Combined Search for UHE Neutrinos from Binary Black Hole Mergers with the Pierre Auger Observatory
Combined Search for UHE Neutrinos from Binary Black Hole Mergers with the Pierre Auger Observatory
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与皮埃尔·俄歇天文台联合搜索双黑洞合并中的 UHE 中微子
DOI：
10.22323/1.395.0968
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发表时间：
2021
期刊：
影响因子：
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通讯作者：
L. Zehrer
中科院分区：
文献类型：
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作者：
M. Schimp;P. Abreu;M. Aglietta;J. Albury;I. Allekotte;A. Almela;J. Alvarez;R. A. Batista;G. A. Anastasi;L. Anchordoqui;B. Andrada;S. Andringa;C. Aramo;P. Ferreira;J. Velazquez;Hernán Asorey;P. Assis;G. Avila;A. Badescu;A. Bakalová;A. Bălăceanu;F. Barbato;R. Luz;K. Becker;J. Bellido;C. Bérat;M. Bertaina;X. Bertou;P. Biermann;V. Binet;K. Bismark;T. Bister;J. Biteau;J. Blažek;C. Bleve;M. Boháčová;D. Boncioli;C. Bonifazi;L. Arbeletche;N. Borodai;A. Botti;J. Brack;T. Bretz;P. G. B. Orchera;F. Briechle;P. Buchholz;A. Bueno;S. Buitink;M. Buscemi;M. Büsken;K. Caballero;L. Caccianiga;F. Canfora;I. Caracas;J. Carceller;R. Caruso;A. Castellina;F. Catalani;G. Cataldi;L. Cazon;M. Cerda;J. Chinellato;J. Chudoba;L. Chytka;R. Clay;A. Cerutti;R. Colalillo;Alan Coleman;M. Coluccia;R. Conceição;A. Condorelli;G. Consolati;F. Contreras;F. Convenga;D. D. Santos;C. Covault;S. Dasso;K. Daumiller;B. Dawson;J. A. Day;R. M. Almeida;J. D. Jesús;S. D. Jong;G. D. Mauro;J. D. M. Neto;I. Mitri;J. D. Oliveira;D. Franco;F. Palma;V. Souza;E. D. Vito;M. Río;O. Deligny;L. Deval;A. Matteo;C. Dobrigkeit;J. D'Olivo;L. M. Mendes;R. Anjos;D. D. Santos;M. Dova;J. Ebr;R. Engel;I. Epicoco;M. Erdmann;C. Escobar;A. Etchegoyen;H. Falcke;J. Farmer;G. Farrar;A. Fauth;N. Fazzini;F. Feldbusch;F. Fenu;B. Fick;J. M. Figueira;A. Filipčič;T. Fitoussi;T. Fodran;M. Freire;T. Fujii;A. Fuster;C. Galea;C. Galelli;B. Garcia;A. Vegas;H. Gemmeke;F. Gesualdi;A. Gherghel;P. Ghia;U. Giaccari;M. Giammarchi;J. Glombitza;F. Gobbi;F. Gollan;G. Golup;M. G. Berisso;P. Vitale;J. P. Gongora;Juan M. Gonzalez;N. González;I. Goos;D. Góra;A. Gorgi;M. Gottowik;T. D. Grubb;F. Guarino;G. Guedes;E. Guido;S. Hahn;P. Hamal;M. Hampel;P. Hansen;D. Harari;V. M. Harvey;A. Haungs;T. Hebbeker;D. Heck;G. Hill;C. Hojvat;J. Hörandel;P. Horváth;M. Hrabovsky;T. Huege;A. Insolia;P. G. Isar;P. Janeček;J. Johnsen;J. Juryšek;A. Kääpä;K. Kampert;N. Karastathis;B. Keilhauer;J. Kemp;A. Khakurdikar;V. Covilakam;H. Klages;M. Kleifges;J. Kleinfeller;M. Köpke;N. Kunka;B. Lago;R. Lang;N. Langner;M. D. Oliveira;V. Lenok;A. Letessier;I. Lhenry;D. L. Presti;Luís Lopes;R. Lopez;Lu Lu;Q. Luce;J. Lundquist;A. Payeras;G. Mancarella;D. Mandát;B. Manning;J. Manshanden;P. Mantsch;S. Marafico;A. Mariazzi;I. Mariş;G. Marsella;D. Martello;S. Martinelli;O. M. Bravo;M. Mastrodicasa;H. Mathes;J. Matthews;G. Matthiae;E. Mayotte;P. Mazur;G. Medina;D. Melo;A. Menshikov;K. Merenda;S. Michal;M. Micheletti;L. Miramonti;S. Mollerach;F. Montanet;C. Morello;M. Mostafá;A. Müller;M. Muller;K. Mulrey;R. Mussa;M. Muzio;W. M. Namasaka;A. Nasr;L. Nellen;M. Niculescu;M. Niechciol;D. Nitz;D. Nosek;V. Novotny;L. Nožka;A. Nucita;L. Núñez;M. Palatka;J. Pallotta;P. Papenbreer;G. Parente;A. Parra;J. Pawlowsky;M. Pech;F. Pedreira;J. Pȩkala;R. Pelayo;J. Peña;E. Martins;J. P. Armand;C. Bertolli;M. Perlin;L. Perrone;S. Petrera;T. Pierog;M. Pimenta;V. Pirronello;M. Platino;B. Pont;M. Pothast;P. Privitera;M. Prouza;A. Puyleart;S. Querchfeld;J. Rautenberg;D. Ravignani;M. Reininghaus;J. Řídký;F. Riehn;M. Risse;V. Rizi;W. Carvalho;J. Rojo;M. Roncoroni;S. Rossoni;M. Roth;E. Roulet;A. Rovero;P. Ruehl;A. Săftoiu;F. Salamida;H. Salazar;G. Salina;J. S. Gomez;F. Sánchez;E. Santos;E. Santos;F. Sarazin;R. Sarmento;C. Sarmiento;R. Sato;P. Savina;C. Schäfer;V. Scherini;H. Schieler;M. Schimassek;F. Schlüter;D. Schmidt;O. Scholten;P. Schovánek;F. Schröder;S. Schröder;J. Schulte;S. Sciutto;M. Scornavacche;A. Segreto;S. Sehgal;R. Shellard;G. Sigl;G. Silli;O. Sima;R. Smida;P. Sommers;J. F. Soriano;J. Souchard;R. Squartini;M. Stadelmaier;D. Stanca;S. Stanič;J. Stasielak;P. Stassi;A. Streich;M. Suárez;T. Sudholz;T. Suomijarvi;A. Supanitsky;Z. Szadkowski;A. Tapia;C. Taricco;C. Timmermans;O. Tkachenko;P. Tobiška;C. T. Peixoto;B. Tomé;Z. Torrès;A. Travaini;P. Trávníček;C. Trimarelli;M. Tueros;R. Ulrich;M. Unger;L. Václavek;M. Vacula;J. F. V. Galicia;L. Valore;E. Varela;A. Vásquez;D. Veberič;C. Ventura;I. D. V. Quispe;V. Verzi;J. Vícha;J. Vink;S. Vorobiov;H. Wahlberg;C. Watanabe;A. Watson;M. Weber;A. Weindl;L. Wiencke;H. Wilczynski;M. Wirtz;D. Wittkowski;B. Wundheiler;A. Yushkov;O. Zapparrata;E. Zas;D. Zavrtanik;M. Zavrtanik;L. Zehrer
我们与皮埃尔·奥格天文台一起探索超高能 (UHE) 中微子 (> 0 . 1 EeV)，跟踪 LIGO 和 Virgo 探测器通过引力波 (GW) 检测到的双黑洞 (BBH) 合并。在这项工作中，迄今为止发表的 BBH 合并被组合为标准蜡烛与假设的各向同性 UHE 中微子光度？ ( ? − ? 0 ) 作为各自合并后时间的函数， ? - ? 0 .假设 UHE 中微子发射光谱遵循幂律分布 ∝ ? - 2 ? 。使用这些假设， ? ( ? − ? 0 ) 被探测，考虑到皮埃尔俄歇天文台对 UHE 中微子的瞬时有效面积和源的 3D 天空定位。尚未发现 UHE 中微子候选者，上限为 ? ( ? − ? 0 ) 分别是在合并后持续 24 小时和 60 天的假设排放情况下获得的。 UHE中微子每个源发射的总能量的相应上限并不取决于发射持续时间，这证明了皮埃尔俄歇天文台拥有专用中微子望远镜的竞争力。
We present searches for ultra-high energy (UHE) neutrinos ( > 0 . 1 EeV) with the Pierre Auger Observatory, following up binary black hole (BBH) mergers detected by the LIGO and Virgo detectors via gravitational waves (GWs). In this work, the so-far published BBH mergers are combined as standard candles with a hypothetical isotropic UHE neutrino luminosity ? ( ? − ? 0 ) as a function of the time after the respective merger, ? − ? 0 . The UHE neutrino emission spectrum is assumed to follow a power law distribution ∝ ? − 2 ? . Using these assumptions, ? ( ? − ? 0 ) is probed, taking into account the instantaneous effective area of the Pierre Auger Observatory to UHE neutrinos and the 3D sky localizations of the sources. No UHE neutrino candidates have been found and upper limits on ? ( ? − ? 0 ) are obtained for the hypothetical cases of emissions lasting 24 hours and 60 days after the merger, respectively. The corresponding upper limit on the total energy per source emitted in UHE neutrinos does not depend on the emission duration and demonstrates the competitiveness of the Pierre Auger Observatory with dedicated neutrino telescopes.