Author: "Wissel, Stephanie" - Searchworks@Jio Institute Digital Library Search Results

Your search keyword '"Wissel, Stephanie"' showing total 115 results

Start Over Author "Wissel, Stephanie"

115 results on '"Wissel, Stephanie"'

1. The Giant Radio Array for Neutrino Detection (GRAND) Collaboration -- Contributions to the 10th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities (ARENA 2024)

Author: Batista, Rafael Alves, Benoit-Lévy, Aurélien, Bister, Teresa, Bohacova, Martina, Bustamante, Mauricio, Carvalho, Washington, Chen, Yiren, Cheng, LingMei, Chiche, Simon, Colley, Jean-Marc, Correa, Pablo, Laurenciu, Nicoleta Cucu, Dai, Zigao, de Almeida, Rogerio M., de Errico, Beatriz, de Jong, Sijbrand, Neto, João R. T. de Mello, de Vries, Krijn D, Decoene, Valentin, Denton, Peter B., Duan, Bohao, Duan, Kaikai, Engel, Ralph, Erba, William, Fan, Yizhong, Ferrière, Arsène, Gou, QuanBu, Gu, Junhua, Guelfand, Marion, Guo, Jianhua, Guo, Yiqing, Guépin, Claire, Gülzow, Lukas, Haungs, Andreas, Havelka, Matej, He, Haoning, Hivon, Eric, Hu, Hongbo, Huang, Xiaoyuan, Huang, Yan, Huege, Tim, Jiang, Wen, Koirala, Ramesh, Kong, ChuiZheng, Kotera, Kumiko, Köhler, Jelena, Lago, Bruno L., Lai, Zhisen, Coz, Sandra Le, Legrand, François, Leisos, Antonios, Li, Rui, Li, Xingyu, Li, YiFei, Liu, Cheng, Liu, Ruoyu, Liu, Wei, Ma, Pengxiong, Macias, Oscar, Magnard, Frédéric, Marcowith, Alexandre, Martineau-Huynh, Olivier, McKinley, Thomas, Minodier, Paul, Mitra, Pragati, Mostafá, Miguel, Murase, Kohta, Niess, Valentin, Nonis, Stavros, Ogio, Shoichi, Oikonomou, Foteini, Pan, Hongwei, Papageorgiou, Konstantinos, Pierog, Tanguy, Piotrowski, Lech Wiktor, Prunet, Simon, Qian, Xiangli, Roth, Markus, Sako, Takashi, Schoorlemmer, Harm, Szálas-Motesiczky, Dániel, Sławiński, Szymon, Tian, Xishui, Timmermans, Anne, Timmermans, Charles, Tobiska, Petr, Tsirigotis, Apostolos, Tueros, Matías, Vittakis, George, Wang, Hanrui, Wang, Jiale, Wang, Shen, Wang, Xiangyu, Wang, Xu, Wei, Daming, Wei, Feng, Wu, Xiangping, Wu, Xuefeng, Xu, Xin, Xu, Xing, Yang, Fufu, Yang, Lili, Yang, Xuan, Yuan, Qiang, Zarka, Philippe, Zeng, Houdun, Zhang, Chao, Zhang, Jianli, Zhang, Kewen, Zhang, Pengfei, Zhang, Qingchi, Zhang, Songbo, Zhang, Yi, Zhou, Hao, Wissel, Stephanie, Zeolla, Andrew, Deaconu, Cosmin, Hughes, Kaeli, Martin, Zachary, Mulrey, Katharine, Cummings, Austin, Krömer, Oliver, Plant, Kathryn, and Schroeder, Frank G.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment, High Energy Physics - Phenomenology
Abstract: This is an index of the contributions by the Giant Radio Array for Neutrino Detection (GRAND) Collaboration to the 10th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities (ARENA 2024, University of Chicago, June 11-14, 2024). The contributions include an overview of GRAND in its present and future incarnations, methods of radio-detection that are being developed for them, and ongoing joint work between the GRAND and BEACON experiments., Comment: Note: To access the list of contributions, please follow the "HTML" link that can be found on the arXiv page
Published: 2024

2. Targeting 100-PeV tau neutrino detection with an array of phased and high-gain reconstruction antennas

Author: Wissel, Stephanie, Zeolla, Andrew, Deaconu, Cosmin, Decoene, Valentin, Hughes, Kaeli, Martin, Zachary, Mulrey, Katharine, Cummings, Austin, Batista, Rafael Alves, Benoit-Lévy, Aurélien, Bustamante, Mauricio, Correa, Pablo, Ferrière, Arsène, Guelfand, Marion, Huege, Tim, Kotera, Kumiko, Martineau, Olivier, Murase, Kohta, Niess, Valentin, Zhang, Jianli, Krömer, Oliver, Plant, Kathryn, and Schroeder, Frank G.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment
Abstract: Neutrinos at ultrahigh energies can originate both from interactions of cosmic rays at their acceleration sites and through cosmic-ray interactions as they propagate through the universe. These neutrinos are expected to have a low flux which drives the need for instruments with large effective areas. Radio observations of the inclined air showers induced by tau neutrino interactions in rock can achieve this, because radio waves can propagate essentially unattenuated through the hundreds of kilometers of atmosphere. Proposed arrays for radio detection of tau neutrinos focus on either arrays of inexpensive receivers distributed over a large area, the GRAND concept, or compact phased arrays on elevated mountains, the BEACON concept, to build up a large detector area with a low trigger threshold. We present a concept that combines the advantages of these two approaches with a trigger driven by phased arrays at a moderate altitude (1 km) and sparse, high-gain outrigger receivers for reconstruction and background rejection. We show that this design has enhanced sensitivity at 100 PeV over the two prior designs with fewer required antennas and discuss the need for optimized antenna designs., Comment: ARENA2024 Conference Proceeding PoS(ARENA2024)058
Published: 2024

3. Ultrahigh-energy neutrino searches using next-generation gravitational wave detectors at radio neutrino detectors: GRAND, IceCube-Gen2 Radio, and RNO-G

Author: Mukhopadhyay, Mainak, Kotera, Kumiko, Wissel, Stephanie, Murase, Kohta, and Kimura, Shigeo S.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology, High Energy Physics - Phenomenology
Abstract: Binary neutron star (BNS) mergers can be sources of ultrahigh-energy (UHE) cosmic rays and potential emitters of UHE neutrinos. The upcoming and current radio neutrino detectors like the Giant Radio Array for Neutrino Detection (GRAND), IceCube-Gen2 Radio, and the Radio Neutrino Observatory in Greenland (RNO-G) are projected to reach the required sensitivities to search for these neutrinos. In particular, in conjunction with the next-generation of gravitational wave (GW) detectors like Cosmic Explorer (CE) and Einstein Telescope (ET), GW-triggered stacking searches can be performed with the UHE neutrino detectors. In this work, we explore the prospects of such searches by implementing in our analysis an upper distance limit based on the sky-localization capabilities of the GW detectors from which meaningful triggers can be collected. We find that if each GW burst is associated with a total isotropic-equivalent energy of $\sim 10^{50} - 10^{51}$ erg emitted in UHE neutrinos, along with a corresponding beaming fraction of $1$\%, GRAND and IceCube-Gen2 Radio have a large probability ($\sim 99$\%) to detect a coincident neutrino event using the joint combination of CE+ET in a timescale of less than 15 years of operation for our fiducial choice of parameters. In case of nondetections, the parameter spaces can be constrained at $3\sigma$ level in similar timescales of operation. We also highlight and discuss the prospects of such joint radio neutrino detector network, their importance, and their role in facilitating synergic GW and neutrino observations in the next era of multimessenger astrophysics., Comment: 18 pages, 6 figures
Published: 2024
Full Text: View/download PDF

4. Secondary Lepton Production, Propagation, and Interactions with NuLeptonSim

Author: Cummings, Austin, Krebs, Ryan, Wissel, Stephanie, Alvarez-Muñiz, Jaime, Carvalho Jr., Washington R., Romero-Wolf, Andrés, Schoorlemmer, Harm, and Zas, Enrique
Subjects: High Energy Physics - Phenomenology
Abstract: Charged current interactions of neutrinos inside the Earth can result in secondary muons and {\tau} - leptons which are detectable by a large swath of existing and planned neutrino experiments through a wide variety of event topologies. Consideration of such events can improve detector performance and provide unique signatures which help with event reconstruction. In this work, we describe NuLeptonSim, a propagation tool for neutrinos and charged leptons that builds on the fast NuTauSim framework. NuLeptonSim considers energy losses of charged leptons, modelled both continuously for performance or stochastically for accuracy, as well as interaction models for all flavors of neutrinos, including the Glashow resonance. We demonstrate the results from including these effects on the Earth emergence probability of various charged leptons from different flavors of primary neutrino and their corresponding energy distributions. We find that the emergence probability of muons can be higher than that of taus for energies below 100 PeV, whether from a primary muon or {\tau} neutrino, and that the Glashow resonance contributes to a surplus of emerging leptons near the resonant energy.
Published: 2023

5. Neutrino propagation through Earth: modeling uncertainties using nuPyProp

Author: Garg, Diksha, Reno, Mary Hall, Patel, Sameer, Ruestle, Alexander, Akaike, Yosui, Anchordoqui, Luis A., Bergman, Douglas R., Buckland, Isaac, Cummings, Austin L., Eser, Johannes, Garcia, Fred, Guépin, Claire, Heibges, Tobias, Ludwig, Andrew, Krizmanic, John F., Mackovjak, Simon, Mayotte, Eric, Mayotte, Sonja, Olinto, Angela V., Paul, Thomas C., Romero-Wolf, Andrés, Sarazin, Frédéric, Venters, Tonia M., Wiencke, Lawrence, and Wissel, Stephanie
Subjects: High Energy Physics - Phenomenology, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Using the Earth as a neutrino converter, tau neutrino fluxes from astrophysical point sources can be detected by tau-lepton-induced extensive air showers (EASs). Both muon neutrino and tau neutrino induced upward-going EAS signals can be detected by terrestrial, sub-orbital and satellite-based instruments. The sensitivity of these neutrino telescopes can be evaluated with the nuSpaceSim package, which includes the nuPyProp simulation package. The nuPyProp package propagates neutrinos ($\nu_\mu$, $\nu_\tau$) through the Earth to produce the corresponding charged leptons (muons and tau-leptons). We use nuPyProp to quantify the uncertainties from Earth density models, tau depolarization effects and photo-nuclear electromagnetic energy loss models in the charged lepton exit probabilities and their spectra. The largest uncertainties come from electromagnetic energy loss modeling, with as much as a 20-50% difference between the models. We compare nuPyProp results with other simulation package results., Comment: 9 pages, 6 figures, Proceedings for International Cosmic Ray Conference (ICRC) 2023
Published: 2023

6. Prospects for joint cosmic ray and neutrino constraints on the evolution of trans-GZK proton sources

Author: Muzio, Marco Stein, Unger, M., and Wissel, Stephanie
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: We consider the prospects for future ultrahigh energy cosmic ray and neutrino observations to constrain the evolution of sources producing a proton flux above 10 EeV (1 EeV = 10^18 eV). We find that strong constraints on the source evolution can be obtained by combining measurements of the cosmic ray proton fraction above 30 EeV with measurement of the neutrino flux at 1 EeV, if neutrinos are predominantly of cosmogenic origin. In the case that interactions in the source environment produce a significant astrophysical neutrino flux, constraints on the source evolution may require measurement of the observed proton fraction, as well as, the neutrino flux at multiple energies, such as 1 EeV and 10 EeV. Finally, we show that fits to current UHECR data favor models which result in a >30 EeV proton fraction and 1 EeV neutrino flux that could realistically be discovered by the next generation of experiments.
Published: 2023

7. Neutrino propagation in the Earth and emerging charged leptons with $\texttt{nuPyProp}$

Author: Garg, Diksha, Patel, Sameer, Reno, Mary Hall, Reustle, Alexander, Akaike, Yosui, Anchordoqui, Luis A., Bergman, Douglas R., Buckland, Isaac, Cummings, Austin L., Eser, Johannes, Garcia, Fred, Guépin, Claire, Heibges, Tobias, Ludwig, Andrew, Krizmanic, John F., Mackovjak, Simon, Mayotte, Eric, Mayotte, Sonja, Olinto, Angela V., Paul, Thomas C., Romero-Wolf, Andrés, Sarazin, Frédéric, Venters, Tonia M., Wiencke, Lawrence, and Wissel, Stephanie
Subjects: Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Phenomenology
Abstract: Ultra-high-energy neutrinos serve as messengers of some of the highest energy astrophysical environments. Given that neutrinos are neutral and only interact via weak interactions, neutrinos can emerge from sources, traverse astronomical distances, and point back to their origins. Their weak interactions require large target volumes for neutrino detection. Using the Earth as a neutrino converter, terrestrial, sub-orbital, and satellite-based instruments are able to detect signals of neutrino-induced extensive air showers. In this paper, we describe the software code $\texttt{nuPyProp}$ that simulates tau neutrino and muon neutrino interactions in the Earth and predicts the spectrum of the $\tau$-lepton and muons that emerge. The $\texttt{nuPyProp}$ outputs are lookup tables of charged lepton exit probabilities and energies that can be used directly or as inputs to the $\texttt{nuSpaceSim}$ code designed to simulate optical and radio signals from extensive air showers induced by the emerging charged leptons. We describe the inputs to the code, demonstrate its flexibility and show selected results for $\tau$-lepton and muon exit probabilities and energy distributions. The $\texttt{nuPyProp}$ code is open source, available on Github., Comment: 42 pages, 21 figures, fixed typo in one of the author's name. Code available at https://github.com/NuSpaceSim/nupyprop
Published: 2022
Full Text: View/download PDF

