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RPC SENSITIVITY TO LOW ENERGY NEUTRONS AND GAMMA RAYS

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EPS-HEP2001 Budapest , july 12-18, 2001. SERGIO P. RATTI INFN and Dipartimento di Fisica Nucleare e Teorica – PAVIA for the Pavia-Bari collaboration in CMS. RPC SENSITIVITY TO LOW ENERGY NEUTRONS AND GAMMA RAYS. RPC SENSITIVITY TO LOW ENERGY NEUTRONS AND GAMMA RAYS. - PowerPoint PPT Presentation
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RPC SENSITIVITY TO LOW ENERGY NEUTRONS AND GAMMA RAYS EPS-HEP2001 Budapest , , july 12-18, 2001 SERGIO P. RATTI SERGIO P. RATTI INFN and Dipartimento di Fisica Nucleare e Teorica – PAVIA for the Pavia-Bari collaboration in CMS RPC SENSITIVITY TO LOW ENERGY NEUTRONS AND GAMMA RAYS
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Page 1: RPC SENSITIVITY  TO LOW ENERGY NEUTRONS AND GAMMA RAYS

RPC SENSITIVITY TO LOW ENERGY NEUTRONS ANDGAMMA RAYS

EPS-HEP2001Budapest, , july 12-18, 2001EPS-HEP2001

Budapest, , july 12-18, 2001

SERGIO P. RATTISERGIO P. RATTIINFN and Dipartimento di Fisica Nucleare e Teorica – PAVIA

for the Pavia-Bari collaboration in CMS

SERGIO P. RATTISERGIO P. RATTIINFN and Dipartimento di Fisica Nucleare e Teorica – PAVIA

for the Pavia-Bari collaboration in CMS

RPC SENSITIVITY TO LOW ENERGY NEUTRONS ANDGAMMA RAYS

Page 2: RPC SENSITIVITY  TO LOW ENERGY NEUTRONS AND GAMMA RAYS

MotivationMotivation

Experimental setupExperimental setup

ResultsResults

Conclusions and Conclusions and outlookoutlook

OUTLINE OF THE TALKOUTLINE OF THE TALK

Page 3: RPC SENSITIVITY  TO LOW ENERGY NEUTRONS AND GAMMA RAYS

Experimental Experimental setupsetupExperimental Experimental setupsetup

BaF2 scintillators

2 single gap/common readout RPC’s2 single gap/common readout RPC’s

sourcesource1717CiCi 252 252Cf:Cf:a-3%a-3% spontaneous fission;spontaneous fission;b-b-97%97% decay decay (irrelevant, (irrelevant,absorbed by the source’absorbed by the source’container).container).

1717CiCi 252 252Cf:Cf:a-3%a-3% spontaneous fission;spontaneous fission;b-b-97%97% decay decay (irrelevant, (irrelevant,absorbed by the source’absorbed by the source’container).container).

1 gap oiled1 gap not oiled1 gap oiled1 gap not oiled

Page 4: RPC SENSITIVITY  TO LOW ENERGY NEUTRONS AND GAMMA RAYS

THE SOURCETHE SOURCETHE SOURCETHE SOURCE

3.8 n/fission3.8 n/fissionEEavav= 2.14 MeV= 2.14 MeV 10.310.3 prompt prompt

per fissionper fission

80% E<1MeV80% E<1MeV

NEUTRON AND NEUTRON AND SPECTRA OF THE SOURCE SPECTRA OF THE SOURCE

Page 5: RPC SENSITIVITY  TO LOW ENERGY NEUTRONS AND GAMMA RAYS

Sensitive area: 35 cm x 35 cmGas mixture (97 % C2H2F4 – 3% iC4H10)

Sensitive area: 35 cm x 35 cmGas mixture (97 % C2H2F4 – 3% iC4H10)

OUTPUT signals: LVDS to the counting electronics

(Low Voltage Differential Signals)

