'Pierre auger' diaporamas de présentation

Presented for Arnulfo Zepeda On behalf of the Mexican Collaboration

PHYSICS AND ASTROPHYSICS OF ULTRA HIGH ENERGY COSMIC RAYS. BUAP CINVESTAV UMSNH UNAM. Presented for Arnulfo Zepeda On behalf of the Mexican Collaboration. Material selected and prepared for Rebeca López. Sep. 2000. GOAL.

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Large Array Astrophysics Detectors (I)

2010 LNF Spring School Frascati, 13 May 2010. Large Array Astrophysics Detectors (I). Giorgio Matthiae University and Sezione INFN of Roma Tor Vergata. Cosmic ray spectrum year 2000. ~ 1 / E 3. 1 particle/km 2 /century. LHC c.m. Cosmic ray spectrum - 2009. knee.

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DOE Annual Program Review Center for Particle Astrophysics Scott Dodelson

DOE Annual Program Review Center for Particle Astrophysics Scott Dodelson. We study Fundamental Physics. Dark Energy Dark Matter Neutrino Mass Seeds of Primordial Structure. These are arguably the most compelling discoveries to date of Physics Beyond the Standard Model.

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Roma Meeting: June 2007

Roma Meeting: June 2007. Recent results from the Pierre Auger Observatory (and comparisons with AGASA and HiRes) Alan Watson University of Leeds a.a.watson@leeds.ac.uk. The Pierre Auger Collaboration. Aim : To measure properties of UHECR with unprecedented

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The Cosmic Ray Observatory Project (CROP): An outreach and education experiment in Nebraska

The Cosmic Ray Observatory Project (CROP): An outreach and education experiment in Nebraska. Funded by a $1,342,000 grant from the National Science Foundation Teacher Enhancement Program and High Energy Physics. A high school based Pierre Auger Observatory. Where is Nebraska?. Fermilab

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The Cosmic Ray Observatory Project (CROP): An outreach and education experiment in Nebraska

The Cosmic Ray Observatory Project (CROP): An outreach and education experiment in Nebraska. Funded by a $1,342,000 grant from the National Science Foundation Teacher Enhancement Program and High Energy Physics. A high school based Pierre Auger Observatory. Where is Nebraska?. Fermilab

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An introduction to COSMIC RAYS

Catch a Cosmic Ray Program. An introduction to COSMIC RAYS. COSMIC RAYS:. Messages from exploding stars and even more powerful objects. What are cosmic rays? How do we detect them? What can we learn from them? Where do they come from?. History of Cosmic Rays: 1785-1902.

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Dan Hooper Theoretical Astrophysics Group Fermi National Laboratory dhooper@fnal

Theoretical Particle-Astrophysics At Fermilab. Dan Hooper Theoretical Astrophysics Group Fermi National Laboratory dhooper@fnal.gov. Annual DOE Review May 17, 2006. How To Study Particle Physics?. Traditionally, particle physics has been studied using collider experiments

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Auger Electron Spectroscopy

Auger Electron Spectroscopy. (AES). Principle of AES. A fine focused electron beam bombards the sample and ejects an electron of the inner shell of the atom. This vacancy must be refilled by an electron from a higher energy level.

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The Pierre Auger Project

The Pierre Auger Project. By Megan Edwards Bancroft-Rosalie. Pierre Auger. Can be considered as the discoverer of the giant air showers in 1938 generated by the interaction of very high-energy cosmic rays with the earth's atmosphere.

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NA61/SHINE physics program: - Critical Point and Onset of Deconfinement , -High p T physics

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A possible origin of ultra-high energy cosmic rays: collisions of two galaxies

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Status of the Pierre Auger Observatory

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