8. Report of the Topical Group on Cosmic Probes of Fundamental Physics for for Snowmass 2021

Author: Adhikari, Rana X., Anchordoqui, Luis A., Fang, Ke, Sathyaprakash, B. S., Tollefson, Kirsten, Lewis, Tiffany R., Engel, Kristi, Aboubrahim, Amin, Akarsu, Ozgur, Akrami, Yashar, Aloisio, Roberto, Batista, Rafael Alves, Ballardini, Mario, Ballmer, Stefan W., Bechtol, Ellen, Benisty, David, Berti, Emanuele, Birrer, Simon, Bonilla, Alexander, Brito, Richard, Bustamante, Mauricio, Caldwell, Robert, Cardoso, Vitor, Chakrabarti, Sukanya, Chen, Thomas Y., Cicoli, Michele, Clesse, Sebastien, Coleman, Alan, Cui, Yanou, Cusin, Giulia, Daylan, Tansu, Dienes, Keith R., Di Valentino, Eleonora, Dvorkin, Cora, Escamilla-Rivera, Celia, Farrar, Glennys R., Feng, Jonathan L., Frusciante, Noemi, Garcia-Bellido, Juan, Canal, Carlos Garcia, Garzelli, Maria Vittoria, Glombitza, Jonas, Golup, Geraldina, Gritsevich, Maria, Haiman, Zoltan, Haro, Jaume, Hazra, Dhiraj Kumar, Heavens, Alan, Holz, Daniel, Horandel, Jorg R., Ishak, Mustapha, Ivanov, Mikhail M., Joudaki, Shahab, Kampert, Karl-Heinz, Karwin, Christopher M., Keeley, Ryan, Klasen, Michael, Konoplich, Rostislav, Krizmanic, John F., Kumar, Suresh, L'Huillier, Benjamin, Levi, Noam, Mandic, Vuk, Marra, Valerio, Martins, C. J. A. P., Matarrese, Sabino, Mayotte, Eric, Mayotte, Sonja, Mersini-Houghton, Laura, Meyers, Joel, Miller, Andrew L., Mottola, Emil, Mukherjee, Suvodip, Murase, Kohta, Muzio, Marco Stein, Nath, Pran, Ng, Ken K. Y., No, Jose Miguel, Nunes, Rafael C., Olinto, Angela V., Pace, Francesco, Pan, Supriya, Bergliaffa, Santiago E. Perez, Pogosian, Levon, Read, Jocelyn, Reininghaus, Maximilian, Reno, Mary Hall, Riess, Adam G., Sakellariadou, Mairi, Sakharov, Alexander S., Salucci, Paolo, Santander, Marcos, Santos, Eva, Sarazin, Fred, Saridakis, Emmanuel N., Sciutto, Sergio J., Shafieloo, Arman, Shoemaker, David H., Sinha, Kuver, Soldin, Dennis, Soriano, Jorge F., Staicova, Denitsa, Sun, Ling, Steer, D. A., Thomas, Brooks, Tomsick, John A., Valera, Victor B., Vazquez, J. Alberto, Venters, Tonia M., Visinelli, Luca, Watson, Scott, Webb, John K., Weltman, Amanda, White, Graham, Wissel, Stephanie, Yadav, Anil Kumar, Yang, Fengwei, Yang, Weiqiang, Yunes, Nicolas, Yushkov, Alexey, and Zhang, Haocheng
Subjects: High Energy Physics - Phenomenology, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Cosmic Probes of Fundamental Physics take two primary forms: Very high energy particles (cosmic rays, neutrinos, and gamma rays) and gravitational waves. Already today, these probes give access to fundamental physics not available by any other means, helping elucidate the underlying theory that completes the Standard Model. The last decade has witnessed a revolution of exciting discoveries such as the detection of high-energy neutrinos and gravitational waves. The scope for major developments in the next decades is dramatic, as we detail in this report., Comment: Report of theTopical Group on Cosmic Probes of Fundamental Physics, for the U.S. decadal Particle Physics Planning Exercise (Snowmass 2021)
Published: 2022

9. High-Energy and Ultra-High-Energy Neutrinos

Author: Ackermann, Markus, Agarwalla, Sanjib K., Alvarez-Muñiz, Jaime, Batista, Rafael Alves, Argüelles, Carlos A., Bustamante, Mauricio, Clark, Brian A., Cummings, Austin, Das, Sudipta, Decoene, Valentin, Denton, Peter B., Dornic, Damien, Dzhilkibaev, Zhan-Arys, Farzan, Yasaman, Garcia, Alfonso, Garzelli, Maria Vittoria, Glaser, Christian, Heijboer, Aart, Hörandel, Jörg R., Illuminati, Giulia, Jeong, Yu Seon, Kelley, John L., Kelly, Kevin J., Kheirandish, Ali, Klein, Spencer R., Krizmanic, John F., Larson, Michael J., Lu, Lu, Murase, Kohta, Narang, Ashish, Otte, Nepomuk, Prechelt, Remy L., Prohira, Steven, Reno, Mary Hall, Resconi, Elisa, Santander, Marcos, Suvorova, Olga Vasil'evna, Valera, Victor B., Vandenbroucke, Justin, Wiencke, Lawrence, Wissel, Stephanie, Yoshida, Shigeru, Yuan, Tianlu, Zas, Enrique, Zhelnin, Pavel, and Zhou, Bei
Subjects: High Energy Physics - Phenomenology, Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment
Abstract: Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy physics. With energies far beyond solar, supernovae, atmospheric, and accelerator neutrinos, high-energy and ultra-high-energy neutrinos probe fundamental physics from the TeV scale to the EeV scale and beyond. They are sensitive to physics both within and beyond the Standard Model through their production mechanisms and in their propagation over cosmological distances. They carry unique information about their extreme non-thermal sources by giving insight into regions that are opaque to electromagnetic radiation. This white paper describes the opportunities astrophysical neutrino observations offer for astrophysics and high-energy physics, today and in coming years., Comment: Contribution to Snowmass 2021, updated to include community feedback
Published: 2022

10. Tau Neutrinos in the Next Decade: from GeV to EeV

Author: Abraham, Roshan Mammen, Alvarez-Muñiz, Jaime, Argüelles, Carlos A., Ariga, Akitaka, Ariga, Tomoko, Aurisano, Adam, Autiero, Dario, Bishai, Mary, Bostan, Nilay, Bustamante, Mauricio, Cummings, Austin, Decoene, Valentin, de Gouvêa, André, De Lellis, Giovanni, De Roeck, Albert, Denton, Peter B., Di Crescenzo, Antonia, Diwan, Milind V., Farzan, Yasaman, Fedynitch, Anatoli, Feng, Jonathan L., Fields, Laura J., Garcia, Alfonso, Garzelli, Maria Vittoria, Gehrlein, Julia, Glaser, Christian, Grzelak, Katarzyna, Hallmann, Steffen, Hewes, V, Indumathi, D., Ismail, Ahmed, Jana, Sudip, Jeong, Yu Seon, Kelly, Kevin J., Klein, Spencer R., Kling, Felix, Kosc, Thomas, Kose, Umut, Koskinen, D. Jason, Krizmanic, John, Lazar, Jeff, Li, Yichen, Martinez-Soler, Ivan, Mocioiu, Irina, Nam, Jiwoo, Niess, Valentin, Otte, Nepomuk, Patel, Sameer, Petti, Roberto, Prechelt, Remy L., Prohira, Steven, Rajaoalisoa, Miriama, Reno, Mary Hall, Safa, Ibrahim, Sarasty-Segura, Carlos, Senthil, R. Thiru, Stachurska, Juliana, Tomalak, Oleksandr, Trojanowski, Sebastian, Wendell, Roger Alexandre, Williams, Dawn, Wissel, Stephanie, Yaeggy, Barbara, Zas, Enrique, Zhelnin, Pavel, and Zhu, Jing-yu
Subjects: High Energy Physics - Phenomenology, Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment
Abstract: Tau neutrinos are the least studied particle in the Standard Model. This whitepaper discusses the current and expected upcoming status of tau neutrino physics with attention to the broad experimental and theoretical landscape spanning long-baseline, beam-dump, collider, and astrophysical experiments. This whitepaper was prepared as a part of the NuTau2021 Workshop., Comment: 155 pages, 63 figures, 10 tables, 69 endorsers, comments welcome, Contribution to Snowmass 2021. v2: published version
Published: 2022
Full Text: View/download PDF

11. Evolving Antennas for Ultra-High Energy Neutrino Detection

Author: Rolla, Julie, Arakaki, Dean, Clowdus, Maximilian, Connolly, Amy, Debolt, Ryan, Deer, Leo, Fahimi, Ethan, Ferstl, Eliot, Gourapura, Suren, Harris, Corey, Letwin, Luke, Machtay, Alex, Patton, Alex, Pfendner, Carl, Sbrocco, Cade, Sinha, Tom, Sipe, Ben, Staats, Kai, Trevithick, Jacob, and Wissel, Stephanie
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: Evolutionary algorithms are a type of artificial intelligence that utilize principles of evolution to efficiently determine solutions to defined problems. These algorithms are particularly powerful at finding solutions that are too complex to solve with traditional techniques and at improving solutions found with simplified methods. The GENETIS collaboration is developing genetic algorithms to design antennas that are more sensitive to ultra high energy neutrino induced radio pulses than current detectors. Improving antenna sensitivity is critical because UHE neutrinos are rare and require massive detector volumes with stations dispersed over hundreds of km squared. The GENETIS algorithm evolves antenna designs using simulated neutrino sensitivity as a measure of fitness by integrating with XFdtd, a finite difference time domain modeling program, and with simulations of neutrino experiments. The best antennas will then be deployed in ice for initial testing. The genetic algorithm's aim is to create antennas that improve on the designs used in the existing ARA experiment by more than a factor of 2 in neutrino sensitivities. This research could improve antenna sensitivities in future experiments and thus accelerate the discovery of UHE neutrinos. This is the first time that antennas have been designed using genetic algorithms with a fitness score based on a physics outcome, which will motivate the continued use of genetic algorithm designed instrumentation in astrophysics and beyond. This proceeding will report on advancements to the algorithm, steps taken to improve the genetic algorithm performance, the latest results from our evolutions, and the manufacturing road map., Comment: 9 pages including references, 6 figures, presented at 37th International Cosmic Ray Conference (ICRC 2021)
Published: 2021

12. Monte Carlo simulations of neutrino and charged lepton propagation in the Earth with nuPyProp

Author: Patel, Sameer, Reno, Mary Hall, Akaike, Yosui, Anchordoqui, Luis, Bergman, Douglas, Buckland, Isaac, Cummings, Austin, Eser, Johannes, Guépin, Claire, Krizmanic, John F., Mackovjak, Simon, Olinto, Angela, Paul, Thomas, Reustle, Alex, Romero-Wolf, Andrew, Sarazin, Fred, Venters, Tonia, Wiencke, Lawrence, and Wissel, Stephanie
Subjects: High Energy Physics - Phenomenology
Abstract: An accurate modeling of neutrino flux attenuation and the distribution of leptons they produce in transit through the Earth is an essential component to determine neutrino flux sensitivities of underground, sub-orbital and space-based detectors. Through neutrino oscillations over cosmic distances, astrophysical neutrino sources are expected to produce nearly equal fluxes of electron, muon and tau neutrinos. Of particular interest are tau neutrinos that interact in the Earth at modest slant depths to produce $\tau$-leptons. Some $\tau$-leptons emerge from the Earth and decay in the atmosphere to produce extensive air showers. Future balloon-borne and satellite-based optical Cherenkov neutrino telescopes will be sensitive to upward air showers from tau neutrino induced $\tau$-lepton decays. We present nuPyProp, a python code that is part of the nuSpaceSim package. nuPyProp generates look-up tables for exit probabilities and energy distributions for $\nu_\tau\to \tau$ and $\nu_\mu\to \mu$ propagation in the Earth. This flexible code runs with either stochastic or continuous electromagnetic energy losses for the lepton transit through the Earth. Current neutrino cross section models and energy loss models are included along with templates for user input of other models. Results from nuPyProp are compared with other recent simulation packages for neutrino and charged lepton propagation. Sources of modeling uncertainties are described and quantified., Comment: 9 pages, 6 figures, PoS(ICRC2021)1203; for associated code, see https://github.com/NuSpaceSim/nupyprop
Published: 2021
Full Text: View/download PDF

