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Photoionization of atoms and ions from endohedral anions

V. K. Dolmatov vkdolmatov@una.edu Department of Chemistry and Physics, University of North Alabama, Florence, Alabama 35632, USA    L. V. Chernysheva Ioffe Institute, 194021 St.Petresburg, Russia, larissa.chernysheva@mail.ioffe.ru    V. G. Yarzhemsky Kurnakov Institute of General and Inorganic Chemistry of RAS, 119991, Moscow, Russia; vgyar@igic.ras.ru
Abstract

We study the interconnection between the results of two qualitatively different approximate calculations of photoionization cross sections, σn\sigma_{n\ell}, for neutral atoms (AA) or their cations (A+A^{+}), centrally confined inside a fullerene-anion shell, CNqC_{N}^{q} , where qq represents the negative excess charge on the shell. One of the approximations, frequently employed in previous studies, assumes a uniform excess negative charge distribution over the entire fullerene shell, by analogy with a charged metallic sphere. The other approximation, not previously discussed in the literature, considers the quantum states of the excess electrons on the shell, determined by specific nn and \ell values of their quantum numbers. Remarkably, both methods yield photoionization cross sections for the encapsulated species that are close to each other. Consequently, we find that the photoionization of the encapsulated atoms or cations inside a CNqC_{N}^{q} anion is minimally influenced by the quantum states of the excess electrons on the fullerene shell. Furthermore, we demonstrate that the aforementioned influence decreases even further with an increasing size of the confining fullerene shell. All this holds true at least under the assumption that the confined atom or cation is compact, i.e., its electron density remains primarily within itself rather than being drawn into the fullerene shell. This remarkable finding results from Hartree-Fock calculations combined with a popular modeling of the fullerene shell, where it is modeled by an attractive spherical annular potential.

I Introduction

Among various theoretical studies on photoionization of atoms, AA, and ions (cations), A+A^{+}, confined inside a negatively or positively charged fullerene shell, CqN{}_{N}^{q} (qq is a charge on the fullerene cage: q=±|q|q=\pm|q| and NN is the number of carbon atoms making the fullerene cage/shell; throughout the rest of the paper, we will use the terms “shell” and “cage” interchangeably), a noticeable body of research results has been obtained within the framework of a simple semi-empirical model DolmMansPRA2006 ; DolmCravenPRA2009 ; LudlowJPB2010 ; KumarVarmaJPCS2015 ; KumarVarmaPRA2016 ; EPJD2016 ; JChemPhys2017 ; VarmaPRA2020 ; VarmaJPB2021 ; VarmaPhysSCR2021 ; DubeyJPB2021 ; CJP2022 ; VarmaPRA2023 . The key assumption inherent in the model is that the excess charge qq on CqN{}_{N}^{q} is uniformly spread over the entire outer surface of the fullerene cage in a direct analogy to a metallic sphere.

In the present paper, we investigate the validity of such assumption in relation to the photoionization process of a neutral atom, AA, or its cation, A+A^{+}, confined inside a fullerene anion, designated as A@CNqA@{\rm C}_{N}^{q} or A+@CNqA^{+}@{\rm C}_{N}^{q} (q<0q<0), respectively.

There are good reasons for such study. Firstly, said approximation neglects to account for the actual quantum state(s) of the excess electron(s) on the fullerene cage, such as the electrons’ principal, nn, and orbital, \ell, quantum numbers. Secondly, in that approximation, the electron density of the excess electron(s) on the shell is uniformly distributed, as has already been mentioned, exclusively along the outer surface of the fullerene shell. Meanwhile, it is known, see, e.g., Lohr ; ABK98 ; Dolm2020 ; Dolm2022 that the excess electron density does spread inside the hollow interior of the fullerene as well. Consequently, the question arises: how will the calculation results obtained within the former model change if one takes into account both the quantum states and the spread of the electron density of excess electrons from the shell into its interior? To the best of our knowledge, such study has not been conducted to date, leaving the question open. We address this question by providing the answer obtained from the research described in the present paper.

To meet the goal, and also to ensure the adequacy for comparing results obtained in both the framework of the former model and the improved model, suggested in the present paper, we retain the same semi-empirical modeling of a neutral CN shell as in the aforementioned previous studies. However, instead of uniformly spreading the excess charge over the neutral shell, we suggest a way to account for the quantum states of the excess charge in AA@CqN{}_{N}^{q} [here and throughout the paper, AA stands for either a neutral atom or a positive ion (cation), for brevity].

Surprisingly, we find that the photoionization of the encapsulated atoms or cations inside a CqN{}_{N}^{q} anion is minimally influenced by the quantum states of the excess electrons on the fullerene shell. Moreover, we demonstrate that said influence decreases with an increasing size of the confining fullerene shell, from C60 to the giant C240, in our study. Our findings hold true at least under the assumption that the confined atom is compact, i.e., its electron density remains primarily within the atom itself rather than being noticeably drawn into the fullerene shell.

We choose the hydrogen atom, H, as well as the He atom and its ion He+ as species to be confined inside a fullerene anion, as a case study.

Atomic system of units (a.u.) (|e|=me==1|e|=m_{\rm e}=\hbar=1, where ee and mem_{\rm e} are the electron’s charge and mass, respectively, is used throughout the paper unless specified otherwise.

