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arxiv: 1906.10539 · v1 · pith:FRF67GIEnew · submitted 2019-06-23 · ⚛️ nucl-th · nucl-ex

Ab initio Gamow in-medium similarity renormalization group with resonance and continuum

Pith reviewed 2026-05-25 17:47 UTC · model grok-4.3

classification ⚛️ nucl-th nucl-ex
keywords Gamow IMSRGBerggren basisnuclear resonancescontinuumab initio calculationshalo nuclei24O22C
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The pith

The Gamow IMSRG in the Berggren framework describes resonance and continuum properties of weakly bound nuclear systems.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

This paper presents the development of an ab initio Gamow in-medium similarity renormalization group method using the complex-energy Berggren basis. The approach is designed to handle resonances and nonresonant continua in open nuclear systems. Using chiral two- and three-nucleon forces, it reproduces resonant states in the neutron-dripline nucleus 24O. Calculations also show the halo structure of the Borromean nucleus 22C, with the continuum s channel contributing significantly to the density distribution.

Core claim

The Gamow IMSRG is capable of describing the resonance and nonresonant continuum properties of weakly bound and unbound nuclear many-body systems, as demonstrated by reproducing resonant states in 24O and the halo structure in 22C where the continuum s channel plays a crucial role.

What carries the argument

Gamow IMSRG extended to the Berggren basis, which allows inclusion of resonant and scattering states in many-body calculations.

If this is right

  • Resonant states observed in 24O are well reproduced.
  • The halo structure of 22C is seen in the density distribution with continuum s channel contribution.
  • Low-lying resonant excited states in 22C are predicted.
  • Tractable ab initio calculations for weakly bound and unbound open quantum systems are enabled.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • This could allow predictions for other unstable nuclei near the dripline.
  • The method might be extended to study nuclear reactions involving continua.
  • Further work could test sensitivity to different chiral force parametrizations.

Load-bearing premise

The Berggren basis with the chosen chiral forces and IMSRG truncation level captures the essential resonance and continuum physics in these nuclei.

What would settle it

Failure to reproduce the observed resonant states in 24O or the halo characteristics in 22C would falsify the claim that the method adequately describes these properties.

Figures

Figures reproduced from arXiv: 1906.10539 by B. S. Hu, F. R. Xu, Q. Wu, Z. H. Sun.

Figure 1
Figure 1. Figure 1: FIG. 1 [PITH_FULL_IMAGE:figures/full_fig_p007_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: FIG. 2. Calculated [PITH_FULL_IMAGE:figures/full_fig_p008_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: FIG. 3. Excited states in [PITH_FULL_IMAGE:figures/full_fig_p010_3.png] view at source ↗
read the original abstract

We have developed a novel ab initio Gamow in-medium similarity renormalization group (Gamow IMSRG) in the complex-energy Berggren framework. The advanced Gamow IMSRG is capable of describing the resonance and nonresonant continuum properties of weakly bound and unbound nuclear many-body systems. As test grounds, carbon and oxygen isotopes have been calculated with chiral two- and three-nucleon forces from the effective field theory. Resonant states observed in the neutron-dripline 24O are well reproduced. The halo structure of the known heaviest Borromean nucleus 22C is clearly seen by calculating the density distribution in which the continuum s channel plays a crucial role. Furthermore, we predict low-lying resonant excited states in 22C. The Gamow IMSRG provides tractable ab initio calculations of weakly bound and unbound open quantum systems.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

2 major / 2 minor

Summary. The manuscript introduces the Gamow IMSRG method formulated in the complex-energy Berggren basis to treat resonances and nonresonant continua in ab initio nuclear many-body calculations. Using chiral two- and three-nucleon forces, the approach is applied to oxygen and carbon isotopes; it reports reproduction of observed resonances in the neutron-dripline nucleus 24O, visualization of the s-wave halo density in the Borromean nucleus 22C, and predictions for low-lying resonant states in 22C.