13. Radio Detection of Ultra-high Energy Cosmic Rays with Low Lunar Orbiting SmallSats

Author: Romero-Wolf, Andrés, Alvarez-Muñiz, Jaime, Anchordoqui, Luis A., Bergman, Douglas, Carvalho Jr., Washington, Cummings, Austin L., Gorham, Peter, Handmer, Casey J., Harvey, Nate, Krizmanic, John, Nishimura, Kurtis, Prechelt, Remy, Reno, Mary Hall, Schoorlemmer, Harm, Varner, Gary, Venters, Tonia, Wissel, Stephanie, and Zas, Enrique
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: Ultra-high energy cosmic rays (UHECRs) are the most energetic particles observed and serve as a probe of the extreme universe. A key question to understanding the violent processes responsible for their acceleration is identifying which classes of astrophysical objects (active galactic nuclei or starburst galaxies, for example) correlate to their arrival directions. While source clustering is limited by deflections in the Galactic magnetic field, at the highest energies the scattering angles are sufficiently low to retain correlation with source catalogues. While there have been several studies attempting to identify source catalogue correlations with data from the Pierre Auger Observatory and the Telescope Array, the significance above an isotropic background has not yet reached the threshold for discovery. It has been known for several decades that a full-sky UHECR observatory would provide a substantial increase in sensitivity to the anisotropic component of UHECRs. There have been several concepts developed in that time targeting the identification of UHECR sources such as OWL, JEM-EUSO, and POEMMA, using fluorescence detection in the Earth's atmosphere from orbit. In this white paper, we present a concept called the Zettavolt Askaryan Polarimeter (ZAP), designed to identify the source of UHECRs using radio detection of the Askaryan radio emissions produced by UHECRs interacting in the Moon's regolith from low lunar orbit., Comment: 6 pages, 2 figures, letter of interest submitted to Snowmass 2021
Published: 2020

14. Evolving Antennas for Ultra-High Energy Neutrino Detection

Author: Rolla, Julie, Connolly, Amy, Staats, Kai, Wissel, Stephanie, Arakaki, Dean, Best, Ian, Blenk, Adam, Clark, Brian, Clowdus, Maximillian, Gourapura, Suren, Harris, Corey, Hasan, Hannah, Letwin, Luke, Liu, David, Pfendner, Carl, Potter, Jordan, Sbrocco, Cade, Sinha, Tom, and Trevithick, Jacob
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Computer Science - Neural and Evolutionary Computing, Physics - Instrumentation and Detectors
Abstract: Evolutionary algorithms borrow from biology the concepts of mutation and selection in order to evolve optimized solutions to known problems. The GENETIS collaboration is developing genetic algorithms for designing antennas that are more sensitive to ultra-high energy neutrino induced radio pulses than current designs. There are three aspects of this investigation. The first is to evolve simple wire antennas to test the concept and different algorithms. Second, optimized antenna response patterns are evolved for a given array geometry. Finally, antennas themselves are evolved using neutrino sensitivity as a measure of fitness. This is achieved by integrating the XFdtd finite-difference time-domain modeling program with simulations of neutrino experiments., Comment: 8 pages including references, 6 figures, presented at 36th International Cosmic Ray Conference (ICRC 2019)
Published: 2020

15. Prospects for High-Elevation Radio Detection of >100 PeV Tau Neutrinos

Author: Wissel, Stephanie, Romero-Wolf, Andrés, Schoorlemmer, Harm, Carvalho Jr., Washington R., Alvarez-Muñiz, Jaime, Zas, Enrique, Cummings, Austin, Deaconu, Cosmin, Hughes, Kaeli, Ludwig, Andrew, Morancy, Joalda, Oberla, Eric, Paciaroni, Caroline, Prohira, Steven, Southall, Dan, Stapel-Kalat, Max, Strutt, Ben, Vasquez, Mercedes, and Vieregg, Abigail
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Tau neutrinos are expected to comprise roughly one third of both the astrophysical and cosmogenic neutrino flux, but currently the flavor ratio is poorly constrained and the expected flux at energies above $10^{17}$ eV is low. We present a detector concept aimed at measuring the diffuse flux of tau neutrinos in this energy range via a high-elevation mountaintop detector using the radio technique. The detector searches for radio signals from upgoing air showers generated by Earth-skimming tau neutrinos. Signals from several antennas in a compact array are coherently summed at the trigger level, permitting not only directional masking of anthropogenic backgrounds, but also a low trigger threshold. This design takes advantage of both the large viewing area available at high-elevation sites and the nearly full duty cycle available to radio instruments. We present trade studies that consider the station elevation, frequency band, number of antennas in the array, and the trigger threshold to develop a highly efficient station design. Such a mountaintop detector can achieve a factor of ten improvement in acceptance over existing instruments with 100 independent stations. With 1000 stations and three years of observation, it can achieve a sensitivity to an integrated $\mathcal{E}^{-2}$ flux of $<10^{-9}$ GeV cm$^{-2}$ sr$^{-1}$ s$^{-1}$, in the range of the expected flux of all-flavor cosmogenic neutrinos assuming a pure iron cosmic-ray composition., Comment: 26 pages, 11 figures
Published: 2020
Full Text: View/download PDF

16. An Andean Deep-Valley Detector for High-Energy Tau Neutrinos

Author: Romero-Wolf, Andres, Alvarez-Muñiz, Jaime, Carvalho Jr., Washington R., Cummings, Austin, Schoorlemmer, Harm, Wissel, Stephanie, Zas, Enrique, Argüelles, Carlos, Barreda, Horacio, Bazo, Jose, Bellido, Jose, Bustamante, Mauricio, Gago, Alberto, and Perca, Rolando
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract: High-energy astrophysical neutrinos, recently discovered by IceCube up to energies of several PeV, opened a new window to the high-energy Universe. Yet much remains to be known. IceCube has excellent muon flavor identification, but tau flavor identification is challenging. This limits its ability to probe neutrino physics and astrophysics. To address this limitation, we present a concept for a large-scale observatory of astrophysical tau neutrinos in the 1-100 PeV range, where a flux is guaranteed to exist. Its detection would allow us to characterize the neutrino sources observed by IceCube, to discover new ones, and test neutrino physics at high energies. The deep-valley air-shower array concept that we present provides highly background-suppressed neutrino detection with pointing resolution <1 degree, allowing us to begin the era of high-energy tau-neutrino astronomy., Comment: 15 pages, 6 figures, white paper submitted to the Latin American Strategy Forum for Research Infrastructure (LASF4RI)
Published: 2020

17. NuRadioMC: Simulating the radio emission of neutrinos from interaction to detector

Author: Glaser, Christian, García-Fernández, Daniel, Nelles, Anna, Alvarez-Muñiz, Jaime, Barwick, Steven W., Besson, Dave Z., Clark, Brian A., Connolly, Amy, Deaconu, Cosmin, de Vries, Krijn, Hanson, Jordan C., Hokanson-Fasig, Ben, Lahmann, R., Latif, Uzair, Kleinfelder, Stuart A., Persichilli, Christopher, Pan, Yue, Pfender, Carl, Plaisier, Ilse, Seckel, Dave, Torres, Jorge, Toscano, Simona, van Eijndhoven, Nick, Vieregg, Abigail, Welling, Christoph, Winchen, Tobias, and Wissel, Stephanie A.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract: NuRadioMC is a Monte Carlo framework designed to simulate ultra-high energy neutrino detectors that rely on the radio detection method. This method exploits the radio emission generated in the electromagnetic component of a particle shower following a neutrino interaction. NuRadioMC simulates everything from the neutrino interaction in a medium, the subsequent Askaryan radio emission, the propagation of the radio signal to the detector and finally the detector response. NuRadioMC is designed as a modern, modular Python-based framework, combining flexibility in detector design with user-friendliness. It includes a state-of-the-art event generator, an improved modelling of the radio emission, a revisited approach to signal propagation and increased flexibility and precision in the detector simulation. This paper focuses on the implemented physics processes and their implications for detector design. A variety of models and parameterizations for the radio emission of neutrino-induced showers are compared and reviewed. Comprehensive examples are used to discuss the capabilities of the code and different aspects of instrumental design decisions., Comment: replaced with published version
Published: 2019
Full Text: View/download PDF

18. Astrophysics Uniquely Enabled by Observations of High-Energy Cosmic Neutrinos

Author: Ackermann, Markus, Ahlers, Markus, Anchordoqui, Luis, Bustamante, Mauricio, Connolly, Amy, Deaconu, Cosmin, Grant, Darren, Gorham, Peter, Halzen, Francis, Karle, Albrecht, Kotera, Kumiko, Kowalski, Marek, Mostafa, Miguel A., Murase, Kohta, Nelles, Anna, Olinto, Angela, Romero-Wolf, Andres, Vieregg, Abigail, and Wissel, Stephanie
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Nongalactic Astrophysics, High Energy Physics - Phenomenology
Abstract: High-energy cosmic neutrinos carry unique information about the most energetic non-thermal sources in the Universe. This white paper describes the outstanding astrophysics questions that neutrino astronomy can address in the coming decade. A companion white paper discusses how the observation of cosmic neutrinos can address open questions in fundamental physics. Detailed measurements of the diffuse neutrino flux, measurements of neutrinos from point sources, and multi-messenger observations with neutrinos will enable the discovery and characterization of the most energetic sources in the Universe., Comment: White paper for the Astro2020 US decadal survey. Companion paper: "Fundamental Physics with High-Energy Cosmic Neutrinos" (1903.04333). Corresponding Authors: Markus Ahlers, Albrecht Karle, Kohta Murase, Anna Nelles, Andres Romero-Wolf, Abigail Vieregg
Published: 2019

19. Fundamental Physics with High-Energy Cosmic Neutrinos

Author: Ackermann, Markus, Ahlers, Markus, Anchordoqui, Luis, Bustamante, Mauricio, Connolly, Amy, Deaconu, Cosmin, Grant, Darren, Gorham, Peter, Halzen, Francis, Karle, Albrecht, Kotera, Kumiko, Kowalski, Marek, Mostafa, Miguel A., Murase, Kohta, Nelles, Anna, Olinto, Angela, Romero-Wolf, Andres, Vieregg, Abigail, and Wissel, Stephanie
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Nongalactic Astrophysics, High Energy Physics - Phenomenology
Abstract: High-energy cosmic neutrinos can reveal new fundamental particles and interactions, probing energy and distance scales far exceeding those accessible in the laboratory. This white paper describes the outstanding particle physics questions that high-energy cosmic neutrinos can address in the coming decade. A companion white paper discusses how the observation of cosmic neutrinos can address open questions in astrophysics. Tests of fundamental physics using high-energy cosmic neutrinos will be enabled by detailed measurements of their energy spectrum, arrival directions, flavor composition, and timing., Comment: White paper for the Astro2020 US decadal survey. Companion paper: "Astrophysics Uniquely Enabled by Observations of High-Energy Cosmic Neutrinos" (1903.04334). Corresponding Authors: Luis Anchordoqui, Mauricio Bustamante, Darren Grant, Andres Romero-Wolf, Abigail Vieregg, Stephanie Wissel
Published: 2019

20. Design and initial performance of the prototype for the BEACON instrument for detection of ultrahigh energy particles

Author: Southall, Dan, Deaconu, Cosmin, Decoene, Valentin, Oberla, Eric, Zeolla, Andrew, Alvarez-Muñiz, Jaime, Cummings, Austin, Curtis-Ginsberg, Zach, Hendrick, Angus, Hughes, Kaeli, Krebs, Ryan, Ludwig, Andrew, Mulrey, Katharine, Prohira, Steven, Carvalho, Washington Rodrigues de, Jr., Rodriguez, Andres, Romero-Wolf, Andres, Schoorlemmer, Harm, Vieregg, Abigail G., Wissel, Stephanie A., and Zas, Enrique
Published: 2023
Full Text: View/download PDF

21. Somatic Mutations and Clonal Hematopoiesis as Drivers of Age-Related Cardiovascular Risk

Author: Haring, Bernhard, Wissel, Stephanie, and Manson, JoAnn E.
Published: 2022
Full Text: View/download PDF

22. Angina pectoris? Fake News. A case report of infective endocarditis with giant aortic root abscess detected by cardiac MRI

