Prospects for dark matter observations in dwarf spheroidal galaxies with the Cherenkov Telescope Array Observatory
Abe, K
Abe, S
Abhir, J
Abhishek, A
Acero, F
Acharyya, A
Adam, R
Aguasca-Cabot, A
Agudo, I
Aguirre-Santaella, A
Alfaro, J
Alfaro, R
Alispach, C
Batista, R
Amans, J
Amato, E
Ambrosi, G
Ambrosino, D
Ambrosino, F
Angel, L
Antonelli, L
Aramo, C
Arcaro, C
Asano, K
Monthly Notices of the Royal Astronomical Society
volume 544
issue 3
2946-2986
(20 Oct 2025)
Measurement of the mean number of muons with energies above 500 GeV in air showers detected with the IceCube Neutrino Observatory
Abbasi, R
Ackermann, M
Adams, J
Agarwalla, S
Aguilar, J
Ahlers, M
Alameddine, J
Amin, N
Andeen, K
Argüelles, C
Ashida, Y
Athanasiadou, S
Axani, S
Babu, R
Bai, X
Baines-Holmes, J
V., A
Barwick, S
Bash, S
Basu, V
Bay, R
Beatty, J
Tjus, J
Behrens, P
Beise, J
Bellenghi, C
Benkel, B
BenZvi, S
Berley, D
Bernardini, E
Besson, D
Blaufuss, E
Bloom, L
Blot, S
Bodo, I
Bontempo, F
Motzkin, J
Meneguolo, C
Böser, S
Botner, O
Böttcher, J
Braun, J
Brinson, B
Brisson-Tsavoussis, Z
Burley, R
Butterfield, D
Campana, M
Carloni, K
Carpio, J
Chattopadhyay, S
Chau, N
Chen, Z
Chirkin, D
Choi, S
Clark, B
Coleman, A
Coleman, P
Collin, G
Connolly, A
Conrad, J
Corley, R
Cowen, D
De Clercq, C
DeLaunay, J
Delgado, D
Delmeulle, T
Deng, S
Desiati, P
de Vries, K
de Wasseige, G
DeYoung, T
Díaz-Vélez, J
DiKerby, S
Dittmer, M
Domi, A
Draper, L
Dueser, L
Durnford, D
Dutta, K
DuVernois, M
Ehrhardt, T
Eidenschink, L
Eimer, A
Eller, P
Ellinger, E
Elsässer, D
Engel, R
Erpenbeck, H
Esmail, W
Eulig, S
Evans, J
Evenson, P
Fan, K
Fang, K
Farrag, K
Fazely, A
Fedynitch, A
Feigl, N
Finley, C
Fischer, L
Fox, D
Franckowiak, A
Fukami, S
Fürst, P
Gallagher, J
Ganster, E
Garcia, A
Garcia, M
Garg, G
Genton, E
Gerhardt, L
Ghadimi, A
Glaser, C
Glüsenkamp, T
Gonzalez, J
Goswami, S
Granados, A
Grant, D
Gray, S
Griffin, S
Griswold, S
Groth, K
Guevel, D
Günther, C
Gutjahr, P
Ha, C
Haack, C
Hallgren, A
Halve, L
Halzen, F
Hamacher, L
Minh, M
Handt, M
Hanson, K
Hardin, J
Harnisch, A
Hatch, P
Haungs, A
Häußler, J
Helbing, K
Hellrung, J
Hennig, L
Heuermann, L
Hewett, R
Heyer, N
Hickford, S
Hidvegi, A
Hill, C
Hill, G
Hmaid, R
Hoffman, K
Hooper, D
Hori, S
Hoshina, K
Hostert, M
Hou, W
Huber, T
Hultqvist, K
Hymon, K
Ishihara, A
Iwakiri, W
Jacquart, M
Jain, S
Janik, O
Jeong, M
Jin, M
Kamp, N
Kang, D
Kang, X
Kappes, A
Kardum, L
Karg, T
Karl, M
Karle, A
Katil, A
Kauer, M
Kelley, J
Khanal, M
Zathul, A
Kheirandish, A
Kimku, H
Kiryluk, J
Klein, C
Klein, S
Kobayashi, Y
Kochocki, A
Koirala, R
Kolanoski, H
Kontrimas, T
Köpke, L
Kopper, C
Koskinen, D
Koundal, P
Kowalski, M
Kozynets, T
Krieger, N
Krishnamoorthi, J
Krishnan, T
Kruiswijk, K
Krupczak, E
Kumar, A
Kun, E
Kurahashi, N
Lad, N
Gualda, C
Arnaud, L
Lamoureux, M
Larson, M
Lauber, F
Lazar, J
DeHolton, K
Leszczyńska, A
Liao, J
Liu, Y
Liubarska, M
Love, C
Lu, L
Lucarelli, F
Luszczak, W
Lyu, Y
Madsen, J
Magnus, E
Mahn, K
Makino, Y
Manao, E
Mancina, S
Mand, A
Mariş, I
Marka, S
Marka, Z
Marten, L
Martinez-Soler, I
Maruyama, R
Mayhew, F
McNally, F
Mead, J
Meagher, K
Mechbal, S
Medina, A
Meier, M
Merckx, Y
Merten, L
Mitchell, J
Molchany, L
Montaruli, T
Moore, R
Morii, Y
Mosbrugger, A
Moulai, M
Mousadi, D
Mukherjee, T
Naab, R
Nakos, M
Naumann, U
Necker, J
Neste, L
Neumann, M
Niederhausen, H
Nisa, M
Noda, K
Noell, A
Novikov, A
Pollmann, A
O’Dell, V
Olivas, A
Orsoe, R
Osborn, J
O’Sullivan, E
Palusova, V
