Forward experiments at lhc how lhc can contribute to cosmic ray physics
Download
1 / 54

Forward Experiments at LHC: how LHC can contribute to Cosmic Ray Physics - PowerPoint PPT Presentation


  • 125 Views
  • Uploaded on

EDS’09: 13th International Conference on Elastic & Diffractive Scattering CERN, 29 June – 3 July 2009. Forward Experiments at LHC: how LHC can contribute to Cosmic Ray Physics. Alessia Tricomi University and INFN Catania. Physics Motivations Forward Experiments Physics performances.

loader
I am the owner, or an agent authorized to act on behalf of the owner, of the copyrighted work described.
capcha
Download Presentation

PowerPoint Slideshow about ' Forward Experiments at LHC: how LHC can contribute to Cosmic Ray Physics' - quilla


An Image/Link below is provided (as is) to download presentation

Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author.While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server.


- - - - - - - - - - - - - - - - - - - - - - - - - - E N D - - - - - - - - - - - - - - - - - - - - - - - - - -
Presentation Transcript
Forward experiments at lhc how lhc can contribute to cosmic ray physics

EDS’09: 13th International Conference on Elastic & Diffractive Scattering

CERN, 29 June – 3 July 2009

Forward Experiments at LHC:how LHC can contribute to Cosmic Ray Physics

Alessia Tricomi

University and INFN Catania

  • Physics Motivations

  • Forward Experiments

  • Physics performances


Ultra high energy cosmic rays
Ultra High Energy Cosmic Rays Diffractive Scattering

  • Experimental observations: at E>100 TeV only EAS

  • (shower of secondary particles)

  • lateral distribution

  • longitudinal distribution

  • particle type

  • arrival direction

Extensive Air Showers

Air shower development (particle interaction in the atmosphere)

  • Astrophysical parameters:

  • (primary particles)

  • spectrum

  • composition

  • source distribution

  • origin and propagation

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


The cosmic ray spectra
The Cosmic Ray Spectra Diffractive Scattering

GZK cutoff: 1020 eV

GZK cutoffwould limit energy to 1020eV (for protons, due to Cosmic Microwave Background

pg(2.7K)DNp

super GZK events?!?

Different results

between different

experiments

Based on data

presented at the 30th ICRC

Merida (Mexico)

Figure prepared by Y. Tokanatsu

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


The cosmic ray spectra1
The Cosmic Ray Spectra Diffractive Scattering

Difference in the energy scale between different experiments???

AGASA x 0.9

HiRes x 1.2

Yakutsk x 0.75

Auger x 1.2

Berezinsky 2007

AGASA Systematics

Total ±18%

Hadron interaction

(QGSJET, SIBYLL) ~10%

(Takeda et al., 2003)

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Hecr composition

PROTON Diffractive Scattering

IRON

Unger, ECRS 2008

HECR composition

Xmax(g/cm2)

The depth of the maximum of the shower Xmax in the atmosphere depends on energy and type of the primary particle.

Different hadronic interaction models give different answers about the composition of HECR.

IRON

LHC

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Hecr composition1
HECR composition Diffractive Scattering

Auger

Xmax measurements favors heavier composition as the energy increases

Anisotropy would favor proton primaries (AGN correlation)

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Modelling cosmic rays at lhc

Astrophysical parameters Diffractive Scattering

- source type

- source distribution

- source spectrum

- source composition

- propagation

Forward Physics

- cross section

- particle spectra

(E, PT, q, h, XF)

Nuclear Interaction

- calibration with data of Monte Carlo used in Cosmic Ray Physics

LHC

Modelling Cosmic Rays at LHC

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Development of atmospheric showers

Cosmic ray spectrum Diffractive Scattering

Tevatron

LHC

A 100 PeV fixed-target interaction with air has the cm energy of a pp collision at the LHC

AUGER

Development of atmospheric showers

Determination of E and mass of cosmic rays depends on description of primary UHE QCD (p+N,O Fe+N,O) interaction

Hadronic MC’s need tuning with data

The dominant contribution to the energy flux is in the very forward region ( 0)

In this forward region the highest energy available measurements of p0 cross section done by UA7 (E=1014 eV, y= 5÷7)

Use LHC (firstly proposed by LHCf)

√s = 14 TeV  Elab=1017 eV

to calibrate MCs

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Charged particles Diffractive Scattering

Neutral particles

Beam pipe

But…

General purpose detectors (ATLAS, CMS,…) cover only the central region

Special detectors to access forward particles are necessary

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


How to access very forward physics at lhc

Charged particles Diffractive Scattering

Neutral particles

Beam pipe

How to access Very Forward Physics at LHC?

