|
|
|||
|
||||
OverviewFull Product DetailsAuthor: Evan ShockleyPublisher: Springer Nature Switzerland AG Imprint: Springer Nature Switzerland AG Edition: 1st ed. 2021 Weight: 0.215kg ISBN: 9783030877545ISBN 10: 303087754 Pages: 119 Publication Date: 01 November 2022 Audience: Professional and scholarly , Professional & Vocational Format: Paperback Publisher's Status: Active Availability: Manufactured on demand We will order this item for you from a manufactured on demand supplier. Table of ContentsTABLE OF CONTENTSLIST OF FIGURES . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . viLIST OF TABLES . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . xiiiACKNOWLEDGMENTS . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . xivABSTRACT . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . xv1 SEARCHING FOR NEW PHYSICS WITH XENON1T . . . . . . . . . . . . . . . 11.1 The XENON1T Detector . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21.1.1 The S1 signal . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 51.1.2 The S2 signal . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 61.1.3 Position reconstruction . . . . . . . . . . . . . . . . . . . . . . . . . . 81.1.4 Particle discrimination: electronic vs. nuclear recoils . . . . . . . . . 81.1.5 Background reduction . . . . . . . . . . . . . . . . . . . . . . . . . . 101.2 Physics reach of XENON1T . . . . . . . . . . . . . . . . . . . . . . . . . . . 111.2.1 Solar axions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 111.2.2 Neutrino magnetic moment . . . . . . . . . . . . . . . . . . . . . . . 201.2.3 Bosonic dark matter . . . . . . . . . . . . . . . . . . . . . . . . . . . 242 EVENT RECONSTRUCTION AND SELECTION . . . . . . . . . . . . . . . . . 262.1 Energy Reconstruction and Resolution . . . . . . . . . . . . . . . . . . . . . 262.1.1 Energy Reconstruction . . . . . . . . . . . . . . . . . . . . . . . . . . 262.1.2 Energy Resolution . . . . . . . . . . . . . . . . . . . . . . . . . . . . 382.2 Detection Eciency . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 412.2.1 Single Photoelectron Acceptance . . . . . . . . . . . . . . . . . . . . 422.2.2 Reconstruction Eciency . . . . . . . . . . . . . . . . . . . . . . . . . 482.2.3 Eciency as function of charge . . . . . . . . . . . . . . . . . . . . . 562.2.4 Eciency as function of reconstructed energy . . . . . . . . . . . . . 572.3 Event Selection . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 633 BACKGROUND + SIGNAL MODELING AND STATISTICAL METHODS . . . 673.1 Background Model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 673.2 Signal Modeling . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 813.3 Statistical Framework . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 834 RESULTS . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 944.1 Background-only t . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 944.2 Investigating the excess . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1004.3 Potential Backgrounds . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1094.3.1 Xenon x-rays . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1094.3.2 37Ar . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 110iv4.3.3 Tritium . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1134.4 Searches for new physics in XENON1T ER data . . . . . . . . . . . . . . . . 1174.5 Search for solar axions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1184.5.1 Main Results . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1184.5.2 Interpretation under specic QCD models . . . . . . . . . . . . . . . 1244.5.3 Including tritium as a background . . . . . . . . . . . . . . . . . . . . 1304.6 Search for an enhanced neutrino magnetic moment . . . . . . . . . . . . . . 1334.6.1 Main Result . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1334.6.2 Including tritium as a background . . . . . . . . . . . . . . . . . . . . 1364.7 Bosonic Dark Matter Results . . . . . . . . . . . . . . . . . . . . . . . . . . 1364.8 Science Run 2 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1404.9 Time Dependence . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1424.10 Updated Analysis . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1454.10.1 Summary of updates . . . . . . . . . . . . . . . . . . . . . . . . . . . 1454.10.2 Results of updated analysis . . . . . . . . . . . . . . . . . . . . . . . 1485 CONCLUSIONS AND OUTLOOK . . . . . . . . . . . . . . . . . . . . . . . . . . 1525.1 Summary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1525.2 Outlook: XENONnT . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1555.3 Conclusion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 156REFERENCES . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157vReviewsAuthor InformationEvan Shockley is currently a postdoctoral scholar at UC San Diego. He obtained his PhD from the University of Chicago in 2020 after earning a MS from the University of Chicago in 2016 and a BA from Saint Mary’s University of Minnesota in 2014. In his final year at University of Chicago he was granted a Grainger Fellowship by the physics department for outstanding experimental research. A member of the XENON collaboration, his research interests center around the search for physics beyond the standard model using some of the world’s most sensitive particle detectors. Tab Content 6Author Website:Countries AvailableAll regions |