Paper Citation Record · LEDGER

Cosmological phase transitions without high-temperature expansions

As of 18 August 2026, this Paper Citation Record lists 100 of 163 outbound references and 10 inbound Pith citation observations for arXiv:2507.07014.

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pith.paper-citation-record.v1
2507.07014 v1

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measured 100 of 163 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-06T18:56:41.292449Z

measured 110 of 110 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T00:43:56.828055Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-07-04T06:59:38.418933Z

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Outbound references

Observation e783644b-8c2b-40c0-8582-6203b3309bb0 · outbound

This paper cites an unresolved cited work.

Cosmological phase transitions without high-temperature expansions Unresolved cited work

Reference 1

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Observation d6fec899-5029-49f1-8196-9b66c1e50279 · outbound

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Cosmological phase transitions without high-temperature expansions Unresolved cited work

Reference 2

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Observation 4e328776-6589-4e32-8070-e6b51b3e79ee · outbound

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Reference 3

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Observation f2f6007c-4cf5-428e-8219-9cf6863089d9 · outbound

This paper cites one-loop.

Cosmological phase transitions without high-temperature expansions one-loop

Reference 4

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Observation 73a44e4e-2ac1-46f8-8bc6-ed2650aa47d3 · outbound

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Cosmological phase transitions without high-temperature expansions Unresolved cited work

Reference 5

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Observation 7d85df7f-859e-4059-8ffa-2de1341cf5df · outbound

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Reference 6

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Observation e907a257-6619-4bb0-8704-a7f11a1f7745 · outbound

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Cosmological phase transitions without high-temperature expansions Unresolved cited work

Reference 7

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Observation 3f5fe682-5223-4a8b-a052-58044225252a · outbound

This paper cites (A18) Here, we define z2 ≡ x2 1/x2 2 and w ≡ √ 1 − 4z−2, while ψ1(x) = d2/dx2 ln Γ(x) is the trigamma function and Li2(x) is the dilogarithm [147].

Cosmological phase transitions without high-temperature expansions (A18) Here, we define z2 ≡ x2 1/x2 2 and w ≡ √ 1 − 4z−2, while ψ1(x) = d2/dx2 ln Γ(x) is the trigamma function and Li2(x) is the dilogarithm [147]

Reference 8

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Observation b272a453-fbde-41c6-8649-57a9e3903925 · outbound

This paper cites (B1) Owing to ∆Π hard R capturing hard-scale effects only, it is well defined in the infrared and can hence be expanded in soft momenta k2 ≲ λT 2 up to O(λ2T 2).

Cosmological phase transitions without high-temperature expansions (B1) Owing to ∆Π hard R capturing hard-scale effects only, it is well defined in the infrared and can hence be expanded in soft momenta k2 ≲ λT 2 up to O(λ2T 2)

Reference 9

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Observation 82b12af2-5a20-46b0-adac-03913fd19b63 · outbound

This paper cites Γ(3) 4d (p0 i = 0, pi → 0) = Γ(3) 3d (p0 i = 0, pi → 0), (B6) where Γ(3) 4d (p0 i = 0, pi → 0) = G + (4d loops), (B7) Γ(3) 3d (p0 i = 0, pi → 0) = G3 + (3d loops).

Cosmological phase transitions without high-temperature expansions Γ(3) 4d (p0 i = 0, pi → 0) = Γ(3) 3d (p0 i = 0, pi → 0), (B6) where Γ(3) 4d (p0 i = 0, pi → 0) = G + (4d loops), (B7) Γ(3) 3d (p0 i = 0, pi → 0) = G3 + (3d loops)

Reference 10

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Observation 1e2016e9-dc2d-4eb2-bcd0-9585a543a2d6 · outbound

This paper cites (E11) arises from a numerical integration that results from the three-loop calculation of the effective potential [119].

Cosmological phase transitions without high-temperature expansions (E11) arises from a numerical integration that results from the three-loop calculation of the effective potential [119]

Reference 11

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Observation c358ca02-bb66-467d-98e3-1545a0664fa6 · outbound

This paper cites Moreover, since the one-loop contribution at O(α3) is independent of the thermal mass, there is no logarithmic dependence on the 3d scale at three-loop order in the O(α3.

