Prospects for high-elevation radio detection of >100 PeV tau neutrinos
Prospects for high-elevation radio detection of >100 PeV tau neutrinos
复制标题
>100 PeV tau 中微子高空无线电探测的前景
DOI：
--
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发表时间：
2020
影响因子：
6.4
通讯作者：
A. Vieregg
中科院分区：
文献类型：
--
作者：
S. Wissel;A. Romero;H. Schoorlemmer;W. R. Jr.;J. Alvarez;E. Zas;A. Cummings;C. Deaconu;K. Hughes;A. Ludwig;Joalda Morancy;E. Oberla;C. Paciaroni;S. Prohira;D. Southall;Max Stapel;B. Strutt;Mercedes Vasquez;A. Vieregg
预计 Tau 中微子约占天体物理和宇宙成因中微子通量的三分之一，但目前风味比例受到的限制很差，并且能量高于 1017 eV 时的预期通量较低。我们提出了一种探测器概念，旨在通过使用无线电技术的高海拔山顶探测器来测量该能量范围内的 tau 中微子的扩散通量。该探测器搜索由掠地 tau 中微子产生的上升空气簇射的无线电信号。来自紧凑阵列中的多个天线的信号在触发电平上相干求和，不仅允许人为背景的定向屏蔽，而且允许较低的触发阈值。这种设计既利用了高海拔地点的大可视区域，又利用了无线电仪器几乎完整的占空比。我们提出权衡研究，考虑站高程、频段、阵列中天线的数量以及触发阈值，以开发高效的站设计。与具有 100 个独立站的现有仪器相比，这种山顶探测器的接受度可以提高十倍。通过 1000 个站和三年的观测，它可以实现对 <10−9 GeV cm−2 sr−1 s−1 的积分 ℰ−2 通量的灵敏度，在假设纯铁宇宙线成分的全味宇宙中微子的预期通量范围内。
Tau neutrinos are expected to comprise roughly one third of both the astrophysical and cosmogenic neutrino flux, but currently the flavor ratio is poorly constrained and the expected flux at energies above 1017 eV is low. We present a detector concept aimed at measuring the diffuse flux of tau neutrinos in this energy range via a high-elevation mountaintop detector using the radio technique. The detector searches for radio signals from upgoing air showers generated by Earth-skimming tau neutrinos. Signals from several antennas in a compact array are coherently summed at the trigger level, permitting not only directional masking of anthropogenic backgrounds, but also a low trigger threshold. This design takes advantage of both the large viewing area available at high-elevation sites and the nearly full duty cycle available to radio instruments. We present trade studies that consider the station elevation, frequency band, number of antennas in the array, and the trigger threshold to develop a highly efficient station design. Such a mountaintop detector can achieve a factor of ten improvement in acceptance over existing instruments with 100 independent stations. With 1000 stations and three years of observation, it can achieve a sensitivity to an integrated ℰ−2 flux of <10−9 GeV cm−2 sr−1 s−1, in the range of the expected flux of all-flavor cosmogenic neutrinos assuming a pure iron cosmic-ray composition.
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影响因子：
8.6
作者：
Aab, A.;Abreu, P.;Zuccarello, F.
通讯作者：
Zuccarello, F.
