東華大學圖書館 |

Language: English

Help

回圖書館首頁

手機版館藏查詢

Back

Switch To: Labeled | MARC Mode | ISBD

Development of a sub-glacial radio t...

Meures, Thomas.

Linked to FindBook

Google Book

Amazon

博客來

Development of a sub-glacial radio telescope for the detection of GZK neutrinos

Record Type:	Electronic resources : Monograph/item
Title/Author:	Development of a sub-glacial radio telescope for the detection of GZK neutrinos/ by Thomas Meures.
Author:	Meures, Thomas.
Published:	Cham :Springer International Publishing : : 2015.,
Description:	xiii, 159 p. :ill., digital ;24 cm.
[NT 15003449]:	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.
Contained By:	Springer eBooks
Subject:	Radio telescopes - Design and construction. -
Online resource:	http://dx.doi.org/10.1007/978-3-319-18756-3
ISBN:	9783319187563 (electronic bk.)

Development of a sub-glacial radio telescope for the detection of GZK neutrinos
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. - Springer theses..

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:

2153664
Radio telescopes
--Design and construction.

LC Class. No.: QB479.2

Dewey Class. No.: 522.682

Development of a sub-glacial radio telescope for the detection of GZK neutrinos
LDR:02215nmm a2200325 a 4500 001 2006615
003 DE-He213
005 20160107135914.0
006 m d
007 cr nn 008maaau
008 160114s2015 gw s 0 eng d
020 $a 9783319187563 (electronic bk.)
020 $a 9783319187556 (paper)
024 7 $a 10.1007/978-3-319-18756-3 $2 doi
035 $a 978-3-319-18756-3
040 $a GP $c GP
041 0 $a eng
050 4 $a QB479.2
072 7 $a PHP $2 bicssc
072 7 $a SCI051000 $2 bisacsh
082 0 4 $a 522.682 $2 23
090 $a QB479.2 $b .M598 2015
100 1 $a Meures, Thomas. $3 2153663
245 1 0 $a Development of a sub-glacial radio telescope for the detection of GZK neutrinos $h [electronic resource] / $c by Thomas Meures.
260 $a Cham : $b Springer International Publishing : $b Imprint: Springer, $c 2015.
300 $a xiii, 159 p. : $b ill., digital ; $c 24 cm.
490 1 $a Springer theses, $x 2190-5053
505 0 $a 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.
520 $a 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.
650 0 $a Radio telescopes $x Design and construction. $3 2153664
650 0 $a Cosmic rays. $3 836138
650 1 4 $a Physics. $3 516296
650 2 4 $a Particle Acceleration and Detection, Beam Physics. $3 893987
650 2 4 $a Astrophysics and Astroparticles. $3 1067087
650 2 4 $a Measurement Science and Instrumentation. $3 1066390
710 2 $a SpringerLink (Online service) $3 836513
773 0 $t Springer eBooks
830 0 $a Springer theses. $3 1314442
856 4 0 $u http://dx.doi.org/10.1007/978-3-319-18756-3
950 $a Physics and Astronomy (Springer-11651)