Cosmological phase transitions without high-temperature expansions Moreover, since the one-loop contribution at O(α3) is independent of the thermal mass, there is no logarithmic dependence on the 3d scale at three-loop order in the O(α3

Reference 12

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Observation ef2a5933-927b-4787-8339-73112f04d94e · outbound

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Cosmological phase transitions without high-temperature expansions Unresolved cited work

Reference 13

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Observation d6b18e2a-3f37-4228-ba90-6fd7203a2865 · outbound

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Cosmological phase transitions without high-temperature expansions Unresolved cited work

Reference 14

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Observation 2c0cf78c-324d-42ad-8743-8562d9bdb8cf · outbound

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Cosmological phase transitions without high-temperature expansions Unresolved cited work

Reference 15

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Observation e6756845-2d0e-405a-af0c-b03bef8e1ec0 · outbound

This paper cites Electroweak baryogenesis.

Cosmological phase transitions without high-temperature expansions Electroweak baryogenesis

Reference 16

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Observation 1391ca91-256c-47a8-a369-bd1c343a6946 · outbound

This paper cites Baryogenesis from the weak scale to the grand unification scale.

Cosmological phase transitions without high-temperature expansions Baryogenesis from the weak scale to the grand unification scale

Reference 17

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Observation e2fb74ba-9d2b-468c-b96e-cb19d340bdc2 · outbound

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Cosmological phase transitions without high-temperature expansions Unresolved cited work

Reference 18

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Observation 3dd90d78-6bcc-44b7-83f6-e386e2b01e12 · outbound

This paper cites The Electroweak Phase Transition: A Collider Target.

Cosmological phase transitions without high-temperature expansions The Electroweak Phase Transition: A Collider Target

Reference 19

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Observation 6829f6b2-aa1b-496c-8aec-ac0130c26f92 · outbound

This paper cites Science with the space-based interferometer eLISA. II: Gravitational waves from cosmological phase transitions.

Cosmological phase transitions without high-temperature expansions Science with the space-based interferometer eLISA. II: Gravitational waves from cosmological phase transitions

Reference 20

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Observation 29bab692-c4de-4ae5-b005-ca642204e939 · outbound

This paper cites Detecting gravitational waves from cosmological phase transitions with LISA: an update.

Cosmological phase transitions without high-temperature expansions Detecting gravitational waves from cosmological phase transitions with LISA: an update

Reference 21

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Observation eaadbcb9-b7c7-49d8-98da-3144de94e1a4 · outbound

This paper cites Cosmology with the Laser Interferometer Space Antenna.

Cosmological phase transitions without high-temperature expansions Cosmology with the Laser Interferometer Space Antenna

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Observation 7ee2086a-826d-438b-8061-6dea7220a06b · outbound

This paper cites Laser Interferometer Space Antenna.

Cosmological phase transitions without high-temperature expansions Laser Interferometer Space Antenna

Reference 23

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Observation a7730ebc-bbfc-48f9-840f-50d74ee4ecaf · outbound

This paper cites The Effective Potential and First-Order Phase Transitions: Beyond Leading Order.

Cosmological phase transitions without high-temperature expansions The Effective Potential and First-Order Phase Transitions: Beyond Leading Order

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Observation b52fb3ad-53c6-4b4b-b58c-dd19ae0479b0 · outbound

This paper cites 3D Physics and the Electroweak Phase Transition: Perturbation Theory.

Cosmological phase transitions without high-temperature expansions 3D Physics and the Electroweak Phase Transition: Perturbation Theory

Reference 25

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Observation d1a76b2f-0502-44dd-b382-1807a02696a1 · outbound

This paper cites Effective Field Theory Approach to High-Temperature Thermodynamics.

Cosmological phase transitions without high-temperature expansions Effective Field Theory Approach to High-Temperature Thermodynamics

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Observation 1d862b96-343d-4374-b625-c176c797bb13 · outbound

This paper cites Basics of thermal field theory -- a tutorial on perturbative computations.