II Theory

II.1 Review of the former modeling of AA@CqN{}_{N}^{q}

The quintessence of the model is as follows.

Firstly, a neutral CN cage is modeled by a UC(r)U_{\rm C}(r) spherical annular, i.e., rectangular in the radial coordinate potential of a certain inner radius, r0r_{0}, thickness, Δ\Delta, and depth, U0U_{0}:

UC(r)={U0,if r0rr0+Δ0,otherwise.\displaystyle U_{\rm C}(r)=\left\{\begin{array}[]{ll}-U_{0},&\mbox{if $r_{0}\leq r\leq r_{0}+\Delta$}\\ 0,&\mbox{otherwise.}\end{array}\right. (3)

Such modeling of a CN cage was apparently first proposed by Puska and Nieminen PuskaPRA93 . Later, it was widely used in numerous theoretical studies on photoionization and other elementary processes involving endohedral fullerenes (also referred to as endohedral atoms/ions in this paper), AA@CN. The reader is referred to the works cited above, as well as, for example, to a relatively recent review DeshmukhEPJD2021 on these topics).

Secondly, following the work DolmMansPRA2006 , the effect of the charged shell CqN{}_{N}^{q} on elementary atomic processes involving fullerene anions, AA@Cq<0N{}_{N}^{q<0}, is taken into account by a uniform distribution of the excess charge qq over the entire outer surface of the CN cage. This leads to the appearance of an additional Coulomb spherical potential, Vq(r)V_{q}(r), both inside and outside the fullerene cage:

Vq(r)={qr0+Δ,if 0rr0+Δqr,otherwise.\displaystyle V_{q}(r)=\left\{\begin{array}[]{ll}\frac{q}{r_{0}+\Delta},&\mbox{if $0\leq r\leq r_{0}+\Delta$}\\ \frac{q}{r},&\mbox{otherwise.}\end{array}\right. (6)

Consequently, the entire model potential, UCq(r)U_{\rm C}^{q}(r), for a charged CqN{}_{N}^{q} cage, is taken as the sum of the two potentials: UC(r)U_{\rm C}(r) [Equation (3)], and Vq(r)V_{q}(r) [Equation (6)]. That is,

UCq(r)=UC(r)+Vq(r).\displaystyle U_{\rm C}^{q}(r)=U_{\rm C}(r)+V_{q}(r). (7)

Next, to address the calculation of the structure and spectra of the encaged atom/ion, AA, in the endohedral fullerene anion, AA@CqN{}_{N}^{q}, the Vq(r)V_{q}(r) potential is added to the Shrödinger equation (for a single-electron atom), or to the Hartree-Fock, or the relativistic Dirac-Fock equations, or to the equations of other kinds of approximations for a multielectron atom.

For instance, the thus modified non-relativistic Hartree-Fock equation, applicable to AA@CqN{}_{N}^{q}, is as follows:

[Δ2Zr+UCq(r)]ψi(r)+j=1NAψj(r)|rr|\displaystyle\left[-\frac{\Delta}{2}-\frac{Z}{r}+U_{\rm C}^{q}(r)\right]\psi_{i}({\vec{r}})+\sum_{j=1}^{N_{A}}\int{\frac{\psi^{*}_{j}({\vec{r}}^{\prime})}{|{\vec{r}}-{\vec{r}}^{\prime}|}}
×[ψj(r)ψi(r)ψi(r)ψj(r)]dr=ϵiψi(r).\displaystyle\times[\psi_{j}({\vec{r}}^{\prime})\psi_{i}({\vec{r}})-\psi_{i}({\vec{r}}^{\prime})\psi_{j}({\vec{r}})]d{\vec{r}}^{\prime}=\epsilon_{i}\psi_{i}({\vec{r}}). (8)

Here, NAN_{A} is the number of electrons in the multielectron atom AA, ii (and, similar, jj) denotes the set of the principal (nin_{i}), orbital (i\ell_{i}), magnetic (mim_{\ell_{i}}) and spin-magnetic (msim_{s_{i}}) quantum numbers for the ii-th atomic electron in AA@CqN{}_{N}^{q}. For the continuum spectrum of the ii’s electron, ϵi\epsilon_{i} is to be replaced by the energy of the continuum spectrum, ϵ\epsilon. Furthermore, the function ψniimi(r)\psi_{n_{i}\ell_{i}m_{\ell_{i}}}({\vec{r}}) of the ii’s electron admits a separable representation: ψniimi(r)=r1Pnii(r)Yimi(θ,ϕ)\psi_{n_{i}\ell_{i}m_{\ell_{i}}}({\vec{r}})=r^{-1}P_{n_{i}\ell_{i}}(r)Y_{\ell_{i}m_{\ell_{i}}}(\theta,\phi).

We will frequently refer to such model of the fullerene anion as “structureless” model or approximation in this paper, to underline that it ignores possible quantum states of the excess electronic charge on the cage.

