Relevant bibliographies by topics / High-energy starting events

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  1. Journal articles
  2. Dissertations / Theses
  3. Conference papers

Academic literature on the topic 'High-energy starting events'

Author: Grafiati
Published: 4 June 2021
Last updated: 1 February 2022

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Journal articles on the topic "High-energy starting events"

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Esmaili, Arman, and Kohta Murase. "Constraining high-energy neutrinos from choked-jet supernovae with IceCube high-energy starting events." Journal of Cosmology and Astroparticle Physics 2018, no. 12 (2018): 008. http://dx.doi.org/10.1088/1475-7516/2018/12/008.

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Pikounis, Konstantinos, Ekaterini Tzamariudaki, and Christos Markou. "Analysis of High Energy Starting Events with the KM3NeT/ARCA detector." EPJ Web of Conferences 207 (2019): 02006. http://dx.doi.org/10.1051/epjconf/201920702006.

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KM3NeT is a research infrastructure housing the next generation neutrino detectors in the depths of the Mediterranean Sea. The ARCA detector, which is currently under construction, is optimized for neutrino searches from astrophysical sources as well as measurements of the diffuse high energy astrophysical flux. The unambiguous detection of neutrinos of extraterrestrial origin by IceCube has led to the first measurement of a high energy astrophysical neutrino flux. The cutting-edge technology used for the design and construction of KM3NeT Digital Optical Modules along with the properties of se
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Moharana, Reetanjali, and Soebur Razzaque. "Angular correlation between IceCube high-energy starting events and starburst sources." Journal of Cosmology and Astroparticle Physics 2016, no. 12 (2016): 021. http://dx.doi.org/10.1088/1475-7516/2016/12/021.

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Ono, M., A. Ishihara, S. Yoshida, and the IceCube Collaboration. "Identification of extremely-high energy starting neutrino events with the IceCube observatory." Journal of Physics: Conference Series 120, no. 6 (2008): 062029. http://dx.doi.org/10.1088/1742-6596/120/6/062029.

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Stachurska, Juliana. "IceCube High Energy Starting Events at 7.5 Years - New Measurements of Flux and Flavor." EPJ Web of Conferences 207 (2019): 02005. http://dx.doi.org/10.1051/epjconf/201920702005.

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The IceCube Neutrino Observatory at the South Pole, which detects Cherenkov light from charged particles produced in neutrino interactions, firmly established the existence of an astrophysical high-energy neutrino component. Here I present IceCube’s High-Energy Starting Event sample and the new results obtained with a livetime of about 7.5 years. I will focus on the new measurement of the flavor composition performed using this sample. IceCube is directly sensitive to each neutrino flavor via the single cascade, track and double cascade event topologies, the latter being the topology produced
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Tkachev, I. I. "The Puzzle of the Ultra-High Energy Cosmic Rays." International Journal of Modern Physics A 18, supp01 (2003): 91–112. http://dx.doi.org/10.1142/s0217751x03016604.

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In early years the cosmic ray studies were ahead of the accelerator research, starting from the discovery of positrons, through muons, to that of pions and strange particles. Today we are facing the situation that the puzzling saga of cosmic rays of the highest energies may again unfold in the discovery of new physics, now beyond the Standard Model; or it may bring to life an "extreme" astrophysics. After a short review of the Greisen-Zatsepin-Kuzmin puzzle, I discuss different models which were suggested for its resolution. Are there any hints pointing to the correct model? I argue that the s
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Palladino, Andrea, and Walter Winter. "A multi-component model for observed astrophysical neutrinos." Astronomy & Astrophysics 615 (July 2018): A168. http://dx.doi.org/10.1051/0004-6361/201832731.

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Aims. We investigated the origin of observed astrophysical neutrinos. Methods. We propose a multi-component model for the observed diffuse neutrino flux. The model includes residual atmospheric backgrounds, a Galactic contribution (e.g., from cosmic ray interactions with gas), an extragalactic contribution from pp interactions (e.g., from starburst galaxies), and a hard extragalactic contribution from photo-hadronic interactions at the highest energies (e.g., from tidal disruption events or active galactic nuclei). Results. We demonstrate that this model can address the key problems of astroph
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KLAPDOR-KLEINGROTHAUS, H. V., I. V. KRIVOSHEINA, and I. V. TITKOVA. "THEORETICAL INVESTIGATION OF PULSE SHAPES OF DOUBLE BETA EVENTS IN A 76Ge DETECTOR, THEIR DEPENDENCE ON PARTICLE PHYSICS PARAMETERS, AND THEIR SEPARABILITY FROM BACKGROUND GAMMA EVENTS." Modern Physics Letters A 21, no. 16 (2006): 1257–78. http://dx.doi.org/10.1142/s0217732306020524.