Pandya, H
Parenti, A
Park, N
Parrish, V
Paudel, E
Paul, L
de los Heros, C
Pernice, T
Peterson, J
Plum, M
Pontén, A
Poojyam, V
Popovych, Y
Rodriguez, M
Pries, B
Procter-Murphy, R
Przybylski, G
Pyras, L
Raab, C
Rack-Helleis, J
Rad, N
Ravn, M
Rawlins, K
Rechav, Z
Rehman, A
Reistroffer, I
Resconi, E
Reusch, S
Rho, C
Rhode, W
Riedel, B
Rifaie, A
Roberts, E
Robertson, S
Rongen, M
Rosted, A
Rott, C
Ruhe, T
Ruohan, L
Saffer, J
Salazar-Gallegos, D
Sampathkumar, P
Sandrock, A
Sanger-Johnson, G
Santander, M
Sarkar, S
Savelberg, J
Schaile, P
Schaufel, M
Schieler, H
Schindler, S
Schlickmann, L
Schlüter, B
Schlüter, F
Schmeisser, N
Schmidt, T
Schröder, F
Schumacher, L
Schwirn, S
Sclafani, S
Seckel, D
Seen, L
Seikh, M
Seunarine, S
Myhr, P
Shah, R
Shefali, S
Shimizu, N
Skrzypek, B
Snihur, R
Soedingrekso, J
Søgaard, A
Soldin, D
Soldin, P
Sommani, G
Spannfellner, C
Spiczak, G
Spiering, C
Stachurska, J
Stamatikos, M
Stanev, T
Stezelberger, T
Stürwald, T
Stuttard, T
Sullivan, G
Taboada, I
Ter-Antonyan, S
Terliuk, A
Thakuri, A
Thiesmeyer, M
Thompson, W
Thwaites, J
Tilav, S
Tollefson, K
Toscano, S
Tosi, D
Trettin, A
Upadhyay, A
Upshaw, K
Vaidyanathan, A
Valtonen-Mattila, N
Valverde, J
Vandenbroucke, J
Van Eeden, T
van Eijndhoven, N
van Santen, J
Vara, J
Varsi, F
Venugopal, M
Vereecken, M
Carrasco, S
Verpoest, S
Veske, D
Vijai, A
Villarreal, J
Walck, C
Wang, A
Warrick, E
Weaver, C
Weigel, P
Weindl, A
Wen, A
Wendt, C
Werthebach, J
Weyrauch, M
Whitehorn, N
Wiebusch, C
Williams, D
Witthaus, L
Wolf, M
Wrede, G
Xu, X
Yañez, J
Yao, Y
Yildizci, E
Yoshida, S
Young, R
Yu, F
Yu, S
Yuan, T
Zegarelli, A
Zhang, S
Zhang, Z
Zhelnin, P
Zilberman, P
Physical Review D
volume 112
issue 8
082004
(15 Oct 2025)
Wed, 29 Oct 2025
16:00
16:00
L6
Hard Unknot Diagrams and Arc Presentations
Sam Ketchell
(Mathematical Institute University of Oxford )
Abstract
Abstract: There exist diagrams of the unknot that are "hard" in the sense that any sequence of Reidemeister moves rearranging them into the standard unknot diagram must at some point increase the crossing number beyond what it was originally. I will discuss how such diagrams can be produced and what is known and unknown about them.
Then, I will define and discuss the arc index of a knot, an invariant that behaves more nicely than the crossing number from this perspective, and in some other ways.
Wed, 29 Oct 2025
13:00
13:00
Quillen Room N3.12
A chaotic introduction to Lyapunov exponents
Marta Bucca
Abstract
Strong chaos, the butterfly effect, is a ubiquitous phenomenon in physical systems. In quantum mechanical systems, one of the diagnostics of quantum chaos is an out-of-time-order correlation function, related to the commutator of operators separated in time. In this talk we will review the work of Maldacena, Shenker and Stanford (arxiv:1503.01409), who conjectured that the influence of chaos on this correlator can develop no faster than exponentially, with Lyapunov exponent λL ≤ 2πkBT/\hbar. We will then discuss a system that displays a maximal Lyapunov exponent: the SYK model.
Generalized charges, part II: Non-invertible symmetries and the symmetry TFT
Bhardwaj, L
Schäfer-Nameki, S
SciPost Physics
volume 19
issue 4
(15 Oct 2025)
Bounding phenotype transition probabilities via conditional complexity
Dingle, K
Hagolani, P
Zimm, R
Umar, M
O'Sullivan, S
Louis, A
Journal of The Royal Society Interface
volume 22
issue 231
20240916
(08 Oct 2025)