Next, the dipole photoionization cross section, σn\sigma_{n\ell}, of a nn\ell-subshell of the encapsulated atom is calculated using the standard formula (see, e.g., Amusia_book ):

σn(ω)=4πα2Nn3(2l+1)ω[lD12+(+1)D+12].\displaystyle\sigma_{n\ell}(\omega)=\frac{4\pi{{}^{2}}\alpha N_{n\ell}}{3(2l+1)}\omega[lD_{\ell-1}^{2}+(\ell+1)D_{\ell+1}^{2}]. (9)

Here, ω\omega is the photon energy, α\alpha is the fine structure constant, NnN_{n\ell} is the number of electrons in the nn\ell subshell, Dl±1D_{l\pm 1} is a radial dipole photoionization amplitude,

D±1=0Pϵ±1(r)rPn(r)𝑑r.\displaystyle D_{\ell\pm 1}=\int_{0}^{\infty}{P_{\epsilon\ell\pm 1}(r)rP_{n\ell}(r)dr}. (10)

II.2 Accounting for quantum states of the excess electrons in AA@CqN{}_{N}^{q}

In our modeling of A@CqN{}_{N}^{q}, the extra electron(s) in the A@CqN{}_{N}^{q} fullerene anion is(are) bound by the central field which is the sum of the fields of the atom and neutral CN cage. Therefore, the excess electronic states are characterized by quantum numbers nn and \ell. Let us designate such endohedral fullerene anions as A@C(n)Nq{}_{N}^{q}(n\ell) or A@C(n,n)Nq{}_{N}^{q}(n\ell,n^{\prime}\ell^{\prime}) and so on, depending on how many excess electrons exist and how many different nn\ell-states they occupy in the fullerene anion. For example, He@C(2s)N1{}_{N}^{-1}(2s) means that the single attached electron resides in a 2s2s state on the singly-charged fullerene shell, He@C(2s2p)N2{}_{N}^{-2}(2s2p) indicates that one of the two attached electrons in the doubly-charged anion is in a 2s2s state and the other electron is in a 2p2p state, and so on.

To account for the nn\ell-structure of the excess electronic charge in the anion and, at the same time, retain the spirit of the semi-empirical framework for modeling the fullerene cage, we follow the methodology outlined in Dolm2020 . The essence of the latter is as follows.

The A@C(n,)Nq{}_{N}^{q}(n\ell,...) system is a complete (or “single”) system in the sense that the state(s) of the attached electron(s) is(are) affected by the field of the encapsulated atom, whereas the states of the atomic electrons, in turn, are affected by both the field of the cage itself, UC(r)U_{\rm C}(r), and by the field(s) of the attached electron(s). To account for the mutuality of the states of the atomic electrons and those of the excess electrons on the fullerene cage, we simply solve, simultaneously, a system of the NtotN_{tot} Hartree-Fock equations for the “atom + fullerene anion” system, where Ntot=NA+NqN_{tot}=N_{A}+N_{q}, with NqN_{q} being the number of the excess electrons on the fullerene cage, and NAN_{A} the number of the electrons in the encapsulated atom.

[Δ2Zr+UC(r)]ψi(r)+j=1Ntotψj(r)|𝒓r|\displaystyle\left[-\frac{\Delta}{2}-\frac{Z}{r}+U_{\rm C}(r)\right]\psi_{i}({\vec{r}})+\sum_{j=1}^{N_{\rm tot}}\int{\frac{\psi^{*}_{j}({\vec{r}}^{\prime})}{|{\bm{r}}-{\vec{r}}^{\prime}|}}
×[ψj(r)ψi(r)ψi(r)ψj(r)]dr=ϵiψi(r).\displaystyle\times[\psi_{j}({\vec{r}}^{\prime})\psi_{i}({\vec{r}})-\psi_{i}({\vec{r}}^{\prime})\psi_{j}({\vec{r}})]d{\vec{r}}^{\prime}=\epsilon_{i}\psi_{i}({\vec{r}}). (11)

Here, ii and jj now run from unity to NtotN_{\rm tot}: i,j=1,,Ntoti,j=1,...,N_{\rm tot}. This system of equations differs from Equation (8) in that the NN number is replaced by NtotN_{\rm tot} and the UCqU_{\rm C}^{q} potential is replaced by UCU_{\rm C}, [Equation (3)]. It allows one to calculate the needed energies, ϵi\epsilon_{i}, and the wavefunctions, ψi(r)\psi_{i}({\vec{r}}), of both the atomic and excess electrons in A@C(n,)Nq{}_{N}^{q}(n\ell,...) and apply them to calculations of the photoionization cross sections of the thus confined atom A.

We will frequently refer to such model of the fullerene anion as “structured” model or approximation in this paper, to underline that it accounts for possible quantum states of the excess electronic charge on the cage.

Now, however, a complication arises due to the existence of various total terms for the A@C(n,)Nq{}_{N}^{q}(n\ell,...) system, which is now an open-shell system. In the present study, we bypass this complication by utilizing the term-average Hartree-Fock formalism YarzhCher2024 to calculate the energies and wavefunctions of both the atomic and excess electrons in the A@C(n,)Nq{}_{N}^{q}(n\ell,...) system. To avoid diverting the reader’s attention from the main topic of the paper, a review of the term-average Hartree-Fock formalism is provided in Appendix.

