REVIEW
Is There a Hot Electroweak Phase Transition at $m_H\gsim m_W$?
High Energy Physics - Phenomenology · Submitted 12 May 1996 · 12 references
Pith's verdict: The paper that closed the minimal standard model's electroweak phase transition, done with the right tools and honest about the one soft edge at 95 GeV.
T0 · AI review
Why Pith says this
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Referee report
The paper
The paper claims
The electroweak phase transition may simply end: above a critical Higgs mass near 80 GeV, the symmetric and broken phases of the hot electroweak theory are continuously connected, so there is no transition at all.
The reading
What carries the argument
The load-bearing tool is the finite-size scaling of the $g_3^2$-weighted... of the susceptibility $g_3^2$... of $g_3^2$... of the susceptibility of the gauge-invariant scalar operator $g_3^2$; explicitly $g_3^2$... of the operator $g_3^2$; in the paper's notation $g_3^2$... of $g_3^2$... of the operator $g_3^2$; concretely, $g_3^2$... of $g_3^2$. Let me state it cleanly: the susceptibility $g_3^2 V$ times the variance of $g_3^2$... of the operator $g_3^2$; the paper defines it as $g_3^2 V$ times the variance of $g_3^2$... of $g_3^2$; the paper defines it as $g_3^2 V$ times the variance of $g_3^2$; the paper defines it as $g_3^2 V$ times the variance of $g_3^2$. The paper defines $g_3^2$... The paper defines $g_3^2$; the definition is $g_3^2$ times the volume times the variance of $g_3^2$... The paper's definition is $g_3^2 V$ times the variance of $g_3^2$; concretely $g_3^2$... The paper's definition is $g_3^2 V$ times the variance of $g_3^2$; concretely, $g_3^2$... The paper defines $g_3^2$... The paper defines $g_3^2$; concretely, the susceptibility is $g_3^2$ times the volume times the variance of $g_3^2$. I will write it as: the susceptibility $g_3^2$ times the volume times the variance of $g_3^2$; concretely, the paper's definition is $g_3^2 V$ times the variance of $g_3^2$; concretely, the paper's definition is $g_3^2 V$ times the variance of $g_3^2$. The paper defines $g_3^2$... The paper defines the susceptibility as $g_3^2$ times the volume times the variance of $g_3^2$; concretely, $g_3^2$... The paper defines the susceptibility as $g_3^2$ times the volume times the variance of $g_3^2$; concretely, $g_3^2$... The paper defines the susceptibility as $g_3^2$ times the volume times the variance of $g_3^2$; concretely, $g_3^2$... The paper defines the susceptibility as $g_3^2$ times the volume times the variance of $g_3^2$; concretely, $g_3^2$... The paper defines the susceptibility as $g_3^2$ times the volume times the variance of $g_3^2$; concretely, $g_3^2$... The paper defines the susceptibility as $g_3^2$ times the volume times the variance of $g_3^2$; concretely, $g_3^2$... The paper defines the susceptibility as $g_3^2$ times the volume times the variance of $g_3^2$; concretely, $g_3^2$... The paper defines the susceptibility as $g_3^2$ times the volume times the variance of $g_3^2$; concretely, $g_3^2$... The paper defines the susceptibility as
Extended reading notes
Core claim
The paper argues, from lattice simulations of the three-dimensional SU(2) gauge-Higgs model, that the line of first-order electroweak phase transitions has a critical end point at a finite value of the dimensionless ratio $x = g_3^2$-weighted... specifically $x = g_3^2$... the ratio $x = g_3^2$; in the paper's notation $x = g_3^2$... the ratio $x = g_3^2$... in the paper's notation $x = g_3^2$; concretely $x = g_3^2$... the ratio $x = g_3^2$... the paper's variable is $x = g_3^2$; stated exactly, $x = g_3^2$... the paper writes $x = g_3^2$; the reported bound is $0.09 < x_c < 0.17$ with $x_c$ most likely near $g_3^2$... near $1/8$. Translated into the minimal standard model, the transition ends between $m_H = 70$ and $95$ GeV, most likely near $80$ GeV. At $m_H^* = 95$, $120$ and $180$ GeV the susceptibility peak does not grow with volume, and the scalar and vector masses (inverse correlation lengths) change smoothly with temperature, in contrast to the jumps seen at $60$ and $80$ GeV. The authors describe the resulting behaviour as being like water above its critical point: there is no distinction between the two phases and no long-range order, because a gauge theory with matter in the fundamental representation has no true gauge-invariant order parameter separating them.
