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Paper Citation Record · LEDGER

The abundance of primordial black holes depends on the shape of the inflationary power spectrum

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 18 inbound Pith citation observations for arXiv:1805.04087.

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

pith.paper-citation-record.v1
1805.04087 v4

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 18 of 18 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00

measured 18 of 18 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T11:33:44.675318Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

254
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 339e8327-f161-473b-8519-3423cde76401 · inbound

Constraints on Primordial Black Holes cites this paper.

Constraints on Primordial Black Holes The abundance of primordial black holes depends on the shape of the inflationary power spectrum

Reference 42

Resolution
verified exact
local_arxiv, observed 2026-05-15T02:52:31.983158Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-15T02:52:31.574358Z digest=sha256:c7a81eef0a76dd9c78c8fc52a5dc9f5075433adfc02edc4593eb530e0cdf25fb

Observation 283e8426-731b-454a-9736-4e1358bfc79b · inbound

Primordial Black Holes as Dark Matter: Recent Developments cites this paper.

Primordial Black Holes as Dark Matter: Recent Developments The abundance of primordial black holes depends on the shape of the inflationary power spectrum

Reference 74

Resolution
verified exact
local_arxiv, observed 2026-05-16T12:15:13.411388Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-16T12:15:12.881226Z digest=sha256:8cdb7506067da68c7a209f14444dffba3d0872385c20718eca588514470547c0

Observation ea89f491-a9a9-4199-9ce3-bf64363f4785 · inbound

Tensor induced gravitational waves cites this paper.

Tensor induced gravitational waves The abundance of primordial black holes depends on the shape of the inflationary power spectrum

Reference 124

Resolution
unresolved
no resolver link, observed 2026-08-06T11:33:44.675318Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T11:33:44.675318Z digest=sha256:7b112d880be3cb239e2051abbe4815fe13a105308672168d5f9cd9e1565549da

Observation b1646a84-c972-49f7-bdfa-0cc953a30d11 · inbound

Implications for Pulsar Timing Arrays of Sub-solar Black Hole Detections: From LVK to Einstein Telescope and Cosmic Explorer cites this paper.

Implications for Pulsar Timing Arrays of Sub-solar Black Hole Detections: From LVK to Einstein Telescope and Cosmic Explorer The abundance of primordial black holes depends on the shape of the inflationary power spectrum

Reference 193

Resolution
unresolved
no resolver link, observed 2026-08-05T15:54:21.184918Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T15:54:21.184918Z digest=sha256:ddeedfd083f78cc5ee0a773b5d5685f3fe6e98a424104e1f5657f6feb726334b

Observation 19505c2d-4e65-4e09-85a7-308b39e51535 · inbound

Constraints on Primordial Black Holes from Galactic Diffuse Synchrotron Emissions cites this paper.

Constraints on Primordial Black Holes from Galactic Diffuse Synchrotron Emissions The abundance of primordial black holes depends on the shape of the inflationary power spectrum

Reference 10

Resolution
verified exact
local_arxiv, observed 2026-05-16T11:00:52.249230Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-16T10:58:02.187531Z digest=sha256:2ad05762e1142dacc03c407c264dca78d608e5677d9ad62679c4c1eaa6952c94

Observation 949ce865-9289-453f-8a95-b9144d168bd5 · inbound

Memory-Burden Suppression of Hawking Radiation and Neutrino Constraints on Primordial Black Holes cites this paper.

Memory-Burden Suppression of Hawking Radiation and Neutrino Constraints on Primordial Black Holes The abundance of primordial black holes depends on the shape of the inflationary power spectrum

Reference 16

Resolution
verified exact
arxiv_id, observed 2026-05-11T05:51:09.352545Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-10T17:55:02.157201Z digest=sha256:13e2c9ab7cba17c0cf9f146538ab21025c8e08a92c1870e4c2b8480e04e45c77

Observation 64cc631d-ef97-444e-ba85-7c2aa5e5866f · inbound

Microscopic primordial black holes as macroscopic dark matter from large extra dimensions cites this paper.

Microscopic primordial black holes as macroscopic dark matter from large extra dimensions The abundance of primordial black holes depends on the shape of the inflationary power spectrum

Reference 94

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verified exact
arxiv_id, observed 2026-05-10T10:14:09.758766Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-10T10:13:01.240539Z digest=sha256:38c9c001c5ace1f19ad55cc883e8737aa6d4503adb76920637f679bc4c61402e

Observation 0794fda6-6e9a-47aa-819f-11e1366cf7d6 · inbound

Purely quadratic non-Gaussianity from tachyonic instability: Primordial black holes and scalar-induced gravitational waves cites this paper.

Purely quadratic non-Gaussianity from tachyonic instability: Primordial black holes and scalar-induced gravitational waves The abundance of primordial black holes depends on the shape of the inflationary power spectrum

Reference 153

Resolution
verified exact
arxiv_id, observed 2026-05-10T01:04:50.401060Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-10T00:55:18.764549Z digest=sha256:4fdb99bcaf5c40e82ca1239f2fb98efa7d411c3951f9a1920a1e46d67102e428

Observation 9d2eefac-e3e2-46f7-b899-5bf89345ff4c · inbound

Purely quadratic non-Gaussianity from tachyonic instability: Primordial black holes and scalar-induced gravitational waves cites this paper.

Purely quadratic non-Gaussianity from tachyonic instability: Primordial black holes and scalar-induced gravitational waves The abundance of primordial black holes depends on the shape of the inflationary power spectrum

Reference 153

Resolution
unresolved
no resolver link, observed 2026-08-02T15:57:09.282767Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T15:57:09.282767Z digest=sha256:1b81b196a700ca79ca9b237e308f48a0b56587ddf985bbdf35cc1a157ec53ee7

Observation a97a4194-9461-42e5-a4a5-3a6a362b4a02 · inbound

Primordial black hole dark matter from axion inflation cites this paper.

Primordial black hole dark matter from axion inflation The abundance of primordial black holes depends on the shape of the inflationary power spectrum

Reference 74

Resolution
verified exact
arxiv_id, observed 2026-05-12T09:51:27.020420Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-07T09:07:09.900700Z digest=sha256:ad4e11d55f886cf78dc060bce5ab4a86f9453ba94f6fceabeb172e6ae3440f11

Observation a77928cf-e6ba-40d3-876c-ca44d594c2c5 · inbound

Primordial Black Hole from Tensor-induced Density Fluctuation: First-order Phase Transitions and Domain Walls cites this paper.

Primordial Black Hole from Tensor-induced Density Fluctuation: First-order Phase Transitions and Domain Walls The abundance of primordial black holes depends on the shape of the inflationary power spectrum

Reference 163

Resolution
verified exact
local_arxiv, observed 2026-05-15T02:59:42.033221Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-15T02:53:41.149271Z digest=sha256:1fc6ebba7b2993d8307dd126e15be88d2f662313d01fd7bfe3bb548debfc7c57

Observation e7e8e272-794c-4c8a-9215-dcf4ff3b5837 · inbound

Primordial Black Hole from Tensor-induced Density Fluctuation: First-order Phase Transitions and Domain Walls cites this paper.

Primordial Black Hole from Tensor-induced Density Fluctuation: First-order Phase Transitions and Domain Walls The abundance of primordial black holes depends on the shape of the inflationary power spectrum

Reference 163

Resolution
unresolved
no resolver link, observed 2026-08-02T14:03:44.984176Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T14:03:44.984176Z digest=sha256:b70ad569ea35ab1997e55ee2bf7c9684231ebb3a74e831fdbedb68e7e862c45a

Observation 356bde1c-11bc-49d2-b4bd-654733836d44 · inbound

Primordial Black Hole Triggered Type Ia Supernovae II: Comparison with Supernova Remnants and Galactic Chemical Evolution cites this paper.

Primordial Black Hole Triggered Type Ia Supernovae II: Comparison with Supernova Remnants and Galactic Chemical Evolution The abundance of primordial black holes depends on the shape of the inflationary power spectrum

Reference 146

Resolution
verified exact
local_arxiv, observed 2026-06-27T22:51:22.292173Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:33d2785bfcb608aa2b03e2747181e9f7f259dfea6c9b7ea4b7e27e23e138836a

Observation ee839022-46b7-4c4a-a591-e08e2a84b2af · inbound

Exploring Gravitational Wave Signatures Due to Primordial Non-gaussianity and Large Scale Structure Using SKAO cites this paper.

Exploring Gravitational Wave Signatures Due to Primordial Non-gaussianity and Large Scale Structure Using SKAO The abundance of primordial black holes depends on the shape of the inflationary power spectrum

Reference 261

Resolution
verified exact
local_arxiv, observed 2026-06-27T01:20:21.375324Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:bb323ac020c4f15ed3650a69ff1e0e1bf6ed7841e71e1d5ca17f55c6923da947

Observation 87a88d37-f1b7-4fdb-9b57-38f82d581e04 · inbound

Compaction function in stochastic inflation: a \texttt{FOREST} of type I and II primordial black holes cites this paper.

Compaction function in stochastic inflation: a \texttt{FOREST} of type I and II primordial black holes The abundance of primordial black holes depends on the shape of the inflationary power spectrum

Reference 82

Resolution
verified exact
local_arxiv, observed 2026-06-30T14:24:45.671366Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-06-30T05:26:28.825729Z digest=sha256:4cba53ea0c884899a11eae7da83c0233afc06e03a938c9c1009bb3722cde64ce

Observation a204584a-fa39-47bf-94a8-bbd2eee173dc · inbound

The statistics of curvature-profile dispersion in primordial black hole formation cites this paper.

The statistics of curvature-profile dispersion in primordial black hole formation The abundance of primordial black holes depends on the shape of the inflationary power spectrum

Reference 40

Resolution
verified exact
local_arxiv, observed 2026-07-10T02:26:42.913493Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-07-10T02:22:09.448925Z digest=sha256:f648d9c894d214a2b1071da3046020468c855c0563c477c07ff916565e49476c

Observation a6f56b4c-5cd4-456d-b8de-091064b1dc1d · inbound

The statistics of curvature-profile dispersion in primordial black hole formation cites this paper.

The statistics of curvature-profile dispersion in primordial black hole formation The abundance of primordial black holes depends on the shape of the inflationary power spectrum

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-02T07:53:09.291546Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T07:53:09.291546Z digest=sha256:ac93b2ac8ba9ca84b532726b860affc4b4a5c49ffbd048608260775eae002ae2

Observation cdc8a3d1-7451-4f3e-9c15-98a3bec56b9a · inbound

Scalar-induced gravitational waves from a box-shaped curvature power spectrum cites this paper.

Scalar-induced gravitational waves from a box-shaped curvature power spectrum The abundance of primordial black holes depends on the shape of the inflationary power spectrum

Reference 47

Resolution
unresolved
no resolver link, observed 2026-07-14T09:40:09.826288Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T09:40:09.826288Z digest=sha256:084620c2330536cabc74c5ee381e6eab4acd961c33f2d86c85bdcddd94734a33