Total cross section measurements for positron scattering from acetone
© Brunger et al 2010
Received: 15 July 2010
Accepted: 7 October 2010
Published: 7 October 2010
We report results from total cross section measurements for positron-acetone scattering. The energy range of these experiments was 0.2-23 eV, while the energy resolution of our positron beam was ~260 meV. The present data clearly highlight the important role played by the strong permanent dipole moment and significant dipole polarisability of the acetone molecule on the low-energy scattering dynamics of this system. For positron energies above about 6 eV the present data is found to be in quite good agreement with the only other total cross section results available in the literature from the Yamaguchi group, however, at lower energies the level of agreement is rather poor. To the best of our knowledge, no theoretical calculations are currently available for positron-acetone scattering.
PACS Codes: 34.80.Uv
In our previous studies on water , tetrahydrofuran , 3-hydroxy-tetrahydrofuran  and di-hydropyran , all of which have significant permanent dipole moments (μ) and dipole polarisabilities (α) of important magnitude, we observed that for each species the total cross sections (TCSs) increased significantly in value with decreasing incident positron impact energies. In a joint collaboration with theorists, in that case for formic acid which also possesses a strong dipole moment and dipole polarisability, we were able to explicitly demonstrate  that the observed low energy behaviour of the TCSs was due to those (μ, α) physico-chemical properties of the target molecule in question. Very recently  the San Diego group has also demonstrated the important role that the dipole moment plays in enhancing positron binding to molecules, clearly indicating the crucial role that it plays in positron scattering dynamics.
In the next section we describe our experimental apparatus and measurement techniques. Thereafter the current results are presented and discussed, before some conclusions from the present study are given.
2. Experimental Details
The positron spectrometer employed at the University of Trento was developed by Zecca and co-workers, and has been described in detail many times [see e.g. [1–5]]. We therefore do not repeat those details again here, except to note that a tungsten moderator of thickness 1 μm or a nickel moderator of 2 μm was employed in conjunction with a radioactive 22Na isotope (current activity ~ 2.2 mCi) and some electrostatic optics in order to produce the positron beam. Full details on the comparative performance of these moderators can be found in Zecca et al. , with consistent TCS results being obtained in either case. Here we note that most of the present data were collected with the tungsten moderator. We further note that it is a standard practice in our laboratory, as a check for the validity of our techniques and procedures, to perform preliminary validation measurements using targets for which the positron scattering total cross sections are considered well known. Such a standard system might be drawn from the lighter rare gases  or as a consequence of our recent detailed study involving molecular nitrogen (A. Zecca, L. Chiari, A. Sarkar and M. J. Brunger: Positron scattering from the isoelectronic molecules N2, CO and C2H2, unpublished).
where I1 is the positron beam count rate at pressure P1, the pressure being measured with the acetone routed to the scattering cell, k is Boltzmann's constant, T is the temperature of the acetone vapour (K), σ is the total cross section, I0 is the positron count rate at P0, the pressure with the acetone diverted into the vacuum chamber i.e. away from the scattering cell, and L is the length of the scattering region.
For a physical application of equation (1) several crucial precautions should be taken and care must be exercised during the measurements. Those considerations include minimising double-scattering events and ensuring the TCSs are independent of pressure. In addition, only a high-purity acetone sample (> 99.8%) was used (Merck). Note that while acetone is a liquid at room temperatures, it is sufficiently volatile to be able to perform our measurements. Further note that to minimise any possible impurities affecting our measurements freeze-pump-thaw cycles were employed here.
The geometrical length of the scattering region is 22.1 ± 0.1 mm, with apertures of 1.5 mm diameter at both the entrance and exit of the scattering chamber. End effects were minimised in this study by having relatively small diameter entrance and exit apertures in the scattering chamber. As a consequence we believe their contribution to the uncertainty in the value of L is likely to be less than 0.2%. In our application of equation (1), the value of L used is always corrected to account for the path increase caused by the gyration of the positrons in the focussing axial magnetic field (~ 12 G) present in the scattering region. For the present study this led to the value of L to be increased by ~6%. From a consideration of the size of the entrance and exit apertures of our scattering cell, and their separation, the angular acceptance (Δθ) of the Trento spectrometer is ≈ 4°, which compares favourably with that from the Yamaguchi spectrometer (Δθ ≈ 7°) (C. Makochekanwa, 2010, private communication) and the Detroit spectrometer (Δθ ≈ 16°) . The gyration of the positrons can also potentially increase the angular resolution error compared to the no-field case . Using some of the analytic formulae detailed in Kauppila et al. , but for the typical experimental conditions of our measurements, estimates of the energy-dependent angular discrimination can be obtained. We found that they varied from ~17° at 1 eV positron energy to ~5.4° at 10 eV. This can also be corrected for, provided appropriate absolute elastic differential cross sections (theory or experimental) are available. Unfortunately, such differential cross sections are not usually available so that the TCSs we report here represent a lower bound on the exact values. We shall return to this point again in the next section.
