Conserved quantities for a charged rotating black holes in 5D Einstein Maxwell Chern Simons theory

These properties of the LIGO black hole binaries would come naturally from early universe models of PBH formation from large peaks in the matter power spectrum, arising both in

Figure 1: RG flows from SYM (dotted lines) and between CFT’s (solid lines) dual to BPS domain-wall solutions within the SU(3) and SO(4) invariant sectors of the dyonic ISO(7)-

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

By translating the cross section limits into ADD model expectations, we can exclude the production of semiclassical black holes with a minimum mass varying from 3.9 to 5.3 TeV

Typical benchmark signal points for some of the models studied, corresponding leading- order cross sections σ, optimal selections on the minimum decay multiplicity (N ≥ N min )

(Spectroscopic typing is facilitated by the fact that, due to the fast ejecta velocities expected of KNe, 0.03 –0.30c, their spectra are expected to be featureless or only have

Although the cut-off dependence of the HEE In section 8.1 we have argued that for θ ≤ 0, in order to extract the structure of terms for general higher-curvature gravities, it suffices

The paper’s novelties include: (i) a mathematical treatment of fragments and a seaming mechanism of proxies to enable inter-fragment referencing, (ii) fragmentation strategies,