Surrounding the beam pipe with detectors

Simple way, but still miss very very forward particles

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


How to access very forward physics at lhc1

Charged particles Diffractive Scattering

Beam pipe

Neutral particles

How to access Very Forward Physics at LHC?

Install detectors inside the beam pipe

Challenging but ideal for charged particle

(TOTEM)

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


How to access very forward physics at lhc2
How to access Very Forward Physics at LHC? Diffractive Scattering

Charged particles

LHCf

Neutral particles

Beam pipe

Y shape chamber enables us whole neutral measurements

Zero Degree Calorimeters

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Key measurements at lhc
Key Measurements at LHC Diffractive Scattering

E0

EM

shower

E leading hadron

Cross section

Elasticity / inelasticity

Forward spectra

TOTEM

ATLAS Fwd (ALFA)

Neutrals in ZDCs / LHCf: neutrons, mesons (p0,K0s g )

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Pseudo rapidity coverage at lhc
Pseudo rapidity coverage at LHC Diffractive Scattering

pseudorapidity: h = - ln (tanq/2)

Particle production at LHC over Dh≅±10

All phase space covered thanks to dedicated forward detectors!

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Lhc experiments
LHC experiments Diffractive Scattering

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Ip1 atlas forward detector
IP1: ATLAS forward detector Diffractive Scattering

LUCID (Cerenkov Tubes, 17m): Cerenkov hits over 5.4 < |η| < 6.1

ZDC (W/Q-fiber calo, 140m):

Neutral calorimetry over |η| > 8.3

ALPHA (Sci-Fi RPs):

Proton taggers at ± 240 m

FP220,FP420 (Si trackers, timing): Proton tracking at ±220, 420 m

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Ip1 lhcf detector
IP1: Diffractive ScatteringLHCf detector

UHECR-oriented experiment

(~30 Japan-European Collaborators)

Installed at ±140 m on both side of IP1 in TAN region

Double ARM detector:

ARM1: Sci/W + 4 XY Sci Fiber Layers

ARM2: Sci/W + 4 XY Si m-strip Layers

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Ip2 ip8 alice lhcb forward detectors
IP2-IP8: ALICE/ Diffractive ScatteringLHCb forward detectors

ZDCs also at ±7m, ±100 m

Good capabilities for heavy Q, QQ, gauge boson measurements

(low x-PDFs)

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Ip5 cms forward totem detectors
IP5: CMS Diffractive Scatteringforward+TOTEM detectors

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Ip5 cms forward totem detectors1
IP5: CMS Diffractive Scatteringforward+TOTEM detectors

TOTEM-T1,T2 (CSC/GEM telescopes):

Tracking over 3.1 < |η| < 4.7, 5.3 < |η| < 6.7

CASTOR (W/Q-fiber calo):

Calorimetry over 5.1 < |η| < 6.6

ZDC (W/Q-fiber calo):

Neutral calorimetry for |η| > 8.3

TOTEM (Si Roman Pots):

Proton taggers at ±147, ±220 m

FP420 (Si trackers, timing):

Proton tracking at ±420 m

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Totem p p total cross section
TOTEM: Diffractive Scatteringp-p total cross section

~ l n 2 s

Extrapolations vary by σ(LHC) = 90-130 mb

TOTEM goal: ≅1% precision

special run/optics: various β*, low lumi

(E710/811–CDF 2.6σ disagreement)

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Zdc zero degree calorimeters

ALICE, ATLAS & CMS ZDC (complemented by CASTOR) Diffractive Scattering

Total energy flow, wide aperture, high energy resolution for hadrons, (proton measurement only by ALICE ZDC)

enhance acceptance of central detectors for diffractive Physics

kinematics and production spectra of forward particles

Characterize Event:

Count spectator neutrons

Measure centrality (magnitude and

direction of impact parameter)

ZDC: Zero Degree Calorimeters

ppPhysics

ATLAS ZDC

ATLAS ZDC

HIPhysics

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Zero degree calorimeters lhcf

LHCf Diffractive Scattering: same h coverage as other ZDCs but fully dedicated experiment to HECR Physics

Double ARM calorimeters with imaging and PID capabilities

Excellent energy resolution(<5%) for g and p0, p0 mass resolution (< 5%) and Spatial resolution (40-200 mm)

Good neutron energy resolution (<30%)

Zero Degree Calorimeters: LHCf

Energy Resolution:

SPS electron data

Very important tool

to calibrate energy scale

Spatial Resolution:

SPS-200 GeV electrons

Dm/m < 4%

Spatial Resolution:

SPS-200 GeV electrons

1.04 107 events

≅20 min @L=1029cm-2s-1

Number of event

σx=40 mm

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009

x-pos[mm]