Lastly, in performed calculations for the present study, we used the values for r0r_{0}, Δ\Delta and U0U_{0} for C60/C240 as stated and discussed in DolmBrMans2008 : r05.8/12.6r_{0}\approx 5.8/12.6, Δ1.9/1.9\Delta\approx 1.9/1.9, U00.302/0.378U_{0}\approx 0.302/0.378 a.u., respectively.

III Results and Discussion

III.1 H(1s)@CN1{\rm H}(1s)@{\rm C}_{N}^{-1} versus H(1s)@CN1(n){\rm H}(1s)@{\rm C}_{N}^{-1}(n\ell)

Here, we present and discuss calculated results concerning the photoionization of the ground-state hydrogen atom, H(1s)(1s), encapsulated inside the singly-charged fullerene anion (q=1q=-1). These results were obtained in the framework of both aforementioned models for the endohedral fullerene anions - the structureless [H(1s)@CNq{\rm H}(1s)@{\rm C}_{N}^{q}] and structured [H(1s)@CNq(n){\rm H}(1s)@{\rm C}_{N}^{q}(n\ell)] models. As case studies, we arbitrarily choose n=2pn\ell=2p and 3d3d, and we run calculations for CN fullerene cages with both N=60N=60 and N=240N=240 carbon atoms in the cage, respectively.

In Figure 11, the P1sP_{1s} radial function of the encapsulated H atom is depicted. Additionally, the P2p(r)P_{2p}(r) and P3d(r)P_{3d}(r) radial functions are depicted for the 2p2p and 3d3d orbitals of the attached electron, respectively, within the endohedral fullerene anions.

Refer to caption
Figure 1: (Color online) (a) Calculated P1s(r)P_{1s}(r) radial functions for H@C601{\rm H}@{\rm C}_{60}^{-1} as well as the P1s(r)P_{1s}(r), P2p(r)P_{2p}(r) and P3d(r)P_{3d}(r) electronic radial functions for H@C601(n){\rm H}@{\rm C}_{60}^{-1}(n\ell) with n=2pn\ell=2p and n=3dn\ell=3d (see text), as designated in the figure. (b) Calculated P1s(r)P_{1s}(r) radial functions for H@C2401{\rm H}@{\rm C}_{240}^{-1} as well as the P1s(r)P_{1s}(r), P2p(r)P_{2p}(r) and P3d(r)P_{3d}(r) electronic radial functions for H@C2401(n){\rm H}@{\rm C}_{240}^{-1}(n\ell) with n=2pn\ell=2p and n=3dn\ell=3d (see text), as designated in the figure. Note, the P1sP_{1s} function for the encapsulated hydrogen atom depends so little on both the presence and state of the excess electron in the fullerene shell in all calculations that all graphs for P1sP_{1s} are practically totally blended with each other in the figure.

Firstly, it can be concluded from Figure 1 that the 1s1s electron density in the encapsulated atom remains largely unaffected by the excess charge on the fullerene cage, especially in the case of the C240 cage.

Secondly, note how the P2p(r)P_{2p}(r) and P3d(r)P_{3d}(r) functions of the excess electron extend, to some degree, into the hollow interior of the CN shell, thereby overlapping with the P1sP_{1s} function of the encapsulated H atom. This, obviously, should make the 1s1s-photoionization cross section, σ1s\sigma_{1s}, of the H(1s)@CN1(n){\rm H}(1s)@{\rm C}_{N}^{-1}(n\ell) system differ from that of the structureless H(1s)@CN1{\rm H}(1s)@{\rm C}_{N}^{-1} system. How strong can the difference be? One of the aims of the present study is to answer this question.

Thirdly, one can see that the overlap of the P1sP_{1s} function with the functions for the 2p2p and 3d3d excess electrons is far less significant in the case associated with a C240 shell than in the other case. Hence, it is reasonable to expect that any differences in values of σ1s\sigma_{1s} between the H(1s)@CN1{\rm H}(1s)@{\rm C}_{N}^{-1} and H(1s)@CN1(n){\rm H}(1s)@{\rm C}_{N}^{-1}(n\ell) systems will diminish with the increasing size of the fullerene cage.

Fourthly, interestingly, the 2p2p and 3d3d functions of the excess electron differ insignificantly, especially in the case of the giant C240 cage. A similar situation was observed and explained for the PnP_{n\ell} functions of the nn\ell-electron attached to the empty fullerene cage Dolm2022 . The reason for the noted indistinguishability between the functions with different \ell values (the P2pP_{2p} and P3dP_{3d} functions in our case) arises from the electrons’ primary localization on the cage itself, which has a large radius. Consequently, the centrifugal barrier (+1)2r2\frac{\ell(\ell+1)}{2r^{2}}, which induces the dependence of PnP_{n\ell} on \ell, becomes so small that the difference between the functions with close \ell values effectively vanishes. The latter is particularly true for the case of the giant C240 cage.

Calculated σ1s\sigma_{1s} photoionization cross sections of H@C1N{}_{N}^{-1} and H@C(n)N1{}_{N}^{-1}(n\ell) with n=2pn\ell=2p and 3d3d are depicted in Figure 22.

