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Events on Monday, October 26th, 2026

Theory Seminar (High Energy/Cosmology)
Prospects for Supernova Magnetometry with Neutrinos
Time: 11:30 am - 1:00 pm
Place: Chamberlin 5280
Speaker: Garv Chauhan, Arizona State University
Abstract: A Galactic supernova neutrino burst could offer a way to investigate the magnetic fields of a newly formed neutron star. Electron spin polarization in a strong magnetic field introduces a directional dependence in neutrino interactions, potentially producing anisotropic emission from the proto–neutron star. If the magnetic axis is inclined to the rotation axis, this anisotropy can generate a periodic modulation in the neutrino signal observed at Earth. In this talk, I will discuss the physical origin of this effect and a phenomenological framework for estimating its impact on the electron-antineutrino flux. I will examine the prospects for detecting such a modulation with IceCube, discussing the potential detection reach and whether the modulation’s amplitude and temporal evolution could constrain the magnetic-field strength and its evolution near the neutrinosphere. I will also discuss the potential role of complementary neutrino observations with DUNE, gravitational-wave measurements, and future IceCube-Gen2 capabilities. This approach could open a new avenue for supernova magnetometry, offering insight into the magnetic fields of newborn neutron stars.
Host: Toni Bertólez-Martínez
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Plasma Physics (Physics/ECE/NE 922) Seminar
A Dipole Approach to Fusion Power in Space
Time: 12:00 pm - 1:00 pm
Place: 2241 Chamberlin Hall
Speaker: Edward Hinson, Zephyr Fusion
Abstract: Access to power beyond tens of kilowatts remains a central constraint on activity in space. Numerous mission architectures studied in detail for microgravity manufacturing, human habitation, and propulsion, among others, call for power at the megawatt scale and above. However, the largest power systems in orbit are solar arrays operating at the 100 to 200 kW level, on crewed, government-operated platforms. Because array power scales with collecting area, arrays become impractically large at megawatt power levels. At the megawatt scale and above, the remaining options are nuclear. Fission systems at the few-kilowatt electric level have flown, and megawatt-class designs have been studied, but fission carries regulatory and programmatic risk. Fusion has received comparatively little study as a space power source.

Fusion plasmas in space do not need to be as compact, or as high power as is customary in magnetic fusion, though launched components are bound by fairing volume and mass. For some magnetic configurations, the space environment can provide access to a large magnetized vacuum volume at low marginal cost. Zephyr Fusion is developing a superconducting dipole as the basis for a megawatt-class fusion power system in space.

The talk outlines the requirements and advantages specific to a fusion system in the space environment, along with Zephyr Fusion's development path, including the partnerships assembled in its first year and an orbital superconducting magnet demonstration targeted for 2028.

Bio: Edward Hinson is co-founder and CEO of Zephyr Fusion, a Y Combinator company based in San Diego, California. He received his Ph.D. in Nuclear Engineering and Engineering Physics from the University of Wisconsin–Madison in 2015.
Host: Vladimir Zhdankin
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