Three dimensional massive gravity and the bigravity black hole

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It is for this reason that we are able to calculate all of the parameters and functions of the emergent theory: the gauge group and the matter content; the Yukawa couplings and

To conclude, we have performed the first dedicated search for microscopic black holes at a particle accelerator and set limits on their production in the model with large

Let us now explore the consequences of (6.10); we will take τ = 2π iβ in what follows, so that we have an ordinary partition function. In other words, in the high temperature

Abstract: We study the first-order in α 0 corrections to non-extremal 4-dimensional dy- onic Reissner-Nordstr¨ om (RN) black holes with equal electric and magnetic charges in

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

Known as Generalized quasi-topological gravities (GQGs), such theories repre- sent extensions of GR that are free of instabilities and ghosts at the linear level, and whose equations

In order to analyze if the candidate genes contained in the amplicons are altered in primary tumors and other cell lines, we analyzed expression data obtained in a previous study