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Paper Citation Record · LEDGER

Effective field theories for dark matter pairs in the early universe: Debye mass effects

As of 11 August 2026, this Paper Citation Record lists 87 of 87 outbound references and 3 inbound Pith citation observations for arXiv:2501.03327.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2501.03327 v2

Coverage vector

measured 87 of 87 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-10T21:59:47.185862Z

measured 90 of 90 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-03T09:23:17.300830Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T09:27:48.804061Z

Reference resolution

87 of 87 outbound references displayed

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  • verified fuzzy4
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External citation measurements

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Outbound references

Observation 58512b07-da22-42d5-b0be-14b2554a4b62 · outbound

This paper cites Zwicky,Die Rotverschiebung von extragalaktischen Nebeln, Helv.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Zwicky,Die Rotverschiebung von extragalaktischen Nebeln, Helv

Reference 1

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Observation bb328b7d-7a07-4776-a823-93ffbbb96507 · outbound

This paper cites Rubin, N.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Rubin, N

Reference 2

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Observation 1c4e8c6f-1848-4e42-8ad8-f3647c2fa795 · outbound

This paper cites A direct empirical proof of the existence of dark matter.

Effective field theories for dark matter pairs in the early universe: Debye mass effects A direct empirical proof of the existence of dark matter

Reference 3

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Observation 0d484d7b-c86b-4560-a6a3-739cf2b4f8ca · outbound

This paper cites Dark Matter Candidates from Particle Physics and Methods of Detection.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Dark Matter Candidates from Particle Physics and Methods of Detection

Reference 4

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Observation 97164199-efee-460a-820a-9b3dd8fe0742 · outbound

This paper cites A History of Dark Matter.

Effective field theories for dark matter pairs in the early universe: Debye mass effects A History of Dark Matter

Reference 5

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Observation 379ac625-9067-4188-874c-fb7acf750a79 · outbound

This paper cites Planck 2018 results. I. Overview and the cosmological legacy of Planck.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Planck 2018 results. I. Overview and the cosmological legacy of Planck

Reference 6

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Observation b7e290d7-b092-474c-b765-30804967dd05 · outbound

This paper cites WIMP dark matter candidates and searches - current status and future prospects.

Effective field theories for dark matter pairs in the early universe: Debye mass effects WIMP dark matter candidates and searches - current status and future prospects

Reference 7

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Observation cdc67e41-aa28-423c-874e-942542a86075 · outbound

This paper cites The moment of truth for WIMP Dark Matter.

Effective field theories for dark matter pairs in the early universe: Debye mass effects The moment of truth for WIMP Dark Matter

Reference 8

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Observation 7a14287b-777d-4b37-bb42-480ff5dc3290 · outbound

This paper cites Gondolo and G.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Gondolo and G

Reference 9

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Observation 5bf8806e-cc9d-4d10-aec9-28ad88f16392 · outbound

This paper cites Griest and D.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Griest and D

Reference 10

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Observation 42eab168-8903-416d-ba01-b87f74839a57 · outbound

This paper cites Sommerfeld,Über die Beugung und Bremsung der Elektronen, Annalen Phys.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Sommerfeld,Über die Beugung und Bremsung der Elektronen, Annalen Phys

Reference 11

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Observation 382b632f-8f5e-44cb-8eb2-b05c1cb36cbe · outbound

This paper cites Non-Perturbative Effect on Dark Matter Annihilation and Gamma Ray Signature from Galactic Center.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Non-Perturbative Effect on Dark Matter Annihilation and Gamma Ray Signature from Galactic Center

Reference 12

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Observation f1f23c9a-f33b-40f8-a652-85c0f5556c19 · outbound

This paper cites Hidden Charged Dark Matter.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Hidden Charged Dark Matter

Reference 13

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Observation ec6f1511-61f4-4ee7-9ae5-eb406539ab9d · outbound

