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Gorham PW, Allison P, Barwick SW, Beatty JJ, Besson DZ, Binns WR, Chen C, Chen P, Clem JM, Connolly A, Dowkontt PF, Duvernois MA, Field RC, Goldstein D, Goodhue A, Hast C, Hebert CL, Hoover S, Israel MH, Kowalski J, Learned JG, Liewer KM, Link JT, Lusczek E, Matsuno S, Mercurio BC, Miki C, Miocinović P, Nam J, Naudet CJ, Ng J, Nichol RJ, Palladino K, Reil K, Romero-Wolf A, Rosen M, Ruckman L, Saltzberg D, Seckel D, Varner GS, Walz D, Wang Y, Wu F. New limits on the ultrahigh energy cosmic neutrino flux from the ANITA experiment. Phys Rev Lett 2009; 103:051103. [PMID: 19792479 DOI: 10.1103/physrevlett.103.051103] [Citation(s) in RCA: 7] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 12/16/2008] [Revised: 04/15/2009] [Indexed: 05/28/2023]
Abstract
We report initial results of the first flight of the Antarctic Impulsive Transient Antenna (ANITA-1) 2006-2007 Long Duration Balloon flight, which searched for evidence of a diffuse flux of cosmic neutrinos above energies of E(nu) approximately 3 x 10(18) eV. ANITA-1 flew for 35 days looking for radio impulses due to the Askaryan effect in neutrino-induced electromagnetic showers within the Antarctic ice sheets. We report here on our initial analysis, which was performed as a blind search of the data. No neutrino candidates are seen, with no detected physics background. We set model-independent limits based on this result. Upper limits derived from our analysis rule out the highest cosmogenic neutrino models. In a background horizontal-polarization channel, we also detect six events consistent with radio impulses from ultrahigh energy extensive air showers.
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Affiliation(s)
- P W Gorham
- Department of Physics and Astronomy, University of Hawaii, Manoa, Hawaii 96822, USA
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2
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Gorham PW, Barwick SW, Beatty JJ, Besson DZ, Binns WR, Chen C, Chen P, Clem JM, Connolly A, Dowkontt PF, DuVernois MA, Field RC, Goldstein D, Goodhue A, Hast C, Hebert CL, Hoover S, Israel MH, Kowalski J, Learned JG, Liewer KM, Link JT, Lusczek E, Matsuno S, Mercurio B, Miki C, Miocinović P, Nam J, Naudet CJ, Ng J, Nichol R, Palladino K, Reil K, Romero-Wolf A, Rosen M, Ruckman L, Saltzberg D, Seckel D, Varner GS, Walz D, Wu F. Observations of the Askaryan effect in ice. Phys Rev Lett 2007; 99:171101. [PMID: 17995315 DOI: 10.1103/physrevlett.99.171101] [Citation(s) in RCA: 10] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 12/13/2006] [Revised: 06/15/2007] [Indexed: 05/25/2023]
Abstract
We report on observations of coherent, impulsive radio Cherenkov radiation from electromagnetic showers in solid ice. This is the first observation of the Askaryan effect in ice. As part of the complete validation process for the ANITA experiment, we performed an experiment at the Stanford Linear Accelerator Center in June 2006 using a 7.5 metric ton ice target. We measure for the first time the large-scale angular dependence of the radiation pattern, a major factor in determining the solid-angle acceptance of ultrahigh-energy neutrino detectors.
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Affiliation(s)
- P W Gorham
- Department of Physics and Astronomy, University of Hawaii, Manoa, Hawaii 96822, USA
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3
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Barwick SW, Beatty JJ, Besson DZ, Binns WR, Cai B, Clem JM, Connolly A, Cowen DF, Dowkontt PF, Duvernois MA, Evenson PA, Goldstein D, Gorham PW, Hebert CL, Israel MH, Learned JG, Liewer KM, Link JT, Matsuno S, Miocinović P, Nam J, Naudet CJ, Nichol R, Palladino K, Rosen M, Saltzberg D, Seckel D, Silvestri A, Stokes BT, Varner GS, Wu F. Constraints on cosmic neutrino fluxes from the Antarctic Impulsive Transient Antenna experiment. Phys Rev Lett 2006; 96:171101. [PMID: 16712284 DOI: 10.1103/physrevlett.96.171101] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 12/09/2005] [Indexed: 05/09/2023]
Abstract
We report new limits on cosmic neutrino fluxes from the test flight of the Antarctic Impulsive Transient Antenna (ANITA) experiment, which completed an 18.4 day flight of a prototype long-duration balloon payload, called ANITA-lite, in early 2004. We search for impulsive events that could be associated with ultrahigh energy neutrino interactions in the ice and derive limits that constrain several models for ultrahigh energy neutrino fluxes and rule out the long-standing -burst model.
