High Energy Physics - Phenomenology · arXiv:hep-ph/0412332 v1 · submitted 22 Dec 2004 · 21 references
QGSJET-II: towards reliable description of very high energy hadronic interactions
The paper says
“Since a number of years the QGSJET model has been successfully used by different groups in the field of high energy cosmic rays. Current work is devoted to the first general update of the model.”
more of the abstract
The key improvement is connected to an account for non-linear interaction effects which are of crucial importance for reliable model extrapolation into ultra-high energy domain. The proposed formalism allows to obtain a consistent description of hadron-hadron cross sections and hadron structure functions and to treat non-linear effects explicitely in individual hadronic and nuclear collisions. Other ameliorations concern the treatment of low mass diffraction, employment of realistic nuclear density profiles, and re-calibration of model parameters using a wider set of accelerator data.
from the abstract
Pith says
Machine review · deepseek-v4.1-flash · 13 Nov 2026 · what was read was not recorded · not checked by a person
Reviewed in 2026 with later literature in view.
It can be wrong. Challenge this review or reply to it.
Holds up, with conditions. A real methodological step for QGSJET, honestly presented as a summary — but the all-orders claim is bounded only within the loopless fan topologies, and the paper never says how much it is leaving out. This line is wrong
3 major objections · 8 minor
How often objections from reviews like this one are right: not yet measured
Not checked: figures, code, what the 21 references say.
The paper says, at §3, sentence immediately preceding Fig. 6
The review did not quote this passage.
Pith says: Objection 1 of 3 · major
The text states: 'Then, neglecting subdominant contributions of Pomeron loops, the final result for hadron-hadron interaction eikonal can be represented in the graphical form as shown in Fig. 6.' The abstract (abstract:s3, abstract:s2) nonetheless advertises an all-order resummation and a reliable ultra-high-energy extrapolation.
more of objection 1
The resummation is all-order only within the loopless subset of fan and generalized-fan topologies (Figs. 4 and 5); Pomeron loops are precisely the class of enhanced diagrams whose relative weight is expected to grow with energy, and the fan series alone does not by itself preserve t-channel unitarity asymptotically. No estimate of the neglected loop contribution is given at, e.g., 10^19-10^20 eV. The internal comparison in Figs. 7 and 8 (full versus dashed 'without enhanced diagrams') tests enhanced-versus-none, not loops-versus-no-loops, so it cannot speak to this point. Either provide a quantitative or at least scaling estimate of the loop contribution in the UHE domain, or qualify the abstract so that the all-order claim is explicitly restricted to the fan/generalized-fan class.
The paper says, at §4 and Figs. 7-8
The review did not quote this passage.
Pith says: Objection 2 of 3 · major
Section 4 states that 'All model parameters have been re-calibrated using a wider set of accelerator data', but the manuscript never says which observables entered that calibration. The two figures then compare the model to the pp total cross section (Fig. 7) and to F2 from H1, ZEUS and NMC (Fig. 8), which are exactly the observables most likely to sit in the calibration sample.
more of objection 2
If they do, these figures are illustrations of the fit, not tests of it, and the abstract's claim of a 'consistent description of hadron-hadron cross sections and hadron structure functions' (abstract:s3) rests on a comparison that is partly circular by construction. The figure text in §4 does say 'we illustrate the importance of Pomeron-Pomeron interactions', which is the correct framing; the abstract should match it. Please list explicitly which data sets were used in the re-calibration, and state clearly for each of Figs. 7 and 8 whether it is a fit or a prediction. If both are in the fit, either add one genuinely independent observable or soften the abstract wording.
The paper says, at §3, paragraph introducing Fig. 3
The review did not quote this passage.
Pith says: Objection 3 of 3 · major
The authors are commendably explicit that 'We make a basic assumption that [Pomeron-Pomeron interactions] are dominated by partonic processes at comparatively low virtuality scale, |q^2| < Q0^2', and that multi-Pomeron vertices therefore involve only soft Pomerons or the soft ends of semihard Pomerons.
more of objection 3
This assumption is load-bearing: it is what closes the fan and generalized-fan recursions and fixes the topology of the resummed eikonal in Fig. 6, and hence the screening strength that produces the curves in Figs. 7 and 8. Since the assumption is acknowledged, the remaining issue is that no argument or estimate is given for the size of a possible high-virtuality component in the triple-Pomeron vertex. A short qualitative statement — expected sign of the correction, its energy dependence, and whether it would strengthen or weaken screening — would let the reader judge how much of the agreement in Figs. 7 and 8 is robust. This, like the two comments above, is addressable by explicit statement rather than by new calculation, and I would not insist on a full numerical study within a proceedings length.
