Pith. sign in

Paper Citation Record · LEDGER

How heavy can dark matter be? Constraining colourful unitarity with SARAH

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2012.09022.

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

pith.paper-citation-record.v1
2012.09022 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T15:04:38.705495Z

measured 0 of 1 external citation measurements

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 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.

source=pdf_text observed=2026-08-07T15:04:38.705495Z digest=sha256:320e95087ca4e318f77de7385d466df3998519add9868dc837ea8e45f46b96a0

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-06-28T05:02:44.747731Z digest=sha256:4327f4c557b638371930b192dc9f8da91c61629cead138f43ad4238f27a8d298