Can the universe be matter-dominated after a supercooled first-order phase transition? | Paper Citation Record

Observation 4ce8f01b-16f0-4d31-a1bb-99c0cc50f09a · outbound

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

Can the universe be matter-dominated after a supercooled first-order phase transition? Is There a Hot Electroweak Phase Transition at $m_H\gsim m_W$?

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.524788Z

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Observation 8a24cc50-23ac-45b3-98c2-1beef4d9d027 · outbound

This paper cites The order of the quantum chromodynamics transition predicted by the standard model of particle physics.

Can the universe be matter-dominated after a supercooled first-order phase transition? The order of the quantum chromodynamics transition predicted by the standard model of particle physics

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.530766Z

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Observation 9a681540-1d61-405c-ba31-52b8c7be7016 · outbound

This paper cites an unresolved cited work.

Can the universe be matter-dominated after a supercooled first-order phase transition? Unresolved cited work

Reference 3

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Observation 3f5d74a3-9f41-446d-a1e1-a66f36c1c99c · outbound

This paper cites an unresolved cited work.

Can the universe be matter-dominated after a supercooled first-order phase transition? Unresolved cited work

Reference 4

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Observation 3837d2d7-32d2-4450-92dd-e39e6dec810c · outbound

This paper cites an unresolved cited work.

Can the universe be matter-dominated after a supercooled first-order phase transition? Unresolved cited work

Reference 5

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Observation a830fb5e-fe44-46cd-94a0-44b37be45076 · outbound

This paper cites an unresolved cited work.

Can the universe be matter-dominated after a supercooled first-order phase transition? Unresolved cited work

Reference 6

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Observation 92c9ade9-fa0c-456e-aeb3-8efc3cb66333 · outbound

This paper cites Gouttenoire, Beyond the Standard Model Cocktail.

Can the universe be matter-dominated after a supercooled first-order phase transition? Gouttenoire, Beyond the Standard Model Cocktail

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.555468Z

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Observation 18ca16de-c94d-4102-aee0-e659cb9377d3 · outbound

This paper cites an unresolved cited work.

Can the universe be matter-dominated after a supercooled first-order phase transition? Unresolved cited work

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.560268Z

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Observation 36427b95-6df5-448d-84b0-e2f99b4f5bee · outbound

This paper cites Electroweak Bubble Wall Speed Limit.

Can the universe be matter-dominated after a supercooled first-order phase transition? Electroweak Bubble Wall Speed Limit

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.565076Z

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Observation 45549496-02d5-4456-91c0-33368a63126c · outbound

This paper cites Towards an all-orders calculation of the electroweak bubble wall velocity.

Can the universe be matter-dominated after a supercooled first-order phase transition? Towards an all-orders calculation of the electroweak bubble wall velocity

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.569958Z

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Observation 4ccacf4d-6e2c-4ef4-9808-1fea0b1aa231 · outbound

This paper cites Bubble wall velocity: heavy physics effects.

Can the universe be matter-dominated after a supercooled first-order phase transition? Bubble wall velocity: heavy physics effects

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.574955Z

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Observation 623c9734-30d2-4bac-9c36-309648c2b0a8 · outbound

This paper cites Friction pressure on relativistic bubble walls.

Can the universe be matter-dominated after a supercooled first-order phase transition? Friction pressure on relativistic bubble walls

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.580098Z

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Observation 201871e6-32dd-4a9e-976c-bc77d86ad44a · outbound

This paper cites Quantisation Across Bubble Walls and Friction.

Can the universe be matter-dominated after a supercooled first-order phase transition? Quantisation Across Bubble Walls and Friction

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.584826Z

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Observation 027f2343-1a4e-4da1-9da1-28109bf0a294 · outbound

This paper cites Bubble wall dynamics from nonequilibrium quantum field theory.

Can the universe be matter-dominated after a supercooled first-order phase transition? Bubble wall dynamics from nonequilibrium quantum field theory

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.589335Z

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Observation 6a96d2a9-951d-4c47-b747-120b7710720a · outbound

This paper cites Super-cool Dark Matter.

Can the universe be matter-dominated after a supercooled first-order phase transition? Super-cool Dark Matter

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.593728Z

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Observation 778b9fba-4c30-481e-ae00-87dcaad30eb9 · outbound

This paper cites Filtered Dark Matter at a First Order Phase Transition.