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For the first time the expected pulse shapes to be observed for neutrinoless double beta events in a big 76 Ge detector have been calculated starting from their Monte Carlo calculated time history and spatial energy distribution. It is shown that with the spatial resolution of a large size Ge detector for the majority of 0νββ events it is not possible to differentiate between the contributions of different particle physics parameters entering into the 0νββ decay process — in the mass mechanism the effective neutrino mass and the right-handed weak current parameters λ, η. It is shown that on th
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Scrivner, Craig W., and Donald V. Helmberger. "Preliminary work on an early warning and rapid response program for moderate earthquakes." Bulletin of the Seismological Society of America 85, no. 4 (1995): 1257–65. http://dx.doi.org/10.1785/bssa0850041257.

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Abstract Warning of imminent ground shaking due to a large earthquake would be useful to a variety of agencies. This kind of ground-motion prediction is possible in southern California for events with magnitude less than 6, where path effects dominate. The 28 June 1991 Sierra Madre earthquake is presented as a test case for this concept. A single-station inversion of the record from the Pasadena station 20 km SW of the epicenter produces reasonable source parameters for the event. With these source parameters and a library of Green's functions calculated for an average southern California crus
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Kühn, Michael, and Tim Schöne. "Investigation of the influence of earthquakes on the water level in the geothermal reservoir of Waiwera (New Zealand)." Advances in Geosciences 45 (August 30, 2018): 235–41. http://dx.doi.org/10.5194/adgeo-45-235-2018.

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Abstract. The water level of the Waiwera geothermal reservoir is mainly governed by the production operations due to a commonly strong pumping signal. However, in the hours and days after the Kaikoura earthquake on 14 November 2016, it increased by more than 0.5 m, indicating that seismic events can have an influence as well. In a continuous time series consisting of monthly means of water level data and pumping rates starting in 1986, we tried to determine if events above a certain strength alter groundwater dynamics at Waiwera in general. We applied an empirical equation and calculated the o
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Dissertations / Theses on the topic "High-energy starting events"

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Usner, Marcel. "Search for Astrophysical Tau-Neutrinos in Six Years of High-Energy Starting Events in the IceCube Detector." Doctoral thesis, Humboldt-Universität zu Berlin, 2018. http://dx.doi.org/10.18452/19458.

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Astrophysikalische Neutrinos können in der Wechselwirkung kosmischer Strahlungsteilchen mit Materie oder Photonen nahe derer Quellen entstehen. Die auf der Erde erwartete Flavor-Zusammensetzung kann mögliche Neutrino Produktionsmechanismen einschränken. Tau-Neutrinos sind aufgrund von Flavor-Oszillationen über kosmische Distanzen zu erwarten. Das IceCube Neutrino Observatorium hat astrophysikalische Neutrinos bei Energien zwischen ~60 TeV und ~10 PeV entdeckt. Die gemessene Flavor-Zusammensetzung ist kompatibel mit ~1:1:1, wie vom Pion Produktionsszenario erwartet wird. Die Elektron- und Tau-N
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Usner, Marcel [Verfasser], Marek [Gutachter] Kowalski, Sebastian [Gutachter] Böser, and Achim [Gutachter] Stahl. "Search for Astrophysical Tau-Neutrinos in Six Years of High-Energy Starting Events in the IceCube Detector / Marcel Usner ; Gutachter: Marek Kowalski, Sebastian Böser, Achim Stahl." Berlin : Humboldt-Universität zu Berlin, 2018. http://d-nb.info/1185497757/34.

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Conference papers on the topic "High-energy starting events"

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Farrag, Kareem. "Highlights from the Seven-Year High Energy Starting Events Sample in IceCube." In Eighth Meeting on CPT and Lorentz Symmetry. WORLD SCIENTIFIC, 2020. http://dx.doi.org/10.1142/9789811213984_0056.

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Schneider, Austin. "Characterization of the Astrophysical Diffuse Neutrino Flux with IceCube High-Energy Starting Events." In 36th International Cosmic Ray Conference. Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.358.1004.

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Illuminati, Giulia, Alexis Coleiro, and Javier Barrios. "Search for time correlations between ANTARES neutrino candidates and IceCube/High-Energy Starting Events." In 35th International Cosmic Ray Conference. Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.301.0987.

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Usner, Marcel. "Search for Astrophysical Tau Neutrinos in Six Years of High-Energy Starting Events in IceCube." In 35th International Cosmic Ray Conference. Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.301.0974.

