pith. sign in

arxiv: 2605.16890 · v1 · pith:3MLLAGMSnew · submitted 2026-05-16 · ⚛️ nucl-th

A self-consistent spectral framework for inclusive non-elastic breakup, with the Trojan Horse method as the sub-Coulomb resonant limit

Pith reviewed 2026-05-19 19:08 UTC · model grok-4.3

classification ⚛️ nucl-th
keywords Trojan Horse Methodinclusive non-elastic breakupdistorted-wave Born approximationresonance strengthsub-Coulomb reactionsIAV frameworkR-matrixoptical potential ansatz
0
0 comments X

The pith

The Trojan Horse Method resonance formula reduces from the per-pole DWBA cross section under four specific approximations.

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

This paper connects the Ichimura-Austern-Vincent inclusive non-elastic breakup framework to the Trojan Horse Method used for low-energy resonance strengths in nuclear astrophysics. It introduces a diagonal isolated-pole spectral ansatz for the absorptive participant-target optical potential that reduces the IAV cross section to a sum of per-pole DWBA pole cross sections weighted by branching ratios in the isolated-resonance limit. The factorized PWIA-THM formula then appears as a further non-perturbative reduction of each per-pole DWBA term when plane-wave substitution, zero-range or surface-localized interaction, on-shell vertex evaluation, and post-form remnant neglect are applied. A reader would care because this makes the per-pole DWBA pole cross section the direct quantity for sub-Coulomb resonance-strength extraction rather than an ad-hoc correction to the THM formula.

Core claim

The factorized PWIA-THM resonance-strength formula is identified as a non-perturbative reduction of the per-pole DWBA cross section under four approximations: plane-wave substitution on the entrance and exit distorted waves, zero-range or surface-localized treatment of the spectator-participant interaction, on-shell evaluation of the binary subreaction vertex, and post-form remnant neglect. The IAV inclusive cross section reduces in the isolated-resonance limit to a sum of per-pole DWBA pole cross sections weighted by channel branching ratios when the diagonal isolated-pole spectral ansatz is adopted for the absorptive participant-target optical potential. The per-pole DWBA pole cross is the

What carries the argument

The diagonal isolated-pole spectral ansatz for the absorptive participant-target optical potential, which enforces the isolated-resonance limit and allows the IAV cross section to reduce to weighted per-pole DWBA terms.

If this is right

  • Resonance strengths in sub-Coulomb transfer reactions are extracted directly from per-pole DWBA cross sections rather than from a separate THM formula.
  • The four reduction steps become explicit checks that can be validated or relaxed in future analyses.
  • Branching ratios from R-matrix tabulations weight the individual pole contributions in the inclusive breakup spectrum.
  • The same spectral ansatz supplies a diagnostic for continuum decoupling that can be tested against measured spectra.

Where Pith is reading between the lines

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

  • Error budgets for astrophysical reaction rates derived from THM data could be tightened by propagating uncertainties from the four explicit approximations.
  • The framework suggests a path to extend consistent extraction methods above the Coulomb barrier by relaxing only the plane-wave substitution.
  • Direct measurements sensitive to the exit-channel distortion could test whether the DWBA pole term remains the dominant extraction quantity.

Load-bearing premise

The absorptive participant-target optical potential admits a diagonal isolated-pole spectral representation whose three validity conditions hold for the resonances of interest.

What would settle it

A numerical comparison, for a known isolated resonance, between the full IAV cross section computed with the isolated-pole ansatz and the reduced per-pole DWBA expression obtained after applying the four approximations would show whether any extra multiplicative factor appears.

Figures

Figures reproduced from arXiv: 2605.16890 by Jin Lei.

Figure 1
Figure 1. Figure 1: FIG. 1. Two-step non-perturbative reduction from the IAV [PITH_FULL_IMAGE:figures/full_fig_p005_1.png] view at source ↗
read the original abstract

