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High Energy Physics - Phenomenology · arXiv:hep-ph/0304285 v2 · submitted 30 Apr 2003 · 54 references

Chern-Simons production during preheating in hybrid inflation models

Juan Garcia-Bellido, Margarita Garcia Perez, Antonio Gonzalez-Arroyo

The paper says

“We study the onset of symmetry breaking after hybrid inflation in a model having the field content of the SU(2) gauge-scalar sector of the standard model, coupled to a singlet inflaton.”

more of the abstract

This process is studied in (3+1)-dimensions in a fully non-perturbative way with the help of lattice techniques within the classical approximation. We focus on the role played by gauge fields and, in particular, on the generation of Chern-Simons number. Our results are shown to be insensitive to the various cut-offs introduced in our numerical approach. The spectra preserves a large hierarchy between long and short-wavelength modes during the whole period of symmetry breaking and Chern-Simons generation, confirming that the dynamics is driven by the low momentum sector of the theory. We establish that the Chern-Simons production mechanism is associated with local sphaleron-like structures. The corresponding sphaleron rates are of order 10^-5 m^4, which, within certain scenarios of electroweak baryogenesis and a (not unnaturally large) additional source of CP violation, could explain the present baryon asymmetry of the universe.

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.

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Holds up, with conditions. A real first 3+1D lattice measurement of Chern-Simons production during tachyonic preheating, but the headline rate and the cutoff-independence claim are established at mH/mW = 4.65, not at the physical mass ratio. This line is wrong

4 major objections · 9 minor

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The paper says, at Abstract [abstract:s3]; Sec. IV C; Table II; Fig. 7

The review did not quote this passage.

Pith says: Objection 1 of 4 · major

The abstract states without qualification that 'Our results are shown to be insensitive to the various cut-offs introduced in our numerical approach,' but the body establishes this only for model A1. The authors themselves write in Sec. IV C that 'as we decrease the ratio our results, in particular those concerning the Chern-Simons number, become increasingly sensitive to the cutoffs,' and identify m_W a as the controlling scale.

more of objection 1

Table II bears this out: model A3 gives I(45) = 38.00(5.62) at Ns = 48 versus 24.58(2.42) at Ns = 32, a 55% difference; model A4 gives 16.10(1.74) versus 14.17(1.44); model B rises monotonically from 14.89(1.65) at Ns = 32 to 19.89(1.74) at Ns = 64. Only model A1, at m_H/m_W = 4.65, shows the flat behaviour of Fig. 7. The abstract's unqualified claim should either be restricted to the parameter window where it is demonstrated, or supported by an A4 run at reduced m_W a. As written, a reader of the abstract alone would conclude that cutoff independence has been shown for the Standard Model mass ratio, which is not the case.

The paper says, at Sec. IV C, paragraph on model B; Table II

The review did not quote this passage.

Pith says: Objection 2 of 4 · major

The statement that model B, after a time shift of 3.3/m and a 20% rescaling, 'match[es] perfectly' with model A1 is made at a single lattice size (Ns = 48, pmin = 0.15m). Model B is simultaneously the entry with the largest cutoff dependence in Table II, rising by roughly 34% between Ns = 32 and Ns = 64.

more of objection 2

The agreement with A1 is therefore asserted at precisely the point where B's own systematic uncertainty is least controlled, and the 20% rescaling is of the same order as that uncertainty. Either the comparison should be repeated at Ns = 64, or the text should state that the A1-B agreement is established only at one lattice spacing and is subject to B's own cutoff systematics.

The paper says, at Sec. IV D, Figs. 13-14; Abstract [abstract:s5]

The review did not quote this passage.

Pith says: Objection 3 of 4 · major

The abstract states 'We establish that the Chern-Simons production mechanism is associated with local sphaleron-like structures,' but Sec. IV D reports 'a relative time shift Δmt = 2 − 3 between the presence of zeroes in the Higgs field and that of maxima in the charge density.'

more of objection 3

For a static sphaleron the magnetic energy maximum sits at the Higgs zero by construction, so a shift of two to three inverse inflaton masses indicates that the observed objects are dynamical transients rather than sphaleron configurations. The body is appropriately hedged ('one might be tempted to identify'), but the abstract's 'establish' is stronger than the evidence supports. I would ask the authors to either soften the abstract wording to match the body, or to quantify the offset — for instance, by showing the distribution of |φ| at the charge-density peak positions rather than only the contour overlays.

The paper says, at Sec. V, Eqs. (16)-(18)

The review did not quote this passage.

Pith says: Objection 4 of 4 · major

The baryon-asymmetry estimate uses Γ_sph ~ 2 × 10^{-5} m^4, a value read from Table II at m_H/m_W = 4.65 (model A1) and 2.82 (model A2). Fig. 9 shows that I(mt) varies by factors of two to three across the model set and depends sensitively on m_H/m_W, and the paper's own Sec.

more of objection 4

IV C identifies the physical ratio as the case least controlled by the cutoff scan. The derived δ_CP ~ 10^{-3} therefore inherits a factor-of-few uncertainty that is not propagated. Since the conclusion is explicitly order-of-magnitude, this is not fatal, but Eq. (18) should carry an explicit statement of the range of δ_CP implied by the spread in Table II, rather than a single number. Relatedly, the criterion m_W a ≤ 0.40-0.60 used to justify the parameter choices is imported from the vacuum sphaleron study of Ref. [45]; applying it to a far-from-equilibrium dynamical process is an extrapolation beyond the source's stated hypotheses and should be flagged as an assumption in the text rather than presented as an established bound.

