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Studies of the correlations of ultra-high energy cosmic ray directions with extra-Galactic objects, of general anisotropy, of photons and neutrinos, and of other astrophysical effects, with the Pierre Auger Observatory. Contributions to the…

High Energy Astrophysical Phenomena · Physics 2009-07-10 The Pierre Auger Collaboration , J. Abraham , P. Abreu , M. Aglietta , C. Aguirre , E. J. Ahn , D. Allard , I. Allekotte , J. Allen , J. Alvarez-Muñiz , M. Ambrosio , L. Anchordoqui , S. Andringa , A. Anzalone , C. Aramo , E. Arganda , S. Argirò , K. Arisaka , F. Arneodo , F. Arqueros , T. Asch , H. Asorey , P. Assis , J. Aublin , M. Ave , G. Avila , T. Bäcker , D. Badagnani , K. B. Barber , A. F. Barbosa , S. L. C. Barroso , B. Baughman , P. Bauleo , J. J. Beatty , T. Beau , B. R. Becker , K. H. Becker , A. Bellétoile , J. A. Bellido , S. BenZvi , C. Berat , P. Bernardini , X. Bertou , P. L. Biermann , P. Billoir , O. Blanch-Bigas , F. Blanco , C. Bleve , H. Blümer , M. Boháčová , D. Boncioli , C. Bonifazi , R. Bonino , N. Borodai , J. Brack , P. Brogueira , W. C. Brown , R. Bruijn , P. Buchholz , A. Bueno , R. E. Burton , N. G. Busca , K. S. Caballero-Mora , L. Caramete , R. Caruso , W. Carvalho , A. Castellina , O. Catalano , L. Cazon , R. Cester , J. Chauvin , A. Chiavassa , J. A. Chinellato , A. Chou , J. Chudoba , J. Chye , R. W. Clay , E. Colombo , R. Conceição , B. Connolly , F. Contreras , J. Coppens , A. Cordier , U. Cotti , S. Coutu , C. E. Covault , A. Creusot , A. Criss , J. Cronin , A. Curutiu , S. Dagoret-Campagne , R. Dallier , K. Daumiller , B. R. Dawson , R. M. de Almeida , M. De Domenico , C. De Donato , S. J. de Jong , G. De La Vega , W. J. M. de Mello Junior , J. R. T. de Mello Neto , I. De Mitri , V. de Souza , K. D. de Vries , G. Decerprit , L. del Peral , O. Deligny , A. Della Selva , C. Delle Fratte , H. Dembinski , C. DiGiulio , J. C. Diaz , P. N. Diep , C. Dobrigkeit , J. C. D'Olivo , P. N. Dong , A. Dorofeev , J. C. dos Anjos , M. T. Dova , D. D'Urso , I. Dutan , M. A. DuVernois , R. Engel , M. Erdmann , C. O. Escobar , A. Etchegoyen , P. Facal San Luis , H. Falcke , G. Farrar , A. C. Fauth , N. Fazzini , F. Ferrer , A. Ferrero , B. Fick , A. Filevich , A. Filipčič , I. Fleck , S. Fliescher , C. E. Fracchiolla , E. D. Fraenkel , W. Fulgione , R. F. Gamarra , S. Gambetta , B. García , D. GarcíaGámez , D. Garcia-Pinto , X. Garrido , G. Gelmini , H. Gemmeke , P. L. Ghia , U. Giaccari , M. Giller , H. Glass , L. M. Goggin , M. S. Gold , G. Golup , F. Gomez Albarracin , M. Gómez Berisso , P. Gonçalves , M. Gonçalves do Amaral , D. Gonzalez , J. G. Gonzalez , D. Góra , A. Gorgi , P. Gouffon , S. R. Gozzini , E. Grashorn , S. Grebe , M. Grigat , A. F. Grillo , Y. Guardincerri , F. Guarino , G. P. Guedes , J. Gutiérrez , J. D. Hague , V. Halenka , P. Hansen , D. Harari , S. Harmsma , J. L. Harton , A. Haungs , M. D. Healy , T. Hebbeker , G. Hebrero , D. Heck , V. C. Holmes , P. Homola , J. R. Hörandel , A. Horneffer , M. Hrabovský , T. Huege , M. Hussain , M. Iarlori , A. Insolia , F. Ionita , A. Italiano , S. Jiraskova , M. Kaducak , K. H. Kampert , T. Karova , P. Kasper , B. Kégl , B. Keilhauer , E. Kemp , R. M. Kieckhafer , H. O. Klages , M. Kleifges , J. Kleinfeller , R. Knapik , J. Knapp , D. -H. Koang , A. Krieger , O. Krömer , D. Kruppke-Hansen , F. Kuehn , D. Kuempel , K. Kulbartz , N. Kunka , A. Kusenko , G. LaRosa , C. Lachaud , B. L. Lago , P. Lautridou , M. S. A. B. Leão , D. Lebrun , P. Lebrun , J. Lee , M. A. Leigui de Oliveira , A. Lemiere , A. Letessier-Selvon , M. Leuthold , I. Lhenry-Yvon , R. López , A. Lopez Agüera , K. Louedec , J. Lozano Bahilo , A. Lucero , H. Lyberis , M. C. Maccarone , C. Macolino , S. Maldera , D. Mandat , P. Mantsch , A. G. Mariazzi , I. C. Maris , H. R. Marquez Falcon , D. Martello , O. Martínez Bravo , H. J. Mathes , J. Matthews , J. A. J. Matthews , G. Matthiae , D. Maurizio , P. O. Mazur , M. McEwen , R. R. McNeil , G. Medina-Tanco , M. Melissas , D. Melo , E. Menichetti , A. Menshikov , R. Meyhandan , M. I. Micheletti , G. Miele , W. Miller , L. Miramonti , S. Mollerach , M. Monasor , D. Monnier Ragaigne , F. Montanet , B. Morales , C. Morello , J. C. Moreno , C. Morris , M. Mostafá , C. A. Moura , S. Mueller , M. A. Muller , R. Mussa , G. Navarra , J. L. Navarro , S. Navas , P. Necesal , L. Nellen , C. Newman-Holmes , D. Newton , P. T. Nhung , N. Nierstenhoefer , D. Nitz , D. Nosek , L. Nožka , M. Nyklicek , J. Oehlschläger , A. Olinto , P. Oliva , V. M. Olmos-Gilbaja , M. Ortiz , N. Pacheco , D. Pakk Selmi-Dei , M. Palatka , J. Pallotta , G. Parente , E. Parizot , S. Parlati , S. Pastor , M. Patel , T. Paul , V. Pavlidou , K. Payet , M. Pech , J. Pȩkala , I. M. Pepe , L. Perrone , R. Pesce , E. Petermann , S. Petrera , P. Petrinca , A. Petrolini , Y. Petrov , J. Petrovic , C. Pfendner , R. Piegaia , T. Pierog , M. Pimenta , T. Pinto , V. Pirronello , O. Pisanti , M. Platino , J. Pochon , V. H. Ponce , M. Pontz , P. Privitera , M. Prouza , E. J. Quel , J. Rautenberg , O. Ravel , D. Ravignani , A. Redondo , B. Revenu , F. A. S. Rezende , J. Ridky , S. Riggi , M. Risse , C. Rivière , V. Rizi , C. Robledo , G. Rodriguez , J. Rodriguez Martino , J. Rodriguez Rojo , I. Rodriguez-Cabo , M. D. Rodríguez-Frías , G. Ros , J. Rosado , T. Rossler , M. Roth , B. Rouillé-d'Orfeuil , E. Roulet , A. C. Rovero , F. Salamida , H. Salazar , G. Salina , F. Sánchez , M. Santander , C. E. Santo , E. M. Santos , F. Sarazin , S. Sarkar , R. Sato , N. Scharf , V. Scherini , H. Schieler , P. Schiffer , A. Schmidt , F. Schmidt , T. Schmidt , O. Scholten , H. Schoorlemmer , J. Schovancova , P. Schovánek , F. Schroeder , S. Schulte , F. Schüssler , D. Schuster , S. J. Sciutto , M. Scuderi , A. Segreto , D. Semikoz , M. Settimo , R. C. Shellard , I. Sidelnik , B. B. Siffert , G. Sigl , A. Śmiałkowski , R. Šmída , B. E. Smith , G. R. Snow , P. Sommers , J. Sorokin , H. Spinka , R. Squartini , E. Strazzeri , A. Stutz , F. Suarez , T. Suomijärvi , A. D. Supanitsky , M. S. Sutherland , J. Swain , Z. Szadkowski , A. Tamashiro , A. Tamburro , T. Tarutina , O. Taşcău , R. Tcaciuc , D. Tcherniakhovski , D. Tegolo , N. T. Thao , D. Thomas , R. Ticona , J. Tiffenberg , C. Timmermans , W. Tkaczyk , C. J. Todero Peixoto , B. Tomé , A. Tonachini , I. Torres , P. Travnicek , D. B. Tridapalli , G. Tristram , E. Trovato , M. Tueros , R. Ulrich , M. Unger , M. Urban , J. F. Valdés Galicia , I. Valiño , L. Valore , A. M. vandenBerg , J. R. Vázquez , R. A. Vázquez , D. Veberič , A. Velarde , T. Venters , V. Verzi , M. Videla , L. Villaseñor , S. Vorobiov , L. Voyvodic , H. Wahlberg , P. Wahrlich , O. Wainberg , D. Warner , A. A. Watson , S. Westerhoff , B. J. Whelan , G. Wieczorek , L. Wiencke , B. Wilczyńska , H. Wilczyński , C. Wileman , M. G. Winnick , H. Wu , B. Wundheiler , T. Yamamoto , P. Younk , G. Yuan , A. Yushkov , E. Zas , D. Zavrtanik , M. Zavrtanik , I. Zaw , A. Zepeda , M. Ziolkowski

In this chapter I give an overview of shock acceleration, including a discussion of the maximum energies possible and the shape of the spectrum near cut-off, interactions of high energy cosmic rays with, and propagation through, the…

