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MINILENS - A Scalable Prototype Detector for LENS LONU-LENS: Mini-Workshop on Low-Energy Solar Neutrinos and LENS Blacksburg, VA, October 14-15 Mark Pitt Virginia Tech

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Page 1: MINILENS - A Scalable Prototype Detector for LENS LONU-LENS: Mini-Workshop on Low-Energy Solar Neutrinos and LENS Blacksburg, VA, October 14-15 Mark Pitt

MINILENS -A Scalable Prototype Detector for

LENS

LONU-LENS: Mini-Workshop on Low-Energy Solar Neutrinos and LENS

Blacksburg, VA, October 14-15

Mark PittVirginia Tech

Page 2: MINILENS - A Scalable Prototype Detector for LENS LONU-LENS: Mini-Workshop on Low-Energy Solar Neutrinos and LENS Blacksburg, VA, October 14-15 Mark Pitt

5” PMTPassiveShield Mirror 5” PMTPassiveShield Mirror

Opt segmentation cage

InLS500 mm

InLS

LS Envelope

500 mm

• 6 x 6 x 6 array of cubic cells, 12.5 cm on a side

• Optical foil segmentation cage • InLS : 128 L

• PC Envelope (active shield) : 200 L

• Indium mass ~ 20 – 40 kg (8 – 16 % by weight)

• Read out with 108 5 inch PMT’s (on three perpendicular faces; mirrors on other sides)

MINILENSFinal Test detectorfor LENS

Page 3: MINILENS - A Scalable Prototype Detector for LENS LONU-LENS: Mini-Workshop on Low-Energy Solar Neutrinos and LENS Blacksburg, VA, October 14-15 Mark Pitt

5” PMTPassiveShield Mirror 5” PMTPassiveShield Mirror

Opt segmentation cage

InLS500 mm

InLS

LS Envelope

500 mm

MINILENSFinal Test detectorfor LENS

Goals for MINILENS

• Test detector technology Medium Scale InLS production Design and construction

• Test background suppression of In radiations by 10-11

Expect ~ 5 kHz In -decay singles rate; adequate to test trigger design, DAQ, and background suppression schemes

• Demonstrate In solar signal detection in the presence of high background (via “proxy”)

Direct blue print for full scale LENS

Page 4: MINILENS - A Scalable Prototype Detector for LENS LONU-LENS: Mini-Workshop on Low-Energy Solar Neutrinos and LENS Blacksburg, VA, October 14-15 Mark Pitt

MINILENS Mark Pitt, Virginia Tech, October 2006

Cosmic Proton SecondariesCC -capture in 115In to excited isomeric level in 115Sn

SneeIne115

s)4.76( tagdelayedsignalsolar

115 )/(

Excitation of the 713.6 keV isomeric state via

115In (p,n) from cosmic proton secondaries can produce the same tag that mimics neutrino capture

At 2000 mwe, this will be suppressed:

BUT at surface this mechanism can be usedas a PROXY for the solar neutrino events.

Page 5: MINILENS - A Scalable Prototype Detector for LENS LONU-LENS: Mini-Workshop on Low-Energy Solar Neutrinos and LENS Blacksburg, VA, October 14-15 Mark Pitt

MINILENS Mark Pitt, Virginia Tech, October 2006

Indium --Background Topology – Space / Time coincidence

Background

Signal

E() -114 keV

116 keV

497 keV

115In

115Sn

e/

=4.76s

Background:

Random time and space coincidencebetween two -decays ( );Extended shower ( ) can be created by:a) 498 keV from decay to excited

state;b) Bremsstrahlungs -rays created by ;c) Random coincidence (~10 ns) of

more -decays;Or any combination of a), b) and c).

Signal Signature:

Prompt e- ( )followed bylow energy (e-/) ( )and Compton-scattered ( )

115In

β0 + n (BS) (Emax = 499 keV)

498 keV

*Cattadori et al: 2003

β1 (Emax< 2 keV)(b = 1.2x10-6)*

115Sn

Page 6: MINILENS - A Scalable Prototype Detector for LENS LONU-LENS: Mini-Workshop on Low-Energy Solar Neutrinos and LENS Blacksburg, VA, October 14-15 Mark Pitt

MINILENS Mark Pitt, Virginia Tech, October 2006

Proxy pp events in MINILENS from cosmogenic 115In(p,n)115Sn isomers

• Pretagged via , p tracks• Post tagged via 115In(n,) and 230 s delay

Gold plated 100 keV events (proxy pp), Tagged by same cascade as In- events

Can measure detection efficiency of tag for our analysis cut scheme

Expect ~ 40 events of this type per year at the surface

Proxy pp- events in MINILENS

Page 7: MINILENS - A Scalable Prototype Detector for LENS LONU-LENS: Mini-Workshop on Low-Energy Solar Neutrinos and LENS Blacksburg, VA, October 14-15 Mark Pitt

MINILENS Mark Pitt, Virginia Tech, October 2006

• 115In -decay is a rare fourth forbidden unique type; current best measurements of it are from 1979 Bell Labs In-spectra with only ~ 100 g of In

• MINILENS will provide high statistics measurements of both the beta and bremsstrahlung spectra from 115In -decay needed to validate the input spectracurrently being used in the Monte Carlo

• Recently there has been a claim of a rare < 2 keV endpoint energy beta branch in 115In decay; these high statistics measurements could confirm its existence and measure its properties if it does exist (such a low endpoint energy case could be of interest to direct neutrino mass measurements)

Physics from MINILENS

Page 8: MINILENS - A Scalable Prototype Detector for LENS LONU-LENS: Mini-Workshop on Low-Energy Solar Neutrinos and LENS Blacksburg, VA, October 14-15 Mark Pitt

MINILENS Mark Pitt, Virginia Tech, October 2006

MINILENS: Scalable prototype LENS detector to test all the concepts and the technology developed so far & demonstrate Indium solar signal detection (via cosmic proton proxy)

Summary

● Ongoing work on the optical foils• Teflon identified as best material (nylon breaks down in the acidic PC)• both single and double foil schemes being investigated• Anti-reflection coating with SiO2 nano-particles being investigated to minimize Fresnel losses

Current work on MINILENS:

Plan for MINILENS:

First phase: Run at surface where we expect ~ 40 “proxy” events per year

Second phase: Run at ~ 2000 mwe depth at the VT-NRL low background facility at the Kimballton mine