REVIEW 3 major objections 4 minor 5 cited by
Preparing two ultracold molecules in the ro-vibrational pair (0,1)+(1,0) creates a strong repulsive van der Waals interaction that suppresses collisional loss by up to seven orders of magnitude and enables evaporative cooling of Fermi mixtu
Reviewed by Pith at T0; open to challenge. T0 means a machine referee read the full paper against a public rubric. the ladder, T0–T4 →
T0 review · deepseek-v4-flash
2026-08-03 01:41 UTC pith:3SZWU6W5
load-bearing objection The ro-vibrational vdW interaction is a real and novel mechanism with solid coupled-channel support; the paper should be peer reviewed, but the abstract's evaporation claim goes beyond what is shown. the 3 major comments →
Ro-vibrational van der Waals interaction between ultracold polar molecules
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
The paper demonstrates that a pair of molecules in the ro-vibrational states (v,j)+(v',j')=(0,1)+(1,0) is coupled by the dipole-dipole interaction to the nearly degenerate pair (0,0)+(1,1). The degeneracy is broken by rotation-vibration coupling: the rotational constant is slightly smaller in v=1 because the molecule's bond is stretched, so the energy defect is 2αe. This virtual transition produces a second-order interaction ±C6 R^-6 with C6 = de^4/(9αe), repulsive in the entrance channel of interest. For NaK the coefficient is 7×10^7 a.u. and for the ultrapolar species KAg it reaches 10^10 a.u., giving van der Waals lengths of 1700 and 7400 bohr. Coupled-channel calculations including full
What carries the argument
The central object is the rotation-vibration coupling constant αe of the Dunham expansion, which measures how much the rotational constant decreases when the molecule is vibrationally excited. Its small size (roughly 1–100 MHz for assembled ultracold molecules) sets the energy denominator for the virtual dipole-allowed transition between (0,1)+(1,0) and (0,0)+(1,1), producing the strong van der Waals coefficient C6 = de^4/(9αe). The paper's quantitative engine is a coupled-channel scattering calculation that includes vibrational states in the monomer Hamiltonian, with an absorbing boundary condition modeling sticky collisions; a minimal two-channel model captures the universal scaling.
Load-bearing premise
The application to evaporative cooling assumes that vibrationally excited molecules (v=1, j=0) can be prepared, held, and rethermalized within their ~10–100 ms spontaneous-emission lifetime, so that decay-induced heating does not outpace evaporative cooling; the paper states the lifetime but does not demonstrate a cooling trajectory.
What would settle it
Measure the two-body loss rate coefficient for fermionic NaK molecules in the (0,1)+(1,0) ro-vibrational pair at a few hundred gauss and temperatures around 1 µK, with both molecules in their lowest hyperfine states; the central claim predicts a loss rate near or below 10^-14 cm^3/s with an elastic-to-inelastic ratio of order 15. Finding loss rates orders of magnitude higher (e.g., close to universal s-wave loss) would falsify the repulsive-ro-vibrational-vdW picture. A complementary test is a direct measurement of the C6 coefficient, e.g., through the position of shape resonances or photoasso
If this is right
- Direct evaporative cooling of Fermi mixtures of molecules can work without microwave or electric-field shielding; the computed elastic-to-inelastic ratios are on the order of tens at 1 µK and improve at lower temperature.
- The interaction is universal: for any linear diatomic molecule, the scattering length in units of R_d depends only on αe/E_d, so predictions transfer from NaK and KAg to other species.
- The ro-vibrational vdW force can be combined with double microwave shielding to simultaneously suppress losses in v=0+v=0, v=0+v=1, and v=1+v=1 collisions, enabling stable pseudo-spin 1/2 mixtures with tunable dipolar interactions.
- Because the repulsion is orders of magnitude stronger than the rotational vdW repulsion used previously, it can raise the single-molecule loading fidelity in optical tweezers beyond the ~80% limit.
- The same mechanism can stabilize fermionic molecules in optical lattices against pair loss and provides a state-dependent interaction resource for synthetic dimensions.
