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Cosmic ray physics and AUGER latest results

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What is at stake<br />

109<br />

■<br />

Major discoveries related to CRs<br />

◆ Non-thermal astronomy!<br />

◆ Central role of CRs in Galactic ecology<br />

◆ Existence of CRs up to >10 20 eV!<br />

◆ CR astronomy is possible!<br />

(ionisation, heating, magnetic<br />

fields, astrochemistry, LiBeB<br />

nucleosynthesis, star<br />

formation…)<br />

challenge for particle<br />

acceleration!<br />

Overcome isotropization by magnetic field<br />

underst<strong>and</strong>ing<br />

of propagation<br />

CRs at source<br />

+ acceleration<br />

+ (astro)<strong>physics</strong><br />

of sources<br />

■<br />

■<br />

■<br />

Physics of powerful, HE sources<br />

Physics in “extreme conditions”<br />

Multi-scale problem + conditions<br />

very different from laboratory exp.<br />

underst<strong>and</strong>ing<br />

of acceleration<br />

astro<strong>physics</strong> of the<br />

intervening medium<br />

+ propagation <strong>physics</strong><br />

■<br />

■<br />

Access to high-energy processes<br />

Signatures of “exotic” <strong>physics</strong><br />

→ “astroparticle <strong>physics</strong>”<br />

Paris, 9 th June 2008 — IDAPPʼs two days 2008 — E. Parizot (APC / Univ. Paris 7)

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