Cosmological phase transitions without high-temperature expansions Basics of thermal field theory -- a tutorial on perturbative computations

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Observation 056da6a4-ab34-4f41-9dc0-b6879eb14521 · outbound

This paper cites Chiral gauge theories revisited.

Cosmological phase transitions without high-temperature expansions Chiral gauge theories revisited

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Cosmological phase transitions without high-temperature expansions Dolan and R

Reference 29

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Observation ed44db6e-afd3-4996-af2c-61f7d7f9ecba · outbound

This paper cites Weinberg, Gauge and global symmetries at high tem- perature, Phys.

Cosmological phase transitions without high-temperature expansions Weinberg, Gauge and global symmetries at high tem- perature, Phys

Reference 30

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Cosmological phase transitions without high-temperature expansions Laine and M

Reference 31

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Cosmological phase transitions without high-temperature expansions Unresolved cited work

Reference 32

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Cosmological phase transitions without high-temperature expansions Kajantie, M

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Cosmological phase transitions without high-temperature expansions Appelquist and R

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Cosmological phase transitions without high-temperature expansions The pressure of hot QCD up to g^6 ln(1/g)

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This paper cites How to resum long-distance contributions to the QCD pressure?.

Cosmological phase transitions without high-temperature expansions How to resum long-distance contributions to the QCD pressure?

Reference 37

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Cosmological phase transitions without high-temperature expansions Cool quark matter

Reference 38

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Cosmological phase transitions without high-temperature expansions The Electroweak Phase Transition: A Non-Perturbative Analysis

Reference 39

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This paper cites Is There a Hot Electroweak Phase Transition at $m_H\gsim m_W$?.

Cosmological phase transitions without high-temperature expansions Is There a Hot Electroweak Phase Transition at $m_H\gsim m_W$?

Reference 40

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Cosmological phase transitions without high-temperature expansions Farakos, K

Reference 41

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This paper cites The 2-loop MSSM finite temperature effective potential with stop condensation.

Cosmological phase transitions without high-temperature expansions The 2-loop MSSM finite temperature effective potential with stop condensation

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Cosmological phase transitions without high-temperature expansions High Temperature Dimensional Reduction of the MSSM and other Multi-Scalar Models

Reference 43

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Cosmological phase transitions without high-temperature expansions Supersymmetric Electroweak Phase Transition: Beyond Perturbation Theory

Reference 44

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Cosmological phase transitions without high-temperature expansions Laine, Effective theories of MSSM at high tem- perature, Nucl

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This paper cites Dimensional Reduction of the Two-Higgs Doublet Model at High temperature.

Cosmological phase transitions without high-temperature expansions Dimensional Reduction of the Two-Higgs Doublet Model at High temperature

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Cosmological phase transitions without high-temperature expansions Higgs sector CP-violation at the electroweak phase transition

Reference 47

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Cosmological phase transitions without high-temperature expansions Two Higgs doublet dynamics at the electroweak phase transition: a non-perturbative study

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Cosmological phase transitions without high-temperature expansions Pressure of the Standard Model Near the Electroweak Phase Transition

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Cosmological phase transitions without high-temperature expansions Pressure of the Standard Model at High Temperatures

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Cosmological phase transitions without high-temperature expansions Dimensional reduction of the Standard Model coupled to a new singlet scalar field

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Cosmological phase transitions without high-temperature expansions Nonperturbative Analysis of the Electroweak Phase Transition in the Two Higgs Doublet Model

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Cosmological phase transitions without high-temperature expansions Three-dimensional effective theories for the two Higgs doublet model at high temperature

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Observation efa1334a-d9f0-45a9-b369-fbbc6da118da · outbound

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Cosmological phase transitions without high-temperature expansions Electroweak phase transition in the $\Sigma$SM - I: Dimensional reduction

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Cosmological phase transitions without high-temperature expansions Robust approach to thermal resummation: Standard Model meets a singlet

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Cosmological phase transitions without high-temperature expansions Combining thermal resummation and gauge invariance for electroweak phase transition

Reference 56

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Cosmological phase transitions without high-temperature expansions DRalgo: a package for effective field theory approach for thermal phase transitions

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Observation 48b59a0b-a90c-449f-b3e4-5f913467238e · outbound

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Cosmological phase transitions without high-temperature expansions Speed of sound in cosmological phase transitions and effect on gravitational waves

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Observation 42e96d07-90b4-43f9-87aa-d356ca3f78bf · outbound

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Cosmological phase transitions without high-temperature expansions Strong electroweak phase transition in $t$-channel simplified dark matter models

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Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.049005Z

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Observation d3478eac-862e-4de6-ae8b-0914ffe8b7a7 · outbound

This paper cites Exact relation of lattice and continuum parameters in three-dimensional SU(2)+Higgs theories.

