REVIEW 3 major objections 5 minor 91 references
Pion photoproduction off nucleons in covariant chiral perturbation theory
T0 review · 3 major / 5 minor · reviewed 2026-08-14 · deepseek-v4-flash
Pith's one-line read This paper claims that near-threshold pion photoproduction in all four charge channels is described by an O(p^3) covariant chiral perturbation theory calculation in the extended-on-mass-shell scheme that explicitly includes the Δ(1232)…
desk verdict A credible O(p^3) EOMS ChPT calculation with explicit Delta that convincingly shows the Delta is essential, but the quantitative LEC values and the claimed advantage over O(p^4) without Delta remain provisional because the fitted d18 is unstable under higher-order variations. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The central technical object is the extended-on-mass-shell (EOMS) renormalization scheme combined with the δ-counting, in which the mass difference δ = mΔ − mN ≈ 300 MeV is treated as O($p^{{1/2}}$), so the Δ(1232) resonance enters the chiral power counting systematically. The EOMS scheme restores the power counting by absorbing finite shifts into the low-energy constants while preserving Lorentz covariance and the analytic structure of the amplitudes. The one-loop O($p^{3}$) amplitudes are built from the chiral Lagrangian for pions, nucleons, and the Δ(1232), with ultraviolet divergences removed in modified minimal subtraction and EOMS finite shifts applied to m, g, c1, c6, and c7. The wave-function renormalization and mass corrections are applied consistently, and the Δ propagator uses an energy-dependent width at the relevant order.
What would settle it
Measure the near-threshold γp→π0p differential cross section and the E0+ multipole with sufficiently small statistical and systematic errors over the range from threshold to roughly 30 MeV above it, and compare the energy slope to the prediction of Fit I: if the steep rise driven by the Δ tail is absent, or if the Δ-less O($p^{4}$) calculation reproduces the slope equally well, the paper's central claim that the Δ is essential would be refuted.
Extended reading notes
Core claim
In the extended-on-mass-shell (EOMS) scheme of covariant baryon chiral perturbation theory, a complete one-loop calculation at O($p^{3}$) in the delta-counting, with the Δ(1232) treated explicitly, reproduces the available near-threshold data of pion photoproduction off nucleons for all charge channels. The model achieves an overall chi-squared per degree of freedom of 3.22 with most low-energy constants fixed from other processes; removing the Δ mechanisms worsens the same fit to 29.5, showing that the Δ(1232) tail is decisive even close to threshold. The improvement over earlier O($p^{4}$) heavy-baryon and covariant results without an explicit Δ is attributed to the systematic δ-counting and the resonance contribution, not to additional free parameters. The paper also extracts the combination d8+d9 with high precision from the neutral-pion channel, while other third-order constants are less constrained by the scarce charged-pion data.
Load-bearing premise
The chiral expansion has converged enough at O($p^{3}$) that the fitted low-energy constants and the quoted chi-squared values are meaningful; if higher-order contributions are not small, the fitted constants and the apparent improvement from the Δ are not stable predictions.
Editorial extensions
If this is right
- If the central claim holds, explicit Δ(1232) degrees of freedom should be regarded as mandatory in chiral perturbation theory analyses of pion photoproduction, not merely as an optional improvement.
- The tightly determined combination d8+d9 serves as a benchmark low-energy constant that can be used as input in related processes, such as weak pion production, for which data are scarce.
- The framework, at the same order and scheme, provides a consistent starting point for extending the calculation to O(p^{7/2}) and O(p^4), incorporating higher-order Δπ and Δγ couplings.
- The near-threshold description of the γp → π0p channel, where the Δ contribution is most visible, is expected to improve substantially over Δ-less O(p^4) calculations, as the authors demonstrate through the χ2 behavior with photon energy.
- New measurements in the charged-pion channels, especially γn → π−p, would directly constrain the currently poorly known third-order constants d9, d20, and d21.
Reading between the lines
- A skeptical reader would note that the paper itself observes the fitted value of d18 shifts significantly under O(p^4) variations, indicating that the quoted chi-squared and the fitted constants may not be stable if higher-order contributions are not small; this is a testable concern rather than a proven flaw.
