neutron detection in the new stt configuration...neutron detection in the new stt configuration l....

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Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala

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Page 1: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

Neutron detection in the new STT configuration

L. Di Noto, F. Ferraro, P. Sala

Page 2: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

Geometry

OLD NEW

6 blocks, each composed of one module with graphite target followed by 12 standard CH2 modules with target slab and radiator

Page 3: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

Geometry – zoom

OLD NEW

Page 4: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

Geometry – zoom again

OLD NEW

Page 5: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

Neutron spectrum at vertex

We should better compare this spectrum with the one used in GEANT

Details on interactions on H and C in the following slide

Page 6: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

Neutron spectrum at vertexinteractions on H and C

We should better compare these spectra with the ones used in GEANT

Page 7: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

Disclaimer on the efficiency

• When we say “w/o endcaps” we do not consider at all the neutrons causing hits in the endcaps (as if they were not even generated)

• The endcaps are not yet completely simulated (homogeneous material)

• We can certainly study the efficiency without a time cut, but it has to be considered in the real experiment

• In this comparison we are not considering the time resolution (we are considering the MC truth)

Page 8: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

Effect of the 50 ns time cut – old geometry

Detected at larger time!

From vertexBarrel without time cutBarrel with time cutStt without time cutStt with time cut

The time cut is prevalently affecting low-momentum neutrons from interactions on C

Page 9: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

Detection efficiencyw/o endcapsw/o 50 ns time cut

OLD NEW

59.7%47.4%21.5%

37.9%30.5%12.0%

Page 10: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

Detection efficiencyw/o endcapsw/ 50 ns time cut

OLD NEW

36.2%29.9%10.4%

32.2%24.3%11.9%

Page 11: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

Detection efficiencyw/ endcapsw/o 50 ns time cut

OLD NEW

75.8%47.0%39.3%29.6%

55.6%35.9%23.4%21.5%

Page 12: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

Detection efficiencyw/ endcapsw/ 50 ns time cut

OLD NEW

52.3%32.2%21.4%14.6%

47.4%28.5%17.0%13.0%

Page 13: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

Energy reconstructionw/o endcapsw/o 50 ns time cut

OLD NEW

Page 14: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

Energy reconstruction (w/i 30% from true value)w/o endcapsw/o 50 ns time cut

OLD NEW

3255/9173 ≅ 35.5% 4093/12318 ≅ 33.2%

Of detected events

Page 15: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

Energy reconstructionw/o endcapsw/o 50 ns time cut

OLD NEW

3255/9173 ≅ 35.5% 4093/12318 ≅ 33.2%

Of detected events

Page 16: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

Multiplicityw/o endcapw/o 50 ns time cut

OLD NEW

Undetected! Undetected!

Page 17: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module
Page 18: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

Efficiency plot for monochromatic neutronstowards barrel or endcap in new and old geometry

Page 19: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

New geometry - low density test (LDT)upward neutron beam (towards barrel)

new - LDT

BARRELENDCAPSSTT

No time cut 50 ns time cut

Page 20: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

w/o endcapsw/ timecut

eff stt: 0.0416264eff barrel: 0.0914848eff endcap: 3.33278e-05eff combined: 0.114481

w/o endcapsw/o timecut

eff stt: 0.0640227eff barrel: 0.220897eff endcap: 3.33278e-05eff combined: 0.254991

Comparison – old, new and new-LDT(no beam towards the endcaps in new-LDT)

w/ endcapsw/ timecut

eff stt: 0.062075eff barrel: 0.131925eff endcap: 0.036775eff combined: 0.177225

new - LD

Lower density => lower endcap eff., higher barrel and stt eff. Lower density => very little difference

No time cut

Page 21: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

/eos/user/l/ldinoto/Neutron_traj_STTNEW_40file.root

/eos/user/l/ldinoto/Neutron_xFederico_v1_STTNEW_40file.root

Page 22: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

For 68% of neutrons detected at time>500 ns and interacting inside SAND, the neutrons trajectory was studied

The time of last interaction of a primary neutron is quite similar to its time of detectionexcept for those (about 40% of this group) where the primary neutron interacts early, emitting secondary neutrons which wanders around interacting later

Page 23: Neutron detection in the new STT configuration...Neutron detection in the new STT configuration L. Di Noto, F. Ferraro, P. Sala Geometry OLD NEW 6 blocks, each composed of one module

Summary

We looked at the new STT configuration, in particular:• Interacting nuclei• neutron detection efficiency, where we found some differences that should

be investigated further• Energy reconstruction• Neutron multiplicity• Some tests to address the “efficiency issue”

We looked at the behavior of the neutrons detected at very late times:• some neutrons are going outside and/or wandering a lot before they are

detected