Published January 13, 2025
0 views Journal article Open Access Open Access

Inference of the Mass Composition of Cosmic Rays with Energies from 10^{18.5} to 10^{20}  eV Using the Pierre Auger Observatory and Deep Learning.

Creators

  • 1. University of Adelaide, Adelaide, South Australia, Australia.
  • 2. University of Adelaide
  • 3. Laboratório de Instrumentação e Física Experimental de Partículas-LIP and Instituto Superior Técnico-IST, Universidade de Lisboa-UL, Lisboa, Portugal.
  • 4. INFN, Sezione di Torino, Torino, Italy.
  • 5. Istituto Nazionale di Fisica Nucleare
  • 6. Osservatorio Astrofisico di Torino (INAF), Torino, Italy.
  • 7. Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina.
  • 8. Institute of Nuclear Physics PAN, Krakow, Poland.
  • 9. IMAPP, Radboud University Nijmegen, Nijmegen, The Netherlands.
  • 10. Radboud University Nijmegen
  • 11. Nationaal Instituut voor Kernfysica en Hoge Energie Fysica (NIKHEF), Science Park, Amsterdam, The Netherlands.
  • 12. Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina.
  • 13. Universidad Tecnológica Nacional-Facultad Regional Buenos Aires, Buenos Aires, Argentina.
  • 14. Gran Sasso Science Institute, L'Aquila, Italy.
  • 15. INFN Laboratori Nazionali del Gran Sasso, Assergi (L'Aquila), Italy.
  • 16. Instituto Galego de Física de Altas Enerxías (IGFAE), Universidade de Santiago de Compostela, Santiago de Compostela, Spain.
  • 17. University of Santiago de Compostela
  • 18. INFN, Sezione di Catania, Catania, Italy.
  • 19. Università di Catania, Dipartimento di Fisica e Astronomia "Ettore Majorana", Catania, Italy.
  • 20. Department of Physics and Astronomy, Lehman College, City University of New York, Bronx, New York, USA.
  • 21. City University of New York
  • 22. INFN, Sezione di Milano, Milano, Italy.
  • 23. Università di Milano, Dipartimento di Fisica, Milano, Italy.
  • 24. INFN, Sezione di Napoli, Napoli, Italy.
  • 25. RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany.
  • 26. RWTH Aachen University
  • 27. Università Torino, Dipartimento di Fisica, Torino, Italy.
  • 28. Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Michoacán, México.
  • 29. Observatorio Pierre Auger and Comisión Nacional de Energía Atómica, Malargüe, Argentina.
  • 30. Università dell'Aquila, Dipartimento di Scienze Fisiche e Chimiche, L'Aquila, Italy.
  • 31. Institute of Physics of the Czech Academy of Sciences, Prague, Czech Republic.
  • 32. Academy of Sciences of the Czech Republic
  • 33. Colorado School of Mines, Golden, Colorado, USA.
  • 34. Université Grenoble Alpes, CNRS, Grenoble Institute of Engineering Univ. Grenoble Alpes, LPSC-IN2P3, 38000 Grenoble, France.
  • 35. University of Grenoble
  • 36. Departamento de Física and Departamento de Ciencias de la Atmósfera y los Océanos, FCEyN, Universidad de Buenos Aires and CONICET, Buenos Aires, Argentina.
  • 37. University of Buenos Aires
  • 38. IFLP, Universidad Nacional de La Plata and CONICET, La Plata, Argentina.
  • 39. Instituto de Astronomía y Física del Espacio (IAFE, CONICET-UBA), Buenos Aires, Argentina.
  • 40. Instituto de Física de Rosario (IFIR)-CONICET/U.N.R. and Facultad de Ciencias Bioquímicas y Farmacéuticas U.N.R., Rosario, Argentina.
  • 41. Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), and Universidad Tecnológica Nacional-Facultad Regional Mendoza (CONICET/CNEA), Mendoza, Argentina.
