Interaction Length A. Murakami. L = 38.83 (interaction length of proton in carbon by PDG) change of constant : means uncertainty of L (change 0.8, 0.9,

Slides:



Advertisements
Similar presentations
Beam direction and flux measured by MUMON K. Matsuoka (Kyoto) for the MUMON group Contents: 1.Beam stability (direction/flux) 2.Absolute  beam flux.
Advertisements

HARP Anselmo Cervera Villanueva University of Geneva (Switzerland) K2K Neutrino CH Meeting Neuchâtel, June 21-22, 2004.
T2K neutrino experiment at JPARC Approved since 2003, first beam in April Priorities : 1. search for, and measurement of,   e appearance  sin.
Pion yield studies for proton drive beams of 2-8 GeV kinetic energy for stopped muon and low-energy muon decay experiments Sergei Striganov Fermilab Workshop.
Surplus Hits Ratio Leon R. C&A Meeting Oct. 31, 2001.
1 Vertex fitting Zeus student seminar May 9, 2003 Erik Maddox NIKHEF/UvA.
Calorimetry Study Update Jaewon Park University of Rochester MINERvA/Jupiter Group Meeting, Mar 22, 2006.
IDS-NF Target Studies H. Kirk (BNL) July 8, 2009.
2015/6/23 1 How to Extrapolate a Neutrino Spectrum to a Far Detector Alfons Weber (Oxford/RAL) NF International Scoping Study, RAL 27 th April 2006.
Neutrino Study Group Dec 21, 2001 Brookhaven Neutrino Super-BeamStephen Kahn Page 1 Horn and Solenoid Capture Systems for a BNL Neutrino Superbeam Steve.
SMRD April 2007 Status of the atmospheric muon studies Piotr Mijakowski OUTLINE: Primary muon spectrum at the sea level Primary muon.
Status of the Beamline Simulation A.Somov Jefferson Lab Collaboration Meeting, May 11, 2010.
Recent results from the K2K experiment Yoshinari Hayato (KEK/IPNS) for the K2K collaboration Introduction Summary of the results in 2001 Overview of the.
Status of the NO ν A Near Detector Prototype Timothy Kutnink Iowa State University For the NOvA Collaboration.
The Earth Matter Effect in the T2KK Experiment Ken-ichi Senda Grad. Univ. for Adv. Studies.
Status of Phase II Energy Loss Studies 1. FLUKA with “simple” CERN-provided input file modeling ~40m around primary collimators used for all SLAC studies.
Inter-comparison of Medium-Energy Neutron Attenuation in Iron and Concrete (8) H. Hirayama and Attenuation Length Sub-Working Group in Japan.
Simulations on “Energy plus Transmutation” setup, 1.5 GeV Mitja Majerle
Particle Production at 3 GeV (update) X. Ding, UCLA Target Studies Sept. 23, /23/13.
Beam MC activity A.K.Ichikawa for beam group For more details,
Mass production (Super-K) Setup of jnubeam – 3 horn 250 kA – 30-GeV proton beam of Gaussian distribution (  x,y = cm) – On center, parallel beam.
UC Davis June st Rosi Reed Low Energy Test Run Results Rosi Reed University of California at Davis.
Žarko Pavlović, 2 Patricia Vahle, 1 Sacha Kopp, 2 1 University College, London 2 University of Texas at Austin Flux Uncertainties for the NuMI Beam.
E.C. AschenauerFebruary Inclusive Structure functions in eA or why momentum resolutions are important E.C. Aschenauer February How to extract.
10 mm depth 16 mm depth BEFORE AFTER. TiTi alloyDiff. % 2 mm10 mm16 mm2 mm10 mm16 mm Adriana GEANT ~7% Luis FLUKA ~10.
Beam MC progresses for beam MC sub-group. Summary of update in 09b,c,10a 09b Geometry of baffle, target, 1st horn, dump and MUMON is updated. 09c MUMON.
HARP measurements of pion yield for neutrino experiments Issei Kato (Kyoto University) for the HARP collaboration Contents: 1.HARP experiment Physics motivations.
1 Question to the 50GeV group 3GeV からの 54π と 81π 、 6.1π の関係 fast extraction 部の acceptance (81π?) Comments on neutrino beamline optics?
Inclusive Measurements of inelastic electron/positron scattering on unpolarized H and D targets at Lara De Nardo for the HERMES COLLABORATION.
Meson Production of Carbon Target at 3 GeV X. Ding, UCLA Target Studies 17/18/13.
Carbon Target Design and Optimization for an Intense Muon Source X. Ding, UCLA H.G. Kirk, BNL K.T. McDonald, Princeton Univ MAP Winter Collaboration.
Fiber target simulation for S-2S experiment Toshiyuki Gogami 2015/10/15.
Proposal for the study to define what is really necessary and what is not when the data from beam, ND and SK are combined A.K.Ichikawa 2008/1/17.
