Cosmic Ray Muon Detection Department of Physics and Space Sciences Florida Institute of Technology Georgia Karagiorgi Julie Slanker Advisor: Dr. M. Hohlmann.

Slides:



Advertisements
Similar presentations
Trigger issues for KM3NeT the large scale underwater neutrino telescope the project objectives design aspects from the KM3NeT TDR trigger issues outlook.
Advertisements

Double Chooz: Outer Veto
COSMIC RAY MUON DETECTION USING SCINTILLATION COUNTER AND WAVELENGTH SHIFTING FIBERS ARUNODAYA BHATTACHARYA VSRP-2009,TIFR,MUMBAI 6/7/09.
正および負電荷の ミューオンの物質中での寿命 July 1 st, 2014 Suguru Tamamushi List of Contents 1.Purpose 2.Decay of Positive and Negative Muons 3.Experimental Procedure and.
Shantanu Menon Thomas Irons Michael Jacoutot. Cosmic Rays  High energy particles (mainly protons) from outer space.  Have up to 10 million times more.
Experimental Method Experimental Method Kihyeon Cho Kyungpook National University Spring Semester 2005 Experimental Method and Data Process.
A Muon Veto for the Ultra-Cold Neutron Asymmetry Experiment Vince Bagnulo LANL Symposium 2006 Outline ● UCNA Experiment ● Muon background ● Proposed Veto.
A Muon Veto for the Ultra Cold Neutron Asymmetry Experiment Vince Bagnulo with Dr. Jeff Martin Electrons Ultra Cold Neutrons Cosmic Ray Muons Protons Pions.
Quark Net 2010 Wayne State University Physics Department.
Design and First Results of a Cosmic Ray Telescope For Use In Testing a Focusing DIRC M. P. Belhorn University of Cincinnati The BELLE group at the University.
Xinjun Guo Dec. 16, Cosmic Rays  Primary: protons( ), light nuclei  Secondary:,, others  Decay product:,,
Cosmic Rays Basic particle discovery. Cosmic Rays at Earth – Primaries (protons, nuclei) – Secondaries (pions) – Decay products (muons, photons, electrons)
CRAnE: A JAS-based Data Acquisition System for Cosmic Rays Jennifer Docktor & Manuel Reyes Mentors Tom Glanzman & Willy Langeveld August 13, 2003 Department.
Muon Decay Experiment John Klumpp And Ainsley Niemkiewicz.
How We Became Experimentalists Suzanne Levine Saba Zuberi Len Zheleznyak REU 2002.
SCIPP Summer Outreach Project July Cosmic Ray Detectors Cosmic Ray Detectors Detector Testing Detector Testing Muon Lifetime Experiment Muon Lifetime.
Timing Properties of T0 Detectors At PHOBOS Saba Zuberi, Erik Johnson, Nazim Khan, Frank Wolfs, Wojtek Skulski University of Rochester.
Using muon physics to teach relativity, radiation, and instrumentation Daniel W. Koon 1 and Jeremy Ouellette Department of Physics St. Lawrence University.
SPHERE PEG GAY FAIRBURY JR SR HIGH SCHOOL. PROJECT SPHERE  Cherenkov light: radiation which is emitted whenever charged particles pass through matter.
Cosmic Ray Detection Experimental Report Alisa Bredensteiner Endeavour Institute Santa Cruz Institute of Particle Physics Quarknet August 2010.
Forward Detectors and Measurement of Proton-Antiproton Collision Rates by Zachary Einzig, Mentor Michele Gallinaro INTRODUCTION THE DETECTORS EXPERIMENTAL.
QuarkNet 2011 Mohamed Ali-Hussein Ayasha Jabber. Cosmic Rays Discovered by Victor Hess in 1912 High energy particles (atoms, protons, electrons) traveling.
LIGO-G Z D. Ugolini, Charging Workshop July UV Illumination Studies at Trinity University Dennis Ugolini, Mark Girard 2007 Workshop on.
Jimmy McCarthy International Cosmic Ray Day 26 th September 2012 Detecting Cosmic Rays.
The Transverse detector is made of an array of 256 scintillating fibers coupled to Avalanche PhotoDiodes (APD). The small size of the fibers (5X5mm) results.
RADAR Detection of Extensive Air Showers Nils Scharf III. Physikalisches Institut A Bad Honnef Nils Scharf III. Physikalisches Institut A Bad.
Dominik Wermus (Virginia Military Institute, Lexington, VA 24450), Doug Higinbotham (Thomas Jefferson National Accelerator Facility, Newport News, VA,
QuarkNet Muon Data Analysis with Shower Array Studies J.L. FISCHER, A. CITATI, M. HOHLMANN Physics and Space Sciences Department, Florida Institute of.
Scintillators, DAQ boards, and PMTs Getting Familiarized With the Equipment By Melissa Sussmann and Alex Bonnifield.
