Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos | Paper Citation Record

Observation 7f0bfea3-18a6-4644-8bcc-69b5ec01c880 · outbound

This paper cites Abu-Zayyad et al.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Abu-Zayyad et al

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.234370Z

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Observation 6ea70ef0-872f-40e5-a5f1-ef10566df44e · outbound

This paper cites Ivanov (Telescope Array), PoS ICRC2019, 298 (2020).

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Ivanov (Telescope Array), PoS ICRC2019, 298 (2020)

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.239025Z

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Observation 1045e3b2-94bf-40ae-849e-f673075b8c8f · outbound

This paper cites Abraham et al.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Abraham et al

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.243493Z

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Observation 27bbb690-db4f-4129-b6e5-106937716289 · outbound

This paper cites A Catalog of the Highest-Energy Cosmic Rays Recorded During Phase I of Operation of the Pierre Auger Observatory.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos A Catalog of the Highest-Energy Cosmic Rays Recorded During Phase I of Operation of the Pierre Auger Observatory

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.248053Z

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Observation 3697b339-fc86-43c8-90ed-f3242217662c · outbound

This paper cites An extremely energetic cosmic ray observed by a surface detector array.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos An extremely energetic cosmic ray observed by a surface detector array

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.252997Z

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Observation a7097b4d-bd17-4b2a-9da4-31fd38117f50 · outbound

This paper cites Combined fit of spectrum and composition data as measured by the Pierre Auger Observatory.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Combined fit of spectrum and composition data as measured by the Pierre Auger Observatory

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.257793Z

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Observation fd776de0-6bc4-4ced-833b-d334fcc7f388 · outbound

This paper cites Constraining the sources of ultra-high-energy cosmic rays across and above the ankle with the spectrum and composition data measured at the Pierre Auger Observatory.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Constraining the sources of ultra-high-energy cosmic rays across and above the ankle with the spectrum and composition data measured at the Pierre Auger Observatory

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.262747Z

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Observation 01ef2e44-6fd2-46f9-a596-f421f869d6c9 · outbound

This paper cites an unresolved cited work.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Unresolved cited work

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.267510Z

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Observation befcada7-20f7-4945-ba22-504c09000638 · outbound

This paper cites an unresolved cited work.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Unresolved cited work

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.272582Z

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Observation 77691811-ff08-45cb-8e0d-d39edf47c7a1 · outbound

This paper cites Binary neutron star mergers as the source of the highest energy cosmic rays.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Binary neutron star mergers as the source of the highest energy cosmic rays

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.277142Z

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Observation fe4cd1cf-96d3-4d80-9d3a-9c4a3cb6a0a7 · outbound

This paper cites Ultraheavy Ultrahigh-Energy Cosmic Rays.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Ultraheavy Ultrahigh-Energy Cosmic Rays

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.281802Z

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Observation 0a8cae1d-a83a-4202-9b37-7b105ca9699d · outbound

This paper cites GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.286473Z

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Observation fd8606a5-93cb-442d-9459-bff718fb0508 · outbound

This paper cites Multi-messenger Observations of a Binary Neutron Star Merger.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Multi-messenger Observations of a Binary Neutron Star Merger

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.291350Z

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Observation ebbc91f0-3483-4aec-afb9-9d702e21a254 · outbound

This paper cites Origin of the heavy elements in binary neutron-star mergers from a gravitational wave event.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Origin of the heavy elements in binary neutron-star mergers from a gravitational wave event

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.295622Z

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Observation 78fa20b4-727f-4b28-85fa-1a406adee9bf · outbound

This paper cites Modeling GW170817 based on numerical relativity and its implications.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Modeling GW170817 based on numerical relativity and its implications

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.300198Z

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Observation 385e8bc7-cb05-4398-8c9a-95961bcfb2b3 · outbound

This paper cites Kilonovae.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Kilonovae

