Events Calendar

 May 2025        
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Marcus DuPont, Spherical Bondi accretion in a binary black hole system (12:30 PM - 1:30 PM)

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Risa Wechsler, Unveiling the nature of dark matter with small-scale cosmic structure (2:00 PM - 3:15 PM)

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Joan La Madrid, Comments on Gravity (4:00 PM - 5:30 PM)

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Calvin Chen, The Power of Precision Astrometry (10:00 AM - 11:30 AM)

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, HEP Journal Club (12:30 PM - 1:30 PM)

Harikrishnan Ramani, Improving prospects for the direct detection of Higgsino dark matter (2:00 PM - 3:15 PM)

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1
Lyman Page, A New Experiment to Search for QCD Axions as Dark Matter (12:30 PM - 1:30 PM)

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Lyman Page, Exploring the Birth of the Universe with the CMB (4:00 PM - 5:30 PM)

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Calkins (3:30 PM - 4:30 PM)

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Wenzer Qin, A new way to form supermassive black holes (12:30 PM - 1:30 PM)

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Tetyana Pitik, Accretion-Induced Collapse of White Dwarfs: A Pathway to Gamma-Ray Bursts and Heavy Element Nucleosynthesis (2:00 PM - 3:15 PM)

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, HEP Journal Club (12:30 PM - 1:30 PM)

Howie Haber, RG-stable parameter relations of a scalar field theory in absence of a symmetry (2:00 PM - 3:15 PM)

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Vladimir Rosenhaus, Renormalization Group in wave turbulence (11:10 AM - 12:30 PM)

-- Abstract: *HOSTED BY COURANT - OF POTENTIAL INTEREST TO CCPP* Renormalization Group (RG) is a powerful concept -- one calculates partition functions by successively integrating out short distance degrees of freedom, until one has an effective Hamiltonian describing only large scale modes. The most famous application is Wilson's use of RG to calculate the critical scaling exponents at the water-vapor phase transition. We apply RG concepts to a vastly different class of states, which are far from equilibrium. It is known that a large class of weakly interacting nonlinear systems have states that are spatially homogeneous, time-independent, and scale invariant. Such states, in which mode k has occupation number $n_k = k^{-gamma}$, go under the name of Kolmogorov-Zakharov states in wave turbulence. Canonical examples are waves on the surface of the ocean, or waves in the nonlinear Schrodinger equation. We compute one loop beta functions in such states, which encode how the effective coupling changes with scale. The beta functions tells us if the spectrum of occupation numbers is steeper or less steep than Kolmogorov-Zakharov scaling. Depending on the sign of the beta function, nonlinear effects may either cause a minor shift of the state in the IR, or completely change the nature of the state. Focusing on nearly marginal interactions (ones in which the strength of the nonlinearity is weakly scale dependent), we construct an analog of Wilson's epsilon expansion and IR fixed points, with epsilon now set by the scaling of the interaction rather than the spacetime dimension. In the language of RG flow, critical balance scaling -- having applications in fields as varied as astrophysics and ocean waves -- corresponds to the state dynamically adjusting itself along the RG flow until the interaction becomes marginal.

Calkins (3:30 PM - 4:30 PM)

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Sebastian Ellis, Classical and Quantum Detection of Gravitational Waves (11:00 AM - 12:15 PM)

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, HEP Journal Club (12:30 PM - 1:30 PM)

Zach Weiner, Searching for coupled, hyperlight scalars across cosmic history (4:00 PM - 4:30 PM)

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Soichiro Shimamori, Boundary Scattering and Non-invertible Symmetries in 1+1 Dimensions (1:00 PM - 2:00 PM)

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Louis Hamaide, New insights into optomechanical detection of ultralight dark matter (2:00 PM - 3:00 PM)

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, Binary Accretion Discussion (11:00 AM - 12:30 PM)

Sebastian Cespedes, Causality Bounds on the Primordial Power Spectrum (2:00 PM - 3:15 PM)

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