Author: Wissel, Stephanie, primary, Drayß, Maria, additional, Christa, Martin, additional, Leyh, Rainer G, additional, and Frantz, Stefan, additional
Published: 2024
Full Text: View/download PDF

23. High-energy and ultra-high-energy neutrinos: A Snowmass white paper

Author: Ackermann, Markus, Bustamante, Mauricio, Lu, Lu, Otte, Nepomuk, Reno, Mary Hall, Wissel, Stephanie, Agarwalla, Sanjib K., Alvarez-Muñiz, Jaime, Alves Batista, Rafael, Argüelles, Carlos A., Clark, Brian A., Cummings, Austin, Das, Sudipta, Decoene, Valentin, Denton, Peter B., Dornic, Damien, Dzhilkibaev, Zhan-Arys, Farzan, Yasaman, Garcia, Alfonso, Garzelli, Maria Vittoria, Glaser, Christian, Heijboer, Aart, Hörandel, Jörg R., Illuminati, Giulia, Seon Jeong, Yu, Kelley, John L., Kelly, Kevin J., Kheirandish, Ali, Klein, Spencer R., Krizmanic, John F., Larson, Michael J., Murase, Kohta, Narang, Ashish, Prechelt, Remy L., Prohira, Steven, Resconi, Elisa, Santander, Marcos, Valera, Victor B., Vandenbroucke, Justin, Vasil'evna Suvorova, Olga, Wiencke, Lawrence, Yoshida, Shigeru, Yuan, Tianlu, Zas, Enrique, Zhelnin, Pavel, Zhou, Bei, Anchordoqui, Luis A., Ashida, Yosuke, Bagheri, Mahdi, Balagopal, Aswathi, V, Basu, Vedant, Beatty, James, Bechtol, Keith, Bell, Nicole, Bishop, Abigail, Book, Julia, Brown, Anthony, Burgman, Alexander, Campana, Michael, Chau, Nhan, Chen, Thomas Y., Coleman, Alan, Connolly, Amy, Conrad, Janet M., Correa, Pablo, Creque-Sarbinowski, Cyril, Curtis-Ginsberg, Zachary, Dasgupta, Paramita, De Kockere, Simon, de Vries, Krijn, Deaconu, Cosmin, Desai, Abhishek, DeYoung, Tyce, di Matteo, Armando, Elsaesser, Dominik, Fürst, Phillip, Fan, Kwok Lung, Fedynitch, Anatoli, Fox, Derek, Ganster, Erik, Minh, Martin Ha, Haack, Christian, Hallman, Steffen, Halzen, Francis, Haungs, Andreas, Ishihara, Aya, Judd, Eleanor, Karg, Timo, Karle, Albrecht, Katori, Teppei, Kochocki, Alina, Kopper, Claudio, Kowalski, Marek, Kravchenko, Ilya, Kurahashi, Naoko, Lamoureux, Mathieu, León Vargas, Hermes, Lincetto, Massimiliano, Liu, Qinrui, Madsen, Jim, Makino, Yuya, Mammo, Joseph, Marka, Zsuzsa, Mayotte, Eric, Meagher, Kevin, Meier, Maximilian, Miramonti, Lino, Moulai, Marjon, Mulrey, Katharine, Muzio, Marco, Naab, Richard, Nelles, Anna, Nichols, William, Nozdrina, Alisa, O'Sullivan, Erin, OD́ell, Vivian, Osborne, Jesse, Pandey, Vishvas, Paudel, Ek Narayan, Pizzuto, Alex, Plum, Mattias, Pobes Aranda, Carlos, Pyras, Lilly, Raab, Christoph, Rechav, Zoe, Rojo, Juan, Romero Matamala, Oscar, Savina, Pierpaolo, Schroeder, Frank, Schumacher, Lisa, Sciutto, Sergio, Sclafani, Stephen, Ful Hossain Seikh, Mohammad, Silva, Manuel, Singh, Rajeev, Smith, Daniel, Spencer, Samuel Timothy, Springer, Robert Wayne, Stachurska, Juliana, Suvorova, Olga, Taboada, Ignacio, Toscano, Simona, Tueros, Matias, Twagirayezu, Jean Pierre, van Eijndhoven, Nick, Veres, Péter, Vieregg, Abigail, Wang, Winnie, Whitehorn, Nathan, Winter, Walter, Yildizci, Emre, and Yu, Shiqi
Published: 2022
Full Text: View/download PDF

24. A lower bound on the number of cosmic ray events required to measure source catalogue correlations

Author: Dolci, Marco, Romero-Wolf, Andrew, and Wissel, Stephanie
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: Recent analyses of cosmic ray arrival directions have resulted in evidence for a positive correlation with active galactic nuclei positions that has weak significance against an isotropic source distribution. In this paper, we explore the sample size needed to measure a highly statistically significant correlation to a parent source catalogue. We compare several scenarios for the directional scattering of ultra-high energy cosmic rays given our current knowledge of the galactic and intergalactic magnetic fields. We find significant correlations are possible for a sample of $>$1000 cosmic ray protons with energies above 60 EeV., Comment: 23 pages, 9 figures
Published: 2015
Full Text: View/download PDF

25. Modeling Neutrino and Background Signals for the Payload for Ultrahigh Energy Observations (PUEO) Experiment

Author: Cummings Austin, Krizmanic John, and Wissel Stephanie
Subjects: Physics, QC1-999
Abstract: In the current age of multi-messenger astrophysics, Very High Energy (VHE) cosmic neutrinos (E > 1 PeV) represent a unique observation window into the most extreme astrophysical events in the universe. Measurements of the neutrino flux in this high energy regime provide information regarding the distribution and composition of Ultra-High Energy Cosmic Rays (UHECR), details of source acceleration mechanics, and definitive tests of physics beyond the standard model. Observations in multiple different detection channels (e.g. optical, radio, direct particle counting) are being explored to extend the sensitivity to neutrinos above PeV energies. The Payload for Ultrahigh Energy Observations (PUEO) is a long duration balloon experiment that builds on the successes of the Antarctic Impulsive Transient Antenna (ANITA) experiment to probe the cosmic neutrino flux above EeV energies. PUEO, like ANITA, seeks to measure coherent radio emission in the form of Askaryan emission from in-ice neutrino interactions and both geomagnetic and Askaryan emission from Extensive Air Showers (EAS) produced by the decays of Earth-emergent τ-leptons sourced from τ neutrinos. To evaluate the sensitivity of PUEO (and other detectors) to a given flux of neutrinos, it is necessary to accurately model i) the propagation of neutrinos through the Earth ii) the emission generated from the neutrino-sourced particle shower iii) the detector performance to a generated signal and iv) relevant backgrounds. Numerous software frameworks exist to model these different mechanisms independently, but often require significant work to use together. ν SpaceSim is an open source, end-to-end neutrino simulation package that models these described mechanisms for an arbitrary detector geometry in both the optical and radio emission channels. For a given experimental design,ν SpaceSim is designed to model the sensitivity to both the cosmogenic neutrino flux and to astrophysical neutrino transient events. The highly modular design of ν SpaceSim allows for comparison and exploration of different physics models within the same code base. In this contribution, we detail the state of the ν SpaceSim code as it pertains to modeling the sensitivity of the PUEO experiment, and highlight the mechanisms necessary to perform this calculation. We also describe the near-term improvements to the radio emission calculation in ν SpaceSim and the modeling of the most relevant backgrounds for PUEO: the direct (above-the-limb) cosmic rays, and the indirect (ice-reflected) cosmic ray signals.
Published: 2023
Full Text: View/download PDF

26. Radiofrequency ice dielectric measurements at Summit Station, Greenland

Author: Aguilar, Juan Antonio, primary, Allison, Patrick, additional, Besson, Dave, additional, Bishop, Abby, additional, Botner, Olga, additional, Bouma, Sjoerd, additional, Buitink, Stijn, additional, Cataldo, Maddalena, additional, Clark, Brian A., additional, Couberly, Kenny, additional, Curtis-Ginsberg, Zach, additional, Dasgupta, Paramita, additional, de Kockere, Simon, additional, de Vries, Krijn D., additional, Deaconu, Cosmin, additional, DuVernois, Michael A., additional, Eimer, Anna, additional, Glaser, Christian, additional, Hallgren, Allan, additional, Hallmann, Steffen, additional, Hanson, Jordan Christian, additional, Hendricks, Bryan, additional, Henrichs, Jakob, additional, Heyer, Nils, additional, Hornhuber, Christian, additional, Hughes, Kaeli, additional, Karg, Timo, additional, Karle, Albrecht, additional, Kelley, John L., additional, Korntheuer, Michael, additional, Kowalski, Marek, additional, Kravchenko, Ilya, additional, Krebs, Ryan, additional, Lahmann, Robert, additional, Latif, Uzair, additional, Mammo, Joseph, additional, Marsee, Matthew J., additional, Meyers, Zachary S., additional, Michaels, Kelli, additional, Mulrey, Katharine, additional, Muzio, Marco, additional, Nelles, Anna, additional, Novikov, Alexander, additional, Nozdrina, Alisa, additional, Oberla, Eric, additional, Oeyen, Bob, additional, Plaisier, Ilse, additional, Punsuebsay, Noppadol, additional, Pyras, Lilly, additional, Ryckbosch, Dirk, additional, Scholten, Olaf, additional, Seckel, David, additional, Seikh, Mohammad Ful Hossain, additional, Smith, Daniel, additional, Stoffels, Jethro, additional, Southall, Daniel, additional, Terveer, Karen, additional, Toscano, Simona, additional, Tosi, Delia, additional, Van Den Broeck, Dieder J., additional, van Eijndhoven, Nick, additional, Vieregg, Abigail G., additional, Vischer, Janna Z., additional, Welling, Christoph, additional, Williams, Dawn R., additional, Wissel, Stephanie, additional, Young, Robert, additional, and Zink, Adrian, additional
Published: 2023
Full Text: View/download PDF

27. Updated studies of radio propagation through polar firn using paraPropPython

Author: Kyriacou, Alexander, primary, Allison, Patrick, additional, Beatty, James, additional, Besson, Dave, additional, Connolly, Amy, additional, Cummings, Austin, additional, Deaconu, Cosmin, additional, De Kockere, Simon, additional, de Vries, Krijn, additional, Frikken, Dylan, additional, HAST, Carsten, additional, Huesca Santiago, Erique, additional, Kuo, Chung-Yun, additional, Kyriacou, Alex, additional, Latif, Uzair Abdul, additional, Lukic, Vesna, additional, Mulrey, Katharine, additional, Nam, Jiwoo, additional, Nivedita, Krishna, additional, Nozdrina, Alisa, additional, Oberla, Eric, additional, Prohira, Steven, additional, Ralston, John, additional, Seikh, Mohammad, additional, Stanley, Rose S, additional, Toscano, Simona, additional, Van den Broeck, Dieder, additional, van Eijndhoven, Nick, additional, and Wissel, Stephanie, additional
Published: 2023
Full Text: View/download PDF

28. Using Genetic Algorithms to Optimize Antenna Designs for Improved Sensitivity to Ultra-High Energy Neutrinos

Author: Machtay, Alexander Louis, primary, Patton, Alex, additional, Rolla, Julie Anne, additional, Banzhaf, Wolfgang, additional, Calderon, Dennis, additional, Chen, Chi-Chih, additional, Connolly, Amy, additional, Debolt, Ryan, additional, Fahimi, Ethan, additional, King, Nick, additional, Legersky, Maya, additional, Melotti, Ezio, additional, Reynolds, Bryan, additional, Sipe, Ben, additional, Staats, Kai, additional, Stephens, Autumn, additional, Tillman, Jack, additional, Weiler, Jacob, additional, Wells, Dylan, additional, Wissel, Stephanie, additional, and Zinn, Audrey, additional
Published: 2023
Full Text: View/download PDF

29. Using Genetic Algorithms to Evolve Antenna Gain Patterns with Greater Sensitivity to Ultra-High Energy Neutrinos

Author: Reynolds, Bryan, primary, Rolla, Julie Anne, additional, Fahimi, Ethan, additional, Banzhaf, Wolfgang, additional, Calderon, Dennis, additional, Chen, Chi-Chih, additional, Connolly, Amy, additional, Debolt, Ryan, additional, King, Nick, additional, Legersky, Maya, additional, Machtay, Alex, additional, Melotti, Ezio, additional, Patton, Alex, additional, Sipe, Ben, additional, Staats, Kai, additional, Stephens, Autumn, additional, Tillman, Jack, additional, Weiler, Jacob, additional, Wells, Dylan, additional, Wissel, Stephanie, additional, and Zinn, Audrey, additional
Published: 2023
Full Text: View/download PDF

30. TAMBO: Searching for Tau Neutrinos in the Peruvian Andes

Author: Thompson, Will, primary, Alvarez-Muniz, Jaime, additional, Argüelles, Carlos, additional, Bazo, Jose, additional, Bellido, Jose, additional, Bustamante, Mauricio, additional, Cummings, Austion, additional, Delgado, Diyaselis, additional, Fernández, Pablo, additional, Gago, Alberto, additional, Garcia-Soto, Alfonso, additional, Kheirandish, Ali, additional, Lazar, Jeffrey, additional, Romero-Wolf, Andres, additional, Safa, Ibrahim, additional, Schoorlemmer, Harm, additional, Vincent, Aaron, additional, Wissel, Stephanie, additional, Zas, Enrique, additional, Zhelnin, Pavel, additional, and Jr., Washington Carvalho, additional
Published: 2023
Full Text: View/download PDF

31. Results from a low-threshold ultrahigh-energy neutrino search with the Askaryan Radio Array

Author: Hughes, Kaeli Autumn, primary, Allison, Patrick, additional, Archambault, S., additional, Beatty, James, additional, Besson, David Zeke, additional, Bishop, Abigail, additional, Chen, C.C., additional, Chen, C.H., additional, Chen, P., additional, Chen, Y.C., additional, Clark, Brian, additional, Clay, W., additional, Connolly, Amy, additional, Cremonesi, Linda, additional, Dasgupta, Paramita, additional, Davies, J., additional, de Cocker, Simon, additional, de Vries, Krijn, additional, Deaconu, Cosmin, additional, DuVernois, Michael, additional, Flaherty, Justin, additional, Friedman, Elizabeth, additional, Gaior, R., additional, Hanson, Jordan, additional, Harty, N., additional, Hendricks, Bryan L., additional, Hoffman, Kara, additional, Hong, Eugene, additional, Hsu, S.Y., additional, Hu, L., additional, Huang, J.J., additional, Huang, M.-H. A., additional, Ishihara, A., additional, Karle, Albrecht, additional, Kelley, John, additional, Kim, K.-C., additional, Kim, M.-C., additional, Kravchenko, I., additional, Krebs, Ryan, additional, Ku, Yuchieh, additional, Kuo, C.Y., additional, Kurusu, K., additional, Landsman, H., additional, Latif, Uzair Abdul, additional, Li, C.-J., additional, Liu, T.-C., additional, Lu, M.-Y., additional, Madison, B., additional, Madison, K., additional, Mase, K., additional, Meures, Thomas, additional, Nam, J., additional, Nichol, Ryan James, additional, Nir, G., additional, Novikov, A., additional, Nozdrina, Alisa, additional, Oberla, Eric, additional, Osborn, J., additional, Pan, Yue, additional, Pfendner, Carl G, additional, Punsuebsay, N., additional, Roth, J., additional, Seckel, David, additional, Shiao, Y.-S., additional, Shultz, A., additional, Smith, Daniel, additional, Toscano, Simona, additional, Torres, Jorge, additional, Touart, J., additional, van Eijndhoven, Nick, additional, Varner, Gary, additional, Vieregg, Abigail G., additional, Wang, M.-Z., additional, Wang, S.-H., additional, Want, Y.H., additional, Wissel, Stephanie, additional, Xie, C., additional, Yoshida, S., additional, Young, R., additional, and Seikh, M. F. H., additional
Published: 2023
Full Text: View/download PDF

32. Detection of Radio Emission by Cosmic Rays with the BEACON Prototype

Author: Zeolla, Andrew James, primary, Alvarez-Muniz, Jaime, additional, Cummings, Austin, additional, Deaconu, Cosmin, additional, Decoene, Valentin, additional, Hughes, Kaeli Autumn, additional, Krebs, Ryan, additional, Ludwig, Andrew, additional, Mulrey, Katie, additional, Oberla, Eric, additional, Prohira, Steven, additional, Jr., Washington Carvalho, additional, Romero-Wolf, Andres, additional, Schoorlemmer, Harm, additional, Southall, Daniel, additional, Vieregg, Abigail G., additional, Wissel, Stephanie, additional, and Zas, Enrique, additional
Published: 2023
Full Text: View/download PDF

33. The Radar Echo Telescope for Cosmic Rays

Author: Stanley, Rose S, primary, Allison, Patrick, additional, Beatty, James, additional, Besson, Dave, additional, Connolly, Amy, additional, Cummings, Austin, additional, Deaconu, Cosmin, additional, De Kockere, Simon, additional, de Vries, Krijn, additional, Frikken, Dylan, additional, HAST, Carsten, additional, Huesca Santiago, Enrique, additional, Kuo, Chung-Yun, additional, Kyriacou, Alex, additional, Latif, Uzair Abdul, additional, Lukic, Vesna, additional, Mulrey, Katharine, additional, Nam, Jiwoo, additional, Nivedita, Krishna, additional, Nozdrina, Alisa, additional, Oberla, Eric, additional, Prohira, Steven, additional, Ralston, John, additional, Seikh, Mohammad, additional, Toscano, Simona, additional, Van den Broeck, Dieder, additional, van Eijndhoven, Nick, additional, and Wissel, Stephanie, additional
Published: 2023
Full Text: View/download PDF

34. Particle Astrophysics at Zettavolt Energies with Radio Detectors in Low Lunar Orbit

Author: Romero-Wolf, Andrew, Alvarez-Muñiz, Jaime, Anchordoqui, Luis A, Bergman, Douglas, Carvalho Jr., Washington, Cummings, Austin L, Gorham, Peter, Handmer, Casey J, Harvey, Nate, Krizmanich, John, Nishimura, Kurtis, Prechelt, Remy, Reno, Mary Hall, Schoorlemmer, Harm, Varner, Gary, Venters, Tonia, Wissel, Stephanie, and Zas, Enrique
Published: 2021

35. Particle Astrophysics at Zettavolt Energies with Radio Detectors in Low Lunar Orbit

Author: Zas, Enrique, Wissel, Stephanie, Venters, Tonia, Varner, Gary, Schoorlemmer, Harm, Reno, Mary Hall, Prechelt, Remy, Nishimura, Kurtis, Krizmanich, John, Harvey, Nate, Handmer, Casey J, Gorham, Peter, Cummings, Austin L, Carvalho Jr., Washington, Bergman, Douglas, Anchordoqui, Luis A, Alvarez-Muñiz, Jaime, and Romero-Wolf, Andrew
Published: 2021

36. The Beamforming Elevated Array for COsmic Neutrinos (BEACON): A Radio Detector for Earth-Skimming Tau Neutrinos

Author: Zeolla, Andrew James, primary, Alvarez-Muniz, Jaime, additional, Cummings, Austin, additional, Curtis-Ginsberg, Zachary, additional, Deaconu, Cosmin, additional, Decoene, Valentin, additional, Hendrick, Angus, additional, Hughes, Kaeli Autumn, additional, Krebs, Ryan, additional, Ludwig, Andrew, additional, Mulrey, Katie, additional, Oberla, Eric, additional, Prohira, Steven, additional, Rodrigues de Carvalho, Washington, additional, Rodriguez, A., additional, Romero-Wolf, Andres, additional, Schoorlemmer, Harm, additional, Southall, Dan, additional, Vieregg, Abigail G., additional, Wissel, Stephanie, additional, and Zas, Enrique, additional
Published: 2023
Full Text: View/download PDF

37. Prospects for joint cosmic ray and neutrino constraints on the evolution of trans-Greisen-Zatsepin-Kuzmin proton sources

Author: Muzio, Marco Stein, primary, Unger, Michael, additional, and Wissel, Stephanie, additional
Published: 2023
Full Text: View/download PDF

38. Neutrino propagation in the Earth and emerging charged leptons with nuPyProp

Author: Garg, Diksha, primary, Patel, Sameer, additional, Reno, Mary Hall, additional, Reustle, Alexander, additional, Akaike, Yosui, additional, Anchordoqui, Luis A., additional, Bergman, Douglas R., additional, Buckland, Isaac, additional, Cummings, Austin L., additional, Eser, Johannes, additional, Garcia, Fred, additional, Guépin, Claire, additional, Heibges, Tobias, additional, Ludwig, Andrew, additional, Krizmanic, John F., additional, Mackovjak, Simon, additional, Mayotte, Eric, additional, Mayotte, Sonja, additional, Olinto, Angela V., additional, Paul, Thomas C., additional, Romero-Wolf, Andrés, additional, Sarazin, Frédéric, additional, Venters, Tonia M., additional, Wiencke, Lawrence, additional, and Wissel, Stephanie, additional
Published: 2023
Full Text: View/download PDF

39. Tau neutrinos in the next decade: from GeV to EeV

Author: Abraham, Roshan Mammen, primary, Alvarez-Muñiz, Jaime, additional, Argüelles, Carlos A, additional, Ariga, Akitaka, additional, Ariga, Tomoko, additional, Aurisano, Adam, additional, Autiero, Dario, additional, Bishai, Mary, additional, Bostan, Nilay, additional, Bustamante, Mauricio, additional, Cummings, Austin, additional, Decoene, Valentin, additional, de Gouvêa, André, additional, De Lellis, Giovanni, additional, De Roeck, Albert, additional, Denton, Peter B, additional, Di Crescenzo, Antonia, additional, Diwan, Milind V, additional, Farzan, Yasaman, additional, Fedynitch, Anatoli, additional, Feng, Jonathan L, additional, Fields, Laura J, additional, Garcia, Alfonso, additional, Garzelli, Maria Vittoria, additional, Gehrlein, Julia, additional, Glaser, Christian, additional, Grzelak, Katarzyna, additional, Hallmann, Steffen, additional, Hewes, Jeremy, additional, Indumathi, D, additional, Ismail, Ahmed, additional, Jana, Sudip, additional, Jeong, Yu Seon, additional, Kelly, Kevin J, additional, Klein, Spencer R, additional, Kling, Felix, additional, Kosc, Thomas, additional, Kose, Umut, additional, Koskinen, D Jason, additional, Krizmanic, John, additional, Lazar, Jeff, additional, Li, Yichen, additional, Martinez-Soler, Ivan, additional, Mocioiu, Irina, additional, Nam, Jiwoo, additional, Niess, Valentin, additional, Otte, Nepomuk, additional, Patel, Sameer, additional, Petti, Roberto, additional, Prechelt, Remy L, additional, Prohira, Steven, additional, Rajaoalisoa, Miriama, additional, Reno, Mary Hall, additional, Safa, Ibrahim, additional, Sarasty-Segura, Carlos, additional, Senthil, R Thiru, additional, Stachurska, Juliana, additional, Tomalak, Oleksandr, additional, Trojanowski, Sebastian, additional, Wendell, Roger Alexandre, additional, Williams, Dawn, additional, Wissel, Stephanie, additional, Yaeggy, Barbara, additional, Zas, Enrique, additional, Zhelnin, Pavel, additional, and Zhu, Jing-yu, additional
Published: 2022
Full Text: View/download PDF

40. Concept and analysis for a 1-10 PeV Tau Neutrino observatory

Author: Romero-Wolf, Andres, Carvalho, Washington, Alvarez-Muniz, Jaime, Cummings, Austin, Schoorlemmer, Harm, Wissel, Stephanie, and Zas, Enrique
Published: 2019

41. Concept and analysis for a 1-10 PeV Tau Neutrino observatory

Author: Zas, Enrique, Wissel, Stephanie, Schoorlemmer, Harm, Cummings, Austin, Alvarez-Muniz, Jaime, Carvalho, Washington, and Romero-Wolf, Andres
Abstract: UNKNOWN
Published: 2019

42. A New Concept for High-Elevation Radio Detection of Tau Neutrinos

Author: Wissel Stephanie, Alvarez-Muñiz Jaime, Carvalho Washington R., Romero-Wolf Andrés, Schoorlemmer Harm, and Zas Enrique
Subjects: Physics, QC1-999
Abstract: Cosmic neutrinos are expected to include a significant flux of tau neutrinos due to flavor mixing over astronomical length scales. However, the tau-neutrino content of astrophysical neutrinos is poorly constrained and a significant flux of cosmogenic tau neutrinos awaits discovery. Earth-skimming tau neutrinos undergo charged-current interactions that result in a tau lepton exiting the Earth. The tau lepton decay generates anextensive air shower and geomagnetic radio emission. To target the tau neutrinos, we present a new tau neutrino detector concept that uses phased antenna arrays placed on high elevation mountains. Simulation studies indicate that a modest array size and small number of stations can achieve competitive sensitivity, provided the receivers are at highs enough elevation.
Published: 2019
Full Text: View/download PDF

