status of lhcf
DESCRIPTION
Status of LHCf. Alessia Tricomi University of catania & INFN catania on behalf of the LHCf collaboration. Forward photon energy spectrum at √s = 7 TeV p-P collisions Prospects for new analyses Detector upgrade. CSN1Napoli, July 5, 2011. Physics motivations. - PowerPoint PPT PresentationTRANSCRIPT
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AL
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STATU
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LHCF
CSN1 Napoli, July 5, 2011
• Forward photon energy spectrum at √s = 7 TeV p-P collisions
• Prospects for new analyses• Detector upgrade
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
PHYSICS M
OTIVATI
ONS
I MP A
CT
ON
HE
CR
PH
YS
I CS
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
UHECR OBSERVATIONS (10 YEARS AGO AND NOW)
Debate in AGASA, HiRes results in 10 years agoNow Auger, HiRes (final), TA indicate cutoffAbsolute values differ between experiments and
between methods
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
ESTIMATE OF PARTICLE TYPE (XMAX)
Xmax gives information of the primary particle
Results are different between experiments
Interpretation relies on the MC prediction and has quite strong model dependence
0g/cm2
Xmax
Proton and nuclear showers of same total energy
AugerTA
HiRes
Both in th
e energy determinatio
n and X max
prediction M
C simulatio
ns are used, a
nd are one
of the greater s
ources o
f uncerta
inty.
Experimental te
sts of h
adron interacti
on models
are necessary!
LHCf
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
LHCF
@ L
HC
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
Detectors installed in the TAN region, 140 m away from ATLAS Interaction Point (IP1)
Charged particles
Neutral particles
Beam pipe
Protons
LHCF EXPERIMENTAL SET-UP
Here the beam pipe splits in 2 separate tubes. Charged particle are swept away by magnets We cover |h|>8
Front Counters: thin scintillators with 8x8cm2 acceptance installed in front of each main detector
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
ARM1 & ARM2 DETECTORSARM1
2 towers 24 cm long
stacked vertically
with 5 mm gap
Lower: 2 cm x 2 cm
area
Upper: 4 cm x 4 cm
area
Arm#1
90m
m
290mm
Arm#2
ARM22 towers 24 cm long stacked on their edges and offset from one another
Lower: 2.5 cm x 2.5 cmUpper: 3.2 cm x 3.2 cm
16 scintillator layers (3 mm
thick)Trigger and
energy profile measurements
Energy
Impact point (h)
4 pairs of scintillating fiber layers for tracking purpose (6, 10, 32, 38 r.l.)
4 pairs of silicon microstrip layers (6, 12, 30, 42 r.l.) for tracking purpose (X and Y directions)
Absorber22 tungsten layers 7– 14 mm thick (2-4 r.l.) (W: X0 = 3.5mm, RM = 9mm)
Expected Performance Energy resolution (> 100GeV) < 5% for & g p0, 30% for neutrons Position resolution < 200μm (Arm#1), 40μm (Arm#2)
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
LHC
SPS
AUGER
Cosmic ray spectrum
LHC gives us the unique opportunity to measure hadronic interactions at 1017eV
Tevatron
HOW LHCF CAN CONTRIBUTE?
Status of LHCf
High energy flux !! Low multiplicity !!
DPMJET3
η
∞
8.5
7TeV+7TeV → Elab = 1017eV 3.5TeV+3.5TeV → Elab = 2.6x1016eV450GeV+450GeV → Elab = 2x1014eV
Forward region is very effective on air shower development.
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
LHCF OPERATIONS @900 GEV & 7 TEV
With Stable Beam at 900 GeV Dec 6th – Dec 15th 2009With Stable Beam at 900 GeV May 2nd – May 27th 2010
With Stable Beam at 7 TeV March 30th - July 19th 2010
We took data with and without 100 μrad crossing angle for different vertical detector positions
Shower Gamma Hadron π0
Arm1 172,263,255 56,846,874 111,971,115 344,526
Arm2 160,587,306 52,993,810 104,381,748 676,157
Shower Gamma Hadron
Arm1 46,800 4,100 11,527
Arm2 66,700 6,158 26,094
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
INCLU
SIVE
PHOTON
SPECTR
UM A
NALYSIS
L HC
F DA
T A T
AK
I NG
PA P E R A C C E P T E D F O R P U B L I C AT I O N O N P L B
“ M E A S U R E M E N T O F Z E R O D E G R E E S I N G L E P H O T O N E N E R G Y S P E C T R A F O R √ S = 7 T E V P R O T O N - P R O T O N C O L L I S I O N S AT L H C “
A R X I V: 1 1 0 4 . 5 2 9 4
C E R N - P H - E P - 2 0 1 1 - 0 6 1
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
DATA SET FOR INCLUSIVE PHOTON SPECTRUM ANALYSIS• Data– Date : 15 May 2010 17:45-21:23 (Fill Number : 1104) except runs during the luminosity scan.
