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Study of the Doppler broadening of positron annihilation radiation in silicon

Abstract

We report the measurement of Doppler broadening annihilation radiation in silicon, using 22Na as a positron source, and two Ge detectors arrangement. The two-dimensional coincidence energy spectrum was fitted using a model function. The model function included at rest positron annihilation with valence band, 2p, 2s, and 1s electrons. In-flight positron annihilation was also fitted. The detectors response functions included backscattering, and a combination of Compton effects, pileup, ballistic deficit, and pulse shaping problems. The obtained results agree well with the literature.


APPLIED PHYSICS AND INSTRUMENTATION

Study of the Doppler broadening of positron annihilation radiation in silicon

E. do NascimentoI; O. HeleneI; V. R. VaninI; M. MorallesII

IInstituto de Física, Universidade de São Paulo, C.P. 66318, 05315-970, São Paulo, SP, Brazil

IIInstituto de Pesquisas Energéticas e Nucleares - IPEN, C.P. 11049, 05422-970, São Paulo, SP, Brazil

ABSTRACT

We report the measurement of Doppler broadening annihilation radiation in silicon, using 22Na as a positron source, and two Ge detectors arrangement. The two-dimensional coincidence energy spectrum was fitted using a model function. The model function included at rest positron annihilation with valence band, 2p, 2s, and 1s electrons. In-flight positron annihilation was also fitted. The detectors response functions included backscattering, and a combination of Compton effects, pileup, ballistic deficit, and pulse shaping problems. The obtained results agree well with the literature.

I. INTRODUCTION

Doppler broadening study of positron-electron annihilation radiation is an important tool in the field of materials science [1, 2]. Usually, the results of Doppler broadening experiments have been analyzed through the comparison of the calculated annihilation probability density with the experimental data. In this work we went in the inverse direction: a model function was fitted to the experimental data in order to obtain the distribution of electron momenta, similar to the analysis accomplished for the aluminum [3, 4]. In these works the coincidence energy spectrum was fitted using a model function, accounting for both Doppler broadening and detector system response. Intensities of the thermalized positron annihilation with band, 2p, 2s, and 1s electrons, and in-flight positron annihilation were fitted. The binding energies of the 1s, 2s, and 2p electrons and the Fermi cutoff parameters of the band electrons were also fitted. This procedure allows the experimental determination of the annihilation parameters and response function parameters with their uncertainties and the c2-test of the obtained results.

II. EXPERIMENTAL SETUP

The two annihilation gamma-rays energies E1 and E2 were measured using two Ge detectors forming an angle of 180º with each other and separated by 5 cm. A 3.7×105 Bq (10 µCi) 22Na source was placed between two 2 mm thick silicon mono-crystal sheets (Czochralski). Previous lifetime measurements results obtained were 219.0 ps with 97.7% of intensity, 473 ps with 2.0% of intensity, and 2800 ps with 0.3% of intensity. An 192Ir source was simultaneously measured in order to calibrate the detectors and to follow any energy calibration drift during the experiment. 60Co and 137Cs sources were also measured. A two dimensional spectrum was taken for about 730 h. The two dimensional histogram in the E1, E2 plane in the region of interest is presented in (Figure 1).


This spectrum of Figure 1 can be interpreted as follows. The crest along the line E1+E2 = 1022 keV is mainly due to at rest positron annihilation with core and band electrons. The ridges parallel to the axes are due to the coincidence between an annihilation gamma-ray and a Compton scattered gamma-ray (either the other annihilation radiation or the 1274.5 keV gamma-ray from 22Na decay). When in-flight positron annihilates with a low momentum electron, two gamma rays are emitted. Near the 511 keV-511 keV peak in the two dimensional spectrum this annihilation can be approximated by a crest along a circular arc function centered at E1 = E2 = 3/2mc2 [4]. This curve can be barely seen in (Figure 1).

