Spherical Time Projection Chamber (STPC) for future neutrino and dark matter experiments
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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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Zhimin wang liu ruoqing tang chenyang charling tao changgen yang changjiang dai

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 DetectorDeveloped 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

  • 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


Run with ar ch 4 3g 3 he @ 200 mb spc 130cm @ lsm

RunwithAr/CH4 + 3g 3He @ 200 mb SPC 130cm Ø @ LSM

NB: no start

=> risetime records place and/or history of energydeposition

210Po

5.3 MeV

If localisedenergydeposition, rise time depends of radius

(diffusion)

n capt on 3He

764 keV

Rise time (s)

alpha

If track, rise time depends on orientation of track

(different drift times)

222Rn 218Po 214Po

derivative

de/dx

Amplitude


Run with ar ch 4 3g 3 he @ 200 mb spc 130cm @ lsm1

RunwithAr/CH4 + 3g 3He @ 200 mb SPC 130cm Ø @ LSM

210Po

5.3 MeV

from 210Pb

@ Cu surface

R = 15 cm

210Po

5.3 MeV

Taux 400 capt/j

n capt on 3He

764 keV

Rise time (s)

n capt on 3He

=> p + T

3

2

1

Unwanted Radon daughter deposit on surface

222Rn 218Po 214Po

Amplitude

2 : fast neutron expected here


Basic performance

Basic performance

  • 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

Applications

  • 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

arXiv:1401.7902Gerbier et al.

DM WIMP

Reactor neutrino


Lsm neutron flux

doi:10.1088/1742-6596/203/1/012030

LSM neutron flux

From Savvidisilias


An international working group news

An international working group “NEWS”

from G. Gerbier


Activities at ihep tsinghua

Activities at IHEP &Tsinghua

Detector performance studies

  • Plan to measure neutrons in Jinping with 1g He3


Stpc goals

STPC goals

  • 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 simulation (1997?)

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


Zhimin wang liu ruoqing tang chenyang charling tao changgen yang changjiang dai

Dark matter detection with hydrogen proportional counters

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 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

  • 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

MIMAC

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


Zhimin wang liu ruoqing tang chenyang charling tao changgen yang changjiang dai

Bi-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


Zhimin wang liu ruoqing tang chenyang charling tao changgen yang changjiang dai

Background in LSM


Electron vs nuclei recoil

Electron vs 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 keV He4 recoils


3d track reconstruction 34 kev

3D-Track reconstruction 34 keV


Some tracks in mimac

Some tracks in MIMAC

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 1m3 in preparation


Wimp distribution

WIMP distribution


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