Pith.

High Energy Physics - Phenomenology · arXiv:hep-ph/0310342 v1 · submitted 30 Oct 2003 · 48 references

Baryon asymmetry from electroweak tachyonic preheating

Anders Tranberg, Jan Smit

The paper says

“We consider a scenario in which the baryon asymmetry was created in the early universe during a cold electroweak transition.”

more of the abstract

The spinodal instability of the Higgs field caused by a rapid change of sign of its effective mass-squared parameter induces tachyonic preheating. We study the development of Chern-Simons number in this transition by numerical lattice simulations of the SU(2)-Higgs model with an added effective CP-violating term. A net asymmetry is produced, and we study its dependence on the size of CP violation and the ratio of Higgs to W mass.

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. First 3+1D lattice measurement of the Chern-Simons response to CP violation in tachyonic preheating; the qualitative result holds, the δ_CP number is an order-of-magnitude estimate the authors themselves flag as statistically unsettled. This line is wrong

4 major objections · 9 minor

How often objections from reviews like this one are right: not yet measured

Are you an author? What you can do.

Not checked: figures, code, what the 48 references say.

The paper says, at §5.3, eqs. (5.6)–(5.9); §6, eq. (6.4)

The review did not quote this passage.

Pith says: Objection 1 of 4 · major

The slope that sets the headline number is not stably determined by the data presented. For m_H = m_W, a fit through the origin gives (0.32 ± 0.15)×10⁻⁵ k with χ²/d.o.f. = 2.4 (eq. 5.6), while a fit through the two lowest-k points gives (0.79 ± 0.31)×10⁻⁵ k (eq. 5.8), a factor 2.5 apart; for m_H = √2 m_W the analogous numbers are (0.79 ± 0.36)×10⁻⁵ k (eq. 5.7) and ≃1.4×10⁻⁵ k with no error quoted (eq. 5.9).

more of objection 1

The final estimate δ_CP ≃ 0.7×10⁻⁵ (eq. 6.4) is derived from eq. (5.7) without propagating this ambiguity. The authors acknowledge that they 'lack sufficient statistics to draw a conclusion' about where the linear regime ends, but the abstract and conclusion still present a single number. Either a proper uncertainty should be propagated into eq. (6.4) and eqs. (6.1)–(6.2), or the headline should be stated as an order-of-magnitude range.

The paper says, at §6, eq. (6.4) compared with eq. (1.4)

The review did not quote this passage.

Pith says: Objection 2 of 4 · major

The concluding 'encouragement' rests on the statement that δ_CP ≃ 0.7×10⁻⁵ is 'smaller than the Standard Model J ≃ 3×10⁻⁵'. These are not the same kind of object: δ_CP is the dimensionless coefficient of a dimension-six operator normalized by M = m_W (eq. 1.6), whereas J is a rephasing-invariant product of CKM elements.

more of objection 2

The comparison is therefore not automatically meaningful, and the paper does not justify why the two should be compared on equal footing. Since this comparison is the main physics takeaway of the conclusion, it needs either a supporting argument or a clear statement that it is only a heuristic order-of-magnitude juxtaposition.

The paper says, at §5.5

The review did not quote this passage.

Pith says: Objection 3 of 4 · major

The conclusion that sphaleron wash-out is avoided is not demonstrated within the simulation. The argument combines an equilibrium temperature estimate (eq. 5.21), effective temperatures and chemical potentials taken from the companion paper [34] (eq. 5.22), and an assertion that W and Higgs decays will rapidly cool the plasma.

more of objection 3

The authors themselves note that the large chemical potential implies the low-momentum occupation numbers are large and 'the actual rate may be larger than one would expect from the temperature alone'. Fig. 9 shows Γ_eff is still not small at the end of the run. The manuscript should state explicitly the time interval over which wash-out must be absent for the asymmetry to survive, and whether the simulated window (m_H t = 100) covers it; as written, the no-wash-out claim is an extrapolation beyond the data.

The paper says, at §5.2, Figs. 3–4

The review did not quote this passage.

Pith says: Objection 4 of 4 · major

The ensemble averages are formed from Chern-Simons numbers at m_H t = 100, but the text states that for some configurations N_CS settles only as late as m_H t = 500. Since the asymmetry is extracted from a small difference of order 10⁻⁵ in the distribution of integer shifts, an unrelaxed tail could bias the mean.

more of objection 4

The paper should quantify how many configurations are unsettled at the measurement time and estimate the resulting systematic error on ⟨N_CS⟩, or show that the ensemble average is stable against extending the run.