8 minor objections
The paper says, at Fig. 6 and caption
Pith says: minor objection 1 of 8
Figure 6 is a graphical equation carrying most of the paper's technical content, but the caption does not define its symbols: the meaning of the '=1', '>=0' and '>=2' labels, the role of the explicit '1/2 chi_tot' subtraction term, and the correspondence between the vertical lines and the full set of Fig. 6 diagrams are all left to the reader. An expanded caption or a short legend is needed for the figure to be usable independently of Ref. [15].
The paper says, at Fig. 7
Pith says: minor objection 2 of 8
The figure legend shows two entries both labelled 'p+p', and the caption does not say which curve is which or what the plotted points represent. Please label the full and dashed curves explicitly in the legend and state the source and energy range of the data points.
show 6 more
The paper says, at Fig. 8
Pith says: minor objection 3 of 8
The caption should state whether the H1, ZEUS and NMC points are shown at Q^2 = 2 GeV^2 directly or have been evolved/interpolated to that scale, and it should note that Q^2 = 2 GeV^2 sits at the lower boundary of applicability of the QCD ladder treatment used for the semihard Pomeron. A sentence on how the charm-exclusion caveat affects the comparison at small x would also help.
The paper says, at References [15] and [16]
Pith says: minor objection 4 of 8
The two references that carry the derivation of the resummation, the Monte Carlo sampling procedure, and the hadron-nucleus and EAS results are listed as 'in preparation' and 'these proceedings' respectively, so neither is available to the reader. A schematic of the sampling procedure — how cuts of the Fig. 6 diagrams are re-summed into event weights — would make the manuscript self-contained enough to be cited.
The paper says, at §2, AGK cutting rules
Pith says: minor objection 5 of 8
The step from 'calculating various unitarity cuts ... according to AGK cutting rules' to expressions for total and inelastic cross sections is the non-trivial part of the construction once triple-Pomeron vertices are present. One sentence on why the AGK cancellations survive in the presence of enhanced vertices — which is also what underlies the factorization statement in §4 — would strengthen the argument considerably.
The paper says, at §4, factorization statement
Pith says: minor objection 6 of 8
The claim that non-factorizable contributions vanish from inclusive high-pt jet spectra 'due to the AGK cancellations' is interesting and checkable, but it is asserted without argument or reference. Please indicate where this is demonstrated, or sketch the cancellation.
The paper says, at §1 and abstract, typography and grammar
Pith says: minor objection 7 of 8
Several small corrections are needed: 'explicitely' should be 'explicitly' (abstract, §1, §4); 'This condition cease to be valid' should be 'ceases'; 'partons resulted from the QCD cascades' should be 'partons resulting from'; and the virtuality cutoff is typeset inconsistently as 'Q 20' where Q_0^2 is intended (abstract of §2 and §3). Hyphenation of 're-summed'/'resummed' should be made uniform.
The paper says, at General
Pith says: minor objection 8 of 8
The manuscript contains no numbers at all: no fitted parameter values, no chi^2 or quality-of-fit measure, and no quoted cross-section or F2 values. Even for a proceedings, one or two representative numbers would let the reader gauge the quality of the agreement in Figs. 7 and 8 rather than judging it by eye.
What would settle it
Compute the leading Pomeron-loop correction to the Fig. 6 eikonal explicitly: insert one additional Pomeron exchange joining two generalized-fan contributions (the first topology omitted by the 'neglecting Pomeron loops' step) and evaluate its ratio to the fan-resummed eikonal at b = 0 for sqrt(s) = 10^4, 10^6 and 10^8 GeV. If that ratio stays below roughly 10-20% through 10^8 GeV (about 10^20 eV), the loop-neglect approximation is quantitatively defensible and the concern dissolves. If it grows past that level, the 'all orders' and 'reliable ultra-high-energy extrapolation' language needs an explicit energy-range qualification.
from the skeptic's reading
How the review went
4 readings by deepseek-v4.1-flash · 13 Nov 2026
- Reader holds up, with conditions
- Skeptic partly agrees
- Editor wrote the verdict above
- Referee minor revision: 3 major objections, 8 minor
Not run on this paper: the simulated authors' defence.
