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Rovibrational Levels of Helium Hydride Ion Version 3.0 Rovibrational levels of helium hydride ion Krzysztof Pachucki¤ Faculty of Physics, University of Warsaw, Ho_za 69, 00-681 Warsaw, Poland Jacek Komasay Faculty of Chemistry, A. Mickiewicz University, Grunwaldzka 6, 60-780 Pozna¶n,Poland (Dated: November 5, 2012) Abstract 4 + Dissociation energy (D0) of rovibrational levels of HeH has been predicted theoretically to the accuracy of the order of 0:01 cm¡1. The calculations take into account adiabatic and nona- diabatic corrections as well as relativistic and QED e®ects. For the ground rovibrational level ¡1 D0 = 14 874:213(10) cm and it di®ers by several tens of the inverse centimeter from previous theoretical estimations. For a collection of about ¯fty transition energies measured between dipole connected levels the di®erence between theory and experiment is of the order of hundredths of cm¡1 or less. ¤Electronic address: [email protected] yElectronic address: [email protected] 1 I. INTRODUCTION Formed by the most abundant elements, the hydrohelium plays an important role in astrophysics. According to the standard Big Bang model, the helium hydride ion HeH+ is + the ¯rst molecule, along with He2 , formed in the Universe [1, 2] and its signi¯cance in the early Universe chemistry cannot be overestimated [3]. Because of its low abundance, caused by processes competitive to its formation, HeH+ is expected to be di±cult to observe. Several rotational lines have been selected as candidates for such observations [4, 5]. Although HeH+ is expected to be observable in a variety of astrophysical environments [6{9], no unequivocal detection has been reported to date. HeH+ is present in helium-hydrogen plasma produced in a variety of experiments and most of the spectroscopic data available today originates from the laboratory measurements. Large permanent dipole moment of HeH+ enables acquisition of highly accurate spectra in the gas phase. The knowledge of the rovibrational spectrum of the bound and quasi-bound states allows an evaluation of cross sections for spontaneous and stimulated processes of formation of HeH+ in the interstellar space [10]. Such cross sections, in turn, enable prediction of pertinent reaction rates indispensable for understanding the reactions mechanisms [11] and for veri¯cation of cosmological models. Interestingly, experimental and theoretical studies of 3HeT+ [12] at that time were mo- tivated by the neutrino mass measurements. Experimental data for other isotopomers are available in literature [13{15], hence the isotopic substitution e®ect can be studied. Such data have been used by Coxon and Hajigeorgiu [16] in solving an inverse rovibrational prob- lem, i.e. to construct an empirical Born-Oppenheimer (BO) interaction potential. Their estimated interaction energy at the equilibrium of the BO potential (16 456:24 § 0:1 cm¡1) is by 0:83 cm¡1 smaller than the exact value of Ref. [17]. + HeH is a relatively simple heteronuclear molecular ion, isoelectronic with H2, which makes it of a fundamental signi¯cance from the theoretical point of view. There is extensive literature reporting quantum chemical calculations on this system. Apart from correlated methods based on the one-electron approximation [18{20], more sophisticated methods of explicitly correlated wave functions expanded in the James-Cooledge (JC) or