- The Delta-dominance claim suggests a sharp prediction: the energy dependence of the neutral-pion E0+ and M1+ multipoles near threshold should show a rapid rise tied to the Δ tail, which future high-precision angular and polarization measurements could directly verify.
- The same EOMS plus δ-counting machinery could be carried to electroproduction, where the additional photon virtuality would give a further test of whether the Δ contribution and the fitted LECs remain stable.
- Because the charged-pion channels are relatively insensitive to the third-order operators, the paper implicitly predicts that the main benefit of improved charged-pion data will be to pin down d9 and d20 rather than to change the neutral-pion conclusions.
Signed reviews
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript presents a covariant chiral perturbation theory calculation of threshold pion photoproduction off nucleons at O(p^3) in the EOMS scheme, with an explicit Delta(1232) included through the delta counting. The authors fit the combinations d8+d9, d8-d9, and the LECs d20, d21, and gM to 957 data points covering all four charge channels, while fixing most other LECs from independent analyses and restricting d18 to its piN-scattering prior. Their main result is Fit I with chi2/dof = 3.22; removing the Delta gives Fit II at 29.5, and leaving d18 free gives Fit III at 1.58 but with a d18 value that is hardly compatible with g_piN. They conclude that the Delta is essential and that the model reproduces the data better over a wider energy range than published O(p4) calculations without the Delta.
Significance. If the O(p^3) truncation is reliable, this is a significant step: it shows that a covariant EOMS treatment with explicit Delta can describe a global multi-channel database, constrains previously poorly known LECs, and explains the energy dependence of pion photoproduction without invoking higher-order Delta-less terms. The paper has genuine strengths: it uses a large and heterogeneous database, fixes most LECs from independent processes, reports both statistical and truncation uncertainties, and demonstrates the qualitative Delta effect in a controlled way through Fit I versus Fit II. The main caveat is that the quantitative claims rest on an LEC, d18, that the authors themselves find to be strongly affected by O(p^4) variations; until that sensitivity is understood, the advertised 'good agreement' and the comparison with O(p^4) calculations remain provisional.
major comments (3)
- [Section IV A, Table II] The load-bearing quantitative claim rests on constraining d18 to the 1-sigma range given in Table I. When d18 is left free in Fit III, chi2/dof improves from 3.22 to 1.58, but d18 moves to 5.69 +/- 0.14 GeV^-2, a value the authors describe as hardly compatible with g_piN. Section IV A also states that d18 is strongly affected by O(p^4) variations, such as the choice of wave-function renormalization, the use of m versus m2 in the loops, and the tree-level terms e48, e50, and e112. This means the O(p^3) minimum is not demonstrably chiral-stable. The central claim that the model reproduces the data well should be made conditional on a higher-order calculation, or the paper should provide a quantitative stability analysis showing that the relevant observables and the Delta-essentiality conclusion are unchanged under these variations.
- [Summary and Section IV A, Fig. 5] The claim that the agreement is better, and for a wider range of energies, than in O(p^4) calculations without the Delta is not directly quantified in this manuscript. The comparison with Refs. [18,19] is based on published pi0-only figures, whereas the present chi2 is computed over a different 957-point database. Within this paper, the only direct controlled comparison is Fit I versus Fit II at O(p^3). Since Fit I still has chi2/dof = 3.22, an absolute statement of superiority over O(p^4) would require either a common re-fit of the Delta-less O(p^4) amplitudes on the same dataset or a table comparing chi2 per channel and energy range on matched datasets.
- [Section III C, Eq. (28)] The truncation uncertainty estimator uses only the lowest-order and current-order amplitudes. Given the observed sensitivity of d18 to O(p^4) variations, this estimator may understate the systematic uncertainty in the plotted error bands and in the quoted LEC errors. The authors should state explicitly whether the bands in Figs. 6-13 include the spread generated by the O(p^4)-variation study of d18, or whether those variations are only discussed textually.
minor comments (5)
- [Introduction] There is a typo in 'low energy contants' near the end of the first section; it should read 'low energy constants'.
