Search arXiv⌕ Search
Home/Archive/arXiv

arXiv · 2511.03883

Physics Briefing Book: Input for the 2026 update of the European Strategy for Particle Physics

Jorge de Blas·Monica Dunford·Emanuele Bagnaschi·Ayres Freitas·Pier Paolo Giardino·Christian Grefe·Michele Selvaggi·Angela Taliercio·Falk Bartels·Andrea Dainese·Cristinel Diaconu·Chiara Signorile-Signorile·Néstor Armesto·Roberta Arnaldi·Andy Buckley·David d'Enterria·Antoine Gérardin·Valentina Mantovani Sarti·Sven-Olaf Moch·Marco Pappagallo·Raimond Snellings·Urs Achim Wiedemann·Gino Isidori·Marie-Hélène Schune·Maria Laura Piscopo·Marta Calvi·Yuval Grossman·Thibaud Humair·Andreas Jüttner·Jernej F. Kamenik·Matthew Kenzie·Patrick Koppenburg·Radoslav Marchevski·Angela Papa·Guillaume Pignol·Justine Serrano·Pilar Hernandez·Sara Bolognesi·Ivan Esteban·Stephen Dolan·Valerie Domcke·Joseph Formaggio·M. C. Gonzalez-Garcia·Aart Heijboer·Aldo Ianni·Joachim Kopp·Elisa Resconi·Mark Scott·Viola Sordini·Fabio Maltoni·Rebeca Gonzalez Suarez·Benedikt Maier·Timothy Cohen·Annapaola de Cosa·Nathaniel Craig·Roberto Franceschini·Loukas Gouskos·Aurelio Juste·Sophie Renner·Lesya Shchutska·Jocelyn Monroe·Matthew McCullough·Yohei Ema·Paolo Agnes·Francesca Calore·Emanuele Castorina·Aaron Chou·Monica D'Onofrio·Maksym Ovchynnikov·Tina Pollman·Josef Pradler·Yotam Soreq·Julia Katharina Vogel·Gianluigi Arduini·Philip Burrows·Jacqueline Keintzel·Deepa Angal-Kalinin·Bernhard Auchmann·Massimo Ferrario·Angeles Faus Golfe·Roberto Losito·Anke-Susanne Mueller·Tor Raubenheimer·Marlene Turner·Pierre Vedrine·Hans Weise·Walter Wuensch·Chenghui Yu·Thomas Bergauer·Ulrich Husemann·Dorothea vom Bruch·Thea Aarrestad·Daniela Bortoletto·Shikma Bressler·Marcel Demarteau·Michael Doser·Gabriella Gaudio·Inés Gil-Botella·Andrea Giuliani·Fabrizio Palla
View original source ↗Read source document ↗Export metadata ↓

Abstract

The European Strategy for Particle Physics (ESPP) reflects the vision and presents concrete plans of the European particle physics community for advancing human knowledge in fundamental physics. The ESPP is updated every five-to-six years through a community-driven process. It commences with the submission of specific proposals and other input from the community at large, outlining projects envisioned for the near-, mid-, and long-term future. All submitted contributions are evaluated by the Physics Preparatory Group (PPG), and a preliminary analysis is presented at a Symposium meant to foster a broad community discussion on the scientific value and feasibility of the various ideas proposed. The outcomes of the analysis and the deliberations at the Symposium are synthesized in the current Briefing Book, which provides an important input in the deliberations of the Strategy recommendations by the European Strategy Group (ESG).

Explore related subjects

hep-ex

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Jorge de Blas, Monica Dunford, Emanuele Bagnaschi, Ayres Freitas, Pier Paolo Giardino, Christian Grefe, Michele Selvaggi, Angela Taliercio, Falk Bartels, Andrea Dainese, Cristinel Diaconu, Chiara Signorile-Signorile, Néstor Armesto, Roberta Arnaldi, Andy Buckley, David d'Enterria, Antoine Gérardin, Valentina Mantovani Sarti, Sven-Olaf Moch, Marco Pappagallo, Raimond Snellings, Urs Achim Wiedemann, Gino Isidori, Marie-Hélène Schune, Maria Laura Piscopo, Marta Calvi, Yuval Grossman, Thibaud Humair, Andreas Jüttner, Jernej F. Kamenik, Matthew Kenzie, Patrick Koppenburg, Radoslav Marchevski, Angela Papa, Guillaume Pignol, Justine Serrano, Pilar Hernandez, Sara Bolognesi, Ivan Esteban, Stephen Dolan, Valerie Domcke, Joseph Formaggio, M. C. Gonzalez-Garcia, Aart Heijboer, Aldo Ianni, Joachim Kopp, Elisa Resconi, Mark Scott, Viola Sordini, Fabio Maltoni, Rebeca Gonzalez Suarez, Benedikt Maier, Timothy Cohen, Annapaola de Cosa, Nathaniel Craig, Roberto Franceschini, Loukas Gouskos, Aurelio Juste, Sophie Renner, Lesya Shchutska, Jocelyn Monroe, Matthew McCullough, Yohei Ema, Paolo Agnes, Francesca Calore, Emanuele Castorina, Aaron Chou, Monica D'Onofrio, Maksym Ovchynnikov, Tina Pollman, Josef Pradler, Yotam Soreq, Julia Katharina Vogel, Gianluigi Arduini, Philip Burrows, Jacqueline Keintzel, Deepa Angal-Kalinin, Bernhard Auchmann, Massimo Ferrario, Angeles Faus Golfe, Roberto Losito, Anke-Susanne Mueller, Tor Raubenheimer, Marlene Turner, Pierre Vedrine, Hans Weise, Walter Wuensch, Chenghui Yu, Thomas Bergauer, Ulrich Husemann, Dorothea vom Bruch, Thea Aarrestad, Daniela Bortoletto, Shikma Bressler, Marcel Demarteau, Michael Doser, Gabriella Gaudio, Inés Gil-Botella, Andrea Giuliani, Fabrizio Palla. 2025-11-05. Physics Briefing Book: Input for the 2026 update of the European Strategy for Particle Physics. https://doi.org/10.17181/cern.35ch.2o2p

