Tenure track hiring committee
The tenure track hiring committee will meet in POT 721
Qualifying Exam
Title: Non-Vanishing Homology of the Matching Complex
Abstract: A matching on a graph G is any subgraph where the maximum vertex degree is 1. Since edge-deletion preserves the property of being a matching, the set of all matchings on G forms a simplicial complex M(G). We will survey results on the lowest non-vanishing homology group for M(K_n) and discuss the extension of these results to more general graphs, specifically the r-stable ones. Prior familiarity with simplicial complexes and homology is assumed.
Physics and Astronomy Colloquium: The Rainbow, the Rowland Circle, and other Geometric Adventures in Flat Space
The word "geometry" invokes imagery of curved space and singularities to physicists, warp drives and worm holes to physics enthusiasts, and Euclidean Dementors to middle-schoolers. But geometry (the structure of space) is at the heart of all physics, even in plain flat space. This talk is a series of three loosely-connected vignettes aspiring to illustrate the ubiquity of geometry in understanding our local environment.
Refreshments will be served in CP 179 at 3:15 PM
Astro Seminar: Evidence for New relations between Gamma Ray Bursts Prompt and X-ray Afterglow Emission from 10 Years of Swift
Gamma-Ray Bursts (GRBs) are the most energetic transient events in the Universe.
Not only do they represent the violent end of a massive star and the birth of
a black hole, but their explosions allows us to trace them throughout the
entire Universe. With the launch of the NASA Swift Gamma-Ray Burst Explorer
Mission our knowledge of GRBs has been revolutionized. With its fast slew
capacity it is able to be on the position of a GRB within a minute or two after
the GRB is detected, giving us access to the earliest phases of a GRB afterglow.
Since its launch in November 2004, Swift has discovered more than 900 bursts,
about 280 with spectroscopic redshift measurements - providing us the
largest sample in history with prompt and afterglow observations. This unique
sample enables us to perform unprecedented statistical studies of GRBs.
In my talk I will review the history of GRB discoveries and their importance to
astrophysics. I will present the Swift mission and explain what is unique and
exciting about it and how Swift has given us new evidence for
connections between the GRB prompt and afterglow emission. The fate of the
burst is already determined during the explosion of the star.
I will finish the talk by looking into the future and explain how we can use
predictive data mining tools to determine the afterglow light curves and the
redshifts of the bursts based on observed properties of the burst.
The talk is primarily based on results published in
Grupe et al., 2013, ApJS, 209, 20
Condensed Matter Seminar: Transport and Surface Potential Characterizations of Metal Oxides: Understanding Interplay among Charges, Surface Plasmons, and Photons
Discrete CATS Seminar
Title: An Introduction to Symmetric Functions, part II
Abstract: In this pair of talks, I will provide an overview of basic results regarding symmetric functions. My goal will be to create a "road map" for anyone who is interested in reading more about these objects in Chapter 7 of Stanley's Enumerative Combinatorics, Volume 2 (if you have a copy and are interested, it might be helpful to bring it with you). We will motivate the study of symmetric functions by interpreting them as generalizations of subsets and multisubsets of [n], so these talks should be accessible to anyone who is familiar with the material from the first part of MA 614.