- [Figure 6 caption] The caption says the inner band is obtained by varying the LECs 'as shown in Table I', but the fitted LECs appear in Table II; Table I lists the externally fixed constants.
- [Table II header] The header 'Fit II - /Delta' is unclear; please spell out that this is the fit without Delta mechanisms.
- [Equation (28)] The notation in the truncation-error formula is hard to follow: the condition nLO <= j <= k <= n and the exponents Q^{n-nLO+1} and Q^{n-j} should be defined with a brief example or a reference to the original derivation.
- [Section IV A, footnote 10] The footnote 'In Fit II, it rises up to chi2 = 31.7 at d18 = 0.6 GeV^-2' is ambiguous; clarify whether this refers to the d18 scan in Fit I or to a separate scan in Fit II.
Circularity Check
No significant circularity: fitted LECs are endpoints, the Delta effect is tested by deletion, and self-cited inputs are independent observables.
full rationale
The paper's derivation chain is a conventional EOMS chiral perturbation theory calculation: it constructs the O(p^3) amplitude, fits a small set of unknown LECs to 957 photoproduction data points, and fixes the remaining LECs from independent processes (magnetic moments, axial radius, Delta widths, and piN scattering). The central claim that the Delta(1232) is significant is tested by switching off Delta mechanisms (Fit II vs Fit I) at the same chiral order, so the conclusion is not forced by construction. The fitted LECs are endpoints of the analysis, not inputs that secretly encode the pion photoproduction result; in particular, d18 is constrained by an external piN-scattering analysis, and the paper explicitly explores an unconstrained refit (Fit III). The self-citations (Refs. [48-50,80]) supply LEC values derived from other observables—external, independently falsifiable inputs—rather than from the process under study, so they do not constitute circularity. The authors' caveat that d18 is strongly affected by O(p^4) variations is a chiral-convergence and robustness concern, appropriately classified as correctness risk rather than circularity, because no prediction reduces to its own input by definition or by fit. Overall, the analysis is self-contained against data and the cited external inputs do not embed the target result.
Assumptions & free parameters
free parameters (6)
- d8 + d9 =
1.16 +/- 0.01 GeV^-2 (Fit I)
- d8 - d9 =
1.09 +/- 0.18 GeV^-2 (Fit I)
- d20 =
-0.74 +/- 0.17 GeV^-2 (Fit I)
- d21 =
4.32 +/- 0.14 GeV^-2 (Fit I)
- gM =
2.90 +/- 0.01 (Fit I)
- d18 (constrained in Fit I) =
0.60 GeV^-2 (upper edge of 1-sigma range [-1.0, 0.60] from Table I)
assumptions (6)
- domain assumption EOMS renormalization restores the chiral power counting in the presence of baryon loops.
- domain assumption Delta-counting with delta = m_Delta - m_N ~ O(p^{1/2}) and the diagram power counting of Eq. (10).
- domain assumption Low-energy constants from other processes (Table I) are valid at O(p^3) in the same EOMS plus Delta framework.
- domain assumption Isospin symmetry is assumed; mass splittings near threshold are neglected.
- domain assumption The spectator model extraction of gamma n -> pi- p cross sections from deuteron data and the inverse radiative capture data are reliable enough for fitting.
- domain assumption The chiral truncation uncertainty formula (Eq. 28) from Refs [42,82] is a valid estimate of missing higher orders.
Cite this review
Pith. "Pith review of Pion photoproduction off nucleons in covariant chiral perturbation theory." pith.science (2026). https://pith.science/paper/JSG63S35
@misc{pith2026190800890,
author = {Pith},
title = {Pith review of: Pion photoproduction off nucleons in covariant chiral perturbation theory},
year = {2026},
howpublished = {\url{https://pith.science/paper/JSG63S35}},
note = {Machine review of arXiv:1908.00890}
}
abstract
Pion photoproduction off the nucleon close to threshold is studied in covariant baryon chiral perturbation theory at O($p^3$) in the extended-on-mass-shell scheme, with the explicit inclusion of the $\Delta(1232)$ resonance using the $\delta$ counting. The theory is compared to the available data of cross sections and polarization observables for all the charge channels. Most of the necessary low energy constants are well known from the analysis of other processes and the comparison with data strongly constrains some of the still unknown ones. The $\Delta(1232)$ contribution is significant in improving the agreement with data, even at the low energies considered.
