Solvation of atomic fluorine in bulk superfluid ⁴He

Bosonic density functional theory calculations were carried out for fluorine atom solvated in superfluid ⁴He with an emphasis on the formation of dimeric species in the liquid. Atomic fluorine displays a relatively strong binding and anisotropic interaction with helium and hence the resulting solvat...

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Дата:2011
Автор: Eloranta, J.
Формат: Стаття
Мова:English
Опубліковано: Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України 2011
Назва видання:Физика низких температур
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Цитувати:Solvation of atomic fluorine in bulk superfluid ⁴He / J. Eloranta // Физика низких температур. — 2011. — Т. 37, № 5. — С. 491–493. — Бібліогр.: 18 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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spelling irk-123456789-1185682017-05-31T03:08:15Z Solvation of atomic fluorine in bulk superfluid ⁴He Eloranta, J. 8th International Conference on Cryocrystals and Quantum Crystals Bosonic density functional theory calculations were carried out for fluorine atom solvated in superfluid ⁴He with an emphasis on the formation of dimeric species in the liquid. Atomic fluorine displays a relatively strong binding and anisotropic interaction with helium and hence the resulting solvation structure contains highly localized liquid helium layers. These solvent layers modify the gas phase dimer potentials by inclusion of a recombination barrier, which provides stabilization for the solvated fluorine atoms. At 0 K and saturated vapor pressure, the recombination barrier for the formation of molecular fluorine (²Σ⁺g) in superfluid helium is predicted to be 26.8 K. At temperatures below 1 K, this barrier prevents the F–F recombination as all the other electronic states correlating with the ground state atoms are essentially repulsive. It is concluded that it should be possible to stabilize fluorine atoms in superfluid helium below 1 K temperatures. 2011 Article Solvation of atomic fluorine in bulk superfluid ⁴He / J. Eloranta // Физика низких температур. — 2011. — Т. 37, № 5. — С. 491–493. — Бібліогр.: 18 назв. — англ. 0132-6414 PACS: 36.40.Mr, 67.25.D– http://dspace.nbuv.gov.ua/handle/123456789/118568 en Физика низких температур Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
topic 8th International Conference on Cryocrystals and Quantum Crystals
8th International Conference on Cryocrystals and Quantum Crystals
spellingShingle 8th International Conference on Cryocrystals and Quantum Crystals
8th International Conference on Cryocrystals and Quantum Crystals
Eloranta, J.
Solvation of atomic fluorine in bulk superfluid ⁴He
Физика низких температур
description Bosonic density functional theory calculations were carried out for fluorine atom solvated in superfluid ⁴He with an emphasis on the formation of dimeric species in the liquid. Atomic fluorine displays a relatively strong binding and anisotropic interaction with helium and hence the resulting solvation structure contains highly localized liquid helium layers. These solvent layers modify the gas phase dimer potentials by inclusion of a recombination barrier, which provides stabilization for the solvated fluorine atoms. At 0 K and saturated vapor pressure, the recombination barrier for the formation of molecular fluorine (²Σ⁺g) in superfluid helium is predicted to be 26.8 K. At temperatures below 1 K, this barrier prevents the F–F recombination as all the other electronic states correlating with the ground state atoms are essentially repulsive. It is concluded that it should be possible to stabilize fluorine atoms in superfluid helium below 1 K temperatures.
format Article
author Eloranta, J.
author_facet Eloranta, J.
author_sort Eloranta, J.
title Solvation of atomic fluorine in bulk superfluid ⁴He
title_short Solvation of atomic fluorine in bulk superfluid ⁴He
title_full Solvation of atomic fluorine in bulk superfluid ⁴He
title_fullStr Solvation of atomic fluorine in bulk superfluid ⁴He
title_full_unstemmed Solvation of atomic fluorine in bulk superfluid ⁴He
title_sort solvation of atomic fluorine in bulk superfluid ⁴he
publisher Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України
publishDate 2011
topic_facet 8th International Conference on Cryocrystals and Quantum Crystals
url http://dspace.nbuv.gov.ua/handle/123456789/118568
citation_txt Solvation of atomic fluorine in bulk superfluid ⁴He / J. Eloranta // Физика низких температур. — 2011. — Т. 37, № 5. — С. 491–493. — Бібліогр.: 18 назв. — англ.
