| 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: | 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: Information located in an entanglement island in semiclassical gravity can be nonperturbatively reconstructed from distant radiation, implying a radical breakdown of effective field theory. We show that this occurs well outside of the black hole stretched horizon. We compute the island associated to large angular momentum Hawking modes of a four-dimensional Schwarzschild black hole. These modes typically fall back into the black hole but can be extracted to infinity by relativistic strings or, more abstractly, by asymptotic boundary operators constructed using the timelike tube theorem. Remarkably, we find that their island can protrude a distance parametrically larger than the Planck scale and icomparable to the Bohr radius for supermassive black holes. Therefore, in principle, a distant observer can determine experimentally whether the black hole information paradox is resolved by complementarity, or by a firewall. , 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 |