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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


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Yalçın KALKAN Uludağ University

and... Cluster Ions Cluster Ions

15th RD51 Collaboration Meeting, CERN, (16-20 March 2015) 15th RD51 Collaboration Meeting, CERN, (16-20 March 2015)

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Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 2

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Pad Gate Cathode wires F i e l d w i r e s A n

  • d

e w i r e s

TPC TPC

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Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 4

Ar+ Reactions How fast the Reactions ? Ne+ Reactions

( Rate Cons. from Vincent G. Anicich (1993) and John Hornbeck (1951) ( Rate Cons. from V.G. Anicich and W.T. Huntress, Jr.(1986) and Boris M. Smirnov, (1992) ( Rate Cons. from Boris M. Smirnov, (1992)

Atmospheric pressure and 10 % mixture Atmospheric pressure and 10 % mixture

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Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 5

CO2

+ Reactions

How fast the Reactions ?

( )

(Rate Cons. from Boris M. Smirnov, (1992) Rate Cons. from Vincent G. Anicich (1993)

110 ps 7 - 20 ps

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Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 6

* 90 % of the initial ions are Ar+

Clustering dynamics 8 torr 8 torr

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Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 7

Cluster size

Andreas J. Illies(1988) The Cluster does not grow further at 300 K and low pressure (70 - 400 Pa). Andreas J. Illies(1989) n ≈ 4.3 (on 18 molecules) ~ Atmospheric pressure H.W. Ellis et al. (1976) Y . Ikezoe et al. (1982) N= 0-4 At low and atmospheric pressure

Pressure : 0.5 – 3 Torr Pressure : 0.5 – 3 Torr n=1 n=1

n = 2-8 (HCO+.CO2) At atmospheric pressure

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Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 8

Transition Transition

After a few microseconds there will be only : After a few microseconds there will be only : * CO * CO2

2CO2

CO2.

. Clusters

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 !

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Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 9

Mobilitiy of CO2 and CO2 clusters

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Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 10

in in in

 Clusters

Clusters

P .A. Coxon and J.L. Moruzzi (1979)

Conflicting data S =2.2 Compatible data S = 1.3 No data

1.07±0.04% cm2/V.s

at 53-67 Pa

P .A. Coxon and J.L. Moruzzi (1979)

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Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 11

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Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 12

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Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 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-CO2 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).

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Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 14

Blanc's law : mobility in mixture

K

0: reduced mobility

and

f 1 f 2 : molar fractions

if the component gases react between them : FAIL If there is clustering in the gas : mobility will change

1 K mix = f 1 K1

0 +

f 2 K2

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Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 15

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Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 16

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Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 17

Conclusions Conclusions

The signal ions are just CO The signal ions are just CO2

2.(CO

.(CO2

2) clusters, they

) clusters, they are not CO are not CO+

+ 2 2 or noble gas ions.

  • r noble gas ions.

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 !

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Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 18

Ionisation rates

Plots prepared by Özkan Şahin by using Magboltz 10.6

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Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 19

e e-

  • 0.013 Pa

(Rate Cons. from V.G. Anicich and W.T. Huntress,(1986) and Boris M. Smirnov, (1992)

300 ns

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Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 20

TPC measurements TPC measurements

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Yalçın KALKAN, 15th RD51 Collaboration Meeting, CERN 21