pith. sign in
Pith Number

pith:XOVA52VI

pith:2026:XOVA52VI4WRXYDN2VKHAXSO2HM
not attested not anchored not stored refs resolved

Secondary Gravitational Wave Signatures from 5D Rotating Primordial Black Holes in the Dark Dimension

George K. Leontaris, Waqas Ahmed

Rotating five-dimensional primordial black holes produce a stochastic gravitational wave background detectable by LISA and DECIGO that could confirm a micron-scale extra dimension, PBH dark matter, and memory burden suppression.

arxiv:2605.12948 v1 · 2026-05-13 · hep-ph · astro-ph.CO · gr-qc · hep-th

Add to your LaTeX paper
\usepackage{pith}
\pithnumber{XOVA52VI4WRXYDN2VKHAXSO2HM}

Prints a linked badge after your title and injects PDF metadata. Compiles on arXiv. Learn more · Embed verified badge

Record completeness

1 Bitcoin timestamp
2 Internet Archive
3 Author claim open · sign in to claim
4 Citations open
5 Replications open
Portable graph bundle live · download bundle · merged state
The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same current state with the deterministic merge algorithm.

Claims

C1strongest claim

A detection of the predicted gravitational wave background would provide simultaneous evidence for a micron-sized extra dimension, PBH dark matter, and the memory burden effect, offering a decisive test of quantum gravity and extra-dimensional physics.

C2weakest assumption

The assumption of a log-normal primordial power spectrum with fixed σ=1 and f_PBH=1, together with the memory burden exponent p=2 applied to 5D rotating black holes, which directly sets the amplitude and shape of the computed GW spectrum.

C3one line summary

5D rotating PBHs in the Dark Dimension with memory burden produce a stochastic GW background peaking at nHz to Hz frequencies, detectable by future observatories within the mass window 10^10 to 10^21 g.

References

100 extracted · 100 resolved · 0 Pith anchors

[1] Bernard J. Carr and S. W. Hawking. Black holes in the early Universe.Mon. Not. Roy. Astron. Soc., 168:399–415, 1974 1974
[2] Gravitationally collapsed objects of very low mass.Mon 1971
[3] George F. Chapline. Cosmological effects of primordial black holes.Nature, 253(5489):251–252, 1975 1975
[4] Observational evidence for primordial black holes: A positivist perspective.Phys 2024
[5] Revisiting Primordial Black Holes Constraints from Ionization History 2016

Formal links

2 machine-checked theorem links

Receipt and verification
First computed 2026-05-18T03:09:09.448575Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

bbaa0eeaa8e5a37c0dbaaa8e0bc9da3b34341a9da7deeb2d7b8058ee8780b95e

Aliases

arxiv: 2605.12948 · arxiv_version: 2605.12948v1 · doi: 10.48550/arxiv.2605.12948 · pith_short_12: XOVA52VI4WRX · pith_short_16: XOVA52VI4WRXYDN2 · pith_short_8: XOVA52VI
Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/XOVA52VI4WRXYDN2VKHAXSO2HM \
  | jq -c '.canonical_record' \
  | python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: bbaa0eeaa8e5a37c0dbaaa8e0bc9da3b34341a9da7deeb2d7b8058ee8780b95e
Canonical record JSON
{
  "metadata": {
    "abstract_canon_sha256": "c7cd07f0534194ca2090d140b750d700dcd71906877ef30d87a0ecfc8ba1f93a",
    "cross_cats_sorted": [
      "astro-ph.CO",
      "gr-qc",
      "hep-th"
    ],
    "license": "http://creativecommons.org/licenses/by-nc-sa/4.0/",
    "primary_cat": "hep-ph",
    "submitted_at": "2026-05-13T03:31:33Z",
    "title_canon_sha256": "6b3d68baf87d6c89d4510a0e9460d3e20fe8759077f086c4a7dbb90378fd6997"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2605.12948",
    "kind": "arxiv",
    "version": 1
  }
}