The Trojan Horse Method (THM) extracts low-energy charged-particle resonance strengths through a plane-wave impulse approximation (PWIA) reduction of a three-body transfer matrix element. The Ichimura-Austern-Vincent (IAV) inclusive non-elastic breakup framework has not been brought to the sub-Coulomb astrophysical regime where THM operates. I introduce a diagonal isolated-pole spectral ansatz for the absorptive participant-target optical potential with three explicit validity conditions, two closed by $R$-matrix tabulations and the third a model-dependent continuum-decoupling diagnostic. The IAV inclusive cross section reduces in the isolated-resonance limit to a sum of per-pole distorted-wave Born approximation (DWBA) pole cross sections weighted by channel branching ratios. The factorized PWIA-THM resonance-strength formula is then identified as a non-perturbative reduction of the per-pole DWBA cross section under four approximations (plane-wave substitution on the entrance and exit distorted waves, zero-range or surface-localized treatment of the spectator-participant interaction, on-shell evaluation of the binary subreaction vertex, and post-form remnant neglect), not a multiplicative correction factor. The per-pole DWBA pole cross section is the natural extraction quantity for sub-Coulomb resonance-strength analysis.

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

3 major / 2 minor

Summary. The manuscript introduces a diagonal isolated-pole spectral ansatz for the absorptive participant-target optical potential, subject to three validity conditions (two closed by R-matrix tabulations and one a model-dependent continuum-decoupling diagnostic). Under this ansatz, the IAV inclusive non-elastic breakup cross section reduces in the isolated-resonance limit to a sum of per-pole DWBA pole cross sections weighted by branching ratios. The factorized PWIA-THM resonance-strength formula is then derived as a non-perturbative reduction of the per-pole DWBA cross section under four approximations (plane-wave substitution, zero-range/surface-localized spectator-participant interaction, on-shell binary vertex evaluation, and post-form remnant neglect), rather than a multiplicative correction; the per-pole DWBA pole cross section is identified as the natural quantity for sub-Coulomb resonance-strength analysis.

Significance. If the spectral ansatz and its validity conditions hold for the relevant sub-Coulomb systems, the framework supplies a rigorous, non-perturbative link between the IAV inclusive breakup theory and the Trojan Horse Method. This would elevate the per-pole DWBA cross section to the primary extraction observable for resonance strengths, improving the theoretical grounding of astrophysical reaction-rate determinations that rely on THM data. The explicit enumeration of the four reduction approximations and the emphasis on channel branching ratios are constructive contributions.

major comments (3)
  1. [spectral ansatz section] The section introducing the diagonal isolated-pole spectral ansatz: the third validity condition (the model-dependent continuum-decoupling diagnostic) is stated without explicit numerical tests, counter-examples, or error analysis at the low energies relevant to sub-Coulomb THM applications; because the reduction of the IAV cross section to per-pole DWBA quantities rests directly on this ansatz, the absence of such validation leaves the central claim unsupported.
  2. [reduction to DWBA paragraph] The paragraph deriving the reduction to per-pole DWBA pole cross sections: no explicit intermediate equations or steps are supplied showing how the diagonal isolated-pole representation of the absorptive potential produces the weighted sum of DWBA pole cross sections; without these derivations the claimed non-perturbative character cannot be verified.
  3. [PWIA-THM identification paragraph] The identification of the PWIA-THM formula as a reduction of the per-pole DWBA cross section under the four listed approximations: the abstract states the result but provides neither the explicit operator substitutions nor a demonstration that the approximations are applied consistently to the DWBA matrix element; this step is load-bearing for the claim that THM is not merely a multiplicative correction.
minor comments (2)
  1. [notation introduction] Notation for the participant-target optical potential and its spectral decomposition should be introduced with a clear equation number on first use to aid readability.
  2. [abstract] The abstract would benefit from a single sentence stating the three validity conditions explicitly rather than summarizing them.

Simulated Author's Rebuttal

3 responses · 0 unresolved

We thank the referee for the careful and constructive report. The comments identify places where additional detail and validation will strengthen the presentation of the spectral ansatz and its reductions. We address each major comment below and will revise the manuscript accordingly.

read point-by-point responses
  1. Referee: [spectral ansatz section] The section introducing the diagonal isolated-pole spectral ansatz: the third validity condition (the model-dependent continuum-decoupling diagnostic) is stated without explicit numerical tests, counter-examples, or error analysis at the low energies relevant to sub-Coulomb THM applications; because the reduction of the IAV cross section to per-pole DWBA quantities rests directly on this ansatz, the absence of such validation leaves the central claim unsupported.

