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Development of a Sub-Glacial Radio Telescope for the Detection of Gzk Neutrinos (2015)

Development of a Sub-glacial Radio Telescope for the Detection of GZK Neutrinos

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"Development of a Sub-glacial Radio Telescope for the Detection of GZK Neutrinos" by Thomas Meures is a astronomy book and space science reference focused on Deep Sky & Solar System. Best for students, researchers, and serious astronomy enthusiasts.

The goal of the project presented in this book is to detect neutrinos created by resonant interactions of ultrahigh energy cosmic rays on the CMB photon field filling the Universe. In this pioneering first analysis, the author puts forward much of the analysis framework, including calibrations of the electronic hardware and antenna geometry, as well as the development of algorithms for event reconstruction and data reduction. While only two of the 37 stations planned for the Askaryan Radio Array were used in this assessment of 10 months of data, the analysis was able to exclude neutrino fluxes above 10 PeV with a limit not far from the best current limit set by the IceCube detector, a result which establishes the radio detection technique as the path forward to achieving the massive volumes needed to detect these ultrahigh energy neutrinos.

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Best For: Researchers and students in astrophysics and nuclear physics focusing on neutrino detection.
Focus: Development and calibration of a sub-glacial radio telescope system to detect ultrahigh energy neutrinos.
Covers: Electronic hardware calibration, antenna geometry, event reconstruction algorithms, and data reduction techniques.
Why It Matters: Provides foundational analysis and methodology for detecting GZK neutrinos, contributing to understanding cosmic ray interactions with the cosmic microwave background.

"Development of a Sub-glacial Radio Telescope for the Detection of GZK Neutrinos" by Thomas Meures is a astronomy book and space science reference focused on Deep Sky & Solar System. Best for students, researchers, and serious astronomy enthusiasts.

Topic: Deep Sky & Solar System

Author: Thomas Meures

Who this is for:

  • Astronomy students
  • Researchers and advanced hobbyists
  • Readers exploring space science topics

Why this book matters: It matters because it helps readers build a stronger understanding of astronomy concepts, observations, and scientific ideas related to space.

The goal of the project presented in this book is to detect neutrinos created by resonant interactions of ultrahigh energy cosmic rays on the CMB photon field filling the Universe. In this pioneering first analysis, the author puts forward much of the analysis framework, including calibrations of the electronic hardware and antenna geometry, as well as the development of algorithms for event reconstruction and data reduction. While only two of the 37 stations planned for the Askaryan Radio Array were used in this assessment of 10 months of data, the analysis was able to exclude neutrino fluxes above 10 PeV with a limit not far from the best current limit set by the IceCube detector, a result which establishes the radio detection technique as the path forward to achieving the massive volumes needed to detect these ultrahigh energy neutrinos.

AuthorThomas Meures
PublisherSpringer
Published2015-06-12
ISBN-139783319187556
BindingHardcover
LanguageEnglish
SubjectsScience
TopicDeep Sky & Solar System
SeriesSpringer Theses

Format: Hardcover

Language: English

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