Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-03T06:50:36.035421Z
Paper Citation Record · LEDGER
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity
As of 19 August 2026, this Paper Citation Record lists 100 of 122 outbound references and 6 inbound Pith citation observations for arXiv:2601.22219.
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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T15:37:14.155688Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-03T13:08:08.048368Z
Reference resolution
100 of 122 outbound references displayed
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External citation measurements
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Outbound references
Observation 67219c5f-31c8-473c-a9cf-145ccf52150e · outbound
This paper cites Starobinsky,A New Type of Isotropic Cosmological Models Without Singularity,Phys.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Starobinsky,A New Type of Isotropic Cosmological Models Without Singularity,Phys
Reference 1
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Observation 58d722ae-8e00-4ed9-b4a9-beb2233012d6 · outbound
This paper cites Sato,First-order phase transition of a vacuum and the expansion of the Universe,mnras 195(1981) 467.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Sato,First-order phase transition of a vacuum and the expansion of the Universe,mnras 195(1981) 467
Reference 2
- Resolution
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Observation e7d48cd9-00dd-4680-936c-a7920dd9f8fa · outbound
This paper cites Guth,The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems,Phys.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Guth,The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems,Phys
Reference 3
- Resolution
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Observation 6633d380-cb0b-4883-9661-0f6d8020fed2 · outbound
This paper cites Linde,A New Inflationary Universe Scenario: A Possible Solution of the Horizon, Flatness, Homogeneity, Isotropy and Primordial Monopole Problems,Phys.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Linde,A New Inflationary Universe Scenario: A Possible Solution of the Horizon, Flatness, Homogeneity, Isotropy and Primordial Monopole Problems,Phys
Reference 4
- Resolution
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Observation 17096d6e-6ca8-4902-a57b-40e11ea8c6fb · outbound
This paper cites Albrecht and P.J.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Albrecht and P.J
Reference 5
- Resolution
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Unavailable: canonical work link unavailable.
Observation a01292aa-0e33-40e4-a977-462133d6fbd1 · outbound
This paper cites Starobinsky,Spectrum of relict gravitational radiation and the early state of the universe,JETP Lett.30(1979) 682.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Starobinsky,Spectrum of relict gravitational radiation and the early state of the universe,JETP Lett.30(1979) 682
Reference 6
- Resolution
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Observation f940a453-c3a2-4873-b07e-82e40aefaab6 · outbound
This paper cites Mukhanov and G.V.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Mukhanov and G.V
Reference 7
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Observation 17ec9392-0e70-4dab-9027-fffd2b377f73 · outbound
This paper cites Guth and S.Y.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Guth and S.Y
Reference 8
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Observation 8c9696e5-c576-4cfd-89de-07fde81832a2 · outbound
This paper cites Planck 2018 results. X. Constraints on inflation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Planck 2018 results. X. Constraints on inflation
Reference 10
- Resolution
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Observation fe7b95d1-66cd-42ac-8bc8-e96981d1574a · outbound
This paper cites Quantum Discord of Cosmic Inflation: Can we Show that CMB Anisotropies are of Quantum-Mechanical Origin?.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Quantum Discord of Cosmic Inflation: Can we Show that CMB Anisotropies are of Quantum-Mechanical Origin?
Reference 12
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Observation 38e06d55-c740-4fe6-bd46-c159e668e697 · outbound
This paper cites Starobinsky,STOCHASTIC DE SITTER (INFLATIONARY) STAGE IN THE EARLY UNIVERSE,Lect.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Starobinsky,STOCHASTIC DE SITTER (INFLATIONARY) STAGE IN THE EARLY UNIVERSE,Lect
Reference 13
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Observation 1e67daa1-46ca-480d-b1aa-2bac3060209b · outbound
This paper cites Semiclassicality and Decoherence of Cosmological Perturbations.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Semiclassicality and Decoherence of Cosmological Perturbations
Reference 14
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Observation 23dad4a3-91a9-453c-91e1-81e4055db618 · outbound
This paper cites Quantum-to-classical Transition of Cosmological Perturbations for Non-vacuum Initial States.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Quantum-to-classical Transition of Cosmological Perturbations for Non-vacuum Initial States
Reference 15
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Observation a7f9c0b2-5e75-4e04-917b-abd74bc2bdb6 · outbound
This paper cites Quantum-to-classical transition for fluctuations in the early Universe.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Quantum-to-classical transition for fluctuations in the early Universe
Reference 16
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Observation b42c1a35-83b4-4100-ad1c-24abd0373a16 · outbound
This paper cites Why do cosmological perturbations look classical to us?.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Why do cosmological perturbations look classical to us?