Significance. If validated, the method supplies a tractable ab initio route to open quantum systems near the dripline, extending the IMSRG framework to handle continuum degrees of freedom without phenomenological adjustments. This addresses a long-standing limitation in calculations of weakly bound and unbound nuclei.

major comments (2)
  1. [§4] §4 (results on 24O): the claim that resonant states are 'well reproduced' is presented without reported uncertainties, basis-size extrapolations, or comparisons against independent many-body methods; this quantitative support is load-bearing for the central assertion that the Gamow IMSRG is capable of describing resonance properties.
  2. [§3, §5] §3 (Berggren implementation) and §5 (22C density): no convergence tests with respect to the number of discretized continuum states, choice of contour, or IMSRG truncation level (e.g., IMSRG(2) vs. higher) are shown; the sufficiency of these modeling choices for capturing continuum-induced correlations is therefore untested and directly underpins the halo-structure and prediction claims.
minor comments (2)
  1. [§2] Notation for the Berggren basis states and the complex scaling parameter should be defined explicitly in the text rather than only in a figure caption.
  2. [§2] The abstract states that 'chiral two- and three-nucleon forces from the effective field theory' are employed; the specific interaction (e.g., NNLO_sat or EM1.8/2.0) and cutoff values should be stated in the methods section for reproducibility.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for the positive assessment of the work's significance and for the detailed, constructive comments. We respond to each major comment below and indicate planned revisions.

read point-by-point responses
  1. Referee: [§4] §4 (results on 24O): the claim that resonant states are 'well reproduced' is presented without reported uncertainties, basis-size extrapolations, or comparisons against independent many-body methods; this quantitative support is load-bearing for the central assertion that the Gamow IMSRG is capable of describing resonance properties.

    Authors: We agree that the claim would be strengthened by additional quantitative support. In the revised manuscript we will add basis-size extrapolations for the 24O resonant states, report estimated uncertainties arising from the chiral interactions and model-space choices, and include comparisons with available results from other ab initio approaches. revision: yes

  2. Referee: [§3, §5] §3 (Berggren implementation) and §5 (22C density): no convergence tests with respect to the number of discretized continuum states, choice of contour, or IMSRG truncation level (e.g., IMSRG(2) vs. higher) are shown; the sufficiency of these modeling choices for capturing continuum-induced correlations is therefore untested and directly underpins the halo-structure and prediction claims.

    Authors: We acknowledge that explicit convergence tests are needed. In the revised manuscript we will include figures and discussion demonstrating convergence with respect to the number of discretized continuum states and the choice of contour in both §3 and §5. The present implementation is at the IMSRG(2) level; we will add a discussion of the expected truncation error and note that systematic studies at higher truncation orders are planned for future work. revision: partial

Circularity Check

0 steps flagged

No significant circularity; computational outputs from ab initio method validated against external data

full rationale

The paper presents the Gamow IMSRG method in the Berggren basis with chiral NN+3N forces from EFT. Results consist of direct numerical computations for carbon and oxygen isotopes, reproducing known resonant states in 24O and computing halo densities plus new predictions for 22C. These are not reductions of outputs to inputs by construction, nor do they rely on fitted parameters renamed as predictions, self-definitional loops, or load-bearing self-citations that substitute for independent derivation. Validation occurs via comparison to external experimental observations rather than internal tautology. Standard citations to prior IMSRG formalism are present but do not carry the uniqueness or central claim; the method is self-contained against benchmarks.

Axiom & Free-Parameter Ledger

0 free parameters · 1 axioms · 0 invented entities

The central claim rests on domain-standard assumptions in nuclear many-body theory; no free parameters or invented entities are introduced in the abstract beyond the established chiral EFT forces and Berggren basis.

axioms (1)
  • domain assumption Chiral effective field theory supplies appropriate two- and three-nucleon forces for ab initio nuclear calculations
    The paper applies these forces to carbon and oxygen isotopes as the interaction input.

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Works this paper leans on

61 extracted references · 61 canonical work pages

  1. [1]

    Okoowicz, M

    J. Okoowicz, M. Poszajczak, and I. Rotter, Phys. Rep. 374, 271 (2003)

  2. [2]

    Michel, W

    N. Michel, W. Nazarewicz, M. P/suppress loszajczak, and T. Vertse , J. Phys. G: Nucl. Part. Phys. 36, 013101 (2009)

  3. [3]

    Tanihata, H

    I. Tanihata, H. Hamagaki, O. Hashimoto, Y. Shida, N. Yosh ikawa, K. Sugimoto, O. Yamakawa, T. Kobayashi, and N. Takahashi, Phys. Rev. Lett. 55, 2676 (1985)

  4. [4]

    A. S. Jensen, K. Riisager, D. V. Fedorov, and E. Garrido, Rev. Mod. Phys. 76, 215 (2004)

  5. [5]

    Id Betan, R

    R. Id Betan, R. J. Liotta, N. Sandulescu, and T. Vertse, Phys. Rev. Lett. 89, 042501 (2002)

  6. [6]

    Michel, W

    N. Michel, W. Nazarewicz, M. P/suppress loszajczak, and K. Bennac eur, Phys. Rev. Lett. 89, 042502 (2002) . 11

  7. [7]