III. FITTING - FUNCTION MODEL

To describe quantitatively the measured spectrum, a two dimensional function was fitted to the experimental histogram in an 87 keV x 87 keV region around the two photon annihilation peak. Positron annihilation with valence band was represented by

along the line E1+E2+Bv = 1022 keV, where Bv is the gap energy of the silicon [5],E1 and E2 are energies in detectors 1 and 2 respectively, ai are the cutoff parameters (Ci = 0 when |E1-E2| > ai ). The parabolas were used in the fitting because they fitted better to the experimental data. Positron annihilation with 2p electrons was fitted by

along the line E1+E2+B2p = 1022 keV, where B2p is the 2p electron binding energy [6]. Positron annihilation with 2s electrons was fitted by

along the line E1+E2+B2s = 1022 keV, where B2s is the 2s electron binding energy [6]. Positron annihilation with 1s electrons was fitted by

along the line E1+E2+B1s = 1022 keV, where B1s is the 1s electron binding energy [6]. Finally, when (E1,E2) is a point inside the circle centered at (3m0c2/2,3m0c2/2), a function given by

where

is the distance from (3m0c2/2,3m0c2/2) to (E1, E2), and was used to take into account the in-flight positron annihilation. Finally, two internal (E < Eg) and two external (E > Eg) exponential queues were included in order to simulate the non-Gaussian part of the detectors response functions. Two internal and two external ridges along the lines E1 = 511 keV and E2 = 511 keV, proportional to the peak intensity, were included in the fit. The background in channel (i,j) was empirically considered as proportional to the product of the total number of counts (peak excluded) along the lines j=constant by the total number of counts along the line i=constant; the single fitted parameter was the proportionality factor. The backscattering was described by a parabola, along the line E1+E2 = 1022 keV and centered at 511keV-511keV. Functions f1s,2s,2p,v and the four exponential queues, after summing, were convoluted with the detector response functions given by two Gaussians. The fitted parameters were A1s, A2s, A2p, Av, s1s, s2s, s2p, sv, C1,2, a1,2, a1,2, the background parameter, the peak positions in the two energy axes, the angular inclination of the E1+E2 = 1022 keV line respect to the main axes, the sixteen exponential queues parameters (eight amplitudes and eight attenuation factors), the detector resolutions, and four parameters for the ridges intensities. Differently from ref. [4], the electron binding energies were not fitted. The fit was done by using the least-squeares method. The Gauss-Marquardt method was used to consider the non-linear parameters [7],[8]. The chi-squared value was calculated by

where nij is the number of observed events in channel (i,j) of the two dimensional spectrum (Figure 2), and Fij is the fitted function (Figure 3).



IV. RESULTS AND CONCLUSION

The obtained results to the core (2p, 2s, and 1s electrons) and valence band annihilation intensities were 2.27(3)% and 97.73(3)%, respectively. The intensities obtained of literature [9] to the core and valence band were 2% and 98%, respectively. We have found that a complete analysis of the two-dimensional Doppler annihilation radiation spectrum, in the case of the silicon, is possible. Unlike the usual approach, this procedure allows the determination of the data uncertainties. Thus, hypotheses can be tested and different results can be averaged.

Ackonowledgments

We wish to acknowledge the support of Conselho Nacional de Desenvolvimento Cientí fico e Tecnológico - CNPq and Fundação de Amparo à Pesquisa do Estado de São Paulo, and the help of Dr. M. C. A. Fantini.

V. REFERENCES

Received on 15 July, 2005

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  • [2] A W Hunt, D B Cassidy, F A Selim, R Haakenaasen, T E Cowan, R H Howell, K G Lynn, and J A Golovchenko, Nucl Instr and Meth B (2000) 44.
  • [3] E do Nascimento, O Helene, V R Vanin, and C Takiya, Braz J Phys 34, 1017 (2004).
  • [4] E do Nascimento, O Helene, C Takiya, and V R Vanin, Nucl Instr Meth A 538, 723 (2005).
  • [5] N W Ashcroft, N D Mernin (1976) Solid State Physics, Saunders College Publishing, USA
  • [6] R B Firestone and V S Shirley, Table of Isotopes, eighth edition, vol II, John Willey & Son, (1996)
  • [7] V. R. Vanin, G. Kenchian, M. Moralles, O. A. M. Helene, and P. R. Pascholati, Nucl Instr Meth A 391, 338 (1997).
  • [8] D. W. Marquardt, J Soc Appll Math 11, 431 (1963).
  • [9] M Hakala, M J Puska, and R M Nieminen, Phys Rev B 57, 7621 (1998).

Publication Dates

  • Publication in this collection
    07 Nov 2005
  • Date of issue
    Sept 2005

History

  • Received
    15 July 2005
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