Constraining Lorentz Invariance Violation using the muon content of extensive air showers measured at the Pierre Auger Observatory

Trimarelli, Caterina; Abreu, Pedro; Aglietta, M.; Albury, Justin M.; Allekotte, I.; Almela, A.; Álvarez-Muñiz, J.; Batista, Rafael Alves; Anastasi, Gioacchino Alex; Anchordoqui, Luis A.; Andrada, Belén; Andringa, S.; Aramo, C.; Ferreira, Paulo Ricardo Araújo; Velázquez, Juan Carlos Arteaga; Asorey, H.; Assis, P.; Ávila, G.; Badescu, Alina Mihaela; Bakalová, Alena; Bălăceanu, Alexandru; Barbato, Felicia; Luz, Ricardo Jorge Barreira; Becker, Karl‐Heinz; Bellido, J. A.; Bérat, C.; Bertaina, M.; Bertou, X.; Biermann, Peter L.; Binet, Virginia; Bismark, Kathrin; Bister, Teresa; Biteau, J.; Blažek, Jiří; Bleve, C.; Bohã̌cov́a, M.; Boncioli, D.; Bonifazi, C.; Arbeletche, Luan Bonneau; Borodai, N.; Botti, Ana Martina; Brack, Jeffrey; Bretz, T.; Orchera, P. Gabriel Brichetto; Briechle, Florian Lukas; Buchholz, P.; Bueno, A.; Buitink, S.; Buscemi, Mario; Büsken, Max; Caballero-Mora, K. S.; Caccianiga, Lorenzo; Canfora, F.; Caracas, Ioana; Carceller, Juan Miguel; Caruso, R.; Castellina, A.; Catalani, Fernando; Cataldi, G.; Cazón, L.; Cerda, Marcos; Chinellato, J.; Chudoba, J.; Chytka, L.; Clay, R. W.; Cerutti, Agustín Cobos; Colalillo, R.; Coleman, Alan; Coluccia, M. R.; Conceição, R.; Condorelli, Antonio; Consolati, G.; Contreras, F.; Convenga, Fabio; Santos, Diego Correia dos; Covault, C. E.; Dasso, S.; Daumiller, K.; Dawson, B. R.; Day, Jarryd A.; Almeida, R. M. de; Jesús, Joaquín de; Jong, Sijbrand J. de; Mauro, G. De; Neto, João de Mello; Mitri, I. De; Oliveira, Jaime de; Franco, D.; Palma, F. de; Souza, Vítor de; Vito, Emanuele De; Río, Mariano del; Deligny, O.; Deval, Luca; Matteo, Armando di; Dobrigkeit, C.; D’Olivo, Juan Carlos; Mendes, Luis Miguel Domingues; Anjos, Rita dos; Santos, Diego dos; Dova, M. T.; Ebr, Jan; Engel, R.; Epicoco, Italo; Erdmann, M.; Escobar, C.; Etchegoyen, A.; Falcke, H.; Farmer, John; Farrar, Glennys R.; Fauth, A. C.; Fazzini, N.; Feldbusch, Fridtjof; Fenu, Francesco; Fick, B.; Figueira, J. M.; Filipčić, A.; Fitoussi, Thomas; Fodran, Tomáš; Freire, M. M.; Fujii, Toshihiro; Fuster, Alan; Galea, C.; Galelli, Claudio; García, Beatriz; Vegas, Adrianna Luz García; Gemmeke, H.; Gesualdi, Flavia; Gherghel-Lascu, A.; Ghia, P. L.; Giaccari, U.; Giammarchi, M.; Glombitza, Jonas; Gobbi, Fabian; Gollan, Fernando; Golup, G.; Berisso, M. Gómez; Vitale, Primo F. Gómez; Gongora, Juan Pablo; González, Juan Manuel; González, Nicolás Martín; Goos, Isabel; Góra, Dariusz; Gorgi, A.; Gottowik, Marvin; Grubb, Trent D.; Guarino, F.; Guedes, G. P.; Guido, Eleonora; Hahn, Steffen; Hamal, P.; Hampel, Matías Rolf; Hansen, Patricia María; Harari, D.; Harvey, Violet M.; Haungs, A.; Hebbeker, T.; Heck, D.; Hill, G. C.; Hojvat, C.; Hörandel, J. R.; Horváth, P.; Hrabovský, M.; Huege, T.; Insolia, A.; Isar, P. G.; Janeček, Petr; Johnsen, Jeffrey A.; Jurýšek, Jakub; Kääpä, Alex; Kampert, Karl-Heinz; Karastathis, N.; Keilhauer, B.; Kemp, J.; Khakurdikar, Abha; Covilakam, Varada Varma Kizakke; Klages, H. O.; Kleifges, M.; Kleinfeller, J.; Köpke, Marcel; Kunka, Norbert; Lago, Bruno