Events Calendar

 May 2023        
MondayTuesdayWednesdayThursdayFriday
1
Xuyao Hu, The Sachdev-Ye-Kitaev model and turbulence (12:30 PM - 1:30 PM)

, Grad Pheno Journal Club (2:00 PM - 3:00 PM)

2
Austin McDowell, Constraining GRB Properties with Afterglow Light Curves (10:30 AM - 12:00 PM)

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

(2:00 PM - 3:15 PM)

3
, HEP Journal Club (12:30 PM - 1:30 PM)

Linda Xu, The continuum and the line: new analyses of Fermi gamma-ray data (2:00 PM - 3:00 PM)

+ Abstract:

4
, Equity & Inclusion Committee (12:30 PM - 2:00 PM)

Dave Thirumalai, Collective Movement in cells - From jamming to superdiffusion (4:00 PM - 5:15 PM)

5
Nicolas Boulanger, New higher-spin topological systems in 3D (2:00 PM - 3:15 PM)

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Zare (3:30 PM - 5:30 PM)

8
Francis Bernardeau, Nulling properties of tomographic cosmic shear observations (2:00 PM - 3:15 PM)

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9
Michael Unger, New Models of the Magnetic Field of the Galaxy (2:00 PM - 3:00 PM)

-- Abstract: Galaxies are known to be permeated by large-scale magnetic fields with energy densities comparable to the turbulent and thermal energy densities of the interstellar mediums. A good knowledge of the global structure of these fields is important to understand their origin and to infer their effect on galactic dynamics and the propagation of charged particles in galaxies. In this talk I will present new studies of the global structure of the magnetic field of our Galaxy based on the analysis of recent new full-sky data of extragalactic rotation measures and the final polarized intensity maps from WMAP and Planck. Our analysis employs the latest models for the thermal electron density tuned to the dispersion measures of Galactic pulsars and state-of-the-art cosmic-ray electrons models, needed to predict the rotation measures and synchrotron emission from the Galaxy, respectively. We have developed new divergence-free parametric models of the global structure of the magnetic field, with parameters tuned to the data. As a result, I will present a major revision of the widely-used Jannson-Farrar 2012 model of the magnetic field of the Galaxy. In addition to our fiducial magnetic field model, we produced a suite of alternative models that fit the data with similar quality, but use different model assumption. This suite of models is then used to place a lower limit on the model uncertainties. As an application, we will discuss the uncertainties of the predicted deflection of the predicted deflection of ultrahigh-energy cosmic rays in the Galaxy.

10
Dam Thanh Son, Bosonization of Fermi surfaces and coadjoint orbits (2:00 PM - 3:00 PM)

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11
, Equity & Inclusion Committee (12:30 PM - 2:00 PM)

Yue Hu, Characterizing 3D Galactic Magnetic Fields with Anisotropic MHD turbulence (12:30 PM - 1:00 PM)

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12
Benedikt Schosser, 21cm Parameter Inference (11:00 AM - 11:45 AM)

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Burt Ovrut, Realistic Heterotic Vacua, Inflation and FIMP Dark Matter (2:00 PM - 3:15 PM)

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Zare (3:30 PM - 5:30 PM)

15
Xingyang Yu, Dualities and Symmetries of Quantum Field Theories from Brane Engineering (2:00 PM - 4:00 PM)

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16
17
Laurent Baulieu, Gravitons, BRST-BMS4 Symmetry and its Cocycles from Horizontality Conditions (1:00 PM - 2:15 PM)

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18
19
Zare (3:30 PM - 5:30 PM)

22
23
Zihui Wang, New topics in quantum chromodynamics and astro-particle probes of dark matter (10:00 AM - 12:00 PM)

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24
25
Xingchen Xu, Non-perturbative Interactions Between Dark Matter and Baryons: Scattering, Capture, and Experimental Constraints (9:00 AM - 11:00 AM)

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John Davis, Observations spanning multiple astronomical scales point to the existence of an unknown form of matter (11:00 AM - 12:15 PM)

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Zare (2:00 PM - 4:00 PM)

Ben Wandelt, AI-Driven Discoveries at the Frontiers of Cosmology (4:00 PM - 5:15 PM)

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26
29
30
31
Kate Storey-Fisher, Tools for Large-Scale Structure and Galaxy Formation (12:30 PM - 2:00 PM)

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