FISICA ED ASTRONOMIA "Ettore Majorana"PhysicsAcademic Year 2022/2023

1015695 - COSMIC RAY PHYSICS

Teacher: ROSSELLA CARUSO

Expected Learning Outcomes

The learning objectives of the Cosmic Ray Physics course consist of providing an overview on the properties of the charged "Cosmic Radiation" (Cosmic Rays): astrophysical sources of cosmic rays, transportation, propagation and acceleration of the primary cosmic rays in the galactic and extra-galactic environment, interaction and production of particle showers (secondary cosmic rays) in the terrestrial atmosphere, investigation of their Energy Spectrum, Mass Composition and Anisotropy in their arrival direction on the Earth (at the top of atmosphere) with a particular attention to the high and ultra high energy intervals.

Moreover the techniques of direct and indirect measurements of the low, medium, high, very-high, ultra-high and extreme energy cosmic rays will be examined. The scientific results of the main past and present experiments in the Cosmic Ray Physics  will be analyzed, the status of works and the future perspectives will be discussed.

In particular, concerning the Dublin Descriptors, the course proposes the following objectives:

Knowledge and understanding:

Applying knowledge and understanding

Making judgements:

The

of the student are trained and tested during the course by means the introduction of three ongoing tests, named "In-depth Analysis" . In that test the student must individually study in detail one of the topics presented during the course. His in-depth analysis is based on the study of scientific peer-reviewed papers, on their elaboration and critical presentation in the form of seminar, by using blackboard or slides, during specific days within in the presence of other students that participate asking questions and discussing in a round table.  

Communication skills

The

of the student are trained and tested during the course, a part from the "In-Depth Analyses", by means of writing an essay (25 pages at maximum) and presenting a seminar on a selected topic based on the detailed study of original literature (three papers at minimum). That project represents the final examination for the student. 

Learning skills

All the following main topics, considered in the Dublin Descriptor, in particular case: 

of the student are properly formed, encouraged, trained and testes during the Cosmic Ray Physics Course on the basis of the course contents (in particular concerning the study of main present experiments, the opportunity to access to the corresponding databases and bibliographic and scientific resources) and the custom of on-going seminars - a part from the final examination - that oblige the student to exercise oneself and implement all the above-mentioned abilities. 

Course Structure

Lectures (class taught lessons) for a total amount of 6 CFU = 42 hours ( 1 CFU = 7 hours) developed by the faculty member using slides projected by means of an overhead projector and partially carried out on the blackboard. Reading, in depth analysis and detailed study of reference scientific articles in the Cosmic Ray Physics sector. Articles and references will be provided lecture by lecture, before or during each lecture; collection of the slides used during each lecture will be given at the end of the course.


Required Prerequisites

Fundamentals of General Physics 1 and 2, Classic Electromagnetism, Special Relativity. Basics of Nuclear Physics, Particle Physics, Astroparticle Physics. Elements of Radiation-Matter Interactions. Fundamentals of operating principles of Particle Detectors. 

Attendance of Lessons

The attendance of this course is usually mandatory (please, refer to the "Regolamento Didattico del Corso di Studi").

Detailed Course Content

0) Introduction: Cosmic Ray Physics in the context of the Astroparticle Physics

1) The discovery of the Cosmic Rays or Cosmic Radiation: the hystorical path  

2) Introduction to the Cosmic Ray Physics: properties, origin, acceleration and propagation of the primary Cosmic Rays 

3) Measurements of the Cosmic Rays for E<10^15eV (direct measurements)

4) The Extensive Air Showers (EAS) and the hybrid technique for the detection of the Extensive Air Showers

5)  Measurements of the Cosmic Rays for E>10^15 eV (indirect measurements): use of the Surface Detectors

6) Measurements of the Cosmic Rays for E>10^15 eV (indirect measurements): use of the Fluorescence Detectors

7) The Pierre Auger Observatory

Textbook Information

  1. T. Stanev "High Energy Cosmic Rays", Springer (Berlin, 2004)
  2. M.S. Longair “High Energy Astrophysics”  Cambridge University Press (Cambridge, 1990)
  3. T.K. Gaisser "Cosmic Rays and Particle Physics", Cambridge University Press (Cambridge, 1990)
  4. D. Perkins "Particle Astrophysics", Oxford University Press (Oxford, 2003)
  5. Dr. Peter K.F. Grieder  "Extensive Air Showers -  High Energy Phenomena and Astrophysical Aspects A Tutorial, Reference Manual and Data Book" - Volume 1 & Volume 2  (Springer Verlag Berlin Heidelberg 2010)
  6. A. De Angelis, M.Pimenta "Introduction to Particle and Astroparticle Physics - Multimessenger Astronomy and its Particle Physics Foundations" - Springer (1st edition, 2015)

Course Planning

 SubjectsText References
10) Introduction: Cosmic Ray Physics in the context of the Astroparticle Physics1. Stanev (Chapter 1)
21) The discovery of the Cosmic Rays or Cosmic Radiation: the hystorical path 7. De Angelis-Pimenta (Chapter 3);
32) Introduction to the Cosmic Ray Physics: properties, origin, acceleration and propagation of the primary Cosmic Rays1. Stanev (Chapters 2, 3, 4, 9); 2. Longair (Chapters 15, 16, 17, 18); 3. Gaisser (Chapters 1, 9, 11, 12); 4. Perkins (Part 3, Chapter 9)
43) Measurements of the Cosmic Rays for E<10^15eV (direct measurements)1. Stanev (Chapters 5, 7); 7. De Angelis-Pimenta (Chapter 4);
54) The Extensive Air Showers (EAS) and the hybrid technique for the detection of the EAS1. Stanev (Chapters 6, 8); 3. Gaisser (Chapters 14, 15, 16); 6. Grieder (Part 1 - Chapters 3, 4, 5, 6, 7, 8, 9)
65) Measurements of the Cosmic Rays for E>10^15 eV (indirect measurements): use of the Surface Detectors7. De Angelis-Pimenta (Chapter 4); 6. Gredier (Part 2 - Chapters 1, 8)
76) Measurements of the Cosmic Rays for E>10^15 eV (indirect measurements): use of the Fluorescence Detectors7. De Angelis-Pimenta (Chapter 4); 6. Gredier ( Part 2 - Chapters 1, 5, 6)
87) The Pierre Auger Observatory scientific papers

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