1. Introduction
MoEDAL (Monopole and Exotics Detector at the LHC), the Large Hadron Collider’s (LHC’s) newest experiment [
1]—which started official data taking in 2015—is totally different to other collider detectors. It is currently comprised of passive tracking, using plastic Nuclear Track Detectors (NTDs) and trapping sub-detectors that are capable of retaining a permanent direct record of discovery and even capturing new particles for further study in the laboratory. It also has a small TimePix pixel device array for monitoring beam-related backgrounds. MoEDAL is designed to only detect highly ionizing avatars of new physics and is insensitive to Standard Model physics signals. Thus, it can operate without an electronic trigger. A full GEANT4 (GEometry And Tracking platform) model of MoEDAL is now available. A visualization of this model is shown in
Figure 1.
The primary aim of the General Purpose LHC Detectors (GPLDs), ATLAS and CMS, is to discover the Higgs boson and study its properties as precisely as possible. As we all know the discovery a new particle by ATLAS and CMS, which is now largely identified with the Standard Model Higgs boson, was announced on 4 July 2014 [
2]. In a similar way, the main aim of the MoEDAL experiment is to search for the Magnetic Monopole. The main modern conception of the magnetic monopole is that it is a topological “excitation” in the Higgs field of the underlying theory. In this way, the main physics aims of the GPLDs and MoEDAL are complementary. Their experimental sensitivity is also complementary in that GPLDS have quite limited sensitivity to Highly Ionizing Particles (HIPs), which MoEDAL is designed to detect. On the other hand, MoEDAL cannot detect the decays of new particles into Standard Model states.
However, MoEDAL, similar to the GPLDs, can do much more. MoEDAL is pioneering experiment designed to search for highly ionizing avatars of new physics such as magnetic monopoles or massive (pseudo-)stable charged particles [
3]. Its groundbreaking physics program defines over 34 scenarios that yield potentially revolutionary insights into such foundational questions as: Are there extra dimensions or new symmetries? What is the mechanism for the generation of mass? Does magnetic charge exist? What is the nature of dark matter? How did the big bang develop from the earliest times.
Another important development is the planning and prototyping of a new MoEDAL subdetector, MAPP (MoEDAL Apparatus for Penetrating Particles). MAPP is planned for deployment for LHC’s Run-3. A prototype MAPP detector is already deployed. MAPP will extend MoEDAL’s physics reach by allowing the search for milli-charged particles and new very long-lived particles. A further new sub-detector, in the longer term planning phase, is MALL (MoEDAL Apparatus for extremely Long Lived Particles). This detector is aimed at the search for new massive charged particles with lifetimes that can reach the order of 10 years.
The high-risk nature of MoEDAL’s extensive program is justified not only by the prospect of a revolutionary breakthrough with impact beyond the realm of particle physics, but also by its now proven ability to provide unique and wide reaching constraints on new physics. MoEDAL is now preparing a proposal to continue data taking during LHC’s Run-3.
3. Physics Results
In August 2016, MoEDAL published its first physics analysis paper [
7] on the search for magnetic monopoles based on data taken at a center-of-mass energy (E
cm) of 8 TeV. In this paper, MoEDAL placed the best limits in the world in the search for magnetic monopoles with Dirac magnetic charge greater than or equal to
. In February 2017, we published the results of our first paper on LHC RUN-2 data taken at an E
cm of 13 TeV [
8]. In this paper, we were still the only LHC experiment placing limits on
. Additionally, we pushed the direct search for multiple magnetically charged particles to
, with masses up to 6 TeV, for the first time ever. Using a Drell–Yan (DY) model for monopole-pair production with spin-1/2 monopoles, this translates into monopole mass limits exceeding 1 TeV, the strongest to date at a collider experiment [
9] for charges ranging 2–4 times
.
These last two papers placed limits on spin-0 and spin-1/2 monopole production, as is usual for searches at accelerators. Our latest paper [
10] was published in July 2018. In this paper, we pushed the search to spin-1 magnetic monopoles for the first time at a collider experiment. In addition, we placed limits for both
-dependent and
-independent monopole couplings, another first for direct searches for monopoles. The results of our last three papers are summarized in
Figure 6 and compared with our only competition (so far) at the high-energy frontier, coming from the ATLAS experiment [
11]. Additionally, we placed monopole-pair direct production cross-section upper-limits in the range 40–105 fb for magnetic monopole charges up to 5g
D and monopole masses up to 6 TeV.
We a currently have two papers in preparation and due to be published to the archive in early 2019. The first to be completed details the search for monopole-pair production via photon-fusion, and DY production. This paper follows on from a detailed theoretical study of these process carried out by MoEDAL authors [
12]. In this paper, we have employed duality arguments to justify an effective monopole-velocity-dependent magnetic charge in monopole-matter scattering processes. Based on this, we conjecture that such
-dependent magnetic charges might also characterize monopole production. In addition, we introduced a magnetic-moment term proportional to a new phenomenological parameter
describing the interactions of these monopoles with photons for spins 1/2 and 1. The lack of unitarity and/or renormalizability is restored when the monopole effective theory adopts a SM form.
The other paper that is in-progress reports a search using, for the first time, our NTD (the previous results used our trapping arrays) system to search for highly electrically charged particles. In this case we are searching for highly electrically charged particles, rather than magnetically charged particles. To date, the only LHC limit we can find comes from the ATLAS Collaboration [
11] where they placed limits on electrically charged particles with charge (Z) in the range: 10e < Z < 60e. We envisage that we will be able to place a much better limit on highly electrically charged particle production.
