Jorge Armando Rueda Hernandez

Professor - Joint appointment UNIFE-ICRANet

University of Ferrara

Italy

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About

Jorge Armando Rueda Hernandez is a Professor with a joint appointment at UNIFE-ICRANet, affiliated with the University of Ferrara in Italy. His research focuses on astrophysical phenomena, including black holes, neutron stars, and dark matter, as reflected in his recent publications. Notable areas of study include the dynamics of magnetized neutron star binary mergers, the role of mass in black hole formation, and the connections between gamma-ray bursts and compact objects.

Articles (21)

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2022

Collaborators (3)

Cristiano Guidorzi

Associate Professor

University of Ferrara

ITALY

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Liang Li

Faculty (tenure associate professor)

ITALY

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Simonetta FILIPPI

Full Professor of Theoretical Physics

Università Campus Bio-Medico di Roma

ITALY

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Jorge Armando Rueda Hernandez

Research Interests

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About

Articles (21)

Short GRB 090510: A magnetized neutron star binary merger leading to a black hole

Fermionic dark matter spikes: Origin and growth of black hole seeds

Role of the irreducible mass in repetitive Penrose energy extraction processes in a Kerr black hole

Long and short GRB connection

Can the Central Compact Object in HESS J1731–347 Be Indeed the Lightest Neutron Star Observed?

Probing Electromagnetic Gravitational-wave Emission Coincidence in a Type I Binary-driven Hypernova Family of Long Gamma-Ray Bursts at Very High Redshift

Baryon-induced Collapse of Dark Matter Cores into Supermassive Black Holes

Impact of stratified rotation on the moment of inertia of neutron stars

Occurrence of Gravitational Collapse in the Accreting Neutron Stars of Binary-driven Hypernovae

Neutron Star Binaries Produced by Binary-Driven Hypernovae, Their Mergers, and the Link between Long and Short GRBs

Matching Slowly Rotating Spacetimes Split by Dynamic Thin Shells

On the growth of supermassive black holes formed from the gravitational collapse of fermionic dark matter cores

Fermionic Dark Matter: Physics, Astrophysics, and Cosmology

Galaxy Rotation Curves and Universal Scaling Relations: Comparison between Phenomenological and Fermionic Dark Matter Profiles

On the Optical Transients from Double White-dwarf Mergers

GRB-SN Association within the Binary-driven Hypernova Model

The Double White Dwarf Merger Progenitors of SDSS J2211+1136 and ZTF J1901+1458

On the X-Ray, Optical, and Radio Afterglows of the BdHN I GRB 180720B Generated by Synchrotron Emission

Evidence for the transition of a Jacobi ellipsoid into a Maclaurin spheroid in gamma-ray bursts

First minutes of a binary-driven hypernova

What does lie at the Milky Way centre? Insights from the S2-star orbit precession

Collaborators (3)

Cristiano Guidorzi

Liang Li

Simonetta FILIPPI

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