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MAIN RESEARCH INTERESTS

My research program explores the interface between quantum gravity phenomenology, nuclear astrophysics, and quantum field theory, with a unifying focus on testing fundamental physics through both theoretical modeling and observational signatures. At the core of this effort lies the development of beyond-Standard-Model frameworks that probe the limits of spacetime symmetry, high-energy interactions, and emergent gravity.

 

In quantum gravity phenomenology, I investigate:​

  • Higher-order gravity in arbitrary dimensions, where derivative expansions modify Einstein-Hilbert dynamics and black hole solutions, with implications for renormalizability and unitarity;

  • Analogue gravity models in condensed-matter systems, which simulate exotic spacetime geometries (e.g., acoustic horizons) to test semiclassical gravity predictions;

  • Lorentz symmetry violation (LSV) via the Standard Model Extension (SME), constraining spacetime anisotropy through astrophysical neutrinos, gamma-ray bursts, and gravitational waves.

 

My work in nuclear astrophysics connects these theoretical constructs to extreme environments:​

  • Neutron star interiors as laboratories for modified electromagnetism (e.g., nonlinear Maxwell extensions) and nonminimal couplings;

  • Neutrino propagation in strong magnetic fields, with attention to spin-flip transitions and magnetic moment anomalies;

  • Exotic compact objects with quark matter or topological defects (e.g., magnetic monopoles), where higher-derivative terms alter mass-radius relations.

Within quantum field theory, I specialize in:​

  • Neutral-particle electrodynamics, including Aharonov-Casher-type effects and emergent gauge structures;

  • Gyromagnetic ratio deviations from Dirac’s prediction, probing composite models or spacetime granularity;

  • Nonminimal couplings (e.g., axion-photon, curvature-fermion) that generate testable thresholds in high-energy collisions or cosmic-ray spectra.

 

This integrated approach—spanning mathematical consistency, astrophysical viability, and experimental constraints—aims to identify observational windows into quantum spacetime structure while advancing the dialogue between formal theory and multimessenger astronomy.

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