Reference 17
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Observation 3e381cc3-90bd-47ed-bc6e-30bd83623e78 · outbound
This paper cites In search of an observational quantum signature of the primordial perturbations in slow-roll and ultra slow-roll inflation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity In search of an observational quantum signature of the primordial perturbations in slow-roll and ultra slow-roll inflation
Reference 18
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Observation c4d592e1-9e4b-4b5d-b394-10a133135eda · outbound
This paper cites Grishchuk and Y.V.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Grishchuk and Y.V
Reference 19
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Observation 3a9c3151-81ed-4ec2-9495-f632a0f3c16b · outbound
This paper cites Canonical transformations and squeezing formalism in cosmology.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Canonical transformations and squeezing formalism in cosmology
Reference 20
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Observation d837e400-1cba-40bd-90df-c95fa4263ee0 · outbound
This paper cites Does inflation squeeze cosmological perturbations?.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Does inflation squeeze cosmological perturbations?
Reference 21
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Observation e06e1bcf-18ca-4a3a-8dc9-9f50b463369e · outbound
This paper cites Minimal decoherence from inflation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Minimal decoherence from inflation
Reference 22
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Observation 48e2f04a-5599-481f-80d1-344dbb2f33e7 · outbound
This paper cites Decoherence due to the Horizon after Inflation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Decoherence due to the Horizon after Inflation
Reference 23
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Observation d23eeaa5-3226-4ff0-b28a-c863650a2b11 · outbound
This paper cites Joos and H.D.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Joos and H.D
Reference 24
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Observation 7efd1c6c-4aee-40ec-abcd-3f0789c82541 · outbound
This paper cites Zurek,Pointer basis of quantum apparatus: Into what mixture does the wave packet collapse?,Phys.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Zurek,Pointer basis of quantum apparatus: Into what mixture does the wave packet collapse?,Phys
Reference 25
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Observation 1984e434-1a3c-403c-8a46-b3dc9962fa04 · outbound
This paper cites Brandenberger, R.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Brandenberger, R
Reference 26
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Observation aabd9d38-7c00-43d3-9a70-d2983363169b · outbound
This paper cites Decoherence during Inflation: the generation of classical inhomogeneities.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Decoherence during Inflation: the generation of classical inhomogeneities
Reference 27
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Observation b1f83629-12da-4695-a809-fc045b8eb84b · outbound
This paper cites On the Decoherence of Primordial Fluctuations During Inflation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity On the Decoherence of Primordial Fluctuations During Inflation
Reference 28
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Observation d8f76f9a-e114-46d7-88bd-a3e4f4185df8 · outbound
This paper cites On the Decoherence of Primordial Fluctuations During Inflation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity On the Decoherence of Primordial Fluctuations During Inflation
Reference 29
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Observation 8280b024-b271-48ad-a2a1-7c3d39d13795 · outbound
This paper cites Quantum Decoherence During Inflation from Gravitational Nonlinearities.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Quantum Decoherence During Inflation from Gravitational Nonlinearities
Reference 30
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Observation 501814e3-6f27-4d5e-b21e-608bdf1f4ade · outbound
This paper cites A cosmological open quantum system.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity A cosmological open quantum system
Reference 31
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Observation 0a0403fa-2393-41e2-83a5-ca4b4103d286 · outbound
This paper cites Observational constraints on quantum decoherence during inflation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Observational constraints on quantum decoherence during inflation
Reference 32
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Observation c1f50eea-2e53-4ba1-94e3-aad28b1b1aff · outbound
This paper cites Non Gaussianities from Quantum Decoherence during Inflation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Non Gaussianities from Quantum Decoherence during Inflation
Reference 33
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Observation 19d1b114-7f24-437b-bcdc-e8aa72400757 · outbound
This paper cites Discord and Decoherence.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Discord and Decoherence
Reference 34
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Observation e6acf084-4f4f-4a06-9278-9cb8325ab883 · outbound
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When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Benchmarking the cosmological master equations
Reference 35
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Observation 03f6eb23-46eb-4182-b5da-b6fad60de518 · outbound
This paper cites Quantum recoherence in the early universe.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Quantum recoherence in the early universe
Reference 36
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Observation 5c1ebd34-1a13-42b2-9863-eb861e8b6aa5 · outbound
This paper cites Cosmic decoherence: primordial power spectra and non-Gaussianities.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Cosmic decoherence: primordial power spectra and non-Gaussianities
