REVIEW
Finite temperature field theory and phase transitions
High Energy Physics - Phenomenology · Submitted 14 Jan 1999 · 73 references
Pith's verdict: Solid, honest lecture notes on finite-temperature field theory; the physics is standard and correctly worked out, and the Higgs-mass washout bounds are era-specific numbers rather than new results.
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Referee report
The paper
The paper claims
The paper translates the requirement that sphalerons not erase the baryon asymmetry into upper bounds on the Higgs mass: about 42 GeV in the Standard Model and roughly 105 GeV in the MSSM.
The reading
What carries the argument
The load-bearing object is the finite-temperature sphaleron suppression factor $��exp[-E_{��rm sph}(T)/T]$, which controls how fast baryon-number-violating transitions proceed after the phase transition. The paper combines the zero-temperature sphaleron energy $E_{��rm sph}=(2m_W/��_W)B(��/g^2)$ with the finite-temperature scaling law $E_{��rm sph}(T)=E_{��rm sph}��langle��(T)��rangle/��langle��(0)��rangle$, then integrates the washout equation to get an exponent $X��sim 10^{10}��kappa��zeta^7 e^{-��zeta}$ with $��zeta=E_{��rm sph}(T_c)/T_c$. Requiring $X��lesssim 10$ yields $��zeta��gtrsim 45$, and the chain closes through the cubic term $E T��^3$ in the effective potential, which fixes $��(T_c)/T_c$ and hence the Higgs mass.
Extended reading notes
Core claim
The paper's central claim is that the condition of not washing out any previously generated baryon asymmetry can be translated, in both the Standard Model and the MSSM, into upper bounds on the Higgs mass. The chain runs through the finite-temperature sphaleron energy: requiring $E_{��rm sph}(T_c)/T_c ��gtrsim 45$ implies $��(T_c)/T_c ��gtrsim 1.3$, and using $��(T_c)/T_c ��sim 4 E v^2/m_h^2$ gives $m_h ��lesssim 42��{GeV}$ in the Standard Model. Because that value is already excluded, the Standard Model cannot preserve a pre-existing baryon asymmetry; the MSSM, with a light right-handed stop enhancing the cubic term in the effective potential, can push the bound to about $105��{GeV}$ while remaining consistent with the absence of color-breaking minima in a wide parameter region. The review presents this as a way to convert baryogenesis from a cosmological story into a constraint on the Higgs sector.
Load-bearing premise
The load-bearing premise is that the finite-temperature sphaleron energy scales linearly with the Higgs vacuum expectation value, $E_{��rm sph}(T)=E_{��rm sph}(0)��langle��(T)��rangle/��langle��(0)��rangle$, an approximation imported from Refs. 49 and 50 rather than tested here.
Editorial extensions
If this is right
- In the Standard Model the washout bound, about $42��{GeV}$, lies below the experimental Higgs-mass limit, so electroweak baryogenesis is ruled out in that model.
- In the MSSM with a light right-handed stop, the same logic leaves a viable window with $m_h$ between roughly $90$ and $105��{GeV}$ and stop masses of order $100$ to $165��{GeV}$, making the scenario a collider target.
- A strong first-order transition requires $��(T_c)/T_c ��gtrsim 1$, not merely a nonzero jump in the order parameter.
- Color-breaking minima in the stop direction constrain the allowed MSSM region; the paper separates absolute stability, metastability, and two-step transitions.
- Two-loop corrections can strengthen the transition for small right-handed stop masses, so the one-loop Higgs-mass ceiling is not the final word.
Reading between the lines
- If the linear sphaleron scaling is only approximate, the numerical Higgs-mass ceilings should be recomputed with a temperature-dependent sphaleron profile; a shift of a few GeV would move the MSSM window relative to collider reach.
- The same washout argument gives a model-independent design target for any extension of the Standard Model: new light bosons coupled to the Higgs that generate a large cubic term while avoiding color-breaking or charge-breaking minima.
- A future collider that measures a Higgs mass above about $110��{GeV}$ would not by itself kill all MSSM baryogenesis, but it would exclude the minimal light-stop window described here unless additional states or a two-step transition reopen it.
