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Dark Matter: an Experimental Perspective CATERINA DOGLIONI [SHE/HER] - LUND UNIVERSITY

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Dark Matter: an Experimental Perspective CATERINA DOGLIONI [SHE/HER] - LUND UNIVERSITY Dark Matter: an experimental perspective CATERINA DOGLIONI [SHE/HER] - LUND UNIVERSITY MEMBER OF THE ATLAS COLLABORATION AT CERN Inputs and discussion: European Strategy PPG BSM/DM/Higgs, Snowmass EF, RF and CF, ATLAS Collaboration, iDMEu proponents, Antonio Boveia, Boyu Gao, Isabelle John, Matt McCullough, Jocelyn Monroe, Marco Rimoldi, Ulrike Schnoor, Francesca Ungaro, Christoph Weniger, Jodi Cooley, Hugh Lippincott @CatDogLund http://www.hep.lu.se/staff/doglioni/ 1 Introduction DM @ Accelerators DM @ Direct & indirect detection Complementarity Outline Introduction from a particle experimentalist 1 perspective Dark matter experiments: 1. Dark matter at accelerators (particle colliders/intensity frontier experiments) Disclaimer #1: My main expertise is in DM @ particle colliders, so this part will be more detailed than the others 2. Direct detection of dark matter 3. Indirect detection of dark matter (+ cosmic probes) Synergies and complementarity between these different ways of detecting DM ⇒ link to the relevant Snowmass topical group Disclaimer 2: this talk is not an inclusive talk for DM, but rather a personal perspective of things I’ve learned along the way as ATLAS Dark Matter Forum/WG organizer && in the European Strategy && in the Snowmass process 1 for the perspective of a dark matter experimentalist, see page 3 of arXiv:1712.06615 Caterina Doglioni - 2020/10/30 - SEC Colloquium on Dark Matter 2 Introduction DM @ Accelerators DM @ Direct & indirect detection Complementarity WhyWhat should do we knowdark matterabout dark be a matter? particle? Caterina Doglioni - 2020/10/30 - SEC Colloquium on Dark Matter 3 LHC: the biggest man-made discovery machine 3 Introduction DM @ Accelerators DM @ Direct & indirect detection Complementarity What do we knowWhy about not? dark matter? us & our experiments, made of particles LHC: the biggestCaterina man-made Doglioni - 2020/10/30 discovery - SEC Colloquium machine on Dark Matter 4 In this talk I will assume Einstein’s gravity does not need modifications… 4 Introduction DM @ Accelerators DM @ Direct & indirect detection Complementarity The relic density ΛCDM = Λ Cold Dark Matter model https://sci.esa.int/s/Wnqq4bw Image: Planck/NASA/ESA Dark matter constitutes most of the matter in the universe 5 % The DM we measure today [relic DM density] 68 % already points at some properties of DM candidates (e.g. dark, stable) 27 % can it guide us further? Ordinary Matter Dark Matter Dark Energy Caterina Doglioni - 2020/10/30 - SEC Colloquium on Dark Matter 5 Introduction DM @ Accelerators DM @ Direct & indirect detection Complementarity How did the relic density come to be? SM ⟷ DM SM → DM creation processes decrease thermal Freeze-out until a new SM ⟷ DM equilibrium is reached equilibrium Relic density Couplings too small SM → DM creation processes increase for SM ⟷ DM Freeze-in until equilibrium is reached equilibrium Universe expands and cools down Examples of DM ⟷ SM processes Isabelle John's thesis Note: simplified picture, for a more complete one see https://arxiv.org/abs/1706.07442 Commonality of many of these models: they require some form of interaction (it can be more or less significant) between ordinary matter and dark matter interaction ⇔ particles & forces Caterina Doglioni - 2020/10/30 - SEC Colloquium on Dark Matter 6 Introduction DM @ Accelerators DM @ Direct & indirect detection Complementarity WhatDM do weis a know much-sought about dark particle matter? https://benty-fields.com/trending Papers on the arXiv with the words in the title or abstract LHC: the biggestCreditsCaterina man-made for findingDoglioni it: -Xenon1T, 2020/10/30 discovery Twitter - SEC Colloquium machine on Dark Matter 7 Disclaimer: website not to be used as input by funding agencies 7 Introduction DM @ Accelerators DM @ Direct & indirect detection Complementarity WhatFinding do we newknow particles about dark takes matter? time Particle physics discoveries require large instruments and time It looks like you’re searching for dark matter. Have you tried starting with the ones you know about already? Caterina Doglioni - 2020/10/30 - SEC Colloquium on Dark Matter 8 LHC: the biggest man-made discovery machine 8 Introduction DM @ Accelerators DM @ Direct & indirect detection Complementarity WhatFinding do we newknow particles about dark takes matter? time It looks like you’re searching for dark matter. Have you tried starting with the ones you know about already? Caterina Doglioni - 2020/10/30 - SEC Colloquium on Dark Matter 9 LHC: the biggest man-made discovery machine 9 Introduction DM @ Accelerators DM @ Direct & indirect detection Complementarity Generic production of invisible