*Chih-Hsiang Yeh, Sergei Chekanov (Argonne National Lab), Ashutosh Kotwal (Duke University), Shin-Shan Eiko Yu (National Central University)
Physics potential of timing layers in future collider detectors
2020/11/11
Physics potential of timing layers in future collider detectors - - PowerPoint PPT Presentation
Physics potential of timing layers in future collider detectors *Chih-Hsiang Yeh, Sergei Chekanov (Argonne National Lab), Ashutosh Kotwal (Duke University), Shin-Shan Eiko Yu (National Central University) 2020/11/11 Outline Motivation
*Chih-Hsiang Yeh, Sergei Chekanov (Argonne National Lab), Ashutosh Kotwal (Duke University), Shin-Shan Eiko Yu (National Central University)
Physics potential of timing layers in future collider detectors
2020/11/11
Outline
Motivation
Add Timing Info
Publications of our studies
References
physics at a 100TeV pp collider [JINST/P06009]
TeV pp collider[JINST/P05008]
→ →
6Publications of our studies
References
→ →
7Software and Structure
), 35
𝖽𝗇𝟥 𝖸𝟣
9The advantage of TL2
production vertex”
particle back-scattered hits can be identified.
→
10Capability of timing
12Peaks are smaller than 1ns Seen as instantaneous hits
→
Resolution: 1ns Resolution: 10ps Distinguish the different particles apart(1GeV) 𝖴𝖴𝖬𝟥 − 𝖴𝖴𝖬𝟤 = 𝖴 (1) (2) Landau peak: 0.7ns Mean: 1.4ns Peak: 0.5ns Peak: 0.5ns Peak: 0.5ns Distinguishable! Non-distinguishable! GEANT4 Simulation! Leading in time hits
Semi-analytic 3- hypothesis
σ
13L: Length of particle’s trajectory : Resolution of the detector m: Particle mass p: Momentum of particle : Reference particle mass
σ𝖴𝖯𝖦 𝗇𝖦
If the condition is met, particle can be distinguished from
𝗇 𝗇𝖦
(JHEP 04 (2019) 037 [arXiv:1807.05453)]
The showcase of 3- hypothesis
σ
14K mesons from Pions Heavy particle(BSM) from particle(BKG)
α
With 1ns resolution, 300MeV-500MeV can be achieved=>Not enough for FCC! Minimum~0.5GeV L= 2m from vertex to ECAL
3GeV
BSM studies General cases
700GeV 70GeV 0.4GeV
Another case
15L=0.2m from TL1 to TL2
100GeV 200GeV
Beneficial for particles produced in events with large pile-up (multiple pp interactions)! Also, we don’t need to know about the interaction vertex
0.2m TL1 TL2 Heavy particle(BSM) from particle(BKG)
α
15GeV
Showcase of Dark QCD model
P P
MX MX
SM quark Dark quark SM quark Dark quark Dark Pion Emerging jet
Dark Pion Emerging jet
Test the capability of using the timing to tag the Dark Pion
16 DecayJHEP 05 (2015) 059
Setup
CMS s = 𝟤𝟦𝖴𝖿𝖶 SiFCC s = 𝟥𝟪𝖴𝖿𝖶 Production Vertex to ECAL(L) L=1.2m L=2m Dark Pion(m) Momentum of Dark Pion(p) particle ( )
α mF
Momentum of Dark Pion(p)
17Track acceptance vs. Calorimeter with the timing
18Cover the different ranges! Dark Pion Mass=5GeV, Varying the ctau and Mediator Mass
JHEP 02 (2019) 179
Emerging jets with the same condition as CMS
19Dark Pion Mass=5GeV, Varying the ctau and Mediator Mass With the higher resolution With the higher lifetime The acceptance is higher!
Emerging jets for HL-LHC with SiFCC
20Mediator Mass=10TeV, Varying the ctau and Dark Pion mass With the higher resolution With the higher lifetime The acceptance is higher!
Conclusion
the standard ~0.5 - 1 ns readout
Q&A TIME