9 minor objections

The paper says, at §5.3

Pith says: minor objection 1 of 9

There is a typographical error in the sentence 'For the case m_H = √2 m_H this would lead to a too large, not meaningful error'; the second m_H should presumably be m_W.

The paper says, at §5.3, eq. (5.9)

Pith says: minor objection 2 of 9

Eq. (5.9) is quoted without an uncertainty while eq. (5.8) has one; the reader cannot judge the weight of the m_H = √2 m_W result. A quoted error, even if large, would be preferable to none.

show 7 more

The paper says, at §5.3, Fig. 7

Pith says: minor objection 3 of 9

The k = 16 point is excluded from the fits without an explicit justification beyond a parenthetical remark; the criterion for exclusion should be stated.

The paper says, at §5.4, eq. (5.20)

Pith says: minor objection 4 of 9

The growth rate c is introduced via A^a_{k,0} = C^a_k e^{cμt} and then inferred from ⟨B²⟩ ∝ exp(4cμt); the factor of 4 and the definition of c relative to μ should be spelled out so the reader can reproduce the quoted c ≃ 0.67.

The paper says, at §6, eqs. (6.1)–(6.2)

Pith says: minor objection 5 of 9

The conversion from the slopes in eqs. (5.7)–(5.8) to the coefficients 0.79×10⁻² and 0.46×10⁻² in eqs. (6.1)–(6.2) is not shown; a short intermediate step would make the estimate reproducible.

The paper says, at §5.6

Pith says: minor objection 6 of 9

The statement that Γ_eff/m_H⁴ ≈ 0.35×10⁻⁵ is 'about the same value as obtained in [16]' should be qualified, since [16] used different parameters and a different quenching procedure.

The paper says, at §6

Pith says: minor objection 7 of 9

The claim that the quoted values are 'upper limits' on the generated asymmetry is asserted rather than argued; the individual approximations (instantaneous quench, zero initial temperature, omitted damping) should each be connected to the direction of the resulting bias.

The paper says, at Whole manuscript

Pith says: minor objection 8 of 9

There are numerous spacing artifacts in the typeset text (for example 'Amsterda m', 'crea ted', 'sp inodal', 'T achyonic', 'sufficently', 'Higss', 'a mply', 'b aryon', 'ther e', 'e stimate', 's imulation', 'p resumably', 'fo r', 'd ifferent', 'w ith', 'o f', 'i n'). A careful typographical pass is needed before publication.

The paper says, at §5.3, Fig. 7

Pith says: minor objection 9 of 9

The label 'Just the half' in the figure legend is inconsistent with 'Just-the-half' used in the text and section heading; the naming should be made uniform.

What would settle it

Re-run the m_H = √2 m_W ensemble with 500-1000 configurations (instead of 45) at k = 0, 1.5, 3, and recompute the slope with paired-difference errors (same initial conditions for each k). If the slope moves outside the quoted [0.43, 1.15]×10^-5 band, or if the k = 5, 8, 10 points deviate from linearity by more than the new error, the δ_CP estimate is not robust. A cheaper check: extend to k = 0.5, 1 and verify the slope is stable as k → 0.

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 high
  2. Skeptic partly agrees 2 min 35 s · 23,945 tokens read, 9,013 written
  3. Editor wrote the verdict above 16 s · 25,065 tokens read, 891 written
  4. Referee major revision: 4 major objections, 9 minor 1 min 14 s · 24,351 tokens read, 4,423 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

The thing worth knowing: this is the first 3+1D lattice simulation of CP violation during a tachyonic electroweak transition, and it does produce a net Chern-Simons asymmetry that grows with the CP-violating parameter k. The authors' earlier work was 1+1D, and the one prior 3+1D attempt found nothing. So the qualitative claim — a cold quench with an effective CP term generates an asymmetry proportional to k — is a real, new, simulation-backed result. That part I believe. The initial-rise analytic estimate in section 5.4 (eq. 5.20) agreeing with the measured bump is a genuinely nice cross-check, and the lattice machinery in the appendices — the symmetrized F F-tilde, the implicit solver, the Gauss-constraint sampling — is careful work. The paper is also honest about its limits in a way that is unusual and welcome: it says outright that it lacks statistics to pin the linear regime and that the effective operator is a crude placeholder for (E)SM fermion CP violation. The wash-out discussion flags the large chemical potentials from their prior work as a possible enhancement rather than waving it away. Credit for all of that. Where it gets soft is the headline number. The stress-test concern lands: for mH = mW the two fits give (0.32 ± 0.15) and (0.79 ± 0.31) × 10−5 k — a factor 2.5 apart, with χ²/d.o.f. = 2.4 on the through-origin fit — and the final δ_CP ≈ 0.7 × 10−5 uses eq. 5.7, whose error is not independently verified. With 45 configurations per point and the asymmetry living in integer-shift probabilities, the quoted errors probably understate the discreteness. The authors say as much. So the