This paper cites Bound-state formation for thermal relic dark matter and unitarity.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Bound-state formation for thermal relic dark matter and unitarity

Reference 14

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Observation 94f96341-a54f-4c3c-9341-a53e222f784e · outbound

This paper cites Heavy neutralino relic abundance with Sommerfeld enhancements - a study of pMSSM scenarios.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Heavy neutralino relic abundance with Sommerfeld enhancements - a study of pMSSM scenarios

Reference 15

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Observation e92249af-2f75-4987-a0d0-14b2f3199b93 · outbound

This paper cites Radiative bound-state-formation cross-sections for dark matter interacting via a Yukawa potential.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Radiative bound-state-formation cross-sections for dark matter interacting via a Yukawa potential

Reference 16

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Observation 957679be-1dfa-414b-ae8b-11877ddd7561 · outbound

This paper cites Kim and M.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Kim and M

Reference 17

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Observation 80da8171-c909-4321-8ce7-4ba7a05962c4 · outbound

This paper cites Relic density of wino-like dark matter in the MSSM.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Relic density of wino-like dark matter in the MSSM

Reference 18

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Observation 96e613a6-fe2f-4a01-88e7-c94cee875be7 · outbound

This paper cites Cosmological Implications of Dark Matter Bound States.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Cosmological Implications of Dark Matter Bound States

Reference 19

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Observation 5688d165-a73b-4b21-a501-8075e7a2b84b · outbound

This paper cites Re-derived overclosure bound for the inert doublet model.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Re-derived overclosure bound for the inert doublet model

Reference 20

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Observation 8baaad89-676d-46bf-b9df-b618f232ae5e · outbound

This paper cites Radiative bound-state formation in unbroken perturbative non-Abelian theories and implications for dark matter.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Radiative bound-state formation in unbroken perturbative non-Abelian theories and implications for dark matter

Reference 21

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Observation a3e6ecbe-67d0-4769-8e63-e5c528bc9937 · outbound

This paper cites Thermal dark matter co-annihilating with a strongly interacting scalar.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Thermal dark matter co-annihilating with a strongly interacting scalar

Reference 22

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Observation ac59627c-a61a-4ca8-8d80-ace2926725a1 · outbound

This paper cites Bound-state effects for dark matter with Higgs-like mediators.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Bound-state effects for dark matter with Higgs-like mediators

Reference 23

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Observation de733e39-6a88-49a4-92ef-9ca1597965c9 · outbound

This paper cites Coloured coannihilations: Dark matter phenomenology meets non-relativistic EFTs.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Coloured coannihilations: Dark matter phenomenology meets non-relativistic EFTs

Reference 24

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Observation c6cff58e-b19b-4082-a8b1-db5d192e02a7 · outbound

This paper cites Dark Matter Sommerfeld-enhanced annihilation and Bound-state decay at finite temperature.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Dark Matter Sommerfeld-enhanced annihilation and Bound-state decay at finite temperature

Reference 25

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Observation b8f1d75e-470b-4c88-b3a9-be04955ac954 · outbound

This paper cites Dark matter bound states via emission of scalar mediators.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Dark matter bound states via emission of scalar mediators

Reference 26

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Observation 5124a650-5ffd-4287-9289-d2d9f9b5d671 · outbound

This paper cites Dark matter bound state formation via emission of a charged scalar.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Dark matter bound state formation via emission of a charged scalar

Reference 27

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Observation c09bdf78-65b6-4232-82ce-12380bef9ed5 · outbound

This paper cites Higgs-mediated bound states in dark-matter models.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Higgs-mediated bound states in dark-matter models

Reference 28

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Observation a51f2316-fe62-4c2b-ace8-2b5627646683 · outbound

This paper cites Rapid bound-state formation of Dark Matter in the Early Universe.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Rapid bound-state formation of Dark Matter in the Early Universe

Reference 29

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Observation 6a3209a8-8ea9-466a-9861-2ab78b0f82e5 · outbound