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Kaurin, Christian, Hans Panjaitan, Jacob Dybwad, and Per Damsleth. "Dynamic Behavior of Flexible vs Rigid Spools During Seismic Loading Events." In ASME 2017 36th International Conference on Ocean, Offshore and Arctic Engineering. American Society of Mechanical Engineers, 2017. http://dx.doi.org/10.1115/omae2017-61837.

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In regions of high seismic activity, the most severe loading experienced by subsea production systems during earthquake events can be significantly greater than normal static design loads. The major components of such systems comprising pipelines, manifolds and wells linked by tie-in spools and jumpers all respond differently when excited by seabed accelerations. Individual components may resonate or move out of phase with each other. It is of vital importance that the design of the system accounts for the dynamic loading at interfaces such as flanges, connectors and pipe supports. High dynami
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Arguelles, Carlos, and Hrvoje Dujmovic. "Searches for Connections Between Dark Matter and Neutrinos with the IceCube High-Energy Starting Event Sample." In 36th International Cosmic Ray Conference. Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.358.0839.

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Dor, Isabelle, Jean-Franc¸ois Pignatel, Christian Poette, Franck Morin, and Fre´de´ric Bertrand. "ETDR Project: Investigation of System Effects With the CATHARE Code." In 16th International Conference on Nuclear Engineering. ASMEDC, 2008. http://dx.doi.org/10.1115/icone16-48619.

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The Gas Fast Reactor (GFR) is one of the six concepts selected for further studies in the frame of the GEN IV forum and it is of high priority in the French Atomic Commission (CEA) R&D program on the future Nuclear Energy Systems. The conceptual design is shared between European partners through the GCFR 6th Framework Program. The ETDR (Experimental Technology Demonstrator Reactor) will be the first GFR ever built. The main characteristics of the ETDR ([1]) are a 50 MW concept with a starting core design with existing or close-to-existing technology (MOX pin S/A with metallic cladding) to
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Holst, D., G. Pechlivanoglou, C. T. Kohlrausch, C. N. Nayeri, and C. O. Paschereit. "sHAWT Design: Airfoil Aerodynamics Under the Influence of Roughness." In ASME Turbo Expo 2016: Turbomachinery Technical Conference and Exposition. American Society of Mechanical Engineers, 2016. http://dx.doi.org/10.1115/gt2016-56377.

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Small horizontal axis wind turbines (sHAWTs) are mostly designed by smaller companies with no or just small possibilities of aerodynamic testing and hence, airfoil selection is often based on published performance data and minimal or no experimental testing from the blade designer’s side. This paper focuses on the aerodynamic consequences resulting from an unqualified airfoil selection and accumulating surface soiling. The high performance low Reynolds profile FX 63-137 is compared to an Eppler-338 wing section as well as to a high performance utility scale wind turbine airfoil, AH 93-W-174 -1
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Manohar, Krishpersad, Annil Rampartap, and Rikhi Ramkissoon. "Self-Starting Hybrid ‘H’ Type Wind Turbine." In ASME 2007 Energy Sustainability Conference. ASMEDC, 2007. http://dx.doi.org/10.1115/es2007-36187.

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Wind energy is one of the fastest growing alternative energy resources being taped into worldwide. Vertical axis Darrieus ‘H’ type lift turbines have the potential to compete effectively with the more widely used conventional horizontal axis wind turbines. However, a disadvantage is when the rotor is stationary, no net rotational force arises, even at high wind speed. The rotor must already be spinning to generate torque and the design is normally not self-starting. In this study a hybrid Darrieus ‘H’ type lift turbine was designed to operate as a self-starting drag type turbine at low rotatio
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Miscia, Giuseppe, Vincenzo Rotondella, Andrea Baldini, Enrico Bertocchi, and Luca D’Agostino. "Aluminum Structures in Automotive: Experimental and Numerical Investigation for Advanced Crashworthiness." In ASME 2015 International Mechanical Engineering Congress and Exposition. American Society of Mechanical Engineers, 2015. http://dx.doi.org/10.1115/imece2015-51724.

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Ductility of aluminum alloys is highly used in automotive applications where crashworthiness becomes relevant. Due to its physical and mechanical properties, aluminum allows structures to be designed with good capacity to absorb energy, without increasing the overall weight of cars. In particular, high elongation allows for the conversion of a great amount of kinetic energy related to crash events in plastic deformation. If this was not the case, the energy involved during an accident could interest also the occupants, causing serious injuries. During large deformation of structures, chassis c
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