Can the universe be matter-dominated after a supercooled first-order phase transition? Filtered Dark Matter at a First Order Phase Transition

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.598277Z

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Observation 5203f113-3c44-4e84-83e9-42c65a0cba83 · outbound

This paper cites Hunting WIMPs with LISA: Correlating dark matter and gravitational wave signals.

Can the universe be matter-dominated after a supercooled first-order phase transition? Hunting WIMPs with LISA: Correlating dark matter and gravitational wave signals

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.603186Z

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Observation eaca4221-0dda-4a32-8c17-874f14e17d4e · outbound

This paper cites Dark matter phase-in: producing feebly-interacting particles after a first-order phase transition.

Can the universe be matter-dominated after a supercooled first-order phase transition? Dark matter phase-in: producing feebly-interacting particles after a first-order phase transition

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.608010Z

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Observation 8be60396-8c79-4b62-b6f2-814a4361e802 · outbound

This paper cites Watkins and L.

Can the universe be matter-dominated after a supercooled first-order phase transition? Watkins and L

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.612835Z

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Observation df8e30e3-8833-4a1c-a342-9323925d5a65 · outbound

This paper cites Preheating and symmetry restoration in collisions of vacuum bubbles.

Can the universe be matter-dominated after a supercooled first-order phase transition? Preheating and symmetry restoration in collisions of vacuum bubbles

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.617003Z

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Observation af8d6750-1c08-46d1-830c-5810b6e4919b · outbound

This paper cites Natural Cold Baryogenesis from Strongly Interacting Electroweak Symmetry Breaking.

Can the universe be matter-dominated after a supercooled first-order phase transition? Natural Cold Baryogenesis from Strongly Interacting Electroweak Symmetry Breaking

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.621277Z

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Observation a31428a1-5bab-4781-8049-b12f33a2f132 · outbound

This paper cites Non-thermal Dark Matter Production from the Electroweak Phase Transition: Multi-TeV WIMPs and "Baby-Zillas".

Can the universe be matter-dominated after a supercooled first-order phase transition? Non-thermal Dark Matter Production from the Electroweak Phase Transition: Multi-TeV WIMPs and "Baby-Zillas"

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.625814Z

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Observation 515628b1-1565-4b4a-9619-e585e8477c99 · outbound

This paper cites On Particle Production from Phase Transition Bubbles.

Can the universe be matter-dominated after a supercooled first-order phase transition? On Particle Production from Phase Transition Bubbles

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.630476Z

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Observation 8e8c7e03-b647-45ee-853a-e810b560704d · outbound

This paper cites Aspects of Particle Production from Bubble Dynamics at a First Order Phase Transition.

Can the universe be matter-dominated after a supercooled first-order phase transition? Aspects of Particle Production from Bubble Dynamics at a First Order Phase Transition

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.635152Z

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Observation 1e1ec310-d154-4777-a9c0-0bbd9f339e5c · outbound

This paper cites Nonthermal Heavy Dark Matter from a First-Order Phase Transition.

Can the universe be matter-dominated after a supercooled first-order phase transition? Nonthermal Heavy Dark Matter from a First-Order Phase Transition

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.639885Z

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Observation 83cff165-bd69-4910-b614-55416a182359 · outbound

This paper cites Bubbletrons: Ultrahigh-Energy Particle Collisions and Heavy Dark Matter at Phase Transitions.

Can the universe be matter-dominated after a supercooled first-order phase transition? Bubbletrons: Ultrahigh-Energy Particle Collisions and Heavy Dark Matter at Phase Transitions

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.645014Z

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Observation d03f8571-43c6-4cc6-a076-142dbaa48962 · outbound

This paper cites Dark Matter Production from Bubble Collisions during a First-Order Phase Transition at the End of Inflation.

Can the universe be matter-dominated after a supercooled first-order phase transition? Dark Matter Production from Bubble Collisions during a First-Order Phase Transition at the End of Inflation

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.649443Z

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Observation ea4b74b7-d8ea-425a-b61b-2a818b045963 · outbound

This paper cites Particle production from bubble collisions.

Can the universe be matter-dominated after a supercooled first-order phase transition? Particle production from bubble collisions

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.654408Z

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Observation faeb2ee3-2e1b-4572-9b48-8e680a7cc854 · outbound

This paper cites Particle productions during collisions of highly boosted bubble walls.

