ANUBIS: From prototype to Letter of Intent

Figure 1: (a) Complementarity between LLP detector concepts. (b) Schematic of the proposed location for the ANUBIS experiment in the ATLAS cavern.

The prototype was positioned on the top floor of the scaffolding beside ATLAS, pointing at the interaction point — as close to the proposed ANUBIS position as one can get without being in the ceiling (Fig 2b).

Figure 2: (a) Picture of the proANUBIS setup. (b) Location of proANUBIS in the ATLAS cavern.

Data taking with proANUBIS concluded in late 2025 with 177 fb⁻¹ recorded. The first public results, a calibration and performance paper [5], show that proANUBIS reaches the precision required for ANUBIS physics analyses. Individual RPC efficiencies exceed 85% (Fig 3), which for the three-chamber modules planned for ANUBIS translates to better than 99% per module. The measured time resolution is approximately 350 ps, and further studies indicate that 280 ps is within reach with additional calibration. The results were shared with the community at the LLP 2026 workshop in Cambridge, covered in another article [6] of this EP Newsletter, where the timing result is prominently featured.

Figure 3: Efficiency of proANUBIS RPC detectors as a function of applied high voltage for (a) η planes and (b) ϕ planes.
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A second set of proANUBIS results will be released shortly. It combines proANUBIS data with ATLAS data to show the symbiotic potential of the two experiments. This is made possible by an ATLAS Open Data release created for this purpose [7]. Notably, proANUBIS events have been successfully synchronised with ATLAS events. This allows for combining ATLAS muons and hadrons with tracks registered by proANUBIS. Their correlation is/can be studied in several ways, such as calculating the distance between the projected ATLAS muon track and the proANUBIS muon track (Fig 4a), reconstructing vertices of several tracks (Fig 4b), or precisely measuring the velocity of muons using information from both detectors (Fig 5).

Figure 4: (a) Event display of a proANUBIS muon track, linked to its corresponding ATLAS muon track. (b) A proANUBIS event display showing a reconstructed 2-track vertex in LHC collision data.
Figure 5: The velocity of muons β reaching proANUBIS.

In parallel, the Collaboration has been refining its sensitivity projections for the full ANUBIS experiment, starting from the quantity everything else depends on: the background. The dominant contribution comes from energetic SM LLPs – KL and neutrons – interacting hadronically with air molecules in the ANUBIS decay volume to produce displaced vertices. The background is determined through a data-driven projection — the observed rate of displaced vertices in the ATLAS muon spectrometer is extrapolated to ANUBIS, accounting for the relative size of the two detectors, the difference in material composition,  luminosity, and possible differences in vertex reconstruction efficiency [8]. This yields a deliberately conservative estimate of at most 182 ± 12 background events over the full HL-LHC dataset.

With this background prediction, sensitivities have been computed for the benchmark models defined by the Physics Beyond Colliders (PBC) working group, allowing direct comparison with other proposed experiments and existing limits. The landmark ANUBIS result is for Benchmark Case 5 (BC5), in which neutral LLPs are pair-produced via the 125 GeV Higgs boson [8]. Given how conservative the background estimate is, the projection is shown as a band spanning the full-background and background-free limits, providing unique sensitivity beyond existing and approved detectors (Fig 6).

Figure 6: The projected sensitivity of ANUBIS to a 30 GeV long-lived scalar portal particle.

A second projection covers heavy neutral leptons (HNL) in the minimal Majorana model (PBC BC6–BC7) [9]. The production modes ANUBIS is sensitive to are principally Drell-Yan and Wγ fusion. HNLs produced in association with mesons are largely lost to the isolation requirement imposed to suppress background from SM LLPs in punch-through jets; this production mode should be recoverable in detailed studies beyond the selections driven by the data-driven estimate. Its large active volume and proximity to the interaction point put ANUBIS in a good position to probe the high-mass, small-coupling corner, complementing experiments that reach lower masses or larger couplings (Fig 7). Projections for axion-like particles (ALP) are also underway, where ALPs are produced alongside a prompt lepton visible in ATLAS offering a handle for both triggering and further background reduction. The modular simulation framework SET-ANUBIS used to derive the aforementioned results was recently made public and documented in a paper [10], inviting new collaboration on sensitivity analysis of ANUBIS.