  • 42. International Center of Advanced Studies and Instituto de Ciencias Físicas, ECyT-UNSAM and CONICET, Campus Miguelete-San Martín, Buenos Aires, Argentina.
  • 43. Laboratorio Atmósfera-Departamento de Investigaciones en Láseres y sus Aplicaciones-UNIDEF (CITEDEF-CONICET), Villa Martelli, Argentina.
  • 44. Observatorio Pierre Auger, Malargüe, Argentina.
  • 45. Université Libre de Bruxelles (ULB), Brussels, Belgium.
  • 46. Université libre de Bruxelles
  • 47. Vrije Universiteit Brussels, Brussels, Belgium.
  • 48. Centro Brasileiro de Pesquisas Fisicas, Rio de Janeiro, RJ, Brazil.
  • 49. Centro Federal de Educação Tecnológica Celso Suckow da Fonseca, Petropolis, Brazil.
  • 50. Instituto Federal de Educação, Ciência e Tecnologia do Rio de Janeiro (IFRJ), RJ, Brazil.
  • 51. Universidade de São Paulo, Escola de Engenharia de Lorena, Lorena, SP, Brazil.
  • 52. University of São Paulo
  • 53. Universidade de São Paulo, Instituto de Física de São Carlos, São Carlos, SP, Brazil.
  • 54. Universidade de São Paulo, Instituto de Física, São Paulo, SP, Brazil.
  • 55. Universidade Estadual de Campinas (UNICAMP), IFGW, Campinas, SP, Brazil.
  • 56. State University of Campinas
  • 57. Universidade Estadual de Feira de Santana, Feira de Santana, Brazil.
  • 58. Universidade Federal de Campina Grande, Centro de Ciencias e Tecnologia, Campina Grande, Brazil.
  • 59. Universidade Federal do ABC, Santo André, SP, Brazil.
  • 60. Universidade Federal do Paraná, Setor Palotina, Palotina, Brazil.
  • 61. Federal University of Paraná
  • 62. Universidade Federal do Rio de Janeiro, Instituto de Física, Rio de Janeiro, RJ, Brazil.
  • 63. Federal University of Rio de Janeiro
  • 64. Universidad de Medellín, Medellín, Colombia.
  • 65. Universidad Industrial de Santander, Bucaramanga, Colombia.
  • 66. Charles University, Faculty of Mathematics and Physics, Institute of Particle and Nuclear Physics, Prague, Czech Republic.
  • 67. Charles University in Prague
  • 68. Palacky University, Olomouc, Czech Republic.
  • 69. CNRS/IN2P3, IJCLab, Université Paris-Saclay, Orsay, France.
  • 70. Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Sorbonne Université, Université de Paris, CNRS-IN2P3, Paris, France.
  • 71. University of Paris
  • 72. Université Paris-Saclay, CNRS/IN2P3, IJCLab, Orsay, France.
  • 73. Bergische Universität Wuppertal, Department of Physics, Wuppertal, Germany.
  • 74. Karlsruhe Institute of Technology (KIT), Institute for Experimental Particle Physics, Karlsruhe, Germany.
  • 75. Karlsruhe Institute of Technology
  • 76. Karlsruhe Institute of Technology (KIT), Institut für Prozessdatenverarbeitung und Elektronik, Karlsruhe, Germany.
  • 77. Karlsruhe Institute of Technology (KIT), Institute for Astroparticle Physics, Karlsruhe, Germany.
  • 78. Universität Hamburg, II. Institut für Theoretische Physik, Hamburg, Germany.
  • 79. University of Hamburg
  • 80. Universität Siegen, Department Physik-Experimentelle Teilchenphysik, Siegen, Germany.
  • 81. INFN, Sezione di Lecce, Lecce, Italy.
  • 82. INFN, Sezione di Roma "Tor Vergata", Roma, Italy.
  • 83. Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo (INAF), Palermo, Italy.
  • 84. Politecnico di Milano, Dipartimento di Scienze e Tecnologie Aerospaziali, Milano, Italy.
  • 85. Polytechnic University of Milan
  • 86. Università del Salento, Dipartimento di Matematica e Fisica "E. De Giorgi", Lecce, Italy.