The motivation behind our introduction of the concept of the magnetic-moment of the monopole introduced above is to enrich the monopole phenomenology with the (undefined) correction terms to the monopole magnetic moment to be treated as free parameters potentially departing from those prescribed for the electron or W± bosons in the SM. As we lack a fundamental microscopic theory of magnetic poles, such an addition appears reasonable. This creates a dependence of the scattering amplitudes of processes on this parameter, which is passed on to the total cross sections and, in some cases, to kinematic distributions. Therefore, the parameter is proposed as a new tool for monopole searches that can be used to explore different models.
Estimates from our above paper [
12] indicate that photon fusion production is the leading mechanism for direct monopole searches at the Large Hadron Collider (LHC). We expect our analysis of this production mechanism, using MoEDAL data, will be the first to be published at the LHC. In addition, our analysis will provide the world’s best mass limits for monopole production, for a spin-1, 1/2 and 1 monopole, via photon-fusion. For example, the most recent limit on photon-fusion, carried our nearly ten years ago, was made using CDF data with the result that the monopole mass must be greater than 370 GeV [
13]. Previously, roughly 13 years ago, the H1 Collaboration at HERA carried out a search, based on monopole-pair production via photon fusion [
14]. Upper limits on the monopole pair production cross-section were set for monopoles with magnetic charges from
to
or more and up to a mass of 140 GeV.
4. The Program for LHC’s LS2 and RUN-3
The luminosity delivered to IP8 during LHC’s Run-2 is shown in
Figure 7. The average luminosity delivered per year over the four years of Run-2 to MoEDAL is 1.7 fb
−1. The luminosity available over the at IP8 will increase substantially to 25–30 fb
−1 over the three years of Run-3, an increase in the average luminosity taken per year at IP8 by roughly a factor of five.
To push the search for new physics to higher Ecm (14 TeV) and also to take advantage of the expected significantly higher luminosity available at Point 8 during Run 3, the MoEDAL Collaboration is requesting to take data as part of the LHC’s Run-3 program. This future physics program involves two additional features: a greater stress on high luminosity searches, to ∼30 fb−1 and beyond, and also the exploitation of the new sub-detectors MAPP and MALL. Good examples of high luminosity studies are searches for new massive long-lived/pseudostable electrically charged particles. Several candidates for such new particles can be found within the arena of supersymmetry: long-lived sleptons within the Gauge-Mediated symmetry-breaking (GMSB) framework; R-hadrons within Split Supersymmetry that contain supersymmetric gluino(s); and long-lived charginos, for example from Anomaly-Mediated Symmetry Breaking (AMSB).
This extension of data taking will also allow us to exploit two new planned sub-detectors MAPP (the MoEDAL Apparatus for Long Lived Particles) and MALL (the MoEDAL apparatus for extremely Long Lived particles) to expand the physics reach of the MoEDAL experiment and allow the search for fractionally charged and long-lived particle messengers of new physics.
4.1. The MAPP Subdetector
The main element of MoEDAL’s upgrade plans for LHC’s RUN-3 is the addition of the MAPP sub-detector to the experiment. The existing baseline detector will continue to run as usual. As discussed above, the MAPP detector is designed to search for milli-charged particles (with charge as small as 0.001e, where e is the electric charge) and new long-lived neutrals.
A sketch of the MAPP detector that will be deployed during the long shutdown is shown in
Figure 8. The detector will be deployed in the UGC8 gallery adjacent to MoEDAL’s intersection point IP8 during the second long LHC shutdown (LS2), some 30 m to 50 m from IP8 (depending on where in the tunnel MAPP is placed), as shown in
Figure 9. The MAPP detector is protected from Standard Model backgrounds from IP8 by approximately 30 m of rock. A prototype of MAPP, corresponding to 1/10th of the from compartment of the full MAPP detector, took data in UGC8 throughout 2018.
The detector is comprised two arrays of 100 (10 cm × 10 cm × 100 cm) high light yield scintillator bars, where each bar is readout by two low noise PMTs. These two sections are sandwiched between three ToF hodoscopes. Thus, a milli-charged particle would see 200 cm of plastic scintillator readout by four low noise PMTs, in coincidence. The whole device is protected by a hermetic veto system. MAPP would be calibrated using muons, from p–p collisions at MoEDAL’s intersection point (IP8) that penetrate the intervening rock.
Additionally, the MAPP detector has a decay zone of 6–10 m in front of the detector (7–11 m to the midpoint of the detector) that makes it possible to measure the decay of new neutral particles in flight at large distances from the IP. Thus, with MAPP we can search for new long-lived neutral states. In addition, we have designed the ToF hodoscopes to have a timing resolution of ∼100 ps to further increase MAPP’s sensitivity to new physics.
4.2. The MALL Subdetector
The MALL subdetector, which is in its planning phase, is intended to push the search for the decays of new charged, massive and very long-lived long-lived particles, with lifetimes well in excess of a year. This is achieved by monitoring the MoEDAL Trapping volumes, contained within the central portion of an hermetic scintillator array, for the decays of trapped particles. A sketch of the MALL sub-detector is shown in
Figure 10. Remarkably, this detector will not be positioned at IP8 on the LHC but rather in a remote deep underground laboratory, such as SNOLAB. In this way, cosmic ray backgrounds can be reduced to a minimum.