It is very important for the energy scale to be calibrated accurately. The zero for the energy scale, in the absence of the target gas, was determined in this investigation with a retarding potential analysis of the positron beam . We now believe that the error in our energy scale is of the order of ± 0.1 eV. Measurements repeated during the last 3-4 years show a surprising stability in the energy zero (variance < 0.05 eV) when using the tungsten moderator. Similar measurements performed on nickel moderators show a comparable stability. The same measurements allow us to evaluate an energy width of the positron beam of ~260 meV with an uncertainty on this determination of at most 100 meV. This value refers to the predominant case of measurements being made with the tungsten moderator. It is also crucial to accurately measure the scattering cell pressure, which we achieve with a MKS 627B capacitance manometer operated at 45 °C. As the manometer temperature was different to that for the target gas in the scattering cell, thermal transpiration corrections to the pressure readings are made using the model of Takaishi and Sensui . Typically this led to a maximum correction on the TCS of 3.3%. One final caveat on the data we report here should be noted. All the experimental data are convoluted with the finite energy resolution of our positron beam (~260 meV), although the effect of this on the measured TCSs is most manifest at positron energies below ~0.5 eV which coincides with where the slope of the TCS as a function of energy is also greatest. In practice this physically implies that, when corrected for this effect, our lowest energy TCSs should be somewhat higher in magnitude than what we present here.
Present total cross sections (×10-20m2) for positron scattering from acetone
3. Results and discussion
Considering figure 2 in more detail we immediately observe that the anticipated low energy behaviour, based on our earlier work [1–5], is indeed found. Namely the magnitude of the TCS increases significantly as the positron impact energy decreases. It is known that the first (direct) ionisation energy of acetone is at 9.71 eV [19, 20], implying a positronium formation threshold energy of 2.91 eV for this molecule . Our TCS is seen to monotonically decrease in value with increasing positron energy, until at about 3 eV where there is a change in slope which we believe is consistent with the positronium formation channel opening. A small structure, which was persistently seen during the many crosscheck measurements we made, is also observed at around 4-5 eV. We do not ascribe this small structure to any possible positron binding to the molecule, rather we suggest that it might reflect the opening of one or more of the electronic states of acetone. Thereafter, the TCS again decreases as the energy increases until the opening of the direct ionisation channel.
There are two previous measurements [11, 12] against which we can compare the present data, both of which originate from Yamaguchi University. To within the combined uncertainties on the respective data sets, for energies greater than about 6 eV, the present TCSs are in good accord with those from Hamada et al.  while those from Kimura et al.  are a little higher in magnitude. However, as you go to lower positron energies, the discrepancies between the current results and those from the Yamaguchi group [11, 12] become progressively worse. For example at 1 eV the present TCS is a factor of ~4 larger than that of Hamada et al. and a factor of ~3.5 larger that that of Kimura et al. . We note that a similar effect was recently reported by Szmytkowski  in his measurements of total cross sections for electrons scattering from acetone, when he compared his data to corresponding results from Yamaguchi University . Makochekanwa et al.  recently demonstrated, using theoretical elastic differential cross sections, that for polar molecules the forward angle scattering corrections at low positron energies could be as large as 67%. Assuming the energy-dependent angular resolution of the Trento apparatus is superior to that of the Yamaguchi spectrometer, which might be reasonable given their apparatus configuration, this effect would explain at least some of the differences between the TCS measurements we see in figure 2. Nonetheless, given the severity of the discrepancies between the Trento and Yamaguchi data below 6 eV, we believe the forward angle scattering effect is unlikely to explain all the differences. As a consequence we believe this scattering system would benefit from a further independent experimental study or theoretical investigation (M. H. F. Bettega, 2010, private communication).
We have reported new total cross section measurements for positron scattering from acetone. The effect of the target molecular dipole moment and dipole polarisability on the scattering dynamics is manifest, particularly at the lower positron impact energies. Indeed when coupled with the recent findings from the San Diego group , we see a clear picture emerging for the pivotal role the molecular dipole moment plays in these systems. Agreement with the previous data from Hamada et al.  at energies above 6 eV was satisfactory, while significant discrepancies with those data and the results from Kimura et al.  at the lower energies were noted. Some of those discrepancies, but not all, we believe are due to the more significant forward angle scattering corrections that need to be applied to the Yamaguchi data compared to the present. We reiterate that a theoretical study of this scattering would be welcome.
This work was supported in part by the Australian Research Council through its Centres of Excellence Programme. We all thank Dr L. Campbell for his help in the preparation of this paper. A.S. also thanks the International Centre for Theoretical Physics - TRIL Program (Italy) for supporting his stay, while M.J.B. thanks the Department of Innovation, Industry, Science and Research for support through their International Science Linkages program. Finally L.C. acknowledges the Provincia Autonoma di Bolzano (Italy) for financial support.
