Hawking radiation in NS5 and little string theory

We construct a one-loop effective metric describing the evaporation phase of a Schwarzschild black hole in a spherically symmetric null- dust model.. This is achieved by quantising

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

The difficulty stems from the fact that the measurement of orbits at the Galactic center requires understanding 5 major components: (1) the astrophysical content near the black

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

The calculations show that the interference pattern of the hole pair is determined by two scattering mechanisms: (i) the electric field excited by the external illumination at the

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

As we have seen, even though the addition of a cosmological constant to Einstein’s eld equations may be the simplest way to obtain acceleration, it has its caveats. For this rea-

We have also shown that the stability of the di fferent moiré patterns is the result of a subtle energy balance between the energy required to corrugate the gra- phene, that