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Development of a sub-glacial radio telescope for the detection of GZK neutrinos[electronic resource] /

紀錄類型:	書目-電子資源 : Monograph/item
杜威分類號:	522.682
書名/作者:	Development of a sub-glacial radio telescope for the detection of GZK neutrinos/ by Thomas Meures.
作者:	Meures, Thomas.
出版者:	Cham : : Springer International Publishing :, 2015.
面頁冊數:	xiii, 159 p. : : ill., digital ;; 24 cm.
標題:
ISBN:	9783319187563 (electronic bk.)
ISBN:	9783319187556 (paper)
內容註:	Introduction -- The GZK Neutrino Flux -- The Askaryan Effect in Dense Media -- The Askaryan Radio Array (ARA) -- The Calibration of the Ice Ray Sampler (IRS2) Chip -- The Calibration of the ARA Station Geometry -- Simulations -- Algorithms for the ARA Data Analysis -- Signal Discrimination in the ARA02-ARA03 Data -- Data Analysis Results -- Summary and Outlook.
摘要、提要註:	?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.#

Development of a sub-glacial radio telescope for the detection of GZK neutrinos[electronic resource] /
Meures, Thomas.

Development of a sub-glacial radio telescope for the detection of GZK neutrinos[electronic resource] /by Thomas Meures. - Cham :Springer International Publishing :2015. - xiii, 159 p. :ill., digital ;24 cm. - Springer theses,2190-5053.

Introduction -- The GZK Neutrino Flux -- The Askaryan Effect in Dense Media -- The Askaryan Radio Array (ARA) -- The Calibration of the Ice Ray Sampler (IRS2) Chip -- The Calibration of the ARA Station Geometry -- Simulations -- Algorithms for the ARA Data Analysis -- Signal Discrimination in the ARA02-ARA03 Data -- Data Analysis Results -- Summary and Outlook.

?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.#

ISBN: 9783319187563 (electronic bk.)

Standard No.: 10.1007/978-3-319-18756-3doiSubjects--Topical Terms:

353965

LC Class. No.: QB479.2

Dewey Class. No.: 522.682

Development of a sub-glacial radio telescope for the detection of GZK neutrinos[electronic resource] /
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