The strongest objection

The central quantitative claim is the slope of ⟨N_CS⟩/(L m_W)^3 vs k, which sets δ_CP ≈ 0.7×10^-5 (eq. 6.4). The paper's own numbers show this slope is not stably determined. For m_H = m_W, a fit through the origin gives (0.32 ± 0.15)×10^-5 k (eq. 5.6, χ²/d.o.f = 2.4), while a fit through the two lowest-k points gives (0.79 ± 0.31)×10^-5 k (eq. 5.8) — a factor 2.5 apart. For m_H = √2 m_W, the analogous numbers are (0.79 ± 0.36)×10^-5 k (eq. 5.7) and ≃1.4×10^-5 k (eq. 5.9, no error quoted). The final extrapolation (eq. 6.2) uses eq. 5.7, whose ±0.36 is not independently verified. The ensembles are 45 configurations (300 only for two k=0/3 thermal cases), and the asymmetry is a difference in the fraction of trajectories that shift by an integer N_CS (Fig. 2 shows a full ±1 shift for a single trajectory). With 45 samples, the statistical error on a probability difference of order 10^-5 is large, and the quoted errors may not capture the discreteness of the shift events. The authors acknowledge 'We lack sufficient statistics to draw a conclusion' and 'it is unclear where it ends' (the linear regime), so the qualitative claim (asymmetry ∝ k) stands, but the quantitative 'below J' claim does not.

The reader's CONDITIONAL verdict is appropriate and I would not change it. I agree with the general thrust: the qualitative result (a net asymmetry proportional to k) is well supported, and the quantitative extrapolation is an order-of-magnitude estimate. I disagree partially with the reader's identification of the weakest assumption. The reader points to the effective operator κφ†φ Tr[F F̃] as a proxy for SM CP violation (eqs. 1.5-1.6). That is a real modeling choice, but the authors explicitly acknowledge it ('crude representation,' 'approximate nature of the model'), so it is not a new finding. The more actionable soft spot is the statistical robustness of the slope, which the authors also partly acknowledge but which directly determines the headline δ_CP number. Two fitting methods on the same data give slopes differing by a factor of 2.5 (eqs. 5.6 vs 5.8), and the final extrapolation uses a slope whose error is not independently verified. I also note a factual slip in the reader's rationale: the reader says 'the best-estimate slope is taken from the fit with the worse chi-squared,' but eq. 5.7 (the best estimate) has χ²/d.o.f = 0.25, the better fit; eq. 5.6 has the worse χ²/d.o.f = 2.4. Separately, eq. 6.3 quotes κ ≃ 2.2×10^-51 TeV², which is dimensionally impossible (κ has mass dimension -2); it should read ≈2.2×10^-5 TeV^-2. This is almost certainly a typo and does not affect the dimensionless δ_CP = 0.7×10^-5, but it is an error in the final result and should be corrected. None of these points changes the verdict; they sharpen the rationale for CONDITIONAL.

The referee's report

This is, to my knowledge, the first 3+1 dimensional lattice study of CP-violation-induced Chern-Simons production in a tachyonic electroweak transition, extending the authors' earlier 1+1 dimensional work and complementing their particle-number study of the same scenario. The lattice formulation is careful: the implicit equations of motion are iterated to double precision, the Gauss constraints are imposed on the initial Higgs and gauge fields with an explicit construction (Appendix B), and the Chern-Simons and winding numbers are implemented with a symmetrized plaquette. The analytic estimate of the initial rise (eq. 5.20) matching the simulated bump is a genuine and non-trivial check. The paper is also candid about its statistical limitations. The result is a parameter-free-in-form prediction of the sign and rough magnitude of the asymmetry, and it yields a falsifiable statement about the size of δ_CP required for the observed baryon asymmetry.

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

The paper asks whether the universe's baryon asymmetry could have been made during a cold, non-thermal electroweak transition rather than a hot first-order phase transition. The setup is a quench: the Higgs effective mass-squared flips sign suddenly, its low-momentum modes grow exponentially (tachyonic preheating), and the resulting rolling and rescattering of the gauge fields can change Chern-Simons number, which the electroweak anomaly converts into baryon number. The authors add a CP-violating term of the form $kappaphi^daggerphi,mathrm{Tr}[F^{munu}tilde F_{munu}]$ to the SU(2)-Higgs model and follow the Chern-Simons number in 3+1 dimensional lattice simulations over an ensemble of classical initial conditions. The payoff, if the modelling holds, is a numerical conversion factor between the CP-violation strength and the final asymmetry, which lets one ask how much CP violation is actually needed. Their answer is that the observed asymmetry could be reached with a CP-violating coefficient below the size the Standard Model is usually credited with, which is the reason the scenario is worth pursuing.