9 minor objections

The paper says, at Abstract

Pith says: minor objection 1 of 9

Grammatical: 'The spectra preserves a large hierarchy' should read 'The spectra preserve a large hierarchy.'

The paper says, at Table I

Pith says: minor objection 2 of 9

The inflaton bare mass is listed as μ = 10^{-5} gv ≈ 0. Please state explicitly in the caption or the surrounding text that μ is set to zero in the evolution, since the equations of motion in Appendix A retain μ_L.

show 7 more

The paper says, at Table II

Pith says: minor objection 3 of 9

The caption says errors are 'computed in the standard fashion from the dispersion within the various configurations.' Please give the formula (standard error of the mean over configurations, or the dispersion of the estimator from a jackknife) so that the reader can judge whether the quoted errors on I(mt) are correlated across times.

The paper says, at Fig. 8

Pith says: minor objection 4 of 9

The caption should state that the pmin = 0.12m data are rescaled by the square root of the volume because ΔN_CS² scales linearly with volume, and should give the number of configurations entering each histogram.

The paper says, at Sec. IV C, paragraph on cutoff independence

Pith says: minor objection 5 of 9

It would help the reader considerably if the values of m_W a for each model and each lattice size were tabulated alongside Table II, so that the comparison with the Ref. [45] criterion can be made without recomputation. At present the reader must reconstruct m_W = m g_W/(2√λ) and ma for each row.

The paper says, at Appendix B

Pith says: minor objection 6 of 9

The residual Gauss-constraint violation is quoted as 'smaller than 10^{-11}.' Please state whether this is an absolute or a relative measure, and over what time interval it holds.

The paper says, at Figs. 3 and 4

Pith says: minor objection 7 of 9

The axis labels and legends in these figures are difficult to read in the current version; the panel structure (six stacked panels per side) also makes it hard to identify which curve corresponds to which cutoff. Consider consolidating or enlarging.

The paper says, at Sec. VI, Conclusions

Pith says: minor objection 8 of 9

The conclusions would be strengthened by an explicit statement of which of the specific objections raised in Ref. [43] are addressed by the present data and which remain open. The rebuttal in Sec. IV B is effective but is not carried through to the concluding summary.

The paper says, at Sec. III B 1 and Appendix B

Pith says: minor objection 9 of 9

The choice to set all propagating gauge modes to zero initially is defended by the argument that there are no tachyonic gauge modes. A short quantitative remark on how large a nonzero initial gauge fluctuation would have to be before I(mt) changes appreciably would make this defence more convincing, since this choice is precisely the point on which Ref. [43]'s criticism turns.

What would settle it

Run model A4 (gW = 0.15, λ = 0.00675, mH/mW = 1.55) at Ns = 96 with pmin = 0.15m (ma ≈ 0.436, mW a ≈ 0.40, at the edge of the paper's stated safe range) and accumulate ~150 configurations, matching the statistics of the Ns = 48 run. Compare I(45) with the tabulated Ns = 48 value of 16.10 ± 1.74 × 10^-5. If the two agree within errors, the physical-ratio rate is cutoff-controlled and the concern does not land; if I(45) shifts by more than the quoted error (as the Ns = 48 vs Ns = 32 discrepancy of ~12% hints), the abstract's unqualified cutoff-insensitivity claim and the 10^-5 m^4 rate are not established at the physical mass ratio. A cheaper intermediate check is Ns = 64 at pmin = 0.20m (ma ≈ 0.49, mW a ≈ 0.45), which should show the trend.

from the skeptic's reading

How the review went

4 readings by deepseek-v4.1-flash · 13 Nov 2026

  1. Reader holds up, with conditions confidence moderate
  2. Skeptic partly agrees 2 min 12 s · 34,041 tokens read, 7,171 written
  3. Editor wrote the verdict above 17 s · 35,161 tokens read, 1,034 written
  4. Referee major revision: 4 major objections, 9 minor 1 min 57 s · 34,454 tokens read, 6,965 written

