SearcharxivSearch

arXiv · 2409.08983

Physics program and performance of the ALICE Forward Calorimeter upgrade (FoCal)

Abstract

The FoCal is a high-granularity forward calorimeter to be installed as an ALICE upgrade subsystem during the LHC Long Shutdown 3 and take data during the LHC Run 4. The FoCal detector, covering a pseudorapidity interval of $3.2 < \eta < 5.8$, extends the ALICE physics program with the capability to investigate gluon Parton Distribution Functions (PDFs) in the low-$x$ regime, down to $x \approx 10^{-6}$. FoCal measurements will provide experimental constraints for PDFs in a region of phasespace where experimental data is scarce, as well as enable the study of non-linear QCD effects like gluon saturation. The FoCal detector consists of two components. The highly-granular Si+W electromagnetic calorimeter (FoCal-E) with pad and pixel longitudinal and transverse segmented readout layers provides high spatial resolution for discriminating between isolated photons and decay photon pairs. The hadronic calorimeter (FoCal-H) is constructed from copper capillary tubes filled with scintillator fibers and is used for isolation energy measurement and jets. With this detector design, FoCal is capable of measuring direct photons, jets, and the photo-production of vector mesons such as the $J/\psi$ in p$-$Pb and Pb$-$Pb ultra-peripheral collisions. In addition, correlations of different probes can be studied, including $\gamma$$-$jet, jet$-$jet and $\pi^{0} - \pi^{0}$ correlations. These measurements will place stringent constraints to various theoretical models incorporating non-linear QCD effects. This contribution gives an overview of the FoCal physics program. Also, recent experimental results of ever-improving prototypes of the detector, which were tested at the Test Beam facilities of CERN in the years 2021$-$2023, as well as simulation studies showcasing the robustness of the detector design and its physics potential are presented.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Laura Maria Huhta. 2024-09-13. Physics program and performance of the ALICE Forward Calorimeter upgrade (FoCal). https://arxiv.org/abs/2409.08983

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