- The prefactor $��kappa$ in the washout rate is the main numerical soft spot; an improved determinant calculation could move the $��zeta��gtrsim 45$ threshold and hence the Higgs-mass bound by several GeV.
Original abstract
We review different aspects of field theory at zero and finite temperature, related to the theory of phase transitions. We discuss different renormalization conditions for the effective potential at zero temperature, emphasizing in particular the MS-bar renormalization scheme. Finite temperature field theory is discussed in the real and imaginary time formalisms, showing their equivalence in simple examples. Bubble nucleation by thermal tunneling, and the subsequent development of the phase transition is described in some detail. Some attention is also devoted to the breakdown of the perturbative expansion and the infrared problem in the finite temperature field theory. Finally the application to baryogenesis at the electroweak phase transition is done in the Standard Model and in the Minimal Supersymmetric Standard Model. In all cases we have translated the condition of not washing out any previously generated baryon asymmetry by upper bounds on the Higgs mass.
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 review different aspects of field theory at zero and finite temperature, related to the theory of phase transitions. We discuss different renormalization conditions for the effective potential at zero temperature, emphasizing in particular the MS-bar renormalization scheme. Finite temperature field theory is discussed in the real and imaginary time formalisms, showing their equivalence in simple examples. Bubble nucleation by thermal tunneling, and the subsequent development of the phase transition is described in some detail. Some attention is also devoted to the breakdown of the perturbative expansion and the infrared problem in the finite temperature field theory. Finally the application to baryogenesis at the electroweak phase transition is done in the Standard Model and in the Minimal Supersymmetric Standard Model. In all cases we have translated the condition of not washing out any previously generated baryon asymmetry by upper bounds on the Higgs mass.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We review different aspects of field theory at zero and finite temperature, related to the theory of phase transitions. | contribution 0.68 | 0.51 | 0.06 | asserted 0.67 |
| s1 | We discuss different renormalization conditions for the effective potential at zero temperature, emphasizing in particular the MS-bar renormalization scheme. | contribution 0.62 | 0.48 | 0.03 | asserted 0.89 |
| s2 | Finite temperature field theory is discussed in the real and imaginary time formalisms, showing their equivalence in simple examples. | contribution 0.52 | 0.48 | 0.04 | asserted 1.00 |
| s3 | Bubble nucleation by thermal tunneling, and the subsequent development of the phase transition is described in some detail. | contribution 0.80 | 0.37 | 0.05 | asserted 0.96 |
| s4 | Some attention is also devoted to the breakdown of the perturbative expansion and the infrared problem in the finite temperature field theory. | contribution 0.55 | 0.26 | 0.03 | asserted 0.64 |
| s5 | Finally the application to baryogenesis at the electroweak phase transition is done in the Standard Model and in the Minimal Supersymmetric Standard Model. | contribution 0.97 | 0.83 | 0.11 | asserted 0.99 |
| s6 | In all cases we have translated the condition of not washing out any previously generated baryon asymmetry by upper bounds on the Higgs mass. | result 0.87 | 0.86 | 0.41 | asserted 0.99 |
What was examined, and what was not
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Figures
Figures reproduced from arXiv:hep-ph/9901312 by the authors.
References
How later papers used it
348 later papers cite it
25 later papers by other authors are listed below: 22 used its method or tool and 3 used its data or values.
Uses its method or tool 22 of 87 papers with this label
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The one-loop corrections $V_1(φ, 0)$ and $ΔV_1(φ, T)$ are calculated using the Coleman-Weinberg [ref] and finite temperature [ref] methods respectively, and are given by [equation] where $i$ counts over all particle species with $+$ for bosons and $-$ for fermions, and $n_i$ and $m_i(φ)$ are the multiplicity and field-dependent mass of species $i$.
Implementing Asymmetric Dark Matter and Dark Electroweak Baryogenesis in a Mirror Two-Higgs-Doublet Model (2021) · One-loop corrections and renormalisation · 1.00
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For negative $y$ (tachyonic regions of the $V_eff$ landscape) we analytically continue $J_B$ using the prescription of Ref. [ref] .
Thermal Metastable Strings in One-Scale Models and Gravitational Waves (2026) · Finite-temperature effective potential · 1.00
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Based its investigation of the phase structure on the daisy-improved one-loop finite-temperature effective potential of this paper.
Strong Supercooling as a Consequence of Renormalization Group Consistency (2019) · 0.99 · paraphrased: the licence does not allow quoting
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Analyzed the finite temperature effective potential of this paper under a simplifying assumption.
Dark Matter and Baryogenesis from Non-Abelian Gauged Lepton Number (2017) · 0.99 · paraphrased: the licence does not allow quoting
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Added the one-loop thermal corrections given by this paper to study the cosmological evolution of its potential.
EFT Interpretation of XENON1T Electron Recoil Excess: Neutrinos and Dark Matter (2020) · 0.99 · paraphrased: the licence does not allow quoting
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We compute the correction to the potential up to one-loop level, including zero-temperature Coleman-Weinberg corrections and finite-temperature corrections [ref] .
Axiogenesis from $SU(2)_R$ phase transition (2021) · Details of effective potential · 0.98
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In order to analyse the strength of the phase transition we use the effective potential, $V_eff$, at one loop order including $T=0$ and finite temperature loop contributions of $ϕ$, the $SU(2)_G$ gauge bosons and two generations of $Ψ$ fermions [ref] .
Gravitational waves from the asymmetric-dark-matter generating phase transition (2017) · The potential · 0.98
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Mainly followed the discussions in this paper.
Phase Transitions in Twin Higgs Models (2018) · 0.98 · paraphrased: the licence does not allow quoting
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Because the Standard Model particles are in the thermal plasma, the potential can be derived using the imaginary time formalism [ref] .
Imperfect Axion Precludes the Domain Wall Problem (2023) · Introduction · 0.96
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Calculated its one-loop thermal effective potential using the standard techniques of this paper.
Dark Quark Nuggets (2018) · 0.96 · paraphrased: the licence does not allow quoting
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Using the imaginary time formalism, it can be calculated as [ref] [equation] where [equation] and $Θ$ is a step function, $δ$ is a Dirac delta function.
Core-collapse Supernova Constraint on the Origin of Sterile Neutrino Dark Matter via Neutrino Self-interactions (2022) · $ϕ$ mediated thermal potential · 0.96
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Employed the conventional 4D perturbative method of this paper to calculate the effective potential.
Gravitational waves from cosmological first-order phase transitions with precise hydrodynamics (2024) · 0.95 · paraphrased: the licence does not allow quoting
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Calculated its nonzero-temperature potential to one-loop level following this paper under the Parwani resummation prescription.
PBH formation and Gravitational Waves as Multi-messenger Signals of First-order Phase Transitions (2026) · 0.94 · paraphrased: the licence does not allow quoting
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Applied the high-temperature expansion of the thermal functions given by this paper.
Electroweak Phase Transition in Singlet Extensions of The Standard Model with Dimension-Six Operators (2024) · 0.94 · paraphrased: the licence does not allow quoting
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Finally the finite temperature correction to the effective potential at one-loop is given by [ref] , [equation] where the thermal bosonic and fermionic function $J_B$ and $J_F$ are defined as : [equation] We have also taken care of the daisy resummation by redefining the field dependent masses of the scalars and longitudinal polarization of the gauge bosons as follows.
Electroweak phase transitions in a $U(1)_D$ extension of the standard model with dimension-six operators: Gravitational waves and LHC signatures (2026) · Phase transitions · 0.92
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On the other hand, the one-loop finite temperature contribution is [ref] [equation] where $J_F(m^2/T^2)$ is the thermal fermionic function (see App. [ref]).