43. Importance of cognitive performance for generic and disease-specific quality of life in chronic heart failure

Author: Wissel, Stephanie
Subjects: Versorgungsprogramm, Chronische Herzinsuffizienz, ddc:610, Selbstwirksamkeit, 610 Medizin und Gesundheit, Lebensqualität
Abstract: Cognitive impairment is highly prevalent in patients with chronic heart failure, but little is known about the health-related quality of life (HRQL) of this special patient group. We aimed to examine whether cognitive impairment is associated with HRQL in heart failure patients and hypothesized that cognitive impairment would negatively impact HRQL. We examined the HRQL of 148 patients of the Cognition.Matters-HF study with chronic heart failure and objectified cognitive impairment ranging from no to severe deficits. With the exception of the self-efficacy scale of the KCCQ, cognitive impairment was not associated with lower health-related quality of life in heart failure patients. The association of self-efficacy with severity of cognitive impairment remained significant after adjustment for duration and severity of heart failure, age, and sex (p, Kognitive Beeinträchtigungen sind bei Patient*innen mit chronischer Herzinsuffizienz weit verbreitet. Auswertungen der Beobachtungsstudie „Cognition.Matters-HF“ konnten belegen, dass Patient*innen mit einer Herzschwäche häufig Gedächtnisstörungen und Aufmerksamkeitsdefizite aufweisen. Die Evidenz für einen Zusammenhang zwischen Kognition und Lebensqualität bei Herzinsuffizienz ist jedoch spärlich. Unser Ziel war es zu untersuchen, ob kognitive Einschränkungen Auswirkungen auf die Lebensqualität (HRQL) von Herzinsuffizienzpatient*innen haben. Anhand der Cognition.Matters-HF Kohorte untersuchten wir die HRQL von 148 Patient*innen mit chronischer Herzinsuffizienz und objektivierten kognitiven Beeinträchtigungen, die von keinen bis hin zu schweren Defiziten reichten. Die Lebensqualität der Teilnehmer*innen wurde über die beiden Selbstbeurteilungsfragebögen, Short Form-36 (SF-36) und Kansas City Cardiomyopathy Questionnaire (KCCQ), erfasst. Mit Ausnahme der Selbstwirksamkeitsskala des KCCQ war der Schweregrad der kognitiven Beeinträchtigung nicht mit Einschränkungen in der Lebensqualität bei Patient*innen mit chronischer Herzinsuffizienz verbunden. Der Zusammenhang zwischen Selbstwirksamkeit und Schweregrad der kognitiven Beeinträchtigung blieb auch nach Anpassung für Dauer und Schweregrad der Herzinsuffizienz, Alter und Geschlecht der Teilnehmer signifikant bestehen (p
Published: 2022
Full Text: View/download PDF

44. Radiofrequency Ice Dielectric Measurements at Summit Station, Greenland

Author: Aguilar, Juan Antonio, Allison, Patrick, Besson, Dave, Bishop, Abby, Botner, Olga, Bouma, Sjoerd, Butink, Stijn, Cataldo, Maddalena, Clark, Brian, Couberly, Kenneth, Curtis-Ginsberg, Zachary, Dasgupta, Paramita, De Kickere, Simon, De Vries, Krijn, Deaconu. Cosmin, DuVernois, Michael, Eimer, Anna, Glaser, Christian, Hallgren, Allan, Hallmann, Steffen, Hanson, Jordan, Hendricks, Bryan, Hendrichs, Jakob, Heyer, Nils, Hornhuber, C, Hughes, Kaeli, Karg, Timo, Karle, Albrecht, Kelley, J. L., Korntheuer, Michael, Kowalski, Marek, Kravchenko, Ilja, Lahman, Robert, Latif, Uzair, Mammo, Joseph, Marsee, Matthew, Meyers, Zachary, Michaels, Kelli, Mulrey, Katharine, Muzio, Marco, Nelles, Anna, Novikov, A., Nozdrina, Alisa, Oberla, Eric, Oyen, Bob, Plaisier, Ilse, Punsuebsay, Noppadol, Pyras, Lilly, Ryckbosch, Dirk, Scholten, Olaf, Seckel, Dave, Seikh, Mohammad, Smith, Daniel, Stoffels, Jethro, Southal, Daniel, Terveer, Karen, Toscano, Simona, Tosi, Delia, Ven Den Broeck, Dieder, Van Eijndhoven, Nick, Vieregg, Abigail, Vischer, Janna, Welling, Christoph, Williams, Dawn, Wissel, Stephanie, Young, R, and Zink, Adrian
Abstract: We recently reported on the radio-frequency attenuation length of cold polar ice at Summit Station, Greenland, based on bistatic radar measurements of radio- frequency bedrock echo strengths taken during the summer of 2021. Those data also include echoes attributed to stratified impurities or dielectric discontinuities within the ice sheet (“lay-ers"), which allow studies of a) estimation of the relative contribution of coherent (discrete layers, e.g.) vs. incoherent (bulk volumetric, e.g.) scattering, b) the magnitude of internal layer reflection coefficients, c) limits on the azimuthal asymmetry of reflections (‘birefringence’), and d) limits on signal dispersion in-ice over a bandwidth of ∼100 MHz. We find that i) after averaging 10000 echo triggers, reflected signal observable over the thermal floor (to depths of approximately 1500 m) are consistent with being entirely coherent, ii) internal layer reflection coefficients are measured at approximately –60 to –70 dB, iii) birefringent effects for vertically propagating signals are smaller by an order of magnitude relative to comparable studies per- formed at South Pole, and iv) within our experimental limits, glacial ice is non-dispersive over the frequency band relevant for neutrino detection experiments.
Published: 2022
Full Text: View/download PDF

45. Concept Study of a Radio Array Embedded in a Deep Gen2-like Optical Array

Author: IceCube-Gen2 Collaboration, Abbasi, Rasha, Ackermann, Markus, Adams, Jenni, Aguilar, Juanan, Ahlers, M., Ahrens, Maryon, Alispach, Cyril Martin, Allison, Patrick, Alves Junior, Antonio Augusto, Amin, Najia Moureen Binte, An, Rui, Andeen, Karen, Anderson, Tyler, Anton, Gisela, Arguelles, Carlos, Arlen, Tim, Ashida, Yosuke, Axani, Spencer, Bai, Xinhua, Balagopal V., Aswathi, Barbano, Anastasia Maria, Bartos, I., Barwick, S. W., Bastian, Benjamin, Basu, Vedant, Baur, Sebastian, Bay, R. C., Beatty, J. J., Becker, K. H., Becker Tjus, Julia, Bellenghi, Chiara, BenZvi, Segev, Berley, D., Bernardini, Elisa, Besson, D. Z., Binder, Gary, Bindig, Daniel, Bishop, Abby, Blaufuss, E., Blot, Summer, Boddenberg, Matthias, Bohmer, Michael, Bontempo, Federico, Borowka, Jürgen, Boser, S., Botner, Olga, Böttcher, Jakob, Bourbeau, Etienne, Bradascio, Federica, Braun, J., Bron, Stephanie, Brostean-Kaiser, Jannes, Browne, Sally-Ann, Burgman, Alexander, Burley, Ryan, Busse, Raffaela, Campana, Michael, Carnie-Bronca, Erin, Cataldo, Maddalena, Chen, Chujie, Chirkin, Dmitry, Choi, Koun, Clark, Brian, Clark, Kenneth, Clark, Rogan, Classen, Lew, Coleman, Alan, Collin, Gabriel, Connolly, Amy, Conrad, J. M., Coppin, Paul, Correa, Pablo, Cowen, D. F., Cross, R., Dappen, Christian, Dave, Pranav, Deaconu, Cosmin, DE CLERCQ, Catherine, De Kockere, Simon, DeLaunay, James, Dembinski, Hans, Deoskar, Kunal, De Ridder, Sam, Desai, Abhishek, Desiati, Paolo, de Vries, Krijn, de Wasseige, Gwenhaël, De With, Meike, DeYoung, Tyce, Dharani, Sukeerthi, Diaz, Alejandro, Diaz-Velez, Juan Carlos, Dittmer, Markus, Dujmovic, Hrvoje, Dunkman, Matt, DuVernois, Michael, Dvorak, Emily, Ehrhardt, Thomas, Eller, Philipp, Engel, Ralph, Erpenbeck, Hannah, Evans, John, Evenson, P. A., Fan, Kwok Lung, Farrag, K., Fazely, A. R., Fiedlschuster, Sebastian, Fienberg, Aaron, Filimonov, Kirill, Finley, Chad, Fischer, Leander, Fox, Derek B., Franckowiak, Anna, Friedman, Elizabeth, Fritz, Alexander, Fürst, Philipp, Gaisser, T. K., Gallagher, Jay, Ganster, Erik, Garcia, Alfonso, Garrappa, Simone, Gartner, Andreas, Gerhardt, L., Gernhaeuser, Roman, Ghadimi, Ava, Giri, Pawan, Glaser, Christian, Glauch, Theo, Glusenkamp, Thorsten, Goldschmidt, A., Gonzalez, Javier, Goswami, Sreetama, Grant, Darren, Grégoire, Timothée, Griswold, Spencer, Gunduz, Mehmet, Günther, Christoph, Haack, Christian, Hallgren, Allan, Halliday, R., Hallmann, Steffen, Halve, Lasse Yannik, Halzen, F., Ha Minh, Martin, Hanson, Kael, Hardin, John, Harnisch, Alexander A., Haugen, Jim, Haungs, Andreas, Hauser, Simon, Hebecker, Dustin, Heinen, Dirk, Helbing, K., Hendricks, Brian, Henningsen, Felix, Hettinger, Emma C., Hickford, Stephanie, Hignight, Joshua, Hill, Colton, Hill, G. C., Hoffman, Kara, Hoffmann, Benjamin, Hoffmann, Ruth, Hoinka, Tobias, Hokanson-Fasig, Benjamin, Holzapfel, Killian, Hoshina, K., Huang, Feifei, Huber, Matthias, Huber, Thomas, Huege, Tim, Hughes, Kaeli, Hultqvist, Klas, Hunnefeld, Mirco, Hussain, Raamis, In, Seongjin, Iovine, Nadège, Ishihara, Aya, Jansson, Matti, Japaridze, George, Jeong, Minjin, Jones, Ben, KALEKIN, Oleg, Kang, Donghwa, Kang, Woosik, Kang, Xinyue, Kappes, Alexander, Kappesser, David, Karg, Timo, Karl, Martina, Karle, Albrecht, Katori, Teppei, Katz, U., Kauer, M., Keivani, A., Kellermann, Moritz, Kelley, J. L., Kheirandish, Ali, Kin, Ken'ichi, Kintscher, Thomas, Kiryluk, Joanna, Klein, Spencer, Koirala, Ramesh, Kolanoski, Hermann, Kontrimas, Tomas, Kopke, Lutz, Kopper, Claudio, Kopper, Sandro, Koskinen, D. J., Koundal, Paras, Kovacevich, Michael, Kowalski, Marek, Kozynets, Tetiana, Krauss, Carsten, Kravchenko, Ilya, Krebs, Ryan, Kun, Emma, Kurahashi, Naoko, Lad, Neha, Lagunas Gualda, Cristina, Lanfranchi, Justin, Larson, M. J., Lauber, Frederik Hermann, Lazar, Jeffrey, Lee, Jiwoong, Leonard, Kayla, Leszczyńska, Agnieszka, Li, Yijia, Lincetto, Massimiliano, Liu, Qinrui, Liubarska, Maria, Lohfink, Elisa, LoSecco, John, Lozano Mariscal, Cristian Jesus, Lu, Lu, Lucarelli, Francesco, Ludwig, Andrew, Luszczak, William, Lyu, Yang, Ma, Wing Yan, Madsen, James, Mahn, Kendall, Makino, Yuya, Mancina, Sarah, Mandalia, S., Maris, Ioana Codrina, Marka, Szabolcs, Marka, Zsuzsa, Maruyama, Reina H., Mase, K., McElroy, Thomas, McNally, Frank, Mead, James Vincent, Meagher, K., Medina, Andres, Meier, Maximilian, Meighen-Berger, Stephan, Meyers, Zackary, Micallef, Jessie, Mockler, Daniela, Montaruli, Teresa, Moore, Roger, Morse, R., Moulai, Marjon, Naab, Richard, Nagai, Ryo, Naumann, Uwe, Necker, Jannis, Nelles, Anna, Nguyen, Le Viet, Niederhausen, Hans, Nisa, Mehr, Nowicki, Sarah, Nygren, Dave, Oberla, Eric, Obertacke Pollmann, Anna, Oehler, Marie, Olivas, A., Omeliukh, Anastasiia, O'Sullivan, Erin, Pandya, Hershal, Pankova, Daria, Papp, Laszlo, Park, Nahee, Parker, Grant, Paudel, Ek Narayan, Paul, Larissa, Perez de los Heros, Carlos, Peters, Lilly, Petersen, Troels, Peterson, Josh, Philippen, Saskia, Pieloth, Damian, Pieper, Sarah, Pinfold, James, Pittermann, Martin, Pizzuto, A., Plaisier, Ilse, Plum, M., Popovych, Yuiry, Porcelli, Alessio, Prado Rodriguez, Maria, Price, P. Buford, Pries, Brandom, Przybylski, Gerald, Pyras, Lilly, Raab, Christoph, Raissi, Amirreza, Rameez, Mohamed, Rawlins, K., Rea, Immacolata Carmen, Rehman, Abdul, Reichherzer, Patrick, Reimann, René, Renzi, Giovanni, Resconi, Elisa, Reusch, Simeon, Rhode, Wolfgang, Richman, Mike, Riedel, Benedikt, Riegel, Michael, Roberts, Ella, Robertson, Sally, Roellinghoff, Gerrit, Rongen, Martin, Rott, Carsten, Ruhe, Tim, Ryckbosch, Dirk, Rysewyk Cantu, Devyn, Safa, Ibrahim, Saffer, Julian, Sanchez Herrera, Sebastian, Sandrock, Alexander, Sandroos, Joakim, Sandstrom, P., Santander, Marcos, Sarkar, Subir, Sarkar, Sourav, Satalecka, Konstancja, Scharf, Maximilian Karl, Schaufel, Merlin, Schieler, Harald, Schindler, Sebastian, Schlunder, P., Schmidt, Torsten, Schneider, Austin, Schneider, Judith, Schröder, Frank G., Schumacher, Lisa Johanna, Schwefer, Georg, Sclafani, Steve, Seckel, D., Seunarine, Surujhdeo, Shaevitz, M. H., Sharma, Ankur, Shefali, Shefali, Silva, Manuel, Skrzypek, Barbara, Smith, Daniel, Smithers, Ben, Snihur, Robert, Soedingrekso, Jan, Soldin, Dennis, SOLDNER-REMBOLD, Stefan, Southall, Daniel, Spannfellner, Christian, Spiczak, Glenn, Spiering, Christian, Stachurska, Juliana, Stamatikos, Michael, Stanev, T., Stein, Robert, Stettner, Jöran Benjamin, Steuer, A., Stezelberger, T., Sturwald, Timo, Stuttard, Thomas, Sullivan, G. W., Taboada, I., Taketa, Akimichi, Tanaka, Hiroyuki, Tenholt, Frederik, Ter-Antonyan, Samvel, Tilav, S., Tischbein, Franziska, Tollefson, Kirsten, Tomankova, Lenka, Tönnis, Christoph, Torres, Jorge, Toscano, Simona, Tosi, Delia, Trettin, Alexander, Tselengidou, Maria, Tung, Chunfai, Turcati, Andrea, Turcotte, Roxanne, Turley, Colin, Twagirayezu, Jean Pierre, Ty, Bunheng, Unland Elorrieta, Martin, Valtonen-Mattila, Nora, Vandenbroucke, Justin, van Eijndhoven, Nick, Vannerom, David, van Santen, Jakob, Veberic, Darko, Verpoest, Stef, Vieregg, Abigail G., Vraeghe, Matthias, Walck, C., Watson, Timothyblake, Weaver, Chris, Weigel, Philip, Weindl, Andreas, Weinstock, Lars Steffen, Weiss, Matthew, Weldert, Jan, Welling, Christoph, Wendt, Chris, Werthebach, Johannes, Weyrauch, Mark, Whitehorn, Nathan, Wiebusch, Christopher, Williams, Dawn, Wissel, Stephanie, Wolf, Martin, Woschnagg, Kurt, Wrede, Gerrit, Wren, Steven, Wulff, Johan, Xu, Xianwu, Xu, Yiqian, Yanez, Juan Pablo, Yoshida, S., Yu, Shiqi, Yuan, Tianlu, Zhang, Zelong, and Zierke, Simon
Subjects: Physics, hybrid, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, ice, Astronomy, Flux, radio wave: detector, IceCube Neutrino Observatory, IceCube, cascade, flux, observatory, detector [radio wave], Cascade, string, optical, surface, ddc:530, Neutrino
Abstract: 37. International Cosmic Ray Conference, ICRC 2021, Berlin, Germany, 15 Jul 2021 - 22 Jul 2021; Proceedings of Science 395, 1182 (2022). doi:10.22323/1.395.1182 special issue: "37th International Cosmic Ray Conference : ICRC2021 : 12-23 July 2021 : Berlin, Germany - Online / Editorial Board: Alexander Kappes, Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, D-48149 Münster, Germany ; Bianca Keilhauer, Karlsruhe Institute of Technology, Institute for Astroparticle Physics (IAP)", Published by SISSA, Trieste
Published: 2022

