Physics Colloquium – Shuntaro Sumita

Lapham 160 3209 N. Maryland Ave., Milwaukee, WI, United States

Shuntaro Sumita, Kyoto University
Topological Gapless Points in Superconductors: from the viewpoint of symmetry
Topology in quantum physics has attracted much attention in recent condensed matter physics. One famous example is the topological insulator, which has a finite gap in its energy spectrum.

Physics Colloquium – Dr. Vincent Smith

Lapham 160 3209 N. Maryland Ave., Milwaukee, WI, United States

Dr. Vincent Smith, Honorary Research Fellow; University of Bristol (UK)
CERN: An In-Depth Look

CERN (near Geneva, Switzerland) was founded in 1954 by 12 European countries and now has 22 “member states.” I have been fortunate to have worked on experiments there since 1976, when the new Super Proton Synchrotron was commissioned. Since the late 1990’s, I have been a member of the Compact Muon Solenoid collaboration, one of the big experiments on CERN's Large Hadron Collider. I worked initially on the development, installation and commissioning of the Electromagnetic Calorimeter, a system of over 75,000 crystals of Lead Tungstate (PbWO_4) to measure the energy and direction of high energy gamma rays, electrons and positrons from collisions in the center of the detector.

No Physics Colloquium: Spring Break

Lapham 160 3209 N. Maryland Ave., Milwaukee, WI, United States

As the University is currently on Spring Break, there is no colloquium scheduled for Friday, March 22.

No Physics Colloquium Scheduled

Lapham 160 3209 N. Maryland Ave., Milwaukee, WI, United States

There is no Physics colloquium currently scheduled for this date.

Physics Colloquium – Aaron Viets

Lapham 160 3209 N. Maryland Ave., Milwaukee, WI, United States

Aaron Viets, PhD Candidate, University of Wisconsin-Milwaukee

Optimizing Advanced LIGO's Scientific Output with Fast, Accurate, Clean Calibration

Fast, accurate calibration of Advanced LIGO data is an essential part of gravitational-wave astronomy, necessary for prompt electromagnetic follow-up of gravitational-wave events and reliable estimation of source parameters.

Physics Colloquium – Victor Muñoz

Lapham 160 3209 N. Maryland Ave., Milwaukee, WI, United States

Victor Muñoz, University of California-Merced

Lessons About Biomolecular Rate Theory from Ultrafast Kinetics and Single-Molecule Spectroscopy of Fast-Folding Proteins

Natural proteins fold and unfold with rates that define their biological properties and vary vastly from protein to protein. Understanding how these rates are determined is essential to decipher the mechanisms of protein folding, but is also a convenient system to explore the fundamental aspects of biomolecular rate theory. Protein (un)folding rates are described as diffusion on a free energy surface obtained by projecting the protein-solvent hyper-dimensional phase space (or folding energy landscape) onto one or few order parameters that capture the reaction’s progress.

Physics Colloquium – Piotr E. Marszalek

Lapham 160 3209 N. Maryland Ave., Milwaukee, WI, United States

Piotr Marszalek, Duke University

Nanomechanics of Biopolymers Beyond Their Entropic Elasticity Regime

Compared to other single-molecule techniques, AFM-based force spectroscopy uses stiff force transducers and it may apply large stretching forces to molecules, enabling their structural modifications and capturing high energy conformations that cannot be examined by (for example) X-ray crystallography or NMR. In my talk, I will present our AFM stretching and relaxation studies, supported by computer simulations of individual molecules of DNA and proteins.

Physics Colloquium – Naomi McClure-Griffiths

Lapham 160 3209 N. Maryland Ave., Milwaukee, WI, United States

Professor Naomi McClure-Griffiths, Professor at the Research School of Astronomy & Astrophysics in the College of Science – Australian National University

The Milky Way and Magellanic Clouds as Laboratories for Understanding the Evolution of Galaxies

Galaxies are not closed box systems. Their evolution is impacted by gas accreted via inflow, gas lost from the disk via large-scale outflows and gas circulations via the halo. Many simulations of galaxy formation and evolution have highlighted the importance of feedback in reproducing the observable Universe. In this talk, I will present an overview of observational evidence for outflows within the Milky Way and Magellanic Clouds.