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Recent measurements of the properties of cosmic rays above 10^17 eV are summarized and implications on our contemporary understanding of their origin are discussed. Cosmic rays with energies exceeding 10^20 eV have been measured, they are…

Astrophysics · Physics 2015-05-13 Joerg R. Hoerandel

These are extended notes of a series of lectures given at the XIth Brazilian School of Cosmology and Gravitation. They provide a selection of topics at the intersection of particle and astrophysics. The first part gives a short introduction…

High Energy Physics - Phenomenology · Physics 2009-11-10 Guenter Sigl

We discuss the most recent developments in our understanding of the acceleration and propagation of cosmic rays up to the highest energies. In particular we specialize our discussion to three issues: 1) developments in the theory of…

Astrophysics · Physics 2009-11-11 Pasquale Blasi

The launch of the Fermi gamma-ray space telescope and the imaging air Cerenkov telescopes H.E.S.S., MAGIC, and VERITAS have substantially transformed our knowledge of gamma-ray sources in the last decade. The extragalactic gamma-ray sky is…

High Energy Astrophysical Phenomena · Physics 2013-09-02 C. Pfrommer

I review several ongoing connections between space physics and astrophysics: a) Measurements of energetic particle spectra have confirmed theoretical prediction of the highest energy to which shocks can accelerate particles, and this has…

Astrophysics · Physics 2009-11-10 David Eichler

A fundamental question that can be answered in the next decade is: WHAT IS THE ORIGIN OF THE HIGHEST ENERGY COSMIC PARTICLES? The discovery of the sources of the highest energy cosmic rays will reveal the workings of the most energetic…

High Energy Astrophysical Phenomena · Physics 2009-03-03 A. V. Olinto , J. H. Adams , C. D. Dermer , J. F. Krizmanic , J. W. Mitchell , P. Sommers , T. Stanev , F. W. Stecker , Y. Takahashi

Gamma Ray Bursts are among the most powerful astrophysical sources and they release up to 1.e54 erg, if isotropic, in less than few hundred seconds. Their detection in the hard X/gamma ray band (at energies >10 keV) and out to very high…

Astrophysics · Physics 2017-08-23 G. Ghirlanda , G. Ghisellini

Gamma-ray Astronomy studies cosmic accelerators through their electromagnetic radiation in the energy range between ~100 MeV and ~100 TeV. The present most sensitive observations in this energy band are performed, from space, by the Large…

High Energy Astrophysical Phenomena · Physics 2011-11-29 Javier Rico

In the last talk of the conference I summarized the main progress and contributions to high energy astrophysics made by studies of microquasars in our Galaxy. To stimulate the general discussion I have underlined some of the questions that…

Astrophysics · Physics 2007-05-23 I. F. Mirabel

In this chapter, we discuss the contributions of gamma-ray astronomy at TeV energies to our understanding of the visible content and structure of the universe. We start from the present epoch with the second most intense electromagnetic…

High Energy Astrophysical Phenomena · Physics 2021-12-14 Elisa Pueschel , Jonathan Biteau

The Proceedings of the 2011 workshop on Fundamental Physics at the Intensity Frontier. Science opportunities at the intensity frontier are identified and described in the areas of heavy quarks, charged leptons, neutrinos, proton decay, new…

