SEARCH FOR PROMPT NEUTRINO EMISSION FROM GAMMA-RAY BURSTS WITH ICECUBE
SEARCH FOR PROMPT NEUTRINO EMISSION FROM GAMMA-RAY BURSTS WITH ICECUBE
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DOI：
10.1088/2041-8205/805/1/l5
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发表时间：
2014-12
期刊：
影响因子：
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通讯作者：
I. C. M. Aartsen;M. Ackermann;J. Adams;J. Aguilar;M. Ahlers;M. Ahrens;D. Altmann;T. Anderson;C. Arguelles;T. Arlen;J. Auffenberg;X. Bai;S. Barwick;V. Baum;R. Bay;J. Beatty;J. Tjus;K. Becker;S. BenZvi;P. Berghaus;D. Berley;E. Bernardini;A. Bernhard;D. Besson;G. Binder;D. Bindig;M. Bissok;E. Blaufuss;J. Blumenthal;D. Boersma;C. Bohm;F. Bos;D. Bose;S. Boser;O. Botner;L. Brayeur;H. Bretz;A. Brown;N. Buzinsky;J. Casey;M. Casier;E. Cheung;D. Chirkin;A. Christov;B. Christy;K. Clark;L. Classen;F. Clevermann;S. Coenders;D. Cowen;A. H. C. Silva;J. Daughhetee;J. Davis;M. Day;J. Andr'e;C. Clercq;S. Ridder;P. Desiati;K. D. Vries;M. With;T. DeYoung;J. C. D'iaz-V'elez;M. Dunkman;R. Eagan;B. Eberhardt;T. Ehrhardt;B. Eichmann;J. Eisch;S. Euler;P. Evenson;O. Fadiran;A. Fazely;A. Fedynitch;J. Feintzeig;J. Felde;K. Filimonov;C. Finley;T. Fischer-Wasels;S. Flis;K. Frantzen;T. Fuchs;T. Gaisser;R. Gaior;J. Gallagher;L. Gerhardt;D. Gier;L. Gladstone;T. Glusenkamp;A. Goldschmidt;G. Golup;J. G. Gonzalez;J. Goodman;D. G'ora;D. Grant;P. Gretskov;J. Groh;A. Gross;C. Ha;C. Haack;A. H. Ismail;P. Hallen;A. Hallgren;F. Halzen;K. Hanson;D. Hebecker;D. Heereman;D. Heinen;K. Helbing;R. Hellauer;D. Hellwig;S. Hickford;G. Hill;K. Hoffman;R. Hoffmann;A. Homeier;K. Hoshina;F. Huang;W. Huelsnitz;P. O. Hulth;K. Hultqvist;A. Ishihara;E. Jacobi;J. Jacobsen;G. Japaridze;K. Jero;O. Jlelati;M. Jurkovič;B. Kaminsky;A. Kappes;T. Karg;A. Karle;M. Kauer;A. Keivani;J. Kelley;A. Kheirandish;J. Kiryluk;J. Klas;S. Klein;J. Kohne;G. Kohnen;H. Kolanoski;A. Koob;L. Kopke;C. Kopper;S. Kopper;D. Koskinen;M. Kowalski;A. Kriesten;K. Krings;G. Kroll;M. Kroll;J. Kunnen;N. Kurahashi;T. Kuwabara;M. Labare;J. Lanfranchi;D. T. Larsen;M. Larson;M. Lesiak-Bzdak;M. Leuermann;J. Lunemann;J. Madsen;G. Maggi;R. Maruyama;K. Mase;H. Matis;R. Maunu;F. McNally;K. Meagher;M. Medici;A. Meli;T. Meures;S. Miarecki;E. Middell;E. Middlemas;N. Milke;J. Miller;L. Mohrmann;T. Montaruli;R. Morse;R. Nahnhauer;U. Naumann;H. Niederhausen;S. Nowicki;D. Nygren;A. Obertacke;S. Odrowski;A. Olivas;A. Omairat;A. O'Murchadha;T. Palczewski;L. Paul;O. Penek;J. Pepper;C. Heros;C. Pfendner;D. Pieloth;E. Pinat;J. Posselt;P. Price;G. Przybylski;J. Putz;M. Quinnan;L. Radel;M. Rameez;K. Rawlins;P. Redl;I. Rees;R. Reimann;M. Relich;E. Resconi;W. Rhode;M. Richman;B. Riedel;S. Robertson;J. Rodrigues;M. Rongen;C. Rott;T. Ruhe;B. Ruzybayev;D. Ryckbosch;S. M. Saba;H. Sander;J. Sandroos;M. Santander;S. Sarkar;K. Schatto;F. Scheriau;T. Schmidt;M. Schmitz;S. Schoenen;S. Schoneberg;A. Schonwald;A. Schukraft;L. Schulte;O. Schulz;D. Seckel;Y. Sestayo;S. Seunarine;R. Shanidze;M. Smith;D. Soldin;G. Spiczak;C. Spiering;M. Stamatikos;T. Stanev;N. Stanisha;Alexander Stasik;T. Stezelberger;R. Stokstad;A. Stossl;E. Strahler;R. Strom;N. Strotjohann;G. Sullivan;H. Taavola;I. Taboada;A. Tamburro;A. Tepe;S. Ter-Antonyan;A. Terliuk;G. Tevsi'c;S. Tilav;P. Toale;M. Tobin;D. Tosi;M. Tselengidou;E. Unger;M. Usner;S. Vallecorsa;N. Eijndhoven;J. Vandenbroucke;J. Santen;S. Vanheule;M. Vehring;M. Voge;M. Vraeghe;C. Walck;M. Wallraff;C. Weaver;M. Wellons;C. Wendt;S. Westerhoff;B. Whelan;N. Whitehorn;C. Wichary;K. Wiebe;C. Wiebusch;D. Williams;H. Wissing;M. Wolf;T. R. Wood;K. Woschnagg;D. Xu;X. Xu;Y. Xu;J. Yáñez;G. Yodh;S. Yoshida;P. Zarzhitsky;J. Ziemann;M. Zoll
中科院分区：
文献类型：
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作者：
I. C. M. Aartsen;M. Ackermann;J. Adams;J. Aguilar;M. Ahlers;M. Ahrens;D. Altmann;T. Anderson;C. Arguelles;T. Arlen;J. Auffenberg;X. Bai;S. Barwick;V. Baum;R. Bay;J. Beatty;J. Tjus;K. Becker;S. BenZvi;P. Berghaus;D. Berley;E. Bernardini;A. Bernhard;D. Besson;G. Binder;D. Bindig;M. Bissok;E. Blaufuss;J. Blumenthal;D. Boersma;C. Bohm;F. Bos;D. Bose;S. Boser;O. Botner;L. Brayeur;H. Bretz;A. Brown;N. Buzinsky;J. Casey;M. Casier;E. Cheung;D. Chirkin;A. Christov;B. Christy;K. Clark;L. Classen;F. Clevermann;S. Coenders;D. Cowen;A. H. C. Silva;J. Daughhetee;J. Davis;M. Day;J. Andr'e;C. Clercq;S. Ridder;P. Desiati;K. D. Vries;M. With;T. DeYoung;J. C. D'iaz-V'elez;M. Dunkman;R. Eagan;B. Eberhardt;T. Ehrhardt;B. Eichmann;J. Eisch;S. Euler;P. Evenson;O. Fadiran;A. Fazely;A. Fedynitch;J. Feintzeig;J. Felde;K. Filimonov;C. Finley;T. Fischer-Wasels;S. Flis;K. Frantzen;T. Fuchs;T. Gaisser;R. Gaior;J. Gallagher;L. Gerhardt;D. Gier;L. Gladstone;T. Glusenkamp;A. Goldschmidt;G. Golup;J. G. Gonzalez;J. Goodman;D. G'ora;D. Grant;P. Gretskov;J. Groh;A. Gross;C. Ha;C. Haack;A. H. Ismail;P. Hallen;A. Hallgren;F. Halzen;K. Hanson;D. Hebecker;D. Heereman;D. Heinen;K. Helbing;R. Hellauer;D. Hellwig;S. Hickford;G. Hill;K. Hoffman;R. Hoffmann;A. Homeier;K. Hoshina;F. Huang;W. Huelsnitz;P. O. Hulth;K. Hultqvist;A. Ishihara;E. Jacobi;J. Jacobsen;G. Japaridze;K. Jero;O. Jlelati;M. Jurkovič;B. Kaminsky;A. Kappes;T. Karg;A. Karle;M. Kauer;A. Keivani;J. Kelley;A. Kheirandish;J. Kiryluk;J. Klas;S. Klein;J. Kohne;G. Kohnen;H. Kolanoski;A. Koob;L. Kopke;C. Kopper;S. Kopper;D. Koskinen;M. Kowalski;A. Kriesten;K. Krings;G. Kroll;M. Kroll;J. Kunnen;N. Kurahashi;T. Kuwabara;M. Labare;J. Lanfranchi;D. T. Larsen;M. Larson;M. Lesiak-Bzdak;M. Leuermann;J. Lunemann;J. Madsen;G. Maggi;R. Maruyama;K. Mase;H. Matis;R. Maunu;F. McNally;K. Meagher;M. Medici;A. Meli;T. Meures;S. Miarecki;E. Middell;E. Middlemas;N. Milke;J. Miller;L. Mohrmann;T. Montaruli;R. Morse;R. Nahnhauer;U. Naumann;H. Niederhausen;S. Nowicki;D. Nygren;A. Obertacke;S. Odrowski;A. Olivas;A. Omairat;A. O'Murchadha;T. Palczewski;L. Paul;O. Penek;J. Pepper;C. Heros;C. Pfendner;D. Pieloth;E. Pinat;J. Posselt;P. Price;G. Przybylski;J. Putz;M. Quinnan;L. Radel;M. Rameez;K. Rawlins;P. Redl;I. Rees;R. Reimann;M. Relich;E. Resconi;W. Rhode;M. Richman;B. Riedel;S. Robertson;J. Rodrigues;M. Rongen;C. Rott;T. Ruhe;B. Ruzybayev;D. Ryckbosch;S. M. Saba;H. Sander;J. Sandroos;M. Santander;S. Sarkar;K. Schatto;F. Scheriau;T. Schmidt;M. Schmitz;S. Schoenen;S. Schoneberg;A. Schonwald;A. Schukraft;L. Schulte;O. Schulz;D. Seckel;Y. Sestayo;S. Seunarine;R. Shanidze;M. Smith;D. Soldin;G. Spiczak;C. Spiering;M. Stamatikos;T. Stanev;N. Stanisha;Alexander Stasik;T. Stezelberger;R. Stokstad;A. Stossl;E. Strahler;R. Strom;N. Strotjohann;G. Sullivan;H. Taavola;I. Taboada;A. Tamburro;A. Tepe;S. Ter-Antonyan;A. Terliuk;G. Tevsi'c;S. Tilav;P. Toale;M. Tobin;D. Tosi;M. Tselengidou;E. Unger;M. Usner;S. Vallecorsa;N. Eijndhoven;J. Vandenbroucke;J. Santen;S. Vanheule;M. Vehring;M. Voge;M. Vraeghe;C. Walck;M. Wallraff;C. Weaver;M. Wellons;C. Wendt;S. Westerhoff;B. Whelan;N. Whitehorn;C. Wichary;K. Wiebe;C. Wiebusch;D. Williams;H. Wissing;M. Wolf;T. R. Wood;K. Woschnagg;D. Xu;X. Xu;Y. Xu;J. Yáñez;G. Yodh;S. Yoshida;P. Zarzhitsky;J. Ziemann;M. Zoll
我们提出的约束来自四年的IceCube数据的搜索提示中微子通量从伽马射线暴（GRBs）。在观测到的506次爆发中，有一次发现了一个与大气中微子背景相符的低显著性中微子。虽然伽玛暴已被提出作为超高能宇宙射线的候选源，我们对中微子通量的限制不利于最新模型的参数空间。我们还发现，最近观测到的天体物理中微子通量中，不超过10.1%是由现有卫星可能观测到的伽马射线暴的瞬发辐射组成的。
We present constraints derived from a search of four years of IceCube data for a prompt neutrino flux from gamma-ray bursts (GRBs). A single low-significance neutrino, compatible with the atmospheric neutrino background, was found in coincidence with one of the 506 observed bursts. Although GRBs have been proposed as candidate sources for ultra-high-energy cosmic rays, our limits on the neutrino flux disfavor much of the parameter space for the latest models. We also find that no more than ∼1% of the recently observed astrophysical neutrino flux consists of prompt emission from GRBs that are potentially observable by existing satellites.