46. The Radio Neutrino Observatory Greenland (RNO-G)

Author: Wissel, Stephanie, primary, Aguilar, Juan A., additional, Allison, Patrick, additional, Beatty, James J., additional, Bernhoff, Hans, additional, Besson, David Zeke, additional, Bingefors, Nils, additional, Botner, Olga, additional, Bouma, Sjoerd, additional, Buitink, Stijn, additional, Carter, Katie, additional, Cataldo, Maddalena, additional, Clark, Brian A., additional, Curtis-Ginsberg, Zachary, additional, Connolly, Amy L., additional, Dasgupta, Paramita, additional, De Kockere, Simon, additional, de Vries, Krijn D., additional, Deaconu, Cosmin, additional, DuVernois, Michael A., additional, Glaser, Christian, additional, Hallgren, Allan, additional, Hallmann, Steffen, additional, Hanson, Jordan C., additional, Hendricks, Bryan L., additional, Hokanson-Fasig, Benjamin, additional, Hornhuber, Christian, additional, Hughes, Kaeli Autumn, additional, Karle, Albrecht, additional, Kelley, John L., additional, Klein, Spencer R., additional, Krebs, Ryan, additional, Lahmann, Robert, additional, Latif, Uzair Abdul, additional, Magnuson, Mitchell, additional, Meures, Thomas, additional, Meyers, Zachary S., additional, Mulrey, Katharine, additional, Nelles, Anna, additional, Novikov, Alexander, additional, Oberla, Eric, additional, Oeyen, Bob, additional, Pandya, Hershal, additional, Plaisier, Ilse, additional, Pyras, Lilly, additional, Ryckbosch, Dirk, additional, Scholten, Olaf, additional, Seckel, David, additional, Smith, Daniel, additional, Southall, Daniel, additional, Torres, Jorge, additional, Toscano, Simona, additional, Tosi, Delia, additional, Van Den Broeck, Dieder J., additional, van Eijndhoven, Nick, additional, Vieregg, Abigail G., additional, Welling, Christoph, additional, Young, Robert, additional, and Zink, Adrian, additional
Published: 2021
Full Text: View/download PDF