Figures
Figures from the paper (10 more)
Reference graph
Works this paper leans on
-
[1]
Representations of the invariant amplitude We write the scattering amplitudeT as T =¯u(p′)[aNq·ϵVN + aEVE + aKq·ϵVK + aEK VEK ] u(p), (A1) where u(p) and ¯u(p′) = u†(p′)γ0 are the Dirac spinors corresponding to the initial and final nucleon states respectively,ϵ is the photon polarization vector, and q is the 4-momentum of the outgoing pion, the coefficients...
-
[2]
Tree level amplitude a. At O (p1) T (1) (a) = C(1) I eg F0 VE, (A12) T (1) (b) = C(1) II eg F0 ( s− m2 N ) ( m2 2− s ) VE + (mN + m2)( m2 2− s ) VEK , (A13) T (1) (c) = C(1) III eg F0 ( m2 N− u ) ( m2 2− u ) VE + 2(mN + m2)( m2 2− u ) q·ϵVN + (mN + m2)( m2 2− u ) VEK , (A14) T (1) (d) = C(1) IV 2 √ 2egmN F0 ( −2m2 N + s +...
-
[3]
S. L. Adler, Annals Phys. 50, 189 (1968), [,225(1968)]
1968
-
[4]
D. Drechsel, S. S. Kamalov, and L. Tiator, Eur. Phys. J. A34, 69 (2007), 0710.0306
arXiv 2007
-
[5]
Weinberg, Physica A96, 327 (1979)
S. Weinberg, Physica A96, 327 (1979)
1979
-
[6]
Gasser and H
J. Gasser and H. Leutwyler, Annals Phys. 158, 142 (1984)
1984
-
[7]
Gasser and H
J. Gasser and H. Leutwyler, Nucl. Phys. B250, 465 (1985)
1985
-
[8]
Scherer and M
S. Scherer and M. R. Schindler, Lect. Notes Phys. 830, pp.1 (2012)
2012
Show all 91 references
-
[9]
N. M. Kroll and M. A. Ruderman, Phys. Rev. 93, 233 (1954), URL https://link.aps.org/doi/ 10.1103/PhysRev.93.233
1954 doi
-
[10]
De Baenst, Nucl
P. De Baenst, Nucl. Phys. B24, 633 (1970)
1970
-
[11]
A. I. Vainshtein and V . I. Zakharov, Nucl. Phys.B36, 589 (1972)
1972
-
[12]
Mazzucato et al., Phys
E. Mazzucato et al., Phys. Rev. Lett. 57, 3144 (1986)
1986
-
[13]
R. Beck, F. Kalleicher, B. Schoch, J. V ogt, G. Koch, H. Stroher, V . Metag, J. C. McGeorge, J. D. Kellie, and S. J. Hall, Phys. Rev. Lett. 65, 1841 (1990)
1990
-
[14]
Drechsel and L
D. Drechsel and L. Tiator, J. Phys. G18, 449 (1992)
1992
-
[15]
Bernard and U.-G
V . Bernard and U.-G. Meissner, Ann. Rev. Nucl. Part. Sci.57, 33 (2007), hep-ph/0611231
2007 arXiv
-
[16]
Bernard, N
V . Bernard, N. Kaiser, J. Gasser, and U. G. Meissner, Phys. Lett.B268, 291 (1991)
1991
-
[17]
Bernard, N
V . Bernard, N. Kaiser, and U. G. Meissner, Nucl. Phys.B383, 442 (1992)
1992
-
[18]
Bernard, N
V . Bernard, N. Kaiser, and U.-G. Meissner, Eur. Phys. J.A11, 209 (2001), hep-ph/0102066. 31
2001 arXiv
-
[19]
Hornidge et al
D. Hornidge et al. (A2, CB-TAPS), Phys. Rev. Lett. 111, 062004 (2013), 1211.5495
2013 arXiv
-
[20]
Fernandez-Ramirez and A
C. Fernandez-Ramirez and A. M. Bernstein, Phys. Lett. B724, 253 (2013), 1212.3237