Pith did not check this review's objections against the paper.
The review in full
The review in brief, machine-written
The thing to know: this is the announcement paper for QGSJET-II, and the substantive advance is genuine. Prior QGSJET kept at most a single triple-Pomeron vertex; here the enhanced diagrams are resummed into a closed total eikonal (Fig. 6) for the uncut amplitude and for the relevant unitarity cuts, and the result is folded into an event-by-event Monte Carlo rather than applied as an average correction. That is the piece the field has been waiting for, and doing it for cut topologies — not just the elastic amplitude — is what makes it usable in a shower generator. The paper is also candid about being a summary, which I appreciate even though it costs it on completeness. The full-versus-dashed curves in Figs. 7 and 8 are a real internal ablation, and getting the pp total cross section and F2 at Q02 = 2 GeV2 out of one parameter set is a nontrivial consistency check, postdiction or not. I would not lean as hard on the calibration-circularity point as the reader does; the ablation is the evidence, and it holds up on its own terms. Where I do think the paper overreaches is the loop sentence in Section 3, just before Fig. 6: 'neglecting subdominant contributions of Pomeron loops.' The stress-test note lands. The resummation is all-orders only within the fan and generalized-fan topologies, and loops are precisely the class whose relative weight grows with energy. No numerical bound is given at 1019-1020 eV, so 'reliable model extrapolation into ultra-high energy domain' in the abstract is asserted, not demonstrated. The soft-dominance assumption for Pomeron-Pomeron vertices is at least flagged as an assumption; the loop truncation is not flagged at all, and the ablation cannot test it. Secondary: the derivation and sampling algorithm sit in ref. [15], 'in preparation', and the nuclear/EAS consequences in [16], 'these proceedings', so nothing here is independently checkable. For a four-page proceedings that is normal, but it means the paper's claims rest on work I cannot see. Who should read it: cosmic-ray people who use QGSJET and need to know what changed, and anyone tracking screening corrections in hadronic generators. Worth a serious referee, with the explicit ask that the companion paper quantify the neglected loops and give parameter values and fit quality.
The strongest objection
The central claim (abstract:s3, abstract:s2) is that enhanced Pomeron diagrams are resummed to all orders into a closed total eikonal (Fig. 6), and that this is what makes the model trustworthy at ultra-high energy. The load-bearing sentence sits in Section 3, immediately before Fig. 6: 'Then, neglecting subdominant contributions of Pomeron loops, the final result for hadron-hadron interaction eikonal can be represented in the graphical form as shown in Fig. 6.' So the resummation is all-orders only within the loopless subset (fan and generalized-fan topologies of Figs. 4 and 5). Pomeron loops are exactly the class of enhanced diagrams whose relative weight is expected to grow with energy; the fan series alone is the standard example of a set that does not by itself preserve t-channel unitarity asymptotically. The paper gives no estimate of the loop contribution at, say, 10^19-10^20 eV, so 'reliable model extrapolation into ultra-high energy domain' (abstract:s2) is asserted rather than bounded. This is a sibling of the reader's soft-dominance point, not the same point: soft dominance fixes which Pomerons may enter a multi-Pomeron vertex; loop neglect fixes which topologies are summed. Both are required for Fig. 6 to close, but only the first is flagged. The internal ablation in Figs. 7 and 8 (full versus dashed 'without enhanced diagrams') tests enhanced-versus-none, not loops-versus-no-loops, so it cannot speak to this. The derivation itself is deferred to reference [15], listed as 'in preparation', so the size of the neglected loops cannot be checked from this document either.