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.304963Z

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Observation 5d7623d4-659a-448e-8335-f26b85236759 · outbound

This paper cites Watson et al.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Watson et al

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.309510Z

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Observation d5fa130d-e05c-418f-ab7c-c639497a7415 · outbound

This paper cites A "kilonova" associated with short-duration gamma-ray burst 130603B.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos A "kilonova" associated with short-duration gamma-ray burst 130603B

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.313606Z

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Observation 3d5304c5-6962-46e3-8760-bde890ee2dea · outbound

This paper cites A possible Macronova in the late afterglow of the `long-short' burst GRB 060614.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos A possible Macronova in the late afterglow of the `long-short' burst GRB 060614

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.318164Z

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Observation 60b65dc2-9f09-42c4-a8e3-5ef3b8e07717 · outbound

This paper cites The Macronova in GRB 050709 and the GRB/macronova connection.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos The Macronova in GRB 050709 and the GRB/macronova connection

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.322655Z

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Observation 38ddd2e2-1459-4e96-9064-2504322c9a8b · outbound

This paper cites Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.327264Z

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Observation 01cfa4ef-9f6d-434d-a27f-cecb25119dd0 · outbound

This paper cites Collapsars as a major source of r-process elements.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Collapsars as a major source of r-process elements

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.331696Z

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Observation 1ddb6c89-e154-4171-abec-aaea394477e1 · outbound

This paper cites Origin of the Heaviest Elements: the Rapid Neutron-Capture Process.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Origin of the Heaviest Elements: the Rapid Neutron-Capture Process

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.337159Z

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Observation 3269ae6c-9561-4e6b-a5a5-7bc2a544b04c · outbound

This paper cites Collapsar R-Process Yields Can Reproduce [Eu/Fe] Abundance Scatter in Metal-Poor Stars.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Collapsar R-Process Yields Can Reproduce [Eu/Fe] Abundance Scatter in Metal-Poor Stars

Reference 24

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:41.510122Z

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No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 34748e7d-69ac-4de5-8dd9-1b4bcd08faee · outbound

This paper cites Metallicity-Suppressed Collapsars Cannot be the Dominant r-Process Source in the Milky Way.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Metallicity-Suppressed Collapsars Cannot be the Dominant r-Process Source in the Milky Way

Reference 25

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:41.489048Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation a1850458-cd39-4b6f-9a28-60863b120d0c · outbound

This paper cites Radio Constraints on $r$-process Nucleosynthesis by Collapsars.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Radio Constraints on $r$-process Nucleosynthesis by Collapsars

Reference 26

Resolution: malformed identifier; local_arxiv, observed 2026-08-15T19:10:41.467420Z

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No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 187dc790-77bc-4d58-98b4-c9ef57c196b4 · outbound

This paper cites Signatures of R-process Enrichment in Supernovae from Collapsars.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Signatures of R-process Enrichment in Supernovae from Collapsars

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.355904Z

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Observation 9fd2b3cf-a8e5-4081-8624-4a5ca1e84c86 · outbound

This paper cites Collapsars as Sites of r-process Nucleosynthesis: Systematic Near-Infrared Follow-up of Type Ic-BL Supernovae.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Collapsars as Sites of r-process Nucleosynthesis: Systematic Near-Infrared Follow-up of Type Ic-BL Supernovae

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.360709Z

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Observation 57c9e129-9651-4d39-a4cf-e04c275fd03a · outbound

This paper cites Hydrodynamic mixing of accretion disk outflows in collapsars: implications for r-process signatures.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Hydrodynamic mixing of accretion disk outflows in collapsars: implications for r-process signatures

Reference 29

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:41.417525Z

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No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 8f684aa5-6b4f-4e6f-a040-6e9859bc8ed6 · outbound

This paper cites Photospheric velocity evolution of SN 2020bvc: signature of $r$-process nucleosynthesis from a collapsar.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Photospheric velocity evolution of SN 2020bvc: signature of $r$-process nucleosynthesis from a collapsar