What carries the argument. The machinery is a classical lattice simulation of the SU(2)-Higgs model in 3+1 dimensions with an added CP-odd operator $kappaphi^daggerphi,mathrm{Tr}[F^{munu}tilde F_{munu}]$, which is inert whenever $phi^daggerphi$ is constant (it becomes a total derivative) and therefore acts only while the Higgs condensate is changing. The quench is modelled as an instantaneous flip of the sign of $mu^2_{rm eff}$, with initial conditions drawn from a Gaussian ensemble built from the free-field quantum two-point functions of the unstable modes, split into 'Just-the-half' and 'Thermal' variants, and with the Gauss constraints imposed globally by solving for the homogeneous momentum components. Because the CP term makes the equations of motion implicit, each timestep is solved by iteration. The observable is the change in Chern-Simons number, computed from the lattice $mathrm{Tr}[Ftilde F]$ density, and cross-checked against the Higgs winding number, which should track it once the gauge field is near pure-gauge.

Core claim. The central claim is that a tachyonic electroweak quench with an effective CP-violating operator produces a net Chern-Simons number whose ensemble average grows approximately linearly with the CP-violation parameter $k = 16pi^2kappa m_W^2$, at least for small $k$. Fitting the difference between runs at $k=0$ and small non-zero $k$ that started from identical initial configurations, the authors report $langle N_{CS}rangle/(Lm_W)^3 = (0.79 pm 0.31)times 10^{-5},k$ for $m_H = m_W$ and about $1.4times 10^{-5},k$ for $m_H = sqrt{2},m_W$ (eqs. 5.8, 5.9), with the second quoted as the preferred slope. Converting through the anomaly equation $B = 3langle N_{CS}rangle$ and an entropy density fixed by an estimated reheat temperature of about 43-74 GeV, they find that the observed $n_B/n_gamma approx 6.5times 10^{-10}$ requires $kappa approx 1.4times 10^{-7},m_W^{-2}$, i.e. $delta_{CP} approx 0.7times 10^{-5}$ if the mass scale in the operator is set to $m_W$. That number sits below the Standard-Model Jarlskog factor $J approx 3times 10^{-5}$, which is the paper's headline: at electroweak-scale CP violation the cold tachyonic route is not obviously out of reach. The authors also give an analytic estimate of the early-time rise, eq. (5.20), which reproduces the size of the initial bump in the data, and they argue that the post-transition effective temperature and the measured effective sphaleron rate leave no room for wash-out on the timescales simulated.

The premise it rests on. The load-bearing premise is that a single hand-added operator, $kappaphi^daggerphi,mathrm{Tr}[F^{munu}tilde F_{munu}]$ with its mass scale set to $m_W$, adequately represents the CP violation of the Standard-Model fermions; if it does not, the derived value of $delta_{CP}$ says nothing about whether the real Standard Model can do the job.

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

The observed baryon-to-photon ratio can be reproduced with an effective CP-violation coefficient $delta_{CP} approx 0.7times 10^{-5}$, roughly a factor of four below the Standard-Model Jarlskog invariant, so weak-scale CP violation need not be ruled out for this scenario on magnitude grounds alone.

The asymmetry scales approximately linearly in the CP-violation strength for small $k$, giving a definite conversion factor that any competing model of cold electroweak baryogenesis must reproduce or beat.

The final effective temperature after the quench, estimated at 43-74 GeV for a Higgs mass near 114 GeV, is low enough that equilibrium sphaleron processes should not erase the generated asymmetry.

The generated asymmetry depends on the Higgs-to-W mass ratio, with the $m_H = sqrt{2},m_W$ case giving a larger slope than $m_H = m_W$, so the scenario makes a (weak) statement about Higgs mass dependence.

The early-time rise of the Chern-Simons density can be predicted analytically from the homogeneous-field approximation and matches the simulation, which gives the mechanism a semi-quantitative explanation rather than a purely numerical one.

If the effective operator is a faithful stand-in for integrated-out fermions, the result suggests the usual lore that Standard-Model CP violation is far too weak for electroweak baryogenesis deserves re-examination at the level of operator coefficients rather than Jarlskog factors alone.

