Einstein’s theory of general relativity is not a fundamental theory, but rather an effective theory that governs the behavior of gravity when it is not too strong. How is this theory corrected when we move away from that regime? Various candidates for the elusive theory of quantum gravity (for example, string theory) predict that corrections to Einstein’s equations appear as additional terms that depend on the curvature of space-time. These modifications will be important in situations where the gravitational field is extremely intense, such as in black holes. To date, the theoretical study of these corrections has been carried out mainly in an approximate way, and has focused mainly on the case of static black holes. This is due to the high level

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of complexity of the problem in question. However, it is Taiwan Phone Number List necessary to extend this analysis to more general situations. For one thing, realistic black holes are not static, but are rotating. On the other, it is probable that certain properties, called non-perturbations, are not captured by a rough analysis. Thermodynamic systems In general, a black hole is characterized by only three numbers: its mass, its angular momentum, and its charge. In Einstein’s theory, there is a single black hole for each value of these parameters: if two holes have the same mass, angular momentum, and charge, then they are identical. On the other hand, one of the most important results of the 20th century in theoretical physics was the discovery that black holes are

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thermodynamic systems. This result, due to the work of many scientists among which Stephen Hawking stands out, reveals that certain properties of a black hole -such as its mass or its area- correspond to thermodynamic properties (analogous, for example, to those of a saucepan with water) such as internal energy, entropy, and temperature. One particularly interesting type of black hole is those with zero temperatures. These are called “extremals” and they were the ones studied by the UAM researchers. “In our work we found that, on the one hand, the corrections modify the black holes of general relativity, altering their size and shape. But unlike what happens in Einstein’s theory, we find that these black holes are not the only ones that exist

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