This paper cites Non-relativistic susceptibility and a dark matter application.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Non-relativistic susceptibility and a dark matter application

Reference 30

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local_arxiv, observed 2026-08-10T21:59:47.985667Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

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Observation 3feb5784-1670-4324-ad00-7e674d3f0677 · outbound

This paper cites Scalar dark matter coannihilating with a coloured fermion.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Scalar dark matter coannihilating with a coloured fermion

Reference 31

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

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Observation d1139c5c-7aa3-4990-84c0-b00f35115e88 · outbound

This paper cites Dark Matter bound-state formation at higher order: a non-equilibrium quantum field theory approach.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Dark Matter bound-state formation at higher order: a non-equilibrium quantum field theory approach

Reference 32

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Observation 5a3bf0d8-8ebb-4807-99a0-fc4a10bd8c99 · outbound

This paper cites Bound-state effects on dark matter coannihilation: Pushing the boundaries of conversion-driven freeze-out.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Bound-state effects on dark matter coannihilation: Pushing the boundaries of conversion-driven freeze-out

Reference 33

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

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Observation 2b8554f6-ef72-4645-b686-dca0a9beeaf8 · outbound

This paper cites Bound-state formation, dissociation and decays of darkonium with potential non-relativistic Yukawa theory for scalar and pseudoscalar mediators.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Bound-state formation, dissociation and decays of darkonium with potential non-relativistic Yukawa theory for scalar and pseudoscalar mediators

Reference 34

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Observation c08f78c1-3463-45d3-ba3f-03c741ba80f2 · outbound

This paper cites Saha equilibrium for metastable bound states and dark matter freeze-out.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Saha equilibrium for metastable bound states and dark matter freeze-out

Reference 35

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local_arxiv, observed 2026-08-10T21:59:47.897131Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

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Observation d0b5c7a8-a0b7-4fdb-b2f9-86301800dba7 · outbound

This paper cites Non-relativistic and potential non-relativistic effective field theories for scalar mediators.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Non-relativistic and potential non-relativistic effective field theories for scalar mediators

Reference 36

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Observation 4b90a331-36bc-4d37-96cc-6de11c6a69cc · outbound

This paper cites Excited bound states and their role in dark matter production.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Excited bound states and their role in dark matter production

Reference 37

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Observation cd0b2d4c-ad57-4a0b-b965-276bd894f342 · outbound

This paper cites Indirect detection of dark matter with (pseudo)-scalar interactions.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Indirect detection of dark matter with (pseudo)-scalar interactions

Reference 38

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source=pdf_text observed=2026-08-10T21:59:46.920045Z digest=sha256:3beee8e3715fb1ccc0a6762e1993233d7e27a66b3860ad0b8904f64272e4d522

Observation 6c618386-328b-41ca-a90b-db7e9fdf73e9 · outbound

This paper cites Effective field theories for dark matter pairs in the early universe: cross sections and widths.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Effective field theories for dark matter pairs in the early universe: cross sections and widths

Reference 39

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source=pdf_text observed=2026-08-10T21:59:46.925198Z digest=sha256:f95c21cbe7440de1505765a2bbf454a04256d9c9cbdcea899c45e6553c4f2b2b

Observation 39f11ac7-d443-410b-b927-9c5d2670a133 · outbound

This paper cites Effective field theories for dark matter pairs in the early universe: center-of-mass recoil effects.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Effective field theories for dark matter pairs in the early universe: center-of-mass recoil effects

Reference 40

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source=pdf_text observed=2026-08-10T21:59:46.930864Z digest=sha256:dd86cd51525a92dd9bd9d7323a91e790c2a05110f544eac2602904afa9174aad

Observation d78ca443-2dc4-42cc-93a0-605e7208bb03 · outbound

This paper cites Neutralino relic density in a Universe with a non-vanishing cosmological constant.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Neutralino relic density in a Universe with a non-vanishing cosmological constant

