Neutrino propagation through Earth: modeling uncertainties using nuPyProp

Autor: 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, Wissel, Stephanie

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

Externí odkaz: http://arxiv.org/abs/2308.13659

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

Autor: 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, Zhang, Haocheng

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,

Externí odkaz: http://arxiv.org/abs/2209.11726

Neutrino Target-of-Opportunity Observations with Space-based and Suborbital Optical Cherenkov Detectors

Autor: Venters, Tonia M., Reno, Mary Hall, Krizmanic, John F.

Publikováno v: PoS(ICRC2021)977

Cosmic-ray accelerators capable of reaching ultra-high energies are expected to also produce very-high energy neutrinos via hadronic interactions within the source or its surrounding environment. Many of the candidate astrophysical source classes are

Externí odkaz: http://arxiv.org/abs/2206.02730

The Future of Gamma-Ray Experiments in the MeV-EeV Range

Autor: Engel, Kristi, Goodman, Jordan, Huentemeyer, Petra, Kierans, Carolyn, Lewis, Tiffany R., Negro, Michela, Santander, Marcos, Williams, David A., Allen, Alice, Aramaki, Tsuguo, Batista, Rafael Alves, Benoit, Mathieu, Bloser, Peter, Bohon, Jennifer, Bolotnikov, Aleksey E., Brewer, Isabella, Briggs, Michael S., Brisbois, Chad, Burgess, J. Michael, Burns, Eric, Caputo, Regina, Carini, Gabriella A., Cenko, S. Bradley, Charles, Eric, Ciprini, Stefano, D'Elia, Valerio, Daylan, Tansu, Distel, James, Donath, Axel, Duvall, Wade, Fleischhack, Henrike, Fletcher, Corinne, Fong, Wen Fe, Gasparrini, Dario, Giardino, Marco, Goldstein, Adam, Griffin, Sean, Grove, J. Eric, Hamburg, Rachel, Harding, J. Patrick, Hare, Jeremy, Hristov, Boyan, Hui, C. Michelle, Jaffe, Tess, Jenke, Pete, Kargaltsev, Oleg, Karwin, Christopher M., Kerr, Matthew, Kim, Dongsung, Kocevski, Daniel, Krizmanic, John, Laha, Ranjan, Di Lalla, Niccolo, Legere, Jason, Leto, Cristina, Leys, Richard, Lucarelli, Fabrizio, Martinez-Castellanos, Israel, Maselli, Alessandro, Mazziotta, M. Nicola, McConnell, Mark, McEnery, Julie, Metcalfe, Jessica, Meyer, Manuel, Moiseev, Alexander A., Mukherjee, Reshmi, Ogasawara, Keiichi, Omodei, Nicola, Peric, Ivan, Perkins, Jeremy S., Perri, Matteo, Pittori, Carlotta, Polenta, Gianluca, Poulson, Daniel, Preece, Robert, Principe, Giacomo, Racusin, Judith L., Roberts, Oliver, Rodd, Nicholas L., Shawhan, Peter, Shutt, Thomas, Sleator, Clio, Smale, Alan, Smedley, John, Smith, Jacob R., Tasson, Jay, Teuben, Peter, Tomsick, John, Veres, Peter, Verrecchia, Francesco, Wadiasingh, Zorawar, Wilson-Hodge, Colleen A., Wood, Joshua, Woolf, Richard S., Yang, Hui, Zhang, Bing, Zhang, Haocheng, Zoglauer, Andreas

Gamma-rays, the most energetic photons, carry information from the far reaches of extragalactic space with minimal interaction or loss of information. They bring messages about particle acceleration in environments so extreme they cannot be reproduce

Externí odkaz: http://arxiv.org/abs/2203.07360

The EUSO-SPB2 fluorescence telescope for the detection of Ultra-High Energy Cosmic Rays

Autor: Adams, James H., Jr., Allard, Denis, Alldredge, Phillip, Anchordoqui, Luis, Anzalone, Anna, Battisti, Matteo, Belov, Alexander A., Bertaina, Mario, Bertone, Peter F., Blin-Bondil, Sylvie, Burton, Julia, Cafagna, Francesco S., Casolino, Marco, Černý, Karel, Christl, Mark J., Colalillo, Roberta, Crawford, Hank J., Creusot, Alexandre, Cummings, Austin, Diesing, Rebecca, Nola, Alessandro Di, Ebisuzaki, Toshikazu, Eser, Johannes, Ferrarese, Silvia, Filippatos, George, Finch, William W., Flaminio, Flavia, Fornaro, Claudio, Fuehne, Duncan, Fuglesang, Christer, Garg, Diksha, Golzio, Alessio, Guarino, Fausto, Guépin, Claire, Heibges, Tobias, Judd, Eleanor G., Klimov, Pavel A., Krizmanic, John F., Kungel, Viktoria, Kupari, Luke, Kuznetsov, Evgeny, Manfrin, Massimiliano, Marszał, Włodzimierz, Matthews, John N., Mese, Marco, Meyer, Stephan S., Mignone, Marco, Miyamoto, Hiroko, Murashov, Alexey S., Nachtman, Jane M., Olinto, Angela V., Onel, Yasar, Osteria, Giuseppe, Panico, Beatrice, Parizot, Ètienne, Paul, Tom, Pech, Miroslav, Perfetto, Francesco, Piotrowski, Lech W., Plebaniak, Zbigniew, Posligua, Jonatan, Prévôt, Guillaume, Przybylak, Marika, Reardon, Patrick, Reno, Mary Hall, Ricci, Marco, Sarazin, Fred, Schovánek, P., Scotti, Valentina, Shinozaki, Kenji, Soriano, Jorge F., Stillwell, Ben K., Szabelski, Jacek, Takizawa, Yoshiyuki, Trofimov, Daniil, Unel, Fredrik, Valore, Laura, Venters, Tonia M., Watts, John, Jr., Wiencke, Lawrence, Wistrand, Hannah, Young, Roy

Publikováno v: In Astroparticle Physics February 2025 165