Neutrino Vertex Reconstruction in South Pole Ice

Reconstruction of potential ultra-high-energy (UHE) neutrino events at the Askaryan Radio Array (ARA) is complicated by the variable index of refraction of South Pole ice, leading to curved radio signal paths from the interaction vertex. Using a spline table framework for fast raytracing approximati...
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Autor*in:	Beheler-Amass M. [verfasserIn] Karle A. [verfasserIn] Kelley J.L. [verfasserIn] Lu M.-Y. [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2019

Übergeordnetes Werk:	In: EPJ Web of Conferences - EDP Sciences, 2010, 216, p 02011(2019)
Übergeordnetes Werk:	volume:216, p 02011 ; year:2019

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DOI / URN:	10.1051/epjconf/201921602011

Katalog-ID:	DOAJ055691803

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allfieldsSound	10.1051/epjconf/201921602011 doi (DE-627)DOAJ055691803 (DE-599)DOAJ172f660ca35e4860ab1e7edc32660f98 DE-627 ger DE-627 rakwb eng QC1-999 Beheler-Amass M. verfasserin aut Neutrino Vertex Reconstruction in South Pole Ice 2019 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Reconstruction of potential ultra-high-energy (UHE) neutrino events at the Askaryan Radio Array (ARA) is complicated by the variable index of refraction of South Pole ice, leading to curved radio signal paths from the interaction vertex. Using a spline table framework for fast raytracing approximation, we perform a GPU-accelerated interferometric reconstruction of the event vertex. We also demonstrate how use of both direct and reflected/refracted radio signals can allow reconstruction of the distance to the interaction vertex, an important step towards neutrino energy reconstruction. Physics Karle A. verfasserin aut Kelley J.L. verfasserin aut Lu M.-Y. verfasserin aut In EPJ Web of Conferences EDP Sciences, 2010 216, p 02011(2019) (DE-627)647306611 (DE-600)2595425-8 2100014X nnns volume:216, p 02011 year:2019 https://doi.org/10.1051/epjconf/201921602011 kostenfrei https://doaj.org/article/172f660ca35e4860ab1e7edc32660f98 kostenfrei https://www.epj-conferences.org/articles/epjconf/pdf/2019/21/epjconf_arena2018_02011.pdf kostenfrei https://doaj.org/toc/2100-014X Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ SSG-OLC-PHA GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2111 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 216, p 02011 2019
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author	Beheler-Amass M.
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title	Neutrino Vertex Reconstruction in South Pole Ice
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title_full	Neutrino Vertex Reconstruction in South Pole Ice
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title_sort	neutrino vertex reconstruction in south pole ice
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title_auth	Neutrino Vertex Reconstruction in South Pole Ice
abstract	Reconstruction of potential ultra-high-energy (UHE) neutrino events at the Askaryan Radio Array (ARA) is complicated by the variable index of refraction of South Pole ice, leading to curved radio signal paths from the interaction vertex. Using a spline table framework for fast raytracing approximation, we perform a GPU-accelerated interferometric reconstruction of the event vertex. We also demonstrate how use of both direct and reflected/refracted radio signals can allow reconstruction of the distance to the interaction vertex, an important step towards neutrino energy reconstruction.
abstractGer	Reconstruction of potential ultra-high-energy (UHE) neutrino events at the Askaryan Radio Array (ARA) is complicated by the variable index of refraction of South Pole ice, leading to curved radio signal paths from the interaction vertex. Using a spline table framework for fast raytracing approximation, we perform a GPU-accelerated interferometric reconstruction of the event vertex. We also demonstrate how use of both direct and reflected/refracted radio signals can allow reconstruction of the distance to the interaction vertex, an important step towards neutrino energy reconstruction.
abstract_unstemmed	Reconstruction of potential ultra-high-energy (UHE) neutrino events at the Askaryan Radio Array (ARA) is complicated by the variable index of refraction of South Pole ice, leading to curved radio signal paths from the interaction vertex. Using a spline table framework for fast raytracing approximation, we perform a GPU-accelerated interferometric reconstruction of the event vertex. We also demonstrate how use of both direct and reflected/refracted radio signals can allow reconstruction of the distance to the interaction vertex, an important step towards neutrino energy reconstruction.
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title_short	Neutrino Vertex Reconstruction in South Pole Ice
url	https://doi.org/10.1051/epjconf/201921602011 https://doaj.org/article/172f660ca35e4860ab1e7edc32660f98 https://www.epj-conferences.org/articles/epjconf/pdf/2019/21/epjconf_arena2018_02011.pdf https://doaj.org/toc/2100-014X
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