16 strips

RPCs Cross RPCs Cross SectionSection

Pickup strips

Page 6: RPC SENSITIVITY  TO LOW ENERGY NEUTRONS AND GAMMA RAYS

FOUR FOUR CONFIGURATIONSCONFIGURATIONS:FOUR FOUR CONFIGURATIONSCONFIGURATIONS:

A) No absorber between RPC and source

B) 6 cm Pb between RPC and source

C) 6 cm Pb and 4 cm PE

D) 6 cm Pb and 10 cm PE

Page 7: RPC SENSITIVITY  TO LOW ENERGY NEUTRONS AND GAMMA RAYS

Experimental method:Experimental method:

TriggerTrigger

Trigger AND

Chamber OR16

Trigger AND

Chamber OR16

RPCRPC

BaF2 scintillatorsBaF2 scintillators

SourceSource

= (Triggers x OR16)/Triggers

= efficiency to fission

= chamber acceptance

= (Triggers x OR16)/Triggers

= efficiency to fission

= chamber acceptance

Compare to simulation

results

Compare to simulation

results

Page 8: RPC SENSITIVITY  TO LOW ENERGY NEUTRONS AND GAMMA RAYS

Experimental dataExperimental data Experimental dataExperimental data

Effective Neutron Interaction length

Xeq

Xeq = XPb/Pb + XPE/PE

=interaction length

Effective Neutron Interaction length

Xeq

Xeq = XPb/Pb + XPE/PE

=interaction length

What we measure is

= (Triggers x OR16)/Triggers

= efficiency to fission

= chamber acceptance

What we measure is

= (Triggers x OR16)/Triggers

= efficiency to fission

= chamber acceptance

GAP oil

Xeq

Double Gap

Xe

q

GAP non oil

Xeq

Page 9: RPC SENSITIVITY  TO LOW ENERGY NEUTRONS AND GAMMA RAYS

Xeq

Experimental data vs simulation results

Experimental data vs simulation results

Data contain contribution from:

a) Prompt rays from source

b) Prompt neutrons from Source

c) Secondary rays from neutron interactions within the different absorbers

Data contain contribution from:

a) Prompt rays from source

b) Prompt neutrons from Source

c) Secondary rays from neutron interactions within the different absorbers

Simulation (with GEANT3.21) used to extract the relative contribution of each component a)

b) c)

Simulation (with GEANT3.21) used to extract the relative contribution of each component a)

b) c)

Page 10: RPC SENSITIVITY  TO LOW ENERGY NEUTRONS AND GAMMA RAYS

Xeq Xeq

-oil-oil

Gamma ray sensitivity (preliminary results)Gamma ray sensitivity (preliminary results)

Prompt rays Secondary rays

Page 11: RPC SENSITIVITY  TO LOW ENERGY NEUTRONS AND GAMMA RAYS

Neutron Sensitivity Results (preliminary)

Neutron Sensitivity Results (preliminary)

Sensitivity independent on oiling!

Xeq

-oil

Page 12: RPC SENSITIVITY  TO LOW ENERGY NEUTRONS AND GAMMA RAYS

CONCLUSIONSCONCLUSIONS

Poor measurements

of this parameter

Sensitivity (S)

less than 1%;

SSn;

Double gap doubles;

S independ

on surface treatment

(at least

at this

low energies

1 MeV)

Poor measurements

of this parameter

Sensitivity (S)

less than 1%;

SSn;

Double gap doubles;

S independ

on surface treatment

(at least

at this

low energies

1 MeV)

Summary of sensitivity results

Single Gap Sensitivity <Energy>(MeV)

Prompt 3,50E-03 0,84

" 7,50E-03 1,45

Secondary 6,50E-03 1,35

Neutron 3,00E-04 2,1

Double Gap Sensitivity <Energy>(MeV)

Prompt 6,00E-03 0,84

" 1,30E-02 1,45

Secondary 1,10E-02 1,35

Neutron 5,30E-04 2,1


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