Reference 30

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:41.397303Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 3f2d1660-a1e2-47e0-85e3-4770282225b2 · outbound

This paper cites Collapsar disk outflows II: Heavy element production.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Collapsar disk outflows II: Heavy element production

Reference 31

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:41.377320Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 72656b1a-9710-46db-99cf-e72512de5489 · outbound

This paper cites Neutrinos and nucleosynthesis of elements.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Neutrinos and nucleosynthesis of elements

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.379309Z

Source-reported events for the cited work

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Observation 7607de65-6c59-491f-af65-78eaf0d180e6 · outbound

This paper cites Isotropic Detectable X-ray Counterparts to Gravitational Waves from Neutron Star Binary Mergers.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Isotropic Detectable X-ray Counterparts to Gravitational Waves from Neutron Star Binary Mergers

Reference 33

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:41.341528Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 56444f5e-e431-4990-b048-f2f89efb86b1 · outbound

This paper cites Bimodal Long-Lasting Components in Short Gamma-Ray Bursts: Promising Electromagnetic Counterparts to Neutron Star Binary Mergers.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Bimodal Long-Lasting Components in Short Gamma-Ray Bursts: Promising Electromagnetic Counterparts to Neutron Star Binary Mergers

Reference 34

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:41.318842Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation f6539eea-fc49-4c85-93e4-384b71eaedf5 · outbound

This paper cites High-Energy Neutrino Emission from Short Gamma-Ray Bursts: Prospects for Coincident Detection with Gravitational Waves.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos High-Energy Neutrino Emission from Short Gamma-Ray Bursts: Prospects for Coincident Detection with Gravitational Waves

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.393100Z

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Observation 6bfa141e-3e2b-4a5f-9a61-e047f1335211 · outbound

This paper cites High Energy Neutrinos from Cosmological Gamma-Ray Burst Fireballs.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos High Energy Neutrinos from Cosmological Gamma-Ray Burst Fireballs

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.397301Z

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Observation 5176b2c1-cb73-4acb-81bd-a06e4edf7821 · outbound

This paper cites Neutrino afterglow from Gamma-Ray Bursts: ~10^{18} eV.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Neutrino afterglow from Gamma-Ray Bursts: ~10^{18} eV

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.402153Z

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Observation c0e15a39-d216-4f9d-b829-9eb1a4a8f07b · outbound

This paper cites M´ esz´ aros and E.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos M´ esz´ aros and E

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.406527Z

Source-reported events for the cited work

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Observation 2c9bd65a-ccc9-4fee-ada0-925f2030abad · outbound

This paper cites an unresolved cited work.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Unresolved cited work

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.410704Z

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Observation fd27d617-f246-4dd3-a07a-8e7f8be6da4c · outbound

This paper cites Neutrinos From Individual Gamma-Ray Bursts in the BATSE Catalog.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Neutrinos From Individual Gamma-Ray Bursts in the BATSE Catalog

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.415430Z

Source-reported events for the cited work

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Observation 4635bbef-72ba-4ceb-9308-84202f922384 · outbound

This paper cites High Energy Neutrino Flashes from Far-Ultraviolet and X-ray Flares in Gamma-Ray Bursts.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos High Energy Neutrino Flashes from Far-Ultraviolet and X-ray Flares in Gamma-Ray Bursts

Reference 41

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:41.235126Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 7ac17b65-ff29-4e5e-a33c-4eb7a27dd157 · outbound

This paper cites Murase, K.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Murase, K

Reference 42

Resolution: verified exact; raw_fallback, observed 2026-08-15T19:10:41.214540Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 7b8f1616-f5db-4f16-9b9e-5a7192be24f1 · outbound

This paper cites Neutrino Emission from Gamma-Ray Burst Fireballs, Revised.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Neutrino Emission from Gamma-Ray Burst Fireballs, Revised

