REVIEW
Photon and Gluon Emission in Relativistic Plasmas
High Energy Physics - Phenomenology · Submitted 29 Apr 2002 · 43 references
Pith's verdict: The gluon half is the real contribution and it holds together, but the step from the two-variable equation (6.3) to the single-variable (6.6) is asserted in one sentence and never checked against anything.
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Referee report
The paper
The paper claims
The paper re-derives the LPM-suppressed photon emission rate in a hot plasma from a classical random background field, and extends the same ladder-resummation machinery to give a leading-order hard gluon emission rate.
The reading
What carries the argument
The load-bearing device is the relativistic one-particle Schrödinger equation for a nearly on-shell hard particle in a soft background field, $i∂_t ψ = E_p ψ$ with the interaction $i g v·A$ and $v = P/p_0$, which is spin-independent at leading order and so lets scalars, fermions and gauge bosons be handled by the same propagator. Combined with the pinching-pole approximation, which replaces the product of the two emitter propagators by $2πδ(p_0 - p_∥)θ(p_∥)/(iδE + Γ_{p+k} + Γ_p)$ with $δE = k(p_⊥^2+m_∞^2)/[2p_∥(k+p_∥)]$, the ladder sum becomes the integral equation of Eq. (3.34) for photons and Eq. (6.6b) for gluons. The second device is the rewriting of the thermal width $Γ_p$ in the same form as the collision term, Eq. (3.28), which turns the kernel into a difference $f(p_⊥) - f(p_⊥-q_⊥)$ and makes the equation manifestly infrared safe. The third is the color-singlet identity behind Eq. (6.9): because $T^a_{R1}+T^a_{R2}+T^a_{R3}$ annihilates the singlet, the gluon-exchange factor between any two rails is $½(C_{R3}-C_{R1}-C_{R2})$, which fixes the three coefficients without further diagrammatics.
Extended reading notes
Core claim
The paper's central claim is that the leading-order hard emission rate for both photons and gluons in an ultra-relativistic plasma can be reduced to a single linear integral equation in transverse momentum space, and that the gluon case is given by Eqs. (6.6a)–(6.6c): a rate formula containing the splitting weight $|J^{(s)}_{p_← p+k}|^2 k^{-3}$ and a three-rail integral equation whose collision kernel is built from the differences $F_s(h) - F_s(h - p_i q_⊥)$ weighted by $C_{R1}+C_{R2}-C_{R3}$-type color factors. The argument for the ladder structure is physical rather than diagrammatic: a wave packet of size $1/gT$ stays localized compared with the mean free path $1/g^2T$, so interactions with a given scatterer must appear consistently ordered on all rails, and only pairwise correlations of the background field survive the average. The authors state that this is the first treatment to give the full correct leading-order high-temperature gluon emission rate because it is the first to treat the scatterers' dynamics correctly, and they show that the photon result follows from the gluon equations by setting $C_A = 0$ and replacing $C_s$ with $q_s^2$.
Load-bearing premise
The random background color field is assumed to have only Gaussian two-point correlations, with higher connected correlations dropped, on the grounds that non-Gaussian and ultra-soft $g^2T$ physics do not affect the leading-order rate — a claim the paper asserts here and defers to its earlier work.
Editorial extensions
If this is right
- The gluon emission rate becomes a computable leading-order ingredient for transport coefficients and for thermalization and jet-quenching phenomenology in a quark-gluon plasma.
- The photon rate of the authors' earlier work is recovered as a limiting case, so the two derivations — diagrammatic and physical — agree by construction rather than by coincidence.
- Because the collision kernel depends on the full frequency- and wavenumber-dependent HTL spectral density $\langle\langle A_+ A_+^*\rangle\rangle$ rather than on a static scattering potential, the result differs quantitatively from static-impurity LPM treatments.
- The cancellation of the $q_⊥ \to 0$ divergence across all three rails shows that the hard emission rate is insensitive to non-perturbative ultra-soft magnetic physics at the $g^2T$ scale.
Reading between the lines
- If the three-rail equation is solved numerically, the resulting gluon rate should differ measurably from static-scatterer LPM formulas at the same coupling, which gives a concrete way to discriminate the two pictures in phenomenological fits.
- The same wave-packet localization argument should apply to any hard probe whose formation time matches the soft scattering time, which suggests the machinery transfers to e.g. heavy-quark energy loss once the emitter's spin-dependent vertices are restored.
- The infrared-safety argument rests on the difference structure of the kernel; a truncated version of the same ladder sum, with external color currents, would retain the divergence, so the cancellation is a diagnostic that a given approximation has kept the right set of diagrams.
Original abstract
We recently derived, using diagrammatic methods, the leading-order hard photon emission rate in ultra-relativistic plasmas. This requires a correct treatment of multiple scattering effects which limit the coherence length of emitted radiation (the Landau-Pomeranchuk-Migdal effect). In this paper, we provide a more physical derivation of this result, and extend the treatment to the case of gluon radiation.
The compiled record
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. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.
The abstract, sentence by sentence
We recently derived, using diagrammatic methods, the leading-order hard photon emission rate in ultra-relativistic plasmas. This requires a correct treatment of multiple scattering effects which limit the coherence length of emitted radiation (the Landau-Pomeranchuk-Migdal effect). In this paper, we provide a more physical derivation of this result, and extend the treatment to the case of gluon radiation.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We recently derived, using diagrammatic methods, the leading-order hard photon emission rate in ultra-relativistic plasmas. | background 0.77 | 0.88 | 0.10 | asserted 1.00 |
| s1 | This requires a correct treatment of multiple scattering effects which limit the coherence length of emitted radiation (the Landau-Pomeranchuk-Migdal effect). | background 0.98 | 0.17 | 0.05 | asserted 1.00 |
| s2 | In this paper, we provide a more physical derivation of this result, and extend the treatment to the case of gluon radiation. | contribution 1.00 | 0.94 | 0.49 | asserted 1.00 |
What was examined, and what was not
- arXiv listing abstract v2
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- P abstract
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Figures
Figures reproduced from arXiv:hep-ph/0204343 by the authors.
References
How later papers used it
230 later papers cite it
2 later papers by other authors are listed below: 2 used its method or tool.
Uses its method or tool 2 of 22 papers with this label
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Obtained emission rates for large-ω inelastic interactions from this paper's AMY integral equation.
Parton energy loss in the reformulated weakly-coupled kinetic approach (2019) · 0.89 · paraphrased: the licence does not allow quoting
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Implemented its own re-calculation of the LO rates from this paper together with those computations to quantify energy loss and evaluate consequences of different scattering kernels.
Leading order, next-to-leading order, and non-perturbative parton collision kernels: effects in static and evolving media (2022) · 0.84 · paraphrased: the licence does not allow quoting
How the literature uses it
223 arXiv papers cite this in 325 sentences
Papers citing it · 171 sentences without a confident label
Builds on it 2 papers
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This polarization can be described by extending the framework developed in [ref] , see App. [ref].
Polarized Photons from the Early Stages of Relativistic Heavy-Ion Collisions · Polarized photon emission · 0.97
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The generalization of ([ref]) is [ For this form, see the discussion surrounding Eq. (6.11) and footnote 24 of Ref. [ref] . ] \begin{align} Γ_3(,t) = (C_R_2 + C_R_3 - C_R_1) Γ̅_2(x_1 ,t) + (C_R_3 + C_R_1 - C_R_2) Γ̅_2(x_2 ,t) + (C_R_1 + C_R_2 - C_R_3) Γ̅_2(x_3 ,t) \end{align} for a $R_1 →R_2 R_3$ splitting process with corresponding momentum fractions \begin{equation} x_1 = 1 , x_2 = x, x_3 = 1-x . \end{equation} For $s →gs$ processes, this gives ([ref]).
Simple Formula for High-Energy Gluon Bremsstrahlung in a Finite, Expanding Medium · Pair Production $g→qq̅$ · 0.98
Uses its method or tool 21 papers
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The formalism developed in Ref. [ref] is employed to account consistently for collisional and radiative energy loss of hard partons in the Arnold-Moore-Yaffe (AMY) approach [ref] .
Jet energy loss and high $p_T$ photon production in hot quark-gluon plasma · Introduction · 1.00
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Radiative energy loss is modeled using the Arnold-Moore-Yaffe approach, where the interference of bremsstrahlung gluons from multiple scatterings is taken into account with an LPM-like integral equation for the energy loss rate [ref] .
Dijet asymmetry at the Large Hadron Collider · Transport of high-energy partons and martini · 0.99
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Radiative energy loss is modeled using the Arnold-Moore-Yaffe approach, where the interference of bremsstrahlung gluons from multiple scatterings is taken into account with an LPM-like integral equation for the energy loss rate [ref] .
Monte-Carlo simulation of jets in heavy-ion collisions · Transport of high-energy partons and martini · 1.00
Compares with it 3 papers
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This is in contrast to the limit of medium-induced branching [ref] , where one investigates emissions with transverse momenta dominated by interactions with the medium, i.e. $p_⊥∼√(q̂ z E)$.
Mapping collinear in-medium parton splittings · Implementing the semi-classical limit · 0.94
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By comparing our findings to previous calculations of parton broadening [ref] and energy loss [ref] in nuclear matter we identify areas where the effective theory calculation will be able to improve the accuracy of existing computations.
An effective theory for jet propagation in dense QCD matter: jet broadening and medium-induced bremsstrahlung · Introduction · 0.96
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In particular we will discuss two limits of the calculation which deal with the results of Refs. [ref] (referred to as the Arnold-Moore-Yaffe (AMY) formalism) and those of Refs. [ref] (referred to as the Armesto-Salgado-Wiedemann (ASW) formalism).
Hard collinear gluon radiation and multiple scattering in a medium · The multiple scattering Resummed single gluon emission kernel. · 0.93
Cites it as background 119 papers
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For the case of approximately on-shell massless particles traveling through an infinite medium, a complete leading-order analysis of such processes was carried out by Jeon and Moore [ref] using the formalism of Arnold, Moore, and Yaffe (AMY) [ref] .
QCD Splitting/Joining Functions at Finite Temperature in the Deep LPM Regime · Introduction and Results · 0.81
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This is often referred to as the scattering stage or the Baier-Dokshitzer-Mueller-Peigne-Schiff (BDMPS) stage [ref] or the Arnold-Moore-Yaffe (AMY) stage [ref] .
The medium modification of high-virtuality partons · Introduction · 0.97
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Formalisms based on Baier-Dokshitzer-Mueller-Peigne-Schiff- (BDMPS) [ref] , including Zakharov's [ref] contribution (BDMPS-Z), or the Arnold-Moore-Yaffe (AMY) [ref] approach, the Djordjevic-Gyulassy-Levai-Vitev [ref] prescription, as well as those inspired from higher twist [ref] have all be used in the past.
Multi-scale evolution of charmed particles in a nuclear medium · Introduction · 0.93
Discussion
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