“Hidden” –Unveiling the Universe’s Dark-Matter Signals

"Hidden" --Unveiling the Universe's Dark-Matter Signals

 

“Perhaps the most significant sign of the existence of dark matter, however, is our very existence,” observes Harvard theoretical physicist, Lisa Randall in Nature about the elusive substance that permeates the universe, exerts detectable gravitational influences, and yet eludes direct detection. “Despite its invisibility, dark matter has been critical to the evolution of our universe and to the emergence of stars, planets and even life.”

Hidden Spaces

Before the Large Hadron Collider (LHC), “the space of possibilities for dark matter was much wider than it is today,” says dark-matter theorist Tim Tait of University of California, Irvine and theory co-convener of the LHC Dark Matter Working Group about the search for the elusive hypothetical particle that may make up an invisible form of matter called dark matter, which is five times more prevalent than ordinary matter and does not directly interact with light, without which there would be no universe as we know it.

“The LHC dark-matter searches have so far come up empty handed,” reports CERN, “as have non-collider searches, but the incredible work and skill put by the LHC researchers into finding it has led them to narrow down many of the regions where the particle may lie hidden—necessary milestones on the path to a discovery.”

A Magnetic Field 100,000 Times Stronger than Earth’s

The LHC is renowned for the hunt for and discovery of the Higgs boson, but in the 10 years since the machine collided protons at an energy higher than previously achieved at a particle accelerator. “The LHC,” says Randall, author of Knocking on Heaven’s Door: How Physics and Scientific Thinking Illuminate the Universe and the Modern World, “is not merely large: the LHC is the biggest machine ever built. It is not merely cold: the 1.9 kelvin (1.9 degrees Celsius above absolute zero) temperature necessary for the LHC’s supercomputing magnets to operate is the coldest extended region that we know of in the universe—even colder than outer space. The magnetic field is not merely big: the superconducting dipole magnets generating a magnetic field more than 100,000 times stronger than the Earth’s are the strongest magnets in industrial production ever made.

“Dark Matter Particles as Big as a Galaxy”

“And the extremes don’t end there,” adds Randall. “The vacuum inside the proton-containing tubes, a 10 trillionth of an atmosphere, is the most complete vacuum over the largest region ever produced. The energy of the collisions are the highest ever generated on Earth, allowing us to study the interactions that occurred in the early universe the furthest back in time.”

Breaking New Ground

“The LHC has really broken new ground in the search for dark matter in the form of weakly interacting massive particles, by covering a wide array of potential signals predicted by either production of dark matter, or production of the particles mediating its interactions with ordinary matter,” observes the CERN team. “All of the observed results have been consistent with models that don’t include dark matter, and give us important information as to what kinds of particles can no longer explain it. The results have both pointed experimentalists in new directions for how to search for dark matter, and prompted theorists to rethink existing ideas for what dark matter could be—and in some cases to come up with new ones.”

Using Telescopes in Space and on the Ground to Look for Signals

To look for dark matter, experiments essentially “make it, break it or shake it.” The LHC has been trying to make it by colliding beams of protons. Some experiments are using telescopes in space and on the ground to look for indirect signals of dark-matter particles as they collide and break themselves out in space. Others still are chasing these elusive particles directly by searching for the kicks, or “shakes,” they give to atomic nuclei in underground detectors.

 

CERN Atlas Experiment

 

The make-it approach is complementary to the break-it and shake-it experiments, and if the LHC detects a potential dark-matter particle, it will require confirmation from the other experiments to prove that it is indeed a dark-matter particle. By contrast, if the direct and indirect experiments detect a signal from a dark-matter particle interaction, experiments at the LHC could be designed to study the details of such an interaction.

“Zero”

So how has the LHC been looking for signs of dark-matter production in proton collisions? The main signature of the presence of a dark-matter particle in such collisions is the so-called missing transverse momentum. To look for this signature, researchers add up the momenta of the particles that the LHC detectors can see—more precisely the momenta at right angles to the colliding beams of protons—and identify any missing momentum needed to reach the total momentum before the collision. The total momentum should be zero because the protons travel along the direction of the beams before they collide.

