black holes, requiring a theory of quantum gravity, is unknown, except, of course, by our small team of CERN students.

This said, we can add that White Holes in the Milky Way have also been observed last summer by our folk Raimondo Panzani when he was riding on his bicycle on the 'Promenade des Anglais' in Nice on the French Riviera. To make it simple a White Hole is the opposite side of a Black Hole, the singularity where all light absorbed by a Black Hole emerges, within a While Hole, in another Time-Space continuum. A White Hole presents a 'negative mass' compared to a Black Hole. Planck demonstrated, in a one of the sudies he published in June 2007, that an 'polar gradient inversion' of the Higgs Field can be observed at the centre of a Black Hole, translating inside the corresponding While Hole into a inverse polarity of the gravitationnal field.

This morning, Einstein, from the overnight measures of the LHC proton-antiproton collision interferometer, made some calculations that proved the possibility that a While Hole might exists in the center of our solar system, actually in the exact center of our Sun. Although it is a very small While Hole with a negative mass of 10 exp -18 Gev/C2, this While Hole is generating a continuous flux of anti-proton which gets instantaneously anihilated by the surrounding Hydrogen nuclei (i.e protons) and where detected by the Perry-Mason interferometer because of these anti-proton/proton anihilations.

On the next issue of Extreme Science, we will provide more details on the companion Back Hole of the SUN's White Back Hole. At the moment, it is time to go and have lunch with this Provence Tableware we just received last week.

See you later.

Ernest Hubble, for the Einstein-Hubble association.