Search for High-energy Neutrino Emission from Galactic X-Ray Binaries with IceCube
Search for High-energy Neutrino Emission from Galactic X-Ray Binaries with IceCube
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DOI：
10.3847/2041-8213/ac67d8
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发表时间：
2022-02
期刊：
影响因子：
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通讯作者：
R. Abbasi;M. Ackermann;J. Adams;J. Aguilar;M. Ahlers;M. Ahrens;J. Alameddine;A. A. Alves-A.;N. M. Amin;K. Andeen;T. Anderson;G. Anton;C. Arguelles;Y. Ashida;S. Axani;X. Bai;V. A.Balagopal;S. Barwick;B. Bastian;V. Basu;S. Baur;R. Bay;J. Beatty;K. Becker;J. Tjus;J. Beise;C. Bellenghi;S. Benda;S. BenZvi;D. Berley;E. Bernardini;D. Besson;G. Binder;D. Bindig;E. Blaufuss;S. Blot;M. Boddenberg;F. Bontempo;J. Borowka;S. Boser;O. Botner;J. Bottcher;E. Bourbeau;F. Bradascio;J. Braun;B. Brinson;S. Bron;J. Brostean-Kaiser;S. Browne;A. Burgman;R. Burley;R. Busse;M. Campana;E. Carnie-Bronca;C. Chen;Z. Chen;D. Chirkin;K. Choi;B. Clark;K. Clark;L. Classen;A. Coleman;G. Collin;J. Conrad;P. Coppin;P. Correa;D. Cowen;R. Cross;C. Dappen;P. Dave;C. Clercq;J. DeLaunay;D. L'opez;H. Dembinski;K. Deoskar;A. Desai;P. Desiati;K. D. Vries;G. Wasseige;M. With;T. DeYoung;A. Diaz;J. C. D'iaz-V'elez;M. Dittmer;H. Dujmovic;M. Dunkman;M. DuVernois;T. Ehrhardt;P. Eller;R. Engel;H. Erpenbeck;J. Evans;P. Evenson;K. L. Fan;A. Fazely;A. Fedynitch;N. Feigl;S. Fiedlschuster;A. Fienberg;C. Finley;L. Fischer;D. Fox;A. Franckowiak;E. Friedman;A. Fritz;P. Furst;T. Gaisser;J. Gallagher;E. Ganster;A. Garcia;S. Garrappa;L. Gerhardt;A. Ghadimi;C. Glaser;T. Glauch;T. Glusenkamp;J. G. Gonzalez;S. Goswami;D. Grant;T. Gr'egoire;S. Griswold;C. Gunther;P. Gutjahr;C. Haack;A. Hallgren;R. Halliday;L. Halve;F. Halzen;M. H. Minh;K. Hanson;J. Hardin;A. Harnisch;A. Haungs;D. Hebecker;K. Helbing;F. Henningsen;E. C. Hettinger;S. Hickford;J. Hignight;C. Hill;G. Hill;K. Hoffman;R. Hoffmann;K. Hoshina;F. Huang;M. Huber;T. Huber;K. Hultqvist;Mirco Hünnefeld;R. Hussain;K. Hymon;S. In;N. Iovine;A. Ishihara;M. Jansson;G. Japaridze;M. Jeong;M. Jin;B. Jones;D. Kang;W. Kang;X. Kang;A. Kappes;D. Kappesser;L. Kardum;T. Karg;M. Karl;A. Karle;U. Katz;M. Kauer;M. Kellermann;J. Kelley;A. Kheirandish;K. Kin;T. Kintscher;J. Kiryluk;S. Klein;A. Kochocki;R. Koirala;H. Kolanoski;T. Kontrimas;L. Kopke;C. Kopper;S. Kopper;D. Koskinen;P. Koundal;M. Kovacevich;M. Kowalski;T. Kozynets;E. Krupczak;E. Kun;N. Kurahashi;N. Lad;C. L. Gualda;J. Lanfranchi;M. Larson;F. Lauber;J. Lazar;J. Lee;K. Leonard;A. Leszczy'nska;Y. Li;M. Lincetto;Q R