Monte Carlo simulations for the ANTARES underwater neutrino telescope

Monte Carlo simulations for the ANTARES underwater neutrino telescope
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DOI：
10.1088/1475-7516/2021/01/064
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发表时间：
2020-10
期刊：
Journal of Cosmology and Astroparticle Physics
影响因子：
6.4
通讯作者：
T. A. C. A. Albert-T.-A.-C.-A.-Albert-1995163959;M. Andr'e;M. Anghinolfi;G. Anton;M. Ardid;J. Aubert;J. Aublin;B. Baret;S. Basa;B. Belhorma;V. Bertin;S. Biagi;M. Bissinger;J. Boumaaza;M. Bouta;M. Bouwhuis;H. Brânzaş;R. Bruijn;J. Brunner;J. Busto;A. Capone;L. Caramete;J. Carr;S. Cecchini;S. Celli;M. Chabab;T. N. Chau;R. Moursli;T. Chiarusi;M. Circella;A. Coleiro;M. Colomer-Molla;R. Coniglione;P. Coyle;A. Creusot;A. Díaz;G. Wasseige;A. Deschamps;C. Distefano;I. Palma;A. Domi;C. Donzaud;D. Dornic;D. Drouhin;T. Eberl;N. Khayati;A. Enzenhofer;A. Ettahiri;P. Fermani;G. Ferrara;F. Filippini;L. Fusco;P. Gay;H. Glotin;R. Gozzini;K. Graf;C. Guidi;S. Hallmann;H. Haren;A. Heijboer;Y. Hello;J. Hernández-Rey;J. Hossl;J. Hofestadt;F. Huang;G. Illuminati;C. James;M. Jong;P. Jong;M. Jongen;M. Kadler;O. Kalekin;U. Katz;N. R. Khan-Chowdhury;A. Kouchner;I. Kreykenbohm;V. Kulikovskiy;R. Lahmann;R. Breton;D. Lefèvre;E. Leonora;G. Levi;M. Lincetto;D. López-Coto;S. Loucatos;J. Mańczak;M. Marcelin;A. Margiotta;A. Marinelli;J. Martínez-Mora;S. Mazzou;K. Melis;P. Migliozzi;M. Moser;A. Moussa;R. Muller;L. Nauta;S. Navas;E. Nezri;A. Núñez-Castiñeyra;B. O’Fearraigh;Mukharbek Organokov;G. Pǎvǎlaş;C. Pellegrino;M. Perrin-Terrin;P. Piattelli;C. Poirè;V. Popa;T. Pradier;N. Randazzo;S. Reck;G. Riccobene;F. Salesa;A. Sánchez-Losa;D. Samtleben;M. Sanguineti;P. Sapienza;J. Schnabel;F. Schussler;M. Spurio;T. Stolarczyk;B. Strandberg;M. Taiuti;Y. Tayalati;T. Thakore;S. Tingay;B. Vallage;V. Elewyck;F. Versari;S. Viola;D. Vivolo;J. Wilms;A. Zegarelli;J. Zornoza;J. Zúñiga
T. A. C. A. Albert-T.-A.-C.-A.-Albert-1995163959;M. Andr'e;M. Anghinolfi;G. Anton;M. Ardid;J. Aubert;J. Aublin;B. Baret;S. Basa;B. Belhorma;V. Bertin;S. Biagi;M. Bissinger;J. Boumaaza;M. Bouta;M. Bouwhuis;H. Brânzaş;R. Bruijn;J. Brunner;J. Busto;A. Capone;L. Caramete;J. Carr;S. Cecchini;S. Celli;M. Chabab;T. N. Chau;R. Moursli;T. Chiarusi;M. Circella;A. Coleiro;M. Colomer-Molla;R. Coniglione;P. Coyle;A. Creusot;A. Díaz;G. Wasseige;A. Deschamps;C. Distefano;I. Palma;A. Domi;C. Donzaud;D. Dornic;D. Drouhin;T. Eberl;N. Khayati;A. Enzenhofer;A. Ettahiri;P. Fermani;G. Ferrara;F. Filippini;L. Fusco;P. Gay;H. Glotin;R. Gozzini;K. Graf;C. Guidi;S. Hallmann;H. Haren;A. Heijboer;Y. Hello;J. Hernández-Rey;J. Hossl;J. Hofestadt;F. Huang;G. Illuminati