gaussian (ECG) basis have been employed. Early calculations were limited to very short expansions and a few internuclear distances R [21{23]. The ¯rst accurate calculations of the Born-Oppenheimer (BO) energy curve can be attributed to Wolniewicz [24]. He applied the obtained wave 2 function to study a formation of HeH+ from HT molecule through the ¯ decay process. Ten years later, KoÃlos and Peek [25, 26] extended the BO calculations to long distances, which enabled studies of quasi-bound energy levels. An important step forward has been made by Bishop and Cheung [27] who have signi¯cantly improved the accuracy of previous results and additionally evaluated the adiabatic correction to the BO curve. A few years ago, accurate nonadiabatic-relativistic energies for rotationless levels have been obtained using ECG functions by Stanke et al. [28]. Very recently, a state-of-the-art BO potential has been obtained with relative accuracy of 10¡12 [17]. Spectroscopists claim that, "the spectroscopic measurements are typically four orders of magnitude more precise than the theoretical spectra!" [29]. The exceptions are the two + electron diatomic molecules, such as H2 and HeH . We report here on results obtained using the methodology applied successfully to hydrogen molecule and its isotopomers [30{ 33]. Those theoretical predictions have been veri¯ed by subsequent experiments [29, 33{39]. Our goal is to supply a theoretically predicted spectrum of the bound states of HeH+ with the highest possible accuracy achievable within the present day stage of theoretical and computational methods. Such a full energy spectrum can be helpful in selection of those astrophysical objects at which HeH+ can potentially be detected. II. METHODOLOGY In the frames of the so-called nonrelativistic quantum electrodynamics (NRQED) [40{42], relativistic and QED e®ects are included in successive terms of the perturbation series E = E(0) + ®2E(2) + ®3E(3) + ®4E(4) + ¢ ¢ ¢ (1) whereas the nonrelativistic component E(0) of the total energy is evaluated using the recently developed nonadiabatic perturbation theory (NAPT) [43, 44]. A short account of the underpinning theory will be presented below. More details will be given only on these items which are new or speci¯c to HeH+. Atomic units will be used throughout unless explicitly stated. 3 A. Nonrelativistic Hamiltonian The nonrelativistic Hamiltonian of an N-electron diatomic molecule entering the SchrÄodingerequation H ª = E ª (2) can be split into the electronic and nuclear parts H = Hel + Hn : (3) The former includes the kinetic energy of the electrons and the Coulomb interactions between all the particles 1 XN H = ¡ r2 + V; (4) el 2 a a=1 with XN XN NX¡1 XN 1 1 1 ZA ZB V = ¡ZA ¡ ZB + + : (5) raA raB rab R a=1 a=1 a=1 b=a+1 The notation employed to describe a location of particles is de¯ned in Figure 1. 1 · ~r1 ~r1A ~ ~ RB R~ RA • • • B O A X 0t 1 FIG. 1: Vectors de¯ning the geometric structure of the molecule. A and B are the hydrogen (ZA = 1) and helium (ZB = 2) nucleus positions, respectively. O is the location of the arbitrarily chosen origin of the coordinate system. Before we write down explicitly the nuclear Hamiltonian of a diatomic molecule, we in- troduce a parameter t which speci¯es the origin, O, of the molecule-¯xed coordinate system. 