Search Results - "Halzen, F."

Astroparticle physics with high energy neutrinos: from AMANDA to IceCube by Halzen, F.

“…Kilometer-scale neutrino detectors such as IceCube are discovery instruments covering nuclear and particle physics, cosmology and astronomy. Examples of their…”
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GZK neutrinos after the Fermi-LAT diffuse photon flux measurement by Ahlers, M., Anchordoqui, L.A., Gonzalez–Garcia, M.C., Halzen, F., Sarkar, S.

“…Cosmogenic neutrinos originate from photo-hadronic interactions of cosmic ray protons with the cosmic microwave background (CMB). The neutrino production rate…”
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Reevaluation of the prospect of observing neutrinos from Galactic sources in the light of recent results in gamma ray and neutrino astronomy by Gonzalez-Garcia, M.C., Halzen, F., Niro, V.

“…In light of the recent IceCube evidence for a flux of extraterrestrial neutrinos, we revisit the prospect of observing the sources of the Galactic cosmic rays…”
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The highest energy neutrinos: First evidence for cosmic origin by Halzen, F.

“…Developments in neutrino astronomy have been to a great extent motivated by the search for the sources of the cosmic rays, leading at a very early stage to the…”
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GRBs on probation: Testing the UHE CR paradigm with IceCube by Ahlers, M., Gonzalez-Garcia, M.C., Halzen, F.

“…► We study the hypothesis that GRBs are the main sources of UHE CRs. ► Our analysis focuses on UHE CR emission in the form of neutrons produced in photo-pion…”
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Tau Neutrino Appearance with a 1000 Megaparsec Baseline by Halzen, F., Saltzberg, D.

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Possible High-Energy Neutrinos from the Cosmic Accelerator RX J1713.7–3946 by Alvarez-Muñiz, J, Halzen, F

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A search for the dark matter annual modulation in South Pole ice by Cherwinka, J., Co, R., Cowen, D.F., Grant, D., Halzen, F., Heeger, K.M., Hsu, L., Karle, A., Kudryavtsev, V.A., Maruyama, R., Pettus, W., Robinson, M., Spooner, N.J.C.

“…► We describe a dark matter experiment using NaI crystals deployed in South Pole ice. ► We explore the sensitivity of a 250kg NaI dark matter experiment. ► A…”
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Neutrino Fluxes from Active Galaxies: A Model-Independent Estimate by Halzen, F, Zas, E

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Neutrinos from individual gamma-ray bursts in the BATSE catalog by Guetta, D., Hooper, D., Alvarez-Muñiz, J., Halzen, F., Reuveni, E.

“…We estimate the neutrino emission from individual γ-ray bursts observed by the BATSE detector on the Compton Gamma-Ray Observatory. Neutrinos are produced by…”
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Quantitative tests of color evaporation: charmonium production by Amundson, J.F., Éboli, O.J.P., Gregores, E.M., Halzen, F.

“…The color evaporation model simply states that charmonium production is described by the same dynamics as D D production, i.e., by the formation of a colored c…”
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Extending the frontiers: Reconciling accelerator and cosmic ray p − p cross sections by Block, M. M., Halzen, F., Stanev, T.

“…We simultaneously fit a QCD-inspired parametrization of all accelerator data on forward proton-proton and antiproton-proton scattering amplitudes, together…”
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IceRay: An IceCube-centered radio-Cherenkov GZK neutrino detector by Allison, P., Beatty, J., Chen, P., Connolly, A., DuVernois, M., Gorham, P., Halzen, F., Hanson, K., Hoffman, K., Karle, A., Kelley, J., Landsman, H., Learned, J., Miki, C., Morse, R., Nichol, R., Rott, C., Ruckman, L., Seckel, D., Varner, G., Williams, D.

“…We discuss design considerations and simulation results for IceRay, a proposed large-scale ultra-high energy (UHE) neutrino detector at the South Pole. The…”
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Neutrinos associated with cosmic rays of top–down origin by Barbot, C., Drees, M., Halzen, F., Hooper, D.

“…Top–down models of cosmic rays produce more neutrinos than photons and more photons than protons. In these models, we reevaluate the fluxes of neutrinos…”
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High energy neutrinos from gamma ray bursts: Event rates in neutrino telescopes by Alvarez-Muñiz, J., Halzen, F., Hooper, D. W.

“…Following Waxman and Bahcall we calculate the event rate, energy and zenith angle dependence of neutrinos produced in the fireball model of gamma ray bursts…”
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Phenomenology of high-energy neutrinos in low-scale quantum-gravity models by Alvarez-Muñiz, J, Halzen, F, Han, T, Hooper, D

“…We show that neutrino telescopes, optimized for detecting neutrinos of TeV to PeV energy, can reveal threshold effects associated with TeV-scale gravity. The…”
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The AMANDA neutrino telescope: principle of operation and first results by Andres, E., Askebjer, P., Barwick, S.W., Bay, R., Bergström, L., Biron, A., Booth, J., Bouchta, A., Carius, S., Carlson, M., Cowen, D., Dalberg, E., DeYoung, T., Ekström, P., Erlandson, B., Goobar, A., Gray, L., Hallgren, A., Halzen, F., Hardtke, R., Hart, S., He, Y., Heukenkamp, H., Hill, G., Hulth, P.O., Hundertmark, S., Jacobsen, J., Jones, A., Kandhadai, V., Karle, A., Koci, B., Lindahl, P., Liubarsky, I., Leuthold, M., Lowder, D.M., Marciniewski, P., Mikolajski, T., Miller, T., Miocinovic, P., Mock, P., Morse, R., Niessen, P., Pérez de los Heros, C., Porrata, R., Potter, D., Price, P.B., Przybylski, G., Richards, A., Richter, S., Romenesko, P., Rubinstein, H., Schneider, E., Schmidt, T., Schwarz, R., Solarz, M., Spiczak, G.M., Spiering, C., Streicher, O., Sun, Q, Thollander, L., Thon, T., Tilav, S., Walck, C., Wiebusch, C., Wischnewski, R., Woschnagg, K., Yodh, G.

“…AMANDA is a high-energy neutrino telescope presently under construction at the geographical South Pole. In the Antarctic summer 1995/96, an array of 80 optical…”
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High-energy neutrinos from radio galaxies by Becker Tjus, J., Eichmann, B., Halzen, F., Kheirandish, A., Saba, S. M.

“…The IceCube experiment has recently reported the first observation of high-energy cosmic neutrinos. Their origin is still unknown. In this paper, we…”
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Neutrino Event Rates from Gamma-Ray Bursts by Halzen, F, Hooper, D. W

“…We recalculate the diffuse flux of high-energy neutrinos produced by gamma-ray bursts in the relativistic fireball model. Although we confirm that the average…”
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Colorless states in perturbative QCD: Charmonium and rapidity gaps by Amundson, J.F., Éboli, O.J.P., Gregores, E.M., Halzen, F.

“…We point out that an unorthodox way to describe the production of rapidity gaps in deep inelastic scattering, recently proposed by Buchmüller and Hebecker,…”
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