Reference 41

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source=pdf_text observed=2026-08-10T21:59:46.936483Z digest=sha256:5c2c1370dada2796a41a37d9d47a9be46ccd1d0ae4ca133b2a4b2b5f8540105a

Observation 74fcead7-ddf1-4bdd-b242-50c66ba0a54f · outbound

This paper cites Probing Neutralino Resonance Annihilation via Indirect Detection of Dark Matter.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Probing Neutralino Resonance Annihilation via Indirect Detection of Dark Matter

Reference 42

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source=pdf_text observed=2026-08-10T21:59:46.942147Z digest=sha256:3b17d8273fbee4148e4e0420f1b2c3cd2360ab420995f183d65a752dcef976fe

Observation f6bf5420-4f91-44c3-95a8-8fbac4a3b32b · outbound

This paper cites Minimal Dark Matter.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Minimal Dark Matter

Reference 43

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source=pdf_text observed=2026-08-10T21:59:46.947178Z digest=sha256:ce18045f74ca29b08c6176d882ea927c925c37ed84b892214055cdc08a303ed6

Observation 954fcb80-33be-48cd-8e7d-89159b95fd80 · outbound

This paper cites Non-relativistic pair annihilation of nearly mass degenerate neutralinos and charginos I. General framework and S-wave annihilation.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Non-relativistic pair annihilation of nearly mass degenerate neutralinos and charginos I. General framework and S-wave annihilation

Reference 44

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source=pdf_text observed=2026-08-10T21:59:46.952679Z digest=sha256:84a873568ef4578c65041ab67cb2c1d465c1795b9c519781d9aa45acc1991a26

Observation f1418c7c-29d7-431f-a8da-40b3c5605b49 · outbound

This paper cites Dark sector portal with vector-like leptons and flavor sequestering.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Dark sector portal with vector-like leptons and flavor sequestering

Reference 45

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source=pdf_text observed=2026-08-10T21:59:46.959757Z digest=sha256:407269e5988b7964ece338781e664a77c89595115b45cf521f0c3834cfd6f3cf

Observation 7be79b48-4e73-4409-a9c1-ac741c6e2879 · outbound

This paper cites Neutralino Relic Density including Coannihilations.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Neutralino Relic Density including Coannihilations

Reference 46

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source=pdf_text observed=2026-08-10T21:59:46.965347Z digest=sha256:76d01b21eba8767074f48279f7df6e60ae7f978263de535b53e9e8abe417a8a4

Observation 8b2af471-c1a9-44d7-b012-6ea0ce716a39 · outbound

This paper cites Calculations of Neutralino-Stop Coannihilation in the CMSSM.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Calculations of Neutralino-Stop Coannihilation in the CMSSM

Reference 47

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source=pdf_text observed=2026-08-10T21:59:46.971037Z digest=sha256:186af139f3859064a7752c196f94fecb6bf8c3fd3565d8216b47443062dee8c3

Observation e09386d7-1a15-4ff8-adcd-57ed38c6104d · outbound

This paper cites Non-Simplified SUSY: Stau-Coannihilation at LHC and ILC.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Non-Simplified SUSY: Stau-Coannihilation at LHC and ILC

Reference 48

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source=pdf_text observed=2026-08-10T21:59:46.975397Z digest=sha256:9144da56a85ac00fa05fe3914435f19a902dd83f430f2f2a99fd146809dfc7d7

Observation a713cfc1-2a12-4edf-ac6f-75a5fade4654 · outbound

This paper cites Signatures of Majorana dark matter with t-channel mediators.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Signatures of Majorana dark matter with t-channel mediators

Reference 49

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source=pdf_text observed=2026-08-10T21:59:46.979699Z digest=sha256:fd4b04cfcdf2dfc8d6ad4719ac8f2c699c80240337b9b474c494377afad1152b

Observation 8001db5f-b299-453b-accf-633669a8a7ac · outbound

This paper cites A universal framework for t-channel dark matter models.