The reader's verdict of CONDITIONAL is right, and the reader's rationale already notes that the derivation and sampling algorithm live in reference [15], 'in preparation'. Where I would sharpen rather than redirect: the reader's weakest_assumption is the soft-dominance premise for Pomeron-Pomeron vertices (Section 3, Fig. 3). That premise is real and is stated as an assumption, but it is one of two approximations that the Fig. 6 closure depends on. The second, stated one sentence earlier in the same paragraph, is the neglect of Pomeron loops. That one is more directly in tension with the paper's own framing, because the abstract sells the result as an all-order resummation valid for ultra-high-energy extrapolation, and loops are the diagrams whose relative importance is conventionally expected to rise with energy. The paper does not quantify the neglected terms anywhere, and the only ablation it shows (full versus dashed curves in Figs. 7 and 8) switches enhanced diagrams on and off wholesale, so it cannot isolate the loop contribution. I therefore read the soft-dominance assumption as necessary but not sufficient for the central claim, and I would put the loop-neglect sentence at the top of the list of things a referee should ask to see bounded. On the evidence side, I share the reader's observation that Figs. 7 and 8 are shown after a re-calibration on a wider accelerator data set and that both observables flow from the same soft and semihard Pomeron parameters, so 'consistent description of cross sections and structure functions' is closer to a two-observable postdiction than to two independent tests. That is a correctness-risk point about how strongly the plots support the claim, not a claim that the numbers are wrong. The paper is honest about being a summary, and the graphical recursions plus the internal ablation are genuine content; nothing here reads as unsound, only as under-quantified. The verdict stays CONDITIONAL, and the concrete test above is the single check that would most cleanly separate 'defensible approximation' from 'unbounded extrapolation claim'.
The referee's report
If the resummation holds, this is a substantive step for the field: it replaces the linear (independent-cascade) Pomeron picture that underlies essentially all hadronic event generators used in air-shower work with a scheme in which screening is sampled event-by-event, and it does so without introducing new parameters relative to the existing model. Two features deserve explicit credit. First, the simultaneous description of two very different observables — the total pp cross section and the low-Q^2 proton structure function — with a single parameter set is a non-trivial consistency check, since the same eikonal controls both. Second, the observation in §4 that the semihard eikonal is no longer factorizable while inclusive high-pt jet spectra remain unaffected by AGK cancellations is a sharp, checkable statement: it predicts where the scheme must reproduce QCD factorization and where it must deviate, and it is the kind of claim that can be falsified against collider jet data. The nuclear extension, in which Pomerons of one enhanced graph may couple to different nucleons, is also a physically consequential prediction (violation of superposition for average EAS characteristics). The
Pith's reading of the paper (a machine's summary, not the authors')
This is the first general update of QGSJET, a hadronic interaction model that cosmic-ray groups use to simulate the cascades of particles that air showers are made of. The problem it attacks is stated early: the standard treatment assumes that the individual parton cascades exchanged in a collision, modelled as Pomerons, develop independently, and that assumption fails at high energy and small impact parameter, where many cascades overlap and screen one another. The paper's move is to resum the 'enhanced' diagrams that describe Pomeron-Pomeron interactions to all orders, both for the uncut elastic amplitude and for every unitarity cut corresponding to a physical final state, arriving at a closed expression for the total eikonal. The payoff claimed is consistency rather than a single number: one parameter set reproduces the measured total proton-proton cross section and the proton structure function $F_2(x,Q_0^2)$ at $Q_0^2=2$ GeV$^2$, and the resulting screening is then applied explicitly within sampled events instead of only on average. The reason a reader outside the field should care is that essentially all cosmic-ray data above $10^{14}$ eV are reconstructed through models of this kind, and the ultra-high-energy extrapolation is precisely where the independent-cascade assumption gives way.
What carries the argument. The carrying object is the total eikonal $X_{tot}(s,b) = X_P(s,b) + X_{sh}(s,b)$, the sum of a soft and a semihard Pomeron eikonal, out of which total, inelastic and configuration probabilities are obtained by applying the Abramovskii-Gribov-Kancheli cutting rules to the multi-Pomeron diagrams. The new ingredient is the replacement of each simple Pomeron exchange in that sum by a re-summed 'generalized fan' built from the recursive equations of Figs. 4 and 5. The recursion closes only because of a stated physical assumption about where Pomeron-Pomeron vertices live, and the closure is what turns an infinite class of enhanced graphs into a single computable eikonal that a Monte Carlo can then cut and sample.