A Cherenkov Radiation Detector for the Auger Project Katarzyna Oldak Research Adviser: Corbin Covault Department of Physics The purpose of this project.
Feb 10, 2005 S. Kahn -- Pid Detectors in G4MicePage 1 Pid Detector Implementation in G4Mice Steve Kahn Brookhaven National Lab 10 Feb 2005.
FLC Group Test-beam Studies of the Laser-Wire Detector 13 September 2006 Maximilian Micheler Supervisor: Freddy Poirier.
High School Cosmic Ray Projects and Training Basalt High School Math and Science Club October 14, 2004.
Energy Distribution of Cosmic Ray Muons Paul Hinrichs With David Lee Advised by Phil Dudero.
Status of the NO ν A Near Detector Prototype Timothy Kutnink Iowa State University For the NOvA Collaboration.
Prototypes For Particle Detectors Employing Gas Electron Multiplier
Preliminary MC study on the GRAND prototype scintillator array Feng Zhaoyang Institute of High Energy Physics, CAS, China GRAND Workshop, Paris, Feb. 015.
1 Cosmic Rate Overview Rustem DZHELYADIN (CERN&IHEP, Protvino) The Set-up: Scintillating counters HV setting Coincidence adjustment Accidentals.
Ronald Bruijn – 10 th APP Symposium Antares results and status Ronald Bruijn.
Experiment Design SCIPP Teacher Workshop Mary Jo Nordyke August 2010.
1 IDM2004 Edinburgh, 9 september 2004 Helenia Menghetti Bologna University and INFN Study of the muon-induced neutron background with the LVD detector.
Programmable logic device Time-to-digital converters 5 Volt DC power To PC serial port Four analog PMT inputs Discriminator threshold adjust GPS input.
Brian Lowery July 11,  Primary  From space ▪ Lower energy cosmic rays come from sun ▪ Higher energy cosmic rays come from other places in the.
Update on the Triple GEM Detectors for Muon Tomography K. Gnanvo, M. Hohlmann, L. Grasso, A. Quintero Florida Institute of Technology, Melbourne, FL.
A.D.O.M Airborne.Detector.of.Muons Tye Barba Anna Chang Natalina DeFusco David Hood.
Cosmic Ray Workshop May 15, Cosmic Ray Detector Kit.
Status of the ETL 9125FLB Photomultiplier Tubes Steve Bache UNC-Wilmington.
QuarkNet and Cosmic Ray Muon Flux Experiments Florida Academy of Sciences Spring Conference 2009 Alfred Menendez and Michael Abercrombie with Dr. Marcus.
The Cosmic Ray Observatory Project in Nebraska Conference on Teacher Research Experiences University of Rhode Island April 2005 An education and.
Calibration instructions for Quarknet Cosmic-Ray Detector How to Plateau the Counters A friendly guide for students and teachers Edited by Jeremy Paschke,
Balloon Detector SCIPP. Purpose To make a project that can be replicated by high school groups To gather data on Muon count rates at different altitudes.
Detecting Air Showers on the Ground
Detecting shielded nuclear contraband using muon tomography Judson Locke, William Bittner, Leonard Grasso, Dr. Kondo Gnanvo; Adviser: Dr. Marcus Hohlmann.
Quesly Daniel, Jr. Florida A&M University Dr. Calvin Howell Duke University, TUNL David Ticehurst UNC-Chapel Hill, TUNL Software for Neutron Detector Capture.
Nuclear Medicine Instrumentation 242 NMT 1 Dr. Abdo Mansour Assistant Professor of radiology
A. Tsirigotis Hellenic Open University N eutrino E xtended S ubmarine T elescope with O ceanographic R esearch Reconstruction, Background Rejection Tools.
Forschungszentrum Karlsruhe Erice, 7th July th International School for Cosmic Rays Astrophysics Motivation Energy Reconstruction Air Fluorescence.
Measurement of the Muon’s Lifetime & Cosmic Ray Flux J.C.Xu Q.Y.Tang
QuarkNet Student Investigations
Muon Lab Theory Muons (standard model) Cosmic rays Life time
QuarkNet and Cosmic Ray Muon Flux Experiments
* Experimental technique
Muon and Neutron detector of KIMS experiment
Particle Physics LECTURE 7
Investigations of CME in muon flux detected in hodoscopic mode
Pulse Processing Chapter No. 17
The Life and Times of Cosmic-ray Muons
Cosmic Ray Showers Cosmic ray activity Figure 3:
DING CONGJIN LU GUICHI MARSEILLE
Muon Lifetime Alden Deran.
Presentation transcript:

