LIP Summer Projects 2018 - Detectors & Instrumentation - CERN
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[ LIP Summer Projects 2018 ] Detectors & Instrumentation
LIP Welcomes You
Coimbra, Lisboa, Minho
~ 200 members
~ 90 PhD
~ 75 students
~ 27 engineers, technicians
7 administrative staff
• Experimental Particle Physics and Astrophysics
• Development of Instrumentation
• Scientific Computing
LIP: Particle Physics
Spanning a magnitude of scales
Detectors from the bottom of deep mines to outer space
Research infrastructure
Detector & instrumentation R&D
Scientific Computing
• Information & Technology R&D
• Participation in digital infrastructures and international consortia
• Support to scientific community
• Students become collaborators in LIP’s research teams
LIP
Summer • 1 week of introductory lectures + hands-on tutorials
Student • Integrate research projects from 2 weeks to 2 months
• 1 day long final workshop where each student present
Program his/her work to fellow students and the LIP researchers
• Locations: Lisbon (3Is complex, IST, FCUL, TagusLIP),
University of Coimbra, and University of Minho
• How to apply? Students select up to 5 projects in order of
Registration: 27/4-18/5
Internships: Jul - Sept preference; to facilitate selection should share interests and
Tutorials: 9-13/7 past experience (academic, research, computing, electronics, etc)
Final workshop: 5/9
www.lip.pt/summer-student-program
2017 in pictures !
Detectors & Instrumentation – 16 April 5-7pm
Project Characterization and development of (hardware and software)
Presentation systems that facilitate scientific research.
Sessions
@IST Physics at the LHC – 17 April 5-7pm
Precision measurements and searches for physics beyond the
Standard Model with data from the LHC experiments
Projects grouped in 4
themes = 4 sessions Astroparticle Physics – 18 April 5-7pm
Physics with cosmic rays, the elusive neutrinos and searches
for dark matter
Be invited to attend
one or all sessions.
Physics of ultra-relativistic hadronic matter – 19 Apr. 5-7pm
Do not hesitate to ask Exploring the structure of matter – from nucleons and nuclei to
your questions! the plasma of quarks and gluonsDetector &
Instrumentation
The art of characterizing and
developing systems
(hardware/software) that allow Auger
the scientific investigation
TagusLip
LOMAC
LabRC NUC-RIAProjects available
9 Projects in Lisbon
1 Project in Coimbra
Experiments (type of project): Auger
o 1x Auger (hardware)
o 1x LabRC (software)
o 1x Muon Tomography (software)
o 2x NUC – RIA (hardware and software) TagusLip
o 1x SNO+ (hardware and software)
o 1x TagusLIP/CMS (hardware)
o 2x ATLAS (hardware & sofware) LOMAC
o 1x Muon detection (Coimbra)
LabRC NUC-RIAPierre Auger
Observatory
Located in the Pampa Amarilla, it is the
largest observatory in the world dedicated to
the study of Ultra High Energy Cosmic Rays
(UHECRs)
The main array is composed by more that
1600 water Cherenkov detectors which are
overlooked by 4 Fluorescence Detectors
The study of UHECRs allows not only to
understand the nature and acceleration
mechanisms of the most energetic known
particles but also can be used to probe
hadronic interaction above LHC energiesAuger:
Develop an RPC - a gaseous
particle detector
In Auger we use RPCs to detect muons. We
have a small test one to be built. Several
solutions can be tested in this system. It will
be the base component of a precision
telescope.
Period: 2 months, June-September
Contact: Pedro Assis
pedjor@lip.ptMuon Tomography
Cosmic ray muons are deeply penetrating particles.
Muon telescopes can form images of the interior of
mines, vulcanos, builidings, and even the nuclear
reactors and cargo containers
Producing and analysing muon tomographic
images.
Period: 2 months, June-September
Contact: Lorenzo Cazon, Sofia Andringa
cazon@lip.ptMonitorização de
LabRC: muões
Desenvolvimento de um
display de taxas de muões atmosféricos
Os muões são partículas criadas na interação
dos raios cósmicos com a atmosfera. No
Laboratório de Raios Cósmicos existem
detectores de cintilação capazes de detectar
estas partículas.