Where Pith is reading between the lines
- The paper does not simulate a full evaporative cooling trajectory; a natural next step is a master-equation study that includes the ~10–100 ms lifetime of v=1 and spontaneous-emission heating, to check whether the favorable γ ratios survive in a realistic cooling ramp.
- Because the energy defect 2αe can be tuned by external fields (AC Stark or microwave dressing), the C6 coefficient might be continuously tunable, turning the ro-vibrational vdW interaction into a control knob rather than a fixed property of each molecule species.
- The mechanism should also apply to mixtures of different molecular species with matching ro-vibrational spacings; if an interspecies energy defect can be engineered, one could create repulsive interspecies vdW interactions for dual-species quantum gas experiments.
- The asymmetry noted for microwave shielding—a v=0 molecule appearing non-polar to other v=0 molecules but polar to v=1 impurities—suggests a direct experimental probe: measuring the momentum-resolved radio-frequency spectrum of a v=0 Fermi bath in the presence of v=1 impurities should reveal the predicted strongly interacting polaron.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper proposes and studies a ro-vibrational van der Waals interaction between ultracold polar molecules, arising from second-order dipole-dipole coupling between the pair (v,j)+(v',j')=(0,1)+(1,0) and (0,0)+(1,1). The rotation-vibration coupling constant α_e shifts the nominal degeneracy, producing an energy defect 2α_e and a state-dependent interaction ±C6/R^6, claimed to be repulsive in the upper channel with C6 = d_e^4/(9α_e). The authors tabulate α_e and related constants for bialkalis, laser-coolable molecules, and alkali-coinage-metal molecules; extend their coupled-channel methodology to include vibrational states; compute loss rates for NaK and KAg; demonstrate universal scaling of the scattering length as a function of α_e/E_d; and discuss applications, chiefly evaporative cooling of a Fermi mixture without active shielding and compatibility with double microwave shielding.
Significance. If the quantitative claims hold, the ro-vibrational vdW interaction is a new and unusually strong state-dependent interaction resource, with C6 values up to 10^10 a.u. for KAg and vdW length scales of thousands of bohr. The main strengths are that the input molecular constants are independently tabulated from spectroscopy or potential-energy-curve fits, and the universal scaling is tested against full coupled-channel calculations for two representative molecules, including hyperfine structure and, in separate calculations, microwave fields. The central interaction mechanism is physically plausible and the numerical checks are substantial. The main weakness is the evaporative-cooling application, which is supported only by a γ≈15 rate-coefficient ratio at 1 μK and lacks the density, trap, and lifetime analysis needed to justify the abstract's unqualified word 'enables.'
major comments (3)
- [VII/Abstract] The claim that the mechanism 'enables evaporative cooling of Fermi mixtures ... without active shielding' is not supported by the evidence presented. For NaK at T=1 μK, Fig. 6(a) gives γ≈15 for the elastic s-wave cross-state collision rate relative to the inelastic p-wave same-state rate. This is below the ratio usually required for practical forced evaporation, and the paper provides no cooling trajectory, density, trap-depth, or loss budget to show that γ≈15 suffices. It also does not include the finite lifetime of the v=1 state or the heating accompanying its decay. The text of Sec. VII is appropriately cautious ('could enable'), so the abstract's unqualified 'enables' should either be backed by a quantitative model or tempered.
- [III, Eq. (3)] The central quantitative result C6 = d_e^4/(9α_e) is asserted rather than derived. The reader cannot verify the angular factor 9, the sign convention for α_e, or the statement that this is the isotropic s-wave coefficient. A short derivation from Eq. (3) and the dipole-dipole operator in Eq. (6), including the sums over magnetic quantum numbers and partial waves, should be included. This is load-bearing because all quantitative predictions—the C6 values for NaK and KAg, the length scales R6, and the universal scaling in Eqs. (14)–(15)—depend on this coefficient.
- [VI, Eqs. (14)–(15)] The analytic expression as/R6 ≈ 0.676 for the repulsive van der Waals potential is attributed to an unpublished 'in preparation' reference [88]. This is a standard zero-energy result, but it should be derived in the paper or cited to a published source. More importantly, Eq. (14) is used in the universal model for elastic properties while the inelastic part is obtained numerically; the paper should state why the adiabatic upper-channel expression is valid when inelastic channels are open. The agreement with full coupled-channel results in Fig. 5 is reassuring, but the derivation should be self-contained.
minor comments (4)
- [Fig. 8 caption] Typo: 'transtition' should be 'transition'.
