Spherical Time Projection Chamber (STPC) for future neutrino and dark matter experiments
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Zhimin Wang Liu Ruoqing , Tang ChenYang , Charling Tao, Changgen Yang , Changjiang Dai, - PowerPoint PPT Presentation

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Spherical Time Projection Chamber (STPC) for future neutrino and dark matter experiments (or Spherical Proportional Counter). Zhimin Wang Liu Ruoqing , Tang ChenYang , Charling Tao, Changgen Yang , Changjiang Dai, Tsinghua & IHEP 2014-10-12, Shanghai.

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Spherical Time Projection Chamber (STPC) for future neutrino and dark matter experiments(or Spherical Proportional Counter)

Zhimin Wang

Liu Ruoqing, Tang ChenYang,

Charling Tao, Changgen Yang , Changjiang Dai,

Tsinghua & IHEP

2014-10-12, Shanghai

A simple new gas detector developed by ioanis giomataris saclay france
A Simple New Gas Detector and dark matter experimentsDeveloped by IoanisGiomataris, Saclay, France

  • Natural focusing:

    • large volumes can be instrumented with a small readout surface and few (or even one) readout lines

  • 4p coverage: better signal

  • Still some spatial information achievable:

    • Signal time dispersion

  • Other practical advantages:

    • Symmetry: lower noise and threshold with large volume

    • Low capacity

    • No field cage

  • Simplicity: few materials. They can be optimized for low radioactivity.

  • Low cost

A prototype
A prototype and dark matter experiments

  • D=1.3 m

  • V=1 m3

  • Spherical vessel made of Cu (6 mm thick)

  • P up to 5 bar possible (up to 1.5 tested up to now)

  • Vacuum tight: ~10-6 mbar (outgassing: ~10-9 mbar/s)

Typical spectra
Typical spectra and dark matter experiments

Run with ar ch 4 3g 3 he @ 200 mb spc 130cm @ lsm
Run and dark matter experimentswithAr/CH4 + 3g 3He @ 200 mb SPC 130cm Ø @ LSM

NB: no start

=> risetime records place and/or history of energydeposition


5.3 MeV

If localisedenergydeposition, rise time depends of radius


n capt on 3He

764 keV

Rise time (s)


If track, rise time depends on orientation of track

(different drift times)

222Rn 218Po 214Po




Run with ar ch 4 3g 3 he @ 200 mb spc 130cm @ lsm1
Run and dark matter experimentswithAr/CH4 + 3g 3He @ 200 mb SPC 130cm Ø @ LSM


5.3 MeV

from 210Pb

@ Cu surface

R = 15 cm


5.3 MeV

Taux 400 capt/j

n capt on 3He

764 keV

Rise time (s)

n capt on 3He

=> p + T




Unwanted Radon daughter deposit on surface

222Rn 218Po 214Po


2 : fast neutron expected here

Basic performance
Basic performance and dark matter experiments

  • Mixtures tested:

    • Ar+10% CO2

    • Ar+2% Isobutane

  • Pressures from 0.25 up to 1.5 bar tested up to now

  • High gains (>104) achieved with simple spherical electrode

  • No need to go to very high V (better for minimizing absorption)

Applications and dark matter experiments

  • Dark Matter

  • Coherent neutrino scattering

  • Double beta decay

  • Axion

  • SN neutrino monitoring


  • Neutron spectroscopy

  • Neutron counter for industrial application

  • Low level neutron counting

  • Radon low level counting

  • Atmospheric neutron and Muon monitoring

  • Gamma ray spectroscopy in harsh environment

Some physics applications
Some physics applications and dark matter experiments

arXiv:1401.7902Gerbier et al.


Reactor neutrino

Lsm neutron flux

doi:10.1088/1742-6596/203/1/012030 and dark matter experiments

LSM neutron flux

From Savvidisilias

An international working group news
An international working group “NEWS” and dark matter experiments

from G. Gerbier

Activities at ihep tsinghua
Activities at IHEP &Tsinghua and dark matter experiments

Detector performance studies

  • Plan to measure neutrons in Jinping with 1g He3

Stpc goals
STPC goals and dark matter experiments

  • NEWS network: 4m detector. Where?

