minilens - a scalable prototype detector for lens lonu-lens: mini-workshop on low-energy solar...
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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](https://reader035.vdocument.in/reader035/viewer/2022072111/5697bf7c1a28abf838c83d03/html5/thumbnails/1.jpg)
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
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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
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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
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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.
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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
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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
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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
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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