4 As shown in Figure 1, t is a fraction of the internuclear distance measured from the 'left' nucleus, so that the nuclear positions are: ~ ~ ~ ~ RA = (1 ¡ t) R and RB = ¡t R (6) and the vectors pointing at the electron 1 from the nuclei are ~ ~ ~r1A = ~r1 ¡ (1 ¡ t) R and ~r1B = ~r1 + t R: (7) With the nuclear masses MA and MB (M = MA + MB), and the nuclear reduced mass ¡1 ¹n = (1=MA + 1=MB) , we can write [45] µ ¶ 1 1 t2 (1 ¡ t)2 H = ¡ r2 ¡ + r2 (8) n 2 ¹ R 2 M M el µ n ¶ A B t 1 ¡ t ~ ~ + ¡ rR ¢ rel : MA MB P ~ N ~ Here we have introduced a shorthand notation rel = a=1 ra. Additionally, we de¯ne a new di®erential operator µ ¶ M r~ = r~ ¡ t ¡ A r~ (9) R M el which has an important feature|its action on the electronic wave function 'el is t-invariant. MA We note, that if t = M i.e. the origin is selected at the center of nuclear mass (CNM), the two above equations simplify|the last term in both cases vanishes. Finally, using the introduced abbreviations, we arrive at the following compact form of the t-dependent nuclear Hamiltonian 1 ~ 2 1 2 Hn = ¡ r ¡ rel : (10) 2 ¹n 2 M B. Adiabatic approximation Our zero-order ansatz is in the form of a product of electronic and nuclear wave functions ~ ~ Áa(~r; R) = Áel(~r) Â(R) ; (11) the former being a solution to the electronic SchrÄodingerequation with the clamped nuclei Hamiltonian (4) Hel 'el = Eel 'el (12) 5 and the latter|to the nuclear SchrÄodingerequation · 2 ¸ rR ~ ~ ¡ + Eel(R) + Ea(R) Â(R) = Ea Â(R) ; (13) 2 ¹n with the adiabatic correction Ea = h'el jHnj 'eliel (14) D ¯ ¯ E ­ ¯ ¯ ® 1 ¯ ~ 2¯ 1 ¯ 2¯ = ¡ 'el ¯r ¯ 'el ¡ 'el rel 'el el 2 ¹n el 2 M included in the potential for the movement of the nuclei. C. Nonadiabatic e®ects The nonadiabatic e®ects can be taken into account using the perturbation theory (NAPT) introduced in Ref. 43 and developed in Ref. 44. According to this theory the leading order correction to energy of a molecular level is given by ¿ ¯ ¯ À ¯ 1 ¯ E(2) = '  ¯H H ¯ '  : (15) na el ¯ n 0 n¯ el (Eel ¡ Hel) Alternatively, the level energy can be obtained as a solution to the nonadiabatic radial SchrÄodingerequation · ¸ 1 @ R2 @ J (J + 1) ¡ 2 + 2 + Y(R) Â~J (R) R @R 2 ¹k(R) @R 2 ¹?(R) R = E Â~J (R) ; (16) where Y(R) = Eel(R) + Ea(R) + ±Ena(R) : (17) The solution ~J (R) is a radial part of  for a given angular momentum J. The energy (2) E includes the adiabatic energy Ea, the second order nonadiabatic correction Ena , and an admixture of higher order corrections. In analogy with the original approach [43, 44], the R-dependent reduced nuclear masses ¹k(R) (vibrational) and ¹?(R) (rotational) are de¯ned through the potentials W(R). 1 1 = + Wk(R) ; (18) 2 ¹k(R) 2 ¹n 1 1 = + W?(R) : (19) 2 ¹?(R) 2 ¹n 6 ~ ~ These, however, di®er from their original counterparts in using r operator rather than rR ¿ ¯ ¯ À 1 1 ¯ 1 ¯ W (R) = Rir~ i' ¯ ¯ Rjr~ j' ; (20) k ¹2 R2 el ¯(E ¡ H )0 ¯ el n µ ¶ el el el 1 1 RiRj W (R) = ±ij ¡ (21) ? ¹2 2 R2 ¿ n ¯ ¯ À ¯ 1 ¯ r~ i' ¯ ¯ r~ j' : el ¯ 0 ¯ el (Eel ¡ Hel) el Referring again to the original formulation, we recall here that the nonadiabatic correction to the BO potential is µ ¶ 2 @ ±E (R) = U(R) + + (V(R) + ±V(R)) : (22) na R @R The three functions of R referenced above are de¯ned as follows ¿ ¯ ¯ À ¯ 1 ¯ U(R) = H ' ¯ ¯ H ' ; (23) n el ¯(E ¡ H )0 ¯ n el ¿ el ¯ el ¯ el À 1 1 ¯ 1 ¯ V(R) = ¡ H ' ¯ ¯ Rir~ i' ; (24) n el ¯ 0 ¯ el ¹n R (Eel ¡ Hel) el 1 dE (R) ±V(R) = ¡ el (25) 2 ¹2 dR ¿ n ¯ ¯ À ¯ 1 ¯ Rir~ i' ¯ ¯ Rjr~ j' : el ¯ 0 2 ¯ el [(Eel ¡ Hel) ] el III.
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