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neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014 Columbia University REU, XENON

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Page 1: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

neriX PMT Calibration and Neutron Generator Simulation

Haley Pawlow

July 31, 2014

Columbia University REU, XENON

Page 2: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Dark Matter

XENON

neriX

Project 1-> PMT Calibration

Project 2-> Neutron Generator Simulation

07/31/14 Haley  Pawlow,  XENON   2  

Page 3: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

•  1933-> Using Virial Theorem to analyze Coma cluster motion, found the visible mass was too small to explain high velocities of galaxies

•  Missing mass could be dark matter

07/31/14 Haley  Pawlow,  XENON   3  

Fritz Zwicky

Coma    cluster  

Page 4: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

07/31/14 Haley  Pawlow,  XENON   4  

Vera Rubin

Ø  1970-> Rubin measured rotational velocity of spiral galaxy as a function of radius

Ø  Used Newtonian Mechanics to compute mass

Ø  Velocity doesn’t obey

Page 5: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Ø  Two hot x-ray gas clouds (red) collide like a shock wave, producing a bullet shape

Ø Dark matter (blue) passes right through each other with no interaction aside from gravitational force

07/31/14 Haley  Pawlow,  XENON   5  

Bullet Cluster

Page 6: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Ø  Leading dark matter candidate because it agrees nicely with super symmetry

Ø Non-baryonic matter

Ø  Interact with weak force

Ø Neutral in charge and color

Ø  nonrelativistic

Ø Stable or have lifetimes comparable to age of Universe

07/31/14 Haley  Pawlow,  XENON   6  

Weakly Interacting Massive Particles (WIMPs)

Page 7: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Detecting WIMPs Indirect Detection Direct Detection

07/31/14 Haley  Pawlow,  XENON   7  

LHC  (Production)  

Fermi  Gamma  Ray  Telescope  

XENON100

Ø Observe particles or gamma rays resulting from WIMP annihilation or decay

Ø  Look for signal from WIMP nuclear recoils

Ø  Leaders are Dual-Phase, liquid noble gas detectors

Page 8: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Dark Matter

XENON

neriX

Project 1-> PMT Calibration

Project 2-> Neutron Generator

07/31/14   Haley  Pawlow,  XENON   8  

Page 9: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Direct Detection

07/31/14 Haley  Pawlow,  XENON   9  

Ø Simultaneous measurement of ionization and scintillation signals enables XENON to discern between nuclear and electronic recoils

Page 10: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Ø 161kg of LXe

Ø Optimize design for low energy threshold

Ø Purify Xenon

Ø Optimize shielding (underground in Gran Sasso, Italy)

07/31/14 Haley  Pawlow,  XENON   10  

XENON100

Page 11: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

07/31/14 Haley  Pawlow,  XENON   11  

Time Projection Chamber (TPC) Ø WIMP scatters with Lxe nucleus,

causing a nuclear recoil where atom collides into other atoms

Ø Atoms can either be ionized, releasing electrons, or excited, emitting photons which are detected by the photomultiplier tubes (scintillation->S1)

Ø Remaining electrons accelerated across electric field to top gas, producing secondary light (ionization->S2)

Page 12: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Ø light yield (s1) = total photons/Energy

Ø charge yield (s2) = # of electrons/Energy

Ø  S2/S1 differentiates between electronic(gamma/beta)

and nuclear recoils

Ø Leff is largest systematic error in reported LXe WIMP

searches

07/31/14 Haley  Pawlow,  XENON   12  

Measuring S1 and S2

Page 13: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Ø S2/S1 differentiates between electronic(gamma/beta) and nuclear recoils

Ø Using drift time and Voltage, calculate distance (z direction)

Ø PMTs record x and y coordinate of event (hit pattern)

Ø Reconstruct position of event

07/31/14 Haley  Pawlow,  XENON   13  

Position of event

Page 14: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Dark Matter

XENON

neriX

Project 1-> PMT Calibration

Project 2-> Neutron Generator

07/31/14   Haley  Pawlow,  XENON   14  

Page 15: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Ø Analyze how different particles, like neutrons and gamma rays, interact with LXe atoms

Ø Measure s1 and s2 to distinguish

electromagnetic background from WIMPs in XENON

Ø Need to convert from measured scintillation in

Photomultiplier tubes (PMTs) to energy

07/31/14 Haley  Pawlow,  XENON   15  

neriX: How can we calibrate XENON?

Page 16: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Ø Neutron generator emits monochromatic neutrons that elastically scatter with atoms inside LXe.