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.428863Z

Source-reported events for the cited work

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Observation a0b06adf-e19d-47a0-857a-e95bfdb1a784 · outbound

This paper cites Li, Phys.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Li, Phys

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.433152Z

Source-reported events for the cited work

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Observation 653c21dc-c260-4087-807e-496b6691106b · outbound

This paper cites Model-dependent high-energy neutrino flux from Gamma-Ray Bursts.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Model-dependent high-energy neutrino flux from Gamma-Ray Bursts

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.437753Z

Source-reported events for the cited work

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Observation 22002896-df80-4727-89bb-9371678363b3 · outbound

This paper cites Diffuse PeV neutrinos from gamma-ray bursts.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Diffuse PeV neutrinos from gamma-ray bursts

Reference 46

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:41.115242Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 1f58c837-7f64-41f5-9ff6-6db1381a7471 · outbound

This paper cites Inspecting the supernova gamma-ray burst connection with high-energy neutrinos.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Inspecting the supernova gamma-ray burst connection with high-energy neutrinos

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.449440Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 77059b4d-240a-4d55-86c9-9912e6a499e2 · outbound

This paper cites Bustamante, P.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Bustamante, P

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.454694Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b7eb955d-14d2-4c72-b5c6-3e5865d29102 · outbound

This paper cites Neutrinos from Gamma-ray Bursts.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Neutrinos from Gamma-ray Bursts

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.458862Z

Source-reported events for the cited work

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Observation 76b7cd7c-2dee-4dc4-a3d9-8bec35afa07d · outbound

This paper cites Chen, R.-C.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Chen, R.-C

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.463219Z

Source-reported events for the cited work

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Observation 43abf20b-c635-4f71-9d5b-d04f3e3ec9b7 · outbound

This paper cites R-process beta-decay neutrino flux from binary neutron star mergers and collapsars.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos R-process beta-decay neutrino flux from binary neutron star mergers and collapsars

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.467253Z

Source-reported events for the cited work

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Observation 545e02f7-7c64-4cb9-9135-679303779571 · outbound

This paper cites Casier, Search for High-Energy Neutrino Production in Short Gamma Ray Bursts with the IceCube Neutrino Observatory, Ph.D.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Casier, Search for High-Energy Neutrino Production in Short Gamma Ray Bursts with the IceCube Neutrino Observatory, Ph.D

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.471689Z

Source-reported events for the cited work

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Observation f6e22368-7431-43e3-bd22-de6a85f74f65 · outbound

This paper cites Albert et al.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Albert et al

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.476276Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8c3ac542-21ad-4d5c-b997-f4730181f738 · outbound

This paper cites Search for high-energy neutrinos from GW170817 with Baikal-GVD neutrino telescope.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Search for high-energy neutrinos from GW170817 with Baikal-GVD neutrino telescope

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.480255Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 43f8e018-3db9-4fc4-9c62-7824c43cae18 · outbound

This paper cites High-Energy Neutrinos from Millisecond Magnetars formed from the Merger of Binary Neutron Stars.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos High-Energy Neutrinos from Millisecond Magnetars formed from the Merger of Binary Neutron Stars

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.485100Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8d171c7a-03b7-4ea9-a9ff-7e7c4cccf145 · outbound

This paper cites Expected neutrino fluence from short Gamma-Ray Burst 170817A and off-axis angle constraints.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Expected neutrino fluence from short Gamma-Ray Burst 170817A and off-axis angle constraints

Reference 56

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:40.962760Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation cf6cf7df-9237-42a3-9b5b-4ce47fbce96e · outbound

This paper cites Trans-Ejecta High-Energy Neutrino Emission from Binary Neutron Star Mergers.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Trans-Ejecta High-Energy Neutrino Emission from Binary Neutron Star Mergers

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.493638Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3ea3753d-bd12-42ce-a316-91941a47aa24 · outbound