– Luminosity : (6.5-6.3)x1028cm-2s-1,– DAQ Live Time : 85.7% for Arm1, 67.0% for Arm2– Integrated Luminosity : 0.68 nb-1 for Arm1, 0.53nb-
1 for Arm2 – Number of triggers : 2,916,496 events for Arm1
3,072,691 events for Arm2 – Detectors in nominal positions and Normal Gain
• Monte Carlo– QGSJET II-03, DPMJET 3.04, SYBILL 2.1, EPOS 1.99 and PYTHIA8.145: about 107 pp inelastic collisions each
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
ANALYSIS FOR THE PHOTON SPECTRA
Analysis Procedure1. Energy Reconstruction from total energy deposition
in a tower (corrections for shower leakage, light yield etc.)
2. Particle Identification by analysis of the longitudinal shower development
3. Remove multi-particle events by looking at transverse energy deposit
4. Two Pseudo-rapidity regions selections, η>10.94 and 8.81<η<8.9
5. Combine spectra between the two detectors6. Compare data with the expectations from the
models
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
ANALYSIS 1. - ENERGY RECONSTRUCTION
Energy reconstruction : Ephoton = f(Σ(dEi)) (i=2,3,…,13)
( dEi = AQi determined at SPS. f() determined by MC. E : EM equivalent energy)
Impact position from lateral distribution
Position dependent corrections– Light collection non-uniformity– Shower leakage-out– Shower leakage-in (in case of two towers event)
Light collection nonuniformityShower leakage-out Shower leakage-in
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
ANALYSIS 1. - ENERGY RECONSTRUCTION
Energy scale can be checked by π0 identification from two tower events.
Mass shift observed both in Arm1 (+7.8%) and Arm2 (+3.7%)
No energy scaling applied, but shifts assigned in the systematic error in energy
m 140=
R
I.P.1
1(E1)
2(E2)
140mR
Arm2 Measurement
Arm2 MC
M = θ√(E1xE2)
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
•QGSJET2-gamma and -hadron are normalized to data(/collision) independently• LPM effects are switched on
Analysis 2. - Particle Identification
PID criteria based on transition curve
500 GeV <EREC<1 TeV
MC/Data comparison done in many energy bins
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
Double hit detection efficiency
ANALYSIS 3. -MULTI-HIT IDENTIFICATION
Reject events with multi-peaks Identify multi-peaks in one tower by position sensitive layers. Select only the single peak events for spectra.
Arm1
Arm2
Small tower Large tower
Single hit detection efficiency
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
ANALYSIS 4. - ACCEPTANCE CUT
R1 = 5mmR2-1 = 35mmR2-2 = 42mmq = 20o
For Small Tower h > 10.94 For Large Tower8.81 < h < 8.99
We define in each tower a region common both to Arm1 and Arm2, to compare the Arm1 and Arm2 reconstructed spectra.
Our final results will be two spectra, one for each acceptance region, obtained by properly weighting the Arm1 and Arm2 spectra
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
ANALYSIS 5. – COMPARISON OF ARM1 AND ARM2 SPECTRA
- Multi-hit rejection and PID correction applied- Energy scale systematic not considered due to strong correlation between Arm1 and Arm2
Deviation in small tower: still unclear, but within systematic errors
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
ANALYSIS 6. – COMBINATION OF ARM1 AND ARM2 SPECTRA
Gray hatch : Systematic Errors
Error bars : statistical Error
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
Beam-Gas backgrounds
BACKGROUNDS
1. Pileup of collisions in one beam crossing Low Luminosity fill, L=6x1028cm-2s-1
7% pileup at collisions, 0.2% at the detectors.
