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Search For Atmospheric Muon Neutrinos And Extraterrestric Neutrino Point Sources In The 1997 Amanda B10 Data
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Book Synopsis Search for Atmospheric Muon Neutrinos and Extraterrestric Neutrino Point Sources in the 1997 AMANDA-B10 Data by : Alexander Biron von Curland
Download or read book Search for Atmospheric Muon Neutrinos and Extraterrestric Neutrino Point Sources in the 1997 AMANDA-B10 Data written by Alexander Biron von Curland and published by . This book was released on 2002 with total page 154 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Book Synopsis A Search for Extraterrestrial Point-sources of Neutrinos with AMANDA-II by : David Arthur Steele
Download or read book A Search for Extraterrestrial Point-sources of Neutrinos with AMANDA-II written by David Arthur Steele and published by . This book was released on 2004 with total page 172 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Book Synopsis Search for Extraterrestrial Point Sources of High Energy Neutrinos with AMANDA-II Using Data 2000-2002 by : You-Ren Wang
Download or read book Search for Extraterrestrial Point Sources of High Energy Neutrinos with AMANDA-II Using Data 2000-2002 written by You-Ren Wang and published by . This book was released on 2005 with total page 130 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Book Synopsis Neutrino Physics - Proceedings Of Nobel Symposium 129 by : Lars Bergstrom
Download or read book Neutrino Physics - Proceedings Of Nobel Symposium 129 written by Lars Bergstrom and published by World Scientific. This book was released on 2006-03-27 with total page 193 pages. Available in PDF, EPUB and Kindle. Book excerpt: Nobel Symposium 129 on Neutrino Physics was held at Haga Slott in Enköping, Sweden during August 19-24, 2004. Invited to the symposium were around 40 globally leading researchers in the field of neutrino physics, both experimental and theoretical.The dominant theme of the lectures was neutrino oscillations, which after several years were recently verified by results from the Super-Kamiokande detector in Kamioka, Japan and the SNO detector in Sudbury, Canada. Discussion focused especially on effects of neutrino oscillations derived from the presence of matter and the fact that three different neutrinos exist. Since neutrino oscillations imply that neutrinos have mass, this is the first experimental observation that fundamentally deviates from the standard model of particle physics. This is a challenge to both theoretical and experimental physics. The various oscillation parameters will be determined with increased precision in new, specially designed experiments. Theoretical physics is working intensively to insert the knowledge that neutrinos have mass into the theoretical models that describe particle physics. The lectures provided a very good description of the intensive situation in the field right now. The topics discussed also included mass models for neutrinos, neutrinos in extra dimensions as well as the “seesaw mechanism,” which provides a good description of why neutrino masses are so small.This book is A4 size and in full color.
Book Synopsis Search for Point Sources of High Energy Neutrinos with Final Data from AMANDA-II. by :
Download or read book Search for Point Sources of High Energy Neutrinos with Final Data from AMANDA-II. written by and published by . This book was released on 2009 with total page pages. Available in PDF, EPUB and Kindle. Book excerpt: We present a search for point sources of high energy neutrinos using 3.8 years of data recorded by AMANDA-II during 2000-2006. After reconstructing muon tracks and applying selection criteria designed to optimally retain neutrino-induced events originating in the Northern Sky, we arrive at a sample of 6595 candidate events, predominantly from atmospheric neutrinos with primary energy 100 GeV to 8 TeV. Our search of this sample reveals no indications of a neutrino point source. We place the most stringent limits to date on E−2 neutrino fluxes from points in the Northern Sky, with an average upper limit of E2?{sub?{sub {mu}}+?{sub {tau}}} ≤ 5.2 x 10−11 TeV cm−2 s−1 on the sum of?{sub {mu}} and {nu}{sub {tau}} fluxes, assumed equal, over the energy range from 1.9 TeV to 2.5 PeV.
