• CGCA Seminar – Reshma Anna Thomas

    Kenwood IRC 2175 Milwaukee, WI, United States

    Low-Frequency Radio Transients
    Reshma Anna Thomas
    Netherlands Institute for Radio Astronomy, University of Amsterdam

    The low-frequency radio sky (<300 MHz) remains comparatively underexplored for fast and slow transients (~ microseconds to minutes), primarily due to strong propagation effects as well as instrumental challenges. However, this regime provides unique leverage on plasma environments and emission physics that are inaccessible at GHz frequencies. Fast radio bursts (FRBs) are extragalactic coherent transients with millisecond durations, often exhibiting sub-millisecond temporal structure. I will present detections of two FRBs at 150 MHz using beamformed searches with LOFAR, which place some of the most stringent constraints to date on free–free absorption in their local environments. In parallel, a new class of Galactic sources, long-period transients (LPTs), has recently emerged, characterized by emission on second-to-minute durations and periodicities spanning minutes to hours.

  • Physics Colloquium – Sarah Villanova Borges

    Chemistry 108 2050 E Kenwood Blvd, Milwaukee, WI, United States

    Constraining Common Envelope Evolution Simulations with Observations
    Sarah Villanova Borges, PhD Candidate
    University of Wisconsin-Milwaukee

    Common Envelope Evolution (CEE) remains one of the biggest unresolved problems in binary stellar evolution, despite being the primary pathway for the formation of close binary systems. One of the main challenges in understanding CEE is its intrinsically multiscale and multiphysics nature, which makes it difficult to model with analytical or 1D models. 3D hydrodynamical simulations have therefore become essential tools for studying this phase. However, validating these simulations requires observational constraints, which are scarce. This lack of direct observations is another major obstacle in modeling CEE. One exception is luminous red novae, which is believed to correspond to CEE events that culminate in stellar mergers.

  • CGCA Seminar – Janeth Valverde

    Kenwood IRC 2175 Milwaukee, WI, United States

    Title and abstract to be determined
    Janeth Valverde
    Marquette University

    The abstract for this talk will be added as soon as it is made available.

  • Physics Colloquium – Nicholas Stone

    Chemistry 108 2050 E Kenwood Blvd, Milwaukee, WI, United States

    Gravitational Waves from Galactic Nuclei
    Nicholas Stone, Assistant Professor
    Department of Astronomy, University of Wisconsin-Madison

    The discovery of GW150914 inaugurated the era of gravitational wave (GW) astronomy, opening a new window to study our Universe's compact objects and through which to test general relativity. Now, a decade later, the LIGO-Virgo-KAGRA (LVK) collaboration has seen hundreds of GW signals, overwhelmingly from mergers of binary stellar mass black holes. Despite the many successes of GW astronomy, a zeroth-order astrophysical question remains unanswered: what astrophysical environments produce the LVK binary black holes, and by what process are they assembled? Although many formation channels have been proposed, one uniquely testable solution is the "AGN channel:" a scenario in which individual black holes pair up and merge in the dissipative gaseous environment of an active galactic nucleus.

  • Physics Colloquium – Thomas D. Killeen

    Kenwood IRC 2175 Milwaukee, WI, United States

    Novel Imaging Techniques for Studying Interactions of Membrane Receptors Among Themselves and with Downstream Signaling Partners
    Thomas D. Killeen, PhD Candidate
    University of Wisconsin-Milwaukee Department of Physics & Astronomy

    Cells rely on complex signaling networks to sense and respond to environmental stimuli, but the bigger picture of how molecular assembly leads to robust cellular signaling is only beginning to emerge. A major challenge in characterizing cellular signaling is the ability to directly observe the dynamic interactions between membrane receptors and intracellular signaling partners in living cells. To address this challenge, this work presents the development of advanced fluorescence imaging and computational analysis tools designed to improve the precision and quantitative power of live-cell micro-spectroscopy for studying protein dynamics in real time.

  • CGCA Seminar – Matt Miles

    Kenwood IRC 2175 Milwaukee, WI, United States

    Galaxy-Scale Gravitational Wave Detection: The MPTA and the Road Ahead
    Dr. Matt Miles
    Vanderbilt University

    Gravitational waves are emitted across a vast spectrum of frequencies. Ground-based detectors such as LIGO/Virgo/KAGRA observe relatively high-frequency waves from compact object mergers, while at the other end of the spectrum, the inspirals of supermassive black hole binaries produce a low-frequency rumble detectable only with a galaxy-scale instrument. By monitoring the pulses emitted by millisecond pulsars distributed across the Milky Way, pulsar timing arrays construct such a detector, spanning thousands of light-years.

  • CGCA Seminar – Shanika Galaudage

    Kenwood IRC 2175 Milwaukee, WI, United States

    Title and abstract to be determined
    Shanika Galaudage
    Northwestern University

    The abstract for this talk will be added as soon as it is made available.

  • Physics Colloquium – Cancelled

    Chemistry 108 2050 E Kenwood Blvd, Milwaukee, WI, United States

    This week's Physics Colloquium has been cancelled.

  • Physics Colloquium – Kyuil Cho

    Chemistry 108 2050 E Kenwood Blvd, Milwaukee, WI, United States

    Superconductors Investigated by High-Energy Particle Irradiation
    Dr. Kyuil Cho, Assistant Professor
    Department of Physics, Hope College

    Superconductor is a material that shows zero resistivity and Meissner effect below its critical temperature. This material has been used for various applications such as superconducting wires, medical device MRI, superconducting magnets for particle accelerators, quantum computing circuits, and many more. The superconductivity research group at Hope College conducts unique research on novel superconductors by using high energy particles. High energy particle irradiation is a useful method to generate homogeneous artificial defects on superconductors. By investigating how the defects affect the properties of superconductors, one can uncover the fundamental mechanism of superconductivity.

  • Physics Colloquium – Jorge Alegre-Cebollada

    Chemistry 108 2050 E Kenwood Blvd, Milwaukee, WI, United States

    Titin-based Molecular Underpinnings of Skeletal and Cardiac Muscle Function
    Jorge Alegre-Cebollada, PhD
    Associate Professor & Group Leader, CNIC (Spanish National Center for Cardiovascular Research)

    Titin is the largest protein in the human body. The function of the protein is not any smaller: it is critical for the contractile activity of muscles in the skeletal system and in the heart. In my presentation, I will introduce fundamental concepts that link titin nanomechanics with the macroscopic mechanical function of muscle. I will focus on our recent data demonstrating dysregulation of titin nanomechanics that can contribute to increased risk of heart failure in diabetic patients.