    Kanungo et al

    R. Kanungo et al. , Phys. Rev. Lett. 114, 192502 (2015)

  8. [8]

    Fossez, J

    K. Fossez, J. Rotureau, N. Michel, Q. Liu, and W. Nazarewi cz, Phys. Rev. C 94, 054302 (2016)

  9. [9]

    Bennaceur, F

    K. Bennaceur, F. Nowacki, J. Oko/suppress lowicz, and M. P/suppress loszajczak, Nucl. Phys. A 651, 289 (1999)

  10. [10]

    Volya and V

    A. Volya and V. Zelevinsky, Phys. Rev. Lett. 94, 052501 (2005)

  11. [11]

    Hagen, D

    G. Hagen, D. J. Dean, M. Hjorth-Jensen, and T. Papenbroc k, Phys. Lett. B 656, 169 (2007)

  12. [12]

    Hagen, M

    G. Hagen, M. Hjorth-Jensen, G. R. Jansen, R. Machleidt, and T. Papenbrock, Phys. Rev. Lett. 108, 242501 (2012)

  13. [13]

    Tsukiyama, T

    K. Tsukiyama, T. Otsuka, and R. Fujimoto, Prog. Theor. Exp. Phys. 2015, 093D01 (2015)

  14. [14]

    S. D. G/suppress lazek and K. G. Wilson,Phys. Rev. D 48, 5863 (1993)

  15. [15]

    Wegner, Ann

    F. Wegner, Ann. Phys. (Leipzig) 506, 77 (1994)

  16. [16]

    S. K. Bogner, R. J. Furnstahl, and R. J. Perry, Phys. Rev. C 75, 061001(R) (2007)

  17. [17]

    Hergert and R

    H. Hergert and R. Roth, Phys. Rev. C 75, 051001(R) (2007)

  18. [18]

    Tsukiyama, S

    K. Tsukiyama, S. K. Bogner, and A. Schwenk, Phys. Rev. Lett. 106, 222502 (2011)

  19. [19]

    Hergert, S

    H. Hergert, S. Bogner, T. Morris, A. Schwenk, and K. Tsuk iyama, Phys. Rep. 621, 165 (2016)

  20. [20]

    Tsukiyama, S

    K. Tsukiyama, S. K. Bogner, and A. Schwenk, Phys. Rev. C 85, 061304(R) (2012)

  21. [21]

    S. K. Bogner, H. Hergert, J. D. Holt, A. Schwenk, S. Binde r, A. Calci, J. Langhammer, and R. Roth, Phys. Rev. Lett. 113, 142501 (2014)

  22. [22]

    Hergert, S

    H. Hergert, S. Binder, A. Calci, J. Langhammer, and R. Ro th, Phys. Rev. Lett. 110, 242501 (2013)

  23. [23]

    S. R. Stroberg, A. Calci, H. Hergert, J. D. Holt, S. K. Bog ner, R. Roth, and A. Schwenk, Phys. Rev. Lett. 118, 032502 (2017)

  24. [24]

    N. M. Parzuchowski, T. D. Morris, and S. K. Bogner, Phys. Rev. C 95, 044304 (2017)

  25. [25]

    N. M. Parzuchowski, S. R. Stroberg, P. Navr´ atil, H. Her gert, and S. K. Bogner, Phys. Rev. C 96, 034324 (2017)

  26. [26]

    Gebrerufael, K

    E. Gebrerufael, K. Vobig, H. Hergert, and R. Roth, Phys. Rev. Lett. 118, 152503 (2017)

  27. [27]

    Berggren, Nucl

    T. Berggren, Nucl. Phys. A 109, 265 (1968)

  28. [28]

    Liotta, E

    R. Liotta, E. Maglione, N. Sandulescu, and T. Vertse, Phys. Lett. B 367, 1 (1996)

  29. [29]

    Hagen, M

    G. Hagen, M. Hjorth-Jensen, and N. Michel, Phys. Rev. C 73, 064307 (2006)

  30. [30]

    Papadimitriou, J

    G. Papadimitriou, J. Rotureau, N. Michel, M. P/suppress loszajc zak, and B. R. Barrett, 12 Phys. Rev. C 88, 044318 (2013)

  31. [31]

    Z. H. Sun, Q. Wu, Z. H. Zhao, B. S. Hu, S. J. Dai, and F. R. Xu, Phys. Lett. B 769, 227 (2017)

  32. [32]

    Tanaka et al

    K. Tanaka et al. , Phys. Rev. Lett. 104, 062701 (2010)

  33. [33]