Refer to caption
Figure 2: (Color online) Calculated σ1s\sigma_{1s} photoionization cross sections for the H(1s)(1s) atom confined inside various fullerene anions: H@C160{}_{60}^{-1}, H@C(2p)601{}_{60}^{-1}(2p), H@C(3d)601{}_{60}^{-1}(3d), H@C1240{}_{240}^{-1} and H@C(2p)2401{}_{240}^{-1}(2p), as designated in the figure.

One can see that some differences between these σ1s\sigma_{1s} cross sections are seen only in the low-energy region. There, the sharp, intense maxima in σ1s\sigma_{1s}’s are somewhat shifted along the energy scale relative to each other without a significant change in their magnitudes. Thus, it is reasonable to summarize that the change in σ1s\sigma_{1s}’s between the H@C160{}_{60}^{-1}, and H@C(n)N{}_{N}(n\ell) systems are minimal. This reveals the first indication that the photoionization cross section of the atom from an endohedral fullerene anion depends little on the state of the excess charge on the anion.

And, as expected, the differences between the discussed σ1s\sigma_{1s}’s are diminishing with the increasing size of the fullerene cage. This is obvious from comparing calculated data plotted in Figure 22a (for C60C_{60}) with those plotted in Figure 22b for the case of a C240 cage. Note that a would-be larger shift in energy between the low-energy maxima in σ1s\sigma_{1s}’s, plotted in Figure 22b, compared to the energy shift in Figure 22a is deceptive. This is because the energy-scale range is less than 1010 eV in Figure 22b, but is much broader, about 3030 eV, in Figure 22a.

Finally, let us comment on the origin and nature of all the maxima in σ1s\sigma_{1s}’s displayed in Figure 22. To meet the goal, we also plotted calculated σ1s\sigma_{1s} photoionization cross sections of the hydrogen atom confined inside a neutral CNC_{N} cage, designated as “H@CN@{\rm C}_{N} (neutral)” in the figure.

Firstly, the calculated σ1s\sigma_{1s} values, plotted in Figure 2a2a or 2b2b, are nearly identical down to about 1414 eV of photon energy. Secondly, for photon energies down to about 1414 eV, all σ1s\sigma_{1s}’s exhibit a maximum around 2222 eV for N=60N=60 (though this maximum is poorly developed) and around 1717 eV for N=240N=240. Therefore, the higher-energy maxima in σ1s\sigma_{1s} for endohedral fullerene anions have the same origin as the maximum in σ1s\sigma_{1s} for the neutral H@CN endohedral fullerene. The origin of such maxima in the σn\sigma_{n\ell} for atoms in neutral A@CN endohedral fullerenes has been extensively studied in previous works, e.g., PuskaPRA93 ; DeshmukhEPJD2021 ; Baltenkov ; ConDolmMans ; DolmAQC (and references therein). These maxima arise from interference between the outgoing photoelectron wave from the encapsulated atom and the photoelectron waves reflected from the fullerene cage boundaries. In ConDolmMans , these resonances were termed confinement resonances. This term has become common in the literature, and we use it in the present paper as well. Thus, the observed higher-energy resonances in σ1s\sigma_{1s} for H@C160{}_{60}^{-1}, H@C(n)N1{}_{N}^{-1}(n\ell), and neutral H@CN are confinement resonances.

Next, in the photon energy region below about 1414 eV, all calculated σ1s\sigma_{1s} values for fullerene anions show a sharp, strong resonance, whereas the σ1s\sigma_{1s} for neutral H@CN does not extend into this region. Thus, these sharp lower-energy resonances originate from a different source compared to the confinement resonances. Such resonances in the photoionization cross sections of atoms encapsulated within fullerene anions were predicted and studied in detail in DolmMansPRA2006 . It was demonstrated that these resonances arise due to an additional Coulomb potential barrier created by the excess charge on the fullerene cage. In DolmMansPRA2006 , these novel resonances in σn\sigma_{n\ell} values were termed Coulomb confinement resonances. To date, Coulomb confinement resonances have been explored in various contexts with different levels of detail in numerous theoretical studies (see, e.g., KumarVarmaJPCS2015 ; KumarVarmaPRA2016 ; VarmaPRA2020 ; VarmaPhysSCR2021 ; VarmaPRA2023 and references therein). Therefore, the lower-energy resonance structures in σ1s\sigma_{1s} for H@CN1{N}^{-1} and H@CN1(n){N}^{-1}(n\ell) are Coulomb confinement resonances.

To conclude, we have unraveled the first indication that the photoionization cross section of the atom within the endohedral fullerene anion is largely independent of the quantum structure of the excess charge on the anion. The most noticeable differences (albeit insignificant) in the photoionization cross sections between the structureless and structured fullerene anions primarily occur in the region of Coulomb confinement resonances.

