Jetting Into the Dark Side: ATLAS’ Precision Search for Dark Matter

ATLAS Event Display: Highest-Momentum Monojet

Figure 1: A monojet event recorded by the ATLAS experiment in 2017, with a single jet of 1.9 TeV transverse momentum recoiling against corresponding missing transverse momentum (MET). The green and yellow bars show the energy deposits in the electromagnetic and hadronic calorimeters, respectively. The MET is shown as the red dashed line on the opposite side of the detector. Credit: ATLAS Collaboration/CERN

The nature of dark matter remains one of the great unsolved puzzles of fundamental physics. Unexplained by the Standard Model, dark matter has led scientists to probe new physics models to understand its existence. Many such theoretical scenarios postulate that dark matter particles could be produced in the intense high-energy proton–proton collisions of the LHC. While the dark matter would escape the ATLAS detector unseen, it could occasionally be accompanied by a visible jet of particles radiated from the interaction point, thus providing a detectable signal.
 
The ATLAS Collaboration set out to find just that. Today, at the International Conference in High-Energy Physics (ICHEP 2020), ATLAS presented a new search for novel phenomena in collision events with jets and high missing transverse momentum (MET). The search was designed to uncover events that could indicate the existence of physics processes that lie outside the Standard Model and, in doing so, open a window to the cosmos.

Precision Search for Dark Matter Physics Briefing

Figure 2: Missing transverse momentum distribution after the monojet selection in data and in the Standard Model predictions. The different background processes are shown with colours. The expected distributions of dark energy, supersymmetric and weakly-interacting massive particle scenarios are illustrated with dashed lines. Credit: ATLAS Collaboration/CERN

To identify such events, physicists exploited the principle of momentum conservation in the transverse detector plane – that is, perpendicular to the beam direction – looking for visible jets recoiling from something invisible. As events with jets are common at the LHC, physicists further refined their parameters: the events had to have at least one highly energetic jet and significant MET, generated by the momentum imbalance of the “invisible” particles. This is known as a monojet event – a spectacular example of which can be seen in Figure 1, a 2017 event display featuring the highest-momentum (1.9 TeV) monojet recorded so far by ATLAS.
 
A plethora of exotic phenomena, not directly detectable by collider experiments, could also have yielded this characteristic monojet signature. ATLAS physicists thus set out to make their study inclusive of several new physics models, including those featuring supersymmetry, dark energy, large extra spatial dimensions, or axion-like particles.

Today’s new result sets the most stringent limit on dark matter of any collider experiment so far – a milestone for the ATLAS Collaboration’s search programme.

Evidence of new phenomena would be seen in an excess of collision events with large MET when compared to the Standard Model expectation. Accurately predicting the different background contributions was a key challenge, as several abundant Standard Model processes could exactly mimic the signal topology – such as the production of a jet plus a Z boson, which then decays to two neutrinos that also leave ATLAS without being directly detected.

Physicists used a combination of data-driven techniques and high-precision theoretical calculations to estimate the Standard Model background. The total background uncertainty in the signal region ranges from about 1% to 4% in the range of MET between 200 GeV and 1.2 TeV. The shape of the MET spectrum was used to enhance the discrimination power between signals and backgrounds, thus increasing the discovery potential. Figure 2 shows a comparison of the MET spectrum observed in the entire dataset collected from the ATLAS experiment during Run 2 (2015–2018), and the Standard Model expectation.

As no significant excess was observed, physicists used the level of agreement between data and the prediction to set limits on the parameters of new physics models. In the context of weakly-interacting massive particles (a popular dark matter candidate), ATLAS physicists were able to exclude dark matter particle masses up to about 500 GeV and interaction axial-vector mediators up to 2 TeV, both at the 95% confidence level. These results provide the most stringent dark matter limits in collider experiments so far, and a milestone of the ATLAS search program.

5 Comments on "Jetting Into the Dark Side: ATLAS’ Precision Search for Dark Matter"

  1. So, have read the article and the linked page of graphs/descriptions. Unless I’m missing something, it’s seems the big takeaway is that they can now more precisely not detect dark matter?

  2. Howard Jeffrey Bender | August 15, 2020 at 11:06 am | Reply

    Another possibility, from a view of String Theory, is that Dark Matter appears to us as an effect of string/anti-string annihilations. As you may know, quantum mechanics requires that strings must be formed as pairs in the quantum foam – a string and an anti-string – that immediately annihilate each other. Quantum mechanics also requires both the string and anti-string to be surrounded by “jitters” that reduce their monstrous vibrating energies. What if this jitter remains for a fraction of an instant after their string/anti-string annihilations? This temporary jitter would be seen by us as matter for that instant before it too returns to the foam. That’s why we never see it – the “mass” lasts only for that instant but is repeated over and over and over, all over. Specifics on this can be found in my YouTube at https://www.youtube.com/watch?v=xdI0wyIiYdk

  3. … Now I wonder, is the morphing 1 dimensional entity on small scale into 3, 4 … what ever dimensional entity there it is,…
    and could that be the reason why there is Uncertainty principle as a fundamental property of the space time on the small scale?
    Could dark matter be just unaccessible to us and that is the reason why we can’t see it.
    There might be different types of the dark matter too…

  4. @BBC, not particularly ‘more precisely not detect dark matter’, but not detect anything non-standard Model, one of the main points of the monojet search is it’s very model-independent. The takeaway here is that the ATLAS monojet search is now pretty precise and agrees well with the Standard Model

  5. Ronald Patrick Marriott | August 18, 2020 at 6:12 am | Reply

    Did you know that the aether field is made in three energy levels ? You can’t remove the aether field from your particle collider experiments at #CERN so you’re going to be getting different results in at least three different energy levels and that gives you different particles. Same particle three or more results depending upon time and position in the field.
    Super string Theory supports this!
    #energy #physics #plasma #science
    #mantledynamics

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