Lhcf monte carlo discrimination
LHCf : Monte Carlo discrimination Diffractive Scattering

106 generated LHC interactions 

1 Minute [email protected] cm-2s-1 luminosity

Discrimination between various models

is feasible

Quantitative discrimination with the help of a properly defined c2 discriminating variable based on the spectrum shape

(see TDR for details)

5% Energy resolution

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Lhcf model dependence of neutron energy distribution
LHCf: model dependence of Diffractive Scatteringneutron energy distribution

Original n energy

30% energy resolution

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


New models
New Models Diffractive Scattering

29

Proton

PICCOEPOS

Drescher, Physical Review D77,

056003 (2008)

p0

Neutron

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Mc model tuning pp @ s 14 tev
MC model tuning: pp @ √ Diffractive Scatterings=14 TeV

Dominated by Soft QCD: underlying events, multiparton interactions, fragmentations

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Mc model tuning p a @ s 8 8 tev
MC Model tuning: Diffractive Scatteringp+A @ √s= 8.8 TeV

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Mc model tuning a a @ s 5 5 tev
MC Model tuning: A+A @ √ Diffractive Scatterings=5.5 TeV

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Conclusions and plans
Conclusions and plans Diffractive Scattering

Compilation of EAS data is affected by the uncertanties of hadron interaction models.

LHC fwd experiments will provide crucial data of hadron interaction for CR study covering the whole phase space

Several detectors already installed

LHCf ready for data taking already during LHC commissioning

We need only to wait LHC restart!

Hoping to answer all our questions and to help EAS experiments to interpret their data

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Aknowledgement
Aknowledgement Diffractive Scattering

Thanks to ALICE, ATLAS, CMS, LHCb, LHCf, TOTEM Collaborations for useful material

In particular, I wish to thank

O. Adriani, K. Eggert, D. D’Enterria, P. Grafstrom, M. Grothe, S. White

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Back up slides
Back-up slides Diffractive Scattering

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Cosmic ray composition
Cosmic Ray Composition Diffractive Scattering

Kascade Results

QGSJET01

SIBYLL 2.1

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Cms castor zdc calorimeters
CMS CASTOR & ZDC calorimeters Diffractive Scattering

  • extends calorimetric coverage of CMS to 5.2 < η < 6.6

  • signal collection through Čerenkov photons transmitted to PMTs through aircore lightguides

  • W absorber & quartz plates sandwich,

  • electromagnetic and hadronic sections

  • 16 seg. in φ, 14 seg in z, none in η

  • 140 m from interaction point in TAN absorber

  • Tungsten/quartz Čerenkov calorimeter with separate e.m. and had. Sections

  • Acceptance for neutrals (γ, π0, n) from η > 8.1, 100% for η > 8.4

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Totem t1 t2 tracking detectors

3m Diffractive Scattering

Test Beam

TOTEM T1 & T2 tracking detectors

  • Gas Electron Multiplier (GEM)

  • Mounted in front of CASTOR

  • 5.3 < | < 6.5

  • 10 planes formed by 20 GEM

    semi-circular modules

  • Radial position from strips, h, from pads

  • Resolution strip~70mm

  • Cathode Strip Chambers (CSC)

  • Mounted in front of HadronForward

    calorimeter of CMS

  • 3.1 < | < 4.7

  • 5 planes with 3 coordinates/plane

  • 6 trapezoidal CSC detectors/plane

  • Resolution  ~ 0.8mm

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Detector 1
Detector #1 Diffractive Scattering

Impact point (h)

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

4 pairs of scintillating fiber layers for tracking purpose (6, 10, 32, 38 r.l.)

Absorber

22 tungsten layers 7mm – 14 mm thick

(W: X0 = 3.5mm, RM = 9mm)

16 scintillator layers (3 mm thick)

Trigger and energy profile measurements

Energy

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Detector 2
Detector # 2 Diffractive Scattering

Impact point(h)

2 towers 24 cm long stacked on their edges and offset from one another

Lower: 2.5 cm x 2.5 cm

Upper: 3.2 cm x 3.2 cm

4 pairs of silicon microstrip layers

(6, 12, 30, 42 r.l.) for tracking purpose (X and Y directions)

16 scintillator layers (3 mm thick)

Trigger and energy profile measurements

Absorber

22 tungsten layers 7mm – 14 mm thick (2-4 r.l.)