- Zecca A, Sanyal D, Chakrabarti M, Brunger MJ: J Phys B. 2006, 39: 1597-10.1088/0953-4075/39/7/004.View ArticleADSGoogle Scholar
- Zecca A, Perazzolli C, Brunger MJ: J Phys B. 2005, 38: 2079-10.1088/0953-4075/38/13/002.View ArticleADSGoogle Scholar
- Zecca A, Chiari L, Sarkar A, Brunger MJ: J Phys B. 2008, 41: 085201-10.1088/0953-4075/41/8/085201.View ArticleADSGoogle Scholar
- Zecca A, Chiari L, Nixon KL, Brunger MJ, Chattopadhyay S, Sanyal D, Chakrabarti M: J Phys Chem A. 2009, 113: 14251-10.1021/jp9024602.View ArticleGoogle Scholar
- Zecca A, Chiari L, Sarkar A, Lima MAP, Bettega MHF, Nixon KL, Brunger MJ: Phys Rev A. 2008, 78: 042707-10.1103/PhysRevA.78.042707.View ArticleADSGoogle Scholar
- Danielson JR, Gosselin JJ, Surko CM: Phys Rev Lett. 2010, 104: 233201-10.1103/PhysRevLett.104.233201.View ArticleADSGoogle Scholar
- Lide DR: CRC Handbook of Chemistry and Physics. 2002, Boca Raton, FL, USA: CRC Press, 83Google Scholar
- Iwata K, Greaves RG, Murphy TJ, Tinkle MD, Surko CM: Phys Rev A. 1995, 51: 473-10.1103/PhysRevA.51.473.View ArticleADSGoogle Scholar
- Nadykto AB, Yu F: J Geophys Res. 2003, 108: 4717-10.1029/2003JD003664.View ArticleGoogle Scholar
- Vadena TD, Lisy JM: Chem Phys Lett. 2005, 408: 54-10.1016/j.cplett.2005.04.002.View ArticleADSGoogle Scholar
- Hamada A, Sueoka O, Takaki H, Kimura M: Bull Phys Soc Japan. 1997, 52: 876-Google Scholar
- Kimura M, Sueoka O, Itikawa Y: American Institute of Physics Conference Proceedings. 2000, 500: 284-296.ADSGoogle Scholar
- Zecca A, Chiari L, Sarkar A, Chattopadhyay S, Brunger MJ: Nucl Instrum Methods B. 2010, 268: 533-536. 10.1016/j.nimb.2009.11.013.View ArticleADSGoogle Scholar
- Jones A, Caradonna P, Makochekanwa C, Slaughter D, Mueller D, Sullivan JP, Buckman SJ: J Phys Conf Ser. 2009, 194: 012033-10.1088/1742-6596/194/1/012033.View ArticleADSGoogle Scholar
- Kauppila WE, Stein TS, Smart JH, Dababneh MS, Ho YK, Downing JP, Pol V: Phys Rev A. 1981, 24: 725-10.1103/PhysRevA.24.725.View ArticleADSGoogle Scholar
- Hamada A, Sueoka O: J Phys B. 1994, 27: 5055-10.1088/0953-4075/27/20/019.View ArticleADSGoogle Scholar
- Zecca A, Brunger MJ: Nanoscale Interactions and Their Applications: Essays in Honour of Ian Mc Carthy. Edited by: Wang F, Brunger MJ. 2007, Trivandrum, India: Research Signpost, 21-26.Google Scholar
- Takaishi T, Sensui Y: Trans Faraday Soc. 1963, 59: 2503-2514. 10.1039/tf9635902503.View ArticleGoogle Scholar
- Snyder EM, Buzza SA, Castleman AW: Phys Rev Lett. 1996, 77: 3347-10.1103/PhysRevLett.77.3347.View ArticleADSGoogle Scholar
- Traeger JC, McLouglin RG, Nicholson AJC: J Am Chem Soc. 1982, 104: 5318-10.1021/ja00384a010.View ArticleGoogle Scholar
- Surko C, Gribakin G, Buckman SJ: J Phys B. 2005, 38: R57-10.1088/0953-4075/38/6/R01.View ArticleADSGoogle Scholar
- Szmytkowski C: J Phys B: At Mol Opt Phys. 2010, 43: 055201-10.1088/0953-4075/43/5/055201.View ArticleADSGoogle Scholar
- Kimura M, Sueoka O, Hamada A, Itikawa Y: Adv Chem Phys. 2000, 111: 537-full_text.Google Scholar
- Makochekanwa C, Bankovic A, Tattersall W, Jones A, Caradonna P, Slaughter DS, Nixon K, Brunger MJ, Petrovic Z, Sullivan JP, Buckman SJ: New J Phys. 2009, 11: 103036-10.1088/1367-2630/11/10/103036.View ArticleGoogle Scholar
This article is published under license to BioMed Central Ltd. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/2.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.