Thu, 02 Aug 2018

11:00 - 12:00
C6

Turbulence models and convergence rates

James Glimm
(Stony Brook University)
Abstract

We discuss three methods for the simulation of turbulent fluids. The issue we address is not the important issue of numerical algorithms, but the even more basic question of the equations to be solved, otherwise known as the turbulence model.  These equations are not simply the Navier-Stokes equations, but have extra, turbulence related terms, related to turbulent viscosity, turbulent diffusion and turbulent thermal conductivity. The extra terms are not “standard textbook” physics, but are hypothesized based on physical reasoning. Here we are concerned with these extra terms.

The many models, divided into broad classes, differ greatly in

Dependence on data
Complexity
Purpose and usage

For this reason, each of the classes of models has its own rationale and domain of usage.

We survey the landscape of turbulence models.

Given a turbulence model, we ask: what is the nature of convergence that a numerical algorithm should strive for? The answer to this question lies in an existence theory for the Euler equation based on the Kolmogorov 1941 turbulent scaling law, taken as a hypothesis (joint work with G-Q Chen).

Wed, 01 Aug 2018

12:00 - 13:00
C6

Bressan’s Conjecture on compactness of flow for BV vector fields

Stefano Bianchini
(SISSA-ISAS)
Abstract

When studying a systems of conservation laws in several space dimensions, A. Bressan conjectured that the flows $X^n(t)$ generated by a smooth vector fields $\mathbf b^n(t,x)$,
\[
\frac{d}{dt} X^n(t,y) = \mathbf b^n(t,X(t,y)),
\]
are compact in $L^1(I\!\!R^d)$ for all $t \in [0,T]$ if $\mathbf b^n \in L^\infty \cap \mathrm{BV}((0,t) \times I\!\!R^d)$ and they are nearly incompressible, i.e.
\[
\frac{1}{C} \leq \det(\nabla_y X(t,y)) \leq C
\]
for some constant $C$. This conjecture is implied by the uniqueness of the solution to the linear transport equation
\[
\partial_t \rho + \mathrm{div}_x(\rho \mathbf b) = 0, \quad \rho \in L^\infty((0,T) \times I\!\!R^d),
\]
and it is the natural extension of a series of results concerning vector fields $\mathbf b(t,x)$ with Sobolev regularity.

We will give a general framework to approach the uniqueness problem for the linear transport equation and to prove Bressan's conjecture.

Mon, 23 Jul 2018

14:00 - 16:00
L6

Shock Refection Problem: Existence and Uniqueness of Solutions

Mikhail Feldman
(University of Wisconsin)
Abstract

We discuss shock reflection problem for compressible gas dynamics, von Neumann conjectures on transition between regular and Mach reflections. Then we describe recent results on existence and uniqueness of regular reflection solutions for potential flow equation, and discuss some techniques involved in the proof. The approach is to reduce the shock reflection problem to a free boundary problem, and prove existence and uniqueness by a version of method of continuity. This involves apriori estimates of solutions in the elliptic region of the equation of mixed type, with ellipticity degenerating on some part of the boundary. For the proof of uniqueness, an important property of solutions is convexity of the free boundary. We will also discuss some open problems.

This talk is based on joint works with G.-Q. Chen and W. Xiang.

 

Tue, 13 Nov 2018

14:15 - 15:30
L4

Even Artin groups of FC-type are polyfree.

Conchita Martinez-Perez
(Universidad de Zaragoza)
Abstract

Polyfree groups are defined as groups having a series of normal
subgroups such that each sucessive quotient is free. This property
imples locally indicability and therefore also right orderability. Right
angled Artin groups are known to be polyfree (a result shown
independently by Duchamp-Krob, Howie and Hermiller-Sunic). Here we show
that Artin FC-groups for which all the defining relation are of even
type  are also polyfree. This is a joint work with Ruven Blasco and Luis
Paris.