Reference 37
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Observation 948180a8-c872-47dd-a65a-5fd4cdb7da0e · outbound
This paper cites Quantum signatures and decoherence during inflation from deep subhorizon perturbations.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Quantum signatures and decoherence during inflation from deep subhorizon perturbations
Reference 38
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Observation 488a0986-28a8-4b79-9262-a26ca2f71bdd · outbound
This paper cites Shortcomings in the Understanding of Why Cosmological Perturbations Look Classical.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Shortcomings in the Understanding of Why Cosmological Perturbations Look Classical
Reference 39
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Observation e0b5f9cc-8014-4ccd-bf57-5b3a064f3061 · outbound
This paper cites Cosmological Inflation and the Quantum Measurement Problem.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Cosmological Inflation and the Quantum Measurement Problem
Reference 40
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Observation f9abbf52-9927-4e4d-ba21-5941c273f14e · outbound
This paper cites The Quantum Information of Cosmological Correlations.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity The Quantum Information of Cosmological Correlations
Reference 41
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Observation fddd76b4-e017-4db4-99b5-2f6371c36c66 · outbound
This paper cites Inflationary spectra and violations of Bell inequalities.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Inflationary spectra and violations of Bell inequalities
Reference 42
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Observation 29365c32-ebb4-40e4-97ed-277165ff1c8f · outbound
This paper cites A model with cosmological Bell inequalities.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity A model with cosmological Bell inequalities
Reference 43
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Observation 461651f7-438f-49bc-8f5f-cd2c433af77b · outbound
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When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Bell's Inequalities for Continuous-Variable Systems in Generic Squeezed States
Reference 44
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Observation 833b7c98-a553-48e6-9cad-7d132b324d30 · outbound
This paper cites Bell violation in the Sky.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Bell violation in the Sky
Reference 45
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Observation 03936768-f4ba-4c96-95fb-25af6b20cfaa · outbound
This paper cites Obstructions to Bell CMB Experiments.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Obstructions to Bell CMB Experiments
Reference 46
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Observation 48e823e5-efbf-405d-897d-8e59e1dc96be · outbound
This paper cites Infinite violation of Bell inequalities in inflation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Infinite violation of Bell inequalities in inflation
Reference 47
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Observation 44b3d312-be7a-40a1-a495-66517c916731 · outbound
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When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Leggett-Garg Inequalities for Squeezed States
Reference 48
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Observation 3476f29a-1bfc-4938-83f3-5bb29166b20c · outbound
This paper cites Bipartite temporal Bell inequalities for two-mode squeezed states.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Bipartite temporal Bell inequalities for two-mode squeezed states
Reference 49
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Observation 26f5489c-bbeb-4c07-b8d4-6882f0cb4534 · outbound
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When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Signals of a Quantum Universe
Reference 50
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Observation 2d104f45-bb62-44a8-9f77-12447fec76d1 · outbound
This paper cites A Flat Space Analogue for the Quantum Origin of Structure.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity A Flat Space Analogue for the Quantum Origin of Structure
Reference 51
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Observation 077038ae-8d38-483c-98f0-70984782eb79 · outbound
This paper cites Quantitative classicality in cosmological interactions during inflation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Quantitative classicality in cosmological interactions during inflation
Reference 52
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Observation 6b016001-9500-458b-9470-9ec234a88af3 · outbound
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When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Belfiglio, R
Reference 53
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Observation ff714898-114d-4a49-8be1-572b89d8a9e5 · outbound
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When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Real-space entanglement of quantum fields
Reference 54
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Observation 8228e3f6-1029-4bf5-86cb-f0f494bcca0e · outbound
This paper cites Real-space entanglement in the Cosmic Microwave Background.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Real-space entanglement in the Cosmic Microwave Background
Reference 55
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When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Real-space Bell inequalities in de Sitter
Reference 56
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Observation 4c3629f1-12dc-40c4-ba4e-240157e7c611 · outbound
This paper cites How ubiquitous is entanglement in quantum field theory?.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity How ubiquitous is entanglement in quantum field theory?
