REVIEW
Di-photon resonance around 750 GeV: shedding light on the theory underneath
High Energy Physics - Phenomenology · Submitted 17 Dec 2015 · 65 references
Pith's verdict: A competent, standard recasting of the 750 GeV excess whose qualitative point survives but whose 0.3 GeV headline number does not.
T0 · AI review
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Referee report
The paper
The paper claims
A 750 GeV diphoton bump can only be explained if the resonance has a large hidden decay channel, and the particles running in its loops are more likely fermions than scalars.
The reading
What carries the argument
The load-bearing device is the two-parameter effective vertex set of Eq. (1): a gluon coupling $kappa_g$ and a hypercharge coupling $kappa_A$ that, after electroweak symmetry breaking, fixes the ratios $mathrm{Br}(H_X to ZZ) : mathrm{Br}(H_X to Zgamma) : mathrm{Br}(H_X to gammagamma)$ at $sin^4theta_W : sin^2theta_Wcos^2theta_W : cos^4theta_W$. That rigid ratio is what lets the authors translate one observed rate into predictions for channels that were not seen, and hence into exclusions. The second device is the $mathrm{Br}(H_X to gg)$ versus $mathrm{Br}(H_X to gammagamma)$ plane, where the observed excess becomes a diagonal band and each search becomes a vertical or horizontal cut, so that the allowed product of branching ratios can be read off for a chosen total width. The one-loop scalar and fermion amplitudes $A_Phi(x)$ and $A_F(x)$, evaluated for masses between roughly 400 GeV and 1 TeV, then convert that product back into statements about the charge and colour of the particles in the loop.
Extended reading notes
Core claim
Working with the minimal Lagrangian $mathcal{L}_{rm eff}=kappa_g, G^a_{munu}G^{munu}_a H_X + kappa_A, B_{munu}B^{munu} H_X$, the authors map the region of $(kappa_g, kappa_A)$ that reproduces the observed diphoton rate against the 8 TeV limits on $H_X to ZZ$, $H_X to Zgamma$, $H_X to jj$ and $H_X to gammagamma$, and against the photon-fusion constraint. They find that no realistic values of the two couplings can produce a total width above roughly 0.3 GeV, so an additional decay width $Gamma_X^{rm add}$ is required to reach the 45 GeV hinted by ATLAS. Rewriting the surviving parameter space as a correlation between $mathrm{Br}(H_X to gg)$ and $mathrm{Br}(H_X to gammagamma)$, they extract a width-dependent band on the product, $0.08times10^{-3} lesssim mathrm{Br}^2(gammatimes gg) lesssim 1.93times10^{-3}$ for $Gamma_X = 1$ GeV and $0.08times10^{-5} lesssim mathrm{Br}^2(gammatimes gg) lesssim 4.28times10^{-5}$ for $Gamma_X = 45$ GeV at $2sigma$. Feeding that band into the one-loop formulas for a new scalar or a vector-like fermion, they conclude that scalars require electric charges near 10 to 20 or more than about 14 colours to work, whereas a colour-triplet, charge-3 vector-like fermion reproduces the excess with $mathrm{Br}(H_X to gg)$ between about 0.01 and 0.1, consistent with the dijet limits.
Load-bearing premise
The claim that no allowed coupling choice can exceed about 0.3 GeV of width rests on applying the photon-fusion bound under the closure condition $mathrm{Br}(H_X to gg)+mathrm{Br}(H_X to gammagamma)=1$, even though the same figures compute the width from four channels; the authors say so themselves and call the resulting $mathrm{Br}(H_X to gg)$ limits purely illustrative.
Editorial extensions
If this is right
- Any model that explains the diphoton excess through loops must also contain a large hidden decay mode, since the gluon and photon couplings alone cap the width near 0.3 GeV.
- : The ratios of $ZZ$ and $Zgamma$ signals to the diphoton signal are fixed by $theta_W$ once the hypercharge coupling dominates, so a confirmed $Zgamma$ or $ZZ$ signal at the predicted ratio would corroborate the effective description.
- : Vector-like fermions with colour and electric charge of a few units are the favoured loop content; scalars need charges around 10 to 20 or more than about 14 colours, which would make them copiously produced and hard to hide.
- : If the width is confirmed to be near 45 GeV, the allowed product $mathrm{Br}(H_X to gammagamma)mathrm{Br}(H_X to gg)$ falls to order $10^{-5}$, pushing the new fermions to lower masses and larger couplings, which improves the reach of a direct search for $gg to H_X^* to Fbar F$.
- : A narrow width near 1 GeV would instead leave little room for observing the loop fermions directly, because the allowed region shifts toward small couplings or heavy masses.