The linear-in-$k$ regime is established only for small $k$ and with limited statistics; a natural follow-up is a dedicated scan at $k lesssim 3$ with several hundred configurations to pin down where linearity ends and whether the apparent curvature is physical.

Because the CP-odd term is only active while $phi^daggerphi$ changes, a finite-rate quench (rather than the instantaneous limit used here) would likely reduce the asymmetry, so the quoted $delta_{CP}$ should be read as a lower bound on the CP violation required in any realistic realisation.

Extending the simulation to include the U(1) hypercharge and the top Yukawa would test whether the operator-based estimate survives when the fermionic sector that supposedly generates the operator is treated dynamically.

Check this review

Pith stored no record of this review's passes and took no fingerprint of it. Reviews made by code from 13 Nov 2026 on carry both.

How often reviews like this one are right

Reviews like this one: written by deepseek-v4.1-flash, where what was read was not recorded.

How often objections from reviews like this one are right: not yet measured

Every value above, in the review's public record (JSON)

Reviews by people

This review was written by a machine. No person has reviewed this paper on Pith yet. A scientist listed on Pith can review it for a fee, and their review is published here whatever it concludes.

Request a human review

How Pith checks papers · The full audit of this paper

The paper

Abstract

We consider a scenario in which the baryon asymmetry was created in the early universe during a cold electroweak transition. The spinodal instability of the Higgs field caused by a rapid change of sign of its effective mass-squared parameter induces tachyonic preheating. We study the development of Chern-Simons number in this transition by numerical lattice simulations of the SU(2)-Higgs model with an added effective CP-violating term. A net asymmetry is produced, and we study its dependence on the size of CP violation and the ratio of Higgs to W mass.

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 0.99

“A net asymmetry is produced, and we study its dependence on the size of CP violation and the ratio of Higgs to W mass.”

How the main claim is stated: asserted 1.00

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.07 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.06 · compares with prior results 0.05 · mentions code or data availability 0.02

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.

SentenceRoleThe authors' own workStates the main conclusionStrength
We consider a scenario in which the baryon asymmetry was created in the early universe during a cold electroweak transition. background 0.57 0.17 0.11 asserted 0.55
The spinodal instability of the Higgs field caused by a rapid change of sign of its effective mass-squared parameter induces tachyonic preheating. background 0.77 0.17 0.05 asserted 1.00
We study the development of Chern-Simons number in this transition by numerical lattice simulations of the SU(2)-Higgs model with an added effective CP-violating term. method 0.96 0.95 0.04 asserted 0.89
A net asymmetry is produced, and we study its dependence on the size of CP violation and the ratio of Higgs to W mass. result 0.87 0.94 0.65 asserted 1.00

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

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, 3,615 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 (9)
Figure 1 of the paper
Figure 1. Volume-averaged Higgs field 2φ†φ/v2 , Chern-Simons number and winding number, for a typical trajectory with Thermal initial conditions, mH/mW = 1, and no CP violation, k = 0. 0 20 40 60 80 100 mH t -1 0 1 2 k = 3 k = 0
Figure 2 of the paper
Figure 2. Example of NCS and Nw for two trajectories with the same initial conditions, without (k = 0) and with (k = 3) CP violation. Thermal initial conditions, mH/mW = 1. they settle near the same integer value (for Nw the difference with the integer is a finite￾lattice spacing effect). The winding number appears to settle first and then the Chern￾Simons number approaches it somewhat later. In
Figure 3 of the paper
Figure 3. The distribution of final NCS and Nw; Thermal initial conditions, mH/mW = 1, no CP violation (k = 0), 303 configurations. -4 -2 0 2 4 Ncs, Nw 0 0.5 1 1.5 2 Nw Ncs
Figure 4 of the paper
Figure 4. As in figure 3 with CP violation, k = 3
Figure 5 of the paper
Figure 5. Averaged observables: 2hφ†φi/v2 , hNCSi and hNwi versus time for mH/mW = 1, Just￾a-half initial conditions and k = 8. In
Figure 6 of the paper
Figure 6. Expectation values 2hφ†φi/v2 and hNCSi for different k; mH/mW = 1 and Thermal initial conditions. 0 5 10 15 20 k -0.0001 0 0.0001 <Ncs>/(Lm W ) 3 "Just the half", mH /mW =1 "Just the half", mH /mW =1.41 "Thermal", mH /mW =1
Figure 7 of the paper
Figure 7. Results for the Chern-Simons density all k, mH/mW and initial conditions. The full lines represent linear fits through the two points with lowest k: k = 0, 3 (mH = mW ) and k = 0, 1.5 (mH = √ 2 mW ). The dashed lines are linear fits through the origin, ignoring the data at k = 0, and also at k = 16 for the case mH = mW . (χ 2/d.o.f = 2.4), hNCSi (LmW ) 3 = (0.32 ± 0.15) × 10−5 k, mH = mW , (5.6) – 16 –
Figure 8 of the paper
Figure 8. The initial rise for various k’s. The inset shows the size of the bump versus k for the estimate (5.20) (line), the results of the simulations (dots) and results shifted by the negative of the value at zero k (see main text); mH/mW = √ 2. at which the curvature in the Higgs potential changes sign and the quadratic approximation (5.12) will be become more strongly affected by non-linearities. Because of finite statistics, there is an overall shift of the results that can be read off from the k = 0 simulation, which should give zero with an infinite number of initial configurations. In
Figure 9 of the paper
Figure 9. The effective sphaleron rate Γeff/m4 H; mH/mW = 1, k = 0, Thermal initial conditions. Inset: integrated rate R t 0 dt′ Γeff(t ′ )/m3 H. In the tachyonic transition such a diffusion regime is preceded by a period of preheating, where the gauge fields acquire energy and as a result a non-zero hN2 CSi. The early-time rate at which this happens does not have anything to do with the equilibrium sphaleron rate. Rather, it is determined by the time scale of the preheating mechanism. Note how this rate is initially in phase with the Higgs field, but it has a large magnitude for small and