Reference 57
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Observation 9f974f1e-fa8f-4c94-a82e-60b7feafffd8 · outbound
This paper cites Entanglement in Cosmology.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Entanglement in Cosmology
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Observation c038cf2e-3781-476d-bc8e-6089d83e25a1 · outbound
This paper cites Belfiglio, O.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Belfiglio, O
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Observation 39a418b0-cb49-4818-a8d0-aaf7a6d828d0 · outbound
This paper cites Inflation does not create entanglement in local observables.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Inflation does not create entanglement in local observables
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- unresolved
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Observation 49a5f7c2-e51e-4dd9-bd3b-5d9567b0fd56 · outbound
This paper cites Ribes Metidieri,Entangling Stories: Exploring Finite-Dimensional Subsystems in Curved Spacetimes Using Relativistic Quantum Information, Ph.D.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Ribes Metidieri,Entangling Stories: Exploring Finite-Dimensional Subsystems in Curved Spacetimes Using Relativistic Quantum Information, Ph.D
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Source-reported events for the cited work
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Observation 79dff0c6-54f4-4252-b5b9-d844a478ee70 · outbound
This paper cites Ribes-Metidieri, I.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Ribes-Metidieri, I
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- unresolved
- no resolver link, observed 2026-08-03T06:50:31.767300Z
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Observation e37a6a98-bc24-4d13-af79-e78787f7fb87 · outbound
This paper cites Correlation and Entanglement partners in Gaussian systems.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Correlation and Entanglement partners in Gaussian systems
Reference 63
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- unresolved
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Observation 8b189a84-c9cf-4921-82f0-fca91ec74110 · outbound
This paper cites Wigner,On the quantum correction for thermodynamic equilibrium,Phys.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Wigner,On the quantum correction for thermodynamic equilibrium,Phys
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- unresolved
- no resolver link, observed 2026-08-03T06:50:31.887172Z
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Observation 2aeb1156-1482-43b5-b6e8-ea891ca4da90 · outbound
This paper cites Case,Wigner functions and Weyl transforms for pedestrians,American Journal of Physics76(2008) 937.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Case,Wigner functions and Weyl transforms for pedestrians,American Journal of Physics76(2008) 937
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Observation 4002e055-2daa-4896-b42e-6d3e7c95473f · outbound
This paper cites an unresolved cited work.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Unresolved cited work
Reference 66
- Resolution
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Observation caa28685-65e7-4018-a557-3a4f7b8af60a · outbound
This paper cites Revzen, P.A.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Revzen, P.A
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- unresolved
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Observation bb54fa43-68a1-48fe-bff6-77d45e27b74e · outbound
This paper cites Revzen,The wigner function as distribution function,Foundations of Physics36(2006) 546.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Revzen,The wigner function as distribution function,Foundations of Physics36(2006) 546
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- unresolved
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Source-reported events for the cited work
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Observation a69093c1-a093-4612-88a2-e5b668303bf7 · outbound
This paper cites Cosmic Inflation, Quantum Information and the Pioneering Role of John S Bell in Cosmology.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Cosmic Inflation, Quantum Information and the Pioneering Role of John S Bell in Cosmology
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- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 14ae128a-f806-42d0-85b0-90faba38718c · outbound
This paper cites Kenfack and K.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Kenfack and K
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- no resolver link, observed 2026-08-03T06:50:32.513619Z
Source-reported events for the cited work
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Observation 0c543fcf-8f5c-4991-b9fc-18f513faafb9 · outbound
This paper cites Resource theory of quantum non-Gaussianity and Wigner negativity.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Resource theory of quantum non-Gaussianity and Wigner negativity
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Observation 3ec91e98-d6a1-413b-b08b-0d28e34c2b14 · outbound
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When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Hudson,When is the wigner quasi-probability density non-negative?,Reports on Mathematical Physics6(1974) 249
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Source-reported events for the cited work
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Observation bb264bc2-a59f-4121-b6e5-e9a9998fdaf3 · outbound
This paper cites Soto and P.