series Физика низких температур
work_keys_str_mv AT elorantaj solvationofatomicfluorineinbulksuperfluid4he
first_indexed 2025-07-08T14:15:10Z
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fulltext © J. Eloranta, 2011 Fizika Nizkikh Temperatur, 2011, v. 37, No. 5, p. 491–493 Solvation of atomic fluorine in bulk superfluid 4He J. Eloranta Department of Chemistry and Biochemistry, California State University, Northridge 18111 Nordhoff St., Northridge, CA 91330, USA E-mail: Jussi.Eloranta@csun.edu Received December 1, 2010 Bosonic density functional theory calculations were carried out for fluorine atom solvated in superfluid 4He with an emphasis on the formation of dimeric species in the liquid. Atomic fluorine displays a relatively strong binding and anisotropic interaction with helium and hence the resulting solvation structure contains highly loca- lized liquid helium layers. These solvent layers modify the gas phase dimer potentials by inclusion of a recombi- nation barrier, which provides stabilization for the solvated fluorine atoms. At 0 K and saturated vapor pressure, the recombination barrier for the formation of molecular fluorine ( 2 g +Σ ) in superfluid helium is predicted to be 26.8 K. At temperatures below 1 K, this barrier prevents the F–F recombination as all the other electronic states correlating with the ground state atoms are essentially repulsive. It is concluded that it should be possible to sta- bilize fluorine atoms in superfluid helium below 1 K temperatures. PACS: 36.40.Mr Spectroscopy and geometrical structure of clusters; 67.25.D– Superfluid phase. Keywords: bulk superfluid helium, fluorine, quantum gel, solvation. 1. Introduction Solvation of atomic and molecular impurities in bulk superfluid 4He has been a subject to a number of experi- mental and theoretical studies [1–5]. On the experimental side absorption and fluorescence spectroscopy of solvated atoms have provided detailed information about the solvent structure surrounding the atomic impurities. Depending on the characteristics of the impurity–helium interaction, the resulting solvation structures can be classified according to two different ideal limits. The “bubble” structure is ob- served for impurities with mostly repulsive interaction with helium (e.g., alkali metal atoms) whereas the “snowball” structure forms around impurities exhibiting strongly bound potentials towards helium (e.g., ions). The strongly bound helium layer around the latter impurities often exhi- bits helium densities that approach the solid helium densi- ty. It was shown recently that such high-density solvent layers around atomic impurities may have important impli- cations for the impurity recombination processes in the liquid [6]. As two impurities surrounded by high-density helium approach each other in the liquid, the gas phase interaction potential is altered mainly due to the repulsive interaction between the solvent layers on the two different centers. This effect was observed experimentally for the first time for doubly doped Mg containing helium droplets [7]. A theoretical investigation employing the bosonic den- sity functional theory later confirmed the interpretation of the experimental results [8]. In bulk superfluid helium ex- periments, it is possible to accumulate a large number of impurity centers in the sample, which may then lead to the formation of macroscopic size quantum gel-type structures [6]. It has been established that this type of structures are not related to the well-known impurity helium solids dis- covered by Gordon et al. [6,9,10]. Up to date no experi- mental observation of such quantum gel formation in the bulk has been published in the literature. To further eluci- date the possible formation of quantum gel structures in the bulk, this study explores the solvation of fluorine atoms in bulk superfluid helium and provides estimates for the sol- vent layer induced energy barrier for F–F molecular re- combination. 