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The Weirdest Galaxies in the Universe

Dr. Julianne Dalcanton (Director, CCA, Flatiron Institute)

The Universe is filled with wonders, great and small.  In many cases, these wonders arise out of the order that the laws of physics imprint on the stars and galaxies that populate our universe.  But sometimes, this remarkable order is disturbed, producing truly outlandish departures from what astronomers consider to be “normal”.  In this talk, Dr. Dalcanton will highlight some of the weirdest galaxies in the universe, many of which are best revealed with the Hubble Space Telescope and its successors.

Register for the event

Conference sponsored by the Department of Philosophy and the Minnesota Center for Philosophy of Science. 215 Humphrey (Wilkins Room) and online, via Zoom. Registration required (deadline of October 17 applies only to conference dinner).

For more info, including zoom link, see the conference website.

Abstract:

Thermodynamics, a venerable physical theory from the 19th century,  is nowadays often regarded as just a limiting case of the various theories in statistical physics in the “thermodynamical limit”;  not as a physical theory on its own.  Nevertheless, there are arguments to take the approach of the 19th century founders of this theory  (Clausius, Kelvin, and Planck a.o.)  seriously even today as thermodynamics is being applied to more exotic objects like black holes. 

I will in this talk review the foundational assumptions of classical thermodynamics and problems and the disputes surrounding them until today.

Abstract: Astronomical transients are signposts of catastrophic events in space, including the most extreme stellar deaths, stellar tidal disruptions by supermassive black holes, and mergers of compact objects. Thanks to new and improved observational facilities we can now sample the night sky with unprecedented temporal cadence and sensitivity across the electromagnetic spectrum and beyond. This effort has led to the discovery of new types of astronomical transients, revolutionized our understanding of phenomena that we thought we already knew, and enabled the first insights into the physics of neutron star mergers with gravitational waves and light. In this talk I will review some very recent developments that resulted from our capability to acquire a truly panchromatic view of transient astrophysical phenomena. I will focus on two key areas of ignorance in the field: (i) What are the progenitors of stellar explosions and what happens in the last centuries before death? (ii) What is the nature of the compact objects produced by these explosions and what happens when compact objects merge? The unique combination of Discovery Power (guaranteed by planned transient surveys across the electromagnetic spectrum, combined with efforts in the realm of artificial intelligence) and Understanding (enabled by multi-messenger observations) is what positions time-domain astrophysics for major advances in the near future.

Abstract:  Quantum mechanics describes the physical world around us with exquisite precision, with no known violations of the theory. Ironically, this precision comes with some additional baggage: the theory permits the existence of a host of complex, delicate entangled states of the physical world, many of which have yet to be produced or observed. The debate of whether their quantum entanglement really captures the fundamental nature of the physical world and is an engineering resource is reaching a critical moment.  Quantum processors with of order 100 qubits based on superconducting circuitry have recently demonstrated computing power on par with the most advanced classical supercomputers for select problems. Current hardware is, however, prone to errors from materials defects, imperfect control systems, and the leakage of quantum information into unwanted modes in the solid-state. I will describe the major decoherence pathways present in state-of-the-art superconducting quantum processors, illustrate techniques to maximize the computing power of imperfect qubits, and highlight recent quantum computations for determining chemical energies, solutions to the transverse-field Ising model, scrambling dynamics in black holes, and nuclear scattering.

Irfan Siddiqi is the Director, Quantum Nanoelectronics Laboratory (QNL) U of CA, Berkeley

Abstract:  Three decades of surveying the sky have culminated in the celebrated cosmological standard model, yet 95% of the mass-energy of the Universe is still a mystery, residing in dark matter and dark energy. To address these mysteries, major cosmological surveys are ongoing and new ones will soon start. There are tremendous modeling and simulation challenges posed by these observations in order to enable the full interpretation of the associated cosmological measurements. In this talk I will discuss recent advances in large-scale simulations on the way to prepare for the arrival of the first exascale supercomputers. I will describe an ambitious end-to-end simulation project that attempts to provide a faithful view of the Universe as seen through the Rubin Observatory's Legacy Survey of Space and Time (LSST). This resulting synthetic sky provides many opportunities for exploring new ways to optimize the science return of LSST.