Events on Thursday, March 12th, 2026
- R. G. Herb Condensed Matter Seminar
- Only the ambidextrous can flock: chirality destroys order in polar active matter
- Time: 10:00 am - 11:00 am
- Place: 5310 Chamberlin Hall
- Speaker: John Toner, University of Oregon
- Abstract: I'll show that flocks of chiral living creatures (i.e., organisms that are right or left handed) moving on a surface, composed of critters can not form a long range ordered flocking state (i.e., a state in which the spatially averaged velocity vector
is non-zero,) even though it is well-known that they can order in this way if they are achiral. "Immortal" flocks (flocks in which the creatures are not being born and dying on the time scales iof interest) prove to be much more nearly ordered than "Malthusian" flocks in which birth and death do occur. Immortal flocks have a phase which, although not truly long-range ordered, better ordered than the "Kosterlitz-Thouless quasi-long-range ordered phase" (KT phase) of the equilibrium 2d XY model. This phase exhibits non-unversal exponents of a type very different from the familiar non-universal exponents of the KT phase. - Host: Alex Levchenko
- Astronomy Colloquium
- Probing Supermassive Black Holes in the Golden Era of Time Domain Astronomy
- Time: 3:30 pm - 4:30 pm
- Place: 4421 Sterling Hall
- Speaker: Dr. Jason Hinkle, University of Illinois Urbana-Champaign
- Abstract: Optical transient surveys have ushered in the golden era of time-domain astronomy and exposed an unexpected diversity of transient phenomena, including nuclear transients: flares powered by accretion onto supermassive black holes (SMBHs). These transients provide a means to identify and study otherwise quiescent SMBHs across a range of masses and redshifts. This complements the longstanding study of actively-accreting SMBHs, or active galactic nuclei (AGNs). In this talk, I will discuss the physics underpinning these transients, the role of the surrounding nuclear environment in setting their observable signatures, and their utility as probes of SMBHs. I will conclude with a look towards the future of nuclear transients in the era of deep surveys like LSST and Roman.