This paper cites High-energy neutrinos from fallback accretion of binary neutron star merger remnants.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos High-energy neutrinos from fallback accretion of binary neutron star merger remnants

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.497964Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fbe07b3d-101a-4fce-9d08-1548114d30cb · outbound

This paper cites High-energy neutrino emission associated with gravitational-wave signals: effects of cocoon photons and constraints on late-time emission.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos High-energy neutrino emission associated with gravitational-wave signals: effects of cocoon photons and constraints on late-time emission

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.502517Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cc55d917-1fc3-4d12-a182-45083f752d22 · outbound

This paper cites Gravitational wave triggered searches for high-energy neutrinos from binary neutron star mergers: prospects for next generation detectors.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Gravitational wave triggered searches for high-energy neutrinos from binary neutron star mergers: prospects for next generation detectors

Reference 60

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:40.900748Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 9933a5bf-22fd-42ec-b414-dfeae74a827a · outbound

This paper cites Ultrahigh-energy neutrino searches using next-generation gravitational wave detectors at radio neutrino detectors: GRAND, IceCube-Gen2 Radio, and RNO-G.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Ultrahigh-energy neutrino searches using next-generation gravitational wave detectors at radio neutrino detectors: GRAND, IceCube-Gen2 Radio, and RNO-G

Reference 61

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:40.880618Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 6760dd8b-0d71-4970-9287-719982dd407b · outbound

This paper cites Investigating binary-neutron-star mergers as production sites of high-energy neutrinos.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Investigating binary-neutron-star mergers as production sites of high-energy neutrinos

Reference 62

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:40.860334Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation cd3d4874-596c-49ac-b066-87edf00e1539 · outbound

This paper cites The rate, luminosity function and time delay of non-Collapsar short GRBs.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos The rate, luminosity function and time delay of non-Collapsar short GRBs

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.521244Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3f67da6f-c9ee-477f-a947-f024a1f80858 · outbound

This paper cites Short vs. Long Gamma-Ray Bursts: A Comprehensive Study of Energetics and Prompt Gamma-Ray Correlations.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Short vs. Long Gamma-Ray Bursts: A Comprehensive Study of Energetics and Prompt Gamma-Ray Correlations

Reference 64

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:40.824723Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation fe7a902e-c561-4d54-9e54-3e9552d7424f · outbound

This paper cites Short GRBs at the dawn of the gravitational wave era.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Short GRBs at the dawn of the gravitational wave era

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.529828Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 046f3ec1-a292-496a-895e-9e8ae2588750 · outbound

This paper cites X-raying extended emission and rapid decay of short gamma-ray bursts.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos X-raying extended emission and rapid decay of short gamma-ray bursts

Reference 66

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:40.789217Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 2f99f859-e0ab-470f-a1bf-16e97b78c4a7 · outbound

This paper cites Short Gamma-Ray Bursts with Extended Emission Observed with Swift/BAT and Fermi/GBM.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Short Gamma-Ray Bursts with Extended Emission Observed with Swift/BAT and Fermi/GBM

Reference 67

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:40.767489Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 476c188d-edc1-4b10-a161-f6882cd28f43 · outbound

This paper cites Methods and results of an automatic analysis of a complete sample of Swift-XRT observations of GRBs.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Methods and results of an automatic analysis of a complete sample of Swift-XRT observations of GRBs

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.543508Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4a2ed3b4-089d-49f5-be29-438a79c81be9 · outbound

This paper cites Signatures of magnetar central engines in short GRB lightcurves.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Signatures of magnetar central engines in short GRB lightcurves

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.548082Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3737a254-5447-4d2c-90bf-5f6b9e2224e3 · outbound

This paper cites Piran, Rev.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Piran, Rev

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.552244Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 32016eb8-9293-439b-a0bd-e02fbb29c7a7 · outbound