DOI：
10.22323/1.358.1036
发表时间：
2019-07
期刊：
Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)
影响因子：
--
作者：
L. Wille;Donglian Xu
通讯作者：
L. Wille;Donglian Xu
通过 ARIANNA 实验瞄准超高能中微子
影响因子：
2.6
作者：
ARIANNA collaboration (…;C. Glaser)
通讯作者：
C. Glaser)
DOI：
10.1016/j.nima.2019.163086
发表时间：
2019-07
期刊：
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
影响因子：
--
作者：
R. Monroe;A. Wolf;G. Hallinan;A. Nelles;M. Eastwood;M. Anderson;L. D'Addario;J. Kocz;Yuankun Wang;Devin Cody;D. Woody;F. Schinzel;G. Taylor;L. Greenhill;Daniel J. Price
通讯作者：
R. Monroe;A. Wolf;G. Hallinan;A. Nelles;M. Eastwood;M. Anderson;L. D'Addario;J. Kocz;Yuankun Wang;Devin Cody;D. Woody;F. Schinzel;G. Taylor;L. Greenhill;Daniel J. Price
DOI：
10.3847/1538-4357/ab791d
发表时间：
2019-08
期刊：
The Astrophysical Journal
影响因子：
--
作者：
M. Aartsen;M. Ackermann;J. Adams;J. Aguilar;M. Ahlers;M. Ahrens;C. Alispach;K. Andeen;T. Anderson;I. Ansseau;G. Anton;C. Argüelles;J. Auffenberg;S. Axani;P. Backes;H. Bagherpour;X. Bai;A. B. V.;A. Barbano;S. Barwick;B. Bastian;V. Baum;S. Baur;R. Bay;J. Beatty;K. Becker;J. Tjus;S. BenZvi;D. Berley;E. Bernardini;D. Besson;G. Binder;D. Bindig;E. Blaufuss;S. Blot;C. Bohm;S. Böser;O. Botner;J. Böttcher;E. Bourbeau;J. Bourbeau;F. Bradascio;J. Braun;S. Bron;J. Brostean-Kaiser;A. Burgman;J. Buscher;R. Busse;T. Carver;C. Chen;E. Cheung;D. Chirkin;S. Choi;K. Clark;L. Classen;A. Coleman;G. Collin;J. Conrad;P. Coppin;P. Correa;D. Cowen;R. Cross;P. Dave;C. Clercq;J. DeLaunay;H. Dembinski;K. Deoskar;S. Ridder;P. Desiati;K. D. Vries;G. Wasseige;M. With;T. DeYoung;A. Diaz;J. C. Díaz-Vélez;H. Dujmovic;M. Dunkman;E. Dvorak;B. Eberhardt;T. Ehrhardt;P. Eller;R. Engel;P. Evenson;S. Fahey;A. Fazely;J. Felde;K. Filimonov;C. Finley;D. Fox;A. Franckowiak;E. Friedman;A. Fritz;T. Gaisser;J. Gallagher;E. Ganster;S. Garrappa;L. Gerhardt;K. Ghorbani;T. Glauch;T. Glüsenkamp;A. Goldschmidt;J. G. Gonzalez;D. Grant;Z. Griffith;S. Griswold;M. Günder;M. Gündüz;C. Haack;A. Hallgren;R. Halliday;L. Halve;F. Halzen;K. Hanson;A. Haungs;D. Hebecker;D. Heereman;P. Heix;K. Helbing;R. Hellauer;F. Henningsen;S. Hickford;J. Hignight;G. Hill;K. Hoffman;R. Hoffmann;T. Hoinka;B. Hokanson-Fasig;K. Hoshina;F. Huang;M. Huber;T. Huber;K. Hultqvist;Mirco Hünnefeld;R. Hussain;S. In;N. Iovine;A. Ishihara;G. Japaridze;M. Jeong;K. Jero;B. Jones;F. Jonske;R. Joppe;D. Kang;W. Kang;A. Kappes;D. Kappesser;T. Karg;M. Karl;A. Karle;U. Katz;M. Kauer;J. Kelley;A. Kheirandish;J. Kim;T. Kintscher;J. Kiryluk;T. Kittler;S. Klein;R. Koirala;H. Kolanoski;L. Köpke;C. Kopper;S. Kopper;D. Koskinen;M. Kowalski;K. Krings;G. Krückl;N. Kulacz;N. Kurahashi;A. Kyriacou;J. Lanfranchi;M. Larson;F. Lauber;J. Lazar;K. Leonard;A. Leszczyńska;M. Leuermann;Q. Liu;E. Lohfink;C. J. L. Mariscal;L. Lu;F. Lucarelli;J. Lünemann;W. Luszczak;Y. Lyu;W. Ma;J. Madsen;G. Maggi;K. Mahn;Y. Makino;P. Mallik;K. Mallot;S. Mancina;I. Mariş;R. Maruyama;K. Mase;R. Maunu;F. McNally;K. Meagher;M. Medici;A. Medina;M. Meier;S. Meighen-Berger;G. Merino;T. Meures;J. Micallef;D. Mockler;G. Momenté;T. Montaruli;R. W. Moore;R. Morse;M. Moulai;P. Muth;R. Nagai;U. Naumann;G. Neer;H. Niederhausen;M. Nisa;S. Nowicki;D. Nygren;A. Pollmann;M. Oehler;A. Olivas;A. O'Murchadha;E. O’Sullivan;T. Palczewski;H. Pandya;D. Pankova;N. Park;P. Peiffer;C. P. de los Heros;S. Philippen;D. Pieloth;E. Pinat;A. Pizzuto;M. Plum;A. Porcelli;P. Price;G. Przybylski;C. Raab;A. Raissi;M. Rameez;L. Rauch;K. Rawlins;I. C. Rea;R. Reimann;B. Relethford;M. Renschler;G. Renzi;E. Resconi;W. Rhode;M. Richman;S. Robertson;M. Rongen;C. Rott;T. Ruhe;D. Ryckbosch;D. Rysewyk;I. Safa;S. Herrera;A. Sandrock;J. Sandroos;M. Santander;S. Sarkar;K. Satalecka;M. Schaufel;H. Schieler;P. Schlunder;T. Schmidt;A. Schneider;J. Schneider;F. Schröder;L. Schumacher;S. Sclafani;S. Seunarine;S. Shefali;M. Silva;R. Snihur;J. Soedingrekso;D. Soldin;M. Song;G. Spiczak;C. Spiering;J. Stachurska;M. Stamatikos;T. Stanev;R. Stein;J. Stettner;A. Steuer;T. Stezelberger;R. Stokstad;A. Stößl;N. Strotjohann;T. Stürwald;T. Stuttard;G. Sullivan;I. Taboada;F. Tenholt;S. Ter-Antonyan;A. Terliuk;S. Tilav;K. Tollefson;L. Tomankova;C. Tönnis;S. Toscano;D. Tosi;A. Trettin;M. Tselengidou;C. Tung;A. Turcati;R. Turcotte;C. Turley;B. Ty;E. Unger;M. U. Elorrieta;M. Usner;J. Vandenbroucke;W. van Driessche;D. van Eijk;N. van Eijndhoven;J. van Santen;S. Verpoest;M. Vraeghe;C. Walck;A. Wallace;M. Wallraff;N. Wandkowsky;T. B. Watson;C. Weaver;A. Weindl;M. Weiss;J. Weldert;C. Wendt;J. Werthebach;B. Whelan;N. Whitehorn;K. Wiebe;C. Wiebusch;L. Wille;D. Williams;L. Wills;M. Wolf;J. Wood;T. R. Wood;K. Woschnagg;G. Wrede;D. Xu;X. Xu;Y. Xu;J. Yáñez;G. Yodh;S. Yoshida;T. Yuan;M. Zöcklein
通讯作者：
M. Aartsen;M. Ackermann;J. Adams;J. Aguilar;M. Ahlers;M. Ahrens;C. Alispach;K. Andeen;T. Anderson;I. Ansseau;G. Anton;C. Argüelles;J. Auffenberg;S. Axani;P. Backes;H. Bagherpour;X. Bai;A. B. V.;A. Barbano;S. Barwick;B. Bastian;V. Baum;S. Baur;R. Bay;J. Beatty;K. Becker;J. Tjus;S. BenZvi;D. Berley;E. Bernardini;D. Besson;G. Binder;D. Bindig;E. Blaufuss;S. Blot;C. Bohm;S. Böser;O. Botner;J. Böttcher;E. Bourbeau;J. Bourbeau;F. Bradascio;J. Braun;S. Bron;J. Brostean-Kaiser;A. Burgman;J. Buscher;R. Busse;T. Carver;C. Chen;E. Cheung;D. Chirkin;S. Choi;K. Clark;L. Classen;A. Coleman;G. Collin;J. Conrad;P. Coppin;P. Correa;D. Cowen;R. Cross;P. Dave;C. Clercq;J. DeLaunay;H. Dembinski;K. Deoskar;S. Ridder;P. Desiati;K. D. Vries;G. Wasseige;M. With;T. DeYoung;A. Diaz;J. C. Díaz-Vélez;H. Dujmovic;M. Dunkman;E. Dvorak;B. Eberhardt;T. Ehrhardt;P. Eller;R. Engel;P. Evenson;S. Fahey;A. Fazely;J. Felde;K. Filimonov;C. Finley;D. Fox;A. Franckowiak;E. Friedman;A. Fritz;T. Gaisser;J. Gallagher;E. Ganster;S. Garrappa;L. Gerhardt;K. Ghorbani;T. Glauch;T. Glüsenkamp;A. Goldschmidt;J. G. Gonzalez;D. Grant;Z. Griffith;S. Griswold;M. Günder;M. Gündüz;C. Haack;A. Hallgren;R. Halliday;L. Halve;F. Halzen;K. Hanson;A. Haungs;D. Hebecker;D. Heereman;P. Heix;K. Helbing;R. Hellauer;F. Henningsen;S. Hickford;J. Hignight;G. Hill;K. Hoffman;R. Hoffmann;T. Hoinka;B. Hokanson-Fasig;K. Hoshina;F. Huang;M. Huber;T. Huber;K. Hultqvist;Mirco