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Fri, 24 Nov 2023
12:00
L3

Thermodynamics of Near Extremal Black Holes in AdS(5)

Finn Larsen
(Michigan)
Abstract
The phase diagram of near extremal black holes is surprisingly rich.  In some regimes quantum effects are so strong that they dominate. On the supersymmetric locus there is a large ground state degeneracy protected by a gap. Throughout, there is an intricate classical interplay between charge and rotation. The talk reviews some of the physical mechanisms and highlights some unresolved tensions between claims in the literature. 
 
Fri, 17 Nov 2023
17:30
Zoom

Twistor Particle Programme Rebooted: A "zig-z̄ag" Theory of Massive Spinning Particles

Joonhwi Kim
(Caltech)

Note: we would recommend to join the meeting using the Zoom client for best user experience.

Abstract

Recently, the Newman-Janis shift has been revisited from the angle of scattering amplitudes in terms of the so-called "massive spinor-helicity variables," tracing back to Penrose and Perjés in the 70s. However, well-established results are limited in the same-helicity (self-dual) sector, while a puzzle of spurious poles arises in mixed-helicity sectors. This talk will outline how massive twistor theory can reproduce the same-helicity results while offering a possible solution to the spurious pole puzzle. Firstly, the Newman-Janis shift in the same-helicity sector is derived from a complexified version of the equivalence principle. Secondly, the massive twistor particle is coupled to background fields from bottom-up and top-down perspectives. The former is based on perturbations of symplectic structures in massive twistor space. The latter provides a generalization of Newman-Janis shift in generic backgrounds, which also leads to "curved massive twistor space" and its deformed massive incidence relation. Lastly, the Feynman rules of the first-quantized massive twistor particle and their physical interpretation are briefly discussed. Overall, a significant emphasis is put on the Kähler geometry ("zig-z̄ag structure") of massive twistor space, which eventually connects to a worldsheet structure of the Kerr solution.

 