Figure 7: The projected sensitivity of ANUBIS to two minimal Majorana HNL scenarios.

The ANUBIS Collaboration is currently preparing its Letter of Intent, to be completed ahead of the Physics Beyond Colliders Roadmap Workshop on 2-4 December [11]. Interested institutes are warmly invited to join the Letter of Intent (for more information, please reach out to anubis-mgt@cern.ch), provided their involvement would not conflict with existing commitments to the Phase-2 ATLAS detector upgrade programme.

[1] M. Bauer, O. Brandt, L. Lee, and C. Ohm, Proposal to search for long-lived neutral particles in CERN service shafts, accepted by APS Open Science Gold, 1909.13022 (2026).

[2] EP Newsletter article: ANUBIS: a guide into the dark sector.

[3] G. Aielli, O. Brandt, J. Burr, O. Kortner, H. Kroha, C. Lester, L. Pizzimento, L. Pontecorvo, M. Revering, T. P. Satterthwaite, A. Shah, D. Soyk, P. Swallow (for the ANUBIS collaboration), Construction of proANUBIS: A proof-of-concept detector for the ANUBIS experiment, Nucl. Instrum. Meth. A. 1091 (2026) 171687,2512.13926 (2025).

[4] G. Aielli, O. Brandt, P. Collins, L. Dartmoor Corpe, J. Dej, O. Kortner, H. Kroha, C. Lester, L. Pizzimento, L. Pontecorvo, M. Revering, A. Shah, D. Soyk, P. Swallow, Y. Wan (for the ANUBIS Collaboration), Commissioning of proANUBIS: A proof-of-concept detector for the ANUBIS experiment, Nucl. Instrum. Meth. A. 1089 (2026) 171501,2512.18414 (2025).

[5] G. Aielli, O. Brandt, J. Burling, P. Collins, J. Dej, C. Fernandez Ruiz, C. Lester, K. Liu, L. Pizzimento, L. Pontecorvo, T. Reymermier, M. Revering, A. Shah, T. Spencer, P. Swallow (for the ANUBIS collaboration), Calibration and Performance of proANUBIS: A proof-of-concept detector for the ANUBIS experiment, accepted by Nucl. Instrum. Meth. A, 2606.26856 (2026).

[6] Designing for the unusual: LLP2026 and the lifetime frontier, https://ep-news.web.cern.ch/designing-for-the-unusual-llp2026-and-the-lifetime-frontier/

[7] ATLAS Collaboration, ATLAS proANUBIS calibration data set, https://opendata.cern.ch/record/atlas-93943 (2026).

[8] T. Adolphus et al (for the ANUBIS Collaboration), The ANUBIS detector and its sensitivity to neutral long-lived particles (PBC BC5 scenario), accepted by Phys. Rev. D 2510.26932 (2025).

[9] M. Bauer, R. Bentham, S. N. Erner, A. Mullin, D. Peng, T. Reymermier, P. N. Swallow (for the ANUBIS Collaboration), Projected sensitivity of the ANUBIS detector to heavy neutral leptons, 2606.26862 (PBC BC6 & BC7 scenarios), accepted by Eur. Phys. J C (2026).

[10] S. N. Erner, A. Mullin, T. Reymermier, P. N. Swallow, O. Brandt (for the ANUBIS Collaboration), SET-ANUBIS: a modular pipeline for ANUBIS long-lived particle sensitivity studies, 2607.26112, subm. to Comp. Phys. Comm. (2026).

[11] 2026 Physics Beyond Colliders and Non-Collider Physics Roadmap Workshop, 2-4 December 2026, https://indico.cern.ch/event/1687237/