All-Sky Measurement of the Anisotropy of Cosmic Rays at 10 TeV and
Mapping of the Local Interstellar Magnetic Field
 Collaboration, H Abeysekara, A Alfaro, R Alvarez, C Álvarez, J Arceo, R Arteaga-Velázquez, J Rojas, D Belmont-Moreno, E BenZvi, S Brisbois, C Capistrán, T Carramiñana, A Casanova, S Cotti, U Cotzomi, J Díaz-Vélez, J León, C Fuente, E Dichiara, S DuVernois, M Espinoza, C Fiorino, D Fleischhack, H Fraija, N Galván-Gámez, A García-González, J González, M Goodman, J Hampel-Arias, Z Harding, J Hernandez, S Hona, B Hueyotl-Zahuantitla, F Iriarte, A Jardin-Blicq, A Joshi, V Lara, A Vargas, H Luis-Raya, G Malone, K Marinelli, S Martínez-Castro, J Martinez, O Matthews, J Miranda-Romagnoli, P Moreno, E Mostafá, M Nellen, L Newbold, M Nisa, M Noriega-Papaqui, R Pérez-Pérez, E Pretz, J Ren, Z Rho, C Rivière, C Rosa-González, D Rosenberg, M Salazar, H Greus, F Sandoval, A Schneider, M Schoorlemmer, H Sinnis, G Smith, A Surajbali, P Taboada, I Tollefson, K Torres, I Villaseño, L Weisgarber, T Wood, J Zepeda, A Zhou, H Collaboration, I Aartsen, M Ackermann, M Adams, J Aguilar, J Ahlers, M Ahrens, M Altmann, D Andeen, K Anderson, T Ansseau, I Anton, G Argüelles, C Auffenberg, J Axani, S Backes, P Bagherpour, H Bai, X Barbano, A Barron, J Barwick, S Baum, V Bay, R Beatty, J Becker, K Tjus, J Berley, D Bernardini, E Besson, D Binder, G Bindig, D Blaufuss, E Blot, S Bohm, C Börner, M Bos, F Böser, S Botner, O Bourbeau, E Bourbeau, J Bradascio, F Braun, J Bretz, H Bron, S Brostean-Kaiser, J Burgman, A Busse, R Carver, T Chen, C Cheung, E Chirkin, D Clark, K Classen, L Collin, G Conrad, J Coppin, P Correa, P Cowen, D Cross, R Dave, P Day, M André, J Clercq, C DeLaunay, J Dembinski, H Deoskar, K Ridder, S Desiati, P Vries, K Wasseige, G With, M DeYoung, T Dujmovic, H Dunkman, M Dvorak, E Eberhardt, B Ehrhardt, T Eichmann, B Eller, P Evenson, P Fahey, S Fazely, A Felde, J Filimonov, K Finley, C Franckowiak, A Friedman, E Fritz, A Gaisser, T Gallagher, J Ganster, E Garrappa, S Gerhardt, L Ghorbani, K Giang, W Glauch, T Glüsenkamp, T Goldschmidt, A Gonzalez, J Grant, D Griffith, Z Haack, C Hallgren, A Halve, L Halzen, F Hanson, K Hebecker, D Heereman, D Helbing, K Hellauer, R Hickford, S Hignight, J Hill, G Hoffman, K Hoffmann, R Hoinka, T Hokanson-Fasig, B Hoshina, K Huang, F Huber, M Hultqvist, K Hünnefeld, M Hussain, R In, S Iovine, N Ishihara, A Jacobi, E Japaridze, G Jeong, M Jero, K Jones, B Kalaczynski, P Kang, W Kappes, A Kappesser, D Karg, T Karle, A Katz, U Kauer, M Keivani, A Kelley, J Kheirandish, A Kim, J Kintscher, T Kiryluk, J Kittler, T Klein, S Koirala, R Kolanoski, H Köpke, L Kopper, C Kopper, S Koskinen, D Kowalski, M Krings, K Kroll, M Krückl, G Kunwar, S Kurahashi, N Kyriacou, A Labare, M Lanfranchi, J Larson, M Lauber, F Leonard, K Leuermann, M Liu, Q Lohfink, E Mariscal, C Lu, L Lünemann, J Luszczak, W Madsen, J Maggi, G Mahn, K Makino, Y Mancina, S Mariş, I Maruyama, R Mase, K Maunu, R Meagher, K Medici, M Medina, A Meier, M Menne, T Merino, G Meures, T Miarecki, S Micallef, J Momenté, G Montaruli, T Moore, R Moulai, M Nagai, R Nahnhauer, R Nakarmi, P Naumann, U Neer, G Niederhausen, H Nowicki, S Nygren, D Pollmann, A Olivas, A O'Murchadha, A O'Sullivan, E Palczewski, T Pandya, H Pankova, D Peiffer, P Heros, C Pieloth, D Pinat, E Pizzuto, A Plum, M Price, P Przybylski, G Raab, C Raissi, A Rameez, M Rauch, L Rawlins, K Rea, I Reimann, R Relethford, B Renzi, G Resconi, E Rhode, W Richman, M Robertson, S Rongen, M Rott, C Ruhe, T Ryckbosch, D Rysewyk, D Safa, I Herrera, S Sandrock, A Sandroos, J Santander, M Sarkar, S Satalecka, K Schaufel, M Schlunder, P Schmidt, T Schneider, A Schneider, J Schöneberg, S Schumacher, L Sclafani, S Seckel, D Seunarine, S Soedingrekso, J Soldin, D Song, M Spiczak, G Spiering, C Stachurska, J Stamatikos, M Stanev, T Stasik, A Stein, R Stettner, J Steuer, A Stezelberger, T Stokstad, R Stößl, A Strotjohann, N Stuttard, T Sullivan, G Sutherland, M Tenholt, F Ter-Antonyan, S Terliuk, A Tilav, S Tobin, M Tönnis, C Toscano, S Tosi, D Tselengidou, M Tung, C Turcati, A Turcotte, R Turley, C Ty, B Unger, E Elorrieta, M Usner, M Vandenbroucke, J Driessche, W Eijk, D Eijndhoven, N Vanheule, S Santen, J Vraeghe, M Walck, C Wallace, A Wallraff, M Wandkowsky, N Wandler, F Watson, T Weaver, C Weiss, M Weldert, J Wendt, C Werthebach, J Westerhoff, S Whelan, B Whitehorn, N Wiebe, K Wiebusch, C Wille, L Williams, D Wills, L Wolf, M Wood, T Woolsey, E Woschnagg, K Wrede, G Xu, D Xu, X Xu, Y Yanez, J Yodh, G Yoshida, S Yuan, T Astrophysical Journal volume 871 96-96 (24 Jan 2019) http://arxiv.org/abs/1812.05682v3