Cosmological phase transitions without high-temperature expansions Exact relation of lattice and continuum parameters in three-dimensional SU(2)+Higgs theories

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.054547Z

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Observation 7cb47bda-e805-42c1-98bd-055ed976e08e · outbound

This paper cites Lattice-continuum relations for 3d SU(N)+Higgs theories.

Cosmological phase transitions without high-temperature expansions Lattice-continuum relations for 3d SU(N)+Higgs theories

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.060959Z

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Observation 8c8f112a-53ad-4df2-860c-37448fdd42ef · outbound

This paper cites Nonperturbative study of the electroweak phase transition in the real scalar singlet extended Standard Model.

Cosmological phase transitions without high-temperature expansions Nonperturbative study of the electroweak phase transition in the real scalar singlet extended Standard Model

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.066652Z

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Observation c5682e99-c54d-4c85-b175-83c02c2f2358 · outbound

This paper cites Perturbative gravitational wave predictions for the real-scalar extended Standard Model.

Cosmological phase transitions without high-temperature expansions Perturbative gravitational wave predictions for the real-scalar extended Standard Model

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.072442Z

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Observation c05593d1-6494-4091-a440-46d3a3d0d59f · outbound

This paper cites Theoretical uncertainties for cosmological first-order phase transitions.

Cosmological phase transitions without high-temperature expansions Theoretical uncertainties for cosmological first-order phase transitions

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.078501Z

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Observation 1b67ffe0-a74e-491f-93d0-14ea5607ba0b · outbound

This paper cites On the perturbative expansion at high temperature and implications for cosmological phase transitions.

Cosmological phase transitions without high-temperature expansions On the perturbative expansion at high temperature and implications for cosmological phase transitions

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.084807Z

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Observation b4e1dfea-f453-4ce1-b056-f4d73cb4dd76 · outbound

This paper cites Effective field theory approach to thermal bubble nucleation.

Cosmological phase transitions without high-temperature expansions Effective field theory approach to thermal bubble nucleation

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.090351Z

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Observation 4b55af85-60bd-41f4-836f-5c3161252d55 · outbound

This paper cites Addressing the Gravitational Wave - Collider Inverse Problem.

Cosmological phase transitions without high-temperature expansions Addressing the Gravitational Wave - Collider Inverse Problem

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.095822Z

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Observation 118669e0-9894-4c5e-b398-69ff5eaa9500 · outbound

This paper cites Gravitational waves from supercooled phase transitions: dimensional transmutation meets dimensional reduction.

Cosmological phase transitions without high-temperature expansions Gravitational waves from supercooled phase transitions: dimensional transmutation meets dimensional reduction

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.101543Z

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Observation d5eedadd-37cb-4353-916e-39d3f5f45e41 · outbound

This paper cites Impact of theoretical uncertainties on model parameter reconstruction from GW signals sourced by cosmological phase transitions.

Cosmological phase transitions without high-temperature expansions Impact of theoretical uncertainties on model parameter reconstruction from GW signals sourced by cosmological phase transitions

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.107125Z

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Observation 86bc2368-b42e-45e2-a90a-265604860a5e · outbound

This paper cites Refining Gravitational Wave and Collider Physics Dialogue via Singlet Scalar Extension.

Cosmological phase transitions without high-temperature expansions Refining Gravitational Wave and Collider Physics Dialogue via Singlet Scalar Extension

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.113497Z

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Observation 7f8830fa-fc90-4723-a44a-6c9ac983759a · outbound

This paper cites Higher-order corrections to phase-transition parameters in dimensional reduction.

