SearcharxivSearch

arXiv · 2504.12797

Status of the Proton EDM Experiment (pEDM)

Abstract

The Proton EDM Experiment (pEDM) is the first direct search for the proton electric dipole moment (EDM) with the aim of being the first experiment to probe the Standard Model (SM) prediction of any particle EDM. Phase-I of pEDM will achieve $10^{-29} e\cdot$cm, improving current indirect limits by four orders of magnitude. This will establish a new standard of precision in nucleon EDM searches and offer a unique sensitivity to better understand the Strong CP problem. The experiment is ideally positioned to explore physics beyond the Standard Model (BSM), with sensitivity to axionic dark matter via the signal of an oscillating proton EDM and across a wide mass range of BSM models from $\mathcal{O}(1\text{GeV})$ to $\mathcal{O}(10^3\text{TeV})$. Utilizing the frozen-spin technique in a highly symmetric storage ring that leverages existing infrastructure at Brookhaven National Laboratory (BNL), pEDM builds upon the technological foundation and experimental expertise of the highly successful Muon $g$$-$$2$ Experiments. With significant R\&D and prototyping already underway, pEDM is preparing a conceptual design report (CDR) to offer a cost-effective, high-impact path to discovering new sources of CP violation and advancing our understanding of fundamental physics. It will play a vital role in complementing the physics goals of the next-generation collider while simultaneously contributing to sustaining particle physics research and training early-career researchers during gaps between major collider operations.

Explore related subjects

Keep this discovery

BibTeXRIS

Jim Alexander, Vassilis Anastassopoulos, Grigor Atoian, Rick Baartman, Stefan Baeßler, Franco Bedeschi, John Benante, Martin Berz, Michael Blaskiewicz, Themis Bowcock, Kevin Brown, Dmitry Budker, Sergey Burdin, Brendan C. Casey, Gianluigi Casse, Giovanni Cantatore, Timothy Chupp, Hooman Davoudiasl, Dmitri Denisov, Bhawin Dhital, Milind V. Diwan, Renee Fatemi, George Fanourakis, Wolfram Fischer, Peter Graham, Frederick Gray, Antonios Gardikiotis, Claudio Gatti, James Gooding, Boxing Gou, Selcuk Haciomeroglu, Georg H. Hoffstaetter, Haixin Huang, Marco Incagli, Hoyong Jeong, David Kaplan, Marin Karuza, David Kawall, Alexander Keshavarzi, On Kim, Younggeun Kim, Ivan Koop, Valeri Lebedev, Jonathan Lee, Soohyung Lee, Alberto Lusiani, William J. Marciano, Marios Maroudas, Andrei Matlashov, Francois Meot, James P. Miller, William M. Morse, James Mott, Zhanibek Omarov, Cenap Ozben, Giovanni Maria Piacentino, Matthew Poelker, Dinko Pocanic, Boris Podobedov, Joe Price, Xin Qian, Surjeet Rajendran, Deepak Raparia, Sergio Rescia, B. Lee Roberts, Yannis K. Semertzidis, Alexander Silenko, Amarjit Soni, Edward Stephenson, Riad Suleiman, Michael Syphers, Pia Thoerngren, Volodya Tishchenko, Nicholaos Tsoupas, Spyros Tzamarias, Alessandro Variola, Graziano Venanzoni, Eva Vilella, Joost Vossebeld, Peter Winter, Bogdan Wojtsekhowski, Eunil Won, Konstantin Zioutas. 2025-04-17. Status of the Proton EDM Experiment (pEDM). https://arxiv.org/abs/2504.12797

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

KEEP EXPLORING

Related papers

Production of Light Nuclei and Hypernuclei in Heavy-Ion Collisions

We review recent STAR and ALICE measurements of light-nucleus and hypernucleus yields, femtoscopic correlations, and collective flow presented at SQM 2026. Statistical-hadronization calculations provide a useful baseline for integrated yields but do not simultaneously describe all measured light-nucleus ratios across collision energies and system sizes. For bound states with mass number $A<4$, current coalescence calculations provide a broadly consistent description of yields, femtoscopic correlations, and collective flow, although the quantitative hypertriton comparison depends on the assumed few-body wave function. The suppressed production of resonant $^{4}$Li relative to compact $^{4}$He indicates an effect of nuclear structure and late-stage dynamics. However, the quantitative model comparison also depends on the treatment of feed-down from unstable states. In high-multiplicity $p$+$p$ collisions, pion-deuteron femtoscopy further indicates that most observed (anti)deuterons are formed through nucleon fusion after strong decays of short-lived resonances. Taken together, these measurements show that production chronology and internal nuclear structure leave measurable imprints on the physics observables.

hep-ex

Search for the process $e^+e^-\to f_1(1285)$ at the SND detector

In the experiment with the SND detector at the VEPP-2000 $e^+e^-$ collider, a search is performed for the direct production of the $C$-even $f_1(1285)$ resonance in $e^+e^-$ collisions. The analysis is based on data with an integrated luminosity of about 200 pb$^{-1}$, accumulated in the center-of-mass energy range of 1.14--1.46 GeV, of which about 72 pb$^{-1}$ were recorded near the maximum of the $f_1(1285)$ resonance. The $f_1(1285)$ production cross section at the resonance maximum $\sigma(e^+e^-\to f_1)=(31\pm 13\pm 2)$ pb and the branching fraction $B(f_1(1285)\to e^+e^-)=(3.5\pm 1.4\pm 0.3)\times 10^{-9}$ have been measured. The significance of the observation of the $e^+e^-\to f_1(1285)$ process is $2.5\sigma$. Since the significance is low, we also present the upper limits at the 90% confidence level: $\sigma(e^+e^-\to f_1)<48\mbox{ pb}$ and $B(f_1(1285)\to e^+e^-)<5.4\times 10^{-9}$.

hep-ex

Projected Sensitivity to Slow Muonphilic Dark Matter with Accelerator Muon Beams

The nature of dark matter (DM) remains one of the most enduring open questions in modern physics, and muonphilic DM has emerged as a promising scenario that complements traditional DM candidates. Following the recently established cosmic-ray muon scattering approach, we investigate the sensitivity for probing slow muonphilic DM with accelerator muon beams. A Geant4-based simulation framework is developed, incorporating the detector geometry from the PKMu muon tomography system and a dedicated elastic $\mu$-DM scattering process. The projected sensitivity is found to be largely insensitive to both the beam energy and the transverse beam size when the beam is fully contained within the detector acceptance. For a benchmark beam intensity of $10^5/\rm{s}$, the simulated pure-muon beam surpasses the existing cosmic-ray limit of $1.61\times10^{-17}$ cm$^2$ at $m_{\rm DM}=1$ GeV within approximately 11 seconds. A realistic muon beam phase-space distribution based on simulations for the High Intensity heavy-ion Accelerator Facility (HIAF) is also implemented, yielding projected limits that improve upon the cosmic-ray results by nearly two orders of magnitude in a one-day exposure. These results demonstrate that a beam-muon scattering experiment offers a robust and promising route toward significantly improved sensitivity to slow muonphilic DM.

hep-ex