and the NEXT collaboration

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Presentation transcript:

and the NEXT collaboration Microscopic simulation of Xenon-based optical TPCs in the presence of additives C. Azevedo, S. F. Biagi, D. Gonzalez-Diaz and the NEXT collaboration @Paris (05/12/2016)

I. The problem

The importance of the ‘topological’ information in NEXT low-diffusion Xe J. Renner et al., arXiv:1609.06202v3 (deep neural network analysis) Xe but what happens to the Xenon scintillation when diffusion is reduced?? Xe low-diffusion mixture ββ0 signal γ-background MC-truth low diffusion pure Xenon

A ‘conceptual’ magic mixture From TPC conference 2014! (Penning)-Fluorescent Low diffusion/light preserving (2 candidate molecules identified) (6+ candidate molecules identified) Able to reduce electron diffusion in gas. Able to reduce electron diffusion in gas. Recombination small. Recombination small. Strongly fluorescent at higher λ and self-transparent. Light mechanisms unaffected. Highly transparent to Xenon-light. Small quenching for S1, S2 and small fluctuations in EL. Allows for EL at lower field due to low-lying excited states of the additive. Suitable for Penning transfer. Can potentially reduce Fano factor. ~’low IP/high-reactive type’ ~’high IP/low-reactive type’

II. The tool

A microscopic software for electron and photon transport in gas Degrad (WI, F, cloud size) (recombination MC/model) [not included here] scintillation MC, and photo-absorption x-section database (S1, S2) Magboltz electron x-section database Magboltz Garfield++ (vd,DL,DT )

III. Basic considerations and input

Electron x-sections of relevant gases Xenon 2016 x-sections for molecules that are plot here are actually old ones (just illustrative!)

Ionization transport characteristics (vd, DL, DT) Outside 20-30V/cm/bar it performs generally worse Ed=20 V/cm/bar, P=15bar H2 CF4 CO2 CH4 N2 Mean Electron Energy H2(0.8%) CF4(0.007%) CO2(0.02%) CH4(0.1%) N2(4%)

Ionization transport characteristics (vd, DL, DT) Outside 20-30V/cm/bar it performs generally worse Ed=20 V/cm/bar, P=15bar C2H6 i-C4H10 CH4 C2H6 i-C4H10 CH4 Mean Electron Energy C2H6 (0.06%) i-C4H10(0.035%) CH4 (0.1%) C2H6 i-C4H10 CH4

II Light transparency i-C4H10 C2H6

Light quenching (generic pathway diagram) III Light quenching (generic pathway diagram) IPXe IPXe2 3body 2body decay example of main (atomic) quenching reactions other continua relevant for S1 relevant for S2 2nd continuum (170nm) Most serious difficulties related to S1: Distribution of initial excited states?. Quenching/decay of Xe**, Xe2** not fully known. S2 much more robust (dominated by low-lying states): Measurements exist.

IV. Electron transport + scintillation model

Computation of probability distribution of excited states Degrad Garfield++

Computation of atomic cascade II Computation of atomic cascade decay constant 2-body collision rates 3-body collision rates each value represents a vector!

III Excimer pathways (analogous for 2p5 and Xe**)

Example of light production code (population evolution from 2p10)

Example of electron transport + light production code time distributions energy spectra

V. Comparison with pure xenon data

Time distributions

Yields VUV region IR region simulated measured (α’s)

VI. Comparison with xenon + additives

Electroluminescence (yield)

Electroluminescence (light fluctuations, Q) 𝑟𝑒𝑠𝑜𝑙𝑢𝑡𝑖𝑜𝑛=2.35 𝐹+𝑄 𝑊 𝐼 ε

Conclusions A new microscopic simulation for photon and electron transport in gaseous Xenon has been developed inside the NEXT collaboration. It can compute the primary and secondary scintillation stemming from X, γ-ray and high energy electron interactions (1keV to several MeV). It provides the time and spectral characteristics, in the range 150nm-1500nm. It can describe the effect of molecular additives and its impact on the light yield. It has shown to be a formidable tool for the R&D on low-diffusion gases within NEXT. Outlook This framework was developed to solve a concrete technological problem… But the authors are interested in tackling a variety of other admixtures used for optical TPC. The new landscape is enormous, so work will continue depending on the interest and the available resources.

VI. Appendix

A low diffusion/light-preserving gas in action

Electron cloud size in Degrad arXiv:1605.06256v3 [physics.ins-det]

! ! Xe-CO2 if assuming a fit gives: The quenching rate of s5 state in CO2 is: !

! Xe-CF4 if assuming and the quenching rate of s5 state in CF4: Predicts a 0.3% scintillation drop in the range of concentrations shown…

An analytic picture… and a simple one (I) Indeed: dominance of triplet state scintillation above 1bar!

Ambiguities in the scintillation model (I)

Ambiguities in the scintillation model (II) default model used in simulations model by J. Escada (predicts no pressure dependence of time spectra!, just a global yield drop)