Can the universe be matter-dominated after a supercooled first-order phase transition? Particle productions during collisions of highly boosted bubble walls

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.659199Z

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Observation 0364d068-0d13-463f-8131-4b3ea8fbfa4d · outbound

This paper cites String Fragmentation in Supercooled Confinement and Implications for Dark Matter.

Can the universe be matter-dominated after a supercooled first-order phase transition? String Fragmentation in Supercooled Confinement and Implications for Dark Matter

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.663859Z

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Observation 40c5a446-652e-4cb2-835b-8b8067dca450 · outbound

This paper cites Supercool Composite Dark Matter Beyond 100 TeV.

Can the universe be matter-dominated after a supercooled first-order phase transition? Supercool Composite Dark Matter Beyond 100 TeV

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.668598Z

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Observation 1647a98b-bcc8-4618-93c7-0ad006686190 · outbound

This paper cites Dark Matter production from relativistic bubble walls.

Can the universe be matter-dominated after a supercooled first-order phase transition? Dark Matter production from relativistic bubble walls

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.673119Z

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Observation f887b64c-7445-473f-b7b5-ad100bc2d77f · outbound

This paper cites Hot and heavy dark matter from a weak scale phase transition.

Can the universe be matter-dominated after a supercooled first-order phase transition? Hot and heavy dark matter from a weak scale phase transition

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.677794Z

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Observation 6a30b6df-9154-4b99-bbb2-5422c8413f35 · outbound

This paper cites Heavy Baryon Dark Matter from $SU(N)$ Confinement: Bubble Wall Velocity and Boundary Effects.

Can the universe be matter-dominated after a supercooled first-order phase transition? Heavy Baryon Dark Matter from $SU(N)$ Confinement: Bubble Wall Velocity and Boundary Effects

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.682078Z

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Observation b88e38dd-f3de-4c10-b8c7-7a113c18bffb · outbound

This paper cites Particle shells from relativistic bubble walls.

Can the universe be matter-dominated after a supercooled first-order phase transition? Particle shells from relativistic bubble walls

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.686751Z

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Observation 511a78e7-f5a8-4be1-9374-fd2275bfe7ee · outbound

This paper cites Populating secluded dark sector with ultra-relativistic bubbles.

Can the universe be matter-dominated after a supercooled first-order phase transition? Populating secluded dark sector with ultra-relativistic bubbles

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.690880Z

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Observation ae987e47-5b48-4469-aee7-a82e2d48baa9 · outbound

This paper cites an unresolved cited work.

Can the universe be matter-dominated after a supercooled first-order phase transition? Unresolved cited work

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.695384Z

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Observation b552fa7b-1e40-4447-9503-df4aff6cb08f · outbound

This paper cites Baryogenesis and Gravitational Waves from Runaway Bubble Collisions.

Can the universe be matter-dominated after a supercooled first-order phase transition? Baryogenesis and Gravitational Waves from Runaway Bubble Collisions

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.699598Z

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Observation ac95b639-0c64-4edd-b1a2-41ca315689e1 · outbound

This paper cites Baryogenesis via relativistic bubble walls.

Can the universe be matter-dominated after a supercooled first-order phase transition? Baryogenesis via relativistic bubble walls

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.704403Z

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Observation 0cd4bd61-5c90-467c-bd36-73d2df01ce95 · outbound

This paper cites Baryogenesis via relativistic bubble expansion.

Can the universe be matter-dominated after a supercooled first-order phase transition? Baryogenesis via relativistic bubble expansion

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.709234Z

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Observation 17b8f807-a076-4f9e-a5c8-886cb78cc6b9 · outbound

This paper cites Bubble-assisted Leptogenesis.

Can the universe be matter-dominated after a supercooled first-order phase transition? Bubble-assisted Leptogenesis

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.713464Z

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Observation 886e0c4e-ca29-4165-afdf-31ab4e781a2d · outbound

This paper cites Baryogenesis and Leptogenesis from Supercooled Confinement.

Can the universe be matter-dominated after a supercooled first-order phase transition? Baryogenesis and Leptogenesis from Supercooled Confinement

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.718298Z

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Observation 1560c5ff-0d2f-411a-bf15-e2a31a3bf0a6 · outbound

This paper cites Leptogenesis via Bubble Collisions.

Can the universe be matter-dominated after a supercooled first-order phase transition? Leptogenesis via Bubble Collisions

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.722751Z

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Observation f313c42f-12da-438f-bd5a-d661077265f2 · outbound

This paper cites Cataldi, K.