High Energy Physics - Experiment · Physics 2012-05-14 J. L. Hewett , H. Weerts , R. Brock , J. N. Butler , B. C. K. Casey , J. Collar , A. de Gouvea , R. Essig , Y. Grossman , W. Haxton , J. A. Jaros , C. K. Jung , Z. T. Lu , K. Pitts , Z. Ligeti , J. R. Patterson , M. Ramsey-Musolf , J. L. Ritchie , A. Roodman , K. Scholberg , C. E. M. Wagner , G. P. Zeller , S. Aefsky , A. Afanasev , K. Agashe , C. Albright , J. Alonso , C. Ankenbrandt , M. Aoki , C. A. Arguelles , N. Arkani-Hamed , J. R. Armendariz , C. Armendariz-Picon , E. Arrieta Diaz , J. Asaadi , D. M. Asner , K. S. Babu , K. Bailey , O. Baker , B. Balantekin , B. Baller , M. Bass , B. Batell , J. Beacham , J. Behr , N. Berger , M. Bergevin , E. Berman , R. Bernstein , A. J. Bevan , M. Bishai , M. Blanke , S. Blessing , A. Blondel , T. Blum , G. Bock , A. Bodek , G. Bonvicini , F. Bossi , J. Boyce , R. Breedon , M. Breidenbach , S. J. Brice , R. A. Briere , S. Brodsky , C. Bromberg , A. Bross , T. E. Browder , D. A. Bryman , M. Buckley , R. Burnstein , E. Caden , P. Campana , R. Carlini , G. Carosi , C. Castromonte , R. Cenci , I. Chakaberia , M. C. Chen , C. H. Cheng , B. Choudhary , N. H. Christ , E. Christensen , M. E. Christy , T. E. Chupp , E. Church , D. B. Cline , T. E. Coan , P. Coloma , J. Comfort , L. Coney , J. Cooper , R. J. Cooper , R. Cowan , D. F. Cowen , D. Cronin-Hennessy , A. Datta , G. S. Davies , M. Demarteau , D. P. DeMille , A. Denig , R. Dermisek , A. Deshpande , M. S. Dewey , R. Dharmapalan , J. Dhooghe , M. R. Dietrich , M. Diwan , Z. Djurcic , S. Dobbs , M. Duraisamy , B. Dutta , H. Duyang , D. A. Dwyer , M. Eads , B. Echenard , S. R. Elliott , C. Escobar , J. Fajans , S. Farooq , C. Faroughy , J. E. Fast , B. Feinberg , J. Felde , G. Feldman , P. Fierlinger , P. Fileviez Perez , B. Filippone , P. Fisher , B. T. Flemming , K. T. Flood , R. Forty , M. J. Frank , A. Freyberger , A. Friedland , R. Gandhi , K. S. Ganezer , A. Garcia , F. G. Garcia , S. Gardner , L. Garrison , A. Gasparian , S. Geer , V. M. Gehman , T. Gershon , M. Gilchriese , C. Ginsberg , I. Gogoladze , M. Gonderinger , M. Goodman , H. Gould , M. Graham , P. W. Graham , R. Gran , J. Grange , G. Gratta , J. P. Green , H. Greenlee , R. C. Group , E. Guardincerri , V. Gudkov , R. Guenette , A. Haas , A. Hahn , T. Han , T. Handler , J. C. Hardy , R. Harnik , D. A. Harris , F. A. Harris , P. G. Harris , J. Hartnett , B. He , B. R. Heckel , K. M. Heeger , S. Henderson , D. Hertzog , R. Hill , E. A Hinds , D. G. Hitlin , R. J. Holt , N. Holtkamp , G. Horton-Smith , P. Huber , W. Huelsnitz , J. Imber , I. Irastorza , J. Jaeckel , I. Jaegle , C. James , A. Jawahery , D. Jensen , C. P. Jessop , B. Jones , H. Jostlein , T. Junk , A. L. Kagan , M. Kalita , Y. Kamyshkov , D. M. Kaplan , G. Karagiorgi , A. Karle , T. Katori , B. Kayser , R. Kephart , S. Kettell , Y. K. Kim , M. Kirby , K. Kirch , J. Klein , J. Kneller , A. Kobach , M. Kohl , J. Kopp , M. Kordosky , W. Korsch , I. Kourbanis , A. D. Krisch , P. Krizan , A. S. Kronfeld , S. Kulkarni , K. S. Kumar , Y. Kuno , T. Kutter , T. Lachenmaier , M. Lamm , J. Lancaster , M. Lancaster , C. Lane , K. Lang , P. Langacker , S. Lazarevic , T. Le , K. Lee , K. T. Lesko , Y. Li , M. Lindgren , A. Lindner , J. Link , D. Lissauer , L. S. Littenberg , B. Littlejohn , C. Y. Liu , W. Loinaz , W. Lorenzon , W. C. Louis , J. Lozier , L. Ludovici , L. Lueking , C. Lunardini , D. B. MacFarlane , P. A. N. Machado , P. B. Mackenzie , J. Maloney , W. J. Marciano , W. Marsh , M. Marshak , J. W. Martin , C. Mauger , K. S. McFarland , C. McGrew , G. McLaughlin , D. McKeen , R. McKeown , B. T. Meadows , R. Mehdiyev , D. Melconian , H. Merkel , M. Messier , J. P. Miller , G. Mills , U. K. Minamisono , S. R. Mishra , I. Mocioiu , S. Moed Sher , R. N. Mohapatra , B. Monreal , C. D. Moore , J. G. Morfin , J. Mousseau , L. A. Moustakas , G. Mueller , P. Mueller , M. Muether , H. P. Mumm , C. Munger , H. Murayama , P. Nath , O. Naviliat-Cuncin , J. K. Nelson , D. Neuffer , J. S. Nico , A. Norman , D. Nygren , Y. Obayashi , T. P. O'Connor , Y. Okada , J. Olsen , L. Orozco , J. L. Orrell , J. Osta , B. Pahlka , J. Paley , V. Papadimitriou , M. Papucci , S. Parke , R. H. Parker , Z. Parsa , K. Partyka , A. Patch , J. C. Pati , R. B. Patterson , Z. Pavlovic , G. Paz , G. N. Perdue , D. Perevalov , G. Perez , R. Petti , W. Pettus , A. Piepke , M. Pivovaroff , R. Plunkett , C. C. Polly , M. Pospelov , R. Povey , A. Prakesh , M. V. Purohit , S. Raby , J. L. Raaf , R. Rajendran , S. Rajendran , G. Rameika , R. Ramsey , A. Rashed , B. N. Ratcliff , B. Rebel , J. Redondo , P. Reimer , D. Reitzner , F. Ringer , A. Ringwald , S. Riordan , B. L. Roberts , D. A. Roberts , R. Robertson , F. Robicheaux , M. Rominsky , R. Roser , J. L. Rosner , C. Rott , P. Rubin , N. Saito , M. Sanchez , S. Sarkar , H. Schellman , B. Schmidt , M. Schmitt , D. W. Schmitz , J. Schneps , A. Schopper , P. Schuster , A. J. Schwartz , M. Schwarz , J. Seeman , Y. K. Semertzidis , K. K. Seth , Q. Shafi , P. Shanahan , R. Sharma , S. R. Sharpe , M. Shiozawa , V. Shiltsev , K. Sigurdson , P. Sikivie , J. Singh , D. Sivers , T. Skwarnicki , N. Smith , J. Sobczyk , H. Sobel , M. Soderberg , Y. H. Song , A. Soni , P. Souder , A. Sousa , J. Spitz , M. Stancari , G. C. Stavenga , J. H. Steffen , S. Stepanyan , D. Stoeckinger , S. Stone , J. Strait , M. Strassler , I. A. Sulai , R. Sundrum , R. Svoboda , B. Szczerbinska , A. Szelc , T. Takeuchi , P. Tanedo , S. Taneja , J. Tang , D. B. Tanner , R. Tayloe , I. Taylor , J. Thomas , C. Thorn , X. Tian , B. G. Tice , M. Tobar , N. Tolich , N. Toro , I. S. Towner , Y. Tsai , R. Tschirhart , C. D. Tunnell , M. Tzanov , A. Upadhye , J. Urheim , S. Vahsen , A. Vainshtein , E. Valencia , R. G. Van de Water , R. S. Van de Water , M. Velasco , J. Vogel , P. Vogel , W. Vogelsang , Y. W. Wah , D. Walker , N. Weiner , A. Weltman , R. Wendell , W. Wester , M. Wetstein , C. White , L. Whitehead , J. Whitmore , E. Widmann , G. Wiedemann , J. Wilkerson , G. Wilkinson , P. Wilson , R. J. Wilson , W. Winter , M. B. Wise , J. Wodin , S. Wojcicki , B. Wojtsekhowski , T. Wongjirad , E. Worcester , J. Wurtele , T. Xin , J. Xu , T. Yamanaka , Y. Yamazaki , I. Yavin , J. Yeck , M. Yeh , M. Yokoyama , J. Yoo , A. Young , E. Zimmerman , K. Zioutas , M. Zisman , J. Zupan , R. Zwaska