    Authors: We agree that the manuscript would be improved by explicit numerical support for the continuum-decoupling diagnostic at sub-Coulomb energies. In the revised version we will add a new subsection containing representative numerical tests, counter-examples, and quantitative error estimates using optical potentials appropriate to low-energy THM systems. This will directly address the referee's concern and better substantiate the applicability of the ansatz. revision: yes

  2. Referee: [reduction to DWBA paragraph] The paragraph deriving the reduction to per-pole DWBA pole cross sections: no explicit intermediate equations or steps are supplied showing how the diagonal isolated-pole representation of the absorptive potential produces the weighted sum of DWBA pole cross sections; without these derivations the claimed non-perturbative character cannot be verified.

    Authors: The referee correctly observes that the intermediate steps are not shown explicitly. We will expand the relevant paragraph in the revision to include the full sequence of operator substitutions and algebraic reductions that demonstrate how the diagonal isolated-pole form of the absorptive potential yields the branching-ratio-weighted sum of per-pole DWBA cross sections, thereby making the non-perturbative character of the reduction verifiable. revision: yes

  3. Referee: [PWIA-THM identification paragraph] The identification of the PWIA-THM formula as a reduction of the per-pole DWBA cross section under the four listed approximations: the abstract states the result but provides neither the explicit operator substitutions nor a demonstration that the approximations are applied consistently to the DWBA matrix element; this step is load-bearing for the claim that THM is not merely a multiplicative correction.

    Authors: We accept that the current text does not supply the explicit operator substitutions or consistency check requested. In the revised manuscript we will augment the identification paragraph (and, if space permits, the abstract) with the concrete substitutions for each of the four approximations and a brief demonstration that they are applied uniformly to the DWBA matrix element, thereby clarifying that the PWIA-THM expression arises as a reduction rather than a multiplicative factor. revision: yes

Circularity Check

0 steps flagged

No significant circularity detected

full rationale

The paper introduces a diagonal isolated-pole spectral ansatz for the absorptive participant-target optical potential, states three validity conditions (two closed externally by R-matrix tabulations), and derives the reduction of the IAV inclusive cross section to per-pole DWBA pole cross sections in the isolated-resonance limit. It then identifies the PWIA-THM formula as a further non-perturbative reduction of the per-pole DWBA cross section under four explicit approximations. These steps form a conditional derivation chain resting on the stated ansatz and approximations rather than any self-definitional loop, fitted input renamed as prediction, or load-bearing self-citation. The framework remains self-contained against the external R-matrix benchmarks cited for the validity conditions, with no evidence that outputs reduce to inputs by construction.

Axiom & Free-Parameter Ledger

0 free parameters · 1 axioms · 1 invented entities

Central claim depends on the newly introduced spectral ansatz and the four listed approximations for identifying THM as a limit; no free parameters are explicitly fitted in the abstract.

axioms (1)
  • ad hoc to paper The absorptive participant-target optical potential admits a diagonal isolated-pole spectral representation under three validity conditions.
    This is the load-bearing modeling choice introduced to enable the reduction of IAV to per-pole DWBA.
invented entities (1)
  • diagonal isolated-pole spectral ansatz no independent evidence
    purpose: To represent the optical potential so that IAV reduces to sum of per-pole DWBA cross sections in the isolated-resonance limit.
    New mathematical construct proposed in the paper; no independent evidence or external validation cited in abstract.

pith-pipeline@v0.9.0 · 5769 in / 1564 out tokens · 63419 ms · 2026-05-19T19:08:41.145845+00:00 · methodology

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Lean theorems connected to this paper

Citations machine-checked in the Pith Canon. Every link opens the source theorem in the public Lean library.

What do these tags mean?
matches
The paper's claim is directly supported by a theorem in the formal canon.
supports
The theorem supports part of the paper's argument, but the paper may add assumptions or extra steps.
extends
The paper goes beyond the formal theorem; the theorem is a base layer rather than the whole result.
uses
The paper appears to rely on the theorem as machinery.
contradicts
The paper's claim conflicts with a theorem or certificate in the canon.
unclear
Pith found a possible connection, but the passage is too broad, indirect, or ambiguous to say the theorem truly supports the claim.

Reference graph

Works this paper leans on

49 extracted references · 49 canonical work pages · 4 internal anchors

  1. [1]

    examines the sensitivity of the IAV inclusive non- elastic breakup cross section to the interior part of the entrance and exit distorted waves through a radial cut-off scheme that retains the full asymptoticS-matrix on the surface and zeroes only the interior region. For deuteron- induced (d, pX) reactions, the cut-off result is suppressed relative to the...

