Evidence for anisotropy of cosmic acceleration

(2018)

Authors:

Jacques Colin, Roya Mohayaee, Mohamed Rameez, Subir Sarkar

Transport of high-energy charged particles through spatially-intermittent turbulent magnetic fields

(2018)

Authors:

LE Chen, AFA Bott, P Tzeferacos, A Rigby, A Bell, R Bingham, C Graziani, J Katz, M Koenig, CK Li, R Petrasso, H-S Park, JS Ross, D Ryu, TG White, B Reville, J Matthews, J Meinecke, F Miniati, EG Zweibel, S Sarkar, AA Schekochihin, DQ Lamb, DH Froula, G Gregori

Analytical estimates of proton acceleration in laser-produced turbulent plasmas

(2018)

Authors:

Konstantin Beyer, Brian Reville, Archie Bott, Hye-Sook Park, Subir Sarkar, Gianluca Gregori

Review of Particle Physics*

American Physical Society (APS) 98:3 (2018) 030001

Authors:

M Tanabashi, K Hagiwara, K Hikasa, K Nakamura, Y Sumino, F Takahashi, J Tanaka, K Agashe, G Aielli, C Amsler, M Antonelli, DM Asner, H Baer, Sw Banerjee, RM Barnett, T Basaglia, CW Bauer, JJ Beatty, VI Belousov, J Beringer, S Bethke, A Bettini, H Bichsel, O Biebel, KM Black, E Blucher, O Buchmuller, V Burkert, MA Bychkov, RN Cahn, M Carena, A Ceccucci, A Cerri, D Chakraborty, M-C Chen, RS Chivukula, G Cowan, O Dahl, G D’Ambrosio, T Damour, D de Florian, A de Gouvêa, T DeGrand, P de Jong, G Dissertori, BA Dobrescu, M D’Onofrio, M Doser, M Drees, HK Dreiner, DA Dwyer, P Eerola, S Eidelman, J Ellis, J Erler, VV Ezhela, W Fetscher, BD Fields, R Firestone, B Foster, A Freitas, H Gallagher, L Garren, H-J Gerber, G Gerbier, T Gershon, Y Gershtein, T Gherghetta, AA Godizov, M Goodman, C Grab, AV Gritsan, C Grojean, DE Groom, M Grünewald, A Gurtu, T Gutsche, HE Haber, C Hanhart, S Hashimoto, Y Hayato, KG Hayes, A Hebecker, S Heinemeyer, B Heltsley, JJ Hernández-Rey, J Hisano, A Höcker, J Holder, A Holtkamp, T Hyodo, KD Irwin, KF Johnson, M Kado, M Karliner, UF Katz, SR Klein, E Klempt, RV Kowalewski, F Krauss, M Kreps, B Krusche, Yu V Kuyanov, Y Kwon, O Lahav, J Laiho, J Lesgourgues, A Liddle, Z Ligeti, C-J Lin, C Lippmann, TM Liss, L Littenberg, KS Lugovsky, SB Lugovsky, A Lusiani, Y Makida, F Maltoni, T Mannel, AV Manohar, WJ Marciano, AD Martin, A Masoni, J Matthews, U-G Meißner, D Milstead, RE Mitchell, K Mönig, P Molaro, F Moortgat, M Moskovic, H Murayama, M Narain, P Nason, S Navas, M Neubert, P Nevski, Y Nir, KA Olive, S Pagan Griso, J Parsons, C Patrignani, JA Peacock, M Pennington, ST Petcov, VA Petrov, E Pianori, A Piepke, A Pomarol, A Quadt, J Rademacker, G Raffelt, BN Ratcliff, P Richardson, A Ringwald, S Roesler, S Rolli, A Romaniouk, LJ Rosenberg, JL Rosner, G Rybka, RA Ryutin, CT Sachrajda, Y Sakai, GP Salam, S Sarkar, F Sauli, O Schneider, K Scholberg, AJ Schwartz, D Scott, V Sharma, SR Sharpe, T Shutt, M Silari, T Sjöstrand, P Skands, T Skwarnicki, JG Smith, GF Smoot, S Spanier, H Spieler, C Spiering, A Stahl, SL Stone, T Sumiyoshi, MJ Syphers, K Terashi, J Terning, U Thoma, RS Thorne, L Tiator, M Titov, NP Tkachenko, NA Törnqvist, DR Tovey, G Valencia, R Van de Water, N Varelas, G Venanzoni, L Verde, MG Vincter, P Vogel, A Vogt, SP Wakely, W Walkowiak, CW Walter, D Wands, DR Ward, MO Wascko, G Weiglein, DH Weinberg, EJ Weinberg, M White, LR Wiencke, S Willocq, CG Wohl, J Womersley, CL Woody, RL Workman, W-M Yao, GP Zeller, OV Zenin, R-Y Zhu, S-L Zhu, F Zimmermann, PA Zyla, J Anderson, L Fuller, VS Lugovsky, P Schaffner

Multi-messenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A

ArXiv 1807.08816 (2018)

Authors:

The IceCube, Fermi-LAT, MAGIC, AGILE, ASAS-SN, HAWC, HES S, INTEGRAL, Kanata, Kiso, Kapteyn, Liverpool telescope, Subaru, Swift NuSTAR, VERITAS, VLA 17B-403 teams

Abstract:

Individual astrophysical sources previously detected in neutrinos are limited to the Sun and the supernova 1987A, whereas the origins of the diffuse flux of high-energy cosmic neutrinos remain unidentified. On 22 September 2017 we detected a high-energy neutrino, IceCube-170922A, with an energy of approximately 290 TeV. Its arrival direction was consistent with the location of a known gamma-ray blazar TXS 0506+056, observed to be in a flaring state. An extensive multi-wavelength campaign followed, ranging from radio frequencies to gamma-rays. These observations characterize the variability and energetics of the blazar and include the first detection of TXS 0506+056 in very-high-energy gamma-rays. This observation of a neutrino in spatial coincidence with a gamma-ray emitting blazar during an active phase suggests that blazars may be a source of high-energy neutrinos.