2013 arXiv
-
[21]
M. Hilt, S. Scherer, and L. Tiator, Phys. Rev. C87, 045204 (2013), 1301.5576
2013 arXiv
-
[22]
Bijnens and G
J. Bijnens and G. Ecker, Ann. Rev. Nucl. Part. Sci. 64, 149 (2014), 1405.6488
2014 arXiv
- [23]
-
[24]
Gasser, M
J. Gasser, M. E. Sainio, and A. Svarc, Nucl. Phys. B307, 779 (1988)
1988
-
[25]
E. E. Jenkins and A. V . Manohar, Phys. Lett. B255, 558 (1991)
1991
-
[26]
E. E. Jenkins and A. V . Manohar, Phys. Lett. B259, 353 (1991)
1991
- [27]
-
[28]
Fuchs, J
T. Fuchs, J. Gegelia, G. Japaridze, and S. Scherer, Phys. Rev. D68, 056005 (2003), hep-ph/0302117
2003 arXiv
-
[29]
J. M. Alarcon, J. Martin Camalich, and J. A. Oller, Annals Phys. 336, 413 (2013), 1210.4450
2013 arXiv
-
[30]
L. S. Geng, J. Martin Camalich, L. Alvarez-Ruso, and M. J. Vicente Vacas, Phys. Rev. Lett. 101, 222002 (2008), 0805.1419
2008 arXiv
-
[31]
Martin Camalich, L
J. Martin Camalich, L. S. Geng, and M. J. Vicente Vacas, Phys. Rev. D82, 074504 (2010), 1003.1929
2010 arXiv
-
[32]
Fuchs, J
T. Fuchs, J. Gegelia, and S. Scherer, J. Phys. G30, 1407 (2004), nucl-th/0305070
2004 arXiv
-
[33]
B. C. Lehnhart, J. Gegelia, and S. Scherer, J. Phys. G31, 89 (2005), hep-ph/0412092
2005 arXiv
-
[34]
M. R. Schindler, T. Fuchs, J. Gegelia, and S. Scherer, Phys. Rev. C75, 025202 (2007), nucl- th/0611083
2007
-
[35]
M. R. Schindler, D. Djukanovic, J. Gegelia, and S. Scherer, Phys. Lett. B649, 390 (2007), hep- ph/0612164
2007
-
[36]
L. S. Geng, J. Martin Camalich, and M. J. Vicente Vacas, Phys. Rev. D79, 094022 (2009), 0903.4869
2009 arXiv
-
[37]
J. M. Alarcon, J. Martin Camalich, and J. A. Oller, Phys. Rev. D85, 051503 (2012), 1110.3797
2012 arXiv
-
[38]
Ledwig, J
T. Ledwig, J. Martin-Camalich, V . Pascalutsa, and M. Vanderhaeghen, Phys. Rev.D85, 034013 (2012), 1108.2523
2012 arXiv
-
[39]
Chen, D.-L
Y .-H. Chen, D.-L. Yao, and H. Q. Zheng, Phys. Rev.D87, 054019 (2013), 1212.1893
2013 arXiv
-
[40]
Alvarez-Ruso, T
L. Alvarez-Ruso, T. Ledwig, J. Martin Camalich, and M. J. Vicente-Vacas, Phys. Rev. D88, 054507 (2013), 1304.0483
2013 arXiv
-
[41]
Ledwig, J
T. Ledwig, J. Martin Camalich, L. S. Geng, and M. J. Vicente Vacas, Phys. Rev. D90, 054502 (2014), 1405.5456
2014 arXiv
-
[42]
Lensky, J
V . Lensky, J. M. Alarc´on, and V . Pascalutsa, Phys. Rev.C90, 055202 (2014), 1407.2574
2014 arXiv
-
[43]
D.-L. Yao, D. Siemens, V . Bernard, E. Epelbaum, A. M. Gasparyan, J. Gegelia, H. Krebs, and U.-G. 32 Meißner, JHEP 05, 038 (2016), 1603.03638
2016 arXiv
-
[44]
Siemens, V
