An Extreme Rotating Black Hole in New Massive Gravity Theory

(Received 4 November 2019; accepted 8 January 2020; published 10 February 2020) We obtain new solutions of Einsteinian cubic gravity coupled to a Maxwell field that describe the

In this article we compute explicitly the first-order α 0 (fourth order in derivatives) corrections to the charge-to-mass ratio of the extremal Reissner-Nordstr¨ om black hole

Although in this case there is no sound horizon as the sound speed is zero, the presence of a nonvanishing anisotropic stress creates a new anisotropic horizon in the evolution of

Given the essential role that the event horizon plays in the thermodynamic descrip- tion of a black hole and in turn of the dual thermal state, it arises the question of

If the starting point of our evolution has a total mass whose Schwarzschild radius is below the wall position, it will never be possible to form a black hole (as the spacetime ends

Following the analogy with the BMS group on null infinity, it has been conjectured that the horizon supertranslations may act non-trivially on the black hole geometry, transform-

In sum, we observe some influence of property rights theory variables on exercising control in the cooperative, mainly when focusing on the time horizon of investments and on

that in the framework of a rotating mass matrix (i.e. one which has an ori- entation in generation space which is scale-dependent) we have constructed earlier [10] to explain