(W: X0 = 3.5mm, RM = 9mm)

Energy

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Lhcf acceptance on p t g e g plane
LHCf: acceptance on P Diffractive ScatteringTg-Eg plane

140

Beam crossing

angle

Detectable events

A vertical beam crossing angle > 0

increases the acceptance of LHCf

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Arm2 position resolution
ARM2 Position Resolution Diffractive Scattering

200 GeV electrons

Number of event

σx=40 mm

x-pos[mm]

Number of event

σy=64 mm

y-pos[mm]

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Arm1 position resolution
ARM1 Position resolution Diffractive Scattering

200 GeV electrons

Number of event

σx[mm]

σx=172 mm

x-pos[mm]

E[GeV]

σy[mm]

σy=159 mm

Number of event

y-pos[mm]

E[GeV]

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Arm2 silicon energy resolution
ARM2-Silicon Energy Resolution Diffractive Scattering

200 GeV electrons

SPS beam test data

No correction/calibration applied

DE/E ~ 12%

ADC

Only silicon energy resolution ~ 10%!!!!!

We can use it as a check for the radiation damage of the scintillators

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Energy resolution

Monte Carlo Diffractive Scattering

Energy Resolution

N Particles

MC predicts that the

leakage is energy independent!

Distance from Edge

SPS beam test

Energy distribution is corrected for leakage

correction

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


G ray energy spectrum for different positions
g Diffractive Scattering ray energy spectrum for different positions

QGSJETII: used model

QGSJET: c2/DOF=107/125

DPMJET3: c2/DOF=224/125

SYBILL: c2/DOF=816/125

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


P 0 spectra
p Diffractive Scattering0 spectra

p0 produced at collision can be extracted by using gamma pair events

Powerful tool to calibrate the energy scale and also to eliminate beam-gas BG

QGSJETII

⇔ DPMJET3χ2= 106 (C.L. <10-6)

⇔ SIBYLL χ2= 83 (C.L. <10-6)

DPMJET3

⇔ SIBYLL χ2= 28 (C.L.= 0.024)

107events DOF = 17-2=15

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


P 0 reconstruction
p CERN 29 Jun - 3 July 20090 reconstruction

g

350 GeV Proton beam

Not in scale!

g

Carbon target (6 cm)

in the slot used for beam monitor

9.15 m

Arm1

>107 proton on target (special setting from the SPS people)

Dedicated trigger on both towers of the calorimeter has been used

Ex:

Dm ~ 8 MeV

Dm/m ~ 6%

Sim:

Dm/m ~ 5%

 250 p0 events triggered (in a quite huge background) and on disk

Preliminary!!!!

Main problems:

  • low photon energy (≥20 GeV)

  • Direct protons in the towers

  • Multi hits in the same tower

(MeV)

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


P 0 rate
p CERN 29 Jun - 3 July 20090 rate

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


The lpm effect

○ w/o LPM CERN 29 Jun - 3 July 2009

■ w/ LPM

The LPM effect

Transition curve of a1 TeV photon w/ and w/o LPM to be measured by LHCf

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


G rate
g CERN 29 Jun - 3 July 2009 rate

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Estimate of the background

beam-beam pipe CERN 29 Jun - 3 July 2009

 E γ(signal) > 200 GeV, OK

background < 1%

beam-gas

 It depends on the beam condition

background < 1% (under 10-10 Torr)

beam halo-beam pipe

 It has been newly estimated from the beam loss rate

background < 10% (conservative value)

Estimate of the background

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Analysis of beam gas events
‘Analysis’ of Beam Gas events CERN 29 Jun - 3 July 2009

We got 116 FC triggers in 8.275.034 BPTX: Nt=116

2.109 protons/bunch

Total # of protons: Np=1.7 x 1016

We try to estimate the gas density r from this rate:

Nt=Np* L * s * r

L=effective lenght ~ 100 m

s=Cross section ~ 80 mbarn = 80 x 10-31 m2

We find: r = 8.5 x 1012 H/m3 = 4.2 x 1012 H2/m3

From the LHC Project Report #783: r = 1012 H2/m3

From the pressure measurement in April 2008: r~ 1012 H2/m3

~ CONSISTENT!!!!!!!!!!!!!

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Low x physycs and uhecr
Low- CERN 29 Jun - 3 July 2009xPhysycs and UHECR

Reduced dN/dη :

Less penetration:

lower X (~ -30 g/cm2)

Reduced charm cross sections: Less muons !

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


Forward qq in alice
Forward QQ in ALICE CERN 29 Jun - 3 July 2009

D. D’Enterria (Trieste May 09)

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


G z w in lhcb 2 h 5
g CERN 29 Jun - 3 July 2009*, Z, W in LHCb (2<h<5

D. D’Enterria (Trieste May 09)

Forward Experiments at LHC EDS'09, CERN 29 Jun - 3 July 2009


ad