Modjaz Group Mtg (2:00 PM - 3:30 PM)

Soubhik Kumar, Primordial Non-Gaussianity as a probe of (ultra high-energy) gauge theories (2:30 PM - 3:30 PM)

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Maria Okounkova, Binary black holes beyond general relativity (2:00 PM - 3:15 PM)

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SPS Room Hold (6:30 PM - 8:30 PM)

Bryan Ostdiek, Machine learning the Milky Way Halo with Gaia: Evidence for a new stellar stream in the solar vicinity (2:00 PM - 3:30 PM)

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Astroparticle Group Mtg (3:30 PM - 5:00 PM)

Dmitri Chklovskii, Reverse Engineering the Brain: A Physicist's Approach (4:00 PM - 5:00 PM)

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CQP UPS (11:00 AM - 12:30 PM)

NYU-CCA (1:00 PM - 2:30 PM)

Pablo Quílez, On the Peccei-Quinn quality problem (1:30 PM - 3:00 PM)

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Modjaz Group Mtg (2:00 PM - 3:30 PM)

Townhall practice (5:00 PM - 6:00 PM)

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Jack Setford, Signatures of Mirror Stars (2:00 PM - 3:30 PM)

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Astroparticle Group Mtg (3:30 PM - 5:00 PM)

David Poland, Critical Phenomena and the Conformal Bootstrap (4:00 PM - 5:00 PM)

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Town Hall (12:00 PM - 2:00 PM)

Andrea Caputo, Looking for Axion Dark Matter: from Dwarf Galaxies to Pulsars (2:00 PM - 3:00 PM)

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Juan Maldacena, Black holes, entropy and quantum information (2:00 PM - 3:30 PM)

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Astroparticle Group Mtg (3:30 PM - 5:00 PM)

Joshua Ruderman, undergrad quantum midterm review (6:30 PM - 11:59 PM)

Mark Van Raamsdonk, Gravity and Entanglement (4:00 PM - 5:00 PM)

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NYU-CCA (1:00 PM - 2:30 PM)

Alexander Vilenkin, Flyover vacuum decay (1:30 PM - 3:00 PM)

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Shengqi Yang, Line Intensity Mapping (12:30 PM - 2:00 PM)

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Modjaz Group Mtg (2:00 PM - 3:30 PM)

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Gopolang Mohlabeng, Inelastic dark matter revives the dark photon explanation of the muon g-2 anomaly (2:00 PM - 3:30 PM)

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Astroparticle Group Mtg (3:30 PM - 5:00 PM)

Josh Ruderman, Knowns and Unknowns in Particle Physics (4:00 PM - 5:00 PM)

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Modjaz Group Mtg (2:00 PM - 3:30 PM)

-- Abstract: The flow of gas into and out of galaxies regulates their evolution over cosmic time. The dynamics of these multiphase flows are sensitive to the small scale processes that mediate the mixing of the hot and cold phases. I will highlight two examples where this is mixing is acutely important: (i) the launching of galactic winds by supernova powered superbubbles, and (ii) the balance of turbulent heating and radiative cooling that determines galactic accretion. Then, based on a suite of high resolution simulations, I will present a new model founded on the fractal nature of radiative turbulent mixing layers that can fully characterize the physical processes that control the multiphase mixing.

Tim Linden, Using Neutron Stars to Probe Fundamental Physics (2:00 PM - 3:30 PM)

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Astroparticle Group Mtg (3:30 PM - 5:00 PM)

Ian Dobbs-Dixon, Modelling Atmospheres of Short Period Gas Planets (4:00 PM - 5:00 PM)

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NYU-CCA (1:00 PM - 2:30 PM)