P&A Colloquium

Colloquium is held at Chemistry-Physics building (CP), 505 Rose street.
Refreshments with the speaker are served at 3:00 pm in CP-179.

A full list of past and upcoming recordings can be found here.

Dynamics at the edge: charge fractionalization and near-stationary high energy state

Host: Murthy

Title:  Dynamics at the edge: charge fractionalization and near-stationary high energy state 

 
Abstract:  Ergodic many-body systems are expected to reach quasi-thermal equilibrium. Indeed, the energy distribution in quantum Hall edge modes with short-range interactions generally relaxes to a near-thermal asymptotic state that can be described in terms of charge fractionalization. Surprisingly, high-energy electrons injected into a single edge mode with finite range interactions can stabilize over a long time scale in a state far from a thermal one: the resulting many-body state consists of rapidly decaying transient components followed by a near-steady-state distribution with a peak near the injection energy. 
Date:
-
Location:
Chem-Phys 155

Quantum Codes from Condensed Matter to Quantum Gravity

Title: Quantum Codes from Condensed Matter to Quantum Gravity

Abstract: I will explore the appearance of quantum codes in diverse contexts, from the toric code of condensed matter physics to holographic codes  in quantum gravity.   The contexts and implementations of these codes  vary widely, but their structures have much in common and suggest a deeper connection between them. 

Date:
-
Location:
Chem-Phys 155

Combining Galaxy and CMB Surveys — all the science that “comes for free”

Host: Su

 

Title: Combining Galaxy and CMB Surveys — all the science that “comes for free”

 

Abstract: The LCDM model has been extraordinarily successful. In the past 20 years, the cosmology community has worked hard to make ever more precise measurements of the LCDM parameters using large datasets from cosmic surveys. As error bars shrink and several tensions arise, we are eager to look for new and different ways of making robust statements of the LCDM paradigm. In this talk I like to focus on one particular direction where we can get new information to help this effort — by combining different cosmic surveys, in particular galaxy and CMB surveys. I will first describe the latest cosmological analysis using the Dark Energy Survey (DES) and CMB lensing from the South Pole Telescope (SPT) and Planck. Then I will talk about combining DES galaxies and the thermal Sunyaev Zel'dovich (tSZ) effect measured from SPT and Planck to learn about the baryonic feedback in our galaxies. These analyses will highlight the power of combining different datasets to tackle some of the most pressing issues in observational cosmology today. 

Date:
-
Location:
Chem-Phys 155

Cosmic Building Blocks: Forming Planets from Tiny Grains of Dust

Host: Su

This colloquium will be remote over zoom.

Title: Cosmic Building Blocks: Forming Planets from Tiny Grains of Dust

Abstract: Planet formation takes place in disks of dust and gas around young stars, where the dust grains are the building blocks to form new planets.  Nevertheless, capturing the planet-formation process is challenging as disks are complex and dynamic environments.    Observational studies of both disks and planet formation are rapidly changing with the development of high resolution and multi-wavelength instrumentation.    With current capabilities, we can characterize structural features in disks, study their chemistry, and even detect young protoplanets embedded in these systems.    In this presentation, I will provide an overview of both current and future capabilities, highlighting stunning images and results.  I will also discuss some of the challenging open questions and how future research may tackle many of these questions.

Date:
-
Location:
Zoom

Cloudy - numerical simulations of non-equilibrium plasmas and their spectra

Title: Cloudy - numerical simulations of non-equilibrium plasmas and their spectraHow Stars Form

Abstract:  Most of the quantitative information we have about the universe comes from spectroscopy, most often of emission lines or the continuous broad-band spectral energy distribution. Observations cover the electromagnetic spectrum from the radio to the gamma-ray.  The material producing the spectrum is so far from thermodynamic equilibrium that concepts like temperature do not apply.  Numerical simulations of the conditions in the plasma must be done from first principles, working back to atomic cross sections and rate coefficients.  A large system of balance equations is solved to determine the level populations within atoms or molecules and the abundance of each ion or molecule.  The cloud is optically thick, so the transfer of radiation out of the cloud and reaching our telescopes must be solved simultaneously. The result is a prediction of the full spectrum with a minimum of free parameters.  Cloudy is an open-source code that solves all these problems.  It was developed almost entirely here in Lexington and is widely used across the astronomical community. I developed Cloudy for my research, and I will describe some of its applications by my group and as well as by the astronomical community.

 

Date:
-
Location:
Chem-Phys 155

The Heavyweight W boson - an Upset to the Standard Model of Particle Physics

Host: Gardner

Title: The Heavyweight W boson - an Upset to the Standard Model of Particle Physics

Abstract: The Standard Model of particle physics has been a crowning achievement of fundamental physics, culminating in the discovery of the Higgs boson in 2012. As a quantum theory of the building blocks of matter and forces, it has been one of the most successful theories in science. The recent measurement of the mass of the W boson disagrees with the theory prediction. This upset to the Standard Model may point towards exciting new discoveries in particle physics in the coming years. We will discuss the Standard Model, the crucial role of the W boson, and how it has become the harbinger of new laws of nature. 

 
Date:
-
Location:
Chem-Phys 155

The superconducting insulator

Host:  Murthy

Title: The Superconducting Insulator

Abstract: Many two-dimensional superconductors undergo a transition to an electric insulator as a function of different parameters such as thickness, disorder, magnetic field, chemical composition etc. This superconductor-insulator-transition has been an active area of research for the last few decades, nevertheless, some fundamental questions remain unsolved. In particular, the nature of the insulating phase, which shows unconventional transport properties, is unclear. One exciting scenario suggests that this phase incorporates superconducting fluctuating islands embedded in an insulating matrix, making it exceptional and unsimilar to any conventional superconductor or insulator.

In this colloquium I will present findings, obtained by our group as well by others, demonstrating the uniqueness of this “superconducting insulator”.  These include a disorder enhanced superconducting energy gap, a novel proximity effect, unusual vortex motion and excess superconducting specific heat in the insulator.  These results provide important insight into the physics governed by the interplay between disorder and two-dimensional superconductivity. 

Date:
-
Location:
Chem-Phys 155

Effective field theory, factorization and renormalization: neutrino interactions, the Fermi function and more

Title:  Effective field theory, factorization and renormalization: neutrino interactions, the Fermi function and more
 
Abstract:  Precisely calculating differences between muon- and electron-neutrino interactions is difficult, but is vital for correctly interpreting neutrino oscillation experiments. I describe recent progress with powerful quantum field theory techniques to precisely determine the ratio of νe and νµ cross sections.  The beta decay Fermi function describes electron propagation in a nuclear Coulomb field, and accounts for QED radiative corrections that are enhanced at small electron velocity β or large nuclear charge Z.  Such enhanced corrections impact a variety of processes in and beyond the Standard Model, ranging from nuclear beta decay to dark matter annihilation signals.  I present the field theory factorization formula for the Fermi function and discuss implications for precision measurements. 
Date:
-
Location:
Chem-Phys 155

Organic Semiconductors: Opportunities (and Obstacles) to Technological Application

Organic light emitting diodes (OLEDs) were introduced into commercial application in the early 2000's and are now used regularly in phone screens and high-end TVs, while organic photovoltaics and transistors have not found the same technological success. In this talk, I will cover some of the fundamental performance and physical reasons that these devices are hindered while OLEDs flourish. Looking into the future beyond traditional electronics, I will discuss the unique physical properties of organic semiconductors that make them suitable for the development of spin-based devices and room temperature excitonic devices.

 

Host: Joe Brill

Date:
-
Location:
CP 155
Event Series:
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