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pith:K3CQSV3U

pith:2026:K3CQSV3UZ44UJ7UIBX7LO2RURC
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Radioactive Source Seeking using Bayesian Optimisation with Movement Penalty

Airlie Chapman, Jeremy M. C. Brown, Joshua Keene, Lysander Miller

Bayesian optimisation with a movement penalty and heteroscedastic Gaussian process localises radioactive sources while achieving sublinear regret.

arxiv:2605.14942 v1 · 2026-05-14 · physics.app-ph · cs.SY · eess.SY

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\pithnumber{K3CQSV3UZ44UJ7UIBX7LO2RURC}

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3 Author claim open · sign in to claim
4 Citations open
5 Replications open
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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

The strategy is shown to generate sublinear regret in the source-seeking task, while simulations demonstrate its effectiveness in localising radioactive sources.

C2weakest assumption

That the radiation intensity field can be adequately modeled by a heteroscedastic Gaussian process whose noise structure remains stable enough for the regret bound to hold in realistic environments.

C3one line summary

A Bayesian optimization method with heteroscedastic Gaussian process surrogate and movement switching cost achieves sublinear regret and effective source localization in simulations for radioactive source seeking.

References

19 extracted · 19 resolved · 0 Pith anchors

[1] Extremum seeking with stochastic perturbations , author=. IEEE Trans. Autom. Control , volume=. 2009 , publisher= 2009
[2] Performance improvement and limitations in extremum seeking control , journal = 2000
[3] Atanasov, Nikolay and Le Ny, Jerome and Michael, Nathan and Pappas, George J. , booktitle=. Stochastic source seeking in complex environments , year=
[4] Radioactive capsule in
[5] Kakade and Matthias W

Formal links

2 machine-checked theorem links

Receipt and verification
First computed 2026-05-17T23:38:55.456192Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

56c5095774cf3944fe880dfeb76a3488baa6b94dc1ff888f005c74d51066b421

Aliases

arxiv: 2605.14942 · arxiv_version: 2605.14942v1 · doi: 10.48550/arxiv.2605.14942 · pith_short_12: K3CQSV3UZ44U · pith_short_16: K3CQSV3UZ44UJ7UI · pith_short_8: K3CQSV3U
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Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/K3CQSV3UZ44UJ7UIBX7LO2RURC \
  | 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: 56c5095774cf3944fe880dfeb76a3488baa6b94dc1ff888f005c74d51066b421
Canonical record JSON
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  "metadata": {
    "abstract_canon_sha256": "8e7a6df8d33f1761f216aea6b3f7ffd0b06341b294cc02d6b5c4cbb039eb6b77",
    "cross_cats_sorted": [
      "cs.SY",
      "eess.SY"
    ],
    "license": "http://creativecommons.org/licenses/by-nc-nd/4.0/",
    "primary_cat": "physics.app-ph",
    "submitted_at": "2026-05-14T15:16:33Z",
    "title_canon_sha256": "6fd2b4c97a9e95ef4ad85fe0a20134eb8f126858fe9422258f6fe5ad130755ca"
  },
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  "source": {
    "id": "2605.14942",
    "kind": "arxiv",
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}