particles Production of invisible particles is common in the Standard Model… Eur. Phys. J. C 77 (2017) 765 Caterina Doglioni - 2020/10/30 - SEC Colloquium on Dark Matter 10 Introduction DM @ Accelerators DM @ Direct & indirect detection Complementarity Generic production of dark matter? What other invisible particles (that are suitable thermal relics) could we produce? DM DM Eur. Phys. J. C 77 (2017) 765 Caterina Doglioni - 2020/10/30 - SEC Colloquium on Dark Matter 11 Introduction DM @ Accelerators DM @ Direct & indirect detection Complementarity Weakly Interacting Massive Particles The minimal option to make up 100% of the relic: DM • only add one particle to the SM • stable TeV-scale particle with weak-force-sized interactions • Weakly Interacting Massive Particle or Higgs • that particle conveniently appears in many SUSY models that also solve other problems in particle physics DM • beautiful and simple, almost miraculous! Caterina Doglioni - 2020/10/30 - SEC Colloquium on Dark Matter 12 Introduction DM @ Accelerators DM @ Direct & indirect detection Complementarity Weakly Interacting Massive Particles The minimal option to make up 100% of the relic: DM • only add one particle to the SM • stable TeV-scale particle with weak-force-sized interactions • Weakly Interacting Massive Particle or Higgs • that particle conveniently appears in many SUSY models that also solve other problems in particle physics DM • beautiful and simple, almost miraculous! • Experimental “advantage”: many experiments can see it in different ways Standard Matter Credit: ESA/Gaia/DPAC. Dark Matter Indirect Detection Direct Detection Colliders Astrophysics Caterina Doglioni - 2020/10/30 - SEC Colloquium on Dark Matter 13 Introduction DM @ Accelerators DM @ Direct & indirect detection Complementarity Dark matter Invisible particles at colliders • Starting from our baseline assumption: WIMP DM • interacts with SM particles → we can produce and detect it at LHC ATLAS, CMS, LHCb RF6 Particle Collider KEK Belle-2 EF colliders experiments {ILC, CLIC, CEPC, FCC, muon … Future } AF3-5 known particle production of collision DM particles Caveat: very simplified diagram A running example: the Large Hadron Collider accelerates and collides protons Collisions are recorded and analyzed by four main experiments LHC collisions schedule: 2022: beginning of Run-3 Caterina Doglioni - 2020/10/30 - SEC Colloquium on Dark ~2027: Matter beginning of Run-4 (HL-LHC)14 Introduction DM @ Accelerators DM @ Direct & indirect detection Complementarity Searches for DM invisible particles at colliders Detector covers all the solid angle and catches ~all visible particles visible particle SM (visible) proton (quark/gluon) proton (quark/gluon) SM (visible) visible particle Caterina Doglioni - 2020/10/30 - SEC Colloquium on Dark Matter 15 Introduction DM @ Accelerators DM @ Direct & indirect detection Complementarity Searches for DM invisible particles at colliders Dark matter doesn’t interact significantly with our detectors → invisible invisible particle (DM) DM (invisible) proton (quark/gluon) proton (quark/gluon) DM (invisible) invisible particle (DM) Caterina Doglioni - 2020/10/30 - SEC Colloquium on Dark Matter 16 Introduction DM @ Accelerators DM @ Direct & indirect detection Complementarity Searches for DM invisible particles at colliders Dark matter doesn’t interact significantly with our detectors → invisible visible particle invisible particle (DM) SM (visible) DM (invisible) proton (quark/gluon) proton (quark/gluon) DM (invisible) invisible particle (DM) Signature of invisible particles (like Dark Matter): missing (transverse) momentum ( ) Caterina Doglioni - 2020/10/30 - SEC Colloquium on Dark Matter 17 Introduction DM @ Accelerators DM @ Direct & indirect detection Complementarity A “monojet event” at ATLAS visible particles interacting in the detector escaping (non-interacting) particles Caterina Doglioni - 2020/10/30 - SEC Colloquium on Dark Matter 18 Introduction DM @ Accelerators DM @ Direct & indirect detection Complementarity A generic search for DM: “X+MET” ISR (jet, photon, V boson…) + MET signature - Background shapes need precise theory predictions EPJC 2017 77:829 - Results can be interpreted in a variety of models - here: vector mediator Phys. Rev. D 97, 092005 (2018) arXiv:1807.11471 EF10 Caterina Doglioni - 2020/10/30 - SEC Colloquium on Dark Matter 19 19 Introduction DM @ Accelerators DM @ Direct & indirect detection Complementarity Is this the only way we can look for WIMP DM? No! If there’s a force other than gravity, there’s a mediator (/portal), and the LHC could detect its decays into visible particles: simplified/portal models are popular collider & accelerator search benchmarks EF10 RF6 LHC Dark Matter Forum & Working Group https://lpcc.web.cern.ch/content/lhc-dm-wg-dark-matter-searches-lhc Phys. Dark Univ. 26 (2019) 100371 & references within, Ann.
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