Thu, 18 Oct 2018

13:00 - 14:00
L4

Dynamic clearing and contagion in an Eisenberg-Noe framework

Zachary Feinstein
((Washington University in St. Louis))
Abstract

We will consider an extension of the Eisenberg-Noe model of financial contagion to allow for time dynamics in both discrete and continuous time. Mathematical results on existence and uniqueness of firm wealths under discrete and continuous-time will be provided. The financial implications of time dynamics will be considered, with focus on how the dynamic clearing solutions differ from those of the static Eisenberg-Noe model.
 

Joint constraints on Galactic diffuse neutrino emission from ANTARES and
IceCube
Albert, A André, M Anghinolfi, M Ardid, M Aubert, J Aublin, J Avgitas, T Baret, B Barrios-Martí, J Basa, S Belhorma, B Bertin, V Biagi, S Bormuth, R Boumaaza, J Bourret, S Bouwhuis, M Brânzaş, H Bruijn, R Brunner, J Busto, J Capone, A Caramete, L Carr, J Celli, S Chabab, M Moursli, R Chiarusi, T Circella, M Coelho, J Coleiro, A Colomer, M Coniglione, R Costantini, H Coyle, P Creusot, A Díaz, A Deschamps, A Distefano, C Palma, I Domi, A Donzaud, C Dornic, D Drouhin, D Eberl, T Bojaddaini, I Khayati, N Elsässer, D Enzenhöfer, A Ettahiri, A Fassi, F Felis, I Fermani, P Ferrara, G Fusco, L Gay, P Glotin, H Grégoire, T Ruiz, R Graf, K Hallmann, S Haren, H Heijboer, A Hello, Y Hernández-Rey, J Hößl, J Hofestädt, J Illuminati, G James, C Jong, M Jongen, M Kadler, M Kalekin, O Katz, U Khan-Chowdhury, N Kouchner, A Kreter, M Kreykenbohm, I Kulikovskiy, V Lachaud, C Lahmann, R Lefèvre, D Leonora, E Levi, G Lotze, M Loucatos, S Marcelin, M Margiotta, A Marinelli, A Martínez-Mora, J Mele, R Melis, K Migliozzi, P Moussa, A Navas, S Nezri, E Nuñez, A Organokov, M Păvălaş, G Pellegrino, C Piattelli, P Popa, V Pradier, T Quinn, L Racca, C Randazzo, N Riccobene, G Sánchez-Losa, A Saldaña, M Salvadori, I Samtleben, D Sanguineti, M Sapienza, P Schüssler, F Spurio, M Stolarczyk, T Taiuti, M Tayalati, Y Trovato, A Vallage, B Elewyck, V Versari, F Vivolo, D Wilms, J Zaborov, D Zornoza, J Zúñiga, J Aartsen, M Ackermann, M Adams, J Aguilar, J Ahlers, M Ahrens, M Samarai, I 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 Tjus, J Becker, K BenZvi, S 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 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 André, J Clercq, C DeLaunay, J Dembinski, H Deoskar, K Ridder, S Desiati, P Vries, K Wasseige, G With, M DeYoung, T Díaz-Vélez, J 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 Franckowiak, A Friedman, E Fritz, A Gaisser, T Gallagher, J Ganster, E 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 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 Koschinsky, J 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 Maruyama, R Mase, K Maunu, R Meagher, K Medici, M 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 Pepper, J Heros, C Pieloth, D Pinat, E Pizzuto, A Plum, M Price, P Przybylski, G Raab, C Rameez, M Rauch, L Rawlins, K Rea, I Reimann, R Relethford, B 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 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 Taboada, I Tenholt, F Ter-Antonyan, S Terliuk, A Tilav, S Toale, P Tobin, M Tönnis, C Toscano, S Tosi, D Tselengidou, M Tung, C Turcati, A 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 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 Gaggero, D Grasso, D Astrophysical Journal Letters volume 868 L20-L20 (20 Nov 2018) http://arxiv.org/abs/1808.03531v2

In many natural systems, such as the climate, the flow of fluids, but also in the motion of certain celestial objects, we observe complicated, irregular, seemingly random behaviours. These are often created by simple deterministic rules, and not by some vast complexity of the system or its inherent randomness. A typical feature of such chaotic systems is the high sensitivity of trajectories to the initial condition, which is also known in popular culture as the butterfly effect.

Subscribe to