Can the universe be matter-dominated after a supercooled first-order phase transition? Cataldi, K

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.727214Z

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Observation f3a6533d-e32f-4a7b-8a8d-0dea4981a800 · outbound

This paper cites Ai, High-frequency gravitational waves from a ﬁrst-order phase transitions , Phys.

Can the universe be matter-dominated after a supercooled first-order phase transition? Ai, High-frequency gravitational waves from a ﬁrst-order phase transitions , Phys

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.731591Z

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Observation ff81eec5-4285-4a8b-b114-283297437e63 · outbound

This paper cites an unresolved cited work.

Can the universe be matter-dominated after a supercooled first-order phase transition? Unresolved cited work

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.735855Z

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Observation 03d84d65-fb82-4ad6-b6b5-265e8a338c54 · outbound

This paper cites Sasaki, H.

Can the universe be matter-dominated after a supercooled first-order phase transition? Sasaki, H

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.740197Z

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Observation bc1fd3d8-e16f-4be5-aac4-e2b8d582cbc3 · outbound

This paper cites Constraining first-order phase transitions with curvature perturbations.

Can the universe be matter-dominated after a supercooled first-order phase transition? Constraining first-order phase transitions with curvature perturbations

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.744542Z

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Observation 67632dce-2dd8-4ee0-8b42-352c8f14288b · outbound

This paper cites General relativistic bubble growth in cosmological phase transitions.

Can the universe be matter-dominated after a supercooled first-order phase transition? General relativistic bubble growth in cosmological phase transitions

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.749224Z

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Observation 90c8c3c8-fc9c-448e-93b7-c0dd94fcd89b · outbound

This paper cites Finite Bubble Statistics Constrain Late Cosmological Phase Transitions.

Can the universe be matter-dominated after a supercooled first-order phase transition? Finite Bubble Statistics Constrain Late Cosmological Phase Transitions

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.754013Z

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Observation f7bdc762-e651-49dd-8ced-a8dd6559df7a · outbound

This paper cites Black holes and gravitational waves from slow phase transitions.

Can the universe be matter-dominated after a supercooled first-order phase transition? Black holes and gravitational waves from slow phase transitions

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.758472Z

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Observation ddb9b24c-2392-4356-a77e-843cf2dd84cf · outbound

This paper cites Dark Radiation Isocurvature from Cosmological Phase Transitions.

Can the universe be matter-dominated after a supercooled first-order phase transition? Dark Radiation Isocurvature from Cosmological Phase Transitions

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.762944Z

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Observation 21501903-28ff-4a35-a53b-76dc1205cdd0 · outbound

This paper cites Primordial black holes and curvature perturbations from false vacuum islands.

Can the universe be matter-dominated after a supercooled first-order phase transition? Primordial black holes and curvature perturbations from false vacuum islands

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.767364Z

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Observation 567008e5-c9c0-41c0-8468-3b40a5aac5d5 · outbound

This paper cites Gravitational effects on fluid dynamics in cosmological first-order phase transitions.

Can the universe be matter-dominated after a supercooled first-order phase transition? Gravitational effects on fluid dynamics in cosmological first-order phase transitions

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.771889Z

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Observation f64e5972-22a0-425d-89f6-71a9dc873aed · outbound

This paper cites an unresolved cited work.

Can the universe be matter-dominated after a supercooled first-order phase transition? Unresolved cited work

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.776918Z

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Observation e500d922-3f36-41e0-a05a-dc8f142cb4d0 · outbound

This paper cites Greene, D.

Can the universe be matter-dominated after a supercooled first-order phase transition? Greene, D

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.781089Z

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Observation 9dc89b8b-1f08-403d-9bba-fdc2430125f6 · outbound

This paper cites Kodama, M.

Can the universe be matter-dominated after a supercooled first-order phase transition? Kodama, M

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.785823Z

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Observation cc239c08-7099-41d1-9cde-7bf0d4a41d85 · outbound

This paper cites an unresolved cited work.

Can the universe be matter-dominated after a supercooled first-order phase transition? Unresolved cited work

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.790156Z

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Observation efbf6911-65b5-47bb-8483-1ca5e2574820 · outbound

This paper cites Primordial black hole production during first-order phase transitions.

Can the universe be matter-dominated after a supercooled first-order phase transition? Primordial black hole production during first-order phase transitions

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.794528Z

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Observation 5cceae01-609c-4e67-a2d0-1d5f63a90f80 · outbound

This paper cites Primordial black holes as a probe of strongly first-order electroweak phase transition.