2. Collisions between secondary's and beam pipes Very low energy particles reach the detector (few % at
100GeV)
3. Collisions between beams and residual gasEstimated from data with non-crossing bunches. <0.1%
Secondary-beam pipe backgrounds
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
SYSTEMATIC UNCERTAINTIES
Uncorrelated uncertainties between ARM1 and ARM2- Energy scale (except p0 error)- Beam center position- PID- Multi-hit selection
Correlated uncertainty- Energy scale (p0 error)- Luminosity error
Estimated for Arm1 and Arm2 by same methods but independently
Estimated by Arm2, and apply it to the both Arm
Please have a look to the paper for detailed explanations!
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
RESULT
S
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
COMPARISON BETWEEN MODELSDPMJET 3.04 SIBYLL 2.1 EPOS 1.99 PYTHIA 8.145 QGSJET II-03
Gray hatch : Systematic Errors
Magenta hatch: MC Statistical errors
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
IMPA
CT ON H
ECR
PHYSICS
UN
DE
RS
TA
ND
I NG
TH
E I M
PA
CT
OF
OU
R M
EA
SU
RE
ME
NT
S
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
UNDERSTANDING THE IMPACT OF OUR MEASUREMENTS ON HECR
• The most tricky part
• We have started a cooperation with several theoreticians
• First meeting in Florence in mid of May• Authors of Corsika – EPOS
• Mini-workshop Catania July 6th-8th • P. Lipari, R. Ulrich, AUGER
• In touch also with Pythia experts • CERN Workshop to be organized together with M. Mangano
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
Π0 SPECTRUM AND AIR SHOWER
Artificial modification of meson spectra (in agreement with differences between models) and its effect to air shower
Importance of E/E0>0.1 mesons
π0 spectrum at Elab = 1019eV
QGSJET II originalArtificial modification
Longitudinal AS development
Ignoring X>0.1 meson
X=E/E0
30g/cm2
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
WHAT’
S NEX
T
DE
TE
CT
OR
UP
GR
AD
E,
AN
ALY
SI S
, I O
N R
UN
S
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
FUTURE ACTIVITIES (I)2011-2012 Replace plastic scintillators with Rad Hard GSO (prepared by Japan
side) in Florence Clean Rooms Produce 2 new silicon modules to replace partly defective ones + 2
spares Modify the silicon layers positions to improve silicon-only energy
resoution Test beam at SPS to calibrate Arm1&Arm2 Improve the dynamic range of silicon detectors (limited by Pace3
saturation effect)?
8 Silicon Layers 6 6 12 12 18 26 34 42 X0
EJ260
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
FUTURE ACTIVITIES (II)
2012Big interest in Ion runs (better if light ions)
LHC Ion run and/or RHIC Discussion on going with LHCC, LHC machine, ATLAS about reinstallation during Ion run (end of 2012?)
Discussion also about the possibility to install and take data at RHIC (geometrical feasibility good)
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
FUTURE ACTIVITIES (III)
• New analyses already started
• Priority list will be discussed during this week
• p0 measurement• Hadron spectra
• pT spectra
• h, k0, L ?• ….
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
NEXT TO FUTURE ACTIVITIES
2014-2015 Re-install Arm1&Arm2 at LHC when the energy will be raised to 13/14 TeV
Necessity to mantain the Cern infrastructures:Control roomElectronics pool materialSafety infrastructuresRacks in underground areasTeam accountEtc. etc. etc.
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
• LHCf Inclusive photon analysis has been completed• Many detailed systematic checks• First comparison of various hadronic interaction models with experimental data in
the most challenging phase space region (8.81 < h < 8.99, h > 10.94)• Large discrepancy especially in the high energy region with all models• Implications on UHECR Physics under study in strict connection with relevant
theoreticians and model developers
• Other analyses are in progress (hadrons, PT distributions, different
h coverage…)• LHCf was removed from the tunnel on July 20, 2010• We are upgrading the detectors to improve their radiation
hardness (GSO scintillators and rearrange silicon layers)• Discussions are under way to come back in the TAN for the
possible p-Pb run in 2012 (LHCC, Alice, LHC, Atlas etc.) or at RHIC for lower energy p-ions runs
• We will anyway come back in LHC for the 14 TeV run with upgraded detector!!!!