- [VIII] The sentence 'The lifetime of vibrationally excited states is tens of milliseconds' appears in the infrared-shielding discussion and seems to refer to NH. Its relevance to the bialkali molecules used in the evaporative-cooling discussion should be clarified, and quantitative lifetimes for NaK/KAg should be given if known.
- [Fig. 2 caption] The gray adiabatic curves are not labeled by hyperfine state or partial wave in the caption. Please specify which hyperfine states and partial waves are shown.
- [IV] The statement that hyperfine and microwave fields are not included simultaneously should be restated near Fig. 7 so that the domain of the simultaneous-shielding calculation is unambiguous.
Circularity Check
No significant circularity: the ro-vibrational vdW coefficient is computed from independent molecular constants and the suppression claim is tested by coupled-channel dynamics, not refit from its own output.
full rationale
The central result, C6 = d_e^4/(9 alpha_e) for the (v,j)+(v',j') = (0,1)+(1,0) pair, is obtained from second-order perturbation theory, Eq. (3), using the energy denominator 2 alpha_e from the Dunham expansion and the rotational transition dipole d_e. These molecular constants (alpha_e, d_e, B_e, etc.) are taken from spectroscopy, potential-energy-curve fits, or ab initio calculations (Table I), not from the collisional loss rates the paper predicts. There is no fitted parameter that is later renamed as a prediction. The paper's quantitative claims about loss suppression are outputs of coupled-channel scattering calculations with an absorbing boundary condition; the universal minimal model in Sec. VI is explicitly compared with full coupled-channel calculations for NaK and KAg (Fig. 5), and agreement is used to verify universality rather than assumed. The self-citations to prior rotational/hyperfine vdW work [36,37] and to the coupled-channel methodology [32] provide background and method, not the target conclusion; the novel ro-vibrational mechanism is derived and computed within this paper. The only mildly notable self-citation is Eq. (14), attributed to an in-preparation work with overlapping authorship [88]; however, it is a standard zero-energy scattering-length formula for a repulsive C6 potential, it is not fitted to the present results, and its use in the universal scaling is corroborated by the numerical universal curves and by the full coupled-channel markers in Fig. 5. The evaporative-cooling discussion in Sec. VII, with gamma ~15 at 1 microkelvin, may be optimistic, but that is an application-sufficiency concern, not circularity of the derivation. Overall, the paper's derivation chain is self-contained and does not reduce to its inputs.
Axiom & Free-Parameter Ledger
axioms (6)
- domain assumption The Dunham expansion (Eq. 1) with constant αe accurately describes ro-vibrational energies for the manifolds used.
- domain assumption The dipole-dipole interaction (Eq. 6) is the only important long-range interaction; electronic vdW and higher multipoles are absorbed into the short-range capture boundary.
- domain assumption Absorbing boundary conditions at short range model universal collisional loss (sticky collisions).
- standard math Second-order perturbation theory (Eq. 3) with non-degenerate states applies to the (0,1)+(1,0) channel.
- domain assumption Molecules can be prepared in v=1, j=0 with sufficient lifetime (tens of ms) for evaporative cooling and collision experiments.
- domain assumption The vibrational transition dipole moment is weak enough to be neglected in the universal two-level model.
read the original abstract
We describe the ro-vibrational van der Waals interaction between ultracold polar molecules. This interaction is strong, leading to fast elastic collisions and orders of magnitude suppression of collisional loss. This enables evaporative cooling of Fermi mixtures of molecules in different ro-vibrational states, without active shielding by applying external fields. The scheme is compatible with microwave shielding, where it enables controlled state dependent interactions, opening up new opportunities for quantum simulation and impurity physics. The interaction can also be used to stabilize fermionic molecules in optical lattices, to control interactions in synthetic dimensions, for enhanced tweezer loading, and direct infrared shielding.