  2. [2]

    Baur, Phys

    G. Baur, Phys. Lett. B178, 135 (1986)

  3. [3]

    Anguloet al., Nucl

    C. Anguloet al., Nucl. Phys. A656, 3 (1999)

  4. [4]

    R. E. Tribble, C. A. Bertulani, M. La Cognata, A. M. Mukhamedzhanov, and C. Spitaleri, Rept. Prog. Phys. 77, 106901 (2014)

  5. [5]

    Tumino, C

    A. Tumino, C. A. Bertulani, M. La Cognata, L. Lamia, R. G. Pizzone, S. Romano, and S. Typel, Ann. Rev. Nucl. Part. Sci.71, 345 (2021)

  6. [6]

    Acharyaet al., Rev

    B. Acharyaet al., Rev. Mod. Phys.97, 035002 (2025)

  7. [7]

    La Cognataet al., Astrophys

    M. La Cognataet al., Astrophys. J.708, 796 (2010)

  8. [8]

    La Cognata, S

    M. La Cognata, S. Palmerini, C. Spitaleri, I. Indelicato, A. M. Mukhamedzhanov, I. Lombardo, and O. Trippella, Astrophys. J.805, 128 (2015)

  9. [9]

    Indelicato, M

    I. Indelicato, M. La Cognata, C. Spitaleri, V. Bur- jan, S. Cherubini, M. Gulino, S. Hayakawa, Z. Hons, V. Kroha, L. Lamia, M. Mazzocco, J. Mrazek, R. G. Piz- zone, S. Romano, E. Strano, D. Torresi, and A. Tumino, Astrophys. J.845, 19 (2017)

  10. [10]

    G. L. Guardo, G. G. Rapisarda, D. L. Balabanski,et al., Universe10, 304 (2024)

  11. [11]

    Petruse, G

    T. Petruse, G. L. Guardo, D. Lattuada, M. La Cognata, D. L. Balabanski,et al., Eur. Phys. J. A61, 4 (2025)

  12. [12]

    X. D. Su, M. La Cognata, N. Vukman,et al., Phys. Rev. Lett.135, 182701 (2025)

  13. [13]

    Tumino, C

    A. Tumino, C. Spitaleri, A. Mukhamedzhanov,et al., Phys. Rev. C78, 064001 (2008)

  14. [14]

    A. M. Mukhamedzhanov and A. S. Kadyrov, Phys. Rev. C82, 051601 (2010)

  15. [15]

    A. M. Mukhamedzhanov, Phys. Rev. C84, 044616 (2011)

  16. [16]

    A. M. Mukhamedzhanov, A. S. Kadyrov, and D. Y. Pang, Eur. Phys. J. A56, 233 (2020)

  17. [17]

    C. A. Bertulani, M. S. Hussein, and S. Typel, Phys. Lett. B776, 217 (2018)

  18. [18]

    Tumino, C

    A. Tumino, C. A. Bertulani, S. Cherubini,et al., Prog. Part. Nucl. Phys.143, 104164 (2025)

  19. [19]

    Lombardo, D

    I. Lombardo, D. Dell’Aquila, A. Di Leva, I. Indelicato, M. La Cognata, M. La Commara, A. Ordine, V. Rigato, M. Romoli, E. Rosato, G. Spadaccini, C. Spitaleri, A. Tu- mino, and M. Vigilante, Phys. Lett. B748, 178 (2015)

  20. [20]

    L. Y. Zhang, A. Y. L´ opez, M. Lugaro, J. J. He, and A. I. Karakas, Astrophys. J.913, 51 (2021)

  21. [21]

    R. J. deBoer, O. Clarkson, A. J. Couture, J. G¨ orres, F. Herwig, I. Lombardo, P. Scholz, and M. Wiescher, Phys. Rev. C103, 055815 (2021)

  22. [22]

    Redigolo, I

    L. Redigolo, I. Lombardo, D. Dell’Aquila, A. Musumarra, M. G. Pellegriti, M. Russo, G. Verde, and M. Vigilante, Nucl. Phys. A1060, 123102 (2025)

  23. [23]