Figures are the authors', reproduced from the paper.

References (48)
  1. [34] J.-I. Skullerud, J. Smit, and A. Tranberg, W and Higgs particle distributions during electroweak tachyonic preheating, JHEP 08 (2003) 045, [ hep-ph/0307094] on PithPith's reviewarXiv
  2. [1] D. N. Spergel et. al. , First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Determination of cosmological parameters , Astrophys. J. Suppl. 148 (2003) 175, [ astro-ph/0302209] on PithPith's reviewarXiv
  3. [2] A. D. Sakharov, Violation of CP invariance, C asymmetry, and baryon asymmet ry of the universe, Pisma Zh. Eksp. Teor. Fiz. 5 (1967) 32–35 on Pith
  4. [3] M. Dine and A. Kusenko, The origin of the matter-antimatter asymmetry , hep-ph/0303065 on PithPith's reviewarXiv
  5. [4] G. ’t Hooft, Symmetry breaking through Bell-Jackiw anomalies , Phys. Rev. Lett. 37 (1976) 8–11 on Pith
  6. [5] N. Cabibbo, Unitary symmetry and leptonic decays , Phys. Rev. Lett. 10 (1963) 531–532 on Pith
  7. [6] M. Kobayashi and T. Maskawa, CP violation in the renormalizable theory of weak interaction, Prog. Theor. Phys. 49 (1973) 652–657 on Pith
  8. [7] Particle Data Group Collaboration, K. Hagiwara et. al. , Review of particle physics , Phys. Rev. D66 (2002) 010001 on Pith
  9. [8] W. Buchmuller, P. Di Bari, and M. Plumacher, The neutrino mass window for baryogenesis , Nucl. Phys. B665 (2003) 445–468, [ hep-ph/0302092] on PithPith's reviewarXiv
  10. [9] V. A. Kuzmin, V. A. Rubakov, and M. E. Shaposhnikov, On the anomalous electroweak baryon number nonconservation in the early universe , Phys. Lett. B155 (1985) 36 on Pith
  11. [10] V. A. Rubakov and M. E. Shaposhnikov, Electroweak baryon number non-conservation in the early universe and in high-energy collisions , Usp. Fiz. Nauk 166 (1996) 493–537, [hep-ph/9603208] on PithPith's reviewarXiv
  12. [11] A. G. Cohen, D. B. Kaplan, and A. E. Nelson, Progress in electroweak baryogenesis, Ann. Rev. Nucl. Part. Sci. 43 (1993) 27–70, [ hep-ph/9302210] on PithPith's reviewarXiv
  13. [12] K. Kajantie, M. Laine, K. Rummukainen, and M. E. Shaposhnikov , The electroweak phase transition: A non-perturbative analysis , Nucl. Phys. B466 (1996) 189–258, [hep-lat/9510020] on PithPith's reviewarXiv
  14. [13] F. Csikor, Z. Fodor, and J. Heitger, Endpoint of the hot electroweak phase transition , Phys. Rev. Lett. 82 (1999) 21–24, [ hep-ph/9809291]. – 28 – on PithPith's reviewarXiv
  15. [14] M. Carena, M. Quiros, and C. E. M. Wagner, Opening the window for electroweak baryogenesis, Phys. Lett. B380 (1996) 81–91, [ hep-ph/9603420] on PithPith's reviewarXiv
  16. [15] M. Laine and K. Rummukainen, The MSSM electroweak phase transition on the lattice , Nucl. Phys. B535 (1998) 423–457, [ hep-lat/9804019] on PithPith's reviewarXiv
  17. [16] J. Garcia-Bellido, D. Y. Grigoriev, A. Kusenko, and M. E. Shapos hnikov, Non-equilibrium electroweak baryogenesis from preheating after inflation , Phys. Rev. D60 (1999) 123504, [hep-ph/9902449] on PithPith's reviewarXiv
  18. [17] L. M. Krauss and M. Trodden, Baryogenesis below the electroweak scale , Phys. Rev. Lett. 83 (1999) 1502–1505, [ hep-ph/9902420] on PithPith's reviewarXiv
  19. [18] E. J. Copeland, D. Lyth, A. Rajantie, and M. Trodden, Hybrid inflation and baryogenesis at the TeV scale , Phys. Rev. D64 (2001) 043506, [ hep-ph/0103231] on PithPith's reviewarXiv
  20. [19] A. Rajantie, P. M. Saffin, and E. J. Copeland, Electroweak preheating on a lattice , Phys. Rev. D63 (2001) 123512, [ hep-ph/0012097] on PithPith's reviewarXiv
show 28 more
  1. [20] E. J. Copeland, S. Pascoli, and A. Rajantie, Dynamics of tachyonic preheating after hybrid inflation, Phys. Rev. D65 (2002) 103517, [ hep-ph/0202031] on PithPith's reviewarXiv
  2. [21] J. Garcia-Bellido, M. Garcia Perez, and A. Gonzalez-Arroyo, Symmetry breaking and false vacuum decay after hybrid inflation , Phys. Rev. D67 (2003) 103501, [ hep-ph/0208228] on PithPith's reviewarXiv
  3. [22] J. Smit and A. Tranberg, Chern-Simons number asymmetry from CP violation at electro weak tachyonic preheating, JHEP 12 (2002) 020, [ hep-ph/0211243] on PithPith's reviewarXiv
  4. [23] J. Garc ´ ıa-Bellido, M. Garcia-Perez, and A. Gonzalez-Arroyo, Chern-Simons production during preheating in hybrid inflation models , hep-ph/0304285 on PithPith's reviewarXiv
