Abstract
The Forward Physics Facility (FPF) is a proposed extension of the HL-LHC program designed to exploit the unique scientific opportunities offered by the intense flux of high energy neutrinos, and possibly new particles, in the far-forward direction. Located in a well-shielded cavern 627 m downstream of one of the LHC interaction points, the facility will support a broad and ambitious physics program that significantly expands the discovery potential of the HL-LHC. Equipped with four complementary detectors—FLArE, FASER ν 2, FASER2, and FORMOSA—the FPF will enable breakthrough measurements that will advance our understanding of neutrino physics, quantum chromodynamics, and astroparticle physics, and will search for dark matter and other new particles. With this Letter of Intent, we propose the construction of the FPF cavern and the construction, integration, and installation of its experiments. We summarize the physics case, the facility design, the layout and components of the detectors, as well as the envisioned collaboration structure, cost estimate, and implementation timeline.
| Original language | English |
|---|---|
| Article number | 117398 |
| Pages (from-to) | 1-73 |
| Number of pages | 73 |
| Journal | Nuclear Physics B |
| Volume | 1026 |
| Early online date | 17 Mar 2026 |
| DOIs | |
| Publication status | Published - May 2026 |
Bibliographical note
Publisher Copyright:Copyright © 2026. Published by Elsevier B.V.
Funding
The work of L.A. Anchordoqui is supported by the U.S. National Science Foundation grant PHY-2412679. The work of A.J. Barr is funded in part through STFC grants ST/R002444/1 and ST/S000933/1, and through research funded by the John Fell Oxford University Press Research Fund. The work of B. Batell is supported by U.S. Department of Energy grant DE-SC-0007914. The work of J. Bian, M.V. Diwan, S. Linden, M. Vicenzi, and W. Wu is supported in part by Heising-Simons Foundation Grant 2022–3319. The work of M. Citron is supported in part by U.S. Department of Energy grant DE-SC0009999. I. Coronado and D. Soldin acknowledge the support and resources from the Center for High Performance Computing at the University of Utah. I. Coronado is also supported by the Summer Undergraduate Research Fellowship Program at the Department of Physics & Astronomy at the University of Utah. The work of J.L. Feng, M. Fieg, F. Kling, R.M. Abraham, and T. Mäkelä is supported in part by U.S. National Science Foundation grants PHY-2111427, PHY-2210283, and PHY-2514888. The work of J.L. Feng is supported in part by Simons Investigator Award #376204, Heising-Simons Foundation Grants 2019-1179 and 2020-1840, and Simons Foundation Grant 623683. The work of R. Francener is supported by Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq, Brazil), Grant 161770/2022-3. The work of E. Hammou is supported by the European Research Council under the European Union’s Horizon 2020 research and innovation Programme (grant agreement n.950246), and partially by the STFC consolidated grant ST/T000694/1 and ST/X000664/1. The work of C.S. Hill is supported in part by U.S. Department of Energy Grant DE-SC0011726. The work of Y.S. Jeong is supported in part by the National Research Foundation of Korea (NRF) grant funded by the Korea government through Ministry of Science and ICT Grant No. RS-2025-00555834. The work of F. Kling is supported in part by the Deutsche Forschungsgemeinschaft under Germany’s Excellence Strategy – EXC 2121 Quantum Universe – 390833306. The work of J. McFayden is supported by the Royal Society grant URF\R1\201519 and STFC grant ST/W000512/1. The work of J. Rojo is partially supported by NWO, the Dutch Research Council, and by the Netherlands eScience Center (NLeSC). The work of S. Trojanowski is supported by the National Science Centre, Poland, research grant No. 2021/42/E/ST2/00031. The work of K. Watanabe is supported by JSPS KAKENHI Grant No. JP25K07286. The work at BNL is under U.S. Department of Energy contract No. DE-SC-0012704.
| Funders | Funder number |
|---|---|
| National Research Foundation of Korea | |
| Nederlandse Organisatie voor Wetenschappelijk Onderzoek | |
| Oxford University Press | |
| European Research Council | |
| Netherlands eScience Center | |
| Ministry of Science and ICT, South Korea | RS-2025-00555834 |
| Narodowe Centrum Nauki | 2021/42/E/ST2/00031 |
| National Science Foundation | PHY-2412679 |
| Science and Technology Facilities Council | ST/S000933/1, ST/R002444/1 |
| Japan Society for the Promotion of Science | DE-SC-0012704, JP25K07286 |
| Conselho Nacional de Desenvolvimento Científico e Tecnológico | 161770/2022-3 |
| Horizon 2020 Framework Programme | ST/X000664/1, 950246, DE-SC0011726, ST/T000694/1 |
| Deutsche Forschungsgemeinschaft | 390833306 |
| University of Utah | PHY-2210283, 2020-1840, PHY-2111427, 376204, PHY-2514888, 2019-1179 |
| Heising-Simons Foundation | DE-SC0009999, 2022–3319 |
| U.S. Department of Energy | DE-SC-0007914 |
| Royal Society | URF\R1\201519, ST/W000512/1 |
| Simons Foundation | 623683 |
Keywords
- Astroparticle physics
- Dark matter
- Experimental design
- Large hadron collider
- Neutrinos
- Parton distribution functions
- QCD
Fingerprint
Dive into the research topics of 'The forward physics facility: Physics opportunities and conceptual design'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver