Limits On Neutrino Emission From Gamma-Ray Bursts With The 40 String Icecube Detector

Abbasi R,Abdou Y, Abu-Zayyad T, Adams J,Aguilar J A,Ahlers M, Andeen K, Auffenberg J,Bai X,Baker M,Barwick S W,Bay R,Bazo Alba J L,Beattie K,Beatty J J, Bechet S,Becker J K,Becker K-H,Benabderrahmane M L,BenZvi S,Berdermann J, Berghaus P, Berley D,Bernardini E,Bertrand D,Besson D Z,Bindig D,Bissok M,Blaufuss E,Blumenthal J,Boersma D J, Bohm C, Bose D,Böser S,Botner O, Braun J,Brown A M,Buitink S,Carson M, Chirkin D,Christy B,Clem J, Clevermann F,Cohen S, Colnard C,Cowen D F,D'Agostino M V,Danninger M,Daughhetee J,Davis J C,De Clercq C, Demirörs L,Depaepe O,Descamps F,Desiati P,de Vries-Uiterweerd G,DeYoung T,Díaz-Vélez J C,Dierckxsens M,Dreyer J,Dumm J P, Ehrlich R,Eisch J,Ellsworth R W,Engdegård O,Euler S,Evenson P A,Fadiran O,Fazely A R,Fedynitch A,Feusels T,Filimonov K,Finley C,Fischer-Wasels T,Foerster M M,Fox B D,Franckowiak A,Franke R,Gaisser T K,Gallagher J,Geisler M,Gerhardt L,Gladstone L, Glüsenkamp T,Goldschmidt A,Goodman J A,Grant D,Griesel T,Gross A,Grullon S,Gurtner M,Ha C, Hallgren A,Halzen F,Han K, Hanson K,Heinen D,Helbing K, Herquet P, Hickford S,Hill G C,Hoffman K D,Homeier A,Hoshina K,Hubert D,Huelsnitz W,Hülss J-P,Hulth P O,Hultqvist K, Hussain S, Ishihara A, Jacobsen J,Japaridze G S,Johansson H,Joseph J M,Kampert K-H, Kappes A,Karg T,Karle A,Kelley J L,Kemming N,Kenny P,Kiryluk J,Kislat F,Klein S R,Köhne J-H,Kohnen G,Kolanoski H, Köpke L, Kopper S,Koskinen D J,Kowalski M, Kowarik T,Krasberg M,Krings T,Kroll G,Kuehn K,Kuwabara T,Labare M,Lafebre S,Laihem K,Landsman H,Larson M J,Lauer R,Lehmann R,Lünemann J,Madsen J,Majumdar P,Marotta A,Maruyama R,Mase K, Matis H S, Meagher K,Merck M,Mészáros P,Meures T,Middell E,Milke N,Miller J,Montaruli T,Morse R,Movit S M,Nahnhauer R,Nam J W,Naumann U,Niessen P,Nygren D R, Odrowski S,Olivas A,Olivo M, O'Murchadha A, Ono M, Panknin S,Paul L,Pérez de los Heros C,Petrovic J,Piegsa A,Pieloth D,Porrata R,Posselt J,Price P B, Prikockis M,Przybylski G T,Rawlins K,Redl P,Resconi E,Rhode W,Ribordy M,Rizzo A,Rodrigues J P,Roth P, Rothmaier F,Rott C,Ruhe T, Rutledge D,Ruzybayev B,Ryckbosch D,Sander H-G,Santander M,Sarkar S, Schatto K,Schmidt T,Schoenwald A,Schukraft A,Schultes A,Schulz O,Schunck M,Seckel D,Semburg B,Seo S H, Sestayo Y,Seunarine S,Silvestri A,Slipak A,Spiczak G M,Spiering C,Stamatikos M,Stanev T,Stephens G,Stezelberger T,Stokstad R G,Stoyanov S,Strahler E A,Straszheim T,Sullivan G W,Swillens Q,Taavola H,Taboada I,Tamburro A,Tarasova O,Tepe A,Ter-Antonyan S,Tilav S,Toale P A,Toscano S,Tosi D,Turčan D,van Eijndhoven N,Vandenbroucke J,Van Overloop A,van Santen J,Vehring M,Voge M,Voigt B,Walck C,Waldenmaier T,Wallraff M,Walter M,Weaver C, Wendt C, Westerhoff S,Whitehorn N,Wiebe K,Wiebusch C H,Williams D R,Wischnewski R,Wissing H,Wolf M,Woschnagg K,Xu C, Xu X W,Yodh G,Yoshida S,Zarzhitsky P,Null Null

PHYSICAL REVIEW LETTERS（2011）

引用 149|浏览77

暂无评分

摘要

IceCube has become the first neutrino telescope with a sensitivity below the TeV neutrino flux predicted from gamma-ray bursts if gamma-ray bursts are responsible for the observed cosmic-ray flux above 10(18) eV. Two separate analyses using the half-complete IceCube detector, one a dedicated search for neutrinos from p gamma interactions in the prompt phase of the gamma-ray burst fireball and the other a generic search for any neutrino emission from these sources over a wide range of energies and emission times, produced no evidence for neutrino emission, excluding prevailing models at 90% confidence.

查看译文

关键词

neutrino,string,muon,charged particle,dissertation,gamma ray burst

AI 理解论文

溯源树

样例

生成溯源树，研究论文发展脉络

Chat Paper

正在生成论文摘要