Core claim. The central claim is that the non-linear, Pomeron-Pomeron interaction effects which spoil the independent-cascade picture can be re-summed to all orders into a usable, closed form, and that the result is a working model. Concretely, Ostapchenko computes the 'fan' diagram contribution from a recursive graphical equation, extends it to a 'generalized fan' that also includes vertices with fans attached to both the projectile and the target, and then, neglecting subdominant Pomeron-loop contributions, writes the full hadron-hadron interaction eikonal in the graphical form of Fig. 6. The elastic amplitude is the usual multi-Pomeron sum with each elementary exchange replaced by that full set of diagrams. The author then takes all unitarity cuts of those diagrams, re-sums cuts of given types, and builds a Monte Carlo procedure that samples interaction events of complicated topologies while accounting for screening in each particular cut-Pomeron configuration. The evidence offered for the whole construction is that the same parameter set lands on the measured total $pp$ cross section (Fig. 7) and on the proton structure function at $Q_0^2=2$ GeV$^2$ (Fig. 8), with and without the enhanced contributions shown side by side. Hadron-nucleus and nucleus-nucleus collisions are handled the same way with no new parameters, with the added feature that Pomerons of one enhanced graph may couple to different nucleons, which strengthens screening and breaks the superposition picture for nucleus-induced showers. A secondary observation is that the semihard contribution to the eikonal is no longer expressible in the factorized form assumed by earlier hadronic generators, though AGK cancellations keep inclusive high-$p_t$ jet spectra factorizable.
The premise it rests on. The load-bearing premise, stated by the author in Section 3, is that Pomeron-Pomeron interactions are dominated by partonic processes at low virtuality, $|q^2| < Q_0^2$, so that multi-Pomeron vertices involve only soft Pomerons or the soft ends of semihard ones.
If the paper is right (Pith's inferences, not the authors')
Cosmic-ray air-shower simulations above $10^{14}$ eV can be generated with screening corrections applied inside each simulated collision, rather than folded in as an average correction to the interaction probability.
The same parameter set should describe hadron-hadron cross sections and hadron structure functions simultaneously, removing a tuning tension between the two in earlier generators.
For nucleus-induced showers, the superposition of independent nucleon-nucleon collisions is expected to fail even for average shower characteristics, because one enhanced graph can couple to several nucleons.
Inclusive high-$p_t$ jet production should remain factorizable despite the new non-factorizable terms in the eikonal, because the AGK cancellations remove those diagrams from the inclusive jet spectrum.
The model is claimed to extrapolate into the ultra-high-energy domain without the independent-Pomeron assumption, which is the regime where previous hadronic generators had no controlled answer.
Because the closure of the fan recursion rests on Pomeron-Pomeron vertices being soft, the model's screening strength is effectively a one-parameter family; a future measurement that pins the high-virtuality content of the triple-Pomeron vertex would sharpen or overturn the whole extrapolation.
The simultaneous fit to the total cross section and to $F_2$ at a single low scale is a consistency check rather than a prediction; the sharper test is whether the same parameters survive at a higher $Q^2$ where the semihard component dominates.
Since nucleus collisions reuse the same machinery with no new parameters, the predicted violation of superposition gives a cleaner discriminator than the $pp$ cross section, which was already well measured before this work.
The statement that inclusive jets stay factorizable while the eikonal does not suggests a useful diagnostic: observables built from AGK-cancelling combinations should be insensitive to the new screening, and any measured sensitivity would point to a breakdown of the soft-vertex assumption.
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The paper
Abstract
Since a number of years the QGSJET model has been successfully used by different groups in the field of high energy cosmic rays. Current work is devoted to the first general update of the model. The key improvement is connected to an account for non-linear interaction effects which are of crucial importance for reliable model extrapolation into ultra-high energy domain. The proposed formalism allows to obtain a consistent description of hadron-hadron cross sections and hadron structure functions and to treat non-linear effects explicitely in individual hadronic and nuclear collisions. Other ameliorations concern the treatment of low mass diffraction, employment of realistic nuclear density profiles, and re-calibration of model parameters using a wider set of accelerator data.
The paper's own sentences, arranged, kept beside the review and separate from it. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. No sentence in this record was written by a model.
abstract compiled · 2026-09-23
The authors' main claim, as the classifier picked it out 0.69
“The proposed formalism allows to obtain a consistent description of hadron-hadron cross sections and hadron structure functions and to treat non-linear effects explicitely in individual hadronic and nuclear collisions.”