Update on ILC Production and Capturing Studies Wei Gai, Wanming Liu and Kwang-Je Kim ILC e+ Collaboration Meeting IHEP Beijing Jan 31 – Feb 2, 2007.
Kaons in the SPL Superbeam Antoine Cazes Laboratoire de L’accélérateur Linéaire.
April 26, McGrew 1 Goals of the Near Detector Complex at T2K Clark McGrew Stony Brook University Road Map The Requirements The Technique.
IDS120j WITH AND WITHOUT RESISTIVE MAGNETS PION AND MUON STUDIES WITHIN TAPER REGION, III ( 20 cm GAPS BETWEEN CRYOSTATS ) Nicholas Souchlas, PBL (9/4/2012)
Comparison HARP data with GEANT4 and MARS Simulations NUFACT06, UC Irvine 28 August 2006 Stephen Brooks 1, Paul Soler 2, Kenny Walaron 2 1 Rutherford Appleton.
1 A study to clarify important systematic errors A.K.Ichikawa, Kyoto univ. We have just started not to be in a time blind with construction works. Activity.
Marina Golubeva, Alexander Ivashkin Institute for Nuclear Research RAS, Moscow AGeV simulations with Geant4 and Shield Geant4 with Dpmjet-2.5 interface.
A complete simulation of cosmic rays access to a Space Station Davide Grandi INFN Milano, ITALY.
Meson Production at Low Proton Beam Energy (Update) X. Ding, UCLA Target Studies May 9, /9/113.
RFA Simulations Joe Calvey LEPP, Cornell University 6/25/09.
Recent Results from NA61 (Flux Related Systematic Uncertainties) and Recent Results from T2K (Overall Systematic Uncertainties) NNN15 Stony Brook Oct.
Alex Howard PH-SFT LCG-PV 10 th May 2006 Neutron Benchmark for Geant4 using TARC – initial status 1)TARC – experimental set-up and aims 2)Geant4 Simulation.
Horns, Hadron production etc. (from hadron production to neutrino beam) A.K.Ichikawa KEK 200/9/26 Study on horns Changing -beam energy Hadron.
BNL neutrino beam. Optimization and simulations Milind Diwan June 10.
G.R.White: F.O.N. T. From Ground Motion studies by A.Seryi et al. (SLAC) ‘Fast’ motion (> few Hz) dominated by cultural noise Concern for structures.
Beam direction and flux measured by MUMON K. Matsuoka (Kyoto) for the MUMON group Contents: 1.Horn focusing effect 2.Beam stability (direction/flux) 3.Beam.
Claudia Strabel, ETH Zurich SPS Annual Meeting June 21 – 22, 2010 Hadro-production measurements for T2K with NA61/SHINE at the CERN SPS.
Extrapolation Techniques  Four different techniques have been used to extrapolate near detector data to the far detector to predict the neutrino energy.
NEAR DETECTOR SPECTRA AND FAR NEAR RATIOS Amit Bashyal August 4, 2015 University of Texas at Arlington 1.
MARS15 Studies of Impact of LBNF Target/Horn Optimization on the Hadron Absorber 6 th High Power Targetry Workshop Merton College, Oxford April 12, 2016.
N_TOF EAR-1 Simulations The “γ-flash” A. Tsinganis (CERN/NTUA), C. Guerrero (CERN), V. Vlachoudis (CERN) n_TOF Annual Collaboration Meeting Lisbon, December.
Observation Gamma rays from neutral current quasi-elastic in the T2K experiment Huang Kunxian for half of T2K collaboration Mar. 24, Univ.
 CC QE results from the NOvA prototype detector Jarek Nowak and Minerba Betancourt.
Mark Dorman UCL/RAL MINOS WITW June 05 An Update on Using QE Events to Estimate the Neutrino Flux and Some Preliminary Data/MC Comparisons for a QE Enriched.
Precision Measurement of Muon Neutrino Disappearance with T2K Alex Himmel Duke University for the The T2K Collaboration 37 th International Conference.
DESY BT analysis - updates - S. Uozumi Dec-12 th 2011 ScECAL meeting.
1 Temp Otani Murakami 2010/8/17 1.Monte Carlo simulation 2.Summary of 10a beam DATA 3.Comparison DATA and MC 4.Syst. error study.
R.W. Assmann, V. Boccone, F. Cerutti, M. Huhtinen, A. Mereghetti
The MiniBooNE Little Muon Counter Detector
Preliminary T2K beam simulation using the G4 2km detector
Inter-comparison of Particle production (2)
MUMON / emulsion total flux uncertainty
EM Linearity using calibration constants from Geant4
Targeting Monitor in K2K
Geant4 in HARP V.Ivanchenko For the HARP Collaboration
NKS2 Meeting with Bydzovsky NKS2 Experiment / Analysis Status
Antoine Cazes Université Claude Bernard Lyon-I December 16th, 2008
Presentation transcript:

