Nader MIRABOLFATHI (.pdf) - Observatoire de Paris

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Nader MIRABOLFATHI (.pdf) - Observatoire de Paris

Nader MIRABOLFATHI (.pdf) - Observatoire de Paris

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List of registered participants - Chalonge School - Observatoire de ...

Annalisa PERISSA (.pdf)

Aurel SCHNEIDER (.pdf)

Sabino MATARRESE (.pdf)

Highlights and Conclusions of the Colloquium (.pdf) - Chalonge ...

Chalonge Medal - Chalonge School - Observatoire de Paris

Peter BIERMANN (.pdf)

Rainer BECK (.pdf)

Julien LESGOURGUES (.pdf)

THE NATURE OF LIGHT DARK MATTER Peter L. Biermann ...

George F. SMOOT (.pdf)

SPRING OPEN SESSION OF SCIENTIFIC CULTURE(.pdf)

Sinziana PADUROIU (.pdf)

Victor DEMARIA-PESCE (.pdf)

Sinziana PADUROIU (.pdf)

W I M P For Ω χ ~0.3: Comoving Number Density σ A ~ electroweak Production = Annihilation (T≥m χ ) ~exp(-m/T) Production suppressed (T

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Page 1: Dark Matter Search: Experiments Nad
Page 5 and 6: Interaction rate (II)
Page 7 and 8: χ Event-by-Event discrimination (I
Page 9 and 10: WIMP-detection Experiments Worldwid
Page 11 and 12: CDMS: Detection Principle • Measu
Page 13 and 14: CDMSII results T1 T2 noisy 14 C con
Page 15 and 16: CDMSII results T1 T2 noisy 14 C con
Page 17 and 18: Noble gas principle (I) Single phas
Page 19 and 20: CLEAN ZEPLIN II Calibration Noble g
Page 21 and 22: Xenon 10 Calibration, Rejection Ast
Page 23 and 24: •CDMS: Increased Ge mass from 1.5
Page 25 and 26: Exciting immediate future (I) CDMS: