Our findings suggest that the entropy bound and the Generalized Second Law of black holes are satisfied in the Einstein gravity under the first-order perturbation from the quadratic curvature corrections, and t
In November 1915, Einstein presented a series of lectures before the Prussian Academy of Sciences in which he described his theory of general relativity. The final lecture climaxed with his introduction of an equation that replaced Newton's law of gravity. This theory considered all observers to ...
Theory of general relativity: This was a reformulation of the law of gravity. In the 1600s,Newtonformulated three laws of motion, among them, outlining how gravity works between two bodies. The force between them depends on how massive each object is, and how far apart the objects are. Ei...
“On the Electrodynamics of Moving Bodies,” where he introduced the special theory of relativity, which changed the way we think about space and time. In 1915, he completed the general theory of relativity, which provided a new interpretation of gravity and described the universe as a four-...
In 1916, Einstein presented his general theory of relativity, proposing that gravity is a curved field in the space-time continuum created by the existence of mass. He received the 1921 Nobel Prize in Physics for his discovery of the law of the photoelectric effect and his work in theoretical...
Expanding his special theory, Einstein’s general theory of relativity states that what we perceive as the force of gravity between two masses actually arises from their warping of space and time. For example, although the sun’s gravity appears to pull the earth towards it, no such force rea...
The solutions show that Einstein–Born–Infeld-dilaton gravity theory admits three novel classes of nonlinearly charged black hole solutions with the non-flat and non-AdS asymptotic behavior. Some of the solutions, in addition to the naked singularity, extreme and two-horizon black holes, produce ...
“Man can only escape the laws of this world for a flash of time. Instants of pausing, of contemplating, of pure intuition… It’s with these flashes that he is capable of the superhuman.” (Simone Weil, “Gravity and Grace”)
A toy model of Einstein gravity with a Gauss-Bonnet classically "entropic"term mimicking a quantum correction is considered. The static black holesolution due to Tomozawa is found and generalized with the inclusion of nontrivial horizon topology, and its entropy evaluated deriving the first law by...
A Matter Of Some Gravity: First Proof Of The Theory Of General Relativity According to Einstein's General Theory of Relativity, gravity is a warping of space-time by mass. If that is correct, then the most massive object in the Solar System (the Sun) should be capable of bending the...