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

This is the paper that puts non-Abelian gauge fields into the tachyonic preheating story and actually measures Chern-Simons number on the lattice. That is the contribution, and it is worth your time. The setup is careful: quantum-matched initial conditions from the linear evolution, a proper lattice action with the Gauss constraint imposed at ti, and Appendices A and B spell out the discretization and the constraint implementation so someone could redo it. The cutoff scan is genuine — Fig. 7 shows I(mt) collapsing across ma = 0.65, 0.87, 1.30 for model A1 — and the statistics (130-210 configurations per point, Gaussian fits with chi-squared near 1) are adequate for a fluctuating quantity like this. The direct answer to Moore's Ref. [43] criticism holds within the parameter range studied, and the localization analysis in Sec. IV D (a few percent of the volume carrying 80-90% of the charge squared, structures of size ~1/mW) is a nice piece of work. The paper is also honest that the lumps are only 'sphaleron-like': it reports the Delta mt = 2-3 offset between Higgs zeros and charge maxima and never compares to the static sphaleron solution, so the identification stays correlational. That is a fair limitation, not a flaw in the lattice result itself. The stress-test concern lands, though. The abstract's 'insensitive to the various cut-offs' and the 10−5 m4 rate are established for model A1, where mH/mW = 4.65 and mW a sits inside the safe range imported from Ref. [45]. The paper's own Sec. IV C says sensitivity grows as the ratio decreases, and model A4 — the closest to physical at mH/mW = 1.55 — has mW a ~ 0.79 at Ns = 48, outside the paper's own stated criterion, with a ~12% discrepancy between Ns = 48 and Ns = 32 in Table II. Convergence of I(mt) for A4 as mW a drops below 0.4 is never shown. So the rate that feeds Sec. V is the one least controlled by the cutoff scan. Sec. V itself is an order-of-magnitude estimate with delta_CP, M_new and T_eff chosen to land on the observed asymmetry; the authors acknowledge this, so it is not a new finding, but the abstract should not read as if the rate were a Standard Model number. For readers working on electroweak baryogenesis or on lattice real-time dynamics this is a must-read and a solid reference. Send it to referees; the revision should either demonstrate A4 convergence or soften the abstract's cutoff claim and the rate's framing.

The strongest objection

The headline rate (abstract:s6) and the unqualified cutoff-insensitivity claim (abstract:s3) rest on Fig. 7 and Table II, which are dominated by model A1 (gW = 0.05, mH/mW = 4.65). The paper's own Sec. IV C states that 'as we decrease the ratio our results, in particular those concerning the Chern-Simons number, become increasingly sensitive to the cutoffs,' and that the controlling scale is mW a. For model A1 at ma = 0.65-1.30, mW a = 0.19-0.40, inside the safe range the paper imports from Ref. [45] (mW a ≤ 0.40-0.60). For model A4 (mH/mW = 1.55, the closest to the physical 125/80 ≈ 1.56), mW = 0.91 m, so at Ns = 48, pmin = 0.15m (ma = 0.87) one has mW a ≈ 0.79 — outside the paper's own stated criterion. Table II shows A4's I(45) differing by ~12% between Ns = 48 (16.10 ± 1.74) and Ns = 32 (14.17 ± 1.44), a larger discrepancy than A1's. The paper never demonstrates convergence of I(mt) for A4 as mW a is reduced below 0.4. Consequently the abstract's 'insensitive to the various cut-offs' and the quoted 10^-5 m^4 are not established at the physical mass ratio; they are established at a ratio where the Higgs is 4.65 times the W, which is not the Standard Model. This is the load-bearing gap: the rate that would feed Sec. V's baryogenesis estimate is the one least controlled by the cutoff scan.

The reader's weakest_assumption correctly locates the soft spot, but frames it as 'the rate depends only on mW a and not on mH a.' The paper does not quite claim that; it claims cutoff independence at fixed model and separately notes the rate depends on mH/mW. The sharper statement is that the cutoff-independence demonstration is confined to model A1 (mH/mW = 4.65), while the physically relevant ratio (A4, mH/mW ≈ 1.55) is the one the paper flags as most cutoff-sensitive and where mW a ≈ 0.79 at Ns = 48 exceeds the paper's own imported safe range. So the concern is real and load-bearing for the abstract's unqualified claim and for the 10^-5 m^4 number that feeds Sec. V. It does not overturn the central lattice result — CS number is generated, locally, with a Gaussian distribution, and A1's cutoff scan is genuine — so the verdict stays CONDITIONAL. The sphaleron-identification concern (Sec. IV D, Δmt = 2-3 offset, no comparison to the static solution) is secondary and the paper hedges with 'sphaleron-like'; the CP-violation gap in Sec. V is acknowledged by the authors. Neither displaces the cutoff concern as the most load-bearing. I therefore agree partially with the reader: same target, sharper framing, same verdict.

The referee's report

If the results hold, this is a substantive contribution: it is one of the first fully nonperturbative (3+1)-dimensional treatments of Chern-Simons production during tachyonic preheating with non-Abelian gauge fields, and it supplies the raw ingredient that the electroweak preheating baryogenesis scenario of Ref. [9] requires. The paper earns credit on several counts. The lattice action, equations of motion, gauge fixing, and the Gauss-constraint initialization are written out in Appendices A and B, so the numerical scheme is reproducible in principle. The statistical effort is real: 128 to 210 configurations per parameter point, with quoted errors, and Gaussian fits to the ΔN_CS distribution with χ² per degree of freedom of order unity. The direct rebuttal of Ref. [43] in Sec. IV B, via spectra at three lattice spacings and three times, is exactly the right kind of evidence to bring to that dispute. The localization analysis in Sec. IV D — the fraction of charge-squared inside 1/m_W spheres, the minimum-distance histograms of Fig. 12 — is a genuine, checkable structural claim. And Sec. V is honestly labelled an order-of-magnitude estimate rather than a prediction. The weaknesses I.