Figures
Forward citations
Cited by 5 Pith papers
-
Deterministic loading of molecular arrays by microwave-assisted collisions
Microwave-assisted collisions with repulsive van der Waals shelving are predicted to load single molecules into tweezers at 87-96% filling fractions, up from the current 30-40%.
-
Deterministic loading of molecular arrays by microwave-assisted collisions
Shelving molecules in rotationally or vibrationally excited states and driving microwave-assisted collisions can suppress loss, eject one molecule deterministically, and yield predicted filling fractions up to 96%.
-
Tunable state-dependent interactions in collisionally stable mixtures of polar molecules
Vibrational states v=0 and v=1 of microwave-shielded polar molecules form a collisionally stable pseudo-spin with tunable dipolar Ising, density-density, and spin-density interactions.
-
Tunable state-dependent interactions in collisionally stable mixtures of polar molecules
Microwave-shielded polar molecules in vibrational states v=0 and v=1 realize tunable Ising, density-density, and spin-density dipolar interactions with suppressed two-body losses.
-
Tunable two-component ultracold molecular gases with vibrational shielding
Vibrational-state-dependent repulsive shielding can stabilize and independently tune two-component ultracold molecular mixtures.
Reference graph
Works this paper leans on
-
[1]
Karman, M
T. Karman, M. Tomza, and J. P´ erez-R ´ ıos, Nature Phys. 20, 722 (2024)
2024
-
[2]
N. R. Cooper and G. V. Shlyapnikov, Phys. Rev. Lett. 103, 155302 (2009)
2009
-
[3]
A. V. Gorshkov, S. R. Manmana, G. Chen, J. Ye, E. Demler, M. D. Lukin, and A. M. Rey, Phys. Rev. Lett. 107, 115301 (2011)
2011
-
[4]
Micheli, G
A. Micheli, G. K. Brennen, and P. Zoller, Nature Physics 2, 341 (2006)
2006
-
[5]
S. L. Cornish, M. R. Tarbutt, and K. R. Hazzard, Nature Physics20, 730 (2024)
2024
-
[6]
DeMille, Phys
D. DeMille, Phys. Rev. Lett.88, 067901 (2002)
2002
-
[7]
D. K. Ruttley, T. R. Hepworth, A. Guttridge, and S. L. Cornish, Nature637, 827–832 (2025)
2025
-
[8]
L. R. Picard, A. J. Park, G. E. Patenotte, S. Gebretsad- kan, D. Wellnitz, A. M. Rey, and K.-K. Ni, Nature637, 821 (2025)
2025
-
[9]
C. M. Holland, Y. Lu, and L. W. Cheuk, Science382, 1143 (2023)
2023
-
[10]
Y. Bao, S. S. Yu, L. Anderegg, E. Chae, W. Ketterle, K.-K. Ni, and J. M. Doyle, Science382, 1138 (2023)
2023
-
[11]
DeMille, N
D. DeMille, N. R. Hutzler, A. M. Rey, and T. Zelevinsky, 13 Nature Physics20, 741 (2024)
2024
-
[12]
M. S. Safronova, D. Budker, D. DeMille, D. F. J. Kimball, A. Derevianko, and C. W. Clark, Rev. Mod. Phys.90, 025008 (2018)
2018
-
[13]
Langen, G
T. Langen, G. Valtolina, D. Wang, and J. Ye, Nature Physics20, 702 (2024)
2024
-
[14]