D. Siemens, V . Bernard, E. Epelbaum, A. Gasparyan, H. Krebs, and U.-G. Meißner, Phys. Rev. C94, 014620 (2016), 1602.02640
2016 arXiv
-
[45]
A. N. Hiller Blin, T. Ledwig, and M. J. Vicente Vacas, Phys. Lett. B747, 217 (2015), 1412.4083
2015 arXiv
-
[46]
A. N. Hiller Blin, T. Ledwig, and M. J. Vicente Vacas, Phys. Rev. D93, 094018 (2016), 1602.08967
2016 arXiv
-
[47]
M. Hilt, B. C. Lehnhart, S. Scherer, and L. Tiator, Phys. Rev. C88, 055207 (2013), 1309.3385
2013 arXiv
-
[48]
T. E. O. Ericson and W. Weise, Pions and Nuclei, vol. 74 (Clarendon Press, Oxford, UK, 1988), ISBN 0198520085, URL http://www-spires.fnal.gov/spires/find/books/www?cl= QC793.5.M42E75::1988
1988
- [49]
-
[50]
Hiller Blin, T
A. Hiller Blin, T. Gutsche, T. Ledwig, and V . E. Lyubovitskij, Phys. Rev. D92, 096004 (2015), 1509.00955
2015 arXiv
-
[51]
D.-L. Yao, L. Alvarez-Ruso, A. N. Hiller Blin, and M. J. Vicente Vacas, Phys. Rev. D98, 076004 (2018), 1806.09364
2018 arXiv
-
[52]
D.-L. Yao, L. Alvarez-Ruso, and M. J. Vicente Vacas, Phys. Lett. B794, 109 (2019), 1901.00773
2019 arXiv
-
[53]
T. R. Hemmert, B. R. Holstein, and J. Kambor, Phys. Lett. B395, 89 (1997), hep-ph/9606456
1997 arXiv
-
[54]
Bernard, N
V . Bernard, N. Kaiser, and U. G. Meißner, Phys. Lett.B331, 137 (1994), hep-ph/9312307
1994 arXiv
-
[55]
Alvarez-Ruso et al., Prog
L. Alvarez-Ruso et al., Prog. Part. Nucl. Phys. 100, 1 (2018), 1706.03621
2018 arXiv
-
[56]
Alvarez-Ruso, Y
L. Alvarez-Ruso, Y . Hayato, and J. Nieves, New J. Phys.16, 075015 (2014), 1403.2673
2014 arXiv
-
[57]
G. F. Chew, M. L. Goldberger, F. E. Low, and Y . Nambu, Phys. Rev.106, 1345 (1957)
1957
-
[58]
A. M. Sandorfi, S. Hoblit, H. Kamano, and T. S. H. Lee, J. Phys. G38, 053001 (2011), 1010.4555
2011 arXiv
-
[59]
Pascalutsa and D
V . Pascalutsa and D. R. Phillips, Phys. Rev.C67, 055202 (2003), nucl-th/0212024
2003 arXiv
-
[60]
Fettes, U.-G
N. Fettes, U.-G. Meißner, M. Mojzis, and S. Steininger, Annals Phys. 283, 273 (2000), [Erratum: Annals Phys.288,249(2001)], hep-ph/0001308
2000 arXiv
- [61]
-
[62]
Pascalutsa, M
V . Pascalutsa, M. Vanderhaeghen, and S. N. Yang, Phys. Rept.437, 125 (2007), hep-ph/0609004
2007 arXiv
-
[63]
Shtabovenko, R
V . Shtabovenko, R. Mertig, and F. Orellana, Comput. Phys. Commun.207, 432 (2016), 1601.01167
2016 arXiv
-
[64]
Mertig, M
R. Mertig, M. Bohm, and A. Denner, Comput. Phys. Commun. 64, 345 (1991)
1991
-
[65]
Lehmann, K
H. Lehmann, K. Symanzik, and W. Zimmermann, Nuovo Cim. 1, 205 (1955)
1955
-
[66]
Fuchs et al., Phys
M. Fuchs et al., Phys. Lett. B368, 20 (1996)
1996
-
[67]