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

arXiv2026

Search for dark matter in a signature with a four-prong large-radius jet in proton-proton collisions at $\sqrt{s}$ = 13 TeV

A search for a pair of nonprompt dark matter (DM) candidates produced in association with an initial-state radiation jet, in a signature containing a four-prong large-radius jet, is presented. The signal model contains a heavy vector or axial-vector mediator, which produces long-lived dark-sector particles that decay to a stable DM particle and a light boson, which decays to quarks. The analysis is based on data collected in the years 2016$-$2018 with the CMS detector at the LHC in proton-proton collisions at $\sqrt{s}$ = 13 TeV, corresponding to an integrated luminosity of 138 fb$^{-1}$. Signal candidates feature large-radius jets, which are identified using a jet substructure tagger based on a graph neural network. The large-radius jet aims to reconstruct the decay of light DM mediators into four quarks, which are produced in association with two stable DM particles. The standard model background contributions are estimated from data using dedicated control regions. The missing transverse momentum spectrum is probed for a potential signal over the expected background. No significant excess over the standard model expectation is observed. Upper limits at 95% confidence level are set on the signal strength as functions of either the mediator mass or the relevant coupling. This is the first search for a pair of nonprompt DM candidates in the Lorentz-boosted topology, characterized by a large-radius jet and large missing transverse momentum.

hep-ex↗
arXiv2026

Charge-dependent atmospheric muon flux at 17 GV geomagnetic cutoff with the mini-ICAL detector

The Iron CALorimeter (ICAL) detector at the India-Based Neutrino Observatory (INO) was conceived as an underground experiment designed to measure atmospheric neutrino oscillation parameters. As part of the R\&D programme, a scaled prototype (mini-ICAL), 85\,ton, approximately 1/600$^{\mathrm{th}}$ the mass of the full detector, was constructed at the IICHEP Transit Campus, Madurai (altitude 150\,m; latitude 9.9372$^\circ$\,N; longitude 78.013$^\circ$\,E; geomagnetic latitude 1.44$^\circ$\,N; vertical cutoff rigidity 17\,GV) and operated between 2018 and 2022. The prototype enabled measurements of charge-dependent cosmic muon spectra in the vicinity of the geomagnetic equator and provided an important validation of detector performance, reconstruction algorithms, and simulation frameworks for the ICAL experiment. Differential fluxes of $μ^{-}$ and $μ^{+}$ were measured over the momentum range $\sim$\,1--5\,GeV/c. The obtained momentum spectra are systematically lower than those reported at sites with smaller geomagnetic cutoff rigidities, consistent with the suppression of low- and intermediate-rigidity primary cosmic rays at the 17\,GV cutoff. The measurements are compared with predictions from different hadronic interaction models available in CORSIKA simulations.

hep-ex↗
arXiv2026

Laboratory constraints on peV-scale mass splitting between ordinary and sterile neutron states

Sterile states of matter, represented by a parallel ``mirror'' sector, may contribute to the observed dark matter in the Universe. We investigated the parameter space of neutron $(n)$ to mirror-neutron $(n')$ oscillations, in the case where the two states are not necessarily mass-degenerate, taking into account interactions in the mirror sector. By tuning the magnitude of an applied magnetic-field in the range $5~μ\mathrm{T} < B < 360~μ\mathrm{T}$ to corresponding resonance conditions for finite mass splitting, we derive exclusion limits for the $n-n'$ oscillation time constant reaching about $20~\text{s}$ over the mass-difference range $0.3 - 22~\text{peV}$. In parts of this parameter range, our limits exceed the model-dependent neutron-star-cooling bound, providing the first experimental constraints in this scenario that are more stringent than this astrophysical estimate.

hep-ex↗