Interaction Length A. Murakami

L = (interaction length of proton in carbon by PDG) change of constant : means uncertainty of L (change 0.8, 0.9, 1.0, 1.1, 1.2) Flux is normalized at peak flux.

Normalized There seems to be no difference... Flux × 30 for looking at the tail Flux × 15 for looking at the tail

Ratio of Normalized zoom to 0~2 GeV Diff. less than 3% Diff. less than 5% constant = 1.1, 1.2 vs 1.0

Ratio of Normalized zoom around 0~2 GeV Diff. less than 3% Diff. more than 5% constant = 0.9, 0.8 vs 1.0

Ratio of Normalized zoom around 0~2 GeV constant = 1.2, 1.1 vs 1.0 Diff. less than 2% Diff. less than 3%

Ratio of Normalized zoom around 0~2 GeV constant = 0.9, 0.8 vs 1.0 Diff. less than 2% Diff. less than 5%

Far / Near constant=1.0, 1.1, 1.2 zoom around 0~2 GeV There seems to be no difference...

Far / Near constant=1.0, 0.9, 0.8 zoom around 0~2 GeV There seems to be no difference...

Comparison of Far/Near constant=1.0, 1.1, 1.2 zoom around 0~2 GeV Diff less than 2% Diff less than 3%

Comparison of Far/Near constant=1.0, 0.9, 0.8 zoom around 0~2 GeV Diff less than 2% Diff less than 4%

Out-target/In-target comparison A.Murakami Confirmation of Nicolas’s study

Zoom

Diff between “out” and “total”< 6%

Primary beam profile A. Murakami

Black : nominal beam profile Blue : Flat beam Red : pencil beam Y-Scale × 40

20 ZOOM

21 ZOOM

22 ZOOM

23 ZOOM

Z binning study binning target exit z position A. Murakami 24

25 Simple simulation by either geant3, mars, fluka, geant4 …… Target is just a 90cm, 2.6cm-diameter rod. Vector information of particles just exit the target is output. Normal use for model comparison 30GeV proton In jnubeam Generate and trace the track inputted. Vector information Simple simulation by geant3 Target is just a 90cm, 2.6cm-diameter rod. Vector information of particles just exit the target is output. But ‘z’ value is modified to simulate the binning condition. This study 30GeV proton In jnubeam Generate and trace the track input. Vector information ‘one bin’ case

27

28

29 ZOOM

30 ZOOM

Secondary interaction in Horn Aluminum A. Murakami 31

32 Super-KND off-axis Red: remove horn aluminum Black : nominal

33

34

35

36

ASSUMED condition (ad hoc) Abs. flux Flux shape Far/ Near Trans. Matrix remakes primaryGfluka v.s. gheisha 35%<10% Sakashita primaryGfluka v.s. K2K- SW 30%10% Sakashita Prod. Point (Z)  z=18cm (  =18/sqrt(12)) 4%3% Murakami Interaction length20%7%4% Murakami Second. Had.prod.Gfluka v.s. gclaor 15%<3% Sakashita Sec. intr. in horn Al20% uncertainty 6% 2% Murakami 30% absorption Out target inter.20% uncertainty 5% 2% Nicolas/Murakami 10~30% out of total Indirect contr. Nicolas Upper number: 0.4<E <1.2GeV region Lower number : E <10GeV Primary interaction Secondary Interaction

Upper number: 0.4<E <1.2GeV region Lower number : E <10GeV Cont’d ASSUMED condition (ad hoc) Abs. flux Flux shape Far/ Near Trans. Matrix remakes Pbeam profileNo profile info.10% 12% 5% Murakami Pbeam position shift Josh Pbeam angle shift Horn alignment Josh Horn current Josh Horn field asym.10%8% Eric Primary Beam Horn