Recent years have seen tremendous progress in our understanding of the extreme universe, which in turn points to even deeper questions to be further addressed. History has shown that the symbiosis between direct observations and laboratory…

Astrophysics · Physics 2007-05-23 Pisin Chen

An emerging theme in modern astrophysics is the connection between astronomical observations and the underlying physical phenomena that drive our cosmos. Both the mechanisms responsible for the observed astrophysical phenomena and the tools…

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

Neutrino astronomy is on the verge of discovering new sources, and this will lead to important advances in astrophysics, cosmology, particle physics, and nuclear physics. This paper is meant for non-experts, so that they might better…

Astrophysics · Physics 2007-06-14 John F. Beacom

Over the last 30 years or so, a handful of events observed in ground-based cosmic ray detectors seem to have opened a new window in the field of high-energy astrophysics. These events have energies exceeding 5x10**19 eV (the region of the…

Astrophysics · Physics 2010-04-15 Murat Boratav

As the Stars and Stellar Evolution (SSE) panel is fully aware, the next decade will see major advances in our understanding of these areas of research. To quote from their charge, these advances will occur in studies of the Sun as a star,…

Instrumentation and Methods for Astrophysics · Physics 2012-08-27 AAS WGLA , : , Nancy Brickhouse , John Cowan , Paul Drake , Steven Federman , Gary Ferland , Adam Frank , Eric Herbst , Keith Olive , Farid Salama , Daniel Wolf Savin , Lucy Ziurys

I review recent developments in cosmology and astrophysics relevant to particle physics, focussing on the following questions: What's new in 1992? What have we learned since the last ICHEP meeting in 1990? and What are the prospects for the…

High Energy Physics - Phenomenology · Physics 2009-09-25 Lawrence M. Krauss

Successfully launched in June 2008, the Fermi Gamma-ray Space Telescope, formerly named GLAST, has been observing the high-energy gamma-ray sky with unprecedented sensitivity for more than two years, opening a new window on a wide variety…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Luca Baldini

We highlight recent theoretical and observational progress in several areas of neutron star astrophysics, and discuss the prospect for advances in the next decade.

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