Effective field theories for dark matter pairs in the early universe: Debye mass effects A universal framework for t-channel dark matter models

Reference 50

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source=pdf_text observed=2026-08-10T21:59:46.985097Z digest=sha256:32a8d06ee186c0fea1431351245123f560ca427360d8fc47a11884edc4fcf760

Observation c1f37479-ddc0-42ab-8fb5-0d1e6b06b3df · outbound

This paper cites Braaten and R.D.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Braaten and R.D

Reference 51

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source=pdf_text observed=2026-08-10T21:59:46.990063Z digest=sha256:ed30ba14d8904401f88100e29191300ef712da9bb5cfd9bab7a5345f2c553673

Observation a6d218ab-b0b3-40e7-8765-d2532d959c76 · outbound

This paper cites Real-time static potential in hot QCD.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Real-time static potential in hot QCD

Reference 52

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source=pdf_text observed=2026-08-10T21:59:46.995063Z digest=sha256:0a46d267f247da8d05a830d25f48607c334775f9966082c643cb5ad4a09ac475

Observation 7e6a9590-4cba-48b9-9f2d-7efe4a664899 · outbound

This paper cites Thermal imaginary part of a real-time static potential from classical lattice gauge theory simulations.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Thermal imaginary part of a real-time static potential from classical lattice gauge theory simulations

Reference 53

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source=pdf_text observed=2026-08-10T21:59:46.999957Z digest=sha256:5fc764be799443211df76a6fa19bcb698d187200208a1d7ef1f40cbdb8a5452d

Observation 49442f4e-2e82-4f6d-9f30-1df577e1b1a8 · outbound

This paper cites Real and imaginary-time $Q\bar{Q}$ correlators in a thermal medium.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Real and imaginary-time $Q\bar{Q}$ correlators in a thermal medium

Reference 54

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source=pdf_text observed=2026-08-10T21:59:47.005844Z digest=sha256:5fbe8cc95eac48d9d8c928d2c6789e491d403f1ee5613efef9a14928dabcd65e

Observation 9c63b59f-b200-4aa5-b354-3a58e2f132a4 · outbound

This paper cites Static quark-antiquark pairs at finite temperature.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Static quark-antiquark pairs at finite temperature

Reference 55

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source=pdf_text observed=2026-08-10T21:59:47.012465Z digest=sha256:f2e77ccd51a8c196af41ae81d7e5153dd618d43e3079d5103c832ca4470113ca

Observation e3904588-6e7b-4560-80a3-91baa8bdf87f · outbound

This paper cites Non-relativistic bound states at finite temperature (I): the hydrogen atom.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Non-relativistic bound states at finite temperature (I): the hydrogen atom

Reference 56

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source=pdf_text observed=2026-08-10T21:59:47.018295Z digest=sha256:5a9f1d5a6e7effbed606daa2cbd6de1543de584ef6c3276e1a0a5c37142e10f1

Observation 452928a7-1da1-47c1-9c2a-6459c0a08e4f · outbound

This paper cites Non-relativistic bound states at finite temperature (II): the muonic hydrogen.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Non-relativistic bound states at finite temperature (II): the muonic hydrogen

Reference 57

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source=pdf_text observed=2026-08-10T21:59:47.023982Z digest=sha256:4becdfd15b8b88a057dda06c052158d18b359a851868596894da9c1f86dd8b97

Observation 7eb62c0c-3ab2-4c8f-ad44-936b22191dbf · outbound

This paper cites Effective field theories for heavy quarkonium.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Effective field theories for heavy quarkonium

Reference 58

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source=pdf_text observed=2026-08-10T21:59:47.028441Z digest=sha256:0d0e2d410db9c0096b537499ccbd1768f967233f7a97c6449fe02c0caf1c07fe