M. L. Wall and L. Carr, Phys. Rev. A82, 013611 (2010)
2010
-
[15]
Trefzger, C
C. Trefzger, C. Menotti, B. Capogrosso-Sansone, and M. Lewenstein, J. Phys. B.44, 193001 (2011)
2011
-
[16]
Capogrosso-Sansone, C
B. Capogrosso-Sansone, C. Trefzger, M. Lewenstein, P. Zoller, and G. Pupillo, Phys. Rev. Lett.104, 125301 (2010)
2010
-
[17]
Barnett, D
R. Barnett, D. Petrov, M. Lukin, and E. Demler, Phys. Rev. Lett.96, 190401 (2006)
2006
-
[18]
A. N. Carroll, H. Hirzler, C. Miller, D. Wellnitz, S. R. Muleady, J. Lin, K. P. Zamarski, R. R. Wang, J. L. Bohn, A. M. Rey,et al., Science388, 381 (2025)
2025
-
[19]
W. Zhang, H. Liu, F. Deng, K. Chen, S. Yi, and T. Shi, arXiv preprint arXiv:2506.23820 (2025)
Pith/arXiv arXiv 2025
-
[20]
Langen, J
T. Langen, J. Boronat, J. S´ anchez-Baena, R. Bomb ´ ın, T. Karman, and F. Mazzanti, Phys. Rev. Lett.134, 053001 (2025)
2025
-
[21]
Ciardi, K
M. Ciardi, K. R. Pedersen, T. Langen, and T. Pohl, Phys. Rev. Lett.135, 153401 (2025)
2025
-
[22]
Mukherjee, J
B. Mukherjee, J. M. Hutson, and K. R. Hazzard, New. J. Phys.27, 013013 (2025)
2025
-
[23]
Sundar, B
B. Sundar, B. Gadway, and K. R. Hazzard, Scientific re- ports8, 3422 (2018)
2018
-
[24]
C. Feng, H. Manetsch, V. G. Rousseau, K. R. Hazzard, and R. Scalettar, Phys. Rev. A105, 063320 (2022)
2022
-
[25]
De Marco, G
L. De Marco, G. Valtolina, K. Matsuda, W. G. Tobias, J. P. Covey, and J. Ye, Science363, 853 (2019)
2019
-
[26]
Valtolina, K
G. Valtolina, K. Matsuda, W. G. Tobias, J.-R. Li, L. De Marco, and J. Ye, Nature588, 239 (2020)
2020
-
[27]
Matsuda, L
K. Matsuda, L. De Marco, J.-R. Li, W. G. Tobias, G. Valtolina, G. Qu´ em´ ener, and J. Ye, Science370, 1324 (2020)
2020
-
[28]
Schindewolf, R
A. Schindewolf, R. Bause, X.-Y. Chen, M. Duda, T. Kar- man, I. Bloch, and X.-Y. Luo, Nature607, 677 (2022)
2022
-
[29]
Bigagli, W
N. Bigagli, W. Yuan, S. Zhang, B. Bulatovic, T. Karman, I. Stevenson, and S. Will, Nature631, 289 (2024)
2024
-
[30]
Z. Shi, Z. Huang, F. Deng, W.-J. Jin, S. Yi, T. Shi, and D. Wang, Bose-einstein condensate of ultracold sodium- rubidium molecules with tunable dipolar interactions (2025), arXiv:2508.20518 [cond-mat.quant-gas]
Pith/arXiv arXiv 2025
-
[31]
W. Yuan, S. Zhang, N. Bigagli, H. Kwak, C. Warner, T. Karman, I. Stevenson, and S. Will, arXiv preprint arXiv:2505.08773 (2025)
Pith/arXiv arXiv 2025
-
[32]
Karman, N
T. Karman, N. Bigagli, W. Yuan, S. Zhang, I. Stevenson, and S. Will, PRX Quantum6, 020358 (2025)
2025
-
[33]
X.-Y. Chen, A. Schindewolf, S. Eppelt, R. Bause, M. Duda, S. Biswas, T. Karman, T. Hilker, I. Bloch, and X.-Y. Luo, Nature614, 59 (2023)
2023
-
[34]
Zhang, W
S. Zhang, W. Yuan, N. Bigagli, H. Kwak, T. Karman, I. Stevenson, and S. Will, Nature651, 601–606 (2026)
2026
-
[35]