Cosmological phase transitions without high-temperature expansions Higher-order corrections to phase-transition parameters in dimensional reduction

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.118984Z

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Observation 029ca06e-8231-4f67-a00a-44dc580057de · outbound

This paper cites The High-Temperature Limit of the SM(EFT).

Cosmological phase transitions without high-temperature expansions The High-Temperature Limit of the SM(EFT)

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.124568Z

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Observation 1849efd4-9c6f-4f35-8057-4fa4b0f2d316 · outbound

This paper cites Kierkla, P.

Cosmological phase transitions without high-temperature expansions Kierkla, P

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.130572Z

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Observation d11b1bbf-f2a8-411e-9c15-8ad2fb1786e6 · outbound

This paper cites Electroweak Bubble Nucleation, Nonperturbatively.

Cosmological phase transitions without high-temperature expansions Electroweak Bubble Nucleation, Nonperturbatively

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.135772Z

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Observation d05d798b-8bb0-47de-b6cf-aa1dbbd64b1c · outbound

This paper cites Non-perturbative computation of the bubble nucleation rate in the cubic anisotropy model.

Cosmological phase transitions without high-temperature expansions Non-perturbative computation of the bubble nucleation rate in the cubic anisotropy model

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.141128Z

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Observation 6997940c-0c08-4b9a-9506-00c91af7264f · outbound

This paper cites Nonperturbative analysis of the gravitational waves from a first-order electroweak phase transition.

Cosmological phase transitions without high-temperature expansions Nonperturbative analysis of the gravitational waves from a first-order electroweak phase transition

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.148059Z

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Observation d6afda27-4553-485f-a896-f7834ce08d87 · outbound

This paper cites First-order electroweak phase transitions: a nonperturbative update.

Cosmological phase transitions without high-temperature expansions First-order electroweak phase transitions: a nonperturbative update

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.153704Z

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Observation 74a70f38-5e62-46cc-9423-da83770e20d0 · outbound

This paper cites Gould, A.

Cosmological phase transitions without high-temperature expansions Gould, A

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.160020Z

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Observation 7fc44fbd-f17d-46e5-9258-4e75281731eb · outbound

This paper cites Expanded ensemble method for bubble nucleation.

Cosmological phase transitions without high-temperature expansions Expanded ensemble method for bubble nucleation

Reference 79

Resolution: verified exact; local_arxiv, observed 2026-08-06T18:56:43.600528Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 0345dd8e-8236-400c-b0ab-ca2eb9f8c1fc · outbound

This paper cites Perturbative effective field theory expansions for cosmological phase transitions.

Cosmological phase transitions without high-temperature expansions Perturbative effective field theory expansions for cosmological phase transitions

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.172182Z

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Observation 60f6d1c8-68c5-49c8-9199-90328e56708a · outbound

This paper cites Radiative first-order phase transitions to next-to-next-to-leading order.

Cosmological phase transitions without high-temperature expansions Radiative first-order phase transitions to next-to-next-to-leading order

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.177295Z

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Observation 21c63632-66a2-4c78-8f4d-c8b2a3fb689d · outbound

This paper cites Cosmological phase transitions at three loops: the final verdict on perturbation theory.

Cosmological phase transitions without high-temperature expansions Cosmological phase transitions at three loops: the final verdict on perturbation theory

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.182782Z

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Observation 826363d2-1856-437e-a32b-8fb9fbe313aa · outbound

This paper cites Linde, Infrared problem in the thermodynamics of the yang-mills gas, Physics Letters B 96, 289 (1980).

Cosmological phase transitions without high-temperature expansions Linde, Infrared problem in the thermodynamics of the yang-mills gas, Physics Letters B 96, 289 (1980)

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.189267Z

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Observation 371df5d6-6876-4211-9918-adb5fa1ce1d1 · outbound

This paper cites Solution to the Perturbative Infrared Catastrophe of Hot Gauge Theories.

Cosmological phase transitions without high-temperature expansions Solution to the Perturbative Infrared Catastrophe of Hot Gauge Theories

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.195271Z

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Observation a17eba7a-40b8-4929-b1a6-30b99a30609d · outbound

This paper cites On the validity of perturbative studies of the electroweak phase transition in the Two Higgs Doublet model.

