THE FIRST LIMITS ON THE ULTRA-HIGH ENERGY NEUTRINO FLUENCE FROM GAMMA-RAY BURSTS

• Main Authors: Vieregg, AG, Palladino, K, Allison, P, Baughman, BM, Beatty, JJ, Belov, K, Besson, DZ, Bevan, S, Binns, WR, Chen, C, Chen, P, Clem, JM, Connolly, A, Detrixhe, M, De Marco, D, Dowkontt, PF, DuVernois, M, Gorham, PW, Grashorn, EW, Hill, B, Hoover, S, Huang, M, Israel, MH, Javaid, A, Liewer, KM, Matsuno, S, Mercurio, BC, Miki, C, Mottram, M, Nam, J, Nichol, RJ, Romero-Wolf, A, Ruckman, L, Saltzberg, D, Seckel, D, Varner, GS, Wang, Y
• Format: Article in Journal/Newspaper
• Language: unknown
• Published: IOP PUBLISHING LTD 2011
• Subjects: gamma-ray burst: general; neutrinos; COSMIC-RAYS; AFTERGLOW; FIREBALLS; Antarctic; The Antarctic; Antarc*
• Online Access: http://discovery.ucl.ac.uk/1324585/

We set the first limits on the ultra-high energy (UHE) neutrino fluence at energies greater than 10(9) GeV from gamma-ray bursts (GRBs) based on data from the second flight of the Antarctic Impulsive Transient Antenna (ANITA). During the 31 day flight of ANITA-II, 26 GRBs were recorded by Swift or Fermi. Of these, we analyzed the 12 GRBs which occurred during quiet periods when the payload was away from anthropogenic activity. In a blind analysis, we observe 0 events on a total background of 0.0044 events in the combined prompt window for all 12 low-background bursts. We also observe 0 events from the remaining 14 bursts. We place a 90% confidence level limit on the E-4 prompt neutrino fluence between 10(8) GeV < E < 10(12) GeV of E-4 Phi = 2.5 x 10(17) GeV3 cm(-2) from GRB090107A. This is the first reported limit on the UHE neutrino fluence from GRBs above 10(9) GeV, and the strongest limit above 10(8) GeV.