A Non-Holomorphic Modular $A_4$ Framework for Resonant Leptogenesis with Gravitational Wave Signatures (2026) · Bias term · 0.81
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The finite temperature contribution to the potential is [ref] V_temp(ϕ_1,ϕ_2, T) = T^4/2π^2 ∑_i n_i ∫_0^∞dy y^2 log(1∓e^-√(m_i^2(ϕ_1,ϕ_2)/T^2 + y^2)) + T/12π ∑_j n'_j {m_j^3(ϕ_1,ϕ_2) - [m^2(ϕ_1,ϕ_2) + Π(T)]_j^3/2} , where in the second line the minus sign corresponds to bosons and the plus sign to fermions, the sum over $i$ incorporates all particles with field-dependent masses, the sum over $j$ includes only bosons, $n_i$ denotes the number of degrees of freedom for a given particle, $n'_j$ is the number of all degrees of freedom in the case of scalars and solely longitudinal ones for vector bosons, $Π(T)$ is the thermal mass matrix, and $[m^2(ϕ_1,ϕ_2) + Π(T)]_j$ are the eigenvalues of the matrix $[m^2(ϕ_1,ϕ_2) + Π(T)]$.
Asymmetric Dark Matter from Gravitational Waves (2022) · Effective potential · 0.89
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Here, $Λ$ represents the renormalization scale, which we fix to be $v_R$, and the CW potential is evaluated in the Landau gauge [ref] ; hence, there are no ghost contributions.
Gravitational Wave Imprints of Left-Right Symmetric Model with Minimal Higgs Sector (2021) · Effective Potential · 0.84
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At zero temperature, the one-loop effective potential $V_1$ receives the Coleman-Weinberg terms [ref] in the $MS$ renormalization scheme [ref] , [equation] where the sum runs over all the particles $i$ coupling to the classical fields, and $m̃_i^2$ are the corresponding particle masses squared in terms of the classical fields.
Phase transition gravitational waves from pseudo-Nambu-Goldstone dark matter and two Higgs doublets (2021) · Effective potential · 0.84
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Used the leading thermal correction given by this paper.
Electroweak Phase Transition with an SU(2) Dark Sector (2020) · 0.81 · paraphrased: the licence does not allow quoting
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In the Landau gauge, with $MS$ renormalization scheme, the CW potential is [ref] V_(R) = 1/64π^2∑_i (-1)^f_i n_i m_i^4(R)[log(m_i^2(R)/μ^2) - c_i ], where $i$ runs over all species coupling to the $SU(2)_R×U(1)_B-L$-breaking field $χ^0_Rr$.
Gravitational Wave imprints of the Doublet Left-Right Symmetric Model (2023) · Effective Potential · 0.89
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To obtain temperature corrections one adds to potential temperature dependent parts [ref] : [equation] $δV_T$ stands for standard temperature corrections of first order: [equation] where $n_i$ and $n_j$ are numbers of degrees of freedom of considered boson or fermion particle with field-dependent mass $m_i(ϕ_k)$ and $J_B$ and $J_F$ are thermal bosonic (B) or fermionic (F) functions defined as follows: [equation] [equation] One should also add infrared contributions from higher order diagrams [ref] , which are of the same order as corrections from ([ref]): [equation] which is the so-called ring improvement of the potential and is sufficient for high temperatures, when $(m/T)≪ 1$.
Spontaneous scale symmetry breaking at high temperature (2022) · Quantum Field Theory at finite temperature: · 0.82
Uses its data or values 3 of 8 papers with this label
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Took its critical temperature of 165 GeV from the effective potential given in this paper.
Relic density of wino-like dark matter in the MSSM (2016) · 0.99 · paraphrased: the licence does not allow quoting
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where the sphaleron energy is $E_sph ≃3.34 m_W(T)/α_2$ [ref] .
Electroweak Baryogenesis from Collapsing Domain Walls (2026) · Introduction · 0.98
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Used the approximate expression for B given by this paper for the standard model.
Baryogenesis: A Symmetry Breaking in the Primordial Universe Revisited (2023) · 0.88 · paraphrased: the licence does not allow quoting
How the literature uses it
357 arXiv papers cite this in 584 sentences
Papers citing it · 365 sentences without a confident label
Uses its method or tool 91 papers
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The thermal functions are defined by the following integrals [ref] , [equation] In the thermal correction we have included also the daisy resummation [ref] , which amounts to the following replacement [equation] for the scalar fields and the longitudinal components of the gauge bosons.
