Modification of jet structure in nuclear collisions: theory overview (and pp perspective)

Nuclear Physics A Elsevier 982 (2019) 149-155

Unveiling the yoctosecond structure of the QGP with top quarks

Nuclear Physics A Elsevier 982 (2019) 795-798

Authors:

Liliana Apolinário, Guilherme Milhano, Carlos A Salgado, Gavin Salam

Hearing without seeing: gravitational waves from hot and cold hidden sectors

ArXiv 1901.11038 (2019)

Authors:

Malcolm Fairbairn, Edward Hardy, Alastair Wickens

Improving Statistical Sensitivity of X-ray Searches for Axion-Like Particles

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) (2019)

Authors:

Joseph P Conlon, Markus Rummel

All-Sky Measurement of the Anisotropy of Cosmic Rays at 10 TeV and Mapping of the Local Interstellar Magnetic Field

Astrophysical Journal American Astronomical Society 871 (2019) 96-96

Authors:

HAWC Collaboration, AU Abeysekara, R Alfaro, C Alvarez, JD Álvarez, R Arceo, JC Arteaga-Velázquez, D Avila Rojas, E Belmont-Moreno, SY BenZvi, C Brisbois, T Capistrán, A Carramiñana, S Casanova, U Cotti, J Cotzomi, JC Díaz-Vélez, C De León, E De la Fuente, S Dichiara, MA DuVernois, C Espinoza, DW Fiorino, H Fleischhack, N Fraija, A Galván-Gámez, JA García-González, MM González, JA Goodman, Z Hampel-Arias, JP Harding, S Hernandez, B Hona, F Hueyotl-Zahuantitla, A Iriarte, A Jardin-Blicq, V Joshi, A Lara, H León Vargas, G Luis-Raya, K Malone, SS Marinelli, J Martínez-Castro, O Martinez, JA Matthews, P Miranda-Romagnoli, E Moreno, M Mostafá, L Nellen, M Newbold, MU Nisa, R Noriega-Papaqui, EG Pérez-Pérez, J Pretz, Z Ren, CD Rho, C Rivière, D Rosa-González, M Rosenberg, H Salazar, F Salesa Greus, A Sandoval, M Schneider, H Schoorlemmer, G Sinnis, AJ Smith, P Surajbali, I Taboada, K Tollefson, I Torres, L Villaseño, T Weisgarber, J Wood, A Zepeda, H Zhou, IceCube Collaboration, MG Aartsen, M Ackermann, J Adams, JA Aguilar, M Ahlers, M Ahrens, D Altmann, K Andeen, T Anderson, I Ansseau, G Anton, C Argüelles, J Auffenberg, S Axani, P Backes, H Bagherpour, X Bai, A Barbano, JP Barron, SW Barwick, V Baum, R Bay, JJ Beatty, K-H Becker, J Becker Tjus, S BenZvi, D Berley, E Bernardini, DZ Besson, G Binder, D Bindig, E Blaufuss, S Blot, C Bohm, M Börner, F Bos, S Böser, O Botner, E Bourbeau, J Bourbeau, F Bradascio, J Braun, H-P Bretz, S Bron, J Brostean-Kaiser, A Burgman, RS Busse, T Carver, C Chen, E Cheung, D Chirkin, K Clark, L Classen, GH Collin, JM Conrad, P Coppin, P Correa, DF Cowen, R Cross, P Dave, M Day, JPAM de André, C De Clercq, JJ DeLaunay, H Dembinski, K Deoskar, S De Ridder, P Desiati, KD de Vries, G de Wasseige, M de With, T DeYoung, JC Díaz-Vélez, H Dujmovic, M Dunkman, E Dvorak, B Eberhardt, T Ehrhardt, B Eichmann, P Eller, PA Evenson, S Fahey, AR Fazely, J Felde, K Filimonov, C Finley, A Franckowiak, E Friedman, A Fritz, TK Gaisser, J Gallagher, E Ganster, S Garrappa, L Gerhardt, K Ghorbani, W Giang, T Glauch, T Glüsenkamp, A Goldschmidt, JG Gonzalez, D Grant, Z Griffith, C Haack, A Hallgren, L Halve, F Halzen, K Hanson, D Hebecker, D Heereman, K Helbing, R Hellauer, S Hickford, J Hignight, GC Hill, KD Hoffman, R Hoffmann, T Hoinka, B Hokanson-Fasig, K Hoshina, F Huang, M Huber, K Hultqvist, M Hünnefeld, R Hussain, S In, N Iovine, A Ishihara, E Jacobi, GS Japaridze, M Jeong, K Jero, BJP Jones, P