Can the universe be matter-dominated after a supercooled first-order phase transition? Primordial black holes as a probe of strongly first-order electroweak phase transition

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.799218Z

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Observation d10aba4e-fd34-4a02-8bec-b7a249228459 · outbound

This paper cites PBH formation from overdensities in delayed vacuum transitions.

Can the universe be matter-dominated after a supercooled first-order phase transition? PBH formation from overdensities in delayed vacuum transitions

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.803769Z

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Observation e1763091-c3f9-4cb3-95b6-d73317556ff8 · outbound

This paper cites Primordial black holes from strong first-order phase transitions.

Can the universe be matter-dominated after a supercooled first-order phase transition? Primordial black holes from strong first-order phase transitions

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.808144Z

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Observation 245c3d81-d61f-486e-92db-ea7a0d89fa15 · outbound

This paper cites Primordial Black Holes from Supercooled Phase Transitions.

Can the universe be matter-dominated after a supercooled first-order phase transition? Primordial Black Holes from Supercooled Phase Transitions

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.813298Z

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Observation 711d48c5-23bd-4d47-adf5-62299d842681 · outbound

This paper cites Primordial black holes as dark matter: Interferometric tests of phase transition origin.

Can the universe be matter-dominated after a supercooled first-order phase transition? Primordial black holes as dark matter: Interferometric tests of phase transition origin

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.817971Z

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Observation b457e20a-5a6a-4355-bb32-2dc7cf2cedb8 · outbound

This paper cites First-order Phase Transition interpretation of PTA signal produces solar-mass Black Holes.

Can the universe be matter-dominated after a supercooled first-order phase transition? First-order Phase Transition interpretation of PTA signal produces solar-mass Black Holes

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.822799Z

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Observation 0841b523-7f58-45ab-b32f-006d0e40c2bb · outbound

This paper cites Supercooling in Radiative Symmetry Breaking: Theory Extensions, Gravitational Wave Detection and Primordial Black Holes.

Can the universe be matter-dominated after a supercooled first-order phase transition? Supercooling in Radiative Symmetry Breaking: Theory Extensions, Gravitational Wave Detection and Primordial Black Holes

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.827465Z

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Observation 59f72654-452a-49fd-9899-434d44acdb5e · outbound

This paper cites Primordial Black Holes from Conformal Higgs.

Can the universe be matter-dominated after a supercooled first-order phase transition? Primordial Black Holes from Conformal Higgs

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.832122Z

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Observation d89c1af5-4b8c-4b26-93d8-209d9058ee90 · outbound

This paper cites Revisiting formation of primordial black holes in a supercooled first-order phase transition.

Can the universe be matter-dominated after a supercooled first-order phase transition? Revisiting formation of primordial black holes in a supercooled first-order phase transition

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.836726Z

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Observation 7b3ebdd2-6c72-4620-9607-fdbae3952000 · outbound

This paper cites Lewicki, P.

Can the universe be matter-dominated after a supercooled first-order phase transition? Lewicki, P

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.841461Z

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Observation 5264e752-467e-450a-9fa4-9bcb1445b085 · outbound

This paper cites Primordial black holes from slow phase transitions: a model-building perspective.

Can the universe be matter-dominated after a supercooled first-order phase transition? Primordial black holes from slow phase transitions: a model-building perspective

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.845799Z

Source-reported events for the cited work

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Observation 2b371c78-8fc1-457f-81f3-a5f0ad920c2f · outbound

This paper cites Primordial Black Holes from First-Order Phase Transition in the xSM.

Can the universe be matter-dominated after a supercooled first-order phase transition? Primordial Black Holes from First-Order Phase Transition in the xSM

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.850623Z

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Observation a982c04f-31f5-4ff6-9529-1d070c842d3b · outbound

This paper cites Primordial Black Holes and Gravitational Waves in the $U(1)_{B-L}$ Extended Inert Doublet Model: A First-Order Phase Transition Perspective.

Can the universe be matter-dominated after a supercooled first-order phase transition? Primordial Black Holes and Gravitational Waves in the $U(1)_{B-L}$ Extended Inert Doublet Model: A First-Order Phase Transition Perspective

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.855154Z

Source-reported events for the cited work

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Observation 9710d8de-bdc3-451d-bcf4-9b894d384cee · outbound

This paper cites Gravitational waves and black holes from the phase transition in models of dynamical symmetry breaking.