How the main claim is stated: asserted 0.85
What the abstract itself states, as probabilities: claims first 0.66 · states limitation 0.09 · human participants 0.02 · controlled comparison 0.05 · randomized assignment 0.01 · states quantitative result 0.04 · compares with prior results 0.24 · mentions code or data availability 0.03
The abstract, sentence by sentence
This table labels the abstract only (arXiv listing abstract v1). The number is the probability the classifier gave the label.
| Sentence | Role | The authors' own work | States the main conclusion | Strength |
|---|---|---|---|---|
| Since a number of years the QGSJET model has been successfully used by different groups in the field of high energy cosmic rays. | background 1.00 | 0.07 | 0.03 | asserted 1.00 |
| Current work is devoted to the first general update of the model. | contribution 0.93 | 0.78 | 0.05 | asserted 0.99 |
| The key improvement is connected to an account for non-linear interaction effects which are of crucial importance for reliable model extrapolation into ultra-high energy domain. | contribution 0.95 | 0.53 | 0.55 | asserted 1.00 |
| The proposed formalism allows to obtain a consistent description of hadron-hadron cross sections and hadron structure functions and to treat non-linear effects explicitely in individual hadronic and nuclear collisions. | contribution 0.47 | 0.81 | 0.34 | asserted 0.85 |
| Other ameliorations concern the treatment of low mass diffraction, employment of realistic nuclear density profiles, and re-calibration of model parameters using a wider set of accelerator data. | contribution 0.87 | 0.83 | 0.07 | asserted 0.99 |
What kind of paper the classifier reports this is: method or tool 0.83 · evidence from simulation or computation 0.49
What was examined, and what was not
Sources read
- arXiv listing abstract v1
Not examined
- full text
- figures and tables
- references and citing sentences
- relations to other papers
Levels run
- P abstract
Not run
- S sections
- T body sentences
- C citations
- R cross-paper relations
How the labels were made
Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,252 input tokens, $0.0002 reported.
Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. This record as JSON
Figures (8)
Showing 5 of the paper's 8 figures. Figures are the authors', reproduced from the paper.
References (21)
- [15] S. Ostapchenko, in preparation on Pith
- [16] S. Ostapchenko, Nucl. Phys. Proc. Suppl. B (2005), these proceedings on Pith
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- [7] S. Ostapchenko et al., J. Phys. G: Nucl. Part. Phys. 28 (2002) 2597. 0 0.5 1 1.5 2 10 -5 10 -4 10 -3 10 -2 10 -1 x F2(x,Q2) Q2=2 GeV2 Figure 8. Proton SF F2 calculated with (full curve) and without (dashed curve) enhanced dia- gram contributions. The data are from [19,20,21] on Pith
- [8] V.N. Gribov, Sov. Phys. JETP 26 (1968) 414 on Pith
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- [12] H.J. Drescher et al. , Phys. Rep. 350 (2001) 93 on Pith
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- [17] N.N. Kalmykov et al. , Proc. 26 th Int. Cosmic Ray Conf. (Salt Lake City), v.1, p.419 (1999) on Pith
- [18] C. Caso et al. , Eur. Phys. J. C3 (1998) 1 on Pith
- [19] S. Aid et al. , H1 Collaboration, Nucl. Phys. B470 (1996) 3 on Pith
- [20] M. Derrick et al. , ZEUS Collaboration, Z. Phys. C72 (1996) 399 on Pith
show 1 more
- [21] M. Arneodo et al., NMC Collaboration, Phys. Lett. B364 (1995) 107 on Pith
Cited by 13 Pith papers
Reviewed papers on Pith that cite this one. The full citation record
- Angular Distribution of Gamma Rays Produced in Proton-Proton Collisions hep-ph · Dec 2024
- Search for ultra-high energy photons: observing the preshower effect with gamma-ray telescopes astro-ph.IM · Aug 2019
- Muons in air showers at the Pierre Auger Observatory: Mean number in highly inclined events astro-ph.HE · Aug 2014
- Parametrization of gamma-ray production cross-sections for pp interactions in a broad proton energy range from the kinematic threshold to PeV energies astro-ph.HE · Jun 2014
- Measurement of the inelastic proton-proton cross section at sqrt(s) = 7 TeV hep-ex · Oct 2012
- Hadronic Multiparticle Production at Ultra-High Energies and Extensive Air Showers hep-ph · Oct 2010
- One-dimensional Hybrid Approach to Extensive Air Shower Simulation astro-ph · Jun 2006
- Chromo: A High-Performance Python Interface to Hadronic Event Generators for Collider and Cosmic-Ray Simulations physics.comp-ph · Jul 2025
- Measurement of the inelastic proton-proton cross section at $\sqrt{s}=$ 13 TeV hep-ex · Feb 2018
- Constraints from the first LHC data on hadronic event generators for ultra-high energy cosmic-ray physics astro-ph.HE · Jan 2011
- Physics at a 100 TeV pp collider: Standard Model processes hep-ph · Jul 2016
- Overview of high-density QCD studies with the CMS experiment at the LHC nucl-ex · May 2024
- Software and computing for Run 3 of the ATLAS experiment at the LHC hep-ex · Apr 2024
How later papers used it
60 later papers cite it
18 later papers by other authors are listed below: 18 used its method or tool.