2. Theory The applied density functional theory (DFT) to model bulk superfluid 4He and the numerical implementation has been described previously [11–14]. The ground state solu- tion was obtained by the imaginary time propagation me- thod using variable time steps to speed up the convergence. The DFT model also included the high density corrections [12] to properly account for liquid localization in the bound parts of the fluorine–helium potential. For calcula- tions at nonzero temperatures, the thermal DFT approach of Toigo et al. was used [15]. All calculations employed J. Eloranta 492 Fizika Nizkikh Temperatur, 2011, v. 37, No. 5 pair potentials based on the published ab initio data [16– 18]. Since the calculations were carried out in a finite 3D box, the number of helium atoms varied slightly depending on the positions of the fluorine atoms and the surrounding solvent layers. This was accounted for by normalizing the system to a constant number of helium atoms and then correcting the total energy appropriately. The zero-point spread for the solvated fluorine was included in the calcu- lation by first optimizing its nuclear wavefunction along- side with the superfluid helium. The resulting fluorine atom density was nearly Gaussian with a full width at half height of 1.05 Bohr. In the subsequent calculations with multiple fluorine atoms their nuclear wavefunctions were kept fixed during the imaginary time propagation as the atomic centers are located far away from each other ensur- ing a minimal overlap between the nuclear wavefunctions. 3. Results and discussion The formation of molecular fluorine in superfluid he- lium presents an interesting system because the atomic fluorine has a 2P ground state and as such it exhibits an anisotropic interaction with the surrounding helium. Sub- sequently the dynamic Jahn–Teller effect should lead to a nonspherical solvation structure. It was recently discovered that the F2 2 g +Σ ground state potential has an unusual hump around 7.3 Bohr with an approximate height of 12 K in the gas phase [17,18]. When this molecular recombina- tion barrier is augmented with the solvent layer induced barrier, the effect becomes even more pronounced as de- monstrated in Fig. 1. In superfluid helium ( < 2.17T K), a barrier of 26.8 K is significant and should hinder thermally induced recombination of fluorine atoms towards F2 2( )g +Σ . Note that all the other states correlating with the ground state atoms are essentially repulsive and therefore only the ground state could lead to the formation of chemi- cally bound F2. By using the thermal DFT model, the effect of tempera- ture on the solvent induced recombination barrier was cal- culated. However, since the liquid structure is dominated by the fluorine–helium pair potential, the thermal effects up to 3 K were found to be very small (less than 3 K). On the other hand, the effect of increased pressure is more pronounced as the higher liquid density strongly amplifies the structure of the bound solvent layers and consequently the solvent layer induced recombination barrier becomes higher (see Fig. 2). At bulk liquid densities higher than 02.5ρ , where 0ρ is the superfluid helium density at 0 K (0.0218360 Å–3), a strongly inhomogeneous solid helium structure forms around the fluorine atoms. Due to the li- mited size of the simulation cube, it was not possible to study this region in detail at present. Ideally the atomic mobility would be greatly diminished in the limit of solid helium. To understand the dynamics of thermal diffusion in- duced recombination of fluorine atoms in superfluid he- lium better, it is instructive to