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Eduardo Gutiérrez

Eduardo Gutiérrez — Postdoctoral Scholar — Postdoc
Office: 301B Whitmore Laboratory
Address: 104 Davey Lab University Park, PA 16802 US
+1 814 863 9605
Eduardo Gutiérrez

I am a Postdoctoral Scholar at the Department of Physics of The Pennsylvania State University.

My research focuses on the multimessenger radiative output from mergers of compact objects. To this aim, I perform numerical simulations of binary neutron star mergers and supermassive binary black holes on the verge of collision. I am especially interested in the physics of the accretion disks, winds, and jets formed in these events, and the high-energy electromagnetic radiation associated with them.

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ORCID: 0000-0001-7941-801X

Publications
  1. Eduardo Gutiérrez, Luciano Combi, Scott Noble, Manuela Campanelli, Julian Krolik, Federico López Armengol, Federico García “Electromagnetic Signatures from Supermassive Binary Black Holes Approaching Merger.” 928 2 (2022) doi:10.3847/1538-4357/ac56de
  2. E. Gutiérrez, F. Vieyro, G. Romero “Nonthermal processes in hot accretion flows onto supermassive black holes: An inhomogeneous model.” 649 (2021) doi:10.1051/0004-6361/202039671
  3. Eduardo Gutiérrez, Rodrigo Nemmen, Fabio Cafardo “A Nonthermal Bomb Explains the Near-infrared Superflare of Sgr A*.” 891 2 (2020) doi:10.3847/2041-8213/ab7998
  4. Gustavo Romero, Eduardo Gutiérrez “The Origin of Matter at the Base of Relativistic Jets in Active Galactic Nuclei.” Universe 6 7 (2020) doi:10.3390/universe6070099
About our wordmark
Monica Rincon Ramirez

The IGC wordmark was created by Monica Rincon Ramirez while she was a graduate student at the Institute. Monica enjoys drawing new connections between fundamental theory and observations. Her graduate work included general relativity, loop quantum gravity, and quantum fields in cosmological backgrounds; her thesis focused on effective quantum corrections to gravitational phenomena from spinfoams and applications to cosmology. She received her PhD in 2024.

The wordmark symbolizes the scope of research at the IGC. The base represents quantum gravity, evoking the quantum geometrical picture from spinfoams and loop quantum gravity — approaches studied at the Center for Fundamental Theory. The middle shows galaxies embedded in a smooth surface characteristic of spacetime in general relativity and the larger physical scales studied at the Center for Theoretical and Observational Cosmology. The top curves to an extreme representing a supermassive black hole accompanied by an energetic jet, with a binary black hole pair nearby — the high-energy phenomena studied at the Center for Multimessenger Astrophysics.