  5. [24] C. Jarlskog, Commutator of the quark mass matrices in the standard electr oweak model and a measure of maximal CP violation , Phys. Rev. Lett. 55 (1985) 1039 on Pith
  6. [25] M. E. Shaposhnikov, Baryon asymmetry of the universe in standard electroweak th eory, Nucl. Phys. B287 (1987) 757–775 on Pith
  7. [26] M. E. Shaposhnikov, Structure of the high temperature gauge ground state and ele ctroweak production of the baryon asymmetry , Nucl. Phys. B299 (1988) 797 on Pith
  8. [27] G. R. Farrar and M. E. Shaposhnikov, Baryon asymmetry of the universe in the minimal Standard Model, Phys. Rev. Lett. 70 (1993) 2833–2836, [ hep-ph/9305274]. [Erratum-ibid.71:210,1993] on PithPith's reviewarXiv
  9. [28] G. R. Farrar and M. E. Shaposhnikov, Baryon asymmetry of the universe in the standard electroweak theory, Phys. Rev. D50 (1994) 774, [ hep-ph/9305275]. [Erratum-ibid.71:210,1993] on PithPith's reviewarXiv
  10. [29] G. R. Farrar and M. E. Shaposhnikov, Note added to ’Baryon asymmetry of the universe in the standard model’ , hep-ph/9406387 on PithPith's reviewarXiv
  11. [30] T. Konstandin, T. Prokopec, and M. G. Schmidt, Axial currents from CKM matrix CP violation and electroweak baryogenesis , hep-ph/0309291 on PithPith's reviewarXiv
  12. [31] J. Smit, “Tachyonic electroweak transition, CP violation and bar yogenesis.” Talk at Cosmo-03, Ambleside, UK on Pith
  13. [32] D. Bodeker, G. D. Moore, and K. Rummukainen, Chern-Simons number diffusion and hard thermal loops on the lattice , Phys. Rev. D61 (2000) 056003, [ hep-ph/9907545]. – 29 – on PithPith's reviewarXiv
  14. [33] G. D. Moore, Measuring the broken phase sphaleron rate nonperturbative ly, Phys. Rev. D59 (1999) 014503, [ hep-ph/9805264] on PithPith's reviewarXiv
  15. [35] J. Ambjorn, T. Askgaard, H. Porter, and M. E. Shaposhnikov , Sphaleron transitions and baryon asymmetry: A numerical real time analysis , Nucl. Phys. B353 (1991) 346–378 on Pith
  16. [36] D. Y. Grigoriev, M. E. Shaposhnikov, and N. Turok, Electroweak baryogenesis: A numerical study in (1+1)- dimensions , Phys. Lett. B275 (1992) 395–402 on Pith
  17. [37] J. Smit and A. Tranberg, Chern-Simons number asymmetry from CP-violation during tachyonic preheating, in Strong and Electroweak Matter 2002 – Proceedings of the SEWM2002 Meeting (M. G. Schmidt, ed.), (Singapore), World Scientific, 2002. http://arXiv.org/abs/hep-ph/0210348 on PithPith's reviewarXiv
  18. [38] J. Smit and A. Tranberg, Classical issues in electroweak baryogenesis , hep-lat/0309082 on PithPith's reviewarXiv
  19. [39] A. Tranberg, “Baryogenesys from CP violation at electroweak tachyonic preheating.” Talk at Cosmo-03, Ambleside, UK on Pith
  20. [40] E. W. Kolb and M. S. Turner, The Early Universe . Addison-Wesley, Reading, Massachusetts, 1990 on Pith
  21. [41] P. J. E. Peebles and A. Vilenkin, Quintessential inflation , Phys. Rev. D59 (1999) 063505, [astro-ph/9810509] on PithPith's reviewarXiv
  22. [42] G. German, G. Ross, and S. Sarkar, Low-scale inflation, Nucl. Phys. B608 (2001) 423–450, [hep-ph/0103243] on PithPith's reviewarXiv
  23. [43] A. Berera and R. O. Ramos, Absence of isentropic expansion in various inflation models , hep-ph/0308211 on PithPith's reviewarXiv
  24. [44] T. Asaka, W. Buchmuller, and L. Covi, False vacuum decay after inflation , Phys. Lett. B510 (2001) 271–276, [ hep-ph/0104037] on PithPith's reviewarXiv
  25. [45] G. N. Felder et. al. , Dynamics of symmetry breaking and tachyonic preheating , Phys. Rev. Lett. 87 (2001) 011601, [ hep-ph/0012142] on PithPith's reviewarXiv
  26. [46] J. Smit, J. C. Vink, and M. Salle, Initial conditions for simulated ’tachyonic preheating’ a nd the Hartree ensemble approximation , hep-ph/0112057. Contribution to Cosmo-01, Rovaniemi, Finland on PithPith's reviewarXiv
  27. [47] B.-J. Nauta and A. Arrizabalaga, Asymmetric Chern-Simons number diffusion from CP-violation, Nucl. Phys. B635 (2002) 255–285, [ hep-ph/0202115] on PithPith's reviewarXiv
  28. [48] B.-J. Nauta, On asymmetric Chern-Simons number diffusion , in Strong and Electroweak Matter 2002 – Proceedings of the SEWM2002 Meeting (M. G. Schmidt, ed.), (Singapore), World Scientific, 2002. http://arXiv.org/abs/hep-ph/0301150. – 30 – on PithPith's reviewarXiv
Cited by 16 Pith papers

Topics: Matter-Antimatter Asymmetry

How later papers used it

48 later papers cite it

Evidence: substantial. 33 of the citing papers share no author with it, and 7 of those carry a confident label from Pith's citation classifier.

Pith read 12 of the 80 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 3 of 8 papers with this label · 1 by the same authors

By the same authors

How the literature uses it

41 arXiv papers cite this in 68 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 · 36 sentences without a confident label

Builds on it 1 paper
Uses its method or tool 8 papers
Compares with it 4 papers
Cites it as background 18 papers
  • Cold Electroweak Baryogenesis is realized if the temperature is well below the electroweak scale when the electroweak transition happens [ref] (further developed in [ref] ).

    Standard Model CP-violation and Cold Electroweak Baryogenesis · Introduction · 0.89

  • The “cold” scenario was originally an attempt to bypass the lack of a strong equilibrium phase transition by invoking an out-of-equilibrium process such as preheating after inflation, and necessary CP-violation was introduced through a hypothetical higher order bosonic operator [ref] .

    Cold Electroweak Baryogenesis in the Two Higgs-Doublet Model · Introduction · 0.88

  • 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

Challenges and discussion

Disagree with the review, or know something it missed? Leave a comment, or challenge this review formally: a challenge becomes a permanent entry in this paper's record, and its decision is published here.

No comments yet.

Sign in to comment