Hünnefeld;R. Hussain;S. In;N. Iovine;A. Ishihara;G. Japaridze;M. Jeong;K. Jero;B. Jones;F. Jonske;R. Joppe;D. Kang;W. Kang;A. Kappes;D. Kappesser;T. Karg;M. Karl;A. Karle;U. Katz;M. Kauer;J. Kelley;A. Kheirandish;J. Kim;T. Kintscher;J. Kiryluk;T. Kittler;S. Klein;R. Koirala;H. Kolanoski;L. Köpke;C. Kopper;S. Kopper;D. Koskinen;M. Kowalski;K. Krings;G. Krückl;N. Kulacz;N. Kurahashi;A. Kyriacou;J. Lanfranchi;M. Larson;F. Lauber;J. Lazar;K. Leonard;A. Leszczyńska;M. Leuermann;Q. Liu;E. Lohfink;C. J. L. Mariscal;L. Lu;F. Lucarelli;J. Lünemann;W. Luszczak;Y. Lyu;W. Ma;J. Madsen;G. Maggi;K. Mahn;Y. Makino;P. Mallik;K. Mallot;S. Mancina;I. Mariş;R. Maruyama;K. Mase;R. Maunu;F. McNally;K. Meagher;M. Medici;A. Medina;M. Meier;S. Meighen-Berger;G. Merino;T. Meures;J. Micallef;D. Mockler;G. Momenté;T. Montaruli;R. W. Moore;R. Morse;M. Moulai;P. Muth;R. Nagai;U. Naumann;G. Neer;H. Niederhausen;M. Nisa;S. Nowicki;D. Nygren;A. Pollmann;M. Oehler;A. Olivas;A. O'Murchadha;E. O’Sullivan;T. Palczewski;H. Pandya;D. Pankova;N. Park;P. Peiffer;C. P. de los Heros;S. Philippen;D. Pieloth;E. Pinat;A. Pizzuto;M. Plum;A. Porcelli;P. Price;G. Przybylski;C. Raab;A. Raissi;M. Rameez;L. Rauch;K. Rawlins;I. C. Rea;R. Reimann;B. Relethford;M. Renschler;G. Renzi;E. Resconi;W. Rhode;M. Richman;S. Robertson;M. Rongen;C. Rott;T. Ruhe;D. Ryckbosch;D. Rysewyk;I. Safa;S. Herrera;A. Sandrock;J. Sandroos;M. Santander;S. Sarkar;K. Satalecka;M. Schaufel;H. Schieler;P. Schlunder;T. Schmidt;A. Schneider;J. Schneider;F. Schröder;L. Schumacher;S. Sclafani;S. Seunarine;S. Shefali;M. Silva;R. Snihur;J. Soedingrekso;D. Soldin;M. Song;G. Spiczak;C. Spiering;J. Stachurska;M. Stamatikos;T. Stanev;R. Stein;J. Stettner;A. Steuer;T. Stezelberger;R. Stokstad;A. Stößl;N. Strotjohann;T. Stürwald;T. Stuttard;G. Sullivan;I. Taboada;F. Tenholt;S. Ter-Antonyan;A. Terliuk;S. Tilav;K. Tollefson;L. Tomankova;C. Tönnis;S. Toscano;D. Tosi;A. Trettin;M. Tselengidou;C. Tung;A. Turcati;R. Turcotte;C. Turley;B. Ty;E. Unger;M. U. Elorrieta;M. Usner;J. Vandenbroucke;W. van Driessche;D. van Eijk;N. van Eijndhoven;J. van Santen;S. Verpoest;M. Vraeghe;C. Walck;A. Wallace;M. Wallraff;N. Wandkowsky;T. B. Watson;C. Weaver;A. Weindl;M. Weiss;J. Weldert;C. Wendt;J. Werthebach;B. Whelan;N. Whitehorn;K. Wiebe;C. Wiebusch;L. Wille;D. Williams;L. Wills;M. Wolf;J. Wood;T. R. Wood;K. Woschnagg;G. Wrede;D. Xu;X. Xu;Y. Xu;J. Yáñez;G. Yodh;S. Yoshida;T. Yuan;M. Zöcklein