'Good measurement' diaporamas de présentation

The pp-chain and the CNO-cycle after KamLAND

The pp-chain and the CNO-cycle after KamLAND. Solar neutrinos after SNO and KamLAND The Boron flux The Beryllium flux Nuclear physics of the pp-chain Can the sun shine with CNO? New challenges for solar model builders The Sun as a laboratory for fundamental physics

492 views • 34 slides

CMMI and Metrics BCS SPIN SG, 19 February 2008 Clifford Shelley OXFORD SOFTWARE ENGINEERING Ltd

CMMI and Metrics BCS SPIN SG, 19 February 2008 Clifford Shelley OXFORD SOFTWARE ENGINEERING Ltd 9 Spinners Court, 53 West End, Witney, Oxfordshire OX28 1NH www.osel.co.uk info@osel.co.uk Tel. +44 (0) 1993 700878. Objective.

392 views • 31 slides

Beam Sizes measured by BaBar

376 views • 27 slides

From Nuclei to Neutrinos The Naming of the Denys Wilkinson Building 21 June 2002 Nick Jelley

From Nuclei to Neutrinos The Naming of the Denys Wilkinson Building 21 June 2002 Nick Jelley. The Optical Model. d s/ d W. 29 MeV 3 He on 14 N 1962. Particle Identification. p. d. 3 H. 3 He. D E. E. 4 He. 10 100 MeV. p. d. 4 He. 3 H.

290 views • 20 slides

215 views • 9 slides