Observation 146bfb2a-a9bf-4072-b10b-cea1a9c96267 · outbound

This paper cites Extra-weakly Interacting Dark Matter.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Extra-weakly Interacting Dark Matter

Reference 59

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source=pdf_text observed=2026-08-10T21:59:47.040092Z digest=sha256:f15f4f75751deec8812f83110884a3206f8c439707d5f6978a9cb5a5906f3b39

Observation 9eb17aa7-fc2e-4dfc-ab23-f1fa5f3c7de4 · outbound

This paper cites U-boson production in e+e- annihilations, psi and Upsilon decays, and Light Dark Matter.

Effective field theories for dark matter pairs in the early universe: Debye mass effects U-boson production in e+e- annihilations, psi and Upsilon decays, and Light Dark Matter

Reference 60

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source=pdf_text observed=2026-08-10T21:59:47.047545Z digest=sha256:97d560c4d9f7a787332e7b20400f8dfcad018d3aab0825f01cce1d293df191a9

Observation dce16dc7-fcca-4559-b74e-c1e85b87d030 · outbound

This paper cites Naturally Light Hidden Photons in LARGE Volume String Compactifications.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Naturally Light Hidden Photons in LARGE Volume String Compactifications

Reference 61

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source=pdf_text observed=2026-08-10T21:59:47.053628Z digest=sha256:c6bd7c51d588d0b74072e1bc9858c6adca574647f323e2f6ab30f0003e0ccf0a

Observation 5866cc8d-aa9b-44b7-9032-95ebc2d4b6aa · outbound

This paper cites Abelian Hidden Sectors at a GeV.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Abelian Hidden Sectors at a GeV

Reference 62

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source=pdf_text observed=2026-08-10T21:59:47.058643Z digest=sha256:ba1e2ca565ffc8bbbd04f6c9cf7d52d35557d8c60947e4b01d5682084647c8c6

Observation 2e61e5a6-47d5-428d-b9b6-d51a99eba80a · outbound

This paper cites Dark Matter and Dark Forces from a supersymmetric hidden sector.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Dark Matter and Dark Forces from a supersymmetric hidden sector

Reference 63

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source=pdf_text observed=2026-08-10T21:59:47.065343Z digest=sha256:f0074aab4bedcd3da67c46305320169d8e8756e94b0eeda062cbf901985496fc

Observation b0ce28b0-72af-4c80-b542-1b938e645acf · outbound

This paper cites Holdom,Two U(1)’s and Epsilon Charge Shifts, Phys.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Holdom,Two U(1)’s and Epsilon Charge Shifts, Phys

Reference 64

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source=pdf_text observed=2026-08-10T21:59:47.071378Z digest=sha256:e19c548f8cf76e24bb342fde72ffc37ef99767c95d9894179e1b5f5f57a518cf

Observation 631dfb15-c210-4d23-a0f4-ae1b97f51552 · outbound

This paper cites Foot and X.-G.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Foot and X.-G

Reference 65

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raw_fallback, observed 2026-08-10T21:59:48.360787Z

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source=pdf_text observed=2026-08-10T21:59:47.076056Z digest=sha256:379e71eebfa25c302f7c9990a67e4517eba9640031f516cd95e22535ffb2eaea

Observation 1b5d873a-d100-4621-82cb-ab42cb3478ba · outbound

This paper cites Looking for the WIMP Next Door.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Looking for the WIMP Next Door

Reference 66

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source=pdf_text observed=2026-08-10T21:59:47.081130Z digest=sha256:69260f3f358c032c8373f338f512b14f108b1229fcf48eea6d705b592b688518

Observation 2bd0c899-b652-4202-8ba1-650f99ff6cf2 · outbound

This paper cites Caswell and G.P.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Caswell and G.P

Reference 67

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source=pdf_text observed=2026-08-10T21:59:47.085626Z digest=sha256:af6e41581a3bae6c847fde707e5f5b3d702d6d412322f3ba915dea222722b8a6