Pith's reading of the paper (a machine's summary, not the authors')

Hybrid inflation ends when the inflaton rolls past a critical value and the Higgs field, held at zero until then, suddenly finds itself with a negative mass squared. The paper asks whether the resulting collapse into the true vacuum also shakes loose Chern-Simons number, the quantity that anomalous electroweak processes convert into baryon number. The authors simulate the $SU(2)$ gauge-Higgs sector plus a singlet inflaton on a $(3+1)$-dimensional lattice, evolving the long-wavelength modes classically and seeding them with the stochastic distribution that linear quantum evolution predicts at the moment those modes become classical. They report that Chern-Simons number does diffuse, at a rate of order $10^{-5}m^4$, that the production sits in compact lumps of size about $1/m_W$ located where the Higgs field lingers near zero, and that the answer barely moves when the lattice spacing or box size is changed. If that holds, the interval right after hybrid inflation supplies the out-of-equilibrium ingredient baryogenesis needs, and the classical lattice treatment survives the objection that its spectra are swamped by short-wavelength artifacts.

What carries the argument. The load-bearing object is the lattice topological charge density, built from $1times1$, $1times2$ and $2times2$ plaquettes combined to cancel the leading $O(a^2)$ error, so that $Q(vec{x},t)$ is measured without adding discretization artifacts of its own. Around it sit three supporting devices: gauge-invariant lattice equations of motion in which Gauss's law, once imposed initially, is shown to propagate (Appendix A); an initialization scheme that leaves the Higgs distribution untouched and puts all the necessary charge into the longitudinal electric field, with the transverse part set to zero (Appendix B); and a cutoff-independence test in which the box size $p_{min}$ and the lattice spacing $ma$ are varied separately, since volume should scale the dispersion $langle Delta N_{CS}^2 rangle$ while the spacing should not.

Core claim. The central claim is that the symmetry-breaking transition after hybrid inflation is itself a Chern-Simons source. Working in the $A_0=0$ gauge with the Gauss constraint imposed on the initial data, the authors measure $I(mt) = m^{-3}V^{-1}m^2 dlangle Delta N_{CS}^2 rangle/dt$ and find it rising from zero around $mt approx 15$, steeply at first with oscillations up to $mt approx 25$, then more gently, reaching values of order $10^{-5}$ in the units shown in their Table II. The distribution of $Delta N_{CS}$ across configurations is Gaussian to within a $chi^2$ of about 1 per degree of freedom, consistent with production in many independent local events of random sign. Those events are resolved: peaks of the topological charge density $Q = 4,mathrm{Tr}(vec{E}cdotvec{B})$ above $7m_W^4$ occupy a few percent of the lattice volume while containing 60 to 90 percent of the charge squared, sit inside spheres of radius $1/m_W$, and appear at the points where the Higgs field stays longest in the false vacuum, with a lag of $Delta mt = 2$ to $3$ between the Higgs zeros and the charge maxima. The authors also argue that the long-wavelength modes stay dominant throughout, so the classical approximation is not undone by the ultraviolet cascade that Ref. [43] warned about.

The premise it rests on. The rate is assumed to depend only on the combination $m_W a$ and not on $m_H a$, a scaling imported from lattice studies of static vacuum sphalerons and applied here to a violently non-equilibrium process; if it fails, the demonstrated cutoff independence does not carry over to physical Higgs-to-W mass ratios.

If the paper is right (Pith's inferences, not the authors')

With a dimension-six CP-odd operator of the form $delta_{CP}(Phi^daggerPhi/M_{new}^2)(3g_W^2/32pi^2)Ftilde{F}$, the rate quoted here gives $n_B/s approx 1.1times10^{-8}delta_{CP}$ for $M_{new} approx 3$ TeV, so $delta_{CP} approx 10^{-3}$ would match the observed asymmetry.

The classical-statistical lattice method, with stochastic initial conditions taken at $mt_i = 5$ rather than at the bifurcation point, is argued to be a valid tool for this problem up to the cutoffs used, answering the spectral-cascade criticism directly.

The Chern-Simons yield depends on the Higgs-to-W mass ratio: the four A-models share $lambda$ and differ only in $g_W$, and their $I(mt)$ curves differ by factors of two or more, so no single number can be read off as the Standard Model value.

The production is spatially clustered and time-lagged relative to the Higgs zeros, which means the mechanism is not a gas of static sphalerons but a set of driven, oscillating configurations whose charge density even flips sign at fixed location.

Model B, with a gauge coupling closer to the Standard Model value, matches model A1 after a time shift of $3.3/m$ and a 20 percent rescaling, suggesting the result tracks $m_H/m_W$ rather than the absolute coupling.

The $Delta mt = 2$ to $3$ lag between a Higgs zero and the charge-density maximum suggests the lumps are not passing through the sphaleron saddle quasistatically; tracking the field trajectory through one lump would show whether it actually crosses the barrier or merely oscillates near it.

Because $Q$ flips sign at a fixed point as $vec{E}$ and $vec{B}$ oscillate out of phase, the net Chern-Simons number accumulated by a single lump nearly cancels; the efficiency of any CP-biased baryogenesis therefore depends on how the bias period compares with the oscillation period, a timing question the paper raises but does not resolve.