A. Schindewolf, J. Hertkorn, I. Stevenson, M. Ciardi, P. Gross, D. Wang, T. Karman, G. Quemener, S. Will, T. Pohl,et al., arXiv preprint arXiv:2512.14511 (2025)
Pith/arXiv arXiv 2025
-
[36]
E. F. Walraven and T. Karman, Phys. Rev. A109, 043310 (2024)
2024
-
[37]
E. F. Walraven and T. Karman, Phys. Rev. A112, 032810 (2025)
2025
-
[38]
X. Ye, M. Guo, M. L. Gonz´ alez-Mart ´ ınez, G. Qu´ em´ ener, and D. Wang, Science advances4, eaaq0083 (2018)
2018
-
[39]
Kozyryev and N
I. Kozyryev and N. R. Hutzler, Phys. Rev. Lett.119, 133002 (2017)
2017
-
[40]
N. R. Hutzler, Quantum Science & Technology5, 044011 (2020)
2020
-
[41]
Anderegg, N
L. Anderegg, N. B. Vilas, C. Hallas, P. Robichaud, A. Jadbabaie, J. M. Doyle, and N. R. Hutzler, Science 382, 665 (2023)
2023
-
[42]
L. D. Augustoviˇ cov´ a and J. L. Bohn, New. J. Phys.21, 103022 (2019)
2019
-
[43]
N. B. Vilas, P. Robichaud, C. Hallas, J. Tao, L. An- deregg, G. K. Li, H. Lampson, L. D. Augustoviˇ cov´ a, J. L. Bohn, and J. M. Doyle, Phys. Rev. X16, 021001 (2026)
2026
-
[44]
K.-K. Ni, S. Ospelkaus, M. De Miranda, A. Pe’Er, B. Neyenhuis, J. Zirbel, S. Kotochigova, P. Julienne, D. Jin, and J. Ye, Science322, 231 (2008)
2008
-
[45]
Takekoshi, L
T. Takekoshi, L. Reichs¨ ollner, A. Schindewolf, J. M. Hut- son, C. R. Le Sueur, O. Dulieu, F. Ferlaino, R. Grimm, and H.-C. N¨ agerl, Phys. Rev. Lett.113, 205301 (2014)
2014
-
[46]
P. K. Molony, P. D. Gregory, Z. Ji, B. Lu, M. P. K¨ oppinger, C. R. Le Sueur, C. L. Blackley, J. M. Hutson, and S. L. Cornish, Phys. Rev. Lett.113, 255301 (2014)
2014
-
[47]
J. W. Park, S. A. Will, and M. W. Zwierlein, Phys. Rev. Lett.114, 205302 (2015)
2015
-
[48]
M. Guo, B. Zhu, B. Lu, X. Ye, F. Wang, R. Vex- iau, N. Bouloufa-Maafa, G. Qu´ em´ ener, O. Dulieu, and D. Wang, Phys. Rev. Lett.116, 205303 (2016)
2016
-
[49]
Stevenson, A
I. Stevenson, A. Z. Lam, N. Bigagli, C. Warner, W. Yuan, S. Zhang, and S. Will, Phys. Rev. Lett.130, 113002 (2023)
2023
-
[50]
Zhelyazkova, A
V. Zhelyazkova, A. Cournol, T. E. Wall, A. Matsushima, J. J. Hudson, E. Hinds, M. Tarbutt, and B. Sauer, Phys. Rev. A89, 053416 (2014)
2014
-
[51]
E. S. Shuman, J. F. Barry, and D. DeMille, Nature467, 820 (2010)
2010
-
[52]
Rockenh¨ auser, F
M. Rockenh¨ auser, F. Kogel, T. Garg, S. A. Morales- Ram ´ ırez, and T. Langen, Phys. Rev. Res.6, 043161 (2024)
2024
-
[53]
A. L. Collopy, S. Ding, Y. Wu, I. A. Finneran, L. An- deregg, B. L. Augenbraun, J. M. Doyle, and J. Ye, Phys. Rev. Lett.121, 213201 (2018)
2018
-
[54]
Dunham, Phys
J. Dunham, Phys. Rev.41, 721 (1932)
1932
-
[55]
C. L. Pekeris, Phys. Rev.45, 98 (1934)
1934
-
[56]
Kratzer, Zeits
A. Kratzer, Zeits. f. Physik3, 289 (1920)
1920
-
[57]
C. E. Burkhardt and J. J. Leventhal, Am. J. Phys.75, 686 (2007)
2007
-
[58]
Docenko, M