Reading between the lines
- The paper's central structural point generalises past this particular resonance: whenever a new state is produced and decays through the same set of effective couplings, the observed rate in one channel fixes the rates in the others, so a single excess can be used to predict where else to look before any of those channels is measured.
- : The argument that a large width demands a hidden sector invites the obvious follow-up of checking whether that hidden sector is itself the dark matter, since the same invisible branching fraction that rescues the width would show up as monojet plus missing energy and as a thermal-relic abundance.
- : The preference for vector-like fermions over scalars is really a statement about how many units of charge-squared per unit of mass the loop can supply; it suggests that any future excess of this type should be read as a measurement of the loop particle's $N_c Q^2 / M$ rather than as evidence for a specific model.
- : The authors' own caveat that the photon-fusion bound assumes $mathrm{Br}(H_X to gg)+mathrm{Br}(H_X to gammagamma)=1$ while the width is computed from four channels means the 0.3 GeV ceiling should be treated as an illustration of the mechanism rather than a sharp number; a fully consistent closure would weaken the ceiling and could reopen part of the coupling space.
Original abstract
Both the ATLAS and CMS collaborations have recently observed an excess in the di-photon invariant mass distribution in the vicinity of 750 GeV with a local significance of $\sim3\sigma$. In this article we try to investigate this excess in the context of a minimal simplified framework assuming effective interactions of the hinted resonance with photons and gluons. We scrutinise the consistency of this observation with possible accompanying yet hitherto unseen signatures of this resonance. Subsequently, we try to probe the nature of new particles, e.g., spin, electric charge and number of colour, etc., that could remain instrumental to explain this excess through loop-mediation.
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
Both the ATLAS and CMS collaborations have recently observed an excess in the di-photon invariant mass distribution in the vicinity of 750 GeV with a local significance of $\sim3\sigma$. In this article we try to investigate this excess in the context of a minimal simplified framework assuming effective interactions of the hinted resonance with photons and gluons. We scrutinise the consistency of this observation with possible accompanying yet hitherto unseen signatures of this resonance. Subsequently, we try to probe the nature of new particles, e.g., spin, electric charge and number of colour, etc., that could remain instrumental to explain this excess through loop-mediation.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | Both the ATLAS and CMS collaborations have recently observed an excess in the di-photon invariant mass distribution in the vicinity of 750 GeV with a local significance of $\sim3\sigma$. | background 0.99 | 0.04 | 0.04 | asserted 0.99 |
| s1 | In this article we try to investigate this excess in the context of a minimal simplified framework assuming effective interactions of the hinted resonance with photons and gluons. | contribution 0.81 | 0.44 | 0.04 | unclear 0.32 |
| s2 | We scrutinise the consistency of this observation with possible accompanying yet hitherto unseen signatures of this resonance. | contribution 0.91 | 0.51 | 0.04 | hedged possibility 0.47 |
| s3 | Subsequently, we try to probe the nature of new particles, e.g., spin, electric charge and number of colour, etc., that could remain instrumental to explain this excess through loop-mediation. | contribution 0.84 | 0.43 | 0.05 | hedged possibility 0.95 |
What was examined, and what was not
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Figures
Showing 5 of the paper's 6 figures. See all figures in the PDF ↗ Figures reproduced from arXiv:1512.05767 by the authors.
References
How the literature uses it
62 arXiv papers cite this in 64 sentences
Papers citing it · 14 sentences without a confident label
Uses its data or values 1 paper
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There is a smaller complimentary excess in the 13 TeV CMS data (2.9$σ$ local) [ref] , which grows to 3.4$σ$ local when combined with their 8 TeV data [ref] .
750 GeV Diphotons from Supersymmetry with Dirac Gauginos · Introduction · 0.96
Cites it as background 47 papers
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Although the significance of this excess is only around $3 σ$ and more statistics is required to draw a firm conclusion, it has already triggered an avalanche of theoretical speculations in terms of a new resonance $X$; see e.g. [ref] .
Asymmetric Dark Matter in the Sun and the Diphoton Excess at the LHC · Introduction · 0.88
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Related studies considering gluon fusion partonic processes have been recently performed in Refs. [ref] , whereas photon fusion was considered in Refs. [ref] .
A 750 GeV Portal: LHC Phenomenology and Dark Matter Candidates · Two Different Scenarios for · 0.98
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This could be an argument against the reality of the diphoton excess, meaning nothing but a statistical fluctuations; but if taken seriously, it put strong constraint on the implied model building [ref] [ Refs. [ref] on this subject appeared at the same time as this work.].
The Minimal Scalar-Stealth Top Interpretation of the Diphoton Excess · Introduction · 0.85
Discussion
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