Cosmological phase transitions without high-temperature expansions On the validity of perturbative studies of the electroweak phase transition in the Two Higgs Doublet model

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.201004Z

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Observation 8b3657cb-3298-4c5a-b825-446eba4c11ec · outbound

This paper cites Real scalar phase transitions: a nonperturbative analysis.

Cosmological phase transitions without high-temperature expansions Real scalar phase transitions: a nonperturbative analysis

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.206487Z

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Observation ee77b7c0-6070-4c65-b0ab-f7e1f12c914f · outbound

This paper cites Higher-dimensional operators at finite-temperature affect gravitational-wave predictions.

Cosmological phase transitions without high-temperature expansions Higher-dimensional operators at finite-temperature affect gravitational-wave predictions

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.212350Z

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Observation 8879698d-88ac-4af8-9659-840782a967cf · outbound

This paper cites Phase Transitions in Dimensional Reduction up to Three Loops.

Cosmological phase transitions without high-temperature expansions Phase Transitions in Dimensional Reduction up to Three Loops

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.217877Z

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Observation 347a2874-496f-4073-b295-3a4e15ac9e68 · outbound

This paper cites Thermal phase transition with full 2-loop effective potential.

Cosmological phase transitions without high-temperature expansions Thermal phase transition with full 2-loop effective potential

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.223572Z

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Observation 8050ac4f-c1e0-45d2-a8f4-0832c214f5ea · outbound

This paper cites Resummation in a Hot Scalar Field Theory.

Cosmological phase transitions without high-temperature expansions Resummation in a Hot Scalar Field Theory

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.228780Z

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Observation 59450568-442b-4a51-a446-c8d985da54a8 · outbound

This paper cites Screened Perturbation Theory.

Cosmological phase transitions without high-temperature expansions Screened Perturbation Theory

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.234634Z

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Observation c8cc9ea6-ede3-45ff-af57-c860c8579c3f · outbound

This paper cites Resummation Methods at Finite Temperature: The Tadpole Way.

Cosmological phase transitions without high-temperature expansions Resummation Methods at Finite Temperature: The Tadpole Way

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.241652Z

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Observation 0fdfb072-3778-473b-946d-91239894d1a2 · outbound

This paper cites Optimized Perturbation Theory at Finite Temperature.

Cosmological phase transitions without high-temperature expansions Optimized Perturbation Theory at Finite Temperature

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.250491Z

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Observation f166920c-93e8-44c8-a274-9c23a2f70702 · outbound

This paper cites Optimized Perturbation Theory at Finite Temperature--- Two-Loop Analysis---.

Cosmological phase transitions without high-temperature expansions Optimized Perturbation Theory at Finite Temperature--- Two-Loop Analysis---

Reference 94

Resolution: verified exact; local_arxiv, observed 2026-08-06T18:56:43.320584Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 89d572ba-0a6e-43ee-945f-06b2cabc74b1 · outbound

This paper cites Scale Invariant Resummed Perturbation at Finite Temperatures.

Cosmological phase transitions without high-temperature expansions Scale Invariant Resummed Perturbation at Finite Temperatures

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.262251Z

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Observation d205a277-9cd2-4d9b-8187-f73b9b4226e0 · outbound

This paper cites Two-loop effective potential, thermal resummation and first-order phase transitions: Beyond the high-temperature expansion.

Cosmological phase transitions without high-temperature expansions Two-loop effective potential, thermal resummation and first-order phase transitions: Beyond the high-temperature expansion

Reference 96

Resolution: verified exact; local_arxiv, observed 2026-08-06T18:56:43.277438Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 094b6626-ef1f-4bae-9b91-4612bf5d3b62 · outbound

This paper cites Thermal Resummation and Phase Transitions.

Cosmological phase transitions without high-temperature expansions Thermal Resummation and Phase Transitions

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.274216Z

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Observation 061af10a-ef8d-45b3-a91c-858191755747 · outbound

This paper cites Gravitational waves and tadpole resummation: Efficient and easy convergence of finite temperature QFT.

