Zobrazeno 1 - 10
of 34
pro vyhledávání: '"Muzio, Marco Stein"'
We investigate the degree to which current ultrahigh energy cosmic ray observations above the ankle support a common maximum rigidity for all nuclei, often called a Peters cycle, over alternative scenarios for the cosmic ray spectra escaping sources.
Externí odkaz:
http://arxiv.org/abs/2309.16518
Autor:
Muzio, Marco Stein, Globus, Noémie
We consider how the cutoff of the ultrahigh energy neutrino spectrum introduces an effective neutrino horizon, allowing for future neutrino detectors to measure an anisotropy in neutrino arrival directions driven by the local large-scale structure. W
Externí odkaz:
http://arxiv.org/abs/2308.16225
Autor:
Dasgupta, Paramita, Muzio, Marco Stein
The Askaryan Radio Array (ARA) is an in-ice ultrahigh energy (UHE, $>10$ PeV) neutrino experiment at the South Pole that aims to detect radio emissions from neutrino-induced particle cascades. ARA has five independent stations which together have col
Externí odkaz:
http://arxiv.org/abs/2308.12125
Autor:
Muzio, Marco Stein
The Radio Neutrino Observatory in Greenland (RNO-G) is the only ultrahigh energy (UHE, ${\gtrsim}30$~PeV) neutrino monitor of the Northern sky and will soon be the world's most sensitive high-uptime detector of UHE neutrinos. Because of this, RNO-G r
Externí odkaz:
http://arxiv.org/abs/2308.07224
Autor:
Muzio, Marco Stein, Globus, Noémie
We present the extent to which anisotropies in the ultrahigh energy neutrino sky can probe the distribution of extreme astrophysical accelerators in the universe. In this talk, we discuss the origin of an anisotropic neutrino sky and show how observe
Externí odkaz:
http://arxiv.org/abs/2308.07211
One of the most challenging open questions regarding the origin of ultrahigh energy cosmic rays (UHECRs) deals with the shape of the source emission spectra. A commonly-used simplifying assumption is that the source spectra of the highest energy cosm
Externí odkaz:
http://arxiv.org/abs/2308.07208
Prospects for joint cosmic ray and neutrino constraints on the evolution of trans-GZK proton sources
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 o
Externí odkaz:
http://arxiv.org/abs/2303.04170
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
Autor:
Muzio, Marco Stein, Farrar, Glennys R.
Interactions of ultrahigh energy cosmic rays in the surroundings of their accelerators can naturally explain the observed spectrum and composition of UHECRs, including the abundance of protons below the ankle. We show that astrophysical properties of
Externí odkaz:
http://arxiv.org/abs/2209.08068
Autor:
Engel, Kristi, Lewis, Tiffany, Muzio, Marco Stein, Venters, Tonia M., Ahlers, Markus, Albert, Andrea, Allen, Alice, Solares, Hugo Alberto Ayala, Anandagoda, Samalka, Andersen, Thomas, Antier, Sarah, Alvarez-Castillo, David, Bar, Olaf, Beznosko, Dmitri, Bibrzyck, Łukasz, Brazier, Adam, Brisbois, Chad, Brose, Robert, Brown, Duncan A., Bulla, Mattia, Burgess, J. Michael, Burns, Eric, Chirenti, Cecilia, Ciprini, Stefano, Clay, Roger, Coughlin, Michael W., Cummings, Austin, D'Elia, Valerio, Dai, Shi, Dietrich, Tim, Di Lalla, Niccolò, Dingus, Brenda, Durocher, Mora, Eser, Johannes, Filipović, Miroslav D., Fleischhack, Henrike, Foucart, Francois, Frontczak, Michał, Fryer, Christopher L., Gamble, Ronald S., Gasparrini, Dario, Giardino, Marco, Goodman, Jordan, Harding, J. Patrick, Hare, Jeremy, Holley-Bockelmann, Kelly, Homola, Piotr, Hughes, Kaeli A., Humensky, Brian, Inoue, Yoshiyuki, Jaffe, Tess, Kargaltsev, Oleg, Kierans, Carolyn, Kneller, James P., Leto, Cristina, Lucarelli, Fabrizio, Martínez-Huerta, Humberto, Maselli, Alessandro, Meli, Athina, Meyers, Patrick, Mueller, Guido, Nasipak, Zachary, Negro, Michela, Niedźwiecki, Michał, Noble, Scott C., Omodei, Nicola, Oslowski, Stefan, Perri, Matteo, Piekarczyk, Marcin, Pittori, Carlotta, Polenta, Gianluca, Prechelt, Remy L., Principe, Giacomo, Racusin, Judith, Rzecki, Krzysztof, Sambruna, Rita M., Schlieder, Joshua E., Shoemaker, David, Smale, Alan, Sośnicki, Tomasz, Stein, Robert, Stuglik, Sławomir, Teuben, Peter, Thorpe, James Ira, Verbiest, Joris P., Verrecchia, Franceso, Vitale, Salvatore, Wadiasingh, Zorawar, Wibig, Tadeusz, Willox, Elijah, Wilson-Hodge, Colleen A., Wood, Joshua, Yang, Hui, Zhang, Haocheng
The last decade has brought about a profound transformation in multimessenger science. Ten years ago, facilities had been built or were under construction that would eventually discover the nature of objects in our universe could be detected through
Externí odkaz:
http://arxiv.org/abs/2203.10074