Differential limit on the extremely-high-energy cosmic neutrino flux in the presence of astrophysical background from nine years of IceCube data
Aartsen, M Ackermann, M Adams, J Aguilar, J Ahlers, M Ahrens, M Al Samarai, I Altmann, D Andeen, K Anderson, T Ansseau, I Anton, G Argueelles, C Auffenberg, J Axani, S Backes, P Bagherpour, H Bai, X Barbano, A Barron, J Barwick, S Baum, V Bay, R Beatty, J Tjus, J Becker, K BenZvi, S Berley, D Bernardini, E Besson, D Binder, G Bindig, D Blaufuss, E Blot, S Bohm, C Borner, M Bos, F Boeser, S Botner, O Bourbeau, E Bourbeau, J Bradascio, F Braun, J Brenzke, M Bretz, H Bron, S Brostean-Kaiser, J Burgman, A Busse, R Carver, T Cheung, E Chirkin, D Christov, A Clark, K Classen, L Collin, G Conrad, J Coppin, P Correa, P Cowen, D Cross, R Dave, P Day, M de Andre, J De Clercq, C DeLaunay, J Dembinski, H Deoskar, K De Ridder, S Desiati, P de Vries, K de Wasseige, G de With, M DeYoung, T Diaz-Velez, J di Lorenzo, V Dujmovic, H Dumm, J Dunkman, M Dvorak, E Eberhardt, B Ehrhardt, T Eichmann, B Eller, P Evenson, P Fahey, S Fazely, A Felde, J Filimonov, K Finley, C Flis, S Franckowiak, A Friedman, E Fritz, A Gaisser, T Gallagher, J Ganster, E Gerhardt, L Ghorbani, K Giang, W Glauch, T Gluesenkamp, 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 Huennefeld, 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 Koepke, L Kopper, C Kopper, S Koschinsky, J Koskinen, D Kowalski, M Krings, K Kroll, M Kruckl, 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 Luenemann, J Luszczak, W Madsen, J Maggi, G Mahn, K Makino, Y Mancina, S Maris, I Maruyama, R Mase, K Maunu, R Meagher, K Medici, M Meier, M Menne, T Merino, G Meures, T Miarecki, S Micallef, J Momente, 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 Pepper, J de Los Heros, C Pieloth, D Pinat, E Pizzuto, A Plum, M Price, P Przybylski, G Raab, C Radel, L 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 Schoenen, S Schoeneberg, 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 Stossl, A Strotjohann, N Stuttard, T Sullivan, G Sutherland, M Taboada, I Tenholt, F Ter-Antonyan, S Terliuk, A Tilav, S Toale, P Tobin, M Tonnis, C Toscano, S Tosi, D Tselengidou, M Tung, C Turcati, A Turley, C Ty, B Unger, E Usner, M Vandenbroucke, J Van Driessche, W van Eijk, D van Eijndhoven, N Vanheule, S van Santen, J Vraeghe, M Walck, C Wallace, A Wallraff, M Wandler, F Wandkowsky, N Watson, T Waza, A Weaver, C Weiss, M Wendt, C Werthebach, J Westerhoff, S Whelan, B Whitehorn, N Wiebe, K Wiebusch, C Wille, L Williams, D Wills, L Wolf, M Wood, J Wood, T Woolsey, E Woschnagg, K Wrede, G Xu, D Xu, X Xu, Y Yanez, J Yodh, G Yoshida, S Yuan, T Collaboration, I PHYSICAL REVIEW D volume 98 issue 6 (12 Sep 2018) http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000444572700001&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=4fd6f7d59a501f9b8bac2be37914c43e
Fri, 27 Jul 2018

16:30 - 17:15
L6

How did Chinese deal with a scientific problem: Building the solar eclipse theory in ancient China (the 7th-10th century AD)

Anjing Qu
(Xi'an)
Abstract

In the 6th century, the phenomena of irregularity of the solar motion and parallax of the moon were found by Chinese astronomers. This made the calculation of solar eclipse much more complex than before. The strategy that Chinese calendar-makers dealt with was different from the geometrical model system like Greek astronomers taken as. What Chinese astronomers chose is a numerical algorithm system which was widely taken as a thinking mode to construct the theory of mathematical astronomy in old China. 

Fri, 27 Jul 2018

16:00 - 16:30
L6

William Burnside and the Mystery Letter

Howard Emmens
Abstract

Relatively little is known about the correspondence of William Burnside, a pioneer of group theory in the UK. There are only a few dozen extant letters from or to him, though they are not without interest. However, one of the most noteworthy letters to or at least about him, in that it had a special mention in his obituary in the Proceedings of the Royal Society, has not been positively identified. It's not clear who it was from or when it was sent. We'll look at some possibilities.

Fri, 27 Jul 2018

15:00 - 15:30
L6

Meeting under the integral sign? The 1936 Oslo International Congress of Mathematicians

Christopher Hollings
(Oxford)
Abstract

The International Congresses of Mathematicians (ICMs) have taken place at (reasonably) regular intervals since 1897, and although their participants may have wanted to confine these events purely to mathematics, they could not help but be affected by wider world events.  This is particularly true of the 1936 ICM, held in Oslo.  In this talk, I will give a whistle-stop tour of the early ICMs, before discussing the circumstances of the Oslo meeting, with a particular focus on the activities of the Nazi-led German delegation.

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