But if the total momentum after the collision is not zero, says the LHC researchers, the missing momentum needed to make it zero could have been carried away by an undetected dark-matter particle.

Two Types of LHC Searches

Missing momentum is the basis for two main types of search at the LHC. One type is guided by so-called complete new physics models, such as supersymmetry (SUSY) models. In SUSY models, the known particles described by the Standard Model of particle physics have a supersymmetric partner particle with a quantum property called spin that differs from that of its counterpart by half of a unit. In addition, in many SUSY models, the lightest supersymmetric particle is a weakly interacting massive particle (WIMP).

WIMPs are one of the most captivating candidates for a dark-matter particle because they could generate the current abundance of dark matter in the cosmos. Searches targeting SUSY WIMPs look for missing momentum from a pair of dark-matter particles plus a spray, or “jet,” of particles and/or particles called leptons.

“Missing” — Could Dark Matter Be a Source of Light In the Universe?

Another type of search involving the missing-momentum signature is guided by simplified models that include a WIMP-like dark-matter particle and a mediator particle that would interact with the known ordinary particles. The mediator can be either a known particle, such as the Z boson or the Higgs boson, or an unknown particle.

These models have gained significant traction in recent years because they are very simple yet general in nature (complete models are specific and thus narrower in scope) and they can be used as benchmarks for comparisons between results from the LHC and from non-collider dark-matter experiments. In addition to missing momentum from a pair of dark-matter particles, this second type of search looks for at least one highly energetic object such as a jet of particles or a photon.

In the context of simplified models, there’s an alternative to missing-momentum searches, which is to look not for the dark-matter particle but for the mediator particle through its transformation, or “decay,” into ordinary particles. This approach looks for a bump over a smooth background of events in the collision data, such as a bump in the mass distribution of events with two jets or two leptons.

No Signs Yet of WIMP Dark Matter

What results have the LHC experiments achieved from these WIMP searches, asks CERN. The short answer, the agency reports, is that they haven’t yet found signs of WIMP dark matter. The longer answer, they say, is that they have ruled out large chunks of the theoretical WIMP territory and put strong limits on the allowed values of the properties of both the dark-matter particle and the mediator particle, such as their masses and interaction strengths with other particles.

“We have completed a large number of dedicated searches for invisible particles and visible particles that would occur in processes involving dark matter, and we have interpreted the results of these searches in terms of many different WIMP dark-matter scenarios, from simplified models to SUSY models,” says ATLAS experiment collaboration member Caterina Doglioni. “This work benefitted from the collaboration between experimentalists and theorists, for example on discussion platforms such as the LHC Dark Matter Working Group, which includes theorists and representatives from the ATLAS, CMS and LHCb collaborations.

“Placing the LHC results in the context of the global WIMP search that includes direct- and indirect-detection experiments has also been a focus of discussion in the dark-matter community, and the discussion continues to date on how to best exploit synergies between different experiments that have the same scientific goal of finding dark matter.”

“We found no instances of this decay but we were able to set the strongest limits to date on the likelihood that it occurs,” says Prisilla Pani, ATLAS experiment co-convener of the LHC Dark Matter Working Group giving a specific example of a result obtained with data from the ATLAS experiment that highlights how the collaboration has recently searched the full LHC dataset from the machine’s second run (Run 2), collected between 2015 and 2018, to look for instances in which the Higgs boson might decay into dark-matter particles.

Dijet Searches

“These so-called dijet searches are very powerful because they can probe a large range of mediator masses and interaction strengths,” says MIT’s Phil Harris, CMS experiment co-convener about the LHC Dark Matter Working Group, highlighting searches for a dark-matter mediator decaying into two jets, such as a recent CMS search based on Run 2 data.