provide estimates for the second order rate constant for this process (i.e., [ ] [ ]22F / = Fd dt k− where [ ]F is the fluorine atom con- centration and 2k is the 2nd order recombination rate con- stant). For reactive collisions, this can be estimated from ( )2 = * 8 / exp /A ak kT N E RTσ πμ − where *σ is the re- active cross-section (estimate 23·10−≈ m2 with a reactive diameter of 3 Å and a steric factor of 1/9), k is the Boltzmann constant, μ is the fluorine atomic mass, AN is the Avogadro's constant, aE is the solvent layer barrier height, and R is the gas constant. Under saturated vapor pressure conditions, the resulting temperature dependency for 2k is shown in Fig. 3. After the temperature exceeds the lambda point, the exponential term leads to a rapid in- crease in 2k as temperature increases. The fluorine atom Fig. 1. F–F recombination potential in superfluid helium (1 g +Σ ). 5 10 15 F–F distance, Bohr –40 –20 0 20 E , K Erc = 26.8 K 20 Fig. 2. F–F recombination potential barrier height as a function of bulk liquid density. 0ρ represents the bulk liquid density at 0 K (see text). 0.5 1.0 1.5 2.0 2.5 20 25 30 35 40 ρ0 B ar ri er h ei g h t, K Solvation of atomic fluorine in bulk superfluid 4He Fizika Nizkikh Temperatur, 2011, v. 37, No. 5 493 concentration as a function of time at selected temperatures are plotted in Fig. 4. Below approximately 1 K tempera- ture, the recombination kinetics is very slow allowing for fluorine atom buildup in bulk superfluid helium. 4. Conclusions The present DFT calculations predict that the F–F mo- lecular recombination barrier is sufficiently high so that isolated fluorine atoms can be stabilized in bulk superfluid helium below 1 K temperature. Financial support from the National Science Foundation grant CHE-0949057 is gratefully acknowledged. 1. J.P. Toennies and A.F. Vilesov, Annu. Rev. Phys. Chem. 49, 1 (1998). 2. A. Hernando, R. Mayol, M. Pi, M. Barranco, F. Ancilotto, O. Bünermann, and F. Stienkemeier, J. Phys. Chem. A111, 7303 (2007). 3. Q. Hui and M. Takami, J. Low Temp. Phys. 119, 393 (2000). 4. T. Kinoshita, K. Fukuda, Y. Takahashi, and T. Yabuzaki, Phys. Rev. A52, 2707 (1995). 5. B. Tabbert, M. Beau, H. Günther, W. Häussler, C. Hönninger, K. Meyer, B. Plagemann, and G. zu Putlitz, Z. Phys. B97, 425 (1995). 6. J. Eloranta, Phys. Rev. B77, 134301 (2008). 7. A. Przystawik, S. Göde, T. Döppner, J. Tiggesbäumker, and K.-H. Meiwes-Broer, Phys. Rev. A78, 021202 (2008). 8. A. Hernando, M. Barranco, R. Mayol, M. Pi, and F. Ancilotto, Phys. Rev. B78, 184515 (2008). 9. E.B. Gordon, L.P. Mezhov-Deglin, and O.F. Pugachev, JETP Lett. 19, 63 (1974). 10. E.B. Gordon and A.F. Shestakov, Fiz. Nizk. Temp. 26, 5 (2000) [Low Temp. Phys. 26, 1 (2000)]. 11. F. Dalfovo, A. Lastri, L. Pricaupenko, S. Stringari, and J. Treiner, Phys. Rev. B52, 1193 (1995). 12. F. Ancilotto, M. Barranco, F. Gaupin, R. Mayol, and M. Pi, Phys. Rev. B72, 214522 (2005). 13. L. Lehtovaara, J. Toivanen, and J. Eloranta, J. Comp. Phys. 221, 148 (2007). 14. L. Lehtovaara, T. Kiljunen, and J. Eloranta, J. Comp. Phys. 194, 78 (2004). 15. F. Ancilotto, F. Faccin, and F. Toigo, Phys. Rev. B62, 17036 (2000). 16. H. Partridge, J.R. Stallcop, and E. Levin, J. Chem. Phys. 115, 6471 (2001). 17. L. Bytautas and K. Ruedenberg, J. Chem. Phys. 130, 204101 (2009). 18. F.A. Evangelista, E. Prochnow, J. Gauss, and H.F. Schaefer III, J. Chem. Phys. 132, 074107 (2010). Fig. 3. Temperature dependence of the 2nd order recombination rate constant 2k predicted by collision theory. 0 0.5 1.0 1.5 2.0 T, K 1 2 3 4 k 2 , 1 0 d m /( m o l· s) 6 3 Fig. 4. Concentration of fluorine atoms [ ]F as a function of time at selected temperatures. The atoms are stabilized below 1 K temperature. 0 0.2 0.4 0.6 0.8 1.0 2 4 6 8 0.4 K 0.6 K 0.8 K 1.0 K 1.2 K [F ] , m o l/ d m 3 Time, 10 s 3 10