The oscillatory dependence of the gauge energy fraction on $g_W$, with a maximum near $g_W = 0.0825$ and a minimum near $0.147$, hints at a resonance between the Higgs oscillation frequency and the gauge field mass, which would be worth mapping before any extrapolation to physical couplings.

A run at $m_H/m_W approx 1$ with $m_H a approx 0.4$ and $N_s gtrsim 148$, which the authors say is beyond their present resources, is the natural next step and would decide whether the quoted rate is a property of the dynamics or of the parameter choice.

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The paper

Abstract

We study the onset of symmetry breaking after hybrid inflation in a model having the field content of the SU(2) gauge-scalar sector of the standard model, coupled to a singlet inflaton. This process is studied in (3+1)-dimensions in a fully non-perturbative way with the help of lattice techniques within the classical approximation. We focus on the role played by gauge fields and, in particular, on the generation of Chern-Simons number. Our results are shown to be insensitive to the various cut-offs introduced in our numerical approach. The spectra preserves a large hierarchy between long and short-wavelength modes during the whole period of symmetry breaking and Chern-Simons generation, confirming that the dynamics is driven by the low momentum sector of the theory. We establish that the Chern-Simons production mechanism is associated with local sphaleron-like structures. The corresponding sphaleron rates are of order 10^-5 m^4, which, within certain scenarios of electroweak baryogenesis and a (not unnaturally large) additional source of CP violation, could explain the present baryon asymmetry of the universe.

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 0.96

“The corresponding sphaleron rates are of order 10^{-5} m^4, which, within certain scenarios of electroweak baryogenesis and a (not unnaturally large) additional source of CP violation, could explain the present baryon asymmetry of the universe.”

How the main claim is stated: hedged possibility 0.98

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.48 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.98 · compares with prior results 0.08 · mentions code or data availability 0.02

The abstract, sentence by sentence

This table labels the abstract only (arXiv listing abstract v2). The number is the probability the classifier gave the label.

SentenceRoleThe authors' own workStates the main conclusionStrength
We study the onset of symmetry breaking after hybrid inflation in a model having the field content of the SU(2) gauge-scalar sector of the standard model, coupled to a singlet inflaton. contribution 0.89 0.55 0.03 asserted 0.81
This process is studied in (3+1)-dimensions in a fully non-perturbative way with the help of lattice techniques within the classical approximation. method 1.00 0.88 0.03 asserted 0.99
We focus on the role played by gauge fields and, in particular, on the generation of Chern-Simons number. contribution 0.97 0.46 0.07 asserted 0.59
Our results are shown to be insensitive to the various cut-offs introduced in our numerical approach. result 0.88 0.94 0.04 asserted 1.00
The spectra preserves a large hierarchy between long and short-wavelength modes during the whole period of symmetry breaking and Chern-Simons generation, confirming that the dynamics is driven by the low momentum sector of the theory. result 0.88 0.94 0.13 asserted 1.00
We establish that the Chern-Simons production mechanism is associated with local sphaleron-like structures. result 0.89 0.93 0.28 asserted 1.00
The corresponding sphaleron rates are of order 10^{-5} m^4, which, within certain scenarios of electroweak baryogenesis and a (not unnaturally large) additional source of CP violation, could explain the present baryon asymmetry of the universe. interpretation 0.91 0.85 0.61 hedged possibility 0.98

What kind of paper the classifier reports this is: simulation study 1.00 · evidence from simulation or computation 1.00

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Figures (15)
Figure 1 of the paper
Figure 1. FIG. 1: Left: The time evolution of the spatial averages of th
Figure 2 of the paper
Figure 2. FIG. 2: The time evolution of the energy fractions for a singl
Figure 3 of the paper
Figure 3. FIG. 3: Left: The UV cutoff dependence of the normalized
Figure 4 of the paper
Figure 4. FIG. 4: The time evolution of
Figure 5 of the paper
Figure 5. FIG. 5: Dependence on the UV cutoff of the Fourier spectra of th
Figure 6 of the paper
Figure 6. FIG. 6: Dependence on the UV cutoff of the Fourier spectra of th
Figure 7 of the paper
Figure 7. FIG. 7: The time evolution of
Figure 8 of the paper
Figure 8. FIG. 8: Combined histogram of values of ∆
Figure 9 of the paper
Figure 9. FIG. 9: The time evolution of
Figure 10 of the paper
Figure 10. FIG. 10: Snapshots of
Figure 11 of the paper
Figure 11. FIG. 11: Left: The spatial profile of the charge density peak fo
Figure 12 of the paper
Figure 12. FIG. 12: Histograms of minimal distance to a peak of the charg
Figure 13 of the paper
Figure 13. FIG. 13: Contour plots of
Figure 14 of the paper
Figure 14. FIG. 14: Contour plots of
Figure 15 of the paper
Figure 15. FIG. 15: Left: Time evolution of the normalized spatial aver

Figures are the authors', reproduced from the paper.