    Kobayashi et al

    N. Kobayashi et al. , Phys. Rev. C 86, 054604 (2012)

  34. [34]

    Gaudefroy et al

    L. Gaudefroy et al. , Phys. Rev. Lett. 109, 202503 (2012)

  35. [35]

    Togano et al

    Y. Togano et al. , Phys. Lett. B 761, 412 (2016)

  36. [36]

    Ekstr¨ om, G

    A. Ekstr¨ om, G. Baardsen, C. Forss´ en, G. Hagen, M. Hjor th-Jensen, G. R. Jansen, R. Machleidt, W. Nazarewicz, T. Papenbrock, J. Sarich, and S . M. Wild, Phys. Rev. Lett. 110, 192502 (2013)

  37. [37]

    Ekstr¨ om, G

    A. Ekstr¨ om, G. R. Jansen, K. A. Wendt, G. Hagen, T. Papenbrock, B. D. Carlsson, C. Forss´ en, M. Hjorth-Jensen, P. Navr´ atil, and W. Nazarewicz, Phys. Rev. C 91, 051301(R) (2015)

  38. [38]

    Hebeler, H

    K. Hebeler, H. Krebs, E. Epelbaum, J. Golak, and R. Skibi ´ nski, Phys. Rev. C 91, 044001 (2015)

  39. [39]

    S. M. Wang and W. Nazarewicz, Phys. Rev. Lett. 120, 212502 (2018)

  40. [40]

    T. D. Morris, N. M. Parzuchowski, and S. K. Bogner, Phys. Rev. C 92, 034331 (2015)

  41. [41]

    Hagen, T

    G. Hagen, T. Papenbrock, D. J. Dean, A. Schwenk, A. Nogga , M. W/suppress loch, and P. Piecuch, Phys. Rev. C 76, 034302 (2007)

  42. [42]

    R. Roth, S. Binder, K. Vobig, A. Calci, J. Langhammer, an d P. Navr´ atil, Phys. Rev. Lett. 109, 052501 (2012)

  43. [43]

    T. Heng, J. P. Vary, and P. Maris, Phys. Rev. C 95, 014306 (2017)

  44. [44]

    B. S. Hu, F. R. Xu, Z. H. Sun, J. P. Vary, and T. Li, Phys. Rev. C 94, 014303 (2016)

  45. [45]

    B. S. Hu, Q. Wu, and F. R. Xu, Chin. Phys. C 41, 104101 (2017)

  46. [46]

    Henderson et al

    J. Henderson et al. , Phys. Lett. B 782, 468 (2018)

  47. [47]

    T. D. Morris, Systematic improvements of ab-initio in-medium similarit y renormalization group calculations (Ph.D. thesis, Michigan State University, Michigan, 2016)

  48. [48]

    F. A. Evangelista, J. Chem. Phys. 141, 054109 (2014)

  49. [49]

    F. A. Evangelista and J. Gauss, Chem. Phys. 401, 27 (2012)

  50. [50]

    R. D. Lawson, Theory of the Nuclear Shell Model (Oxford University Press, 1980)

  51. [51]

    Hagen, T

    G. Hagen, T. Papenbrock, and D. J. Dean, Phys. Rev. Lett. 103, 062503 (2009)

  52. [52]

    C. R. Hoffman et al. , Phys. Lett. B 672, 17 (2009) . 13

  53. [53]

    C. R. Hoffman et al. , Phys. Rev. C 83, 031303(R) (2011)

  54. [54]

    Acharya, C

    B. Acharya, C. Ji, and D. Phillips, Phys. Lett. B 723, 196 (2013)

  55. [55]

    Suzuki, T

    T. Suzuki, T. Otsuka, C. Yuan, and N. Alahari, Phys. Lett. B 753, 199 (2016)

  56. [56]

    X. X. Sun, J. Zhao, and S. G. Zhou, Phys. Lett. B 785, 530 (2018)

  57. [57]

    Nagahisa and W

    T. Nagahisa and W. Horiuchi, Phys. Rev. C 97, 054614 (2018)

  58. [58]

    Kanungo et al

    R. Kanungo et al. , Phys. Rev. Lett. 117, 102501 (2016)

  59. [59]

    Hagen, private communication (2018)

    G. Hagen, private communication (2018)

  60. [60]

    Coraggio, A

    L. Coraggio, A. Covello, A. Gargano, and N. Itaco, Phys. Rev. C 81, 064303 (2010)

  61. [61]

    G. R. Jansen, J. Engel, G. Hagen, P. Navratil, and A. Sign oracci, Phys. Rev. Lett. 113, 142502 (2014) . 14