Observation dda08128-5a7f-411e-b941-b00ef428a83f · outbound

This paper cites Rigorous QCD Analysis of Inclusive Annihilation and Production of Heavy Quarkonium.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Rigorous QCD Analysis of Inclusive Annihilation and Production of Heavy Quarkonium

Reference 68

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source=pdf_text observed=2026-08-10T21:59:47.090653Z digest=sha256:11805f60585339bfff5ea249c57421f6635ce89501a5862d1cb761ad7972c717

Observation 7b6c232f-7c82-47ae-a86b-af07963fcfc3 · outbound

This paper cites Introduction to the NRQCD Factorization Approach to Heavy Quarkonium.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Introduction to the NRQCD Factorization Approach to Heavy Quarkonium

Reference 69

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source=pdf_text observed=2026-08-10T21:59:47.095642Z digest=sha256:fbf8c9c930d3137b2b1be8e0d5dcac9b7cf0e504f799e1887bac3aa7c714fdcf

Observation 21ff4f10-aea6-4639-b4d7-f1231f23fdec · outbound

This paper cites NLO Production and Decay of Quarkonium.

Effective field theories for dark matter pairs in the early universe: Debye mass effects NLO Production and Decay of Quarkonium

Reference 70

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source=pdf_text observed=2026-08-10T21:59:47.100257Z digest=sha256:e93c0c3ef71e2026286fbaa9ebf1cbf6c7f8a67ab36e8f9bcf5e007d0a86dac3

Observation aedb63e3-f555-4d37-9308-288f5100e604 · outbound

This paper cites Matching at one loop for the four-quark operators in NRQCD.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Matching at one loop for the four-quark operators in NRQCD

Reference 71

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source=pdf_text observed=2026-08-10T21:59:47.105248Z digest=sha256:b560cf9cd7f4b919d90c75ce0e10c03b91b74d47a589a06bb939510ed011fc35

Observation 32c6315b-ee83-41a1-9c3a-ee1be978b461 · outbound

This paper cites A theoretical review of heavy quarkonium inclusive decays.

Effective field theories for dark matter pairs in the early universe: Debye mass effects A theoretical review of heavy quarkonium inclusive decays

Reference 72

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local_arxiv, observed 2026-08-10T21:59:47.400414Z

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source=pdf_text observed=2026-08-10T21:59:47.109615Z digest=sha256:c8aba4cd1d0a381581afc4f13b488503e53a4ee3df8d5fecb8ec9c84831b03ae

Observation 5ec8ab01-ea90-4eac-ade4-9ae5896771be · outbound

This paper cites The $\sqrt{m\Lambda_{QCD}$ scale in heavy quarkonium.

Effective field theories for dark matter pairs in the early universe: Debye mass effects The $\sqrt{m\Lambda_{QCD}$ scale in heavy quarkonium

Reference 73

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-10T21:59:47.113926Z digest=sha256:a86b09ce605193620b7e1903be08cb486f77d9944f2b03c528434c94cb4d9d0d

Observation 43bac731-78be-488c-929e-5d7dc28c6569 · outbound

This paper cites Effective Field Theory for Ultrasoft Momenta in NRQCD and NRQED.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Effective Field Theory for Ultrasoft Momenta in NRQCD and NRQED

Reference 74

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Observation 58929f64-6497-42c9-a141-28de8eed0e54 · outbound

This paper cites The Lamb Shift in Dimensional Regularization.

