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LAGUNA/LBNO WP4: secondary beam line status report

LAGUNA/LBNO WP4: secondary beam line status report. LAGUNA/LBNO DS meeting / December 2012. M. Calviani , P. Velten , A. Ferrari, I. Efthymiopoulos, C. Lazaridis (CERN) + M. Zito , V. Galymov (CEA), A. Rubbia, S. Murphy, S. Di Luise (ETHZ). Organization of the WG and activities.

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LAGUNA/LBNO WP4: secondary beam line status report

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  1. LAGUNA/LBNO WP4: secondary beam line status report LAGUNA/LBNO DS meeting / December 2012 M. Calviani, P. Velten, A. Ferrari, I. Efthymiopoulos, C. Lazaridis (CERN) + M. Zito, V. Galymov(CEA), A. Rubbia, S. Murphy, S. Di Luise (ETHZ)

  2. Organization of the WG and activities • Focused (for the moment) on: • Agreement on the main physics parameters (ok now!) • Optimization of beam/target optimization • Configurations of horn • Muons in the ND and configuration of the decay pipe • CERN-oriented meetings held on a ~monthly basis to discuss the activities within the sub-WG • Steering the activities on the LAGUNA/LBNO secondary beam line • Participation to external members working on some aspects of the beam line in other institutes • Important input from the experiment! M. Calviani -- LAGUNA/LBNO DS General Meeting

  3. Target-horn distance and horn current optimization M. Calviani -- LAGUNA/LBNO DS General Meeting

  4. Horn-reflector distance and reflector current optimization M. Calviani -- LAGUNA/LBNO DS General Meeting

  5. M. Calviani -- LAGUNA/LBNO DS General Meeting

  6. M. Calviani -- LAGUNA/LBNO DS General Meeting

  7. nmfluence in ND/FD • dTH=0 cm / IH=220 kA • dHR=6 m / IR=275 kA M. Calviani -- LAGUNA/LBNO DS General Meeting

  8. M. Calviani -- LAGUNA/LBNO DS General Meeting

  9. m± fluence with passive shielding M. Calviani -- LAGUNA/LBNO DS General Meeting

  10. m± fluencewith active toroidal shielding with 29 Tm bending power M. Calviani -- LAGUNA/LBNO DS General Meeting

  11. M. Calviani -- LAGUNA/LBNO DS General Meeting

  12. Conclusions • Much work to do still…! M. Calviani -- LAGUNA/LBNO DS General Meeting

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