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- unresolved
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Source-reported events for the cited work
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Observation 0a13a724-a524-41b7-8fb2-860113c11f7b · outbound
This paper cites Haque, G.
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- Resolution
- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5ca6a928-2849-4e3d-8e06-3487fdef3023 · outbound
This paper cites The Effective Field Theory of Inflation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity The Effective Field Theory of Inflation
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- unresolved
- no resolver link, observed 2026-08-03T06:50:33.058779Z
Source-reported events for the cited work
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Observation 777c4a70-eb5b-46df-96b4-d46e28d9dfb2 · outbound
This paper cites Equilateral Non-Gaussianity and New Physics on the Horizon.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Equilateral Non-Gaussianity and New Physics on the Horizon
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- unresolved
- no resolver link, observed 2026-08-03T06:50:33.213496Z
Source-reported events for the cited work
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Observation 1204b45f-fd28-40b7-b192-5b16c1c9eaed · outbound
This paper cites A Goldstone Boson Equivalence for Inflation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity A Goldstone Boson Equivalence for Inflation
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- unresolved
- no resolver link, observed 2026-08-03T06:50:33.330701Z
Source-reported events for the cited work
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Observation 914d1bcd-289a-4a6d-8936-d1236347e6de · outbound
This paper cites Hamiltonians to all Orders in Perturbation Theory and Higher Loop Corrections in Single Field Inflation with PBHs Formation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Hamiltonians to all Orders in Perturbation Theory and Higher Loop Corrections in Single Field Inflation with PBHs Formation
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- unresolved
- no resolver link, observed 2026-08-03T06:50:33.542981Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c5b9ee9e-12f6-4434-8b6e-9dd460af260a · outbound
This paper cites Non-perturbative Wavefunction of the Universe in Inflation with (Resonant) Features.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Non-perturbative Wavefunction of the Universe in Inflation with (Resonant) Features
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- unresolved
- no resolver link, observed 2026-08-03T06:50:33.648304Z
Source-reported events for the cited work
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Observation 1b2984cd-d6ec-4866-ad88-bf399fd25748 · outbound
This paper cites Non-Gaussian features of primordial fluctuations in single field inflationary models.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Non-Gaussian features of primordial fluctuations in single field inflationary models
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- unresolved
- no resolver link, observed 2026-08-03T06:50:33.708970Z
Source-reported events for the cited work
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Observation 386aae92-f30e-444c-aa9d-1031aa13d566 · outbound
This paper cites On the consistency relation of the 3-point function in single field inflation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity On the consistency relation of the 3-point function in single field inflation
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- unresolved
- no resolver link, observed 2026-08-03T06:50:33.794587Z
Source-reported events for the cited work
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Observation 01856394-b2ee-4be9-8458-6eb9a90ce9fd · outbound
This paper cites (Small) Resonant non-Gaussianities: Signatures of a Discrete Shift Symmetry in the Effective Field Theory of Inflation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity (Small) Resonant non-Gaussianities: Signatures of a Discrete Shift Symmetry in the Effective Field Theory of Inflation
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- unresolved
- no resolver link, observed 2026-08-03T06:50:33.908788Z
Source-reported events for the cited work
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Observation bb43a903-9dae-4ced-942b-d627f536638a · outbound
This paper cites Lagrange,Nouvelle m´ ethode pour r´ esoudre des ´ equations litt´ erales par les moyen des s´ eries,M´ em.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Lagrange,Nouvelle m´ ethode pour r´ esoudre des ´ equations litt´ erales par les moyen des s´ eries,M´ em
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- unresolved
- no resolver link, observed 2026-08-03T06:50:34.008958Z
Source-reported events for the cited work
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Observation 50bd2da7-7602-4902-9bde-3f33184d01b6 · outbound
This paper cites Gessel,Lagrange inversion,Journal of Combinatorial Theory, Series A144(2016) 212.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Gessel,Lagrange inversion,Journal of Combinatorial Theory, Series A144(2016) 212