References (54)
  1. [43] J. Ambjørn, T. Askgaard, H. Porter, and M.E. Shaposhnik ov, Phys. Lett. B 244, 479 (1990); Nucl. Phys. B353, 346 (1991) on Pith
  2. [45] G. D. Moore, Nucl. Phys. B (Proc. Suppl.) 83, 131 (2000); “Do we understand the sphaleron rate?,” in ‘Mar seille 2000, Strong and Electroweak Matter’, World Scientific, Singapor e 2001, pp. 82-94, hep-ph/0009161; D. Bodeker, Nucl. Phys. B (Proc. Suppl.) 94, 61 (2001), and refer... on PithPith's reviewarXiv
  3. [9] L. Kofman, A. Linde and A. A. Starobinsky, Phys. Rev. Lett . 76, 1011 (1996); I.I. Tkachev, Phys. Lett. B 376, 35 (1996) on Pith
  4. [1] Initial conditions for classical evolution In this Subsection we specify in greater detail the initial conditions f or the evolution of the classical system. For the Higgs and inflaton fields they are fixed in the same fashion as in paper I , which is summarized in what follows. ... on Pith
  5. [2] A. D. Sakharov, JETP Lett. 6, 24 (1967) on Pith
  6. [3] For a review, see V. A. Rubakov and M. E. Shaposhnikov, Phy s. Usp. 39, 461 (1996) on Pith
  7. [4] V.A. Kuzmin, V.A. Rubakov, and M.E. Shaposhnikov, Phys. Lett. B155, 36 (1985) on Pith
  8. [5] K. Rummukainen, M. Tsypin, K. Kajantie, M. Laine and M. E. Shaposhnikov, Nucl. Phys. B532, 283 (1998) on Pith
  9. [6] Particle Data Group, http://pdg.web.cern.ch on Pith
  10. [7] An alternative proposal is that of leptogenesis [M. Fuku gita and T. Yanagida, Phys. Lett. B 174, 45 (1986)], which may have occurred via a lepton asymmetry at much higher energies that was later converted into a baryon asymmetry through nonperturbative sphaleron processes abo... on Pith
  11. [8] L. Kofman, A. Linde and A. A. Starobinsky, Phys. Rev. Lett . 73, 3195 (1994); Phys. Rev. D 56, 3258 (1997) on Pith
  12. [10] J. Garc ´ ıa-Bellido, D. Grigoriev, A. Kusenko and M. Shap oshnikov, Phys. Rev. D 60, 123504 (1999) on Pith
  13. [11] L. M. Krauss and M. Trodden, Phys. Rev. Lett. 83, 1502 (1999) on Pith
  14. [12] J. Garc ´ ıa-Bellido and D. Grigoriev, J. High Energy Phy s. 01, 017 (2000) on Pith
  15. [13] D. Grigoriev, “Electroweak Baryogenesis at and after P reheating: What’s the difference?”, in the proceedings of th e 35th Rencontres de Moriond: Electroweak Interactions and U nified Theories, E-print archive: hep-ph/0006115 (2000). J . Garc ´ ıa-Bellido, “Electroweak Baryogene... on PithPith's reviewarXiv
  16. [14] J. M. Cornwall and A. Kusenko, Phys. Rev. D 61, 103510 (2000); J. M. Cornwall, D. Grigoriev and A. Kusenko, Phys. Rev. D 64, 123518 (2001) on Pith
  17. [15] J. Garc ´ ıa-Bellido, “Particle Production and Symmetr y Breaking after Hybrid Inflation”, Plenary talk at COSMO-01 , International Workshop on Particle Physics and the Early Un iverse, 2001, Rovaniemi, Finland. For a transcript of the ta lk see http://www.physics.helsinki.fi/c... on Pith
  18. [16] D. Lyth, Phys. Lett. B 466, 85 (1999) on Pith
  19. [17] N. Arkani-Hamed, H. C. Cheng, P. Creminelli and L. Randa ll, “Extranatural inflation,” Phys. Rev. Lett. 90, 221302 (2003); “Pseudonatural inflation,” hep-th/0302034; D. E. K aplan and N. J. Weiner, “Little Inflatons and Gauge Inflation, ” hep-ph/0302014 on PithPith's reviewarXiv
  20. [18] G. Felder, J. Garc ´ ıa-Bellido, P. Greene, L. Kofman, A. D. Linde, and I. Tkachev, Phys. Rev. Lett. 87, 011601 (2001); G. Felder, L. Kofman and A. D. Linde, Phys. Rev. D 64, 123517 (2001) on Pith
show 34 more
  1. [19] S. Yu. Khlebnikov, and I. I. Tkachev, Phys. Rev. Lett. 77, 219 (1996); 79, 1607 (1997) on Pith
  2. [20] D. Yu. Grigoriev, V. A. Rubakov, and M. E. Shaposhnikov, Phys. Lett. B 216, 172 (1989); Nucl. Phys. B326, 737 (1989) on Pith
  3. [21] D.Yu. Grigoriev, M.E. Shaposhnikov, and N.G. Turok, Ph ys. Lett. B 275, 395 (1992) on Pith
  4. [22] E. J. Copeland, S. Pascoli and A. Rajantie, Phys. Rev. D 65, 103517 (2002) on Pith