As taxas de muões detectadas na Terra
apresentam variações de várias ordens (diárias
e sazonais).
Correlações com observações meteorológicas:
http://meteo.tecnico.ulisboa.pt/obs/live
Variabilidade temporal nas
taxas de muões
atmosféricosDetector cintilador
LabRC:
Desenvolvimento de um
display de taxas de muões
O que se propõe neste trabalho é o
desenvolvimento de software que permita
monitorar em permanência a chegada de
muões à Terra. Para isso será necessário
calcular a sua taxa de deteção, e construir
de seguida um gráfico (display) que permita Leitura Remota
mostrar a taxa ao longo do tempo num ecrã
de computador.
O display poderá ser realizado através da
implementação de um servidor web.
DAQ
Pretende-se que o aparato experimental PC
esteja ligado pela rede a um micro-
computador que será responsável pelo Monitor
display. Dept. Física
Micro PC RedeDetecções de Muões
Atmosféricos
LabRC:
Desenvolvimento de um
display de taxas de muões
Projecto de estágio:
Desenvolvimento de um
display de taxas de muões
Outros projectos:
Optimização de algoritmos através
de métodos de paralelização
Contacts:
Fernando Barão (barao@lip.pt)
Miguel Orcinha (migorc@lip.pt)SNO+:
Energy response calibration of
the SNO+ neutrino experiment person
o High precision neutrino detector located
deep underground (2 km below the surface
in a Canadian mine)!
12 m diameter acrylic sphere
surrounded by 9300 light
sensitive detectors
We are here!
Muons or
neutrinos?Antineutrinos from
nuclear reactor
SNO+: Neutrinos from Antineutrinos from
Energy response calibration of the Sun the Earth
the SNO+ neutrino experiment
o High precision neutrino detector located
deep underground (2 km below the surface
in a Canadian mine)!
o Large physics program & rare event
searches: Important to characterize the
detector for good quality data
Rare decay modes Neutrinos and
to visible particles Antineutrinos from
Supernovae
Rare decay modes
to invisible particle1 2 3 4 5 6
A 18,9
SNO+:
A A
2
Energy response calibration of Oring14*1,5
3
the SNO+ neutrino experiment
24,5
B B
1
15
0,7
4
o Signal type: Scintillation light
3
A SECTION A-A
o Detection mode: Photomultiplier tube (light
C
SCALE 3 : 1
C
sensitive device) hit
DO NOT SCALE DRAWING
UNLESS OTHERWISE SPECIFIED: ISO 2768-fH T is ra ing is
REVISION
Problem: Energy to photons conversion
LIP property. It FIRST ANGLE PROJECTION
o ISO 8015
DIMENSIONS ARE IN MILLIMETERS
can't e
DEBUR AND BREAK SHARP EDGES ISO 13715 repro uce or
communicate Laboratório de Instrumentação e Física Experimental de Partículas
ISO 1302 it out LIP Departamento Física, Universidade de Coimbra 3004 516 Coimbra - Portugal
agreement. www.lip.pt Telef. +351 239 833 376
NAME SIGNATURE DATE Email TITLE:
Solution: Calibration
ITEM NO. PART NUMBER QTY.
o
DRAWN RUI F. ALVES rui2010alves@gmail.com
D
1 4830_23_06_2017_LIPL_SNO_AcrylicInnerContainer-Base-RuiA 1 CHK'D Acrylic Inner Container
APPV'D
2 4833_23_06_2017_LIPL_SNO_AcrylicInnerContainer-Top-RuiA 1
Calibration
MFG
3 4831_23_06_2017_LIPL_SNO_AcrylicInnerContainer-Oring1415-RuiA 1 Q.A MATERIAL:
PMMA DWG NO. LIPD-SNOD-4914-01 A4
4 4834_23_06_2017_LIPL_SNO_AcrylicInnerContainer-Sample-RuiA 3 (anneal) 4832_11_07_2017_LIPL_SNO_AcrylicInnerContainer-Assem-RuiA
1 2 WEIGHT: SCALE:2:1 SHEET 1 OF 1
source
Period: 1-2 months, July-August
Contact: Valentina Lozza
vlozza@lip.ptNUC-RIA:
Produção e caraterização de
filmes finos
• Produção de filmes finos de Ag (~100
nm até 1-2 µm) pela técnica da
evaporação térmica.