“The decay of the Bs meson into two muons is very sensitive to SUSY particles, such as SUSY WIMPs, because the frequency with which the decay occurs can be very different from that predicted by the Standard Model if SUSY particles, even if their masses are too high to be directly detected at the LHC, interfere with the decay,” says Cid Vidal, LHCb experiment co-convener of the LHC Dark Matter WG, pointing out how data from Run 1 and Run 2 on the decay of a particle known as the Bs meson has allowed the LHCb collaboration to place strong limits on SUSY models that include WIMPs.

“Fireflies of the Big Bang” –Did Primordial Black Holes Create Dark Matter?

“Beyond Classical” –Fuzzy Dark Matter to Primordial Black Holes

“Ten years ago, experiments (at the LHC and beyond) were searching for dark-matter particles with masses above the proton mass (1 GeV) and below a few TeV. That is, they were targeting classical WIMPs such as those predicted by SUSY. Fast forward 10 years and dark-matter experiments are now searching for WIMP-like particles with masses as low as around 1 MeV and as high as 100 TeV,” says Tait. “And the null results from searches, such as at the LHC, have inspired many other possible explanations for the nature of dark matter, from fuzzy dark matter made of particles with masses as low as 10−22 eV to primordial black holes with masses equivalent to several suns. In light of this, the dark-matter community has begun to cast a wider net to explore a larger landscape of possibilities.”

"Unveiling the Universe's Hidden Dark-Matter Signals" --The LHC Zeroes In

The possible explanations for the nature of dark matter. (G. Bertone and T. M. P. Tait)

“A New Playground” –The Dark Sector

On the collider front, the LHC researchers have begun to investigate some of these new possibilities. For example, they have started looking at the hypothesis that dark matter is part of a larger dark sector with several new types of dark particles. These dark-sector particles could include a dark-matter equivalent of the photon, the dark photon, which would interact with the other dark-sector particles as well as the known particles, and long-lived particles, which are also predicted by SUSY models.

“Dark-sector scenarios provide a new set of experimental signatures, and this is a new playground for LHC physicists,” says Doglioni.

Strange Lightness of Dark Matter –“It May Be Older Than the Big Bang”

“We are now expanding upon the experimental methods that we are familiar with, so we can try to catch rare and unusual signals buried in large backgrounds. Moreover, many other current and planned experiments are also targeting dark sectors and particles interacting more feebly than WIMPs. Some of these experiments, such as the newly approved FASER experiment, are sharing knowledge, technology and even accelerator complex with the main LHC experiments, and they will complement the reach of LHC searches for non-WIMP dark matter, as shown by the CERN Physics Beyond Colliders initiative.”

“Eureka” –A Dark-Matter Particle in 10 Years

Finally, the LHC researchers are still working on data from Run 2, and the data gathered so far, from Run 1 and Run 2, is only about 5% of the total that the experiments will record. Given this, as well as the immense knowledge gained from the many LHC analyses thus far conducted, there’s perhaps a fighting chance that the LHC will discover a dark-matter particle in the next 10 years.

“It’s the fact we haven’t found it yet and the possibility that we may find it in the not-so-distant future that keeps me excited about my job,” says Harris.

“The last 10 years have shown us that dark matter might be different from what we had initially thought, but that doesn’t mean it is not there for us to find,” says Cid Vidal.

“We will leave no stone unturned, no matter how big or small and how long it will take us,” says Pani.

As the search continues, our universe evolves. “Without dark matter,” says Harvard’s Randall, who was not involved in the CERN search, “radiation would have prevented clumping of the galactic structure for too long, in essence wiping it out and keeping the universe smooth and homogeneous. The galaxy essential to our solar system and our life was formed in the time since the big bang only because of the existence of dark matter.”

The Daily Galaxy, Max Goldberg, via Nature and CERN

Image credits: Top of page Hubble Space Telescope image showing the distribution of dark matter (grey) in the giant galaxy cluster Abell; and the CERN Atlas Experiment via Shutterstock License