Search for Extended Sources of Neutrino Emission in the Galactic Plane with IceCube
Abbasi, R Ackermann, M Adams, J Agarwalla, S Aguilar, J Ahlers, M Alameddine, J Amin, N Andeen, K Anton, G Argüelles, C Ashida, Y Athanasiadou, S Axani, S Bai, X Balagopal, A Baricevic, M Barwick, S Basu, V Bay, R Beatty, J Tjus, J Beise, J Bellenghi, C Benning, C BenZvi, S Berley, D Bernardini, E Besson, D Blaufuss, E Blot, S Bontempo, F Book, J Meneguolo, C Böser, S Botner, O Böttcher, J Bourbeau, E Braun, J Brinson, B Brostean-Kaiser, J Burley, R Busse, R Butterfield, D Campana, M Carloni, K Carnie-Bronca, E Chattopadhyay, S Chau, N Chen, C Chen, Z Chirkin, D Choi, S Clark, B Classen, L Coleman, A Collin, G Connolly, A Conrad, J Coppin, P Correa, P Cowen, D Dave, P De Clercq, C DeLaunay, J Delgado, D Deng, S Deoskar, K Desai, A Desiati, P de Vries, K de Wasseige, G DeYoung, T Diaz, A Díaz-Vélez, J Dittmer, M Domi, A Dujmovic, H DuVernois, M Ehrhardt, T Eller, P Ellinger, E Mentawi, S Elsässer, D Engel, R Erpenbeck, H Evans, J Evenson, P Fan, K Fang, K Farrag, K Fazely, A Fedynitch, A Feigl, N Fiedlschuster, S Finley, C Fischer, L Fox, D Franckowiak, A Fritz, A Fürst, P Gallagher, J Ganster, E Garcia, A Gerhardt, L Ghadimi, A Glaser, C Glauch, T Glüsenkamp, T Goehlke, N Gonzalez, J Goswami, S Grant, D Gray, S Gries, O Griffin, S Griswold, S Groth, K Günther, C Gutjahr, P Haack, C Hallgren, A Halliday, R Halve, L Halzen, F Hamdaoui, H Minh, M Hanson, K Hardin, J Harnisch, A Hatch, P Haungs, A Helbing, K Hellrung, J Henningsen, F Heuermann, L Heyer, N Hickford, S Hidvegi, A Hill, C Hill, G Hoffman, K Hori, S Hoshina, K Hou, W Huber, T Hultqvist, K Hünnefeld, M Hussain, R Hymon, K In, S Ishihara, A Jacquart, M Janik, O Jansson, M Japaridze, G Jeong, M Jin, M Jones, B Kang, D Kang, W Kang, X Kappes, A Kappesser, D Kardum, L Karg, T Karl, M Karle, A Katz, U Kauer, M Kelley, J Zathul, A Kheirandish, A Kiryluk, J Klein, S Kochocki, A Koirala, R Kolanoski, H Kontrimas, T Köpke, L Kopper, C Koskinen, D Koundal, P Kovacevich, M Kowalski, M Kozynets, T Krishnamoorthi, J Kruiswijk, K Krupczak, E Kumar, A Kun, E Kurahashi, N Lad, N Gualda, C Lamoureux, M Larson, M Latseva, S Lauber, F Lazar, J Lee, J DeHolton, K Leszczyńska, A Lincetto, M Liu, Q Liubarska, M Lohfink, E Love, C Mariscal, C Lu, L Lucarelli, F Luszczak, W Lyu, Y Madsen, J Mahn, K Makino, Y Manao, E Mancina, S Sainte, W Mariş, I Marka, S Marka, Z Marsee, M Martinez-Soler, I Maruyama, R Mayhew, F McElroy, T McNally, F Mead, J Meagher, K Mechbal, S Medina, A Meier, M Merckx, Y Merten, L Micallef, J Mitchell, J Montaruli, T Moore, R Morii, Y Morse, R Moulai, M Mukherjee, T Naab, R Nagai, R Nakos, M Naumann, U Necker, J Negi, A Neumann, M Niederhausen, H Nisa, M Noell, A Novikov, A Nowicki, S Pollmann, A O’Dell, V Oehler, M Oeyen, B Olivas, A Orsoe, R Osborn, J O’Sullivan, E Pandya, H Park, N Parker, G Paudel, E Paul, L de los Heros, C Peterson, J Philippen, S Pizzuto, A Plum, M Pontén, A Popovych, Y Rodriguez, M Pries, B Procter-Murphy, R Przybylski, G Raab, C Rack-Helleis, J Rawlins, K Rechav, Z Rehman, A Reichherzer, P Renzi, G Resconi, E Reusch, S Rhode, W Riedel, B Rifaie, A Roberts, E Robertson, S Rodan, S Roellinghoff, G Rongen, M Rott, C Ruhe, T Ruohan, L Ryckbosch, D Rysewyk, D Safa, I Saffer, J Salazar-Gallegos, D Sampathkumar, P Herrera, S Sandrock, A Santander, M Sarkar, S Savelberg, J Savina, P Schaufel, M Schieler, H Schindler, S Schlickmann, L Schlüter, B Schlüter, F Schmeisser, N Schmidt, T Schneider, J Schröder, F Schumacher, L Schwefer, G Sclafani, S Seckel, D Seikh, M Seunarine, S Shah, R Sharma, A Shefali, S Shimizu, N Silva, M Skrzypek, B Smithers, B Snihur, R Soedingrekso, J Søgaard, A Soldin, D Soldin, P Sommani, G Spannfellner, C Spiczak, G Spiering, C Stamatikos, M Stanev, T Stezelberger, T Stürwald, T Stuttard, T Sullivan, G Taboada, I Ter-Antonyan, S Thiesmeyer, M Thompson, W Thwaites, J Tilav, S Tollefson, K Tönnis, C Toscano, S Tosi, D Trettin, A Tung, C Turcotte, R Twagirayezu, J Ty, B Elorrieta, M Upadhyay, A Upshaw, K Valtonen-Mattila, N Vandenbroucke, J van Eijndhoven, N Vannerom, D van Santen, J Vara, J Veitch-Michaelis, J Venugopal, M Vereecken, M Verpoest, S Veske, D Vijai, A Walck, C Weaver, C Weigel, P Weindl, A Weldert, J Wendt, C Werthebach, J Weyrauch, M Whitehorn, N Wiebusch, C Willey, N Williams, D Wolf, A Wolf, M Wrede, G Xu, X Yanez, J Yildizci, E Yoshida, S Young, R Yu, F Yu, S Yuan, T Zhang, Z Zhelnin, P Zimmerman, M Collaboration, I The Astrophysical Journal volume 956 issue 1 20 (01 Oct 2023)

This track is taken from the album There's a Riot Goin' On, where Sly Stone moved away from the upbeat soul of the sixties and filled the sound with a downbeat, hazy instrumentation and vocal. Apparently he wasn't feeling great at the time. Critics think it is great though. Such is art.

