MODELING THE BROAD-BAND EMISSION FROM THE GAMMA-RAY EMITTING NARROW-LINE SEYFERT-1 GALAXIES 1H 0323+342 AND B2 0954+25A

Modeling the Broad-Band Emission from the Gamma-Ray Emitting Narrow-Line Seyfert-1 Galaxies 1H 0323+342 and B2 0954+25A

Prior to the Fermi-LAT era, only two classes of Active Galactic Nuclei (AGN) were thought to harbor relativistic jets that radiate up to gamma-ray energies: blazars and radio galaxies.The detection of variable gamma-ray emission from Narrow Line Seyfert 1 (NLSy1) galaxies has put them on the spotlight as a new class of gamma-ray qf1510 emitting AGN

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Black hole with quantum potential

In this work, we investigate black hole (BH) physics in the context of quantum corrections.These quantum corrections were introduced recently by replacing classical geodesics with quantal (Bohmian) trajectories and hence form a quantum Raychaudhuri equation (QRE).From the QRE, we derive a modified Schwarzschild metric, and use that metric to invest

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