Can the universe be matter-dominated after a supercooled first-order phase transition? Gravitational waves and black holes from the phase transition in models of dynamical symmetry breaking

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.859852Z

Source-reported events for the cited work

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Observation b2acae78-dd36-45fc-b23c-4ba5ab753d23 · outbound

This paper cites Primordial Black Holes (as Dark Matter) from the Supercooled Phase Transitions with Radiative Symmetry Breaking.

Can the universe be matter-dominated after a supercooled first-order phase transition? Primordial Black Holes (as Dark Matter) from the Supercooled Phase Transitions with Radiative Symmetry Breaking

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.864645Z

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Observation 3814d914-6be8-4716-b37f-e05f1bdbae1a · outbound

This paper cites Super-critical primordial black hole formation via delayed first-order electroweak phase transition.

Can the universe be matter-dominated after a supercooled first-order phase transition? Super-critical primordial black hole formation via delayed first-order electroweak phase transition

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.869225Z

Source-reported events for the cited work

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Observation 9561fdaa-bb8b-4877-bcff-d605f9164b92 · outbound

This paper cites Complementary Probes of Warped Extra Dimension: Colliders, Gravitational Waves and Primordial Black Holes from Phase Transitions.

Can the universe be matter-dominated after a supercooled first-order phase transition? Complementary Probes of Warped Extra Dimension: Colliders, Gravitational Waves and Primordial Black Holes from Phase Transitions

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.873915Z

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Observation 4512bf91-7485-4102-819b-faa7e036eb1b · outbound

This paper cites Numerical simulations of density perturbation and gravitational wave production from cosmological first-order phase transition.

Can the universe be matter-dominated after a supercooled first-order phase transition? Numerical simulations of density perturbation and gravitational wave production from cosmological first-order phase transition

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.878438Z

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Observation 1b2b8d0c-6155-4d02-8345-a9d10d463096 · outbound

This paper cites Curvature Perturbations from First-Order Phase Transitions: Implications to Black Holes and Gravitational Waves.

Can the universe be matter-dominated after a supercooled first-order phase transition? Curvature Perturbations from First-Order Phase Transitions: Implications to Black Holes and Gravitational Waves

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.883269Z

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Observation 18c867e4-9564-4adc-a3ac-0b65f74ea7e4 · outbound

This paper cites Wang, Y.-l.

Can the universe be matter-dominated after a supercooled first-order phase transition? Wang, Y.-l

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.888085Z

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Observation 18d20ff0-7c97-4681-a63e-4aff92b7867f · outbound

This paper cites Thermodynamical uncertainties for primordial black holes from cosmological phase transitions.

Can the universe be matter-dominated after a supercooled first-order phase transition? Thermodynamical uncertainties for primordial black holes from cosmological phase transitions

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.892952Z

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Observation e4f1fdd1-5282-4f63-9fdb-a439ed698911 · outbound

This paper cites an unresolved cited work.

Can the universe be matter-dominated after a supercooled first-order phase transition? Unresolved cited work

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.897612Z

Source-reported events for the cited work

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Observation 8017b042-1483-4f01-94a4-d148475bf655 · outbound

This paper cites How large are curvature perturbations from slow first-order phase transitions? A gauge-invariant analysis.

Can the universe be matter-dominated after a supercooled first-order phase transition? How large are curvature perturbations from slow first-order phase transitions? A gauge-invariant analysis

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.903122Z

Source-reported events for the cited work

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Observation 2a8d3075-2800-495e-9757-80656112f7d3 · outbound

This paper cites Numerical simulations of primordial black hole formation via delayed first-order phase transitions.

Can the universe be matter-dominated after a supercooled first-order phase transition? Numerical simulations of primordial black hole formation via delayed first-order phase transitions

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.908037Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 74577814-b31d-496f-9971-bd261348ccbf · outbound

This paper cites Reviving primordial black hole formation in slow first-order phase transitions.

Can the universe be matter-dominated after a supercooled first-order phase transition? Reviving primordial black hole formation in slow first-order phase transitions

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.913113Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 326431e5-afb1-40c7-8678-c38fd0c30388 · outbound

This paper cites Primordial Black Holes from Slow Phase Transitions with Delayed Reheating: A Peak-Theory Approach.