  • 87. Università di Napoli "Federico II", Dipartimento di Fisica "Ettore Pancini", Napoli, Italy.
  • 88. Università di Palermo, Dipartimento di Fisica e Chimica "E. Segrè", Palermo, Italy.
  • 89. Università di Roma "Tor Vergata", Dipartimento di Fisica, Roma, Italy.
  • 90. Benemérita Universidad Autónoma de Puebla, Puebla, México.
  • 91. Unidad Profesional Interdisciplinaria en Ingeniería y Tecnologías Avanzadas del Instituto Politécnico Nacional (UPIITA-IPN), México, D.F., México.
  • 92. Instituto Politécnico Nacional
  • 93. Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas, México.
  • 94. Universidad Nacional Autónoma de México, México, D.F., México.
  • 95. National Autonomous University of Mexico
  • 96. Universidad Nacional de San Agustin de Arequipa, Facultad de Ciencias Naturales y Formales, Arequipa, Peru.
  • 97. University of Łódź, Faculty of High-Energy Astrophysics, Łódź, Poland.
  • 98. "Horia Hulubei" National Institute for Physics and Nuclear Engineering, Bucharest-Magurele, Romania.
  • 99. Institute of Space Science, Bucharest-Magurele, Romania.
  • 100. Center for Astrophysics and Cosmology (CAC), University of Nova Gorica, Nova Gorica, Slovenia.
  • 101. Experimental Particle Physics Department, J. Stefan Institute, Ljubljana, Slovenia.
  • 102. Universidad de Granada and C.A.F.P.E., Granada, Spain.
  • 103. University of Granada
  • 104. Stichting Astronomisch Onderzoek in Nederland (ASTRON), Dwingeloo, The Netherlands.
  • 105. Universiteit van Amsterdam, Faculty of Science, Amsterdam, The Netherlands.
  • 106. University of Amsterdam
  • 107. Case Western Reserve University, Cleveland, Ohio, USA.
  • 108. Case Western Reserve University
  • 109. Michigan Technological University, Houghton, Michigan, USA.
  • 110. New York University, New York, New York, USA.
  • 111. New York University
  • 112. University of Chicago, Enrico Fermi Institute, Chicago, Illinois, USA.
  • 113. University of Chicago
  • 114. University of Delaware, Department of Physics and Astronomy, Bartol Research Institute, Newark, Delaware, USA.
  • 115. University of Delaware
  • 116. University of Wisconsin-Madison, Department of Physics and WIPAC, Madison, Wisconsin, USA.
  • 117. University of Wisconsin-Madison

Description

We present measurements of the atmospheric depth of the shower maximum X_{max}, inferred for the first time on an event-by-event level using the surface detector of the Pierre Auger Observatory. Using deep learning, we were able to extend measurements of the X_{max} distributions up to energies of 100 EeV (10^{20}  eV), not yet revealed by current measurements, providing new insights into the mass composition of cosmic rays at extreme energies. Gaining a 10-fold increase in statistics compared to the fluorescence detector data, we find evidence that the rate of change of the average X_{max} with the logarithm of energy features three breaks at 6.5±0.6(stat)±1(syst)  EeV, 11±2(stat)±1(syst)  EeV, and 31±5(stat)±3(syst)  EeV, in the vicinity to the three prominent features (ankle, instep, suppression) of the cosmic-ray flux. The energy evolution of the mean and standard deviation of the measured X_{max} distributions indicates that the mass composition becomes increasingly heavier and purer, thus being incompatible with a large fraction of light nuclei between 50 and 100 EeV.
Enabled by The Lens

Open Access

Licence Attribution (CC BY)
Publisher Website Access full text