• Caraterização com fonte alfa.
• Medida da espessura em base à
perca de energia das partículas alfa.
Períod: 1 month, July or September
Contacts: Daniel Galaviz, Pamela Teubig
galaviz@lip.ptNUC-RIA:
Uso e automatização do
código AlfaMC
• Simulação com o código AlfaMC do
espetro de partículas alfa emitidas por
fontes radioativas
• Simulação e medida do espectro alfa
após perca de energia em filmes finos
• Automatização para extrair a
espessura de filmes finos por ajuste a
espectros experimentais
Período: 6 semanas, Julho e Setembro
Contacto: Luís Peralta, Daniel Galaviz
luis@lip.pt , galaviz@lip.ptLarge Hadron Collider o 27 km perimeter o The LHC collides protons, and also Pb ions o Coldest place in the galaxy o 40 M p bunch crossings/s!! o Hottest place in the galaxy (interaction point) o Up to 60 pp interactions per bunch crossing
Looking into the origin of the Universe
ATLAS & CMS
Huge & complex detectors
o Cutting edge technology
o 108 electronic channels
o Process in real time 40 M bunch
crossing/second
o Selects ~1000 for offline
analysis
o Dedicated specialized
electronics and softwareThe ATLAS trigger New!!
Under validation!
system
AFPATLAS: jet
Validation of the central
exclusive di-jet trigger jet
o Fundamental for QCD physics
studies
o Responsibility of Portuguese team
o Requires:
o 2 diffracted p, 2 jets
o Nothing else
o Performance study using ATLAS
data
Period: 2 months, July/September
Contact: Patricia Conde Muiño
patricia.conde.muino@cern.chLOMAC Lab
LOMAC Lab (@FCUL, @LIP):
o Dedicated test benches
o Optical characterization of Optical fibers
( Fibrometer )
o Optical characterization of Scintillators
( Tilemeter )
o Sputtering setup for top aluminization of
fibersCells A, BC, D =
1.1 Tilecal main scintillators
ATLAS Upgrade: Cannot be replaced.
Dose increase
1.2
Cells E = gap-crack
Optics Replacement 1.3
accessible
1.4
1.5
Problem: Scintillator and cells are damaged by
1.6
radiation
Effect: light loss during High Luminosity LHC
Extension to 1.75
operation
Solution: TileCal estimate light loss (in
progress)
replace part of the E cells
Motivation: E cells scintillators are important
to improve:
* e/gamma and jet energy
reconstruction
* Fake Jets RejectionATLAS:
Scintillators and fibers for the upgrade of
the TileCal hadron calorimeter of the
ATLAS experiment at CERN
Activities @ LOMAC Lab (@FCUL, @LIP):
o Fibers and Scintillators for ATLAS/Upgrade
o Light Output decrease due to radiation damage
and ageing
o Estimation of scitillators and fibers lifetime
o New design of fiber routing for upgrade
o Fiber bending – curvature radius needs to be
studied
o Scintillators for future detectors (for FCC)
Period: July/1-15 August/September
o Maps of light collection
Contact: Agostinho Gomes
o Tests of new photodetectors;
agomes@lip.ptPositron Emission Tomography (PET)
18
In F-Fluorodeoxyglucose
(FDG) the radioisotope
Fluorine (18F) emits a
positron.
TagusLIP à Noninvasive imaging technique that
provides a functional or metabolic
assessment of tissue
Activities
Positron Emission Tomography (PET)
à In 18F-Fluorodeoxyglucose (FDG) the Positron range in FWHM
is 0.22mm. Half life of
radioisotope
In 18
F-Fluorodeoxyglucose 18
Fluorine ( F) emits a FDG is 110min.
(FDG) the radioisotope
positron.