Uses its method or tool 18 of 35 papers with this label
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Used QGSJETII.4 as one of the high energy hadronic interaction models in its study.
Measurement of the Proton-Air Cross Section with Telescope Array's Middle Drum Detector and Surface Array in Hybrid Mode (2015) · 0.92 · paraphrased: the licence does not allow quoting
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In this analysis we have adopted the CORSIKA [ref] event generator incorporating QGSJET [ref] for the hadronic interaction model to simulate the generation and development of EAS.
Study of cosmic ray events with high muon multiplicity using the ALICE detector at the CERN Large Hadron Collider (2015) · Analysis of the data and simulation · 1.00
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Performed simulations of gamma-ray and cosmic-ray air shower cascades with the CORSIKA v6.99 Monte Carlo package and the QGSJet II-03 hadronic interaction model.
Monte Carlo Studies of medium-size telescope designs for the Cherenkov Telescope Array (2015) · 1.00 · paraphrased: the licence does not allow quoting
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Selected the QGSJET-II-03 hadronic model for high energies in its standard simulated event set.
CORSIKA Simulation of the Telescope Array Surface Detector (2014) · 1.00 · paraphrased: the licence does not allow quoting
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For this purpose we simulated interactions at both beam momenta with the hadronic event generators [ref] and [ref] with the crmc program [ref] .
Measurement of Hadron Production in $\pi^-$-C Interactions at 158 and 350 GeV/c with NA61/SHINE at the CERN SPS (2022) · Simulation · 1.00
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Used the CoREAS plugin of CORSIKA with QGSJETII and FLUKA as the hadronic interaction models.
Probing Atmospheric Electric Fields in Thunderstorms through Radio Emission from Cosmic-Ray-Induced Air Showers (2015) · 0.93 · paraphrased: the licence does not allow quoting
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Used the CoREAS plugin of CORSIKA, employing QGSJETII.04 as the hadronic interaction model, to generate radio emission intensity patterns.
Measuring a Cherenkov ring in the radio emission from air showers at 110-190 MHz with LOFAR (2014) · 1.00 · paraphrased: the licence does not allow quoting
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Obtained its energies from a Monte Carlo simulation of the SD using CORSIKA and the hadronic generator QGSJET II-3.
Search for EeV Protons of Galactic Origin (2016) · 1.00 · paraphrased: the licence does not allow quoting
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Used the QGSJet-II and FLUKA models for high and low energy interactions, respectively.
A phenomenological model of the muon density profile on the ground of very inclined air showers (2009) · 0.99 · paraphrased: the licence does not allow quoting
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Generated most of its showers using the QGSJETII model for high energy and the GHEISHA model for low energy hadronic interactions.
On the Estimation of the Depth of Maximum of Extensive Air Showers Using the Steepness Parameter of the Lateral Distribution of Cherenkov Radiation (2021) · 0.99 · paraphrased: the licence does not allow quoting
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Used simulated extensive air showers generated with the CORSIKA package, using the QGSJet-II-03 model for hadronic interactions, for event reconstruction and detector calibration.
Constraining the $\bar{p}/p$ Ratio in TeV Cosmic Rays with Observations of the Moon Shadow by HAWC (2018) · 1.00 · paraphrased: the licence does not allow quoting
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Utilized the aafrag package, based on the QGSJET-II nuclear interaction model, to calculate cross sections for its gamma-ray spectra.
Spatial dependence of the break in the energy spectrum of cosmic rays in the new anisotropic diffusion approach (2025) · 1.00 · paraphrased: the licence does not allow quoting
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Generated its tables from iron shower simulations produced by CORSIKA 6.702, using QGSJET-II for the high-energy interactions.
Measurement of the Iron Spectrum in Cosmic Rays by VERITAS (2018) · 0.99 · paraphrased: the licence does not allow quoting
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Used Corsika for extensive air-shower cascades with GHEISGA and QGSJET-II attached for hadronic interactions.
Probing new physics with high-multiplicity events: UHE neutrinos at air-shower detector arrays (2018) · 1.00 · paraphrased: the licence does not allow quoting
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Estimated its low mass diffraction correction with QGSJET-II-03.
