![]() ![]() ![]() Within the ergosphere, a particle's energy may become negative (via the relativistic rotation of its Killing vector). Since the ergosphere is outside the event horizon, particles can escape from it. It is unclear which, if any, of these models accurately describes the real universe.įor a classically rotating black hole, the rotation creates an ergosphere outside the event horizon, in which spacetime itself begins to rotate, in a phenomenon known as frame-dragging. ![]() In the zero-energy universe model ("flat" or "Euclidean"), the total amount of energy in the universe is exactly zero: its amount of positive energy in the form of matter is exactly cancelled out by its negative energy in the form of gravity. Ī universe in which positive energy dominates will eventually collapse in a " Big Crunch", while an "open" universe in which negative energy dominates will either expand indefinitely or eventually disintegrate in a " big rip". Conversely, as two massive objects move towards each other, the motion accelerates under gravity causing an increase in the (positive) kinetic energy of the system and, in order to conserve the total sum of energy, the increase of the same amount in the gravitational potential energy of the object is treated as negative. As two object move apart and the distance between them approaches infinity, the gravitational force between them approaches zero from the positive side of the real number line and the gravitational potential approaches zero from the negative side. Conservation of energy requires that this gravitational field energy is always negative, so that it is zero when the objects are infinitely far apart. In classical mechanics, two or more masses always have a gravitational potential. Gravitational energy, or gravitational potential energy, is the potential energy a massive object has because it is within a gravitational field. ![]()
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