Evolution of Randall-Sundrum Black Holes in Dense Media
Veronique Van Elewyck
Abstract
In the framework of Randall-Sundrum model, we discuss the evolution of microscopic black holes created by cosmic particles hitting a neutron or a strange star. We set up the general equations of evolution for the black hole mass and momentum in a dense medium, and discuss the possibility of collapse due to the black hole's growth inside the star.
Create a lesson
Related papers
From Axion Detection to Dark Matter Astronomy
Jae Hyeok Chang, Stefano Profumo
Spurious Singularities in Dipole Subtraction Cross Sections and their Damping with Convergence Factors
Michael H. Seymour, Andrzej Siódmok, James Whitehead
Radiative transitions of hybrid mesons
Shahriyar Jafarzade, Eric S. Swanson
DUNE Beam-Energy Dependence of Sensitivity to the Violation of the Equivalence Principle
Monjowara Khatun, Debajyoti Dutta
Modified hydrogen recombination rate due to non-Hubble redshift effects
I. V Krasnov, N. S. Nedelko
Probing the Axion--Photon--Dark Photon Interaction with LHC Mono-Photons and Fermi-LAT Gamma-Ray Lines
Chuan-Ren Chen, Takaaki Nomura, Van Que Tran