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Affiliation(s)
- S W Barwick
- Department of Physics and Astronomy, University of California at Irvine, USA
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4
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Ahrens J, Bai X, Barwick SW, Becka T, Becker JK, Bernardini E, Bertrand D, Binon F, Biron A, Boersma DJ, Böser S, Botner O, Bouchta A, Bouhali O, Burgess T, Carius S, Castermans T, Chen A, Chirkin D, Collin B, Conrad J, Cooley J, Cowen DF, Davour A, De Clercq C, DeYoung T, Desiati P, Dewulf JP, Ekström P, Feser T, Gaisser TK, Ganugapati R, Gaug M, Geenen H, Gerhardt L, Goldschmidt A, Gross A, Hallgren A, Halzen F, Hanson K, Hardtke R, Harenberg T, Hauschildt T, Helbing K, Hellwig M, Herquet P, Hill GC, Hubert D, Hughey B, Hulth PO, Hultqvist K, Hundertmark S, Jacobsen J, Karle A, Kestel M, Köpke L, Kowalski M, Kuehn K, Lamoureux JI, Leich H, Leuthold M, Lindahl P, Liubarsky I, Madsen J, Mandli K, Marciniewski P, Matis HS, McParland CP, Messarius T, Minaeva Y, Miocinović P, Morse R, Münich K, Nahnhauer R, Neunhöffer T, Niessen P, Nygren DR, Ogelman H, Olbrechts P, Pérez de los Heros C, Pohl AC, Porrata R, Price PB, Przybylski GT, Rawlins K, Resconi E, Rhode W, Ribordy M, Richter S, Rodríguez Martino J, Sander HG, Schinarakis K, Schlenstedt S, Schmidt T, Schneider D, Schwarz R, Silvestri A, Solarz M, Spiczak GM, Spiering C, Stamatikos M, Steele D, Steffen P, Stokstad RG, Sulanke KH, Taboada I, Thollander L, Tilav S, Wagner W, Walck C, Wang YR, Wiebusch CH, Wiedemann C, Wischnewski R, Wissing H, Woschnagg K, Yodh G. Search for extraterrestrial point sources of neutrinos with AMANDA-II. Phys Rev Lett 2004; 92:071102. [PMID: 14995836 DOI: 10.1103/physrevlett.92.071102] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 09/19/2003] [Indexed: 05/24/2023]
Abstract
We present the results of a search for point sources of high-energy neutrinos in the northern hemisphere using AMANDA-II data collected in the year 2000. Included are flux limits on several active-galactic-nuclei blazars, microquasars, magnetars, and other candidate neutrino sources. A search for excesses above a random background of cosmic-ray-induced atmospheric neutrinos and misreconstructed downgoing cosmic-ray muons reveals no statistically significant neutrino point sources. We show that AMANDA-II has achieved the sensitivity required to probe known TeV gamma-ray sources such as the blazar Markarian 501 in its 1997 flaring state at a level where neutrino and gamma-ray fluxes are equal.
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Affiliation(s)
- J Ahrens
- Institute of Physics, University of Mainz, Staudinger Weg 7, D-55099 Mainz, Germany
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5
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Ahrens J, Bai X, Barwick SW, Bay RC, Becka T, Becker KH, Bernardini E, Bertrand D, Biron A, Boeser S, Botner O, Bouchta A, Bouhali O, Burgess T, Carius S, Castermans T, Chirkin D, Conrad J, Cooley J, Cowen DF, Davour A, De Clercq C, DeYoung T, Desiati P, Doksus P, Ekström P, Feser T, Gaisser TK, Ganugapati R, Gaug M, Geenen H, Gerhardt L, Goldschmidt A, Hallgren A, Halzen F, Hanson K, Hardtke R, Hauschildt T, Hellwig M, Herquet P, Hill GC, Hulth PO, Hughey B, Hultqvist K, Hundertmark S, Jacobsen J, Karle A, Kuehn K, Kim J, Köpke L, Kowalski M, Lamoureux JI, Leich H, Leuthold M, Lindahl P, Liubarsky I, Madsen J, Mandli K, Marciniewski P, Matis H, McParland CP, Messarius T, Miller TC, Minaeva Y, Miocinović P, Mock PC, Morse R, Neunhöffer T, Niessen P, Nygren DR, Ogelman H, Olbrechts P, Pérez de los Heros C, Pohl AC, Porrata R, Price PB, Przybylski GT, Rawlins K, Resconi E, Rhode W, Ribordy M, Richter S, Martino JR, Romenesko P, Ross D, Sander HG, Schlenstedt S, Schinarakis K, Schmidt T, Schneider D, Schwarz R, Silvestri A, Solarz M, Stamatikos M, Spiczak GM, Spiering C, Steele D, Steffen P, Stokstad RG, Sulanke KH, Taboada I, Tilav S, Wagner W, Walck C, Wang YR, Wiebusch CH, Wiedemann C, Wischnewski R, Wissing H, Woschnagg K, Wu W, Yodh G, Young S. Limits on diffuse fluxes of high energy extraterrestrial neutrinos with the AMANDA-B10 detector. Phys Rev Lett 2003; 90:251101. [PMID: 12857122 DOI: 10.1103/physrevlett.90.251101] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/25/2003] [Indexed: 05/24/2023]
Abstract
Data from the AMANDA-B10 detector taken during the austral winter of 1997 have been searched for a diffuse flux of high energy extraterrestrial muon neutrinos. This search yielded no excess events above those expected from background atmospheric neutrinos, leading to upper limits on the extraterrestrial neutrino flux measured at the earth. For an assumed E-2 spectrum, a 90% classical confidence level upper limit has been placed at a level E2Phi(E)=8.4 x 10(-7) cm(-2) s(-1) sr(-1) GeV (for a predominant neutrino energy range 6-1000 TeV), which is the most restrictive bound placed by any neutrino detector. Some specific predicted model spectra are excluded. Interpreting these limits in terms of the flux from a cosmological distributions of sources requires the incorporation of neutrino oscillations, typically weakening the limits by a factor of 2.