L.; Lang, Rodrigo Guedes; Langner, Niklas; Oliveira, Marcelo Augusto Leigui de; Lenok, Vladimir; Letessier‐Selvon, A.; Lhenry-Yvon, I.; Presti, Domenico Lo; Lopes, L.; López, Rebeca; Lu, Lu; Luce, Quentin; Lundquist, Jon Paul; Payeras, Allan Machado; Mancarella, G.; Mandát, Dušan; Manning, Bradley C.; Manshanden, Julien; Mantsch, P.; Marafico, Sullivan; Mariazzi, Analisa; Maris, Ioana Codrina; Marsella, G.; Martello, D.; Martinelli, Sara; Bravo, O. Martínez; Mastrodicasa, Massimo; Mathes, H. J.; Matthews, James; Matthiae, G.; Mayotte, E.; Mazur, Péter; Medina‐Tanco, G.; Melo, D.; Menshikov, Alexander; Merenda, Kevin-Druis; Michal, Stanislav; Micheletti, M. I.; Miramonti, L.; Mollerach, Silvia; Montanet, F.; Morello, C.; Mostafá, M.; Müller, Ana L.; Müller, M. A.; Mulrey, Katharine; Mussa, R.; Muzio, Marco Stein; Namasaka, Wilson M.; Nasr-Esfahani, Alina; Nellen, Lukas; Niculescu-Oglinzanu, M.; Niechciol, Marcus; Nitz, D.; Nosek, D.; Novotný, Vladimír; Nožka, L.; Nucita, A. A.; Núñez, Luis A.; Palatka, M.; Pallotta, J.; Papenbreer, P.; Parente, G.; Parra, A.; Pawlowsky, Jannis; Pech, M.; Pedreira, F.; Pękala, Jan; Pelayo, R.; Peña-Rodríguez, Jesús; Martins, Edyvânia Emily Pereira; Armand, Johnnier Perez; Bertolli, Carmina Pérez; Perlín, M.; Perrone, L.; Petrera, S.; Pierog, T.; Pimenta, M.; Pirronello, V.; Platino, M.; Pont, Bjarni; Pothast, Mart; Privitera, P.; Prouza, M.; Puyleart, Andrew; Querchfeld, S.; Rautenberg, J.; Ravignani, D.; Reininghaus, Maximilian; Řídký, J.; Riehn, Felix; Risse, M.; Rizi, Vincenzo; Carvalho, W. Rodrigues de; Rojo, Jorge Rubén Rodriguez; Roncoroni, Matías J.; Rossoni, Simone; Roth, Markus; Roulet, Esteban; Rovero, A. C.; Ruehl, Philip; Sǎftoiu, A.; Salamida, F.; Salazar, H.; Salina, G.; Gomez, Jose Sanabria; Sánchez, F.; Santos, Edivaldo Moura; Santos, Eva; Sarazin, F.; Sarmento, R.; Sarmiento-Cano, C.; Sato, R.; Savina, Pierpaolo; Schäfer, C.; Scherini, V.; Schieler, H.; Schimassek, Martin; Schimp, Michael; Schlüter, Felix; Schmidt, David; Scholten, Olaf; Schovánek, Petr; Schröder, Frank G.; Schröder, Sonja; Schulte, Josina; Sciutto, S. J.; Scornavacche, Marina; Segreto, A.; Sehgal, Srijan; Shellard, R. C.; Sigl, Guenter; Silli, Gaia; Sima, O.; Šmída, R.; Sommers, P.; Soriano, Jorge F.; Souchard, Julien; Squartini, R.; Stadelmaier, Maximilian; Stanca, Denis; Stanič, S.; Stasielak, J.; Stassi, P.; Streich, Alexander; Suárez-Durán, Mauricio; Sudholz, T.; Suomijärvi, T.; Supanitsky, A. D.; Szadkowski, Z.; Tapia, A.; Taricco, Carla; Timmermans, C.; Tkachenko, Olena; Tobiška, Petr; Peixoto, C. J. Todero; Tomé, B.; Torrès, Zoé; Travaini, Andres; Trávničék, P.; Tueros, M.; Ulrich, R.; Unger, Michael; Vaclavek, Lukáš; Vacula, Martin; Galicia, J. F. Valdés; Valore, L.; Varela, E.; Vásquez-Ramírez, Adriana; Veberič, D.; Ventura, Cynthia; Quispe, Indira D. Vergara; Verzi, V.; Vícha, J.; Vink, Jacco; Vorobiov, S.; Wahlberg, H.; Watanabe, Clara Keiko Oliveira; Watson, Alan; Weber, M.; Weindl, A.; Wiencke, L.; Wilczyński, H.; Wirtz, Marcus; Wittkowski, David; Wundheiler, B.; Yushkov, A.; Zapparrata, Orazio; Zas, E.; Zavrtanik, D.; Zavrtanik, M.; Zehrer, Lukas