III.2 (He&He+)@CN1({\rm He\ \&\ He^{+})@C}_{N}^{-1}, (He&He+)@CN1(n)({\rm He\ \&\ He^{+})@C}_{N}^{-1}(n\ell) and (He&He+)@CN2(n,n)({\rm He\ \&\ He^{+})@C}_{N}^{-2}(n\ell,n^{\prime}\ell^{\prime})

As another case study, we examine the photoionization of the He(1s2)(1s^{2}) atom and its ion, He(1s1)+{}^{+}(1s^{1}), confined within the structureless fullerene anion cage, CqN{}_{N}^{q}, compared to when they are encapsulated inside the structured fullerene anion cages, CNq(n){\rm C}_{N}^{q}(n\ell) or CNq(n,n){\rm C}_{N}^{q}(n\ell,n^{\prime}\ell^{\prime}). Specifically, we arbitrarily choose the He@C(2p)N1{}_{N}^{-1}(2p) and He@C(3d)N1{}_{N}^{-1}(3d) singly-charged endohedral fullerene anions, as well as the He@+CN2(2s2p){}^{+}@{\rm C}_{N}^{-2}(2s2p) and He@+CN2(2s3d){}^{+}@{\rm C}_{N}^{-2}(2s3d) doubly-charged anions, with N=60N=60 and 240240.

The corresponding P1sP_{1s}, P2sP_{2s}, P2pP_{2p} and P3dP_{3d} electronic functions are plotted in Figure 3.

Refer to caption
Figure 3: (Color online) (a) Calculated P1s(r)P_{1s}(r) of a neutral He(1s2)(1s^{2}) atom encapsulated inside structureless C601{\rm C}_{60}^{-1}, as well as the P2pP_{2p} and P3dP_{3d} functions of the attached electron in the structured He@C601(2p)@{\rm C}_{60}^{-1}(2p) and He@C601(3d)@{\rm C}_{60}^{-1}(3d) fullerene anions, as designated in the figure. (b) Calculated P1s(r)P_{1s}(r) of the He+ ion encapsulated inside structureless C602{\rm C}_{60}^{-2}, as well as the P2sP_{2s}, P2pP_{2p}, and P3dP_{3d} functions of the attached electron in the corresponding structured He@+C602(2s2p){}^{+}@{\rm C}_{60}^{-2}(2s2p) and He@+C602(2s3d){}^{+}@{\rm C}_{60}^{-2}(2s3d) fullerene anions, as designated in the figure. Note that, similar to the case of the H atom, the P1s(r)P_{1s}(r) functions overlap with each other in each of the considered cases, so we plotted P1s(r)P_{1s}(r) only for one of them in both parts of the figure.

The behavior of the plotted functions follows the same trends as in the previously discussed case of the H atom inside the fullerene anion. Therefore, we believe that they are self-explanatory without new elements in the behavior, and we leave it to the reader to draw their own conclusions regarding these functions. It is important to stress, however, that, as earlier, there is overlap between the P1sP_{1s} atomic function and each of the corresponding P2sP_{2s}, P2pP_{2p}, and P3dP_{3d} functions. Accordingly, we explore below how this overlap between the electronic functions affects the σ1s\sigma_{1s} photoionization cross section of He and He+ from the structured fullerene anions compared to the structureless fullerene anions.

The correspondingly calculated σ1s\sigma_{1s} photoionization cross sections are depicted in Figure 44.

Refer to caption
Figure 4: (Color online) (a) Calculated σ1s\sigma_{1s} photoionization cross sections for He@C601@{\rm C_{60}}^{-1} as well as for He@C60(2p)@{\rm C_{60}}(2p) and He@C60(2p)@{\rm C_{60}}(2p) along with σ1s\sigma_{1s} for the helium atom confined inside a neutral C60C_{60} shell, i.e., for He(1s2)@C60(1s^{2})@C_{60}, as designated in the figure. (b) Calculated σ1s\sigma_{1s} photoionization cross sections for He@+C602{}^{+}@{\rm C_{60}}^{-2}, He@+C602(2s2p){}^{+}@{\rm C_{60}}^{-2}(2s2p) and He@+C602(2s3d){}^{+}@{\rm C_{60}}^{-2}(2s3d), as well as σ1s\sigma_{1s} He+ inside a neutral C60C_{60} shell, i.e., He@+C60{}^{+}@{\rm C_{60}}, as designated in the figure.

Firstly, similar to the hydrogen atom case discussed earlier, Figure 4 reveals that σ1s\sigma_{1s} for the encapsulated helium atom and its ion exhibit a pronounced, low-energy sharp resonance when photoionization occurs from the fullerene anions. This resonance is absent in the photoionization of He and He+ encapsulated inside the neutral C60 cage. Thus, as in the case of the hydrogen atom, these observed features are Coulomb confinement resonances. As photon energy increases, these Coulomb confinement resonances are succeeded by less pronounced resonances in both the charged and neutral endohedral fullerene systems. These latter features are, thus, ordinary confinement resonances.

Secondly, a key finding, however, is that the differences in σ1s\sigma_{1s} between photoionization of He or He+ from the structureless and various structured endohedral fullerene anions, respectively, are primarily observed in the Coulomb confinement resonances. However, these differences are relatively minor, with no significant qualitative or strong quantitative variations. We, thus, have uncovered one more indication that the photoionization cross sections of the atom or its ion confined inside the endohedral fullerene anion depend little on the quantum structure of the excess charge on the fullerene cage.

Next, we present the results for calculated σ1s\sigma_{1s} for He and He+ confined within the structureless and various structured fullerene anions with a giant C240 carbon cage. These calculated σ1s\sigma_{1s}’s are shown in Figure 5.

