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Events on Thursday, March 7th, 2013
 Special Seminar
 The two sides of a semiclassical spin
 Time: 10:00 am
 Place: 5310 Chamberlin
 Speaker: Feifei Li, Northwestern University
 Abstract: A spinning electron and a spinning gyroscope represent the two ultra limits that spin can behave. One is purely quantum, while the other is purely classical. In this talk, I would like to discuss what happens for a semiclassical spin with intermediate magnitude of angular momentum. My talk consists two parts. In the first half, I would like to tell a story about the singlemolecularmagnet Fe_{8}. Fe_{8} is a molecule made of about a hundred atoms, yet it behaves like a single giant spin of J = 10 at low temperatures. Quantum interference causes the tunneling gap of this molecule to oscillate with applied magnetic field and to vanish at certain magnitude and direction of the magnetic fields, known as diabolical points. My story is about how these diabolical points were discovered, missed and rediscovered. The second half of my talk will focus on the quantumclassical correspondence for spin. The quantumclassical correspondence for a particle has been formulated by Moyal, who in a seminal paper, showed that quantum mechanics can be expressed as a quasistatistical theory in the phase space of coordinate and momentum. Moyal's formalism unified Weyl ordering and Wigner quasidistribution function, providing an invertible map between dynamical variables on the classical phase space and operators on the quantum mechanical Hilbert space. Moyal has also shown that the commutator of two operators is the Poisson bracket to leading order of $hbar$. All this was done for position and momentum. Here I present a Moyal treatment for spin, and show that, in the classical limit, the Weyl symbol for a spin commutator is i times the Poisson bracket of the corresponding Weyl symbols.
References
[1] Feifei Li and Anupam Garg, Numerical search for diabolical points in the energy spectrum of the singlemolecule magnet Fe_{8}, Phys. Rev. B 83, 132401 (2011).
[2] José E. Moyal, Quantum Mechanics as a Statistical Theory, Proc. Cambridge Philos. Soc. 45, 99 (1949).
[3] Feifei Li, Carol Braun, and Anupam Garg, The WeylWignerMoyal Formalism for Spin, arXiv:1210.4075v2 (2012).
 Host: Friesen & Coppersmith
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 Astronomy Colloquium
 Stellar Mergers and Interactions: Yes, Virginia, Stars Do Collide.
 Time: 3:30 pm
 Place: 4421 Sterling Hall
 Speaker: Alison Sills, McMaster University
 Abstract:
I will discuss strong interactions between stars in a variety of
environments. Despite the vast (average) interstellar distances, stars are social creatures and tend to live in pairs, multiples, or groups. Under these circumstances, stars can, and do, modify each other's mass, radius, composition, and overall evolution through gravitational encounters ranging from wind mass transfer in a binary system to complete stellar collisions and mergers. I will show how such events can change our understanding of particular stellar systems, how they can explain the properties of many unusual objects, and how interactions could change the environment these stars live in. The emphasis for this
talk will be on the modelling of these interactions, and I will
demonstrate how a combination of stellar evolution, stellar dynamics, and hydrodynamics can bring some understanding to these complicated systems.  Host: Robert Mathieu
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