First measurement of elastic, inelastic and total cross-section at $\sqrt{s}=13$ TeV by TOTEM and overview of cross-section data at LHC energies (2017) · 1.00 · paraphrased: the licence does not allow quoting
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Simulated 5678 proton showers with the Corsika 6.616 code using QGSJetII-03 for high energy hadronic interactions.
The angular resolution of the Pierre Auger Observatory (2009) · 1.00 · paraphrased: the licence does not allow quoting
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Modeled high energy hadronic interactions with QGSJET-II-03.
Dethinning Extensive Air Shower Simulations (2011) · 1.00 · paraphrased: the licence does not allow quoting
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The EAS background is simulated using the CORSIKA [ref] and QGSJET-II-04 [ref] , which model cosmic-ray interactions in the atmosphere and the subsequent development of particle cascades.
From raw data to neutrino candidates: a neural-network pipeline for Baikal-GVD (2026) · Monte Carlo simulations · 1.00
How the literature uses it
41 arXiv papers cite this in 53 sentences
Papers citing it · 17 sentences without a confident label
Uses its method or tool 26 papers
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Average numbers of hadrons $N_(E_,>E_)$ and muons $N_μ(E_,>E_)$ with energies above $E_$ in EAS from primary nucleon of energy $E_$ were obtained with the help of one-dimensional hybrid code CONEX [ref] in regime of cascade equations solution for interaction models QGSJET 01 [ref] , SIBYLL 2.1 [ref] , NEXUS 3.97 [ref] and QGSJET-II-03 [ref] .
Shape of primary proton spectrum in multi-TeV region from data on vertical muon flux · Calculations technique of atmospheric muon and hadron fluxes · 1.00
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The high energy models used in this study are QGSJETII.4 [ref] , QGSJET01 [ref] , SIBYLL [ref] , and EPOS-LHC [ref] .
Measurement of the Proton-Air Cross Section with Telescope Array's Middle Drum Detector and Surface Array in Hybrid Mode · Analysis · 0.92
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In this analysis we have adopted the CORSIKA [ref] event generator incorporating QGSJET [ref] for the hadronic interaction model to simulate the generation and development of EAS.
Study of cosmic ray events with high muon multiplicity using the ALICE detector at the CERN Large Hadron Collider · Analysis of the data and simulation · 1.00
Uses its data or values 1 paper
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where $ρ_μ,19$ is the parametrized ground density for a proton shower simulated at $10^19$ eV with the hadronic interaction model II-03 [ref] .
Muons in air showers at the Pierre Auger Observatory: Mean number in highly inclined events · Reconstruction of the muon number · 0.82
Compares with it 4 papers
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The “crossing energies” derived with QGSM [ref] , PROSA [ref] and GM-VFNS [ref] are almost coincident for KM (close to that for SIBYLL 2.3c [ref] ) and QGSJET-II-03 [ref] taken separately.
High-energy spectra of the atmospheric neutrinos: predictions and measurements · Results and discussion · 0.81
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The measured cross sections are also compared to the predictions of 6 Z2* [ref] and to MC generators based on Regge–Gribov phenomenology: (version 1.12-35) [ref] , (versions 03 and 04) [ref] , and LHC [ref] ; the latter two are commonly used in cosmic-ray physics [ref] .
Measurement of diffraction dissociation cross sections in pp collisions at sqrt(s) = 7 TeV · Monte Carlo simulation · 0.95
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These measurements are compared with predictions of general-purpose MC generators 6.4 [ref] , 8 [ref] for a variety of generator parameter tunes; generators specific to large rapidity gap physics [ref] ; and generators used in cosmic ray physics [ref] , [ref] , and [ref] .
Stairway to discovery: a report on the CMS programme of cross section measurements from millibarns to femtobarns · Total inelastic cross sections · 0.91
Cites it as background 2 papers
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QGSJET01 [ref] , QGSJET II [ref] and SIBYLL [ref] focus on the bulk production of soft particles for simulating extensive air showers caused by high energy CR particles.
Investigating the dark matter signal in the cosmic ray antiproton flux with the machine learning method · Hadronic models · 0.89
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A large family of simulation programs also exists for heavy-ion physics and air showers [ref] .
Snowmass 2021 White Paper: Electron Ion Collider for High Energy Physics · Monte Carlo and Machine Learning · 0.88
Challenges and discussion
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