Liu;M. Liubarska;E. Lohfink;C. J. L. Mariscal;L. Lu;F. Lucarelli;A. Ludwig;W. Luszczak;Y. Lyu;W. Ma;J. Madsen;K. Mahn;Y. Makino;S. Mancina;I. Marics;I. Martinez-Soler;R. Maruyama;S. McCarthy;T. McElroy;F. McNally;J. Mead;K. Meagher;S. Mechbal;A. Medina;M. Meier;S. Meighen-Berger;J. Micallef;D. Mockler;T. Montaruli;R. Moore;R. Morse;M. Moulai;R. Naab;R. Nagai;U. Naumann;J. Necker;L. Nguyen;H. Niederhausen;M. Nisa;S. Nowicki;A. Pollmann;M. Oehler;B. Oeyen;A. Olivas;E. O’Sullivan;H. Pandya;D. Pankova;N. Park;G. K. Parker;E. Paudel;L. Paul;C. Heros;L. Peters;J. Peterson;S. Philippen;S. Pieper;M. Pittermann;A. Pizzuto;M. Plum;Y. Popovych;A. Porcelli;M. Rodriguez;B. Pries;G. Przybylski;C. Raab;J. Rack-Helleis;A. Raissi;M. Rameez;K. Rawlins;I. C. Rea;Z. Rechav;A. Rehman;P. Reichherzer;R. Reimann;G. Renzi;E. Resconi;S. Reusch;W. Rhode;M. Richman;B. Riedel;E. Roberts;S. Robertson;G. Roellinghoff;M. Rongen;C. Rott;T. Ruhe;D. Ryckbosch;D. Cantu;I. Safa;J. Saffer;S. Herrera;A. Sandrock;M. Santander;S. Sarkar;K. Satalecka;M. Schaufel;H. Schieler;S. Schindler;T. Schmidt;A. Schneider;J. Schneider;F. Schroder;L. Schumacher;G. Schwefer;S. Sclafani;D. Seckel;S. Seunarine;A. Sharma;S. Shefali;N. Shimizu;M. Silva;B. Skrzypek;B. Smithers;R. Snihur;J. Soedingrekso;D. Soldin;C. Spannfellner;G. Spiczak;C. Spiering;J. Stachurska;M. Stamatikos;T. Stanev;R. Stein;J. Stettner;T. Stezelberger;T. Sturwald;T. Stuttard;G. Sullivan;I. Taboada;S. Ter-Antonyan;J. Thwaites;S. Tilav;F. Tischbein;K. Tollefson;C. Tonnis;S. Toscano;D. Tosi;A. Trettin;M. Tselengidou;C. Tung;A. Turcati;R. Turcotte;C. Turley;J. P. Twagirayezu;B. Ty;M. U. Elorrieta;N. Valtonen-Mattila;J. Vandenbroucke;N. Eijndhoven;D. Vannerom;J. Santen;J. Veitch-Michaelis;S. Verpoest;C. Walck;W. Wang;T. Watson;C. Weaver;P. Weigel;A. Weindl;M. Weiss;J. Weldert;C. Wendt;J. Werthebach;M. Weyrauch;N. Whitehorn;C. Wiebusch;N. Willey;D. R. Williams;M. Wolf;G. Wrede;J. Wulff;X. Xu;J. Yáñez;E. Yildizci;S. Yoshida;S. Yu;T. Yuan;Z. Zhang;P. Zhelnin
中科院分区：
文献类型：
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作者：
R. Abbasi;M. Ackermann;J. Adams;J. Aguilar;M. Ahlers;M. Ahrens;J. Alameddine;A. A. Alves-A.;N. M. Amin;K. Andeen;T. Anderson;G. Anton;C. Arguelles;Y. Ashida;S. Axani;X. Bai;V. A.Balagopal;S. Barwick;B. Bastian;V. Basu;S. Baur;R. Bay;J. Beatty;K. Becker;J. Tjus;J. Beise;C. Bellenghi;S. Benda;S. BenZvi;D. Berley;E. Bernardini;D. Besson;G. Binder;D. Bindig;E. Blaufuss;S. Blot;M. Boddenberg;F. Bontempo;J. Borowka;S. Boser;O. Botner;J. Bottcher;E. Bourbeau;F. Bradascio;J. Braun;B. Brinson;S. Bron;J. Brostean-Kaiser;S. Browne;A. Burgman;R. Burley;R. Busse;M. Campana;E. Carnie-Bronca;C. Chen;Z. Chen;D. Chirkin;K. Choi;B. Clark;K. Clark;L. Classen;A. Coleman;G. Collin;J. Conrad;P. Coppin;P. Correa;D. Cowen;R. Cross;C. Dappen;P. Dave;C. Clercq;J. DeLaunay;D. L'opez;H. Dembinski;K. Deoskar;A. Desai;P. Desiati;K. D. Vries;G. Wasseige;M. With;T. DeYoung;A. Diaz;J. C. D'iaz-V'elez;M. Dittmer;H. Dujmovic;M. Dunkman;M. DuVernois;T. Ehrhardt;P. Eller;R. Engel;H. Erpenbeck;J. Evans;P. Evenson;K. L. Fan;A. Fazely;A. Fedynitch;N. Feigl;S. Fiedlschuster;A. Fienberg;C. Finley;L. Fischer;D. Fox;A. Franckowiak;E. Friedman;A. Fritz;P. Furst;T. Gaisser;J. Gallagher;E. Ganster;A. Garcia;S. Garrappa;L. Gerhardt;A. Ghadimi;C. Glaser;T. Glauch;T. Glusenkamp;J. G. Gonzalez;S. Goswami;D. Grant;T. Gr'egoire;S. Griswold;C. Gunther;P. Gutjahr;C. Haack;A. Hallgren;R. Halliday;L. Halve;F. Halzen;M. H. Minh;K. Hanson;J. Hardin;A. Harnisch;A. Haungs;D. Hebecker;K. Helbing;F. Henningsen;E. C. Hettinger;S. Hickford;J. Hignight;C. Hill;G. Hill;K. Hoffman;R. Hoffmann;K. Hoshina;F. Huang;M. Huber;T. Huber;K. Hultqvist;Mirco Hünnefeld;R. Hussain;K. Hymon;S. In;N. Iovine;A. Ishihara;M. Jansson;G. Japaridze;M. Jeong;M. Jin;B. Jones;D. Kang;W. Kang;X. Kang;A. Kappes;D. Kappesser;L. Kardum;T. Karg;M. Karl;A. Karle;U. Katz;M. Kauer;M. Kellermann;J. Kelley;A. Kheirandish;K. Kin;T. Kintscher;J. Kiryluk;S. Klein;A. Kochocki;R. Koirala;H. Kolanoski;T. Kontrimas;L. Kopke;C. Kopper;S. Kopper;D. Koskinen;P. Koundal;M. Kovacevich;M. Kowalski;T. Kozynets;E. Krupczak;E. Kun;N. Kurahashi;N. Lad;C. L. Gualda;J. Lanfranchi;M. Larson;F. Lauber;J. Lazar;J. Lee;K. Leonard;A. Leszczy'nska;Y. Li;M. Lincetto;Q R Liu;M. Liubarska;E. Lohfink;C. J. L. Mariscal;L. Lu;F. Lucarelli;A. Ludwig;W. Luszczak;Y. Lyu;W. Ma;J. Madsen;K. Mahn;Y. Makino;S. Mancina;I. Marics;I. Martinez-Soler;R. Maruyama;S. McCarthy;T. McElroy;F. McNally;J. Mead;K. Meagher;S. Mechbal;A. Medina;M. Meier;S. Meighen-Berger;J. Micallef;D. Mockler;T. Montaruli;R. Moore;R. Morse;M. Moulai;R. Naab;R. Nagai;U. Naumann;J. Necker;L. Nguyen;H. Niederhausen;M. Nisa;S. Nowicki;A. Pollmann;M. Oehler;B. Oeyen;A. Olivas;E. O’Sullivan;H. Pandya;D. Pankova;N. Park;G. K. Parker;E. Paudel;L. Paul;C. Heros;L. Peters;J. Peterson;S. Philippen;S. Pieper;M. Pittermann;A. Pizzuto;M. Plum;Y. Popovych;A. Porcelli;M. Rodriguez;B. Pries;G. Przybylski;C. Raab;J. Rack-Helleis;A. Raissi;M. Rameez;K. Rawlins;I. C. Rea;Z. Rechav;A. Rehman;P. Reichherzer;R. Reimann;G. Renzi;E. Resconi;S. Reusch;W. Rhode;M. Richman;B. Riedel;E. Roberts;S. Robertson;G. Roellinghoff;M. Rongen;C. Rott;T. Ruhe;D. Ryckbosch;D. Cantu;I. Safa;J. Saffer;S. Herrera;A. Sandrock;M. Santander;S. Sarkar;K. Satalecka;M. Schaufel;H. Schieler;S. Schindler;T. Schmidt;A. Schneider;J. Schneider;F. Schroder;L. Schumacher;G. Schwefer;S. Sclafani;D. Seckel