Cosmic Ray Muon Detection Department of Physics and Space Sciences Florida Institute of Technology Georgia Karagiorgi Julie Slanker Advisor: Dr. M. Hohlmann

Cosmic Ray Muons            

Main goals Equipment setup Muon flux measurement Investigation of flux variation with –Altitude –Zenith angle –Cardinal points –Overlap area Investigation of count rate variation with –Overlap area –Separation distance between the paddles Investigation of “doubles’ flux” with zenith angle Muon lifetime experiment Air shower experiment

Equipment 2 scintillation detectors developed at Fermilab 2 PMT tubes 2 PM bases 2 Coincidence logic boards (version 1 and version2)

Scintillation Detectors A scintillation detector has the property to emit a small flash of light (i.e. a scintillation) when it is struck by ionizing radiation.

Setup The setup is such that the counter on the DAQ board and the computer are recording “coincidences”, i.e. signals sent from both detectors at the same time

DAQ board resolving time for coincidences = 160ns This technique Results in elimination of background noise Offers a great number of possible experiments

I. Setting up equipment Plateau Measurements for PMTs (Procedure for finding working voltage) Example of a plateau curve: Plateau Onset of regeneration effects (afterpulsing, discharges, etc)

Plateau measurements For coincidences

Plateau measurements For coincidences

II. Flux Muons reach the surface of the Earth with typically constant flux Fμ. (count rate)d 2 Fμ =  (area of top panel)(area of bottom panel) Fμ = 0.48 cm -2 min -1 sterad -1 (PDG theoretical value) Count rate: 0.585cm -2 min -1 (horizontal detectors) Our experimental value: 36min -1 (8% efficiency)

With altitude We collected data on the 7 different floors of Crawford building, on the FIT campus All measurements were taken at a same specific location on each floor, except for the one on floor 7. III. Investigation of flux variation

With altitude Results: III. Investigation of flux variation

With zenith angle θ Expected result: F μ ~ cos 2 θ III. Investigation of flux variation

With zenith angle θ Rotation mount for support of the setup: III. Investigation of flux variation

With zenith angle θ Results: (7 th floor Crawford) III. Investigation of flux variation

With zenith angle θ Results: (7 th floor Crawford) III. Investigation of flux variation

With zenith angle θ Results: (Observatory) III. Investigation of flux variation

With zenith angle θ Results: (Observatory) III. Investigation of flux variation

With cardinal points Results: (Senior Lab) III. Investigation of flux variation

With cardinal points Results: (Senior Lab) III. Investigation of flux variation

With cardinal points Results: (Senior Lab) III. Investigation of flux variation

With cardinal points Results: (Senior Lab) III. Investigation of flux variation

With cardinal points Results: (Senior Lab) III. Investigation of flux variation

With overlap area

Results: III. Investigation of flux variation

IV. Investigation of count rate variation With overlap area Results:

IV. Investigation of count rate variation With separation distance d between the two paddles Expected results: count rate is proportional to stereo angle viewed along a specific direction Values calculated using Mathematica integral output Rectangular arrangement; top/bottom phase constant (lxl); d varies (multiples of l)

IV. Investigation of count rate variation With separation distance d between the two paddles Results:

Using the DAQ v.1 board, we recorded low energy (decaying) muon events on the computer. These events are called “doubles.” V. Investigation of “doubles’ flux” variation

With zenith angle θ Results: (Observatory) V. Investigation of “doubles’ flux” variation

We collected data of double events We plotted t decay of an initial sample N 0 of low energy muons We fit the data to an exponential curve of the form: N(t) = N 0 e^(-t/T); where T = muon lifetime VI. Muon lifetime experiment

Results: y = e x Lifetime T: T = μs T th = μs VI. Muon lifetime experiment

Results: y = e x Lifetime T: T = μs T th = μs VI. Muon lifetime experiment

Results: Lifetime T: T = μs T th = μs VI. Muon lifetime experiment (verification)

Results: Lifetime T: T = μs T th = μs VI. Muon lifetime experiment (verification)

In progress… Make use of: DAQ v.2 board – GPS option Another 5 detector setups assembled during QuarkNet IX. Air shower experiment

References