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Air shower experiments 2 Astrophysical parameters - source type - source distribution - source spectrum - source composition - propagation Image from “The Daily Galaxy” Air shower development - interaction - atmosphere Observations - lateral distribution - longitudinal distribution - particle type - arrival direction
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LHCf Measurements of Very Forward Particles at LHC
Takashi SAKO (Solar-Terrestrial Environment Laboratory, Nagoya
University, Japan) For the LHCf Collaboration XVI International
Symposium on Very High Energy Interactions, 28 Jun-3 Jul 2010,
Fermilab Air shower experiments
2 Astrophysical parameters - source type - source distribution -
source spectrum - source composition - propagation Image from The
Daily Galaxy Air shower development - interaction - atmosphere
Observations - lateral distribution - longitudinal distribution -
particle type - arrival direction Uncertainty in Hadron
Interaction
Auger, PRL (2010) Experimental data at highest energy hadron
collider is indispensible => LHC The arge adron ollider
Collider of 7TeV proton + 7TeV proton labo. System Heavy ion
collisions ATLAS / LHCf LHCb CMS / TOTEM ALICE What to be measured
at colliders multiplicity at LHC 14TeV collisions pseudo-rapidity;
= -ln(tan(/2)) Multiplicity All particles neutral Most of the
collision products are emitted in the central region What to be
measured at colliders multiplicity and energy flux at LHC 14TeV
collisions pseudo-rapidity; = -ln(tan(/2)) Multiplicity Energy Flux
All particles neutral Most of the energy flows into very forward
LHCf Experiment To measure very forward (>8.4; including 0
degree) neutral particles at LHC p-p (ion-ion) collisions
International collaboration of Japan-Europe-USA (36 members) ATLAS
/ LHCf LHCb CMS / TOTEM ALICE LHCf LHCf The LHCf experiment
K.Fukatsu, Y.Itow, K.Kawade, T.Mase, K.Masuda, Y.Matsubara,
G.Mitsuka, K.Noda, T.Sako, K.Suzuki, K.Taki Solar-Terrestrial
Environment Laboratory, Nagoya University, Japan K.Yoshida Shibaura
Institute of Technology, Japan K.Kasahara, M.Nakai, Y.Shimizu,
T.Suzuki, S.Torii Waseda University, Japan T.Tamura Kanagawa
University, Japan Y.Muraki Konan University M.Haguenauer Ecole
Polytechnique, France W.C.Turner LBNL, Berkeley, USA O.Adriani,
L.Bonechi, M.Bongi, R.DAlessandro, M.Grandi, H.Menjo, P.Papini,
S.Ricciarini, G.Castellini INFN, Univ. di Firenze, Italy G.Sinatra,
A.Tricomi INFN, Univ. di Catania, Italy J.Velasco, A.Faus IFIC,
Centro Mixto CSIC-UVEG, Spain D.Macina, A-L.Perrot CERN,
Switzerland Detector Location ATLAS 96mm LHCf Detector(Arm#1)
Two independent detectors at either side of IP1( Arm#1, Arm#2 )
96mm 140m 96mm LHC IP TAN Detector TAN -Neutral Particle Absorber-
transition from one common beam pipe to two pipes Slot : 100mm(w) x
607mm(H) x 1000mm(T) ATLAS & LHCf LHCf Detectors Imaging
sampling shower calorimeters
Two independent calorimeters in each detector (Tangsten 44r.l.,
1.7, sample with plastic scintillators) Arm#1 Detector
20mmx20mm+40mmx40mm 4 XY SciFi+MAPMT Arm#2 Detector
25mmx25mm+32mmx32mm 4 XY Silicon strip detectors Double Arm
Detectors Arm#1 Detector Arm#2 Detector 290mm 90mm Transverse
projection of Arm#1
IP1,ATLAS Arm2 8.7 Shadow of beam pipes between IP and TAN 8.4 This
is photos of our detectors installed in the LHC ring. The red one
is the surface of TAN located 140m far from IP1.we can see our
electronics boxes on TAN but detector were completely in
experimental slots of TAN. Behind of our detectors, Luminosity
monitor BRAN and ATLAS ZDC has been installed. @ 140mrad crossing
angle neutral beam axis Transverse projection of Arm#1 @ zero
crossing angle Expected Results at 14 TeV collisions (assuming
0.1nb-1 statistics)
Detector response not considered Original Plan 34 32 Log(Luminosity
[cm-2s-1]) 30 28 26
Beam energy (TeV) Log(Luminosity [cm-2s-1]) LHCf ideal LHCf removal
LHC nominal Real Life Original target >=2013 May-2010 Mar-2010
Dec-2009
34 32 30 28 26 Original target LHCf Removal End of June-2010
Log(Luminosity [cm-2s-1]) LHCf Ideal >=2013 May-2010 Mar-2010
Dec-2009 Beam energy (TeV) Results at LHC 2009 Operation at 900GeV
Collisions
With stable beams at 900GeV, 06.Dec. 15.Dec 2.6 hours for
commissioning 27.7 hours for physics ~2,800 shower events in Arm1
~3,700 shower events in Arm2 ~5x105 collisionsat IP1 Expected
spectra with each hadron interaction model Gamma-ray Arm2 Hadron
Arm2 with 107 col. First Events at 900GeV collisions
Longitudinal development Lateral (X) Distribution Lateral (Y) Arm1
(SciFi) First Events at 900GeV collisions
Arm2 (Silicon) Longitudinal development Lateral (X) Distribution
Lateral (Y) Distribution Energy scale is calibrated at SPS below
200GeV Particle Identification
A transition curve for Gamma-ray A transition curve for Hadron
Thick for E.M. interaction (44X0) Thin for hadronic
interaction(1.7l) 20mm cal. of Arm1 Definition of L90% MC (QGSJET2)
Data Preliminary Criteria for gamma-rays 16 r.l x SdE Gamma-ray
like Both detectors give same spectra
Comparison between calorimeter towers of Arm2 Gamma-ray like Hadron
like Blue: including 0 degree Red: off axis No angular dependence
Comparison between two Arms Blue:Arm2 Red:Arm1 Preliminary
Preliminary Both detectors give same spectra Spectra Comparison
with MC (QGSJET2) prediction
Conservative systematic error is assigned x15 statistics was
obtained in the 2010 operation 7 TeV (3.5TeV+3.5TeV)
Operation
First collision on 31-March 2010 Already accumulatedabout 14 nb-1
Have you ever seen TeV showers? (except CRs)
Gamma pair from TeV pi0 TeV gamma Pi-zero (10% of full data)
Arm1 Arm2 Energy spectra from first 1% data
Hit map Very low BKG Angular dependence isseen Stronger 0 degree
concentration in hadron candidates Whats next Operation
Analysis
LHC started crossing angle run last week LHCf can enlarge the PT
coverage Due to radiation damage LHCf removes the detectors in this
summer Detector will be upgrated to rad-hard by 14TeV collisions
(2013 earliest) Analysis 15 times more statistics in 900GeV data
>100 time statistics in 7TeV data Systematics study rather than
statistics Conversion to production spectra (cross section)
Comparison with MC Not only highest energy, but energy
dependence
7 TeV 10 TeV 14 TeV QGSJET2 7 TeV 10 TeV 14 SIBYLL Note: LHCf
detector taken into account (biased) 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 Summary LHCf is a dedicated experiment to measure
very forward neutral particles at LHC LHCf successfully started
(and almost finished) data taking at 900GeV and 7TeV collisions We
have sufficient statistics and started careful study in systematics
to test hadron interaction models We will remove the detectors soon
and come back at 14TeV collisions with upgraded detectors Backup
Light Nuclei collisions (Note: Not planned in LHC!!)
Energy flux in Nitrogen collisions Still strong concentration in
the forward region Expected spectra in N-N collisions
Assuming to measure at the LHCf installation location Gamma spectra
at