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and... Cluster Ions Cluster Ions Yaln KALKAN Uluda University - PowerPoint PPT Presentation

and... Cluster Ions Cluster Ions Yaln KALKAN Uluda University 15th RD51 Collaboration Meeting, CERN, (16-20 March 2015) 15th RD51 Collaboration Meeting, CERN, (16-20 March 2015) Yaln KALKAN, 15th RD51 Collaboration Meeting, CERN 2


  1. and... Cluster Ions Cluster Ions Yalçın KALKAN Uludağ University 15th RD51 Collaboration Meeting, CERN, (16-20 March 2015) 15th RD51 Collaboration Meeting, CERN, (16-20 March 2015)

  2. Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 2

  3. TPC TPC Gate Cathode wires A F i n e o l d d e w w i r e i r s e s Pad

  4. How fast the Reactions ? Atmospheric pressure and 10 % mixture Atmospheric pressure and 10 % mixture Ar + Reactions ( Rate Cons. from Vincent G. Anicich (1993) and John Hornbeck (1951) Ne + Reactions ( Rate Cons. from V.G. Anicich and W.T. Huntress, Jr.(1986) and Boris M. Smirnov, (1992) ( Rate Cons. from Boris M. Smirnov, (1992) Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 4

  5. How fast the Reactions ? CO 2 + Reactions ) 7 - 20 ps ( (Rate Cons. from Boris M. Smirnov, (1992) 110 ps Rate Cons. from Vincent G. Anicich (1993) Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 5

  6. Clustering dynamics 8 torr 8 torr * 90 % of the initial ions are Ar + Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 6

  7. Cluster size Pressure : 0.5 – 3 Torr Pressure : 0.5 – 3 Torr n=1 n=1 Andreas J. Illies(1988) The Cluster does not grow further at 300 K and low pressure (70 - 400 Pa). H.W. Ellis et al. (1976) n = 2-8 (HCO + .CO 2 ) At atmospheric pressure Andreas J. Illies(1989) n ≈ 4.3 (on 18 molecules) ~ Atmospheric pressure Y . Ikezoe et al. (1982) N= 0-4 At low and atmospheric pressure Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 7

  8. Transition Transition After a few microseconds there will be only : After a few microseconds there will be only : * CO 2 CO2 . Clusters * CO 2 CO2 . Clusters * Ar Dimers * Ar Dimers * Ne Dimers * Ne Dimers We will estimate the mobilities of this object ! We will estimate the mobilities of this object ! Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 8

  9. Mobilitiy of CO 2 and CO 2 clusters Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 9

  10. in in in  Clusters Clusters 1.07±0.04% cm 2 /V.s No data  at 53-67 Pa P .A. Coxon and J.L. Moruzzi (1979) Compatible data S = 1.3 P .A. Coxon and J.L. Moruzzi (1979) Conflicting data S =2.2 Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 10

  11. Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 11

  12. Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 12

  13. Data sources Data sources NA49 TPC data from Rainer Renfordt (transit time between anode and field wire). ALICE TPC data from Chilo, Marian, Christian Lippmann and Mesut (transit time between anode and cathode wire). Coimbra data from Pedro Encarnação and André F.V. Cortez (20 Td uniform field between GEM and mesh, at 8 torr). P.M.C.C. Encarnação et al., Experimental Ion Mobility measurements in Ar-CO 2 mixtures, Journal of Instrumentation 10 (2015) P01010 (20 Td uniform field between GEM and mesh, at 8 torr). G. Schultz et al., Mobilities of positive ions in some gas mixtures used in proportional and drift chambers, Revue de Physique Appliquée (Paris) 12 (1977) 67–70 (E/N ≤ 20 Td field between 2 wire meshes, at 1 atm). Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 13

  14. Blanc's law : mobility in mixture f 1 f 2 1 = 0 + 0 0 K mix K 1 K 2 0 : reduced mobility K f 1 f 2 : molar fractions and if the component gases react between them : FAIL If there is clustering in the gas : mobility will change Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 14

  15. Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 15

  16. Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 16

  17. Conclusions Conclusions The signal ions are just CO 2 .(CO 2 ) clusters, they The signal ions are just CO 2 .(CO 2 ) clusters, they are not CO + or noble gas ions. are not CO + 2 or noble gas ions. 2 It is experimentally confirmed by the literature. It is experimentally confirmed by the literature. Cluster ions are heavier and slower than CO + Cluster ions are heavier and slower than CO + 2 2 ions. ions. Mass spectrometry unavoidable ! Mass spectrometry unavoidable ! Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 17

  18. Ionisation rates Plots prepared by Özkan Şahin by using Magboltz 10.6 Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 18

  19. e - - e 0.013 Pa 300 ns (Rate Cons. from V.G. Anicich and W.T. Huntress,(1986) and Boris M. Smirnov, (1992) Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 19

  20. TPC measurements TPC measurements Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 20

  21. Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 21

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