Astrophysics · Physics 2007-05-23 R. J. Protheroe

The existence of cosmic ray particles up to the ultra-high energy limit (> 10^20 eV) is now beyond any doubt. The detection of cosmic particles with such energies imposes a challenge for the comprehension of their sources and nature. On one…

We review the main experimental evidences on ultra high energy cosmic rays and their implications in the physics of these extremely energetic particles, also in connection with dark matter and cosmology. We discuss the basis of theoretical…

High Energy Astrophysical Phenomena · Physics 2023-03-01 Roberto Aloisio

This paper deals with the cosmic-ray penetration into molecular clouds and with the related gamma--ray emission. High energy cosmic rays interact with the dense gas and produce neutral pions which in turn decay into two gamma rays. This…

High Energy Astrophysical Phenomena · Physics 2015-06-11 Stefano Gabici

I give a brief overview of cosmic ray physics, highlighting some key questions and how they will be addressed by new experiments.

Astrophysics · Physics 2011-05-12 Thomas K. Gaisser

Physicists have pondered the origin of cosmic rays for over a hundred years. However the last few years have seen an upsurge in the observation, progress in the theory and a genuine increase in the importance attached to the topic due to…

High Energy Astrophysical Phenomena · Physics 2015-06-22 Roger Blandford , Paul Simeon , Yajie Yuan

While there is some level of consensus on a Galactic origin of cosmic rays up to the knee ($E_{k}\sim 3\times 10^{15}$ eV) and on an extragalactic origin of cosmic rays with energy above $\sim 10^{19}$ eV, the debate on the genesis of…

High Energy Astrophysical Phenomena · Physics 2015-06-19 Pasquale Blasi

Cosmic high energy neutrinos are inextricably linked to the origin of cosmic rays which is one of the major unresolved questions in astrophysics. In particular, the highest energy cosmic rays observed possess macroscopic energies and their…

High Energy Physics - Phenomenology · Physics 2007-05-23 G. Sigl

The article gives a brief overview, aimed at nonspecialists, about the goals and selected recent results of the detection of very-high energy gamma-rays (energies above 100 GeV) with ground based detectors. The stress is on the physics…

Astrophysics · Physics 2009-09-25 R. Plaga

The images of ultrahigh-energy cosmic ray sources get distorted, in an energy dependent way, by the effects of Galactic and extragalactic magnetic fields. These deflections can also affect the observed cosmic ray spectrum, specially when…

High Energy Astrophysical Phenomena · Physics 2022-03-02 Silvia Mollerach , Esteban Roulet

Cosmic rays fill up the entire volume of galaxies, providing an important source of heating and ionisation of the interstellar medium, and may play a significant role in the regulation of star formation and galactic evolution. Diffuse…

High Energy Astrophysical Phenomena · Physics 2015-06-03 Troy A. Porter

Cosmic ray nuclei, cosmic ray electrons with energy above a few GeV, and the diffuse gamma-ray background radiation (GBR) above a few MeV, presumed to be extragalactic, could all have their origin or residence in our galaxy and its halo.…

Astrophysics · Physics 2007-05-23 Arnon Dar , A. De Rújula , Nikos Antoniou

We present a brief introduction to the physics of Ultra High Energy Cosmic Rays (UHECRs), concentrating on the experimental results obtained so far and on what, from these results, can be inferred about the sources of UHECRs.

Astrophysics · Physics 2007-05-23 Daniel De Marco

One century ago Viktor Hess carried out several balloon flights that led him to conclude that the penetrating radiation responsible for the discharge of electroscopes was of extraterrestrial origin. One century from the discovery of this…

High Energy Astrophysical Phenomena · Physics 2015-06-18 Pasquale Blasi

Very high energy {\gamma}-rays are one of the most important messengers of the non-thermal Universe. The major motivation of very high energy {\gamma}-ray astronomy is to find sources of high energy cosmic rays. Several astrophysical…

High Energy Astrophysical Phenomena · Physics 2022-01-19 D. Bose , V. R. Chitnis , P. Majumdar , A. Shukla

We study the deflection of ultra high energy cosmic ray protons in different models of the regular galactic magnetic field. Such particles have gyroradii well in excess of 1 kpc and their propagation in the galaxy reflects only the large…

Astrophysics · Physics 2010-11-30 Todor Stanev

The origin of the ultra high energy cosmic rays (UHECR) with energies above E > 1017eV, is still unknown. The discovery of their sources will reveal the engines of the most energetic astrophysical accelerators in the universe. This is a…

High Energy Astrophysical Phenomena · Physics 2016-04-27 M. T. Dova

Very high energy gamma-rays probe the long-standing mystery of the origin of cosmic rays. Produced in the interactions of accelerated particles in astrophysical objects, they can be used to image cosmic particle accelerators. A first…

Astrophysics · Physics 2014-10-13 F. A. Aharonian

We discuss the basic difficulties in understanding the origin of the highest energy particles in the Universe - the ultrahigh energy cosmic rays (UHECR). It is difficult to imagine the sources they are accelerated in. Because of the strong…

Astrophysics · Physics 2017-08-23 Todor Stanev