Can the universe be matter-dominated after a supercooled first-order phase transition? Primordial Black Holes from Slow Phase Transitions with Delayed Reheating: A Peak-Theory Approach

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.918138Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b6de498f-91c9-46bb-962c-de2acb8a42c5 · outbound

This paper cites Super-slow phase transition catalyzed by BHs and the birth of baby BHs.

Can the universe be matter-dominated after a supercooled first-order phase transition? Super-slow phase transition catalyzed by BHs and the birth of baby BHs

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.923252Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 129e169b-53bc-49ce-bfcb-cda1feac6421 · outbound

This paper cites an unresolved cited work.

Can the universe be matter-dominated after a supercooled first-order phase transition? Unresolved cited work

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.928490Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 51dcda7d-a434-4db4-8278-246299eb8714 · outbound

This paper cites an unresolved cited work.

Can the universe be matter-dominated after a supercooled first-order phase transition? Unresolved cited work

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.932953Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5f318dad-c797-448f-92fd-5f8a25eee13c · outbound

This paper cites Primordial Black Hole Formation via Inverted Bubble Collapse.

Can the universe be matter-dominated after a supercooled first-order phase transition? Primordial Black Hole Formation via Inverted Bubble Collapse

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.937515Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 582fa0c7-b64e-4359-85eb-e3ac1de24918 · outbound

This paper cites an unresolved cited work.

Can the universe be matter-dominated after a supercooled first-order phase transition? Unresolved cited work

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.942599Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e752d30c-a8c2-4911-9a81-515021b05ba5 · outbound

This paper cites Examining the end of inflation with primordial black holes mass distribution and gravitational waves.

Can the universe be matter-dominated after a supercooled first-order phase transition? Examining the end of inflation with primordial black holes mass distribution and gravitational waves

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.947245Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d8752ffb-5bd2-4e96-b270-5d6077d24010 · outbound

This paper cites Primordial black holes from bubble collisions during a first-order phase transition.

Can the universe be matter-dominated after a supercooled first-order phase transition? Primordial black holes from bubble collisions during a first-order phase transition

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.952137Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 126024c1-47ce-47a5-b2ec-63585857c6ae · outbound

This paper cites Crawford and D.

Can the universe be matter-dominated after a supercooled first-order phase transition? Crawford and D

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.956646Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e1e8272c-8f45-40f1-8b8e-34c1919574ce · outbound

This paper cites Dark Matter as dark dwarfs and other macroscopic objects: multiverse relics?.

Can the universe be matter-dominated after a supercooled first-order phase transition? Dark Matter as dark dwarfs and other macroscopic objects: multiverse relics?

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.960959Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ad8df484-8568-444b-ab00-37a68241609a · outbound

This paper cites Detailed Calculation of Primordial Black Hole Formation During First-Order Cosmological Phase Transitions.

Can the universe be matter-dominated after a supercooled first-order phase transition? Detailed Calculation of Primordial Black Hole Formation During First-Order Cosmological Phase Transitions

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.965756Z

Source-reported events for the cited work

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Observation 7df1dbe7-d823-4599-bbf5-e7bd5792652e · outbound

This paper cites Primordial black holes from a cosmic phase transition: The collapse of Fermi-balls.

Can the universe be matter-dominated after a supercooled first-order phase transition? Primordial black holes from a cosmic phase transition: The collapse of Fermi-balls

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.970816Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 814a20b5-b50e-4ab4-8a01-cd0d1c905b5c · outbound

This paper cites Primordial black holes from an electroweak phase transition.

Can the universe be matter-dominated after a supercooled first-order phase transition? Primordial black holes from an electroweak phase transition

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.975323Z

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Observation af25a6e0-9d99-4cb3-83ad-20d0ea1baf82 · outbound

This paper cites an unresolved cited work.

Can the universe be matter-dominated after a supercooled first-order phase transition? Unresolved cited work

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.979921Z

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Observation c52a5ec3-3aef-4f8f-a219-4b3fecf1a2e3 · outbound

This paper cites an unresolved cited work.

Can the universe be matter-dominated after a supercooled first-order phase transition? Unresolved cited work

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.984273Z

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Observation d7f8090f-4f30-4d1a-8f1c-7d699e95bdba · outbound

This paper cites Magnetic Fields Produced by Phase Transition Bubbles in the Electroweak Phase Transition.

Can the universe be matter-dominated after a supercooled first-order phase transition? Magnetic Fields Produced by Phase Transition Bubbles in the Electroweak Phase Transition

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-01T12:45:38.988628Z

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