Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
How heavy can dark matter be? Constraining colourful unitarity with SARAH
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2012.09022.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T05:22:16.374577Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-02T10:26:52.216476Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 62ff43a1-ceae-4e5f-a674-e10a59be38b4 · inbound
Interplay of $95$ GeV Diphoton Excess and Dark Matter in Supersymmetric Triplet Model cites this paper.
Interplay of $95$ GeV Diphoton Excess and Dark Matter in Supersymmetric Triplet Model How heavy can dark matter be? Constraining colourful unitarity with SARAH
Reference 116
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T05:22:16.374577Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cd7a410d-6907-4fe0-a65e-0c308c80d7ce · inbound
The Simplest Dark Matter Model at the Edge of Perturbativity cites this paper.
The Simplest Dark Matter Model at the Edge of Perturbativity How heavy can dark matter be? Constraining colourful unitarity with SARAH
Reference 36
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T00:59:20.046855Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e9d83e59-9f4b-44dd-9b3d-b2c5f7672df7 · inbound
Unveiling the inert Triplet desert region with a pNGB Dark Matter and its Gravitational Wave signatures cites this paper.
Unveiling the inert Triplet desert region with a pNGB Dark Matter and its Gravitational Wave signatures How heavy can dark matter be? Constraining colourful unitarity with SARAH
Reference 150
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T15:04:38.705495Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 18b3a844-a331-4ca6-ada1-6bedd87640c7 · inbound
BSMArt 2: simpler and faster parameter space scans cites this paper.
BSMArt 2: simpler and faster parameter space scans How heavy can dark matter be? Constraining colourful unitarity with SARAH
Reference 56
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T10:26:52.218079Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.