Gravitational Wave Imprints of Left-Right Symmetric Model with Minimal Higgs Sector · Effective Potential · 0.90
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In this section, we construct the full one-loop finite temperature effective potential [ref] required to study the nature of the PT associated with the breaking of $SU(2)_R ×U(1)_B-L$.
Gravitational Wave imprints of the Doublet Left-Right Symmetric Model · Effective Potential · 0.92
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To get the parameter space in which an FOPT occurs, we analyze the structure of the effective potential incorporating the tree-level potential $V_tree$, the one-loop Coleman-Weinberg correction $V_CW$ [ref] , and finite-temperature corrections [ref] .
Naturally small Dirac neutrino mass and $B-L$ dark matter · Introduction · 0.92
Uses its data or values 8 papers
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For the standard model, $B$ is approximately given by [ref] [equation] an approximation valid for values of the Higgs mass in the range $25 GeV≤m_H≤250 GeV$.
Baryogenesis: A Symmetry Breaking in the Primordial Universe Revisited · Necessary Conditions for a Successful EWB: The Sphaleron Bound · 0.88
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The thermal Higgs mass is given by $m_h (T)≃0.6T$ [ref] .
Delayed Charged Lepton Yukawa Equilibration in Minimal Seesaw · Introduction · 0.90
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where the sphaleron energy is $E_sph ≃3.34 m_W(T)/α_2$ [ref] .
Electroweak Baryogenesis from Collapsing Domain Walls · Introduction · 0.98
Compares with it 2 papers
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In all these plots, we present a comparison of our full $N^3$LO computation with the frequently used, sole one-loop approximation [ref] (cf. Appendix [ref]).
Speed of sound in cosmological phase transitions and effect on gravitational waves · Computation of the pressure and sound speed · 0.93
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In earlier work (see, e.g., Ref. [ref] ), a value of $X≈10$ was used, corresponding to a dilution of roughly five orders of magnitude.
Baryon Washout, Electroweak Phase Transition, and Perturbation Theory · Baryon number preservation criterion · 0.86
Cites it as support 2 papers
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In the Standard Model, the electroweak phase transition is a first-order phase transition [ref] , but it is insufficiently strong to generate the baryon asymmetry in the Universe.
Spontaneous Symmetry Breaking: From the Effective Action to Cosmological Phase Transitions in the Standard Model and Beyond · Sphalerons · 0.98
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This decoupling limit typically disfavors an SFOEWPT, because the transition strength $ξ_c$ vanishes as the scalar spectrum becomes increasingly decoupled [ref] , effectively placing an upper bound of around $1$ on the BSM Higgs masses [ref] .
Multi-step Strong First-Order Electroweak Phase Transitions in the Inverted Type-I 2HDM: Parameter Space, Gravitational Waves, and Collider Phenomenology · Introduction · 0.97
Cites it as background 89 papers
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The effective potential describes the exact vacuum state [ref] of a theory including finite temperature effects [ref] .
Two Higgs doublets, Effective Interactions and a Strong First-Order Electroweak Phase Transition · Review of Calculational Methods · 0.81
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As we outline in more detail in <ref>, the leading corrections that distinguish $V^eff$ from $V^tree$ are the Coleman-Weinberg term $V^CW$ that corresponds to resummed 1-loop diagrams at $T=0$ [ref] , the thermal one-loop contribution [ref] , $V^T$, and the resummed series of higher order “daisy” diagrams, $V^daisy$ [ref] .
Dynamic Freeze-In: Impact of Thermal Masses and Cosmological Phase Transitions on Dark Matter Production · The Effective Potential · 0.90
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The analysis of the symmetry properties at finite temperatures, see e.g. [ref] , requires the calculation of the one-loop effective (Coleman-Weinberg) potential at zero temperature [ref] in addition to temperature corrections and associated Daisy resummation [ref] .
Effective 2HDM Yukawa Interactions and a Strong First-Order Electroweak Phase Transition · Effective Potential at Finite Temperature · 0.82
Discussion
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