;S. Seunarine;A. Sharma;S. Shefali;N. Shimizu;M. Silva;B. Skrzypek;B. Smithers;R. Snihur;J. Soedingrekso;D. Soldin;C. Spannfellner;G. Spiczak;C. Spiering;J. Stachurska;M. Stamatikos;T. Stanev;R. Stein;J. Stettner;T. Stezelberger;T. Sturwald;T. Stuttard;G. Sullivan;I. Taboada;S. Ter-Antonyan;J. Thwaites;S. Tilav;F. Tischbein;K. Tollefson;C. Tonnis;S. Toscano;D. Tosi;A. Trettin;M. Tselengidou;C. Tung;A. Turcati;R. Turcotte;C. Turley;J. P. Twagirayezu;B. Ty;M. U. Elorrieta;N. Valtonen-Mattila;J. Vandenbroucke;N. Eijndhoven;D. Vannerom;J. Santen;J. Veitch-Michaelis;S. Verpoest;C. Walck;W. Wang;T. Watson;C. Weaver;P. Weigel;A. Weindl;M. Weiss;J. Weldert;C. Wendt;J. Werthebach;M. Weyrauch;N. Whitehorn;C. Wiebusch;N. Willey;D. R. Williams;M. Wolf;G. Wrede;J. Wulff;X. Xu;J. Yáñez;E. Yildizci;S. Yoshida;S. Yu;T. Yuan;Z. Zhang;P. Zhelnin
我们首次对 IceCube 进行的高质量和低质量 X 射线双星高能中微子发射进行全面搜索。银河X射线双星长期以来一直是银河强子宇宙射线和中微子源的候选者。这些系统中的致密物体可能是宇宙射线加速的场所，而中微子可以通过宇宙射线与辐射或气体的相互作用产生，在微类星体的喷流中、在恒星风中或在伴星的大气中。我们使用 7.5 年的 IceCube 数据和三个独立的分析来研究 X 射线双星。首先，我们搜索北方天空中 55 个轨道周期已知的双星的周期性中微子发射。在第二个例子中，整个天空中 102 个双星的 X 射线光变曲线被用作模板来搜索与时间相关的中微子发射。最后，我们搜索了 4 个被识别为微类星体的著名双星的中微子时间积分发射。在没有明显过量的情况下，我们对每个假设的中微子通量设定了上限，并将我们的结果与几个双星的理论预测进行比较。此外，我们还评估了位于南极的下一代中微子望远镜 IceCube-Gen2 的灵敏度，并展示了其识别银河系中这些二元源潜在中微子发射的能力。
We present the first comprehensive search for high-energy neutrino emission from high- and low-mass X-ray binaries conducted by IceCube. Galactic X-ray binaries are long-standing candidates for the source of Galactic hadronic cosmic rays and neutrinos. The compact object in these systems can be the site of cosmic-ray acceleration, and neutrinos can be produced by interactions of cosmic rays with radiation or gas, in the jet of a microquasar, in the stellar wind, or in the atmosphere of the companion star. We study X-ray binaries using 7.5 yr of IceCube data with three separate analyses. In the first, we search for periodic neutrino emission from 55 binaries in the Northern Sky with known orbital periods. In the second, the X-ray light curves of 102 binaries across the entire sky are used as templates to search for time-dependent neutrino emission. Finally, we search for time-integrated emission of neutrinos for a list of 4 notable binaries identified as microquasars. In the absence of a significant excess, we place upper limits on the neutrino flux for each hypothesis and compare our results with theoretical predictions for several binaries. In addition, we evaluate the sensitivity of the next generation neutrino telescope at the South Pole, IceCube-Gen2, and demonstrate its power to identify potential neutrino emission from these binary sources in the Galaxy.