    • Jinping?

    • SNO? Gerbier in Canada with 10 M$ grant

  • Training for low radioactivity gaseous detector for large volume TPC

    • Solar neutrino (HELLAZ like)

    • Directional Dark Matter (also an old idea!)

Hellaz simulation 1997
Hellaz and dark matter experiments simulation (1997?)

1995-1998 The HELLAZ solar pp neutrino project Tom Ypsilantis, Jacques Séguinot et al… , with a Micromegas

Dark matter detection with hydrogen proportional counters and dark matter experiments

G. Gerbier, J. Rich, M. Spiro, C. Tao

Nuclear Physics B - Proceedings SupplementsVolume 13, February 1990, Pages 207-208

Comments : for some DM types

not Mass but Number of nuclei is important

Gaseous detectors are beautiful
Gaseous and dark matter experiments detectors are beautiful!

  • 1975-1979 Cylindrical Drift chamber in PhD thesis back for Fermilab

    DIS muon CHIO in Smithsonian (Washington DC)

  • 1979-1982: UA1 Central Detector 1st W event in UA1 CD

Personalinterest for > 20 years

Technology OK and keeps improving

For DM: needs detection from >2 nuclei

AND directionality!!!

Is our science case compelling enough?

CDM vs WDM debate

Directional dm detectors
Directional DM Detectors and dark matter experiments

  • CYGNUS 2013: 4th Workshop on Directional Detection of Dark Matter Tatsuhiro Naka and KentaroMiuchi- 2013 J. Phys.: Conf. Ser.469 011001

    Workshop Series Boulby 2007 , MIT 2009, Aussois2011

  • Many projects: DMTPC, NEWAGE, DRIFT, MIMAC

  • emulsions

MIMAC and dark matter experiments

MIMAC bi-chamber prototype 1311.0616

  • The MIMAC bi-chamber prototype is composed of two chambers sharing the same cathode being the module of the matrix

  • active volume (V 5:8 l)

  • 70%CF4 + 28%CHF3 + 2%C4H10 at a pressure of 50mbar. The primary electron- ion pairs produced by a nuclear recoil in one chamber of the matrix are detected by driving the electrons to the grid of a bulk micromegasand producing the avalanche in a very thin gap (256 mu).

  • Track reconstruction in MIMAC. The anode is read every 20 ns. The 3D track is reconstructed, from the consecutive number of images

Bi and dark matter experiments-chamber prototype at the

LaboratoireSouterrain de Modane

The bi-chamber prototype at the LaboratoireSouterrain de Modane in June

2012. The bi-chamber module is identified in red and the bluer volume in blue.

The position of peaks of Cd (3.2 keV), Cr (5.4 keV), Fe (6.4 keV), Cu (8.1 keV) and Pb (10.5 and

12.6 keV) tted by a linear calibration in ADC channels as a function of time, highlighting the

gain stability during the data taking period.

4. Preliminary analysis of the first months of data taking

The first available data set of the bi-chamber prototype was started on July 5th 2012

Background in LSM and dark matter experiments

Electron vs nuclei recoil
Electron and dark matter experimentsvs nuclei recoil

The length [cm] vs. Energy [ADC channel] of electrons and proton recoils produced by neutrons of 144 keV in pure isobutane (C4H10) at 50 mbar. The maximum of the proton energy corresponds to 144 keV. (Right): The NIS (normalized integrated straggling) for recoil events (in black) and for electrons (in blue).

1 5 kev he4 recoils
1.5 and dark matter experimentskeV He4 recoils

3d track reconstruction 34 kev
3D-Track reconstruction 34 and dark matter experimentskeV

Some tracks in mimac
Some tracks in MIMAC and dark matter experiments

8 keV hydrogen nucleus in 350 mbar 4He+5%C4H10, a fluorine nucleus leaving 50 keV in ionization in 55 mbar (70% CF4 + 30% CHF3) and a 5.5 MeV alpha particle in 350 mbar 4He+5%C4H10

Mimac 1m 3 in preparation
MIMAC 1m and dark matter experiments3 in preparation

Wimp distribution
WIMP distribution and dark matter experiments