47. Simulation study for the future IceCube-Gen2 surface array

Author: Leszczynska, Agnieszka, primary, Abbasi, Rasha, additional, Ackermann, Markus, additional, Adams, Jenni, additional, Aguilar, Juanan, additional, Ahlers, M., additional, Ahrens, Maryon, additional, Alispach, Cyril Martin, additional, Allison, Patrick, additional, Alves Junior, Antonio Augusto, additional, Amin, Najia Moureen Binte, additional, An, Rui, additional, Andeen, Karen, additional, Anderson, Tyler, additional, Anton, Gisela, additional, Arguelles, Carlos, additional, Arlen, Tim, additional, Ashida, Yosuke, additional, Axani, Spencer, additional, Bai, Xinhua, additional, Balagopal V., Aswathi, additional, Barbano, Anastasia Maria, additional, Bartos, I., additional, Barwick, S. W., additional, Bastian, Benjamin, additional, Basu, Vedant, additional, Baur, Sebastian, additional, Bay, R. C., additional, Beatty, J. J., additional, Becker, K.-H., additional, Becker Tjus, Julia, additional, Bellenghi, Chiara, additional, BenZvi, Segev, additional, Berley, D., additional, Bernardini, Elisa, additional, Besson, D. Z., additional, Binder, Gary, additional, Bindig, Daniel, additional, Bishop, Abigail, additional, Blaufuss, E., additional, Blot, Summer, additional, Boddenberg, Matthias, additional, Bohmer, Michael, additional, Bontempo, Federico, additional, Borowka, Jurgen, additional, Boser, S., additional, Botner, Olga, additional, Boettcher, Jakob, additional, Bourbeau, Etienne, additional, Bradascio, Federica, additional, Braun, J., additional, Bron, Stephanie, additional, Brostean-Kaiser, Jannes, additional, Browne, Sally-Ann, additional, Burgman, Alexander, additional, Burley, Ryan T., additional, Busse, Raffaela, additional, Campana, Michael, additional, Carnie-Bronca, Erin, additional, Cataldo, Maddalena, additional, Chen, Chujie, additional, Chirkin, Dmitry, additional, Choi, Koun, additional, Clark, Brian, additional, Clark, Kenneth, additional, Clark, Rogan, additional, Classen, Lew, additional, Coleman, Alan, additional, Collin, Gabriel, additional, Connolly, Amy, additional, Conrad, J. M., additional, Coppin, Paul, additional, Correa, Pablo, additional, Cowen, D. F., additional, Cross, R., additional, Dappen, Christian, additional, Dave, Pranav, additional, Deaconu, Cosmin, additional, DE CLERCQ, Catherine, additional, De Kockere, Simon, additional, DeLaunay, James, additional, Dembinski, Hans, additional, Deoskar, Kunal, additional, De Ridder, Sam, additional, Desai, Abhishek, additional, Desiati, Paolo, additional, de Vries, Krijn, additional, de Wasseige, Gwenhaël, additional, De With, Meike, additional, DeYoung, Tyce, additional, Dharani, Sukeerthi, additional, Diaz, Alejandro, additional, Diaz-Velez, Juan Carlos, additional, Dittmer, Markus, additional, Dujmovic, Hrvoje, additional, Dunkman, Matt, additional, DuVernois, Michael, additional, Dvorak, Emily, additional, Ehrhardt, Thomas, additional, Eller, Philipp, additional, Engel, Ralph, additional, Erpenbeck, Hannah, additional, Evans, John, additional, Evenson, P. A., additional, Fan, Kwok Lung, additional, Farrag, K, additional, Fazely, A. R., additional, Fiedlschuster, Sebastian, additional, Fienberg, Aaron, additional, Filimonov, Kirill, additional, Finley, Chad, additional, Fischer, Leander, additional, Fox, Derek B, additional, Franckowiak, Anna, additional, Friedman, Elizabeth, additional, Fritz, Alexander, additional, Furst, Philipp, additional, Gaisser, T. K., additional, Gallagher, Jay, additional, Ganster, Erik, additional, Garcia, Alfonso, additional, Garrappa, Simone, additional, Gartner, Andreas, additional, Gerhardt, L., additional, Gernhaeuser, Roman, additional, Ghadimi, Ava, additional, Giri, Pawan, additional, Glaser, Christian, additional, Glauch, Theo, additional, Glusenkamp, Thorsten, additional, Goldschmidt, A., additional, Gonzalez, Javier, additional, Goswami, Sreetama, additional, Grant, Darren, additional, Grégoire, Timothée, additional, Griswold, Spencer, additional, Gunduz, Mehmet, additional, Günther, Christoph, additional, Haack, Christian, additional, Hallgren, Allan, additional, Halliday, R., additional, Hallmann, Steffen, additional, Halve, L., additional, Halzen, F., additional, Ha Minh, Martin, additional, Hanson, Kael, additional, Hardin, John, additional, Harnisch, Alexander A., additional, Haugen, Jim, additional, Haungs, Andreas, additional, Hauser, Simon, additional, Hebecker, Dustin, additional, Heinen, Dirk, additional, Helbing, K., additional, Hendricks, Brian, additional, Henningsen, Felix, additional, Hettinger, Emma C., additional, Hickford, Stephanie, additional, Hignight, Joshua, additional, Hill, Colton, additional, Hill, G. C., additional, Hoffman, Kara, additional, Hoffmann, Benjamin, additional, Hoffmann, Ruth, additional, Hoinka, Tobias, additional, Hokanson-Fasig, Benjamin, additional, Holzapfel, Kilian, additional, Hoshina, K., additional, Huang, Feifei, additional, Huber, Matthias, additional, Huber, Thomas, additional, Huege, Tim, additional, Hughes, Kaeli Autumn, additional, Hultqvist, Klas, additional, Hunnefeld, Mirco, additional, Hussain, Raamis, additional, In, Seongjin, additional, Iovine, Nadège, additional, Ishihara, Aya, additional, Jansson, Matti, additional, Japaridze, George, additional, Jeong, Minjin, additional, Jones, Ben, additional, KALEKIN, Oleg, additional, Kang, Donghwa, additional, Kang, Woosik, additional, Kang, Xinyue, additional, Kappes, Alexander, additional, Kappesser, David, additional, Karg, Timo, additional, Karl, Martina, additional, Karle, A., additional, Katori, Teppei, additional, Katz, U., additional, Kauer, M., additional, Keivani, A., additional, Kellermann, Moritz, additional, Kelley, J. L., additional, Kheirandish, Ali, additional, Kin, Ken'ichi, additional, Kintscher, Thomas, additional, Kiryluk, Joanna, additional, Klein, Spencer, additional, Koirala, Ramesh, additional, Kolanoski, Hermann, additional, Kontrimas, Tomas, additional, Kopke, Lutz, additional, Kopper, Claudio, additional, Kopper, Sandro, additional, Koskinen, D. J., additional, Koundal, Paras, additional, Kovacevich, Michael, additional, Kowalski, Marek, additional, Kozynets, Tetiana, additional, Krauss, Carsten, additional, Kravchenko, Ilya, additional, Krebs, Ryan, additional, Kun, Emma, additional, Kurahashi, Naoko, additional, Lad, Neha Navnitkumar, additional, Lagunas Gualda, Cristina, additional, Lanfranchi, Justin, additional, Larson, M. J., additional, Lauber, Frederik Hermann, additional, Lazar, Jeffrey, additional, Lee, Jiwoong, additional, Leonard, Kayla, additional, Li, Yijia, additional, Lincetto, Massimiliano, additional, Liu, Qinrui, additional, Liubarska, Maria, additional, Lohfink, Elisa, additional, LoSecco, John, additional, Lozano Mariscal, Cristian Jesus, additional, Lu, Lu, additional, Lucarelli, Francesco, additional, Ludwig, Andrew, additional, Luszczak, William, additional, Lyu, Yang, additional, Ma, Wing Yan, additional, Madsen, James, additional, Mahn, Kendall, additional, Makino, Yuya, additional, Mancina, Sarah, additional, Mandalia, S, additional, Maris, Ioana Codrina, additional, Marka, Szabolcs, additional, Marka, Zsuzsa, additional, Maruyama, Reina H., additional, Mase, K., additional, McElroy, Thomas, additional, McNally, Frank, additional, Mead, James Vincent, additional, Meagher, K., additional, Medina, Andres, additional, Meier, Maximilian, additional, Meighen-Berger, Stephan Andrew, additional, Meyers, Zachary Samuel, additional, Micallef, Jessie, additional, Mockler, Daniela, additional, Montaruli, Teresa, additional, Moore, Roger, additional, Morse, R., additional, Moulai, Marjon, additional, Naab, Richard, additional, Nagai, Ryo, additional, Naumann, Uwe, additional, Necker, Jannis, additional, Nelles, Anna, additional, Nguyen, Le Viet, additional, Niederhausen, Hans, additional, Nisa, Mehr, additional, Nowicki, Sarah, additional, Nygren, Dave, additional, Oberla, Eric, additional, Obertacke Pollmann, Anna, additional, Oehler, Marie, additional, Olivas, A., additional, Omeliukh, Anastasiia, additional, O'Sullivan, Erin, additional, Pandya, Hershal, additional, Pankova, Daria, additional, Papp, Laszlo, additional, Park, Nahee, additional, Parker, Grant, additional, Paudel, Ek Narayan, additional, Paul, Larissa, additional, Perez de los Heros, Carlos, additional, Peters, Lilly, additional, Petersen, Troels, additional, Peterson, Josh, additional, Philippen, Saskia, additional, Pieloth, Damian, additional, Pieper, Sarah, additional, Pinfold, James, additional, Pittermann, Martin, additional, Pizzuto, A., additional, Plaisier, Ilse, additional, Plum, M., additional, Popovych, Yuiry, additional, Porcelli, Alessio, additional, Prado Rodriguez, Maria, additional, Price, P. Buford, additional, Pries, Brandom, additional, Przybylski, Gerald, additional, Pyras, Lilly, additional, Raab, Christoph, additional, Raissi, Amirreza, additional, Rameez, Mohamed, additional, Rawlins, K., additional, Rea, Immacolata Carmen, additional, Rehman, Abdul, additional, Reichherzer, Patrick, additional, Reimann, René, additional, Renzi, Giovanni, additional, Resconi, Elisa, additional, Reusch, Simeon, additional, Rhode, Wolfgang, additional, Richman, Mike, additional, Riedel, Benedikt, additional, Riegel, Michael, additional, Roberts, Ella, additional, Robertson, Sally, additional, Roellinghoff, Gerrit, additional, Rongen, Martin, additional, Rott, Carsten, additional, Ruhe, Tim, additional, Ryckbosch, Dirk, additional, Rysewyk Cantu, Devyn, additional, Safa, Ibrahim, additional, Saffer, Julian, additional, Sanchez Herrera, Sebastian, additional, Sandrock, Alexander, additional, Sandroos, Joakim, additional, Sandstrom, P., additional, Santander, Marcos, additional, Sarkar, Subir, additional, Sarkar, Sourav, additional, Satalecka, Konstancja, additional, Scharf, Maximilian Karl, additional, Schaufel, Merlin, additional, Schieler, Harald, additional, Schindler, Sebastian, additional, Schlunder, P., additional, Schmidt, Torsten, additional, Schneider, Austin, additional, Schneider, Judith, additional, Schröder, Frank G., additional, Schumacher, Lisa Johanna, additional, Schwefer, Georg, additional, Sclafani, Steve, additional, Seckel, D., additional, Seunarine, Surujhdeo, additional, Shaevitz, M. H., additional, Sharma, Ankur, additional, Shefali, Shefali, additional, Silva, Manuel, additional, Skrzypek, Barbara, additional, Smith, Daniel, additional, Smithers, Ben, additional, Snihur, Robert, additional, Soedingrekso, Jan, additional, Soldin, Dennis, additional, SOLDNER-REMBOLD, Stefan, additional, Southall, Daniel, additional, Spannfellner, Christian, additional, Spiczak, Glenn, additional, Spiering, Christian, additional, Stachurska, Juliana, additional, Stamatikos, Michael, additional, Stanev, T., additional, Stein, Robert, additional, Stettner, Joeran, additional, Steuer, A., additional, Stezelberger, T., additional, Sturwald, Timo, additional, Stuttard, Thomas, additional, Sullivan, G. W., additional, Taboada, I., additional, Taketa, Akimichi, additional, Tanaka, Hiroyuki, additional, Tenholt, Frederik, additional, Ter-Antonyan, Samvel, additional, Tilav, S., additional, Tischbein, Franziska, additional, Tollefson, Kirsten, additional, Tomankova, Lenka, additional, Tönnis, Christoph, additional, Torres, Jorge, additional, Toscano, Simona, additional, Tosi, Delia, additional, Trettin, Alexander, additional, Tselengidou, Maria, additional, Tung, Chunfai, additional, Turcati, Andrea, additional, Turcotte, Roxanne, additional, Turley, Colin, additional, Twagirayezu, Jean Pierre, additional, Ty, Bunheng, additional, Unland Elorrieta, Martin, additional, Valtonen-Mattila, Nora, additional, Vandenbroucke, Justin, additional, van Eijndhoven, Nick, additional, Vannerom, David, additional, van Santen, Jakob, additional, Veberic, Darko, additional, Verpoest, Stef, additional, Vieregg, Abigail G., additional, Vraeghe, Matthias, additional, Walck, C., additional, Watson, Timothyblake, additional, Weaver, Chris, additional, Weigel, Philip, additional, Weindl, Andreas, additional, Weinstock, Lars Steffen, additional, Weiss, Matthew, additional, Weldert, Jan, additional, Welling, Christoph, additional, Wendt, Chris, additional, Werthebach, Johannes, additional, Weyrauch, Mark, additional, Whitehorn, Nathan, additional, Wiebusch, C. H., additional, Williams, Dawn, additional, Wissel, Stephanie, additional, Wolf, Martin, additional, Woschnagg, Kurt, additional, Wrede, Gerrit, additional, Wren, Steven, additional, Wulff, Johan, additional, Xu, Xianwu, additional, Xu, Yiqian, additional, Yanez, Juan Pablo, additional, Yoshida, S., additional, Yu, Shiqi, additional, Yuan, Tianlu, additional, Zhang, Zelong, additional, and Zierke, Simon, additional
Published: 2021
Full Text: View/download PDF

48. Direction Reconstruction for the Radio Neutrino Observatory Greenland (RNO-G)

Author: Plaisier, Ilse, primary, Aguilar, Juan A., additional, Allison, Patrick, additional, Beatty, James J., additional, Bernhoff, Hans, additional, Besson, David Zeke, additional, Bingefors, Nils, additional, Botner, Olga, additional, Bouma, Sjoerd, additional, Buitink, Stijn, additional, Carter, Katie, additional, Cataldo, Maddalena, additional, Clark, Brian A., additional, Curtis-Ginsberg, Zachary, additional, Connolly, Amy L., additional, Dasgupta, Paramita, additional, De Kockere, Simon, additional, de Vries, Krijn D., additional, Deaconu, Cosmin, additional, DuVernois, Michael A., additional, Glaser, Christian, additional, Hallgren, Allan, additional, Hallmann, Steffen, additional, Hanson, Jordan C., additional, Hendricks, Bryan, additional, Hokanson-Fasig, Benjamin, additional, Hornhuber, Christian, additional, Hughes, Kaeli, additional, Karle, Albrecht, additional, Kelley, John L., additional, Klein, Spencer R., additional, Krebs, Ryan, additional, Lahmann, Robert, additional, Latif, Uzair Abdul, additional, Magnuson, Mitchell, additional, Meures, Thomas, additional, Meyers, Zachary S., additional, Mulrey, Katharine, additional, Nelles, Anna, additional, Novikov, Alexander, additional, Oberla, Eric, additional, Oeyen, Bob, additional, Pandya, Hershal, additional, Pyras, Lilly, additional, Ryckbosch, Dirk, additional, Scholten, Olaf, additional, Seckel, David, additional, Smith, Daniel, additional, Southall, Daniel, additional, Torres, Jorge, additional, Toscano, Simona, additional, Tosi, Delia, additional, Van Den Broeck, Dieder J., additional, van Eijndhoven, Nick, additional, Vieregg, Abigail G., additional, Welling, Christoph, additional, Wissel, Stephanie, additional, Young, Robert, additional, and Zink, Adrian, additional
Published: 2021
Full Text: View/download PDF

49. Monte Carlo simulations of neutrino and charged lepton propagation in the Earth with nuPyProp

Author: Patel, Sameer, primary, Hall Reno, Mary, additional, Krizmanic, John, additional, Akaike, Yosui, additional, Anchordoqui, Luis A., additional, Bergman, Douglas, additional, Buckland, Isaac, additional, Cummings, Austin, additional, Eser, Johannes, additional, Guépin, Claire, additional, Mackovjak, Simon, additional, Olinto, Angela, additional, Paul, Thomas C., additional, Reustle, Alex, additional, Romero-Wolf, Andrew, additional, Sarazin, Fred, additional, Venters, Tonia, additional, Wiencke, Lawrence, additional, and Wissel, Stephanie, additional
Published: 2021
Full Text: View/download PDF

50. Application of parabolic equation methods to in-ice radiowave propagation for ultra high energy neutrino detection experiments

Author: Sbrocco, Cade, primary, Allison, Patrick, additional, Beatty, James, additional, Besson, Dave, additional, Connolly, Amy, additional, Dasgupta, Paramita, additional, Deaconu, Cosmin, additional, De Kockere, Simon, additional, de Vries, Krijn, additional, Frikken, Dylan, additional, HAST, Carsten, additional, Huesca Santiago, Enrique, additional, Kuo, Chung-Yun, additional, Latif, Uzair Abdul, additional, Lukic, Vesna, additional, Meures, Thomas, additional, Mulrey, Katharine, additional, Nam, Jiwoo, additional, Nozdrina, Alisa, additional, Oberla, Eric, additional, Prohira, Steven, additional, Ralston, John, additional, Stanley, Rose S, additional, Torres, Jorge, additional, Toscano, Simona, additional, Van den Broeck, Dieder, additional, van Eijndhoven, Nick, additional, and Wissel, Stephanie, additional
Published: 2021
Full Text: View/download PDF

Catalog

Books, media, physical & digital resources

See catalog results

Searchworks

Select search scope, currently: Articles Catalog books, media & more in Jio Institute collections Articles journal articles & other e-resources

Search

Search Constraints

Refine your results

Search Limiters

Topic

Publication Year Range

Language

Publication Type

Journal

Database

Publisher

115 results on '"Wissel, Stephanie"'

Search Results

Catalog

Select search scope, currently: Articles

Catalog

books, media & more in Jio Institute collections

Articles

journal articles & other e-resources