Cosmological phase transitions without high-temperature expansions Gravitational waves and tadpole resummation: Efficient and easy convergence of finite temperature QFT

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-06T18:56:41.279539Z

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Observation 5eaecfbb-4fa1-461a-9d4a-861776a2c656 · outbound

This paper cites A renormalization group improvement for thermally resummed effective potential.

Cosmological phase transitions without high-temperature expansions A renormalization group improvement for thermally resummed effective potential

Reference 99

Resolution: verified exact; local_arxiv, observed 2026-08-06T18:56:43.216383Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 95d0fbfb-5aeb-4be7-aa1d-331b71e33184 · outbound

This paper cites Refined renormalization group improvement for thermally resummed effective potential.

Cosmological phase transitions without high-temperature expansions Refined renormalization group improvement for thermally resummed effective potential

Reference 100

Resolution: verified exact; local_arxiv, observed 2026-08-06T18:56:43.190953Z

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Pith citing papers

Observation a1ecda55-3e2a-4b3d-a8de-7091beae9196 · inbound

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Testing the effective action approach to bubble nucleation in holography Cosmological phase transitions without high-temperature expansions

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-06T17:14:14.610307Z

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Observation 8cc3cfa3-7cae-4845-9f23-8e422ba9ba89 · inbound

Hot news on the phase structure of the SMEFT cites this paper.

Hot news on the phase structure of the SMEFT Cosmological phase transitions without high-temperature expansions

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-06T15:08:46.001598Z

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Observation f8d23226-c5da-436f-af9e-9bd4ec95b19f · inbound

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Beyond the Daisy Chain: Running and the 3D EFT View of Supercooled Phase Transitions Cosmological phase transitions without high-temperature expansions

Reference 108

Resolution: unresolved; no resolver link, observed 2026-08-04T00:09:34.663181Z

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Observation e3950273-aa82-45f4-ae9e-7fb362eadd6e · inbound

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Revisiting Singlet Fermion Dark Matter with a Scalar Portal: Connecting Higgs Phenomenology and Strong Electroweak Phase Transition Cosmological phase transitions without high-temperature expansions

Reference 103

Resolution: unresolved; no resolver link, observed 2026-08-03T09:45:02.886970Z

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Observation 70b194d1-9cac-41f9-a821-2bb0753d683a · inbound

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Hard thermal contributions to phase transition observables at NNLO Cosmological phase transitions without high-temperature expansions

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-03T03:46:47.454920Z

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Observation 244d7b67-8817-4905-b083-7539671d341a · inbound

SIRENA -- Sum-Integral REductioN Algorithm cites this paper.

SIRENA -- Sum-Integral REductioN Algorithm Cosmological phase transitions without high-temperature expansions

Reference 78

Resolution: verified exact; arxiv_id, observed 2026-05-11T05:05:58.132425Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 0352ce3c-083a-4bed-8e74-b0291d8ecf98 · inbound

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Matching higher-dimensional operators at finite temperature for general models Cosmological phase transitions without high-temperature expansions

Reference 81

Resolution: verified exact; arxiv_id, observed 2026-05-15T02:58:34.032880Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 685378d7-d4de-4356-b7d2-08ada931f0ee · inbound

Theoretical consistency and phenomenology of supercooled cosmological phase transitions cites this paper.

Theoretical consistency and phenomenology of supercooled cosmological phase transitions Cosmological phase transitions without high-temperature expansions

Reference 99

Resolution: metadata mismatch; arxiv_id, observed 2026-07-04T06:59:38.420565Z

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Observation f9f4cfdf-4bf4-4a6d-b9ba-fc047da14902 · inbound

A critical look at low-scale cosmological phase transitions in the PTA era cites this paper.

A critical look at low-scale cosmological phase transitions in the PTA era Cosmological phase transitions without high-temperature expansions

Reference 211

Resolution: verified exact; arxiv_id, observed 2026-07-03T09:27:48.680114Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation dd82811a-1211-49d3-bf6c-99880b6a135e · inbound

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Consistent Thermal Resummation and Phase Transitions with 2PI Methods Cosmological phase transitions without high-temperature expansions

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-08T00:43:56.828055Z

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