Effective field theories for dark matter pairs in the early universe: Debye mass effects The Lamb Shift in Dimensional Regularization

Reference 75

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Observation d80b861e-81e9-4039-8000-3885463539ef · outbound

This paper cites Bellac,Thermal Field Theory, Cambridge Monographs on Mathematical Physics, Cambridge University Press (3, 2011), 10.1017/CBO9780511721700.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Bellac,Thermal Field Theory, Cambridge Monographs on Mathematical Physics, Cambridge University Press (3, 2011), 10.1017/CBO9780511721700

Reference 76

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Observation a7d449bd-26b9-4e34-b676-4cb61772075c · outbound

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

Effective field theories for dark matter pairs in the early universe: Debye mass effects Basics of thermal field theory -- a tutorial on perturbative computations

Reference 77

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Observation c763f3dd-0b0c-4e28-b752-bfefa30b92e7 · outbound

This paper cites Perturbative Thermal QCD: Formalism and Applications.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Perturbative Thermal QCD: Formalism and Applications

Reference 78

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Observation 0b9b29da-415b-4689-92da-ed118b71fe4b · outbound

This paper cites Heavy Quarkonium in a weakly-coupled quark-gluon plasma below the melting temperature.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Heavy Quarkonium in a weakly-coupled quark-gluon plasma below the melting temperature

Reference 79

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Observation 24253db4-3905-4d56-9733-c78751ee251a · outbound

This paper cites Non-Abelian Electric Field Correlator at NLO for Dark Matter Relic Abundance and Quarkonium Transport.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Non-Abelian Electric Field Correlator at NLO for Dark Matter Relic Abundance and Quarkonium Transport

Reference 80

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Observation a0875dcf-eefb-4a7d-845a-f1265f8305fd · outbound

This paper cites Colour-electric spectral function at next-to-leading order.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Colour-electric spectral function at next-to-leading order

Reference 81

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Observation 9abd1a63-cc8e-4a3d-a1d5-255c8a0f15f4 · outbound

This paper cites Gluino Coannihilation Revisited.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Gluino Coannihilation Revisited

Reference 82

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Observation 07d17c95-0e22-4de1-a534-4f865d5832d2 · outbound

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Effective field theories for dark matter pairs in the early universe: Debye mass effects Unresolved cited work

Reference 83

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Observation 8274f3aa-5951-41c5-a2c0-93c172c06e44 · outbound

This paper cites Power corrections to the HTL effective Lagrangian of QED.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Power corrections to the HTL effective Lagrangian of QED

Reference 84

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Observation 38bdf075-2fcb-407d-ba86-47523e6fbf55 · outbound

This paper cites Thermal width and quarkonium dissociation by inelastic parton scattering.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Thermal width and quarkonium dissociation by inelastic parton scattering

Reference 85

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Observation 5464194b-74df-4f79-ba19-1e45d72f1462 · outbound

This paper cites Equilibrium and Non-Equilibrium Hard Thermal Loop Resummation in the Real Time Formalism.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Equilibrium and Non-Equilibrium Hard Thermal Loop Resummation in the Real Time Formalism

Reference 86

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Observation 7ee13914-b1fe-4d01-b900-d3407d3a4574 · outbound

This paper cites Kobes and G.W.

Effective field theories for dark matter pairs in the early universe: Debye mass effects Kobes and G.W

Reference 87

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Pith citing papers

Observation cee3090c-9fc0-4ef7-9f61-e048fe08edf1 · inbound

Self-consistent computation of pair production from non-relativistic effective field theories in the Keldysh-Schwinger formalism cites this paper.

Self-consistent computation of pair production from non-relativistic effective field theories in the Keldysh-Schwinger formalism Effective field theories for dark matter pairs in the early universe: Debye mass effects

Reference 35

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

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Observation 3beea0a5-9f13-462a-a824-3b6540178ca3 · inbound

Thermal effects on Dark Matter production during cosmic reheating cites this paper.

Thermal effects on Dark Matter production during cosmic reheating Effective field theories for dark matter pairs in the early universe: Debye mass effects

Reference 95

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Observation 469b6a64-83e5-401a-a91f-ae4a13d7ab0e · 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 Effective field theories for dark matter pairs in the early universe: Debye mass effects

Reference 203

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verified exact
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