O. Docenko, M. Tamanis, R. Ferber, A. Pashov, H. Kn¨ ockel, and E. Tiemann, Eur. Phys. J. D31, 205 (2004)
2004
-
[59]
Docenko, M
O. Docenko, M. Tamanis, R. Ferber, H. Kn¨ ockel, and E. Tiemann, Phys. Rev. A
-
[60]
Pashov, O
A. Pashov, O. Docenko, M. Tamanis, R. Ferber, H. Kn¨ ockel, and E. Tiemann, Phys. Rev. A72, 062505 (2005)
2005
-
[61]
Pashov, O
A. Pashov, O. Docenko, M. Tamanis, R. Ferber, H. Kn¨ ockel, and E. Tiemann, Phys. Rev. A76, 022511 (2007)
2007
-
[62]
Steinke, H
M. Steinke, H. Kn¨ ockel, and E. Tiemann, Phys. Rev. A 85, 042720 (2012)
2012
-
[63]
Ferber, I
R. Ferber, I. Klincare, O. Nikolayeva, M. Tamanis, H. Kn¨ ockel, E. Tiemann, and A. Pashov, Phys. Rev. A 80, 062501 (2009)
2009
-
[64]
Ivanova, A
M. Ivanova, A. Stein, A. Pashov, H. Kn¨ ockel, and E. Tie- mann, J. Chem. Phys.134, 024321 (2011)
2011
-
[65]
Tiemann, H
E. Tiemann, H. Kn¨ ockel, P. Kowalczyk, W. Jastrzebski, 14 A. Pashov, H. Salami, and A. Ross, Phys. Rev. A79, 042716 (2009)
2009
-
[66]
´Smia lkowski and M
M. ´Smia lkowski and M. Tomza, Phys. Rev. A103, 022802 (2021)
2021
-
[67]
Aymar and O
M. Aymar and O. Dulieu, J. Chem. Phys.122(2005)
2005
-
[68]
Ladjimi and M
H. Ladjimi and M. Tomza, Phys. Rev. A109, 052814 (2024)
2024
-
[69]
Koput, J
J. Koput, J. Comput. Chem.36, 1286 (2015)
2015
-
[70]
Radford and M
H. Radford and M. Litvak, Chem. Phys. Lett.34, 561 (1975)
1975
-
[71]
Wayne and H
F. Wayne and H. Radford, Mol. Phys.32, 1407 (1976)
1976
-
[72]
T¨ orring, W
T. T¨ orring, W. Ernst, and S. Kindt, J. Chem. Phys.81, 4614 (1984)
1984
-
[73]
Private communication from Luk´ aˇ s Paˇ steka and Anasta- sia Borshevsky, based on MRCI calculations similar to those reported in J. Chem. Phys.,151034302 (2019), but using a smaller basis set
2019
-
[74]
K. P. Huber and G. Herzberg,Molecular Spectra and Molecular Structure(Springer US, 1979)
1979
-
[75]
Childs, G
W. Childs, G. Goodman, and L. Goodman, J. Mol. Spectr.115, 215 (1986)
1986
-
[76]
Y. Hao, L. F. Paˇ steka, L. Visscher, P. Aggarwal, H. L. Bethlem, A. Boeschoten, A. Borschevsky, M. Denis, K. Esajas, S. Hoekstra, K. Jungmann, V. R. Marshall, T. B. Meijknecht, M. C. Mooij, R. G. E. Timmermans, A. Touwen, W. Ubachs, L. Willmann, Y. Yin, A. Za- para, and N. eEDM Collaboration), J. Chem. Phys.151, 034302 (2019)
2019
-
[77]
M. A. Anderson, M. D. Allen, and L. M. Ziurys, Astro- phys. J.424, 503 (1994)
1994
-
[78]
Ernst, J
W. Ernst, J. K¨ andler, S. Kindt, and T. T¨ orring, Chem. Phys. Lett.113, 351 (1985)
1985
-
[79]
R. D. Suenram, F. J. Lovas, G. T. Fraser, and K. Mat- sumura, J. Chem. Phys.92, 4724 (1990)
1990
-
[80]
Staanum, A
P. Staanum, A. Pashov, H. Kn¨ ockel, and E. Tiemann, Phys. Rev. A75, 042513 (2007)
2007
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