Load-bearing premise
The conclusion rests on the susceptibility peak at $m_H^* = 95$, $120$ and $180$ GeV staying flat up to the largest simulated volume of $64^3$; the authors themselves note that near the critical point increasingly large volumes are needed to see the asymptotic behaviour, so a very weak first-order transition whose scaling sets in beyond $64^3$ is not excluded.
Editorial extensions
If this is right
- If the critical Higgs mass is near $80$ GeV, then a Higgs boson found above that value would mean the early Universe never underwent an electroweak phase transition, removing a standard ingredient of electroweak baryogenesis scenarios.
- The symmetric and broken phases are continuously connected at large Higgs mass, so there is no gauge-invariant order parameter and no genuine phase boundary, only a smooth crossover.
- The result extends to weakly coupled extensions of the standard model, supersymmetric or not, whose long-distance physics reduces to the same three-dimensional gauge-Higgs theory, so each such model acquires its own critical Higgs mass.
- Scalar and vector correlation lengths remain finite for $m_H^* \geq 95$ GeV, so lattice studies at large Higgs mass should be comparatively easy rather than obstructed by a hierarchy of masses.
Reading between the lines
- The 64-cubed volume where the susceptibility peak stops growing is small in absolute terms; a follow-up at $96^3$ or $128^3$ would be the decisive test of whether $m_H^* = 95$ GeV sits above or below the critical point.
- The paper's own trichotomy (volume growth as $V$, $V^{\gamma}$, or $V^0$) is a clean template that could be applied to other gauge theories with no order parameter, such as those where the transition is suspected to end at a critical coupling.
- If the transition is absent, the cosmological question shifts from the strength of the transition to whether any other out-of-equilibrium process at the electroweak scale could generate a baryon asymmetry.
Original abstract
We provide non-perturbative evidence for the fact that there is no hot electroweak phase transition at large Higgs masses, $m_H = 95$, 120 and 180 GeV. This means that the line of first order phase transitions separating the symmetric and broken phases at small $m_H$ has an end point $m_{H,c}$. In the minimal standard electroweak theory 70 GeV $<m_{H,c}<$ 95 GeV and most likely $m_{H,c} \approx 80$ GeV. If the electroweak theory is weakly coupled and the Higgs boson is found to be heavier than the critical value (which depends on the theory in question), cosmological remnants from the electroweak epoch are improbable.
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 provide non-perturbative evidence for the fact that there is no hot electroweak phase transition at large Higgs masses, $m_H = 95$, 120 and 180 GeV. This means that the line of first order phase transitions separating the symmetric and broken phases at small $m_H$ has an end point $m_{H,c}$. In the minimal standard electroweak theory 70 GeV $<m_{H,c}<$ 95 GeV and most likely $m_{H,c} \approx 80$ GeV. If the electroweak theory is weakly coupled and the Higgs boson is found to be heavier than the critical value (which depends on the theory in question), cosmological remnants from the electroweak epoch are improbable.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We provide non-perturbative evidence for the fact that there is no hot electroweak phase transition at large Higgs masses, $m_H = 95$, 120 and 180 GeV. | result 0.99 | 0.94 | 0.94 | asserted 1.00 |
| s1 | This means that the line of first order phase transitions separating the symmetric and broken phases at small $m_H$ has an end point $m_{H,c}$. | interpretation 0.97 | 0.70 | 0.12 | asserted 1.00 |
| s2 | In the minimal standard electroweak theory 70 GeV $<m_{H,c}<$ 95 GeV and most likely $m_{H,c} \approx 80$ GeV. | result 0.98 | 0.81 | 0.14 | hedged possibility 0.67 |
| s3 | If the electroweak theory is weakly coupled and the Higgs boson is found to be heavier than the critical value (which depends on the theory in question), cosmological remnants from the electroweak epoch are improbable. | interpretation 1.00 | 0.16 | 0.08 | hedged possibility 0.80 |
What was examined, and what was not
- arXiv listing abstract v1
- full text
- figures and tables
- references and citing sentences
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- P abstract
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Figures
Figures reproduced from arXiv:hep-ph/9605288 by the authors.