Multiple zeta values in deformation quantization

Oxford Mathematician Erik Panzer talks about his and colleagues' work on devising an algorithm to compute Kontsevich's star-product formula explicitly, solving a problem open for more than 20 years.

"The transition from classical mechanics to quantum mechanics is marked by the introduction of non-commutativity. For example, let us consider the case of a particle moving on the real line.

From commutative classical mechanics...

Functional calculus for operators

When mathematicians solve a differential equation, they are usually converting unbounded operators (such as differentiation) which are represented in the equation into bounded operators (such as integration) which represent the solutions.  It is rarely possible to give a solution explicitly, but general theory can often show whether a solution exists, whether it is unique, and what properties it has.  For this, one often needs to apply suitable (bounded) functions $f$ to unbounded operators $A$ and obtain bounded operators $f(A)$ with good properties.&

Automating "human-like" example-use in mathematics
 Pease, A Martin, U CEUR Workshop Proceedings volume 2261 6-15 (01 Jan 2018)

Constraining Nonequilibrium Physics

Statistical mechanics (or thermodynamics) is a way of understanding large systems of interacting objects, such as particles in fluids and gases, chemicals in solution, or people meandering through a crowded street. Large macroscopic systems require prohibitively large systems of equations, and so equilibrium thermodynamics gives us a way to average out all of these details and understand the typical behaviour of the large scale system.

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