CONCLUSIONS
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
LHCf ringrazia particolarmente il Presidente uscente per l’affetto, l’incoraggiamento e il sostegno che ha sempre
mostrato al piu’ piccolo dei suoi esperimenti Che speriamo di aver ripagato con una piccola
soddisfazione
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
BACKUP SLI
DES
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
K.Fukatsu, T.Iso, Y.Itow, K.Kawade, T.Mase, K.Masuda, Y.Matsubara, G.Mitsuka, Y.Muraki, T.Sako, K.Suzuki, K.Taki Solar-Terrestrial Environment Laboratory, Nagoya University, JapanH.Menjo Kobayashi-Maskawa Institute, Nagoya University, Japan K.Yoshida Shibaura Institute of Technology, JapanK.Kasahara, Y.Shimizu, T.Suzuki, S.Torii Waseda University, JapanT.Tamura Kanagawa University, JapanO.Adriani, L.Bonechi, M.Bongi, R.D’Alessandro, M.Grandi, P.Papini, S.Ricciarini, G.Castellini INFN, Univ. di Firenze, Italy
K.Noda, A.Tricomi INFN, Univ. di Catania, Italy M.Haguenauer Ecole Polytechnique, France
W.C.Turner LBNL, Berkeley, USA
A-L.Perrot CERN, Switzerland
The LHCf collaboration
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
KEY MEASUREMENTS
E leading baryon
Elasticity / inelasticityForward spectra
(Multiplicity)Cross section
EM shower
E0
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
KEY PARAMETERS FOR THE DEVELOPMENT OF THE SHOWERS
Predictions of the hadronic interaction models most commonly used in the UHECR simulation
Big discrepancy in the high energy region !!!
Total cross section MultiplicityInelasticity/Secondary particles
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
MODEL UNCERTAINTY AT LHC ENERGY
Very similar!?
π0 energy at √s = 7TeV Forward concentration of x>0.1 π0
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
P0 RECONSTRUCTION
Reconstructed mass @ Arm2
measured energy spectrum @ Arm2
preliminary
An example of p0 events
• p0’s are the main source of electromagnetic secondaries in high energy collisions.
• The mass peak is very useful to confirm the detector performances and to estimate the systematic error of energy scale.
25mm 32mm
Silicon strip-X view
m 140=
R
I.P.1
1(E1)
2(E2)
140m
R
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
R&D FOR THE DETECTOR UPGRADE
Plastic scintillators (EJ260) ⇒ GSO scintillators
EJ260
Radiation damage measured by Ion beams
Scintillating Fibers ⇒ GSO bars
MIP peak
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
NEW SILICON LAYERS ARRANGEMENT
8 Silicon Layers 6 6 12 12 18 26 34 42 X0
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
FRONT COUNTER
Fixed scintillation counter
L=CxRFC ; conversion coefficient calibrated during VdM scans
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
CALORIMETERS VIEWED FROM IP
Geometrical acceptance of Arm1 and Arm2
Crossing angle operation enhances the acceptance
η
∞
8.7
θ[μrad]
0
310
η
∞
8.5
0 crossing angle 100urad crossing angle
Projected edge of beam pipe
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
LUMINOSITY ESTIMATION
Luminosity for the analysis is calculated from Front Counter rates:
The conversion factor CF is estimated from luminosity measured during Van der Meer scan
VDM scan
BCNWG paperhttps://lpc-afs.web.cern.ch/lpc-afs/tmp/note1_v4_lines.pdf
Beam sizes sx and sy measured directly by LHCf
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
ESTIMATION OF PILE UP
When the circulated bunch is 1x1, the probability of N collisions per Xing is
The ratio of the pile up event is
The maximum luminosity per bunch during runs used for the analysis is 2.3x1028cm-2s-1
So the probability of pile up is estimated to be 7.2% with σ of 71.5mbTaking into account the calorimeter acceptance (~0.03) only 0.2% of events have multi-hit due to pile-up. It does not affect our results
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
Effect of 1mm shift in the final spectrum
Beam center LHCf vs BPMSW
LHCf online hit-map monitor
BEAM CENTER MEASUREMENT
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
UNCERTAINTY IN STEP.2 Imperfection in L90% distribution
Template fitting A
Template fitting B
(Small tower, single & gamma-like)
Artificial modification in peak position (<0.7 r.l.) and width (<20%)
Original method
ε/P from two methods
(ε/P)B/ (ε/P)A
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
UNCERTAINTY IN STEP.3Fraction of multi-hit and Δεmulti, data-MC
Effect of multi-hit ‘cut’ : difference between Arm1 and Arm2
Single / (single+multi), Arm1 vs Arm2Effect of Δεmulti to single photon spectra
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
SPECTRAL DEFORMATION
Suppression due to multi-hit cut at medium energy Overestimate due to multi-hit detection inefficiency
at high energy (mis-identify multi photons as single)
No correction applied, but same bias included in MC to be compared
TRUEMEASURED
TR
UE/M
EA
SU
RED
True: photon energy spectrum at the entrance of calorimeter
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
SYSTEMATIC ERROR FROM ENERGY SCALE
Two components:- Relatively well known: Detector response, SPS => 3.5%- Unknown: p0 mass => 7.8%, 3.8% for Arm1 and Arm2.