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- unresolved
- no resolver link, observed 2026-08-03T06:50:34.128984Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5c2cc2fa-9a57-4124-a64e-821af8be6fdd · outbound
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When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Starobinsky,Dynamics of Phase Transition in the New Inflationary Universe Scenario and Generation of Perturbations,Phys
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- unresolved
- no resolver link, observed 2026-08-03T06:50:34.195453Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6c3d41da-ad5d-4363-91da-4f21c521dcb5 · outbound
This paper cites Starobinsky,Multicomponent de Sitter (Inflationary) Stages and the Generation of Perturbations,JETP Lett.42(1985) 152.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Starobinsky,Multicomponent de Sitter (Inflationary) Stages and the Generation of Perturbations,JETP Lett.42(1985) 152
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- unresolved
- no resolver link, observed 2026-08-03T06:50:34.305462Z
Source-reported events for the cited work
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Observation e00899e5-eb4b-430a-a58c-6338135360be · outbound
This paper cites A General Analytic Formula for the Spectral Index of the Density Perturbations produced during Inflation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity A General Analytic Formula for the Spectral Index of the Density Perturbations produced during Inflation
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- Resolution
- unresolved
- no resolver link, observed 2026-08-03T06:50:34.412168Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 58d9a16d-ff17-4ef8-ac74-907e1761299b · outbound
This paper cites Super-Horizon Scale Dynamics of Multi-Scalar Inflation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Super-Horizon Scale Dynamics of Multi-Scalar Inflation
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- unresolved
- no resolver link, observed 2026-08-03T06:50:34.529992Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 632de1f6-b706-440a-ae4a-09a9eb28dba0 · outbound
This paper cites A new algorithm for calculating the curvature perturbations in stochastic inflation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity A new algorithm for calculating the curvature perturbations in stochastic inflation
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- unresolved
- no resolver link, observed 2026-08-03T06:50:34.743044Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0c18bcbb-6fe2-40ac-ab7a-475ee967ddcb · outbound
This paper cites Non-perturbative approach for curvature perturbations in stochastic-$\delta N$ formalism.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Non-perturbative approach for curvature perturbations in stochastic-$\delta N$ formalism
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- Resolution
- unresolved
- no resolver link, observed 2026-08-03T06:50:34.826486Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1c99d770-a644-4a9b-af62-e25c827fc6c4 · outbound
This paper cites Correlation Functions in Stochastic Inflation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Correlation Functions in Stochastic Inflation
Reference 92
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T06:50:34.904478Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0f63a678-aa51-4150-91f7-7414ccbb673d · outbound
This paper cites Salopek and J.R.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Salopek and J.R
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- unresolved
- no resolver link, observed 2026-08-03T06:50:34.979723Z
Source-reported events for the cited work
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Observation b3c09102-e855-4a50-b4e2-c94dc06f292a · outbound
This paper cites A new approach to the evolution of cosmological perturbations on large scales.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity A new approach to the evolution of cosmological perturbations on large scales
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- unresolved
- no resolver link, observed 2026-08-03T06:50:35.100925Z
Source-reported events for the cited work
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Observation 7d9b70cc-0a03-4b4b-a7d7-88992f52a44a · outbound
This paper cites Conserved cosmological perturbations.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Conserved cosmological perturbations
Reference 95
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- unresolved
- no resolver link, observed 2026-08-03T06:50:35.238385Z
Source-reported events for the cited work
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Observation 16ded636-c298-4049-99b8-19f9d95a751a · outbound
This paper cites The Separate Universe Approach and the Evolution of Nonlinear Superhorizon Cosmological Perturbations.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity The Separate Universe Approach and the Evolution of Nonlinear Superhorizon Cosmological Perturbations
Reference 96
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- unresolved