A central limit theorem for the number of excursion set components of gaussian fields
Belyaev, D Annals of Probability volume 52 issue 3 882-922 (23 Apr 2024)
Tue, 21 Nov 2023
11:00
L1

Singularity Detection from a Data "Manifold"

Uzu Lim
(Mathematical Institute)

Note: we would recommend to join the meeting using the Teams client for best user experience.

Abstract

High-dimensional data is often assumed to be distributed near a smooth manifold. But should we really believe that? In this talk I will introduce HADES, an algorithm that quickly detects singularities where the data distribution fails to be a manifold.

By using hypothesis testing, rather than persistent homology, HADES achieves great speed and a strong statistical foundation. We also have a precise mathematical theorem for correctness, proven using optimal transport theory and differential geometry. In computational experiments, HADES recovers singularities in synthetic data, road networks, molecular conformation space, and images.

Paper link: https://arxiv.org/abs/2311.04171
Github link: https://github.com/uzulim/hades
 

Tue, 27 Feb 2024

14:00 - 15:00
L5

Modular Reduction of Nilpotent Orbits

Jay Taylor
(University of Manchester)
Abstract

Suppose 𝐺𝕜 is a connected reductive algebraic 𝕜-group where 𝕜 is an algebraically closed field. If 𝑉𝕜 is a 𝐺𝕜-module then, using geometric invariant theory, Kempf has defined the nullcone 𝒩(𝑉𝕜) of 𝑉𝕜. For the Lie algebra 𝔤𝕜 = Lie(𝐺𝕜), viewed as a 𝐺𝕜-module via the adjoint action, we have 𝒩(𝔤𝕜) is precisely the set of nilpotent elements.

We may assume that our group 𝐺𝕜 = 𝐺 × 𝕜 is obtained by base-change from a suitable ℤ-form 𝐺. Suppose 𝑉 is 𝔤 = Lie(G) or its dual 𝔤* = Hom(𝔤, ℤ) which are both modules for 𝐺, that are free of finite rank as ℤ-modules. Then 𝑉 ⨂ 𝕜, as a module for 𝐺𝕜, is 𝔤𝕜 or 𝔤𝕜* respectively.

It is known that each 𝐺 -orbit 𝒪 ⊆ 𝒩(𝑉) contains a representative ξ ∈ 𝑉 in the ℤ-form. Reducing ξ one gets an element ξ𝕜 ∈ 𝑉𝕜 for any algebraically closed 𝕜. In this talk, we will explain two ways in which we might want ξ to have “good reduction” and how one can find elements with these properties. We will also discuss the relationship to Lusztig’s special orbits.

This is on-going joint work with Adam Thomas (Warwick).

Tue, 05 Mar 2024

14:00 - 15:00
L5

Complex crystallographic groups and Seiberg--Witten integrable systems

Oleg Chalykh
(University of Leeds)
Abstract

For any smooth complex variety Y with an action of a finite group W, Etingof defines the global Cherednik algebra H_c and its spherical subalgebra B_c as certain sheaves of algebras over Y/W. When Y is an n-dimensional abelian variety, the algebra of global sections of B_c is a polynomial algebra on n generators, as shown by Etingof, Felder, Ma, and Veselov. This defines an integrable system on Y. In the case of Y being a product of n copies of an elliptic curve E and W=S_n, this reproduces the usual elliptic Calogero­­--Moser system. Recently, together with P. Argyres and Y. Lu, we proposed that many of these integrable systems at the classical level can be interpreted as Seiberg­­--Witten integrable systems of certain super­symmetric quantum field theories. I will describe our progress in understanding this connection for groups W=G(m, 1, n), corresponding to the case Y=E^n where E is an elliptic curves with Z_m symmetry, m=2,3,4,6. 

A mathematical framework for the emergence of winners and losers in cell competition.
Pak, T Pitt-Francis, J Baker, R Journal of theoretical biology volume 577 111666-111666 (11 Nov 2023)
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