Ø Two organic liquid scintillators detect neutrons at fixed signal

Ø Measure light and charge yield

07/31/14 Haley  Pawlow,  XENON   16  

neriX Experimental setup

Page 17: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

07/31/14 Haley  Pawlow,  XENON   17  

neriX Detector Ø Same Dual-phase, TPC concept as XENON100 Ø  neriX has 4 top PMTs and 1 bottom PMT Ø XENON100 has 98 top PMTs and 78 bottom PMTs

Page 18: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Dark Matter

XENON

neriX

Project 1-> PMT Calibration

Project 2-> Neutron Generator

07/31/14   Haley  Pawlow,  XENON   18  

Page 19: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Ø  Incident photon emits a single photoelectron (PE) from photocathode

Ø PE attracted to dynode by applied electric field

Ø PE accelerates, releasing more e-’s, which are all attracted to second dynode

Ø Dynodes multiply amount of charge via photoelectric effect

Ø PMT Gain = # of e produced/photoelectron 07/31/14 Haley  Pawlow,  XENON   19  

PMTs

Page 20: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Ø PMTs give us a voltage signal, we need to convert to photoelectrons using the gain

Ø With the gain we can measure s1 and s2 (light and charge signals)

07/31/14 Haley  Pawlow,  XENON   20  

Why do we need to calibrate PMTs?

Bottom PMT array for

XENON100

Page 21: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Ø Number of PE is a poisson distribution: 90% of signal is noise, 10% of signal from 1 PE. This way contribution of multiple PE is minimized

Ø  1st peak around zero is noise, second peak from one photoelectron

07/31/14 Haley  Pawlow,  XENON   21  

Gaussian Distribution of PMTs

Charge[e]0 500 1000 1500 2000

310×

Freq

uenc

y

0

200

400

600

800

1000 = 0.045speΛMean = 9.50e+05 +/- 1.72e+04,

Signal

Noise

Difference between S/N

Channel 1, PMT 1 at 700 V

Page 22: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

07/31/14 Haley  Pawlow,  XENON   22  

Gaussian Distribution of PMTs

Charge[e]400 600 800 1000 1200 1400 1600 1800 2000

310×

Freq

uenc

y

50

100

150

200

250

300

350

400 = 0.045

speRMean = 9.50e+05 +/- 1.72e+04,

Signal

Noise

Difference between S/N

Channel 1, PMT 1 at 700 VØ Λ = 0.045, the

1-PE peak is 4.5% of signal

Ø Agrees with Poisson distribution

Page 23: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

PMT Calibration

07/31/14 Haley  Pawlow,  XENON   23  

Ø  4 top PMTs and 1 bottom PMT, 4 channels each

Ø PMT Gain = # of electrons produced/PE

Ø PMT gain increases exponentially, seen as line in log linear plot

Page 24: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Dark Matter

XENON

neriX

Project 1-> PMT Calibration

Project 2-> Neutron Generator

07/31/14   Haley  Pawlow,  XENON   24  

Page 25: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Neutron Generator

07/31/14 Haley  Pawlow,  XENON   25  

1. Heat filament and release deuterium gas

2. As cathode heats up, electrons extracted to the grid

3.  Ionized deuterium gas ions accelerate toward titanium deuteride target

4.  Ions collide with target and are either stopped or produce neutrons

5. Neutrons are mono-energetic, minimizing spread in neutron energy at a 90 degree angle

1  

2  3

45  

Page 26: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Ø Increase voltage 40kV->100kV

Ø With a higher voltage we get greater

neutron flux

Ø Faster data collection

07/31/14 Haley  Pawlow,  XENON   26  

Why modify Neutron Generator holder?

Page 27: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Ø Need to avoid electrical discharge at HV cable connection to neutron generator

Ø Analyze electrical breakdown (dielectric strength) for different dielectric materials (Teflon, oil, and air)

07/31/14 Haley  Pawlow,  XENON   27  

Electrical Breakdown across HV cable

Page 28: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Electrical Breakdown in Air

07/31/14 Haley  Pawlow,  XENON   28  

At the HV cable radius, the electric field exceeds electrical breakdown for 100kV

radius [mm]0 1 2 3 4 5 6 7 8 9 10

E(r)[

V/m

m]

0

2000

4000

6000

8000

10000

12000

14000 Air50 kV80kV100kV150kVInner radiusOuter radiusBreakdown Voltage

Page 29: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Electrical Breakdown in Oil

