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Field theory in strong magnetic fields and its applications
NSF
About This Grant
This project explores the physics of extreme environments where strong magnetic fields interact with relativistic matter at very high temperatures and densities. Such conditions occur in the early Universe, within compact stellar objects like magnetars, and in quark-gluon plasma produced during high-energy nuclear collisions at relativistic colliders. Such systems exhibit unusual quantum behavior and offer critical insights into the fundamental forces of nature. The project seeks to deepen our understanding of how strong magnetic fields influence the behavior of matter under extreme conditions. This research aims at advancing scientific discovery in theoretical nuclear and astrophysics. Broader impacts include the training of undergraduate students and postdoctoral researchers. Outreach efforts will support project-based physics education at the university level and help develop a new generation of scientists equipped with advanced theoretical and computational skills. This work promotes the integration of research and education and contributes to building a strong scientific workforce. This research addresses fundamental questions in the theory of strongly magnetized relativistic systems. Using advanced quantum field theory techniques, the project investigates the influence of strong magnetic fields on the self-energy of fermions, the photon and gluon polarization tensors, and the vertex function in relativistic plasmas. While prior work has elucidated the absorptive parts of the self-energy and polarization tensors, this project aims to advance the understanding of their real parts and apply this knowledge to predict a range of observables in relativistic systems. The study focuses on systems where Landau quantization significantly alters the dynamics, such as in the magnetospheres of pulsars, the interiors of neutron stars, heavy-ion collision environments, and possibly the early Universe. Particular emphasis is placed on the interplay between quantum anomalies, such as the chiral anomaly, and strong magnetic fields. By bridging quantum theory with phenomenological applications, the research aims to generate novel predictions and insights that can guide both theoretical developments and experimental investigations in nuclear physics, astrophysics, and cosmology. This project advances the objectives of "Windows on the Universe: the Era of Multi-Messenger Astrophysics", one of the 10 Big Ideas for Future NSF Investments. This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.
Focus Areas
Eligibility
How to Apply
Up to $270K
2028-08-31
One-time $749 fee · Includes AI drafting + templates + PDF export
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