This paper cites M´ esz´ aros, Rep.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos M´ esz´ aros, Rep

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.556332Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4081355d-a9ca-4048-a80c-3c65632b38c1 · outbound

This paper cites Kumar and B.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Kumar and B

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.560636Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5e856a22-7f08-4284-8e91-fcbe97891a98 · outbound

This paper cites Linking extended and plateau emissions of short gamma-ray bursts.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Linking extended and plateau emissions of short gamma-ray bursts

Reference 73

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:40.715883Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 56a85d1e-7dfc-40fc-9e39-b0995fda2a8f · outbound

This paper cites an unresolved cited work.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Unresolved cited work

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.568942Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cec74ef8-d5ae-4ca0-bd50-434c50ec4f04 · outbound

This paper cites Weise, Physics Reports 13, 53 (1974).

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Weise, Physics Reports 13, 53 (1974)

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.573115Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a62b0343-58a8-4ba0-806d-463c313af008 · outbound

This paper cites Arneodo, Phys.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Arneodo, Phys

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.577075Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a54d1e55-d95a-4b0c-a0af-d37b0cd8f659 · outbound

This paper cites Photoproduction off Nuclei and Point-like Photon Interactions Part I: Cross Sections and Nuclear Shadowing.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Photoproduction off Nuclei and Point-like Photon Interactions Part I: Cross Sections and Nuclear Shadowing

Reference 77

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:40.695226Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 7b14c9c1-ec0d-4cb0-91b0-cfc14b60e4a8 · outbound

This paper cites Improved photomeson model for interactions of cosmic ray nuclei.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Improved photomeson model for interactions of cosmic ray nuclei

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.586182Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1e65c9ae-fbef-425c-88c0-c5ca3ba8a2d4 · outbound

This paper cites Monte-Carlo simulations of photohadronic processes in astrophysics.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Monte-Carlo simulations of photohadronic processes in astrophysics

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.591593Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e3d1065d-9cd3-4fb2-bf1d-80930ed8b04a · outbound

This paper cites Proton-nucleus scattering and cross section fluctuations at RHIC and LHC.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Proton-nucleus scattering and cross section fluctuations at RHIC and LHC

Reference 80

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:40.645605Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 37990a9d-6e35-4775-9de1-6096cdda2a5c · outbound

This paper cites Proton-nucleus cross section at high energies.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Proton-nucleus cross section at high energies

Reference 81

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:40.625115Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 6eb6c1ed-ddf6-44ef-ad18-d4d30ce27aad · outbound

This paper cites UHECR escape mechanisms for protons and neutrons from GRBs, and the cosmic ray-neutrino connection.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos UHECR escape mechanisms for protons and neutrons from GRBs, and the cosmic ray-neutrino connection

Reference 82

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:40.603330Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation bb5e2e21-fffc-4f08-b959-101f132144bc · outbound

This paper cites Cosmic-Ray and Neutrino Emission from Gamma-Ray Bursts with a Nuclear Cascade.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Cosmic-Ray and Neutrino Emission from Gamma-Ray Bursts with a Nuclear Cascade

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.609728Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9099de77-9d71-418f-ac1a-fa6070b45758 · outbound

This paper cites UHECR acceleration at GRB internal shocks.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos UHECR acceleration at GRB internal shocks

Reference 84

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:40.566887Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation eabbd75d-03ae-4fd2-aafb-aaa1b43c6e75 · outbound

This paper cites Low-luminosity gamma-ray bursts as the sources of ultrahigh-energy cosmic ray nuclei.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Low-luminosity gamma-ray bursts as the sources of ultrahigh-energy cosmic ray nuclei

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.620185Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 26197859-aa16-4d48-9407-f5956bbeb189 · outbound

This paper cites Ultra High Energy Cosmic Ray Source Models: Successes, Challenges and General Predictions.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Ultra High Energy Cosmic Ray Source Models: Successes, Challenges and General Predictions