doi:10.22323/1.395.0340

Cited by 6 publications

(5 citation statements)

References 20 publications

(24 reference statements)

Supporting

Mentioning

Contrasting

Order By: Relevance

“…• Is Lorentz invariance (still) valid under such conditions [924,13,[925][926][927][928]9]? • How do these particles interact?…”

Section: Scientific Capabilitiesmentioning

confidence: 99%

Ultra-High-Energy Cosmic Rays: The Intersection of the Cosmic and Energy Frontiers

Coleman,

Eser,

Mayotte

et al. 2022

Preprint

View full text Add to dashboard Cite

Pin down the shower energy observable to use μ as a composition-only Reduce hadronic uncertainties interaction model E threshold (TBD) Other messengers Galactic * μ / em separation † * depending on analysis progress † depending on detector configuration• At least one next-generation experiment needs to be able to make high-precision measurements to explore new particle physics and measure particle rigidity on an event-by-event basis. Of the planned next-generation experiments, GCOS is the best positioned to meet this recommendation.• As a complementary effort, experiments with sufficient exposure ( 5 × 10 5 km 2 sr yr) are needed to search for Lorentz-invariance violation (LIV), SHDM, and other BSM physics at the Cosmic and Energy Frontiers, and to identify UHECR sources at the highest energies.• Full-sky coverage with low cross-hemisphere systematic uncertainties is critical for astrophysical studies. To this end, next generation experiments should be space-based or multi-site. Common sites between experiments are encouraged.• Based on the productive results from inter-collaboration and inter-disciplinary work, we recommend the continued progress/formation of joint analyses between experiments and with other intersecting fields of research (e.g., magnetic fields).• The UHECR community should continue its efforts to advance diversity, equity, inclusion, and accessibility. It also needs to take steps to reduce its environmental impacts and improve open access to its data to reduce the scientific gap between countries.vi

show abstract

“…• Is Lorentz invariance (still) valid under such conditions [924,13,[925][926][927][928]9]? • How do these particles interact?…”

Section: Scientific Capabilitiesmentioning

confidence: 99%

Ultra-High-Energy Cosmic Rays: The Intersection of the Cosmic and Energy Frontiers

Coleman,

Eser,

Mayotte

et al. 2022

Preprint

View full text Add to dashboard Cite

show abstract

“…(8). It would be interesting to further investigate such black hole proposals in order to seek for phenomena that could somehow amplify these third order Planck-scale effects even for third order corrections, which has been object of investigation through the presence of amplifiers in different contexts [70][71][72].…”

Section: Final Remarksmentioning

confidence: 99%

Massless Dirac Perturbations in a Consistent Model of Loop Quantum Gravity Black Hole: Quasinormal Modes and Particle Emission Rates

Albuquerque¹,

Lobo²,

Bezerra³

2023

Preprint

View full text Add to dashboard Cite

We consider perturbations of the massless Dirac field in the background of a black hole solution found by Bodendorfer, Mele, and Münch (BMM), using a polymerization technique that furnishes contributions inspired by Loop Quantum Gravity (LQG) Theory. Using the sixth order WKB method, we analyzed its quasinormal modes for several modes, multipole numbers and the two classes of BMM black holes. We also considered the potential that governs these perturbations to analyze the bound on the Greybody Factor (GF) due the emission rates of particles. As results, we found that the Loop Quantum Gravity parameters are responsible for raising the potential and the real and imaginary parts of the quasinormal frequencies and decrease the bound on the Greybody Factor for the two classes of black holes (with more more prominent effects for the de-amplification case, which is compatible with previous analyses done for other fields).

show abstract

“…Indeed, due to the much increased probability of interaction for neutral pions, the hadronic component of the cascade is enhanced, leading in particular to a larger production of muons. In this case, limits on the LIV parameter can be derived comparing the observed strong decrease of the relative fluctuations with the muon fluctuation measurement [38].…”

Section: Beyond the Standard Modelmentioning

confidence: 99%

Astroparticle and particle physics at ultra-high energy: Results from the Pierre Auger Observatory

Castellina

2023

SciPost Phys. Proc.

Self Cite

View full text Add to dashboard Cite

The scientific achievements of the Pierre Auger Collaboration cover diverse and complementary fields of research. The search for the origin of ultra-high energy cosmic rays (UHECRs) is based on the measurement of the energy spectrum and mass composition of the primaries, on studies of multi-messengers, and on extensive anisotropy searches. With the collected data it is also possible to explore the characteristics of hadronic interactions at energies unreachable at human-made accelerators, and to assess the existence of non-standard physics effects. A selection of the latest results is presented and the emerging picture is discussed.

show abstract

Constraining Lorentz Invariance Violation using the muon content of extensive air showers measured at the Pierre Auger Observatory

Cited by 6 publications

References 20 publications

Ultra-High-Energy Cosmic Rays: The Intersection of the Cosmic and Energy Frontiers

Ultra-High-Energy Cosmic Rays: The Intersection of the Cosmic and Energy Frontiers

Massless Dirac Perturbations in a Consistent Model of Loop Quantum Gravity Black Hole: Quasinormal Modes and Particle Emission Rates

Astroparticle and particle physics at ultra-high energy: Results from the Pierre Auger Observatory

Contact Info

Product

Resources

About