Sie sind bereits eingeloggt. Klicken Sie auf 2. tolino select Abo, um fortzufahren.
Bitte loggen Sie sich zunächst in Ihr Kundenkonto ein oder registrieren Sie sich bei bücher.de, um das eBook-Abo tolino select nutzen zu können.
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…mehr
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.
Thomas Meures earned his Diploma in physics at the RWTH-Aachen University in 2010 with a thesis about the reciprocity calibration of acoustic hydrophones in water and ice, written under the supervision of Prof. Dr. Christopher Wiebusch. For his PhD studies he moved from acoustic research to radio neutrino detection at the Université libre de Bruxelles with Prof. Dr. Kael Hanson. Currently he is working on new developments of electronics for astroparticle physics experiments at the University of Wisconsin.
Inhaltsangabe
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.
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.
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.
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.
Es gelten unsere Allgemeinen Geschäftsbedingungen: www.buecher.de/agb
Impressum
www.buecher.de ist ein Internetauftritt der buecher.de internetstores GmbH
Geschäftsführung: Monica Sawhney | Roland Kölbl | Günter Hilger
Sitz der Gesellschaft: Batheyer Straße 115 - 117, 58099 Hagen
Postanschrift: Bürgermeister-Wegele-Str. 12, 86167 Augsburg
Amtsgericht Hagen HRB 13257
Steuernummer: 321/5800/1497