Please note:
- 3.5% is symmetric around measured energy
- 7.8% (3.8%) are asymmetric, because of the p0
mass shift
- No ‘hand made’ correction is applied up to now for safety
Total uncertainty is -9.8% / +1.8% for Arm1 -6.6% / +2.2% for Arm2
Systematic Uncertainty on Spectra is estimated from difference between normal spectra and energy shifted spectra.
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
p0 MASS Arm1 Data
Peak at 145.8 ± 0.1 MeV
• Disagreement in the peak position• No ‘hand made correction’ is applied for safety• Main source of systematic error see later
Arm2 Data
Arm2 MC(QGSJET2)
Peak at 140.0 ± 0.1 MeV
Peak at 135.0 ± 0.2 MeV3.8 % shift
Many systematic checks have been done to understand the energy scale difference
7.8 % shift
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
p0 MASS VS p0 ENERGY
Arm2 DataNo strong energy dependence of reconstructed mass
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
h MASS Arm2 detector, all runs with zero crossing angleTrue h Mass: 547.9 MeVMC Reconstructed h Mass peak: 548.5 ± 1.0 MeVData Reconstructed h Mass peak: 562.2 ± 1.8 MeV (2.6% shift)
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
EFFECT OF MASS SHIFT
Energy rescaling NOT applied but included in energy error
Minv = θ √(E1 x E2)– (ΔE/E)calib = 3.5%–Δθ/θ = 1%– (ΔE/E)leak-in = 2%
=> ΔM/M = 4.2% ; not sufficient for Arm1 (+7.8%)
145.8MeV(Arm1 observed)
135MeV
±7.8% flat probability
±3.5% Gaussian probability
Quadratic sum of two errors is given as energy error(to allow both 135MeV and observed mass peak)
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
Π0 MASS SHIFT IN STUDY
Reanalysis of SPS calibration data in 2007 and 2010 (post LHC) <200GeV
Reevaluation of systematic errors
Reevaluation of EM shower using different MC codes (EPICS, FLUKA, GEANT4)
Cable attenuation recalibration(1-2% improve expected)
Re-check all 1-2% effects…
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
SUMMARY OF SYSTEMATIC ERRORS
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
14TEV: NOT ONLY HIGHEST ENERGY, BUT ENERGY DEPENDENCE…
7 TeV10 TeV14 TeV (1017eV@lab.)
SIBYLL
7 TeV10 TeV14 TeV
QGSJET2
Secondary gamma-ray spectra in p-p collisions at different collision energies (normalized to the maximum energy)
SIBYLL predicts perfect scaling while QGSJET2 predicts softening at higher energy
Qualitatively consistent with Xmax prediction
Note: LHCf detector taken
into account (biased)
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
LHC-COSMIC ?
p-Pb relevant to CR physics? CR-Air interaction is not p-p, but A1-A2 (A1:p,
He,…,Fe, A2:N,O)
LHC Nitrogen-Nitrogen collisionsTop: energy flow at 140m from IPLeft : photon energy spectra at 0 degree
TotalNeutronPhoton
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A L E S S I A T R I C O M I C N S 1 , N A P O L I , J U LY 5 , 2 0 1 1
COMPARISON OF EJ260 AND GSO-RADIATION HARDNESS-
• EJ260 (HIMAC* Carbon beam)10% decrease of light yield after exposure of 100Gy
• GSO (HIMAC Carbon beam)No decrease of light yield even after 7*10^5Gy exposure,BUT increase of light yield is confirmed
• The increase depend on irradiation rate (~2.5%/[100Gy/hour])*HIMAC : Heavy Ion Medical Accelerator in Chiba