  5. [23] J. Smit and A. Tranberg, J. High Energy Phys. 12, 020 (2002) on Pith
  6. [24] J. Smit and A. Tranberg, “Chern-Simons number asymmetr y from CP violation during Tachyonic Preheating”, hep-ph/0210348 on PithPith's reviewarXiv
  7. [25] J. Garc ´ ıa-Bellido and E. Ruiz Morales, Phys. Lett. B 536, 193 (2002) on Pith
  8. [26] T. Asaka, W. Buchmuller, and L. Covi, Phys. Lett. B 510, 271 (2001) on Pith
  9. [27] J. Garc ´ ıa-Bellido, M. Garc ´ ıa P´ erez, and A. Gonz´ alez-Arroyo, Phys. Rev. D 67, 103501 (2003) on Pith
  10. [28] A. Rajantie, P. M. Saffin, and E. J. Copeland, Phys. Rev. D 63, 123512 (2001); E. J. Copeland, D. Lyth, A. Rajantie, and 28 M. Trodden, ibid. 64, 043506 (2001) on Pith
  11. [29] J. Skullerud, J. Smit, and A. Tranberg, ‘W-particle dis tribution in electroweak tachyonic preheating”, hep-ph/0 210349 on Pith
  12. [30] A.D. Linde, Phys. Lett. B 259, 38 (1991); Phys. Rev. D 49, 748 (1994) on Pith
  13. [31] J. Garc ´ ıa-Bellido and A. D. Linde, Phys. Rev. D 57, 6075 (1998) on Pith
  14. [32] J. Garc ´ ıa-Bellido, A. D. Linde, and D. Wands, Phys. Rev . D 54, 6040 (1996) on Pith
  15. [33] M. Bastero-Gil, S. F. King, and J. Sanderson, Phys. Rev. D 60, 103517 (1999) on Pith
  16. [34] G. R. Dvali, Q. Shafi, and R. Schaefer, Phys. Rev. Lett. 73, 1886 (1994) on Pith
  17. [35] K. Wilson, Phys. Rev D 10, 2445 (1974) on Pith
  18. [36] F. Cooper, S. Habib, Y. Kluger, and E. Mottola, Phys. Rev . D 55, 6471 (1997); F. Cooper, S. Habib, Y. Kluger, E. Mottola, J. P. Paz, and P. R. Anderson, Phys. Rev. D 50, 2848 (1994) on Pith
  19. [37] D. Boyanovsky and H. J. de Vega, “Dynamics of Symmetry Br eaking Out of Equilibrium: From Condensed Matter to QCD and the Early Universe,” hep-ph/9909372; Phys. Rev. D 61, 105014 (2000); D. Boyanovsky, D. Cormier, H. J. de Vega, R. Holman, A. Singh, and M. Srednicki, ibid. 56,... on PithPith's reviewarXiv
  20. [38] J. Baacke, K. Heitmann and C. Patzold, Phys. Rev. D 55, 2320 (1997); 55, 7815 (1997); 56, 6556 (1997); J. Baacke and S. Michalski, ibid. 65, 065019 (2002) on Pith
  21. [39] D. Polarski and A. A. Starobinsky, Class. Quantum Grav. 13, 377 (1996); C. Kiefer, D. Polarski, and A. A. Starobinsky, Int. J. Mod. Phys. D 7, 455 (1998) on Pith
  22. [40] T. Prokopec and T. G. Roos, Phys. Rev. D 55, 3768 (1997) on Pith
  23. [41] G. Felder and I.I Tkachev, “LATTICEEASY: A program for l attice simulations of scalar fields in an expanding Universe ”, hep-ph/0011159 on PithPith's reviewarXiv
  24. [42] J. Smit, J. C. Vink and M. Salle, “Initial conditions for simulated Tachyonic Preheating and the Hartree ensemble ap prox- imation”, hep-ph/0112057; Nucl. Phys. B (Proc. Suppl.) 106, 540 (2002) on PithPith's reviewarXiv
  25. [44] G. D. Moore, J. High Energy Phys. 11, 021 (2001) on Pith
  26. [46] M. Garc ´ ıa P´ erez and P. van Baal, Nucl. Phys.B468, 277 (1996) on Pith
  27. [47] N. Manton, Phys. Rev. D 28, 2019 (1983); F. Klinkhamer and N. Manton, Phys. Rev. D 30, 2212 (1984) on Pith
  28. [48] In these points the inflaton takes values around χc. These points are referred to as hot spots in Ref. [21] on Pith
  29. [49] G. ’t Hooft, Phys. Rev. Lett. 37, 8 (1976) on Pith
  30. [50] P. Arnold, L. McLerran, Phys. Rev. D 36, 581 (1987) on Pith
  31. [51] S. Yu. Khlebnikov, M. E. Shaposhnikov, Nucl. Phys. B308, 885 (1988) on Pith
  32. [52] M. E. Shaposhnikov, Nucl. Phys. B299, 797 (1988) on Pith
  33. [53] G. Felder and L. Kofman, Phys. Rev. D 63, 103503 (2001) on Pith
  34. [54] F. R. Klinkhamer and Y. J. Lee, Phys. Rev. D64, 065024 (20 01); F. R. Klinkhamer, “Electroweak baryon number vi- olation”, in Proceedings of 14th Rencontres de Blois: Matte r-Antimatter Asymmetry, Chateau de Blois, France, 2002, hep-ph/0209227 on PithPith's reviewarXiv
Cited by 22 Pith papers