18
Fluorine (18
F) emits a Instead of F as well
11 13 15
positron. possible: C, N, O,
68
Ga,82Rb
Active in development of detector modules
Stefan Gundacker 14th VCI, 18 February 2016 2
and readout electronics for medical
applications:
Positron range in FWHM
is 0.22mm. Half life of T. Niknejad, Jornadas LIP, Evora, 2018
FDG is 110min.
o ASICs for photo-sensors 18
Instead of F as well
possible: 11C, 13N, 15O,
Complete DAQ systems
68
Ga,82Rb
o
o Gamma ray detectors
Stefan Gundacker 14th VCI, 18 February 2016 2
Recently active in development of the
readout system for a large Particle Physics 2048 SiPM channels
experiment based on the same technologyThe Current CMS Detector
TagusLIP :
Overview of the CMS and HL- CMS Detector
SILICON TRACKER
Pixels (100 x 150 μm2)
~1m2 ~66M channels
LHC project Pixels
Microstrips (80-180μm)
~200m2 ~9.6M channels
CRYSTAL ELECTROMAGNETIC
Tracker CALORIMETER (ECAL)
ECAL ~76k scintillating PbWO4 crystals
HCAL
- The current CMS detector Solenoid PRESHOWER
Steel Yoke Silicon strips
Muons ~16m2 ~137k channels
o different layers of detectors measure the
different particles produced in high-energy STEEL RETURN YOKE
~13000 tonnes
collisions in the LHC, and use this key data to
build up a picture of events at the heart of the SUPERCONDUCTING
SOLENOID
Niobium-titanium coil
collision. carrying ~18000 A FORWARD
CALORIMETER
Steel + quartz fibres
~2k channels
HADRON CALORIMETER (HCAL)
Total weight : 14000 tonnes Brass + plastic scintillator MUON CHAMBERS
- The High-Luminosity Large Hadron Collider (HL- Overall diameter
Overall length
:
:
15.0 m
28.7 m
~7k channels Barrel: 2250 Drift Tube & 480 Resistive Plate Chambers
Endcaps: 473 Cathode Strip & 432 Resistive Plate Chambers
Magnetic field : 3.8 T
LHC) project will increase luminosity (rate of collisions)
by a factor of 5 beyond the LHC’s design value Josh Bendavid (CERN/LPC) CMS HL-LHC 2
- Significant upgrades of CMS for HL-LHC
conditions
o Radiation hardness
o Mitigate the impact of the high pile-up dataTagusLIP:
CMS Upgrade: High-precision
timing detetors for HL-LHC
Fact: At the HL - LHC an average of 140 – 200
pileup events (collisions per bunch crossing) will 9 Artur Apresyan | TREDI 2017
occur
Problem: This can degrade the identification and the From past presentations
reconstruction of the interaction
Solution: Use precise time stamp of particles to
provide a 4th dimension to CMS object reconstruction
Requirements: Dedicated detector for precise timing
(~30 ps timing resolution)
o Barrel Timing Layer (BTL) is a new timing
detector in the CMS for charged particlesiming layer in the barrel
TagusLIP:
Use thin (few mm) scintillating crystals to
Barrel
generate Timing Layer (BTL)
light:
– LYSO crystals provide a very bright signal to a
BTL sensor:
osingle MIP (up to ~40000 photons per mm) BTL single
BTL singlesensor
sensortest
test
– 100%
- LYSOefficient
scintillatingto MIPtowith
crystals good
generate lightS/N
- SiPM to detect light
– Good radiation tolerance to HL-LHC conditions
- Readout ASIC
oLIP is responsible for the development of the
Lightreadout
read-out
system ofusing SiPMs:
the new detector including the
development of a new ASIC in collaboration with
– Fast and compact devices
PETsys Electronics (for the first time)
– Vast experience (CMS HCAL) and testing for
Timing wall at CMS
o Summer project: Timing wall at CMS
radiation hardness, collaboration with Period: 1 month, July/August 2018
manufacturers,
- Characterization of different SiPMs (to be used in Location: Taguspark in Oeiras
– BTL) using single photon laser pulse
Strong knowledge from R&D for TOF-PET Contact: Tahereh Niknejad
tniknejad@lip.ptYou can also read