J. C. Bergstrom, J. M. V ogt, R. Igarashi, K. J. Keeter, E. L. Hallin, G. A. Retzlaff, D. M. Skopik, and 33 E. C. Booth, Phys. Rev. C53, R1052 (1996)
1996
-
[68]
J. C. Bergstrom, R. Igarashi, and J. M. V ogt, Phys. Rev.C55, 2016 (1997)
1997
-
[69]
Schmidt et al., Phys
A. Schmidt et al., Phys. Rev. Lett. 87, 232501 (2001), [Erratum: Phys. Rev. Lett.110,039903(2013)], nucl-ex/0105010
2001 arXiv
-
[70]
Blanpied et al., Phys
G. Blanpied et al., Phys. Rev. C64, 025203 (2001)
2001
-
[71]
Rossi et al., Nuovo Cim
V . Rossi et al., Nuovo Cim. A13, 59 (1973)
1973
-
[72]
Benz et al
P. Benz et al. (Aachen-Bonn-Hamburg-Heidelberg-Muenchen), Nucl. Phys. B65, 158 (1973)
1973
-
[73]
Salomon, D
M. Salomon, D. F. Measday, J. M. Poutissou, and B. C. Robertson, Nucl. Phys. A414, 493 (1984)
1984
-
[74]
Bagheri, K
A. Bagheri, K. A. Aniol, F. Entezami, M. D. Hasino ff, D. F. Measday, J. M. Poutissou, M. Salomon, and B. C. Robertson, Phys. Rev. C38, 875 (1988)
1988
-
[75]
INS Data Analysis Center, URL http://gwdac.phys.gwu.edu/
- [76]
-
[77]
R. J. Walker, T. R. Palfrey, R. O. Haxby, and B. M. K. Nefkens, Phys. Rev.132, 2656 (1963)
1963
-
[78]
K. G. Fissum, H. S. Caplan, E. L. Hallin, D. M. Skopik, J. M. V ogt, M. Frodyma, D. P. Rosenzweig, D. W. Storm, G. V . O’Rielly, and K. R. Garrow, Phys. Rev.C53, 1278 (1996)
1996
-
[79]
Ahrens et al
J. Ahrens et al. (GDH, A2), Eur. Phys. J. A21, 323 (2004)
2004
-
[80]
Bauer, J
T. Bauer, J. C. Bernauer, and S. Scherer, Phys. Rev. C86, 065206 (2012), 1209.3872
2012 arXiv
-
[81]
Patrignani et al
C. Patrignani et al. (Particle Data Group), Chin. Phys. C40, 100001 (2016)
2016
-
[82]
D.-L. Yao, L. Alvarez-Ruso, and M. J. Vicente-Vacas, Phys. Rev. D96, 116022 (2017), 1708.08776
2017 arXiv
-
[83]
Bernard, E
V . Bernard, E. Epelbaum, H. Krebs, and U.-G. Meißner, Phys. Rev.D87, 054032 (2013), 1209.2523
2013 arXiv
-
[84]
Epelbaum, H
E. Epelbaum, H. Krebs, and U. G. Meißner, Eur. Phys. J. A51, 53 (2015), 1412.0142
2015 arXiv
- [85]
-
[86]
Korkmaz et al., Phys
E. Korkmaz et al., Phys. Rev. Lett. 83, 3609 (1999)
1999
-
[87]
D. A. McPherson, D. C. Gates, R. W. Kenney, and W. P. Swanson, Phys. Rev.136, B1465 (1964)
1964
-
[88]
D. H. White, R. M. Schectman, and B. M. Chasan, Phys. Rev. 120, 614 (1960)
1960
-
[89]
Wang, Ph
M. Wang, Ph. D. thesis, University of Kentucky (1992)
1992
-
[90]
K. Liu, Ph. D. thesis, University of Kentucky (1994)
1994
-
[91]
Gegelia, U.-G
J. Gegelia, U.-G. Meißner, D. Siemens, and D.-L. Yao, Phys. Lett. B763, 1 (2016), 1608.00517. 34
2016 arXiv
Reviewed August 14, 2026 · model on record in the stance chip above.
Discussion (0). Continue with ORCID to comment.