Refer to caption
Figure 5: (Color online) (a) Calculated σ1s\sigma_{1s} photoionization cross sections for He@C2401@{\rm C_{240}}^{-1} as well as for He@C240(2p)@{\rm C_{240}}(2p) and He@C240(2p)@{\rm C_{240}}(2p) along with σ1s\sigma_{1s} for the helium atom confined inside a neutral C240C_{240} shell, i.e., for He@C240@{\rm C}_{240}, as designated in the figure. (b) Calculated σ1s\sigma_{1s} photoionization cross sections for He@+C2402{}^{+}@{\rm C_{240}}^{-2}, He@+C2402(2s2p){}^{+}@{\rm C_{240}}^{-2}(2s2p) and He@+C2402(2s3d){}^{+}@{\rm C_{240}}^{-2}(2s3d), as well as σ1s\sigma_{1s} He+ inside a neutral C240C_{240} shell, i.e., He@+C240{}^{+}@{\rm C_{240}}, as designated in the figure.

The trends observed in the calculated σ1s\sigma_{1s}’s for the structureless and structured giant fullerene anions mirror those just discussed above for He and He+ confined within the fullerene anions associated with the C60 fullerene cage. It is worth noting, however, that the differences in calculated σ1s\sigma_{1s}’s are significantly smaller in giant fullerene cases compared to the previous ones, which was anticipated.

The results presented in this section uncover that the photoionization cross sections of both the neutral atom and its ion encapsulated inside the fullerene anion cage are affected only little by the quantum structure of the excess charge on the cage.

IV Conclusions

In this study, we investigated the photoionization cross sections of compact H and He atoms, as well as the He+ ion, encapsulated within a fullerene anion cage. The electron density of these encapsulated species remains unaffected by the fullerene cage.

The results and discussions indicate that the photoionization cross section of the centrally encapsulated atom or its cation inside the CqN{}_{N}^{q} fullerene anion cage is minimally influenced by the quantum states of the excess electrons on the cage, provided the electron density of the encapsulated atom/ion remains predominantly within the atom/ion itself. This conclusion is likely extendable to other centrally confined compact atoms as well; we do not see why this would be untrue. The most noticeable differences in the calculated photoionization cross sections, which arise from considering the quantum states of the excess electrons on the fullerene cage, are primarily observed in the Coulomb confinement resonances. However, these differences are relatively small and diminish significantly with the increasing size of the fullerene cage. Consequently, both the original structureless model and the structured model of the fullerene anion yield photoionization cross sections that are in close agreement, especially for the case of the giant fullerene anion. Therefore, as one of the key findings of this research, we conclude that either model is equally effective for studying the photoionization cross sections of atoms encapsulated within the fullerene anion, as long as the electron density of the encapsulated atom/ion remains primarily within the atom/ion itself.

For atoms that significantly contribute their electron density to the fullerene cage, we anticipate that the photoionization cross sections of the inner electrons will depend insignificantly on the quantum structure of the excess electrons on the fullerene cage as well. However, this scenario involving such atoms requires a separate, independent study, which is beyond the scope of this paper.

Appendix A Term-average Hartree-Fock approximation

In this section, we outline the key steps that lead to the term-average methodology for the Hartree-Fock formalism YarzhCher2024 (also with its extention to the calculation of many-body Feynman diagrams) used in the present study.

In the calculation of atomic wavefunctions using the Hartree-Fock method, the combined direct and exchange Coulomb interelectron interaction energy, UcU_{\rm c}, in the atom is given by:

Uc=kλFSLλRllllλ\displaystyle U_{c}=\sum\limits_{k}\sum_{\lambda}F_{SL}^{\lambda}R_{llll}^{\lambda}
+kpμFSLSLLtStμRllllμ\displaystyle+\sum\limits_{k\neq p}\sum\limits_{\mu}F_{SLS^{\prime}L^{\prime}{L_{t}}{S_{t}}}^{\mu}R_{ll^{\prime}ll^{\prime}}^{\mu}
+kpνGSLSLLtStνRllllν.\displaystyle+\sum\limits_{k\neq p}\sum\limits_{\nu}G_{SLS^{\prime}L^{\prime}{L_{t}}{S_{t}}}^{\nu}R_{lll^{\prime}l^{\prime}}^{\nu}. (12)

Here, the sum runs over all atomic subshells k(p)k(p) and all values of λ,μ\lambda,\mu and ν\nu that satisfy the triangular rule Δ(λ)\Delta\left(\ell\lambda\ell\right), Δ(μ)Δ(μ)\Delta\left(\ell\mu\ell\right)\cap\Delta\left(\ell^{\prime}\mu\ell^{\prime}\right) and Δ(ν)\Delta\left(\ell\nu\ell^{\prime}\right), provided the sum of the angular moments in brackets is even.

The Coulomb integral, expressed in terms of the radial parts PnkkP_{n_{k}\ell_{k}} of the atomic wavefunctions, is given by the standard formula:

R1234λ=00r<λr>λ+1\displaystyle R_{\ell_{1}\ell_{2}\ell_{3}\ell_{4}}^{\lambda}=\int_{0}^{\infty}\int_{0}^{\infty}\frac{r_{<}^{\lambda}}{r_{>}^{\lambda+1}}
×Pn11(r)Pn33(r)Pn2l2(r)Pn44(r)drdr.\displaystyle\times P_{n_{1}\ell_{1}}(r)P_{n_{3}\ell_{3}}(r)P_{n_{2}l_{2}}(r^{\prime})P_{n_{4}\ell_{4}}(r^{\prime})dr^{\prime}dr. (13)

Here, r>r_{>} (r<r_{<}) is the larger (smaller) of the two radial parameters rr and rr^{\prime}.