Reference 86

Resolution: verified exact; local_arxiv, observed 2026-08-15T19:10:40.529848Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 0e3cae64-adf4-456c-8f5e-1ae5180985f5 · outbound

This paper cites Constraining models for the origin of ultra-high-energy cosmic rays with a novel combined analysis of arrival directions, spectrum, and composition data measured at the Pierre Auger Observatory.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Constraining models for the origin of ultra-high-energy cosmic rays with a novel combined analysis of arrival directions, spectrum, and composition data measured at the Pierre Auger Observatory

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.629440Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 47cf847d-a3e0-413f-8947-98328af36cc3 · outbound

This paper cites Zhang and H.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Zhang and H

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.634099Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2342c2b9-9d83-422e-af57-24efcd807dc6 · outbound

This paper cites an unresolved cited work.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Unresolved cited work

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.638306Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6338039a-837e-4dd0-b6f9-08a3b28260ec · outbound

This paper cites High energy neutrino production in gamma-ray bursts: dependence of the neutrino signal on the jet composition.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos High energy neutrino production in gamma-ray bursts: dependence of the neutrino signal on the jet composition

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.642755Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6aedcf4e-c7ee-4224-8a14-f2b5cbe66de9 · outbound

This paper cites Signature of Collapsars as Sources for High-energy Neutrinos and $r$-process Nuclei.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Signature of Collapsars as Sources for High-energy Neutrinos and $r$-process Nuclei

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.647014Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c9f99afa-f3ac-46b2-af9e-aed666dd358a · outbound

This paper cites A comprehensive guide to the physics and usage of PYTHIA 8.3.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos A comprehensive guide to the physics and usage of PYTHIA 8.3

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.652452Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 432e5eb5-76ae-4a71-a4c4-b7c8f85d0a44 · outbound

This paper cites CUG Scholar.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos CUG Scholar

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.229607Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ed45f3e5-20b8-48f9-8cdc-0606133ef38c · outbound

This paper cites Determining the fraction of cosmic-ray protons at ultra-high energies with cosmogenic neutrinos.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Determining the fraction of cosmic-ray protons at ultra-high energies with cosmogenic neutrinos

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.661576Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a2514952-6258-471d-8b27-d97ae8786960 · outbound

This paper cites Ahlers and F.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Ahlers and F

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.657140Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 48e25fc9-caa4-498d-ad69-0354592479ea · outbound

This paper cites an unresolved cited work.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Unresolved cited work

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.670718Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b18dfcfa-0410-45f6-b2ad-77070d13c94c · outbound

This paper cites Recent cosmogenic neutrino search results with IceCube and prospects with IceCube-Gen2.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Recent cosmogenic neutrino search results with IceCube and prospects with IceCube-Gen2

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.666048Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation efe43af3-52b1-45a6-8b08-e796a3136598 · outbound

This paper cites Charm contribution to ultrahigh-energy neutrinos from newborn magnetars.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Charm contribution to ultrahigh-energy neutrinos from newborn magnetars

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.681633Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 92de376b-25cc-418d-a9a3-2ad5d0a6598b · outbound

This paper cites The Giant Radio Array for Neutrino Detection (GRAND): Science and Design.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos The Giant Radio Array for Neutrino Detection (GRAND): Science and Design

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.675339Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 23f56c41-e4d6-4a54-92d8-aef096c38106 · outbound

This paper cites Over the range of Γ = 100–1000 considered for the PR phase (see Table I), λ = 2Eob A Eob γb/(Γ2mAϵ∆) > 1 and τAγ ∝ Lγ,isoR−1Γ−2 is approximately independent of EA [see Eq.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Over the range of Γ = 100–1000 considered for the PR phase (see Table I), λ = 2Eob A Eob γb/(Γ2mAϵ∆) > 1 and τAγ ∝ Lγ,isoR−1Γ−2 is approximately independent of EA [see Eq

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-15T19:10:39.223217Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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