Book Synopsis Observation of Atmospheric Muon Neutrinos with AMANDA by : Tyce Robert DeYoung
Download or read book Observation of Atmospheric Muon Neutrinos with AMANDA written by Tyce Robert DeYoung and published by . This book was released on 2001 with total page 166 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Book Synopsis Multi-year Search for a Diffuse Flxu of Muon Neutrinos with AMANDA-II. by :
Download or read book Multi-year Search for a Diffuse Flxu of Muon Neutrinos with AMANDA-II. written by and published by . This book was released on 2008 with total page pages. Available in PDF, EPUB and Kindle. Book excerpt:
Book Synopsis Multi-year Search for a Diffuse Flux of Muon Neutrinos with AMANDA-II by : Jessica Louise Hodges
Download or read book Multi-year Search for a Diffuse Flux of Muon Neutrinos with AMANDA-II written by Jessica Louise Hodges and published by . This book was released on 2007 with total page 140 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Book Synopsis A Search for Point Sources of High Energy Neutrinos with the AMANDA-B10 Neutrino Telescope by : Scott Matthew Young
Download or read book A Search for Point Sources of High Energy Neutrinos with the AMANDA-B10 Neutrino Telescope written by Scott Matthew Young and published by . This book was released on 2001 with total page 538 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Download or read book Contributed Papers written by and published by . This book was released on 1999 with total page 566 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Book Synopsis Observation of High Energy Atmospheric Neutrinos with Antarctic Muon and Neutrino Detector Array by :
Download or read book Observation of High Energy Atmospheric Neutrinos with Antarctic Muon and Neutrino Detector Array written by and published by . This book was released on 2002 with total page 5 pages. Available in PDF, EPUB and Kindle. Book excerpt: The Antarctic Muon and Neutrino Detector Array (AMANDA) began collecting data with ten strings in 1997. Results from the first year of operation are presented. Neutrinos coming through the Earth from the Northern Hemisphere are identified by secondary muons moving upward through the array. Cosmic rays in the atmosphere generate a background of downward moving muons, which are about 106 times more abundant than the upward moving muons. Over 130 days of exposure, we observed a total of about 300 neutrino events. In the same period, a background of 1.05 x 109 cosmic ray muon events was recorded. The observed neutrino flux is consistent with atmospheric neutrino predictions. Monte Carlo simulations indicate that 90 percent of these events lie in the energy range 66 GeV to 3.4 TeV. The observation of atmospheric neutrinos consistent with expectations establishes AMANDA-B10 as a working neutrino telescope.
Download or read book Acta Physica Polonica written by and published by . This book was released on 2004 with total page 782 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Book Synopsis The Search for Muon Neutrinos from Northern HemisphereGamma-Ray Bursts with AMANDA. by :
Download or read book The Search for Muon Neutrinos from Northern HemisphereGamma-Ray Bursts with AMANDA. written by and published by . This book was released on 2007 with total page pages. Available in PDF, EPUB and Kindle. Book excerpt: We present the results of the analysis of neutrino observations by the Antarctic Muon and Neutrino Detector Array (AMANDA) correlated with photon observations of more than 400 gamma-ray bursts (GRBs) in the Northern Hemisphere from 1997 to 2003. During this time period, AMANDA's effective collection area for muon neutrinos was larger than that of any other existing detector. Based on our observations of zero neutrinos during and immediately prior to the GRBs in the dataset, we set the most stringent upper limit on muon neutrino emission correlated with gamma-ray bursts. Assuming a Waxman-Bahcall spectrum and incorporating all systematic uncertainties, our flux upper limit has a normalization at 1 PeV of E2?{sub {nu}} ≤ 6.0 x 10−9 GeV cm−2s−1sr−1, with 90% of the events expected within the energy range of ≈10 TeV to ≈3 PeV. The impact of this limit on several theoretical models of GRBs is discussed, as well as the future potential for detection of GRBs by next generation neutrino telescopes. Finally, we briefly describe several modifications to this analysis in order to apply it to other types of transient point sources.
Book Synopsis A Search for Neutrinos from Cosmic Point Sources Using AMANDA-B10 with Emphasis on Limit Calculation Techniques by : Jan Conrad
Download or read book A Search for Neutrinos from Cosmic Point Sources Using AMANDA-B10 with Emphasis on Limit Calculation Techniques written by Jan Conrad and published by . This book was released on 2003 with total page 160 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Download or read book TAUP ... written by and published by . This book was released on 2003 with total page 574 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Book Synopsis Searching for High Energy Neutrinos with AMANDA-II Detector by : Jodi Ann Cooley-Sekula
Download or read book Searching for High Energy Neutrinos with AMANDA-II Detector written by Jodi Ann Cooley-Sekula and published by . This book was released on 2003 with total page 164 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Book Synopsis Preliminary Limits on the Flux of Muon Neutrinos from Extraterrestrial Point Sources by :
Download or read book Preliminary Limits on the Flux of Muon Neutrinos from Extraterrestrial Point Sources written by and published by . This book was released on 1985 with total page pages. Available in PDF, EPUB and Kindle. Book excerpt: We present the arrival directions of 117 upward-going muon events collected with the IMB proton lifetime detector during 317 days of live detector operation. The rate of upward-going muons observed in our detector was found to be consistent with the rate expected from atmospheric neutrino production. The upper limit on the total flux of extraterrestrial neutrinos>1 GeV is 0.06 neutrinos/cm2-sec. Using our data and a Monte Carlo simulation of high energy muon production in the earth surrounding the detector, we place limits on the flux of neutrinos from a point source in the Vela X-2 system of