- no resolver link, observed 2026-08-03T06:50:35.288471Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7bf35624-f87c-4371-abc4-8277a3659c23 · outbound
This paper cites The inflationary prediction for primordial non-gaussianity.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity The inflationary prediction for primordial non-gaussianity
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- unresolved
- no resolver link, observed 2026-08-03T06:50:35.365595Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 74fa0937-5c31-424e-bbe1-1f126de91c23 · outbound
This paper cites Steinhardt and M.S.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Steinhardt and M.S
Reference 98
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- unresolved
- no resolver link, observed 2026-08-03T06:50:35.438365Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b6556fe4-d65d-4815-a640-e22b9d7e3406 · outbound
This paper cites COBE, Gravitational Waves, Inflation and Extended Inflation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity COBE, Gravitational Waves, Inflation and Extended Inflation
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- unresolved
- no resolver link, observed 2026-08-03T06:50:35.531131Z
Source-reported events for the cited work
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Observation 425facfe-7301-4292-9476-6aadec7b8510 · outbound
This paper cites Formalising the Slow-Roll Approximation in Inflation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Formalising the Slow-Roll Approximation in Inflation
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- unresolved
- no resolver link, observed 2026-08-03T06:50:35.706474Z
Source-reported events for the cited work
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Observation a7481cbc-0c08-410e-8549-fbb58fd52472 · outbound
This paper cites Encyclopaedia Inflationaris.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Encyclopaedia Inflationaris
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- unresolved
- no resolver link, observed 2026-08-03T06:50:35.805726Z
Source-reported events for the cited work
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Observation 7c8c9aa9-0beb-467f-9385-b1bff7146f8f · outbound
This paper cites Horizon crossing and inflation with large \eta.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Horizon crossing and inflation with large \eta
Reference 102
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- unresolved
- no resolver link, observed 2026-08-03T06:50:35.921069Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 240322f7-4315-4902-9a3b-5ccb0e2220df · outbound
This paper cites Ultra Slow-Roll Inflation and the non-Gaussianity Consistency Relation.
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity Ultra Slow-Roll Inflation and the non-Gaussianity Consistency Relation
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- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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Classical and quantum evolution of inflationary fluctuations When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity
Reference 11
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- arxiv_id, observed 2026-07-29T01:24:28.655298Z
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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.
Observation 50b9b8b2-10d7-4236-9827-85d28ee1f5cf · inbound
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A Landscape of Cosmological Decoherence When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity
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- arxiv_id, observed 2026-07-29T01:24:28.655298Z
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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.
Observation ad83a391-e97c-4d0c-a879-0dacb2ab4241 · inbound
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- no resolver link, observed 2026-08-02T12:34:02.227719Z
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Unavailable: canonical work link unavailable.
Observation fef23ce0-0f1a-4cf4-86a9-f549efc761dc · inbound
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Quantum Stochastic Inflation When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity
Reference 28
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- arxiv_id, observed 2026-07-29T01:24:28.655298Z
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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.
Observation 2565b891-b2b7-4ebc-964b-3491b9841e16 · inbound
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Reference 38
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- arxiv_id, observed 2026-07-29T01:24:28.655298Z
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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.
Observation ad7e6258-357c-4ddf-b28b-eee34bda8b36 · inbound
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Tensor Catalyzed Decoherence of Primordial Scalar Fluctuations When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity
Reference 20
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- unresolved
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Source-reported events for the cited work
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