Reviewed papers on Pith that cite this one. The full citation record

  1. DEFROST: A New Code for Simulating Preheating after Inflation hep-ph · Sep 2008
  2. Primordial magnetic fields from preheating at the electroweak scale hep-ph · May 2008
  3. CosmoLattice 2.0 astro-ph.CO · Jul 2026
  4. Potential Surge Preheating: enhanced resonance from potential features astro-ph.CO · Dec 2024
  5. Nonlinear Dynamics of Preheating after Multifield Inflation with Nonminimal Couplings hep-ph · May 2019
  6. Preheating after multifield inflation with nonminimal couplings, II: Resonance Structure astro-ph.CO · Oct 2016
  7. The Standard Model Higgs as the origin of the hot Big Bang hep-ph · Apr 2016
  8. The charged inflaton and its gauge fields: preheating and initial conditions for reheating hep-ph · Mar 2016
  9. Gauge-preheating and the end of axion inflation astro-ph.CO · Feb 2015
  10. Baryogenesis from Strong CP Violation and the QCD Axion hep-ph · Jun 2014
  11. Natural Cold Baryogenesis from Strongly Interacting Electroweak Symmetry Breaking hep-ph · Apr 2011
  12. Gravitational Waves from Abelian Gauge Fields and Cosmic Strings at Preheating astro-ph.CO · Jun 2010
  13. Gravitational signature of Schwarzschild black holes in dynamical Chern-Simons gravity gr-qc · Apr 2010
  14. Perturbations of Schwarzschild black holes in Dynamical Chern-Simons modified gravity gr-qc · Jul 2009
  15. Preheating with Trilinear Interactions: Tachyonic Resonance hep-ph · Feb 2006
  16. Baryon asymmetry from electroweak tachyonic preheating hep-ph · Oct 2003
  17. The art of simulating the early Universe. Part III: Scalar-Gauge-Fluid Dynamics astro-ph.CO · Jul 2026
  18. Parametric Resonance in the Early Universe - A Fitting Analysis astro-ph.CO · Sep 2016
  19. Particle physics models of inflation and curvaton scenarios hep-ph · Jan 2010
  20. The First Three Seconds: a Review of Possible Expansion Histories of the Early Universe astro-ph.CO · Jun 2020
  21. Nonperturbative Dynamics Of Reheating After Inflation: A Review hep-ph · Oct 2014
  22. The origin of the matter-antimatter asymmetry hep-ph · Mar 2003

Topics: Matter-Antimatter Asymmetry

How later papers used it

56 later papers cite it

Evidence: some. 51 of the citing papers share no author with it, and 5 of those carry a confident label from Pith's citation classifier.

Pith read 8 of the 101 citing sentences, choosing only those whose citation markers point at this paper alone, and wrote the paraphrases from them. The summary, the counts, the evidence level, the links and the quotes come from code; the summary counts the papers listed below. A later paper is listed under a label when Pith's citation classifier gives one of its sentences that label at probability 0.8 or more (0.95 for support), Pith's reading finds that the citing paper itself did it, and a second check confirms the paraphrase against the sentence. This section lists uses only. It does not list criticism or disagreement, so their absence here says nothing about how the paper has been received. Papers that share an author with this one are listed apart, under "By the same authors". A quote is the citing authors' own sentence, shown when their paper's licence is CC BY, CC BY-SA or CC0. JSON

Uses its method or tool 1 of 5 papers with this label
  • Introduced a Lagrange multiplier term from this paper into its theory to enforce the unitarity constraint.

    Non-Abelian gauge preheating (2017) · 0.97 · paraphrased: the licence does not allow quoting

Uses its data or values 1 paper
How the literature uses it

41 arXiv papers cite this in 83 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

Papers citing it · 48 sentences without a confident label

Uses its method or tool 5 papers
Uses its data or values 1 paper
Compares with it 2 papers
Cites it as background 18 papers
  • We summarize here briefly the main features of cold baryogenesis and refer the reader to the specific literature for more details [ref] .

    Baryogenesis from Strong CP Violation and the QCD Axion · The Higgs quench from a Higgs-scalar coupling · 0.98

  • In this case, not the temperature dependence of the free energy but the inflation field turns the effective squared Higgs mass parameter negative [ref] .

    Cold electroweak baryogenesis with Standard Model CP violation · Introduction · 0.85

  • Other mechanisms considered include particle creation due to trilinear or higher-order interactions between the inflaton and daughter field(s) [ref] , geometric preheating of fields non-minimally coupled to gravity [ref] , tachyonic preheating after Hybrid inflation of Higgs-like fields [ref] and gauge fields [ref] ), gauge field excitation due to shift-symmetric interactions with an axion-like inflaton [ref] , etc.

    Gravitational wave production from preheating with trilinear interactions · Introduction · 0.98

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