    L. Y. Zhang and others (JUNA Collaboration), Phys. Rev. Lett.127, 152702 (2021)

  24. [24]

    L. Y. Zhang and others (JUNA Collaboration), Phys. Rev. C106, 055803 (2022)

  25. [25]

    Zhang, J

    L. Zhang, J. He, R. J. deBoer, M. Wiescher, A. Heger, et al., Nature610, 656 (2022)

  26. [26]

    Y.-J. Chen, H. Zhang, L.-Y. Zhang, J.-J. He,et al., Nucl. Sci. Tech.35, 143 (2024)

  27. [27]

    W. Liu, B. Guo, J. He, Z. Li, X. Tang, M. Lugaro, and G. Lian, Ann. Rev. Nucl. Part. Sci.75, 271 (2025)

  28. [28]

    Ichimura, N

    M. Ichimura, N. Austern, and C. M. Vincent, Phys. Rev. C32, 431 (1985)

  29. [29]

    M. S. Hussein and K. W. McVoy, Nucl. Phys. A445, 124 (1985)

  30. [30]

    Austern, Y

    N. Austern, Y. Iseri, M. Kamimura, M. Kawai, G. Raw- itscher, and M. Yahiro, Phys. Rept.154, 125 (1987)

  31. [31]

    Reexamining closed-form formulae for inclusive breakup: Application to deuteron and $^6$Li induced reactions

    J. Lei and A. M. Moro, Phys. Rev. C92, 044616 (2015), arXiv:1510.02602 [nucl-th]

  32. [32]

    Lei and A

    J. Lei and A. M. Moro, Phys. Rev. C92, 061602 (2015)

  33. [33]

    Lei and A

    J. Lei and A. M. Moro, Phys. Rev. C97, 011601 (2018)

  34. [34]

    Inclusive breakup calculations in angular momentum basis: application to $^7$Li+$^{58}$Ni

    J. Lei, Phys. Rev. C97, 034628 (2018), arXiv:1712.01433 [nucl-th]

  35. [35]

    Lei and A

    J. Lei and A. M. Moro, Phys. Rev. Lett.123, 232501 (2019)

  36. [36]

    Lei and A

    J. Lei and A. M. Moro, Phys. Rev. C108, 034612 (2023), arXiv:2305.14111 [nucl-th]

  37. [37]

    A. M. Mukhamedzhanov, D. Y. Pang, and A. S. Kadyrov, Phys. Rev. C99, 064618 (2019), arXiv:1806.08828 [nucl- th]

  38. [38]

    Establishing a theory for deuteron induced surrogate reactions

    G. Potel, F. M. Nunes, and I. J. Thompson, Phys. Rev. C92, 034611 (2015), arXiv:1508.04822 [nucl-th]

  39. [39]

    B. V. Carlson, R. Capote, and M. Sin, Few-Body Syst. 57, 307 (2016)

  40. [40]

    Potel, G

    G. Potel, G. Perdikakis, B. V. Carlson,et al., Eur. Phys. J. A53, 178 (2017)

  41. [41]

    B. V. Carlson, T. Frederico, and M. S. Hussein, Phys. Lett. B767, 53 (2017)

  42. [42]

    J. E. Escher, J. T. Harke, F. S. Dietrich, N. D. Scielzo, I. J. Thompson, and W. Younes, Rev. Mod. Phys.84, 353 (2012). 18

  43. [43]

    A. M. Lane and R. G. Thomas, Rev. Mod. Phys.30, 257 (1958)

  44. [44]

    A. J. Koning and J. P. Delaroche, Nucl. Phys. A713, 231 (2003)

  45. [45]

    La Cognata, A

    M. La Cognata, A. M. Mukhamedzhanov, C. Spitaleri, et al., Astrophys. J. Lett.739, L54 (2011)

  46. [46]

    J. Liu, J. Lei, and Z. Ren, Phys. Rev. C108, 024606 (2023)

  47. [47]

    C. M. Vincent and H. T. Fortune, Phys. Rev. C2, 782 (1970)

  48. [48]

    Lei, Phys

    J. Lei, Phys. Rev. C112, 014609 (2025), arXiv:2504.03112 [nucl-th]

  49. [49]

    Hauser and H

    W. Hauser and H. Feshbach, Phys. Rev.87, 366 (1952)