07/31/14 Haley  Pawlow,  XENON   29  

At the HV cable radius, the electric field exceeds electrical breakdown for 100kV

radius [mm]0 1 2 3 4 5 6 7 8 9 10

E(r)[

V/m

m]

0

5000

10000

15000

20000

25000Mineral Oil

50 kV80kV100kV150kVInner radiusOuter radiusBreakdown Voltage

Page 30: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Electrical Breakdown in Teflon

07/31/14 Haley  Pawlow,  XENON   30  

At the HV cable radius, the electric field is well below electrical breakdown for 100kV

radius [mm]0 1 2 3 4 5 6 7 8 9 10

E(r)[

V/m

m]

0

20

40

60

80

100

1203

10×

Teflon50 kV80kV100kV150kVInner radiusOuter radiusBreakdown Voltage

Page 31: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Ø Optimize ratio between Teflon and oil to produce least amount of neutron scatters

07/31/14 Haley  Pawlow,  XENON   31  

GEANT4 Monte Carlo Simulation

Teflon cut radius =

radius of mineral oil

*Image  from  GEANT4  simulation  

Page 32: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Example: Teflon/oil = 1.5743

07/31/14 Haley  Pawlow,  XENON   32  

52% of neutrons scatter

Page 33: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Teflon/Oil Scattered/Total neutrons

1.57 0.522

0.5 0.522

0.19 0.520

07/31/14 Haley  Pawlow,  XENON   33  

Conclusions

Ø  Largest Teflon cut produces least amount of neutron scatters

Ø Amount of scattering is negligible +/- 0.4%

Ø Use maximum amount of Teflon in holder design to keep neutron generator fixed

Page 34: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

SolidWorks Model for Neutron Generator Holder

07/31/14 Haley  Pawlow,  XENON   34  

Ø  Increase holder tube diameter from 2->3’’

Ø  Maximize use of Teflon to minimize neutron scatters

Page 35: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

SolidWorks Neutron Generator Holder Model

07/31/14 Haley  Pawlow,  XENON   35  

ü HV cable surrounded with Teflon to avoid electrical breakdown

ü Neutron Generator firmly secured in carrier

with Teflon/oil ~1.5

Page 36: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Ø Measure nuclear and electronic recoils by varying electric fields across chamber

Ø More precise measurement of gamma rays at low energy with Cs 137 Compton scatters

07/31/14 Haley  Pawlow,  XENON   36  

Next Steps for neriX

Page 37: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

7/31/2014 Haley  Pawlow,  XENON   37  

Takeaways  

ROOT/C++ GEANT4 SolidWorks  

Dark  Matter  ,  XENON,  neriX  

Graduate  School  

Research  Environment  

Particle  Physics  Lectures  

Brookhaven  National  Lab  

Page 38: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Acknowledgements

07/31/14 Haley  Pawlow,  XENON   38  

•  Elena Aprile for giving me this opportunity •  Antonio Melgarejo, Marc Weber, Luke

Goetzke, and Matt Anthony for their support and guidance

•  The XENON team at Nevis for being so inviting

•  John Parsons and Amy Garwood for organizing the REU program

•  NSF REU program for their generous funding

Page 39: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Questions???

Page 40: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Appendix

08/31/14   Haley  Pawlow,  XENON   40  

Page 41: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Gain = # of electrons/photoelectron emitted

PMT Quantum Efficiency = 35% (# photons/PE)

Number of photons from PMT

Light Detection Efficiency

Total # photons emmited (type, Energy, E field)

08/31/14 Haley  Pawlow,  XENON   41  

Measuring # of photons from PMT

Page 42: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Relative scintillation efficiency of nuclear recoils

(Leff)

08/31/14 Haley  Pawlow,  XENON   42  

Leff  is  largest  systematic  error  in  reported  LXe  WIMP  searches  

Page 43: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

08/31/14 Haley  Pawlow,  XENON   43  

Page 44: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

08/31/14 Haley  Pawlow,  XENON   44  

Page 45: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

08/31/14 Haley  Pawlow,  XENON   45  

Page 46: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Monte Carlo Simulation of ideal Teflon/Oil ratio

08/31/14 Haley  Pawlow,  XENON   46  

Page 47: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Teflon/oil= 0.50

08/31/14 Haley  Pawlow,  XENON   47  

52 % of neutrons scatter

Page 48: neriX PMT Calibration and Neutron Generator Simulationxenon.astro.columbia.edu/REU/PawlowTalk.pdf · neriX PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014

Teflon/oil = 0.191

08/31/14 Haley  Pawlow,  XENON   48  

52% of neutrons scatter