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Affiliation(s)
- J Ahrens
- Institute of Physics, University of Mainz, Staudinger Weg 7, D-55099, Mainz, Germany
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6
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Andrés E, Askebjer P, Bai X, Barouch G, Barwick SW, Bay RC, Becker KH, Bergström L, Bertrand D, Bierenbaum D, Biron A, Booth J, Botner O, Bouchta A, Boyce MM, Carius S, Chen A, Chirkin D, Conrad J, Cooley J, Costa CG, Cowen DF, Dailing J, Dalberg E, DeYoung T, Desiati P, Dewulf JP, Doksus P, Edsjö J, Ekström P, Erlandsson B, Feser T, Gaug M, Goldschmidt A, Goobar A, Gray L, Haase H, Hallgren A, Halzen F, Hanson K, Hardtke R, He YD, Hellwig M, Heukenkamp H, Hill GC, Hulth PO, Hundertmark S, Jacobsen J, Kandhadai V, Karle A, Kim J, Koci B, Köpke L, Kowalski M, Leich H, Leuthold M, Lindahl P, Liubarsky I, Loaiza P, Lowder DM, Ludvig J, Madsen J, Marciniewski P, Matis HS, Mihalyi A, Mikolajski T, Miller TC, Minaeva Y, Miocinović P, Mock PC, Morse R, Neunhöffer T, Newcomer FM, Niessen P, Nygren DR, Ogelman H, Pérez de los Heros C, Porrata R, Price PB, Rawlins K, Reed C, Rhode W, Richards A, Richter S, Martino JR, Romenesko P, Ross D, Rubinstein H, Sander HG, Scheider T, Schmidt T, Schneider D, Schneider E, Schwarz R, Silvestri A, Solarz M, Spiczak GM, Spiering C, Starinsky N, Steele D, Steffen P, Stokstad RG, Streicher O, Sun Q, Taboada I, Thollander L, Thon T, Tilav S, Usechak N, Vander Donckt M, Walck C, Weinheimer C, Wiebusch CH, Wischnewski R, Wissing H, Woschnagg K, Wu W, Yodh G, Young S. Observation of high-energy neutrinos using Cerenkov detectors embedded deep in Antarctic ice. Nature 2001; 410:441-3. [PMID: 11260705 DOI: 10.1038/35068509] [Citation(s) in RCA: 138] [Impact Index Per Article: 6.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022]
Abstract
Neutrinos are elementary particles that carry no electric charge and have little mass. As they interact only weakly with other particles, they can penetrate enormous amounts of matter, and therefore have the potential to directly convey astrophysical information from the edge of the Universe and from deep inside the most cataclysmic high-energy regions. The neutrino's great penetrating power, however, also makes this particle difficult to detect. Underground detectors have observed low-energy neutrinos from the Sun and a nearby supernova, as well as neutrinos generated in the Earth's atmosphere. But the very low fluxes of high-energy neutrinos from cosmic sources can be observed only by much larger, expandable detectors in, for example, deep water or ice. Here we report the detection of upwardly propagating atmospheric neutrinos by the ice-based Antarctic muon and neutrino detector array (AMANDA). These results establish a technology with which to build a kilometre-scale neutrino observatory necessary for astrophysical observations.
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Affiliation(s)
- E Andrés
- Department of Physics, University of Wisconsin, Wisconsin, Madison 53706, USA
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