| December 2023 |
| Monday | Tuesday | Wednesday | Thursday | Friday |
| 27 (12:30 PM - 1:30 PM) Zare (2:00 PM - 4:00 PM) | 28 Burçin Mutlu-Pakdil, The Smallest and Faintest Galaxies: Clues to the Nature of Dark Matter and Galaxy Formation (2:00 PM - 3:15 PM) + Abstract: | 29 Asimina Arvanitaki, The Cosmic Neutrino Background (CνB): Its distribution on the surface of the Earth and its manipulation on laboratory scales (2:00 PM - 3:15 PM) + Abstract: | 30 Chiara Mingarelli, The NANOGrav Experiment: Current Results and Future Directions (3:00 PM - 4:30 PM) + Abstract: | 1 Popov, Postdoc HepTh Discussion Group (12:00 PM - 1:30 PM) James Sullivan, Galaxies Remember Inflation - New Aspects of Local Primordial non-Gaussianity in Galaxy Surveys (12:00 PM - 12:30 PM) + Abstract: |
| 4 David Hogg, Is the Milky Way disk two-dimensional? (12:30 PM - 1:30 PM) + Abstract: Zare (2:00 PM - 4:00 PM) Jonathan Morag, Analytic Model of Shock Cooling Emission Fitting In Core-collapse SNe (2:00 PM - 2:45 PM) + Abstract: | 5 (11:00 AM - 12:30 PM) Luca Comisso, From Turbulence to Reconnection to Particle Acceleration: Connecting the Dots (2:00 PM) + Abstract: | 6 Carlos Wagner, The Muon g-2 puzzle (2:00 PM - 3:00 PM) + Abstract: , CCPP Pheno Journal Club (3:30 PM - 4:30 PM) | 7 William Jacobs, Rational Design of Multicomponent Biomolecular Condensates (4:00 PM - 5:30 PM) + Abstract: | 8 Popov, Postdoc HepTh Discussion Group (12:00 PM - 1:30 PM) |
| 11 Michael Blanton, What the Sloan Digital Sky Survey V is up to (12:30 PM - 1:30 PM) + Abstract: | 12 | 13 LianTao Wang, Gravitational wave signals of early universe dynamics (2:00 PM - 3:00 PM) + Abstract: Jacopo Salvalaggio, Modelling the covariance for the galaxy clustering bispectrum (2:00 PM - 3:00 PM) -- Abstract: The galaxy clustering bispectrum, i.e. the Fourier transform of the 3-point correlation function of the galaxy density field, contains a large amount of information on the cosmology and can be used to greatly improve the constraints obtained from the 2-point function alone. However, providing a covariance matrix for it can be a challenging task as a great amount of simulations are needed in order to accurately estimate it numerically. In the presentation I'm going to show my latest results towards an analytical understanding of the bispectrum covariance, accounting for non-linear and window effects. | 14 Jo Dunkley, Looking for cracks in the cosmological model (4:00 PM - 5:30 PM) + Abstract: | 15 Raphael Bousso, New Physics Near Black Holes (2:00 PM - 3:15 PM) + Abstract: , NYU Physics Holiday Party (3:00 PM - 5:00 PM) |
| 18 | 19 | 20 | 21 | 22 |
| 25 , University Closed for Winter Recess | 26 , University Closed for Winter Recess | 27 , University Closed for Winter Recess | 28 , University Closed for Winter Recess | 29 , University Closed for Winter Recess |