;C. James;M. Jong;P. Jong;M. Jongen;M. Kadler;O. Kalekin;U. Katz;N. R. Khan-Chowdhury;A. Kouchner;I. Kreykenbohm;V. Kulikovskiy;R. Lahmann;R. Breton;D. Lefèvre;E. Leonora;G. Levi;M. Lincetto;D. López-Coto;S. Loucatos;J. Mańczak;M. Marcelin;A. Margiotta;A. Marinelli;J. Martínez-Mora;S. Mazzou;K. Melis;P. Migliozzi;M. Moser;A. Moussa;R. Muller;L. Nauta;S. Navas;E. Nezri;A. Núñez-Castiñeyra;B. O’Fearraigh;Mukharbek Organokov;G. Pǎvǎlaş;C. Pellegrino;M. Perrin-Terrin;P. Piattelli;C. Poirè;V. Popa;T. Pradier;N. Randazzo;S. Reck;G. Riccobene;F. Salesa;A. Sánchez-Losa;D. Samtleben;M. Sanguineti;P. Sapienza;J. Schnabel;F. Schussler;M. Spurio;T. Stolarczyk;B. Strandberg;M. Taiuti;Y. Tayalati;T. Thakore;S. Tingay;B. Vallage;V. Elewyck;F. Versari;S. Viola;D. Vivolo;J. Wilms;A. Zegarelli;J. Zornoza;J. Zúñiga
中科院分区：
物理与天体物理2区
文献类型：
--
作者：
T. A. C. A. Albert-T.-A.-C.-A.-Albert-1995163959;M. Andr'e;M. Anghinolfi;G. Anton;M. Ardid;J. Aubert;J. Aublin;B. Baret;S. Basa;B. Belhorma;V. Bertin;S. Biagi;M. Bissinger;J. Boumaaza;M. Bouta;M. Bouwhuis;H. Brânzaş;R. Bruijn;J. Brunner;J. Busto;A. Capone;L. Caramete;J. Carr;S. Cecchini;S. Celli;M. Chabab;T. N. Chau;R. Moursli;T. Chiarusi;M. Circella;A. Coleiro;M. Colomer-Molla;R. Coniglione;P. Coyle;A. Creusot;A. Díaz;G. Wasseige;A. Deschamps;C. Distefano;I. Palma;A. Domi;C. Donzaud;D. Dornic;D. Drouhin;T. Eberl;N. Khayati;A. Enzenhofer;A. Ettahiri;P. Fermani;G. Ferrara;F. Filippini;L. Fusco;P. Gay;H. Glotin;R. Gozzini;K. Graf;C. Guidi;S. Hallmann;H. Haren;A. Heijboer;Y. Hello;J. Hernández-Rey;J. Hossl;J. Hofestadt;F. Huang;G. Illuminati;C. James;M. Jong;P. Jong;M. Jongen;M. Kadler;O. Kalekin;U. Katz;N. R. Khan-Chowdhury;A. Kouchner;I. Kreykenbohm;V. Kulikovskiy;R. Lahmann;R. Breton;D. Lefèvre;E. Leonora;G. Levi;M. Lincetto;D. López-Coto;S. Loucatos;J. Mańczak;M. Marcelin;A. Margiotta;A. Marinelli;J. Martínez-Mora;S. Mazzou;K. Melis;P. Migliozzi;M. Moser;A. Moussa;R. Muller;L. Nauta;S. Navas;E. Nezri;A. Núñez-Castiñeyra;B. O’Fearraigh;Mukharbek Organokov;G. Pǎvǎlaş;C. Pellegrino;M. Perrin-Terrin;P. Piattelli;C. Poirè;V. Popa;T. Pradier;N. Randazzo;S. Reck;G. Riccobene;F. Salesa;A. Sánchez-Losa;D. Samtleben;M. Sanguineti;P. Sapienza;J. Schnabel;F. Schussler;M. Spurio;T. Stolarczyk;B. Strandberg;M. Taiuti;Y. Tayalati;T. Thakore;S. Tingay;B. Vallage;V. Elewyck;F. Versari;S. Viola;D. Vivolo;J. Wilms;A. Zegarelli;J. Zornoza;J. Zúñiga

文献摘要

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蒙特卡罗模拟是检查探测器响应和监测其性能的独特工具。对于深海中微子望远镜，除了可靠地描述探测器的活动部分和物理事件的特征外，还必须考虑可能影响数据采集系统行为的环境条件的多变性，以便产生一组真实的模拟事件。本文描述了用于在望远镜中产生中微子和宇宙线信号的软件工具，以及为表示自然环境和探测器效率的时间演变而开发的策略。
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