The FλF^{\lambda} weight factors for the direct Coulomb interaction for open atomic shells are tabulated for all terms in nk . The FμF^{\mu} weight factors for the direct Coulomb interaction as well as the GνG^{\nu} weight factors for the ‘exchange Coulomb interaction that are presented in (12) depend on the values of LSLS and LSL^{\prime}S^{\prime} for the interacting shells kk and pp as well as on the total values of the LtL_{t} angular and StS_{t} spin moments sob .

For the closed shell atom with N=2(2+1)N=2(2\ell+1) electrons in the shell, the weight factors before the Coulomb integrals are determined as sob :

F0=(4+2)(4+1)2=C(4+2)2,F^{0}=\frac{\left(4\ell+2\right)(4\ell+1)}{2}=C_{\left(4\ell+2\right)}^{2}, (14)

whereas

Fλ=(2+1)2(λ000)2F^{\lambda}=-\left(2\ell+1\right)^{2}\left(\begin{array}[]{ccc}\ell&\lambda&\ell\\ 0&0&0\end{array}\right)^{2} (15)

To avoid accounting for the exact angular-momentum-coupling scheme in our study, for the sake of simplicity, in the present work we use the average-term approximation, the essence of which is based on the introduction of the average direct Coulomb and exchange weight factors into the interelectron interaction potential, as follows.

Since the expression for F0F^{0} is proportional to the number of interacting pairs of electrons in the closed shell of 4+24\ell+2 electrons, it is natural to expect that the same is true for the FλF^{\lambda} coefficients as well. Thus, for the NN-electron open shells, we write Equations (14) and (15) as follows:

F0(N)=N(N1)2=CN2F^{0}(\ell^{N})=\frac{N(N-1)}{2}=C_{N}^{2} (16)
Favλ(lN)=(2+1)2\displaystyle F_{\rm av}^{\lambda}(l^{N})=-\left(2\ell+1\right)^{2}
(×λ000)2N(N1)(4+2)(4+1)\displaystyle\left(\times\begin{array}[]{ccc}\ell&\lambda&\ell\\ 0&0&0\end{array}\right)^{2}\frac{N(N-1)}{\left(4\ell+2\right)(4\ell+1)} (19)

Equation (16) for F0F^{0} is exact for unfilled shells.

The exact FλF^{\lambda} weight factors for λ>0\lambda>0 depend on the values of LL, SS, and additional quantum numbers. These factors are tabulated in nk for all possible terms. The FavλF_{\rm av}^{\lambda} value equals the value of FLSλF_{LS}^{\lambda} averaged over all LSLS terms of the N\ell^{N} configuration using their (2S+1)(2L+1)(2S+1)(2L+1) statistical weights.

Next, for the interaction of two closed shells, (4+2)\ell^{(4\ell+2)} and (4+2)\ell^{\prime(4\ell^{\prime}+2)}, the equations for the weight factors are as follows:

F0(4+2,4+2)=(4+2)((4+2),F^{0}(\ell^{4\ell+2},\ell^{\prime 4\ell^{\prime}+2})=(4\ell+2)((4\ell^{\prime}+2), (20)
Gν(4+2,4+2)=\displaystyle G^{\nu}(\ell^{4\ell+2},\ell^{\prime 4\ell^{\prime}+2})=
2(2+1)(2+1)(ν000)2\displaystyle-2\left(2\ell+1\right)(2\ell^{\prime}+1)\left(\begin{array}[]{ccc}\ell&\nu&\ell^{\prime}\\ 0&0&0\end{array}\right)^{2}\ (23)

For closed shells, Fμ=0F^{\mu}=0 for μ0\mu\neq 0.

Equation (20) indicates that the intershell interaction is proportional to the numbers of electrons in the interacting shells. This allows us to write the average weighs factors for a similar interaction between the open shells as follows

F0(N,N)=NN,F^{0}(\ell^{N},\ell^{\prime N^{\prime}})=NN^{\prime}, (24)

and

Gν(l4+2,4+2)=\displaystyle G^{\nu}(l^{4\ell+2},\ell^{\prime 4\ell^{\prime}+2})=
2(2+1)(2+1)NN(4+2)(4+2)(ν000)2\displaystyle\frac{-2\left(2\ell+1\right)(2\ell^{\prime}+1)NN^{\prime}}{\left(4\ell+2\right)\left(4\ell^{\prime}+2\right)}\left(\begin{array}[]{ccc}\ell&\nu&\ell^{\prime}\\ 0&0&0\end{array}\right)^{2}\ (27)

In our study of the structured open-shell fullerene anions, these weight factors were substituted into the Equation (12) for the interelectron interaction potential to calculate the term-averaged energies and PnP_{n\ell} radial parts of the wavefunctions of electrons.

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