We consider perturbations of the massless Dirac field in the background of a black hole solution found by Bodendorfer, Mele, and M\"{u}nch (BMM), using a polymerization technique that furnishes contributions inspired by Loop Quantum Gravity (LQG) Theory. Using the sixth order WKB method, we analyzed its quasinormal modes for several modes, multipole numbers and the two classes of BMM black holes. We also considered the potential that governs these perturbations to analyze the bound on the Greybody Factor (GF) due the emission rates of particles. As results, we found that the Loop Quantum Gravity parameters are responsible for raising the potential and the real and imaginary parts of the quasinormal frequencies and decrease the bound on the ...
We study the propagation of massless scalar fields non-minimally coupled to gravity in the backgroun...
The system of gravity coupled to the non-rotational dust field is studied at both classical and quan...
Quantum gravity is effective in domains where both quantum effects and gravity are essential, such a...
We consider perturbations of the massless Dirac field in the background of a black hole solution fou...
We study the quantum dynamics of the Lema\^itre-Tolman-Bondi space-times using a polymer quantizatio...
The gravitational collapse plays an important role in the formation of black holes as well as for ou...
We study the greybody factors, quasinormal modes, and shadow of the higher dimensional de-Sitter (dS...
We give a pedagogical introduction to black holes (BHs) greybody factors (GFs) and quasinormal modes...
Greybody factors are transmission probabilities of the Hawking radiation, which are emitted from bla...
We derive effective equations with loop quantum gravity corrections for the Lema\^itre-Tolman-Bondi ...
In modified theories of gravity, the potentials appearing in the Schr\"odinger-like equations that d...
In this work, we consider two recently introduced novel regular black hole solutions and investigate...
Vacuum quantum fluctuations near horizons are known to yield correlated emission by the Hawking effe...
The Effective Field Theory (EFT) of perturbations on an arbitrary background geometry with a timelik...
We calculate numerically the quasinormal frequencies of the Klein-Gordon and Dirac fields moving in ...
We study the propagation of massless scalar fields non-minimally coupled to gravity in the backgroun...
The system of gravity coupled to the non-rotational dust field is studied at both classical and quan...
Quantum gravity is effective in domains where both quantum effects and gravity are essential, such a...
We consider perturbations of the massless Dirac field in the background of a black hole solution fou...
We study the quantum dynamics of the Lema\^itre-Tolman-Bondi space-times using a polymer quantizatio...
The gravitational collapse plays an important role in the formation of black holes as well as for ou...
We study the greybody factors, quasinormal modes, and shadow of the higher dimensional de-Sitter (dS...
We give a pedagogical introduction to black holes (BHs) greybody factors (GFs) and quasinormal modes...
Greybody factors are transmission probabilities of the Hawking radiation, which are emitted from bla...
We derive effective equations with loop quantum gravity corrections for the Lema\^itre-Tolman-Bondi ...
In modified theories of gravity, the potentials appearing in the Schr\"odinger-like equations that d...
In this work, we consider two recently introduced novel regular black hole solutions and investigate...
Vacuum quantum fluctuations near horizons are known to yield correlated emission by the Hawking effe...
The Effective Field Theory (EFT) of perturbations on an arbitrary background geometry with a timelik...
We calculate numerically the quasinormal frequencies of the Klein-Gordon and Dirac fields moving in ...
We study the propagation of massless scalar fields non-minimally coupled to gravity in the backgroun...
The system of gravity coupled to the non-rotational dust field is studied at both classical and quan...
Quantum gravity is effective in domains where both quantum effects and gravity are essential, such a...