Kalaczynski, W Kang, A Kappes, D Kappesser, T Karg, A Karle, U Katz, M Kauer, A Keivani, JL Kelley, A Kheirandish, J Kim, T Kintscher, J Kiryluk, T Kittler, SR Klein, R Koirala, H Kolanoski, L Köpke, C Kopper, S Kopper, DJ Koskinen, M Kowalski, K Krings, M Kroll, G Krückl, S Kunwar, N Kurahashi, A Kyriacou, M Labare, JL Lanfranchi, MJ Larson, F Lauber, K Leonard, M Leuermann, QR Liu, E Lohfink, CJ Lozano Mariscal, L Lu, J Lünemann, W Luszczak, J Madsen, G Maggi, KBM Mahn, Y Makino, S Mancina, IC Mariş, R Maruyama, K Mase, R Maunu, K Meagher, M Medici, A Medina, M Meier, T Menne, G Merino, T Meures, S Miarecki, J Micallef, G Momenté, T Montaruli, RW Moore, M Moulai, R Nagai, R Nahnhauer, P Nakarmi, U Naumann, G Neer, H Niederhausen, SC Nowicki, DR Nygren, A Obertacke Pollmann, A Olivas, A O'Murchadha, E O'Sullivan, T Palczewski, H Pandya, DV Pankova, P Peiffer, C Pérez de los Heros, D Pieloth, E Pinat, A Pizzuto, M Plum, PB Price, GT Przybylski, C Raab, A Raissi, M Rameez, L Rauch, K Rawlins, IC Rea, R Reimann, B Relethford, G Renzi, E Resconi, W Rhode, M Richman, S Robertson, M Rongen, C Rott, T Ruhe, D Ryckbosch, D Rysewyk, I Safa, SE Sanchez Herrera, A Sandrock, J Sandroos, M Santander, S Sarkar, S Sarkar, K Satalecka, M Schaufel, P Schlunder, T Schmidt, A Schneider, J Schneider, S Schöneberg, L Schumacher, S Sclafani, D Seckel, S Seunarine, J Soedingrekso, D Soldin, M Song, GM Spiczak, C Spiering, J Stachurska, M Stamatikos, T Stanev, A Stasik, R Stein, J Stettner, A Steuer, T Stezelberger, RG Stokstad, A Stößl, NL Strotjohann, T Stuttard, GW Sullivan, M Sutherland, I Taboada, F Tenholt, S Ter-Antonyan, A Terliuk, S Tilav, MN Tobin, C Tönnis, S Toscano, D Tosi, M Tselengidou, CF Tung, A Turcati, R Turcotte, CF Turley, B Ty, E Unger, MA Unland Elorrieta, M Usner, J Vandenbroucke, W Van Driessche, D van Eijk, N van Eijndhoven, S Vanheule, J van Santen, M Vraeghe, C Walck, A Wallace, M Wallraff, N Wandkowsky, FD Wandler, TB Watson, C Weaver, MJ Weiss, J Weldert, C Wendt, J Werthebach, S Westerhoff, BJ Whelan, N Whitehorn, K Wiebe, CH Wiebusch, L Wille, DR Williams, L Wills, M Wolf, J Wood, TR Wood, E Woolsey, K Woschnagg, G Wrede, DL Xu, XW Xu, Y Xu, JP Yanez, G Yodh, S Yoshida, T Yuan

Abstract:

We present the first full-sky analysis of the cosmic ray arrival direction distribution with data collected by the HAWC and IceCube observatories in the Northern and Southern hemispheres at the same median primary particle energy of 10 TeV. The combined sky map and angular power spectrum largely eliminate biases that result from partial sky coverage and holds a key to probe into the propagation properties of TeV cosmic rays through our local interstellar medium and the interaction between the interstellar and heliospheric magnetic fields. From the map we determine the horizontal dipole components of the anisotropy $\delta_{0h} = 9.16 \times 10^{-4}$ and $\delta_{6h} = 7.25 \times 10^{-4}~(\pm0.04 \times 10^{-4})$. In addition, we infer the direction ($229.2\pm 3.5^\circ$ RA , $11.4\pm 3.0^\circ$ Dec.) of the interstellar magnetic field from the boundary between large scale excess and deficit regions from which we estimate the missing corresponding vertical dipole component of the large scale anisotropy to be $\delta_N \sim -3.97 ^{+1.0}_{-2.0} \times 10^{-4}$.