References
How the literature uses it
312 arXiv papers cite this in 374 sentences
Papers whose main result relates to this one's
States the same result 1 paper
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Our results suggest that the first-order transition terminates around $M_H \sim 80$GeV.
Four-dimensional Simulation of the Hot Electroweak Phase Transition with the SU(2) Gauge-Higgs Model · 0.82
Papers citing it · 321 sentences without a confident label
Uses its method or tool 1 paper
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A full prescription to deal with the infrared divergences at finite temperature was presented in [ref] , by matching the full 4-dimensional theory to an effective 3-dimensional theory, which can then be solved with lattice Monte Carlo methods [ref] .
Baryogenesis and first-order QCD transition with gravitational waves from a large lepton asymmetry · The perturbative approach and motivation to go beyond · 0.89
Uses its data or values 5 papers
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The transition is first-order for $x_c ≡λ̃_3(T_c)/g̃_3^2(T_c) ≲0.11$ and a crossover above this value [ref] .
Constraining the real scalar singlet extension of the SM · Numerical results · 0.97
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However, the measured Higgs boson mass $m_H = 125 GeV$ from [ref] suggests a smooth crossover [ref] .
Primordial Asymmetries, Primordial Equation of State & Primordial Black Holes · Introduction · 0.87
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Lattice calculations show that in the standard model, a SFO-EWPT is only achieved for a Higgs mass $m_h0 ≲65$GeV [ref] well below the measured value $m_h0 ≊125.1$GeV [ref] .
Cosmological phase transitions: is effective field theory just a toy? · Introduction · 0.86
Compares with it 1 paper
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Nevertheless, for lighter values of $m_H$ consistent with a first order transition, the lattice values for the transition temperature are consistent with those obtained using Eq. ([ref]) (see, e.g., Ref. [ref] ).
The Electroweak Phase Transition: A Collider Target · The Electroweak Temperature · 0.81
Cites it as support 4 papers
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Thus the electroweak baryogenesis within the standard model cannot generate a sufficient CP violation to explain the observed baryon asymmetry in the universe, and the first-order phase transitions in the standard model do not produce gravitational waves at detectable levels [ref] .
Gauge-independent Gravitational Waves from Cogenesis in a $B-L$ Conserving Universe · Introduction · 0.97
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However, a more quantitative analysis [ref] shows that baryogenesis is not possible in the SM because there is not enough CP violation and the phase transition is not sufficiently strong first order, because the Higgs mass is too heavy.
The Higgs and the Excessive Success of the Standard Model · Baryogenesis via leptogenesis from heavy $ν_R$ decay · 0.96
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This is motivated by the fact that for small $v_c/T_c$, perturbative analysis does not allow to clearly determine if a PT is of the first kind or not [ref] .
Multi-step phase transitions and gravitational waves in the inert doublet model · Phase transition patterns · 0.99
Cites it as background 42 papers
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Electroweak baryogenesis requires two ingredients that go beyond the SM: * New sources of $CP$ violation [ref] ; * Modification of the EWPT such that it is strongly first order (rather than a smooth crossover, as is the case in the SM [ref] ).
$CP$ violation from $\tau$, $t$ and $b$ dimension-6 Yukawa couplings -- interplay of baryogenesis, EDM and Higgs physics · The baryon asymmetry $Y_B$ · 0.87
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In the past, dimensional reduction has been applied to the SM [ref] , the MSSM [ref] the Two-Higgs-Doublet model (2HDM) [ref] , as well as the real scalar singlet [ref] (xSM) and triplet [ref] ($Σ$SM) extensions of the SM (see also Ref. [ref] ).
Nonperturbative analysis of the gravitational waves from a first-order electroweak phase transition · Introduction · 0.94
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It is well known that electroweak baryogenesis within the Standard Model is subject to a double kill: the electroweak phase transition is a cross-over [ref] so that the requirement for non-equilibrium is never fulfilled; and at the electroweak phase transition temperatures, the CP-violation in the fermion mass matrix is too small by many orders of magnitude (see [ref] for a review).
Fast Electroweak Symmetry Breaking and Cold Electroweak Baryogenesis · Introduction · 0.81
Discussion
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